مقاله درباره روش NATM

 در تنظیم این مقاله از مجله بلور که در دانشکده متالوژی و معدن دانشگاه تهران منتشر می شود کمک ویژه گرفته شده است و نیز حاشیه هایی از دایره المعارف ویکی پدیا بر آن افزوده شده است.

◄ مقدمه:
روش تونلسازی اتریشی (NATM)، در فاصله سالهای 1957 تا 1965 در اتریش ابداع گردید. نام این روش در سال 1962 در سالزبورگ و جهت تمیز از روش قدیمی تونملسازی اتریشی اعطا گردید. نخستین ارائه دهندگان این روش Ladislaus von Rabcewicz, Leopold Müller و Franz Pacher بودند. ایده نخستین این روش عبارت است از استفاده از فشارهای زمین شناسی در برگیرنده توده سنگ جهت مقاوم سازی ونگهداری تونل.
باید گفت که امروزه مطالعات گسترده ای از سوی متخصصین علم مکانیک سنگ در ارائه طرحی مطمئن برای نگهداری فضاهای زیرزمینی صورت می گیرد که بتواند سیستم نگهداری را به گونه ای طراحی کند که علاوه بر ایمن بودن، از نظر اقتصادی نیز معقول باشد. نتایج این مطالعات بر ضرورت بکارگیری روشهای مشاهده ای همچون NATM در تونلسازی تاکید دارد.

◄ ویژگی های اساسی ناتم:
ناتم روشی است مبتنی بر تابع نگاری رفتار توده های سنگ تحت بار و مونیتورینگ عملیات ساختمان زیرزمینی سنگ. واقعیت اینست که ناتم به عنوان یک مرحله از حفاری و نیز تکنیک های نگهداری مطرح نیست.

ناتم بر هفت ویژگی استوار است:

1-بسیج مقاومت توده سنگ: این متد بر مقاومت ذاتی توده سنگ پیرامون به عنوان یک جز اصلی نگهداری شده در تونل، تکیه می کند. تکیه گاه اولیه طوری هدایت می شود که سنگ را قاد رسازد تا بر خودش تکیه کند.

2-حمایت شاتکریت: سست کردن و نیز تغییر شکل بی اندازه سنگ می بایست به حداقل برسد. این امر با مهیا کردن لایه های نازک شاتکریت بلافاصله پس از پیشروی جبهه کار حاصل می اید.

3-اندازه گیری: هرگونه تغییر شکل ناشی از حفاری باید اندازه گرفته شود. ناتم به نصب تجهیزات اندازه گیری در سطح بالایی نیاز دارد. این در آستر، زمین و گمانه ها جاسازی می شود.

4-تکیه گاه انعطاف پذیر: آسترگیری اولیه نازک است و شرایط لایه بندی اخیر را بازتاب می دهد. این مدل به کارگیری، نسبت به تکیه گاه مجهول سریعتر به کار می اید و موثر می شود. مقاوم سازی با یک آستر بتنی ضخیم به دست نمی اید بلکه با یک ترکیب منعطف از پیچ سنگ، سیم تنیده و شیارهای فولادی حاصل می گردد.

5-بستن وارونگی: بستن سریع وارونگی و ایجاد حلقه حامل بار دارای اهمیت است. این امر در تونلهای حفر شده در زمینهای نرم بسیار وخیم است، جایی که هیچ مقطعی از تونل نباید بطور موقت رها شود.

6-ترتیب قراردادی: دانش ناتم بر اساس اندازه گیری مونیتورینگ پایه ریزی شده است. تغییر در متد تکیه گاه و ساختمان امکان پذیر است. این تنها در شرایطی ممکن است که سیستم قراردادی فادر به تغییرات باشد.

7-اندازه گیری پشتیبانی رده بندی توده سنگ: رده های اصلی سنگ برای تونل و پشتیبانی متناظر آن موجود است. اینها برای هدایت در زمینه تقویت تونل بکار می روند.

◄ اصول کلی ناتم:
تونلزنی به روش جدید اتریشی در خاکهای سست تا سنگ های سخت و مقاوم و در اعماق کم (در جهت به حداقل رساندن نشست سطح) تا اعماق زیاد و بیش از 1000 متر تحت میدانهای تنش ناشی از عملیات معدنکاری انجام گرفته است.

بنابراین اصول زیر به طور کلی قابل اعمال می باشند. این اصول در مقاله آقای دکتر فکر به ترتیب زیر آورده شده است:

1- عنصر اصلی باربری یک تونل، توده سنگ پیرامونی آن می باشد.

2- بنابراین یکی از اصول عبارت می باشد از: حفظ مقاومت اولیه سنگ تا آنجایی که امکان داشته باشد.

3- اتساع یا جابجایی ها باید به حداقل رسانده شود زیرا موجب پایین آوردن مقاومت می گردد.

4- وضعیت تنش تک محوری یا دو محوری، شرایط نامناسب برای تونل بوده و باید از آن اجتناب گردد.

5- دگرشکلی ها باید به طرزی تحت کنترل دراید که توده سنگ پیرامون تشکیل یک حلقه باربر حول تونل را بدهد. به گونه ای که از دست رفتن مقاومت به وسیله اتساع در سطحی قابل قبول نگهداشته شود. با اجرای خوب این کنترل، ایمنی واقتصاد افزایش می یابد.

6- برای رسیدن به این منظور، تکیه گاه اولیه می باست در زمان درست نصب گردد.

7- عامل زمان ویژه سیستم ترگیبی سنگ به اضافه تکیه گاه اولیه، باید به صحت کافی تخمین زده شود.

8- تخمین عامل زمان بستگی دارد به الف: آزمونهای آزمایشگاهی ب: آزمونهای برجا ج: رده بندی توده سنگ

از این سه نرخ دگرشکلی و زمان پابرجایی می تواند استنتاج شده و با رفتار واقعی تونل در حین ساختمان تطبیق و کنترل گردد.

9- هرجا که دگرشکلی ها زیاد بود و یا سست شدن توده سنگ انتظار می رود، می بایست از تماس کامل تکیه گاه اولیه با جدار تونل در محل برخورد اطمینان حاصل اید. این امر با بکار گرفتن شاتکریت به بهترین نحو حاصل می گردد.

10- تکیه گاه اولیه باید نازک و دارای صلبیت خمشی پایین باشد، از این رو گشتاورهای خمشی پایین آورده و وقوع شکستگی ها در اثر خمش به حداقل می رسد.

11- افزایش نگهداری با شبکه توری اضافی، قابهای فولادی، سیمهای فولادی، سیم مهارها یا میل مهارها حاصل می اید نه با آسترگیری ضخیمتر.

12- نوع و مقدار تکیه گاه و زمان نصب، از نتایج اندازه گیری دگرشکلی ها تعیین می گردد.

13- از نظر استاتیکی تونل را می توان لوله ای ضخیم (یا حلقه ای دوبعدی) که از توده، سنگ و آسترگیری تشکیل یافته در نظر گرفت.

14- از آنجا که یک لوله مساعدترین ویژگی پایداری را بدون آنکاه درز داشته باشد داراست، بستن همزمان کف تونل در هنگامیکه سنگ دارای مقاومت کافی نباشد دارای اهمیت است.

15- رفتار توده سنگ با بستن به موقع کف تونل تعیین می گردد. پیشروی های زیاد در طاق منجر به دیر بسته شدن کف و آنهم منجر به تشکیل لوله نیمه آسترگیری اولیه گردیده که نتیجه آن بروز گشتاورهای بزرگ خمشی در جهت محور تونل می باشد که منجر به ایجاد تمرکز تنش زیاد در سنگ، در پای دیواره های جانبی می گردد.

16- حفاری پیشانی کامل، بهترین روش برای دستیابی یک توزیع یکنواخت تنش است. هر چند که در سنگهای سست، حفاری بخش بخش، برای پایداری در حین ساختمان ممکن است لزوم پیدا کند.

17- روند حفاری و نگهداری برای پایداری مهم می باشد. زیرا آنها عامل زمان توده سنگ را تحت تاثیر قرار می دهند.

تغییر در طول دوره حفاری، زمان بستن کف، طول پیشروی طاق، مقاومت و زمان نصب تکیه گاه تماما به طور سیستماتیک برای کنترل فرایند توزیع مجدد تنش و پایدارسازی به کار گرفته میشوند.

19- در موارد آستربندی مضاعف، آستربندی نهایی باید همچنان نازک باشد. تنش عمود می باید بر روی تمام سطح تماس بین آستربندی ها منتقل گردیده و تنش برشی در سطح برخورد می باید پایین باشد.

20- کل سیستم، توده سنگ به اضافه پوشش می بایست با نگهداری اولیه پایدار گردند.

در صورت خورنده بودن آبهای زیرزمینی آستربندی نهایی می بایست قادر به پایدار سازی توده سنگ به تنهایی باشد. سیم مهارها تنها می توانند به عنوان یک نگهدارنده دائمی تلقی گردند، البته در صورتی که از گزند خورندگی در محیطهای خاص در امان باشند.

21- برای کنترل ایمنی سازه تونل، اندازه گیری تنش بتن و تنش برخورد در مرز بین سنگ و آستربندی ضرورت دارد. اندازه گیری دگرشکلی ها همچنان ادامه پیدا می کند.

22- فشار ایستایی آب بر روی پوشش و فشار جریان در توده سنگ با زهکشی مناسب پایین آورده می شود.

به طوری که از این اصول دریافت می شود، ناتم روند و دستور کاری نیست که با دنبال کردن آن به نتیجه مورد نظر رسید بلکه عبارت است از مجموعه ای از ایده ها که به ویژگی های زمین شناسی منطقه توجه ویژه ای دارد. این روش در نتیجه تجربیات متعدد در کار تونلزنی به دست آمده است و برای به دست آوردن هر یک از این ایده ها و نیز جمعبندی آنها به عنوان یک روش سالهای زیادی وقت صرف شده است. نوآوری اساسی این ایده، یک فن ساختمانی یا یک روش خاص محاسباتی نمی باشد، اما برای ساختمان تونل در توده سنگ و چگونگی برخورد با آن ارائه طریق می نماید.

یکی از اصول موفقیت زای این روش گردآوری موضوعات متعدد از مهندسی عمران و مکانیک سنگ می باشد که شامل موضوعات نظری و عملی است.

ادامه مطلب ---/

ادامه نوشته

کانی سازی اورانیوم و فلزات همراه آن

حوضه تلخه رود در آذربایجان خاوری ، بوسیله ارتفاعات و توده های پلوتونی – ولکانیکی احاطه شده و در واقع یک حوضه بین کوهستانی می باشد که درمجموعه ای از قوس های ماگمایی مربوط به اواخر ترسیر، قرار گرفته است . سرشاخه های تلخه رود از ارتفاعاتی چون آتشفشان های سبلان ، بزقوش ،دچان و قوشه داغ سرچشمه گرفته و با شستشو دادن دامنه های مذکور ،مقدار قابل توجهی از اورانیوم موجود آنها را به کانال اصلی رودخانه حمل کرده و در آنجا در لابه لای رسوبات مئاندری رودخانه و پهنه های دلتایی رسوب داده است .بررسی آماری عیار اورانیوم و عناصر دیگر درتوالی رسوبی میوسن بالایی میان تبریز و اهر در تلخه رود وقوع کانی سازی را در منطقه مشخص می سازد ارتباط اورانیوم با مس ، مولیبیدنیوم و وانادیوم و همبستگی ثبت عناصر مزبور است . این همبستگی تنها در ستون چینه ای (Roll front) ،موید کانی سازی از تیپ ماسه سنگ و از نوع هلالی امیدچه مشاهده شده و آنومالی های مربوط هم از نوع اپی ژنتیک می باشد . در گورچین اورانیوم با عناصر شاخص تیپ ماسه سنگی همبستگی منفی نشان می دهتد . حال آن که شیل های تیره در ستون چینه ای این منطقه و هوازدگی سطحی ، از عیار کم و بیش بالای اورانیوم همزمان با رسوب گذاری صورت (leaching) با وجود تاثیر گرفته و کانی سازی مربوطه ، از نوع سین ژنتیک است .فراوانی سیمان کلسیتی در لیتوفاسیس های ماسه سنگی موید وفور (CO3-2) در محیط های دیانژی بوده که نقش مهمی در انتقال اورانیوم درمحیط های مذکور به صورت کربوکسیل اورانیوم ایفا نمونه و محلول های اخیر در نهایت در شرایط احیا محیط های شیمیایی می تواند به اکسید اورانیوم تبدیل شده باشد

مطالعات ژئوشیمیایی:اورانیوم عنصری اکسیفیل( تمایل بهترکیب با اکسیژن دارد) است که با ظرفیت های ٣و ٤و ٥و ٦ بااکسیژن ترکیب می شود . اکسیدهای ٤و ٦ ظرفیتی آن در طبیعت فراوانتر است . میانگین فراوانی در پوسته جامد زمین ppm 2 بوده ( Mason and Moore 1982 ) که این عیار طی فعالیت های ماگمایی درسنگ های آذرین اسیدی و یا قلیایی افزایش می یابد . دراین صورت منشا اصلی آن در بیشتر موارد همان سنگ ها خواهد بود . آزاد شدن اورانیوم از سنگ های منشا و انتقال آن به محیط تحت شرایط مناسب است صورت Eh,PH خاص شیمیایی که مهمتر از همه می گیرد اورانیوم در محیط های اکسیدان محلول است و با بر هم خوردن فاکتورهای فوق ایجاد محیط های احیایی از حالت محلول خارج شده و رسوب می کند. نهشتگی و تجمع اورانیوم بوسیله اکسیدهای آهن ، تیتانیوم و (Absorbe) از طریق جذب منگنز و نیز کانی های رسی و مواد آلی صورت می گیرد .
مقایسه داده های لیتوفاسیسی و سنجش عیار عناصر فلزی مختلف درتلخه رود با عیار همان عناصر در پوسته جامد زمین استداندارد های بین المللی نشان میدهد که توده های آذرین در آذربایجان خاوری و با متعلق به اوایل ترسیر (Teriay) بالاترین عیار اورانیوم به میزان ppm ١٦ منشا اصلی و اولیه این عنصر در منطقه می باشد.در میان لیتوفاسیس های رسوبی منطقه شیل های تیره در مقطع گورچین باعیارppm ١٤
غنی ترین سگ های اورانیوم دار حوضه تلخه رود محسوب می شود .(سامانی ١٣٦٥ ) لازم به ذکر است که محیط های رسوبی احیایی وفور مواد آلی در شیل های مذکور ،نقش بسیار مهمی در جذب و تثبیت اورانیوم داشته است . همچنین مقدار اورانیوم . فلزات همواره در سنگ آهک ها و ماسه سنگ های گورچین و امیدچه و مقایسه آنها با استانداردهای و مساه سنگ های گورچین و امیدچه ومقایسه آنها با استانداردهای بین الملی مشخص کننده استمرار فعالیت کانی سازی در نئوژن در تلخه رود تست این مقایسه روشن می سازد که کانی سازی اورانیوم درشیل ها با کانی سازی در لیتوفاسیس ماسه سنگی و کربناته از روند مشابهی برخوردار نمی باشد .◄  تغییارت عیار:آنالیز های XRF-XRD روی نمونه های تلخه رود در نگاه اول مشخص می سازد که کانی سازی در منطقه با تنوع زیادی از عناصر فلزی همراه می باشد. که مهم ترین آن ها عبارتند از :

اورانیوم ،وانادیوم ،مس، مولیبینیوم ،ترسنیک ،سرب ، توریوم ،آهن ، تیتانیوم ،زیرکونیوم و کبالت رفتار ژئوشیمیایی این عناصر طی انتقال از خاستگاه به میزبان های رسوبی آنها ، بسیار متفاوت بوده و به همین علت تجمع عناصر مذکور در افق های کان سازی یکسان نبوده و عیار آن هم از یکدستی وهمگنی برخوردار نمی باشد . در این قبیل شرایط ، جهت تعیین فراوانی و میزان تمرکز عناصر و شناخت فلزات موجود در هر مجموعه کانی سازی از دیدگاه ( Beus and Grigorian1977 ) استفاده از روش های آماری بسیار مفید می باشد .

درمقاله حاضر بر اساس تغییرات عیار عناصر ، منحنی تغییرات فراوانی تجمعی (cumulative freqenncy) آنها با رسم و پاره ای پارامتر های آماری از قبیل میانگین هندسی geometric mean ) ) بر اساس ٥٠ درصد مشخص شده و بدین ترتیب انحراف معیار در سطوح اطمینان (standard devitaion) بر اساس ٨٤ درصد و آنومالی (anomaly) بر پایه 5/97 مشخص شده و بدین ترتیب گروه های فلزی در تلخه رود تعیین و تفکیک گردیده اند .توضیح آن که هر جا که تغییرات بارز و تعیین کننده ای در فراوانی تجمعی عناصر روی داده باشد ، اثر آن به صورت شکستگی در شیب عمومی منحنی مربوط ظاهر خواهدشد و درنتیجه منحنی هایی که از روند و شیب یکنواخت و ملایمی برخوردار هستند دلالت بر عدم تغییرات معنی دار در فراوانی تجمعی متغیرهای مورد نظر خواند داشت . با تعمیم مفاهیم آماری فوق در زمینه تغییرات عیار عناصر درتوالی های رسوبی درتلخه رود ، می توان نوع وکیفیت کانی سازی را در موارد خاص مشخص نمود .لذا منحنی های تغییرات فراوانی تجمعی عناصر فلزی چنانچه از تغییرات سریع به صورت انحراف معیار و یا آنومالی برخوردار باشند. وقوع کانی سازی را نشان خواهد داد . بر این اساس تغییرات فراوالنی تجمعی فلزات مختلف در امیدچه ،کانی سازی اورانیوم ، مس و انادیوم و مولیبیدنیوم را درحد آنومالی مشخصمی سازد . درحالی که این فعالیت درمورر کانی های دیگراز قبیل زیر کونیوم ،کبالت ،ارسنیک قابل ملاحظه نمی باشد از سوی دیگر شواهد فوق که نشان دهنده تیپ خاصی از کانی سازی در گورچین و خواجه دیده نمی شود . به طوری که تغییرات فروانی تجمعی برخوردار است( شکست واضح در منحنی ) که دلالت بر تمرکز کم و بیش بالای این عناصر در لایه های شیلی دارد. درحالی که تغییرات تجمعی نشان داده و در منحنی های اورانیوم و به ویژه مولیبدنیوم تغییرات معنی دار دیده نمی شود . ◄  همبستگی ژئوشیمیایی بین اورانیوم و سایر عناصر:
پاره ای عناصر به سبب خاصه شیمیایی مشترک ، در شرایط زمین شناسی ویژه .رفتارهای ژئوشیمیایی کم و بیش مشابه و یکسان از خود نشان می دهند . این واقعیت بر اساس نوعی رابطه و همبستگی بین عناصر مختلف بوده که فرآیند های ژئوشیمیایی به کمک آن ها تفسیر می گردد . رابطه و همبستگی اورانیوم با عناصری از قبیل مس ، مولیبدنیوم ،وانادیوم و کبالت و ٠٠٠ از آن جمله است و با مطالعه آن می توان تیپ کانی سازی مجموه عناصر فوق را مشخص نمود از آن جا که هدف اصلی در مقاله حاضر تبیین تیپ کانی سازی اورانیوم درمنطقه مورد مطالعه است ،لذا تعیین رابطه ژئوشیمیایی این عنصر با عناصر دیگر حائز اهیمت است . در امیدچه اورانیوم بالاترین همبستگیرا دارد . این مجموعه فلزی اختصاص به کانی سازی اورانیوم در تیپ های ماسه سنگی داشته و در موارد دیگر مشاهده نشده است .
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Weathering processes

Weathering processes

The response of geologic materials to the environment (physical, chemical, and biological) at or near the Earth's surface. This response typically results in a reduction in size of the weathering materials; some may become as tiny as ions in solution.

 

Types

 

The agents and energies that activate weathering processes and the products resulting therefrom have been classified traditionally as physical and chemical in type. In classic physical weathering, rock materials are broken by action of mechanical forces into smaller fragments without change in chemical composition, whereas in chemical weathering the process is characterized by change in chemical composition. In practice, the two processes commonly overlap, almost inseparably. For example, diminution in particle size facilitates chemical reactivity, and an increase in volume of the products during chemical reaction may physically disintegrate the reactants.

Viewed broadly, environments of weathering and the suite of products from each may be categorized in terms of climate, such as desert, arctic, or tropical rain forest. In cold and dry climates, physical weathering predominates and produces angularity in both rock particles and surficial landforms. In warm humid climates, chemical and biochemical weathering yields rounded rock masses, and hydrated and oxidized mineral compounds which may be developed at great depths.

 

Agents

 

Within each environment, specific agents of weathering may be recognized and correlated with the types of effects they produce. Important agents of weathering are water in all surface occurrences (rain, soil and ground water, streams, and ocean); the atmosphere (H2O, O2, CO2, wind); temperature (ambient and changing, especially at the freezing point of water); insolation (on large bare surfaces); ice (in soil and glaciers); gravity; plants (bacteria and macroforms); animals (micro and macro, including humans). Human modifications of otherwise geologic weathering that have increased exponentially during recent centuries include construction, tillage, lumbering, use of fire, chemically active industry (fumes, liquid, and solid effluents), and manipulation of geologic water systems.

 

Products

 

Products of physical weathering include jointed (horizontal and vertical) rock masses, disintegrated granules, frost-riven soil and surface rock, and rock and soil flows.

Products of chemical weathering include many which have been widely adapted to important economic and technologic uses. Such products include the soil, and the clays used in making ceramic structural products, whitewares, refractories, various fillers and coating of paper, portland cement, absorbents, and vanadium. These are the relatively insoluble products of weathering; characteristically they occur in clays, siltstones, and shales. Sand-size particles resulting from both physical and chemical weathering may accumulate as sandstones.

After precipitation, the relatively soluble products of chemical weathering give rise to products and rocks such as limestone, gypsum, rock salt, silica, and phosphate and potassium compounds useful as fertilizers.

Products of weathering that occur in colloidal sizes, also important qualitatively and quantitatively, are included in the preceding listings.

 

Processes of chemical weathering

 

Chemical reactions involving water and gaseous O2 and CO2 are probably the most important or abundant weathering processes on Earth. In sharp contrast, on the Moon, which is devoid of such an atmosphere, there is essentially no hydration, oxidation, or carbonation. Aqueous dissolution of rocks and minerals is probably the simplest or most straightforward process of chemical weathering. Solution rapidly removes rock salt (NaCl) and gypsum (CaSO4 · 2H2O), but more slowly corrodes carbonate, silicate, and oxide rocks.

 

Hydrolysis

 

Water dissolves O2 and CO2 from the air (possibly 10 times more CO2 from soil atmosphere), enabling it to oxidize and carbonate, as well as to hydrolyze rocks susceptible to those reactions. For example, Fe in silicate minerals is oxidized to Fe2O3, thereby removing Fe from the silicate structure and disrupting that network and making it more vulnerable to further breakdown. Oxidizing water reacts with metallic sulfides to produce the several sulfur-bearing acids, among them sulfuric acid, which is a powerful weathering reagent in itself. The metal constituents of the original sulfides typically become hydroxides or oxides. Fumes containing SO2, Cl2, or F2 from combustion of coal, from smelters, or from industrial furnaces generally combine downwind with water vapor (humidity), rain, fog, or dew to form weathering-effective acids.

Aqueous dissolution of CO2 produces carbonic acid, which has acidic and complexing (carbonate) properties. Dolostone (dolomite) and limestone (calcite) are quickly dissolved as Ca and Mg bicarbonates in carbonic acid, possibly producing topographic sinkholes, caves, and other karstic features, in addition to erosionally lowering the surface of those rocks. Turbulent and rapid flow of water on carbonate rocks markedly increases the rate of dissolution. The less soluble quartz, chert, clay, or iron oxides contained in dissolving limestone are left behind. Monuments and other structures composed of limestone and marble are similarly attacked.

Silicate rocks are attacked primarily by hydrolysis in a general reaction as shown below, where

 

                                                Eq 1

 

 

M refers to metal cations (K, Na, Ca, Mg), subscript n denotes an unspecified ratio of atoms, and the Al following Si substitutes for Si. Thus there are formed, by hydrolysis, soluble alkali-metal hydroxides, soluble silica (the ionic distribution depends upon pH), and relatively insoluble clay mineral (or zeolite), or less commonly, hydrated alumina. If the hydrolysis takes place at pH 9.5 or higher, both silica and alumina will be relatively soluble and mobile. They may then be separated and form bauxite (Al2O3 · nH2O). Under more acid conditions, clay minerals are formed.

 

 

Fig. 1  Exchange-energy relationships between a rootlet and three minerals. (a) A potassium-bearing, primary silicate mineral. (b) A clay mineral well stocked with exchangeable metal cations. (c) A clay mineral scantily stocked with metal cations. The exchange bonding energy (calories per gram-equivalent weight) of K for H in the rootlet exceeds that in only the well-stocked clay mineral which is thus the only one of the three minerals from which nutrient ions can be taken. 1 cal = 4.18 J. (After W. D. Keller, Mineral and chemical alluviation in a unique pedological example, J. Sediment. Petrol., 31:80–86, 1961)

 

 

 

fig 1

 

 

 

Adding hydrogen ions to the hydrolyzing system increases the rate of reaction. Carbonic acid, formed when the carbon dioxide of the air and soil dissolves in water, is a source of hydrogen ions which accelerate the reaction. Organic (humic) and other acids participate in the hydrolysis. Strongly complexing organic acids may mobilize (complex) in solution Al more effectively than Si from Al-silicate minerals. Solubilization in and precipitation from organic solutions are therefore sensitive to both Eh, the oxidation potential, and pH. Another major source of hydrogen ions is their production in the ionic atmosphere about the rootlets of growing plants. During plant growth and metabolism, hydrogen ions are evolved. These are exchanged by the roots for nutrient cations (K+, Ca2+, Mg2+) present in nearby clay colloids and rocks. Thus, the process of nutrition of plants is simultaneously a process of weathering of rocks. Hence, the energy which drives plant growth and is indirectly derived from the Sun likewise furnishes some of the energy for weathering of rocks.

 

Plant activity

 

Plants that are primitive in development apparently possess higher energies of cation exchange than do those that are more advanced. Lichens derive nutrient cations from fresh rock without intermediary soil. It is difficult to assess quantitatively the extent to which bacteria in the soil, and those coating interstices among mineral grains, accomplish chemical rock weathering, but some pedologists consider bacteria to be a major agent. See also: Soil microbiology

Rootlets of macroplants may sorb nutrients from adjacent soil when the mean free-bonding energy of the rootlet exceeds the crystal-bonding energy of mean free-bonding energies of clay minerals or organic substances by which they hold individual nutrient ions in polyionic systems in the soil. Hence, plant nutrition and the activity of agriculture occupy an intermediate position in the weathering sequence between fresh rock-forming minerals and intensely weathered “final” products of weathering (Figs. 1 and 2). Chelating organic substances extract cations from rocks, implementing rock breakdown. Partial weathering makes the rock constituents more available to plants, but extended weathering removes the nutrient materials entirely.

 

 

Fig. 2  Comparison of binding energy (calories per gram-equivalent weight) on nutrient metal cation (indicated by M) by rocks and soil minerals with exchange binding energy on cation by plant roots. The relation of plant nutrition to weathering and abundance of nutrients is shown. 1 cal = 4.18 J. (After W. D. Keller, Mineral and chemical alluviation in a unique pedological example, J. Sediment. Petrol., 31:80–86, 1961)

 

 

 

fig 2

 

 

 

 

 

Results of chemical weathering

 

As shown by the hydrolysis reaction, the products from it may be broadly grouped into relatively soluble and relatively insoluble categories. The ultimate destination of the soluble products is the ocean, where they are concentrated in solution or removed by precipitation. Potassium released in solution by weathering, although as soluble as sodium, is more tightly sorbed by clay minerals and may be fixed in crystals of hydrous mica. Dissolved potassium is therefore less abundant than sodium in seawater. Magnesium may be incorporated in chloritic varieties of clay minerals. See also: Clay minerals

The most abundant weathering products of silicate rocks are the clay minerals. Weathering (hydrolysis) taking place in an environment such that high concentrations of calcium, magnesium, and iron (particularly ferrous) are built up tends to produce the smectite group of clays. Such a high concentration of ions occurs where evaporation exceeds precipitation, ground-water drainage is poor, or hydrolysis is rapid (as in weathering of volcanic dust). The kaolin group of clay minerals is developed where rainfall exceeds evaporation and leaching is intense. Oxidation of iron is then ordinarily high. Under conditions of very drastic leaching and continual wetting of the rocks, as in a tropical rain forest, silica and most cations dissolve, leaving hydrated oxides of alumina and ferric iron (bauxite and laterite). Rising groundwater solutions may carry Al and Fe upward and, because of evaporation or oxidation of organic complexes, leave deposits of both in the tropical subsoil. A high K+/H+ ratio in the aqueous-weathering system of Al-silicates yields the illite clay mineral (disordered K-mica). Weathering processes apparently reach a state of near-equilibrium with respect to kaolinite or smectite in environments such as those that prevailed where thick, valuable deposits of the clays were formed. In contrast, surface-exposed weathering of boulders and outcrops yields highly varied and changing products, quasimineral compounds, and rock wreckage.

Clay minerals, although relatively stable products of weathering in one environment, may be decomposed if subjected to more drastic leaching in another environment by processes of the removal of exchangeable cations, the more tightly fixed potassium of illite (hydrous mica) and possibly silica. Clay minerals are said to be degraded when their structures are partly destroyed. Entirely desilicated clays become bauxite or laterite. See also: Bauxite; Laterite

Walter D. Keller

 

Bibliography

 

 

D. Atkinson,Access to Geography: Weathering, Slopes and Landforms, 2005

W. J. Bland and D. Rolls, Weathering: An Introduction to the Basic Principles, 1998

M. J. Johnsson and A. Basu (eds.), Processes Controlling the Composition of Clastic Sediments, 1994

A. Lerman and M Meybeck (eds.), Physical and Chemical Weathering in Geochemical Cycles, 1988

R. Littke, Deposition, Diagenesis, and Weathering of Organic Matter-Rich Sediments, 1993

Underground mining


 

 

The extraction of ore from beneath the surface of the ground. Underground mining is also applied to deposits of industrial (nonmetallic) minerals and rocks, and underground or deep methods are used in coal mining. Some ores and industrial minerals can be recovered from beneath the ground surface by solution mining or in-place leaching using boreholes.  See also: Coal mining; Solution mining

Underground mining involves a larger capital investment and higher production cost per ton of ore than open pit mining. It is done where mineral deposits are situated beyond the economic depth of open pit mining; it is generally applied to steeply dipping or thin deposits and to disseminated or massive deposits for which the cost of removing the overburden and the maintaining of a slope angle in adjacent waste rock would be prohibitive. In some situations, the shallower portion of a large orebody will be mined by open pit methods, and the deeper portion will be mined by underground methods.  See also: Open-pit mining

Underground mine entries are by shaft, adit, incline, or spiral ramp (Fig. 1). Development workings, passageways for gaining access to the orebody from stations on individual mine levels, are called drifts if they follow the trend of the mineralization, and cross-cuts if they are driven across the mineralization. Workings on successive mine levels are connected by raises, passageways that are driven upward. Winzes are passageways that are sunk downward, generally from a lowermost mine level.

 

Fig. 1  Underground mining entries and workings.

 

 

 

fig 1

 

 

 

In a fully developed mine with a network of levels, sublevels, and raises for access, haulage, pumping, and ventilation, the ore is mined from excavations referred to as stopes. Pillars of unmined material are left between stopes and other workings for temporary or permanent natural support. In large-scale mining methods and in methods where an orebody and its overlying waste rock are allowed to break and cave under their own weight, the ore is extracted in large collective units called blocks, panels, or slices.  See also: Mining

 

Exploration

 

Exploration and development constitute the preproduction stage of underground mining. Exploration refers to the delineation of a newly discovered mineral deposit or an extension of a known deposit and to its evaluation as a prospect. During exploration, the deposit is investigated in sufficient detail to estimate its tonnage and grade, its metallurgical recovery characteristics, and its suitability for mining by various methods.

Information on the size, shape, and attitude of a deposit and information for estimating the tonnage and grade of the ore is taken from drill holes and underground exploration workings. Diamond core drilling provides intact samples of ore and rock for assaying and for detailed geologic and geotechnical study; percussion drilling provides chips of material for the recognition of ore and waste boundaries and for additional sampling. Underground exploration workings are used for bulk and detailed sampling, rock mechanics testing, and the siting of machinery for underground drilling.  See also: Drilling, geotechnical

The tonnage and the grade of the material available in a mineral deposit are interrelated. The cutoff grade is the weakest mineralization that can be mined at a profit. Ore reserves are calculated in respect to the amount of ore in place at potential cutoff grades, the tonnages and average grades in identified blocks of ore, and the ultimate tonnage and grade of ore that should be available under projected conditions of recovery and wall rock dilution in mining. The suitability of a deposit for mining is determined in testing and evaluation work related to the physical and chemical nature of the ore, hydrologic conditions, and the needs for ground control.  See also: Rock mechanics

 

Mine Development

 

Where high topographic relief allows for an acceptable tonnage of ore above a horizontal entry site, an adit or blind tunnel is driven as a cross-cut to the deposit or as a drift following the deposit from a portal at a favorable location for the surface plant, drainage facilities, and waste disposal. In situations where the deposit lies below or at a great distance from any portal site for an adit, entry must be made from a shaft collar or from an incline or decline portal. A large mine will commonly have a main multipurpose entry and several more shafts or adits to accommodate personnel, supplies, ventilation, communication, and additional production.

Adits

 

Access by adit generally provides for relatively low-cost underground mining. The broken ore from above the adit level can be brought to the portal in trains, conveyor belts, and rubber-tired trucks without the need for hoisting, and the workings can be drained without pumping. The driving of an adit is generally less expensive per unit distance of advance than the sinking of a shaft or the driving of an inclined access. In areas of low topographic relief and in the mining of deep orebodies, the sinking of a shaft will often be a more economical approach than the driving and maintaining of a considerably longer incline or adit from a remote part of the site.

 

Shafts

 

Production shafts are generally located in stable ground on the footwall side of a dipping deposit rather than in the deposit itself or in the hanging-wall side, where protective pillars would be needed to maintain stability as mining progresses. A shaft may be inclined to follow the dip of the deposit and avoid increasingly longer cross-cuts to the ore at greater depth, but vertical shafts are more common because of their lower construction and maintenance cost per unit of depth and their better efficiency for hoisting ore. Shafts are sunk as rectangular or circular openings 15–30 ft (5–9 m) in diameter; they are equipped with a headframe and hoisting system and are lined with timber, steel forms, or concrete for ground support. Smaller shafts 5– 15 ft (1.5–5 m) in diameter, generally for escapeways and ventilation, may be bored by mechanical drilling machines.

 

Inclines

 

Inclines equipped with hoists, declines for access by rubber-tired equipment, and gently inclined spiral ramps for diesel-powered truck haulage allow for direct access to relatively deep mine levels without having to transfer the ore and materials to hoisting systems.

 

Development workings

 

Development workings in the deposit consist of mine levels and sublevels, with drifts in the ore zone or in the more stable rock on the footwall side of the ore zone. Level workings serve as passageways for miners and low-profile equipment and as haulageways. In broken or unstable ground, passageways and haulageways are supported by timber sets and steel beams or arches; further stabilization is given by rock bolts, sometimes in combination with cable bolting and wire mesh, and the walls may be lined with concrete or spray-on shotcrete.

The raises that connect levels and sublevels provide for the removal of broken ore (chutes and ore passes), for access by miners, and for ventilation and supply routes.

In conventional mining and in the most common development procedures, headings are advanced in a cyclic sequence of drilling, blasting, mucking (removal of broken rock), and installing ground support. In continuous mining, the cycle is replaced by rapid excavation, a single operation in which headings are advanced by powerful tunnel boring and road header machines with teeth that break rock from the face. In situations where the uniformity and texture of the rock and ore permit development by continuous mining, the walls of the resulting passageways are smoother and more stable than would be provided by conventional cyclic operations involving blasting.  See also: Tunnel

The continuous mining procedure of raise boring is well established. Shaft boring is used in the sinking of small-diameter ventilation shafts and escapeways. The driving of mine level development headings by cutting and boring machinery is more common in coal, potash, and salt deposits and in relatively soft sandstones and shales than in hard ore and rock.

Hydraulic breakers provide successively smaller rock sizes at development headings, and the broken rock is collected at the face by mechanical loading machinery and transferred to the mine haulage system by mobile conveyors or rubber-tired load-haul-dump machines. Haulage beyond the transfer point has been done by electric-powered locomotives with trains of cars but now is increasingly done by rubber-tired electric- or diesel-powered shuttle cars or trucks and by conveyor belt systems. In shaft mines, the broken rock is collected in underground storage pockets and loaded into skips for hoisting to the surface.

The entire sequence in mine development—the advance of headings, breaking of rock, loading, haulage, and hoisting—is increasingly automated. Teleoperated and autonomous machines have become central to every stage in mining, and new mines are developed with the use of geographic information systems (GIS) technology to accommodate the extensive communication systems and mining methods that relate to operations by remote control.  See also: Geographic information systems

 

 

Mining Methods

 

A fundamental condition in the choice of mining method is the strength of the ore and wall rock. Strong ore and rock permit relatively low-cost methods with naturally supported openings or with a minimum of artificial support. Weaker ore and wall rock necessitate more costly methods requiring wide-spread temporary or permanent artificial support such as rock bolting. Large deposits with weak ore and weak walls that collapse readily and provide suitably broken material for extraction may be mined by low-cost caving methods. Few mineral deposits are so uniform that a single method can be used without modification in all parts of the mine. Mining to an increasing depth with higher stress conditions and mining from a thicker portion of an orebody into thinner or less uniform portions will especially call for changes in method.

 

Naturally supported openings

 

The stopes remain open, essentially by their own strength, during ore extraction. Stability may be maintained to some extent by timbers, rock bolts, and accumulations of broken ore. The workings may collapse with time or may eventually need to be filled with waste material to protect workings in adjacent areas. Backfilling involves the placement of a paste of cemented waste rock or mill tailings. The methods range from gophering, an unsystematic small-scale practice, to carefully planned and executed systems using limits determined by rock mechanics investigations.

Open stoping

 

This is used in steeply dipping and thin orebodies with relatively strong ore and wall rock. In overhand methods the ore is stoped upward from a sill pillar by miners working on a staging composed of stulls (round timbers) and lagging (planks). With the drilling and blasting of successive small blocks of ore from the back (roof), the broken ore falls onto lower stagings and to the bottom of the stope; it is collected on the haulage level through draw points or chutes. In underhand stoping the ore is mined downward in a series of benches, and the broken ore is scraped or hauled into a raise or ore pass for collection on a lower mine level. The width of an open stope is limited by the strength of the ore and its capability to stand unsupported. Occasional pillars, generally of waste or low-grade zones in a vein, are left for support; timber stulls may be wedged between the stope walls for stability as well as for access, and rock bolts may also be used to maintain wall stability.

 

Sublevel stoping

 

Also referred to as longhole or blasthole stoping, sublevel stoping is practiced in steeply dipping and somewhat wider orebodies with strong ore and strong walls (Fig. 2). Sublevel drifts and raises or slots are driven at the ends of a large block of ore so that a series of thinner horizontal slices can be provided. Miners in the sublevels drill patterns of radial holes (ring or fan drilling) or quarrylike parallel holes (slashing). Beginning at the open face of the initial slot, the ore is blasted in successive increments, and the broken ore falls directly to the bottom of the stope. A crown pillar is generally left unmined at the top of the stope to support the next major level.

 

Fig. 2  Sublevel stoping, with ring drilling.

 

 

 

fig 2

 

 

 

 

Vertical crater retreat

 

This is a method of sublevel stoping in which large-diameter blastholes are drilled in a parallel pattern between major levels, and the ore is broken from the bottom of the stope in a sequence of localized blasts. All of the drilling, loading, and blasting are done by miners and teleoperated machinery in the upper level, so there is no need for access to the ore from below as the stope progresses upward.

 

Room-and-pillar mining

 

This is also referred to as stope-and-pillar mining when done in a less regular pattern. Room-and-pillar mining is done in coal seams and in flat-lying or gently dipping ore and industrial mineral deposits (Fig. 3). It is a low-cost method of underground mining because fast-moving rubber-tired equipment can operate freely, especially in large rooms and haulageways. Thin-bedded deposits are generally mined in a single stage (pass) by conventional or continuous mining; thicker deposits are mined in a two-stage benching operation. In deposits of considerable thickness, an underground quarrying operation follows the first-stage opening of a development level for sufficient access by open-pit-type blasthole drills. Room-and-pillar mining is generally limited to depths on the order of 3000 ft (914 m) in hard-rock mines and to lesser depths in coal mines because of rock bursts and similar manifestations of high-stress concentration on the pillars. Extraction in mining generally amounts to about two-thirds of the ore in a bedded deposit, with the remaining ore being left in pillars; in places where pillars can be “robbed” and the roof allowed to settle, extraction can be increased to 90% or more.  See also: Rock burst

 

Fig. 3  Room-and-pillar mining; two-stage benching operation.

 

 

 

fig 3

 

 

 

 

Shrinkage stoping

 

This is an overhand method in which broken ore accumulates in the stope, affording temporary support for the walls and a working platform for miners (Fig. 4). Shrinkage stoping is most applicable to steeply dipping veins with strong ore that will stand across a span and with relatively strong wall rock that would slough into the stope in places if left completely unsupported. When ore is broken, it has an expansion or swell factor; this necessitates a periodic drawing (shrinking) of some of the broken ore from the draw points and chutes to allow for continued access to the top of the stope. When all of the ore has been broken except for that left in pillars to protect the adjacent raises and mine levels, the entire content (the magazine) of the stope is drawn. The empty stope may be left open or filled with waste rock, and the pillars may eventually be mined.

 

Fig. 4  Shrinkage stoping, longitudinal section.

 

 

 

fig 4

 

 

 

 

 

Artificially supported openings

 

In these methods, workings are kept open during mining by using waste material, timber, and hydraulic props. After the ore is extracted, the workings are filled to maintain stability or are allowed to cave.

 

Cut-and-fill stoping

 

This method, also referred to as drift-and-fill, is used in steeply dipping orebodies in which the ore has sufficient strength to be self-supporting but the walls are too weak to stand entirely without support (Fig. 5). Most cut-and-fill stoping is done overhand, with the drilling and blasting phase similar to that in shrinkage stoping; the broken ore, however, is removed from each new cut or slice along the back, and the floor of the stope is built up of waste material such as sand or mill tailings brought in by pipeline as a water slurry. The smooth and compacted or cemented fill material provides an especially suitable floor for rubber-tired machinery. Variations in cut-and-fill mining include the ramp-in-stope system, in which load-haul-dump equipment can move rapidly in and out of the stope on an inclined surface of fill material, and the less-mechanized system of resuing in narrow veins. In resuing, ore and waste material are broken separately and the waste material is left to accumulate as fill. One additional system, undercut-and-fill, is applied to bodies of weaker ore. It provides a solid artificial back of reinforced and cemented fill for the mining of successively underlying slices of ore.

 

 

Fig. 5  Cut-and-fill stoping with sand slurry and ramp.

 

 

 

fig 5

 

 

 

 

Square set stoping

 

This is a labor-intensive and high-cost method that has been classically used in situations where the ore is too weak to stand across a wide or long back and the walls are not strong enough to support themselves. A square set, a skeletal box of keyed timbers, is filled and wedged into the available space as each small block of ore is removed by drilling and blasting. Mining continues by overhand or underhand stoping, and the stope becomes a network of interlocked square sets. The sets in the mined portion of the stope are filled with mill tailings or waste rock and pillars are left between mined-out stopes for additional wall support while the remainder of the deposit is being mined. Because of its high cost, square setting is no longer in use; it has been superseded in many mines by cut-and-fill, top slicing, and sublevel caving methods.

 

Longwall mining

 

This method is applicable to uniform and extensive but relatively thin deposits. Primarily a highly mechanized and increasingly automated coal mining method at depths where rock pressures are too high for safe room-and-pillar mining, it has also been used in potash deposits and to some extent in bedded iron, copper, and uranium orebodies. In the South African deep gold mines, a form of longwall mining is used in the thin-bedded ore zones.

In longwall mining, practically all of the coal or ore is recovered except for that left in safety pillars to protect surface structures.

The basic practice is to maintain a temporary opening in a uniform line along a working face and then to allow the roof to cave onto the floor or waste fill (gob) behind the active area. In a typical mechanized longwall coal operation, the roof support units are canopies with hydraulic-powered adjustable legs or chocks that are moved ahead as the coal is shaved into slices by shearing and plowing machinery with integrated conveyor systems. In the mining of South African gold reef deposits, longwall-type mining is done by drilling and blasting; the active area is kept open by hydraulic props and timber-concrete packs, and the mined-out areas are filled to some extent by waste rock or cemented mill tailings.

Longwall mining systems allow for a high abutment pressure to build up in solid ore or coal in advance of the face, a low-pressure zone to exist in the working area just behind the face, and a normal lithostatic pressure to build up again in the mined-out and caved or gob-filled area as the face is moved ahead.

 

Top slice mining

 

Seldom used today, this method has been applied to wide and steeply dipping deposits with weak ore and weak walls. It has been of use in recovering pillars that have been left between filled stopes. It is a relatively expensive and labor-intensive method with a requirement for abundant timber, but it permits nearly total extraction of the ore. Top slicing is ultimately a caving method of mining, but the ore must first be drilled and blasted, and temporary support is needed between the taking of each successive downward slice or horizontal cut of ore. Working begins in drifts and cross-cuts on a mining floor at the top of a raise; after the driving of a series of adjacent cross-cuts so that a slice of sufficient width has been taken, a mat of timber and scrap lumber is laid down on the floor and the supporting timbers are blasted to cave the overlying rock. A new slice is mined laterally from drifts and cross-cuts under the mat, with the mat supported by timber props (stulls). A mat is again laid down, supports are blasted, and subsequent slices are mined beneath the subsiding accumulation of timber mats and waste rock.

 

 

Caving methods

 

These methods are used in large orebodies with relatively weak ore and with weak wallrock that will collapse as the ore is removed. Geologic conditions must permit subsidence, and the ore must be sufficiently jointed or fractured to form fragments small enough to be handled in drawpoints and raises. Ore recovery in mining is generally quite high, but a certain amount of dilution from waste rock must be accepted.

 

Sublevel caving

 

This type is most suited to large and steeply dipping orebodies with weak walls and with ore that has enough stability to maintain sublevels (Fig. 6). It is similar to sublevel open stoping, but in this method the walls and the back are allowed to collapse. The ore is mined in downward increments that are drilled, blasted, and drawn from levels below the ore. Access drifts are driven on the footwall side of the orebody, sublevel cross-cuts are driven in ore, and fans of blastholes are drilled at intervals in the cross-cuts. A steplike succession of slices is mined in retreat from the hanging wall, with the wall rock collapsing and following the extraction of the ore. As each fan of holes is blasted, the broken ore caves into the sublevel, where it is loaded and transported to the ore pass. Broken waste rock fills the void as the ore is drawn. When an excess of waste rock begins to dilute the broken ore, the drawing is stopped and the next fan of holes is blasted.

 

 

Fig. 6  Sublevel caving, with stages of development and mining.

 

 

 

fig 6

 

 

 

 

Block caving

 

This is applied to large and relatively uniform bodies in which both ore and waste will cave readily (Fig. 7). Production on the order of 50,000–75,000 tons (45,000–68,000 metric tons) per day can be achieved at a very low mining cost, but the capital cost of a block-caving mine is high. A mine is prepared for block-caving operations by establishing a principal haulage level, driving raises to production levels (slusher or grizzly levels), and driving a larger number of raises to workings on an undercut level beneath the orebody or block to be mined. Caving is initiated by drilling and blasting a slice of ore above the undercut level and, if necessary, by excavating narrow stopes at the boundaries of the block. With the drawing of the initially broken ore, the block begins to cave under its own weight. With further drawing, the entire column of ore and overburden rock continues to subside and break upward for as much as 4000 ft (1220 m) to the surface, where a depression forms. The ore, broken and crushed in caving, flows through cone-shaped draw holes and finger raises. The finger raises are carefully monitored at draw points on the grizzly level so that the caving action is kept uniform and salient channels of subsiding waste rock are not allowed to form prematurely. Broken ore collected from finger raises reaches the haulage level through transfer raises.  See also: Explosive; Mining; Prospecting

William C. Peters

 

 

Fig. 7  Block caving, with principal haulage level, driving raises to production (grizzly) levels, and raises to workings.

 

 

 

fig 7

 

 

 

 

 

  • R. E. Gertsch and R. L. Bullock (eds.), Techniques in Underground Mining, SME, 1998
  • H. L. Hartman and J. M. Mutmansky, Introductory Mining Engineering, 2002
  • H. L. Hartman (ed.), SME Mining Engineering Handbook, 2 vol., 1992
  • B. Stack, Handbook of Mining and Tunnelling Equipment, 1982
  • K. S. Stout, Mining Methods and Equipment, 1980
  • Cretaceous

     

    During Cretaceous time the breakup of Gondwana, the great late Paleozoic-Triassic supercontinent, became complete (Fig. 2). For pre-Cretaceous time the positions of continents can be roughly derived from the remanent magnetic vectors in their rocks, which record the directions toward and the distance to the poles. But for Cretaceous and later times the positions may be more precisely tracked by the “growth lines” of crustal plates, visible in magnetic maps of the oceanic areas. As the Earth's magnetic field reversed, the continuous growth of ocean floors along the mid-oceanic ridge system occurred alternately in normal and in reversed polarity. Imprinted in the rocks, the remanent magnetism reinforces the present magnetic field above the crust grown in normal polarity and diminishes it over that grown in reversed fields.

     

     

    Fig. ۱  Late Cretaceous global tectonics, showing inferred lithosphere plate configurations with spreading, subduction, and transform boundaries; generalized continental outlines are shown for reference. (After R. H. Dott, Jr., and R. L. Batten, Evolution of the Earth, 3d ed., McGraw-Hill, 1988)

     

     

     

    fig 2

     

     

     

    Laurasia had already separated from Africa by the development of Tethys and became split into North America and Eurasia by the opening of the North Atlantic (though tenuous land connections continued to exist in the far north). These new, deep oceanic areas continued to grow in Cretaceous time. India broke away from Australia and Australia from Antarctica. South America tore away from Africa by the development of the South Atlantic Ocean, while India brushed past Madagascar on its way north to collide with southeast Asia. As these new oceanic areas grew, comparable areas of old ocean floor plunged into the mantle in subduction zones such as those that still ring the Pacific Ocean, marked by deep oceanic trenches and by the development of mountain belts and volcanism on adjacent continental margins (Fig. ۲).  See also: Continents, evolution of; Plate tectonics; Subduction zones

     

     

    Fig. ۲ Schematic view of North America in Cretaceous time. Cretaceous seas are shaded, and Cretaceous sediments in cross section (in the black-and-white strip) are dotted. Note the counterclockwise rotation of the continent shown by the lines of Cretaceous latitude.

     

     

     

    fig 3

     

     

     

    The face of the globe was also affected by changes in sea level. Sea level at times in the early Cretaceous stood at levels comparable to the present, but subsequently the continents were flooded with relatively shallow seas to an extent probably not attained since Ordovician-Silurian times. Maximal flooding, in the Turonian Stage, inundated at least 40% of present land area. Cretaceous seas covered most of western Europe, though old mountain belts such as the Caledonides of Scandinavia and Scotland remained dry and archipelagos began to emerge in the Alpine belt. In America (Fig. 3), seas flooded the southeastern flank of the Appalachian Mountains, extended deep into what is now the Mississippi Valley, and advanced along the foredeep east of the rising Western Cordillera to link at times the Gulf of Mexico with the Arctic Ocean. In the far west, accretionary prisms of subducted Cretaceous deep-water fans and oceanic sediments, partly mixed with ophiolites in the Franciscan melange, became juxtaposed with forearc sediments.

    Large seas extended over parts of Asia, Africa, South America, and Australia. The wide spread of the chalk facies is essentially due to this deep inundation of continents, combined with the trapping of detrital sediments near their mountain-belt sources, in deltas or in turbidite-fed deep-water fans such as the classical Alpine Flysch. At the same time, carbonate platforms were still widespread, and the paratropical dry belts were commonly associated with evaporite deposits.  See also: Paleogeography; Saline evaporites

     

    Tectonic and igneous activity

     

    The North American plate, in the process of separating from Europe, continued to have a western convergent margin of growing mountains, and a southeastern passive margin. Convergent or active margins such as those surrounding the Pacific Ocean (then as now a “ring of fire”) became intruded by great batholiths of granitic composition, such as those of the British Columbia Coast Range, the Sierra Nevada, the Peninsular Ranges of southern and Baja California, and the great Andean batholiths. Above these there accumulated superstructures of andesitic volcanics. Exotic island arc terranes riding on the Pacific plate but resisting subduction came to be welded to this margin of North America. The eastern margin of this Western Cordillera overthrust and incorporated the margin of the subsiding Western Interior Foredeep, presaging development of the Rocky Mountains (Fig. 3). Passive continental margins, such as those bordering the Atlantic, came to be sites of massive sediment accumulations, the classical geosynclines of older literature, from which mountain systems have developed locally as in the Caribbean or have yet to arise.  See also: Geosyncline

    Flood basalts of Cretaceous time include the early Aptian outpourings of basalts on the mid-Pacific floor, perhaps the largest on record. Early Cretaceous emplacement of the Rajmahal basalts of India and Bangladesh was followed by the eruption of the Deccan basalts of India, emplaced during the short magnetic interval (chron 29R) that includes the Cretaceous/Tertiary (K-T) boundary. The beginnings of the “Brito-Arctic” basalts also go back to Maastrichtian time.

     

    Climate and oceans

     

    In parts of early Cretaceous time, ice extended to sea level in the polar regions, as shown by glendonites, concretionary calcite pseudomorphs of the cold-water mineral ikaite; and in marine mudstones containing exotic pebbles, dropstones melted out of icebergs. But during most of Cretaceous time, climates were in the hothouse or greenhouse mode, showing lower latitudinal temperature gradients. Tropical climates may have been much like present ones, and paratropical deserts existed as they do now, but terrestrial floras and faunas suggest that nearly frost-free climates extended to the polar circles as did abundant rainfall, and no ice sheets appear to have reached sea level.

    The cause for these climatic changes may be sought in variations in the heat-retaining character of the atmosphere (abundance of greenhouse gases such as carbon dioxide or methane) or in oscillations of solar luminosity. The hydrologic cycle appears to have been intensified, with more heating and therefore more water evaporation in the tropics, leading to massive transport of water vapor to the polar regions warmed by its condensation.

    With a mean temperature of about 38°F (3°C), the present ocean lies 27°F (12°C) below the mean surface temperature of the Earth. This refrigerator is maintained by the sinking of cold waters in the circumpolar regions. Temperatures calculated from the oxygen isotope ratios in Cretaceous deep-water foraminiferans yield values as high as 62°F (16°C), and suggest an ocean much closer to mean surface temperature. In this ocean circulation, visualized long ago by T. C. Chamberlin, warm saline waters of the dry paratropics were the main source of dense waters and sank to the bottom when only moderately cooled. The implication is not only altered current directions and deep-water temperature regimes but also a diminished oxygen supply to the depths. This diminished oxygen is documented by the widespread development of black shales, deposited on bottoms from which most or all scavengers were excluded by lack of oxygen. The resulting excess burial of organic matter yielded an abundance of petroleum source beds, reflected in the large petroleum reserves in Jurassic and Cretaceous rocks. Occasional episodes of black shale deposition, such as that of the Bonarelli event near the end of the Cenomanian Stage, became circumglobal and buried enough organic matter to alter the carbon isotope ratios in the entire ocean-atmosphere system, but the circumstances of their origin remain unknown.  See also: Oceanography; Oil shale; Paleoclimatology; Petroleum reserves

     

    Life

     

    A walk along a Cretaceous beach or a visit to a surf-beaten cliff would have yielded many snail and bivalve shells and sea urchins differing from living ones only at the level of species. Yet there are some notable differences. Two families of bivalves rose to particular prominence in Cretaceous time. The inoceramids were a widespread and diversified group that developed species 5 ft (1.5 m) wide, the largest of all known clams, while the rudistids came to resemble corals in form and largely replaced corals as reef builders in Cretaceous time. Among cephalopods, ammonites were prominent swimmers in Cretaceous seas, as were belemnites—squids with a heavy calcareous skeleton. The calcareous microplankton had only in latest Jurassic time reached an abundance sufficient to produce widespread chalks, and in the Cretaceous two major elements of this, the prymnesiophyte coccolithophorids and the planktonic foraminiferans, reach maximal species diversity. Bony fishes evolved extensively in Cretaceous time, but prominent among marine predators were reptiles, some of them gigantic. Marine turtles have persisted, the dolphinlike ichthyosaurs died out in Turonian-Coniacian time, while the massive, sea-lion-like plesiosaurs and the lizard-derived mosasaurs lasted to the end of the period. Flightless birds populated some of the late Cretaceous seas.  See also: Bivalvia; Gastropoda; Reptilia

    On land, flowering plants (angiosperms) first appeared in early Cretaceous time, as opportunistic plants in marginal settings, and then spread to the understory of woodlands, replacing cycads and ferns. In late Cretaceous time, evergreen angiosperms, including palms, thus came to dominate the tropical rainforests. Evergreen conifers maintained dominance in the drier midlatitude settings, while in the moist higher latitudes forests of broad-leaved deciduous trees dominated. Grasslands, however, were not developed until Tertiary time. Insects became highly diverse, and many modern families have their roots in the Cretaceous. Amphibians and small reptiles were present. Larger land animals included crocodiles and crocodilelike reptiles, turtles, and dinosaurs. Dinosaurs, derived from reptilian stock in Triassic time, rose to become the largest land animals of all time. The very size of these animals implies complex circulatory, digestive, and respiratory systems unlike those of reptiles. Evidence for temperature control is emerging, and it is speculated that some dinosaurs were feathered. Thus, there is growing support for classification of dinosaurs not as a branch of the class Reptilia but as a separate class. The mammals, another reptilian offshoot in the Triassic, remained comparatively minor elements in the Cretaceous faunas. In early Cretaceous time, egg-laying and marsupial mammals were joined by placentals, but Cretaceous mammals were in general small, and lack of color vision in most modern mammalians suggests a nocturnal ancestry and a furtive existence in a dinosaurian world. Birds had arisen, from dinosaurs in Jurassic time, but their fossil record from the Cretaceous is poor and largely one of water birds. More common are the remains of flying reptiles, the pterosaurs, which in Cretaceous time reached a wingspan of 35 ft (11 m), the largest known flying animals by far.  See also: Dinosauria; Mammalia; Marsupialia; Pterosauria

     

    K/T boundary crisis

     

    Most species of the inoceramid and rudistid bivalves died out in a crisis within the Maastrichtian Stage. Some millions of years later, during the reversed magnetic interval known as chron 29R, a collision with an asteroid or comet showered the entire Earth with impact debris, preserved in many places as a thin “boundary clay” enriched in the trace element iridium. This event coincided with the great wave of extinctions—the K/T crisis—which serve to bound the Cretaceous (Kreide) Period against the Tertiary.

    The Chicxulub crater is located at the northwestern edge of what was then the Yucatán Carbonate Platform and now the Yucatán Peninsula. Buried under some thousands of feet of Tertiary limestone, it forms a geophysical anomaly explored for oil by a number of boreholes. With a diameter of 110 mi (180 km) excluding possible peripheral rings, this is the largest crater known from Phanerozoic time. Like comparable craters on the Moon and Mars, it has a central peak and peripheral ejecta blanket. It is filled with partly melted impact debris (suevite) derived from sediments and the underlying igneous-metamorphic complex. Quartz grains with shock lamellae confirm the impact origin, and abundant glass yields the K/T boundary age of 65 ± 0.5 million years. The ejecta blanket, where exposed at the surface in the Mexico-Belize border country 300 mi (400 km) distant, consists mainly of middle to late Cretaceous carbonates in blocks up to 10 ft (3 m), mixed with carbonate lapilli and altered glass lumps. Rare cobbles of limestone and chert were melted and quenched. In surrounding regions, deeper-water marls of latest Cretaceous and earliest Tertiary age are separated by a few feet of unusual sediment: a thin bed contains chips of limestone, blebs of glass generally altered to clay, and shocked quartz. In the Gulf of Mexico region this is followed by cross-beds interpreted as deposits of a “tidal wave” (tsunami) that swept repeatedly across the Gulf. A centimeters-scale layer of clay, extending around the world, contains microscopic silicates, while electron microscopy reveals crystals of spinel with excessive degrees of oxidation. Shocked quartz, abundant and relatively coarse in America, becomes scarce and fine with distance.

    The iridium content associated with the fallout implies an impactor with a composition similar to that of planetary interiors. The size, estimated at 6 mi (10 km), implies an asteroid or a correspondingly larger comet. Traveling at 16 mi/s (25 km/s), the body would have struck with the explosive force of 1014 tons of TNT. Quite aside from local and regional devastation, global effects must have included earthquake shock many orders of magnitude greater than any found in human history; associated land slips and tidal waves; a dust blackout of sunlight that must have taken many months to clear; a sharp drop in temperatures that would have brought frost to the tropics; changes in atmospheric and water chemistry; and disturbance of existing patterns of atmospheric and oceanic circulation.

    It is possible that earthquakes influenced volcanic eruptions. The first flows of the Deccan basalts predate polarity chron 29R and the impact, but the great body of basalt poured out within that brief chron, possibly emitting enough sulfur to add to the crisis.

    Different biotic communities were affected to different degrees. The pelagic community, sensitive to photosynthetic productivity, was severely struck, with coccolithophores and planktonic foraminiferans reduced to a few species, while ammonites, belemnites, plesiosaurs, and mosasaurs were eliminated. Yet dinoflagellates, endowed with the capacity to encyst under stress, suffered no great loss. Benthic life was only moderately damaged beyond the loss of species, excepting destruction of the reef community. While North American trees underwent far more extinction at the specific level than formerly believed, land floras escaped with little damage, presumably because they were generally equipped to handle stress by dormancy and seed survival. The plant-fodder-dependent dinosaurs perished, as did their predators and scavengers. The fresh-water community, buffered by ground water against temperature change and food-dependent mainly on terrestrial detritus, was little affected. While a great many individual organisms must have been killed by the immediate effects of the impact, the loss of species and higher taxa must have occurred on land and in shallowest waters mainly in the aftermath of darkness, chill, and starvation, and in the deeper waters in response to changed regimes in currents, temperatures, and nutrition.

    The Cretaceous crash led above all to an evolutionary outburst of the mammals, which in the succeeding tens of millions of years not only filled and multiplied the niches left by dinosaurs but also invaded the seas, to become successors to plesiosaurs and mosasaurs. Humans, among others, owe their existence to that devastating event of 65 million years ago.

     

    Alfred G. Fischer

     

    Bibliography

     

     

    • W. Alvarez et al. (eds.), Geochronology. Time Scales and Global Stratigraphic Correlation, SEPM Spec. Publ., no. 54, 1995
    • R. H. Dott, Jr., and D. R. Prothero, Evolution of the Earth, 1992
    • L. A. Frakes, J. E. Francis, and J. I. Syktus, Climatic Modes of the Phanerozoic, 1992
    • J. L. Powell, Night Comes to the Cretaceous, 1998

    Jurassic


     

     

    The system of rocks deposited during the middle part of the Mesozoic Era, and encompassing an interval of time between about 200 and 142 million years ago, based on radiometric dating. It takes its name from the Jura Mountains of Switzerland. Its rich marine invertebrate faunas in western Europe have been the subject of intensive study since the pioneering days of geology in the early nineteenth century, and provided the basis for the fundamental stratigraphic concepts of stages and biozones.  See also: Dating methods

     

    Subdivisions

     

    The Jurassic System is subdivided into 11 stages which, with the exception of the Tithonian, are named from localities in England, France, and Germany (Fig. 1). These, and the much greater number of zones, are based upon ammonites, which are by far the most valuable fossils biostratigraphically because of their high rate of species turnover in time due to rapid evolution and extinction. The most refined stratigraphic subdivisions have been made in the British Isles, with 54 zones and 176 subzones. Because of biogeographic provinciality, with different ammonite taxa inhabiting Boreal and Tethyan realms, difficulties of correlation can occur for younger Jurassic strata; and the youngest stage in the Tethyan Realm, the Tithonian, embracing most of the world, is equivalent to the Volgian stage of the Boreal Realm, extending from northern Eurasia to northern North America. The ammonites of the Volgian are quite different from those of the stratigraphically equivalent Tithonian. In the absence of ammonites, dinoflagellates are the most useful marine fossils for correlation, but in nonmarine strata problems of correlation are considerable, and stratigraphically less satisfactory pollen and spores have to be used.  See also: Stratigraphy

     

     

    Fig. 1  Succession of Jurassic stages, with estimated radiometric ages in millions of years. (After J. Palfy et al., A U-Pb and 40Ar/39Ar time scale for the Jurassic, Can. J. Earth Sci., 37:923–944, 2000)

     

     

     

    fig

     

     

     

     

    Paleogeography and sea level

     

    The main continental masses were grouped together as the supercontinent Pangaea, with a northern component, Laurasia, separated from a southern component, Gondwana, by a major seaway, Tethys, which expanded in width eastward (Fig. 2). From about Middle Jurassic times onward, this supercontinent began to split up, with a narrow ocean being created between eastern North America and northwestern Africa, corresponding to the central sector of the present Atlantic Ocean. At about the same time, and continuing into the Late Jurassic, separation began between the continents that now surround the Indian Ocean, namely Africa, India, Australia, and Antarctica. As North America moved westward, it collided with a number of oceanic islands in the eastern part of the PaleoPacific. Because the impingement was an oblique one, there was a general tendency for these accreted landmasses to be displaced northward along the cordilleran zone of the subcontinent. Other examples of so-called displaced terranes are known on the Asian side of the North Pacific, and some of the accretion of oceanic islands took place in Jurassic times.

     

     

    Fig. 2  Approximate distribution of land and sea in the Oxfordian stage. Small islands are excluded, but boundaries of modern continents are included as a reference.

     

     

     

    fig 2

     

     

     

    There were also important paleogeographic changes later in the period involving the Tethys zone. An older, so-called Palaeotethys was progressively closed as an extensive, narrow continent known as Cimmeria, extending east-west, and collided with the southern margin of Eurasia. The name comes from the Crimean Peninsula of Russia, where there is well-displayed evidence of an intra-Jurassic orogenic disturbance indicative of continental collision.  See also: Orogeny; Paleogeography

    Sea level rose progressively through the period, with a corresponding flooding of the continents by shallow epeiric seas, that is, shallow seas that covered part of the continents but remained connected to the ocean. At the beginning, such seas covered less than 5% of the continents, but near the end, in Oxfordian and Kimmeridgian times, they covered approximately 25% (Fig. 2). The Jurassic sea-level curve also shows a succession of smaller-scale changes, of a duration of a few million years. Some of these, such as the Early Toarcian sea-level rise, are clearly global or eustatic, but others are more controversial and may reflect regional tectonic activity rather than truly global phenomena. It is uncertain by how much the sea level rose during the course of the period; but by using a hypsometric method, an estimate of between 330 and 500 ft (100 and 150 m) can be made.  See also: Paleoceanography

     

    Climate

     

    The climate of Jurassic times was clearly more equable than at present, as indicated by two sets of facts. The first concerns the distribution of fossil organisms. Thus a number of ferns whose living relatives cannot tolerate frost are distributed over a wide range of paleolatitudes, sometimes as far as 60° N and S. Similarly, coral reefs, which are at present confined to the tropics, occur in Jurassic strata in western and central Europe, beyond the paleotropical zone. Many other groups of organisms had wide latitudinal distribution, and there was much less endemism (restriction to a particular area) with respect to latitude than there is today. The second set of facts concerns the lack of evidence for polar icecaps, such as extensive tillites or striated pavements.

    However, there must have been strong seasonal contrasts of temperature within the Pangean supercontinent, and climatic modeling suggests winter temperatures at zero Celsius at or close to the paleopoles. A limited amount of evidence from northern Siberia and arctic North America, in the form of apparent glacial dropstones and glendonites, suggests the possibility of some ice, but this ice is likely to have been seasonally transient and small in volume.

    There is no evidence of any significant change in the temperature regime through the Jurassic, but there are indications of a change in the humidity-aridity spectrum. Unlike the present, there were no tropical rainforests. Instead, a large area of western Pangea experienced an arid to semiarid climate in low latitudes, especially at some distance from the ocean. Precipitation is likely to have been dominantly monsoonal rather than zonal, a pattern unlike that of today. For most of the period, the continental area represented today by Eurasia had a comparatively humid climate, as indicated in nonmarine sediments by coals and the abundance of the clay mineral kaolinite. Toward the end of the Jurassic, however, there was a change to a more arid climate, indicated by the disappearance of coals and kaolinite and the occurrence of evaporites such as rock salt and gypsum. The reason for this change is unclear, but it may be bound up with a rainshadow effect created by the collision of the Cimmerian continent.  See also: Paleoclimatology; Saline evaporites

     

    Tectonics and volcanicity

     

    Most of Pangea experienced tensional tectonics as the supercontinent began to break up. This is manifested by graben and half-graben structures, with associated alkaline volcanicity. By far the largest flood basalt province is that of the Karoo in South Africa, most of the basalts and associated igneous rocks being erupted in the Early Jurassic, prior to the breakup of Africa, Madagascar, and India. The Middle Jurassic Ferrar dolerites of Victoria Land, Antarctica, and the contemporaneous Tasmanian dolerites are further manifestations of tensional tectonics, as are earliest Jurassic basalts in eastern North America and Morocco, again signifying tension prior to the Atlantic opening. The North Sea region of western Europe is in effect an aborted oceanic rift, with a major phase of tensional activity and associated volcanicity in the Middle and Late Jurassic. This did not lead, however, to the creation of true ocean.  See also: Basalt; Graben

    Compressional tectonics associated with subduction of ocean floor took place in many parts of the Pacific margins, with associated calc-alkaline volcanicity. An excellent example is the Andes. The North Pacific margins were also associated with significant strike-slip faulting bound up with the accretion of displaced terranes. The other important zone of compressional tectonics was along the southern margin of Eurasia, and is involved with the collision of the Cimmerian continent.  See also: Fault and fault structures

    Since it is not plausible to invoke the melting and freezing of polar ice caps to account for Jurassic sea-level change, this change must be bound up with tectonic activity. The most plausible mechanism for accounting for long-term sea-level rise is the growth of oceanic ridges, displacing seawater onto the continents, but the cause of short-term sea-level changes is more obscure and remains controversial.  See also: Continents, evolution of; Geosyncline; Mid-Oceanic Ridge; Plate tectonics; Subduction zones

     

    Vertebrate fauna

     

    The vertebrate terrestrial life of the Jurassic Period was dominated by the reptiles. The dinosaurs had first appeared late in the Triassic from a thecodont stock, which also gave rise to pterosaurs and, later, birds. From small bipedal animals such as Coelophysis, there evolved huge, spectacular creatures. These include the herbivorous Apatosaurus, Brontosaurus, Brachiosaurus, Diplodocus, and Stegosaurus as well as the carnivorous, bipedal Allosaurus. Only two rich dinosaur faunas are known from Jurassic deposits, the Morrison Formation of the United States Western Interior and the approximately contemporary Tendaguru Beds of Tanzania. The two faunas are strikingly similar at family and generic level, which strongly suggests that free land communications existed between western North America and East Africa until quite late in the period, a fact that is not easy to reconcile with some paleogeographic reconstructions.  See also: Dinosauria

    Flying animals include the truly reptilian pterosaurs and the first animals that could be called birds as distinct from reptiles, as represented by the pigeon-sized Archaeopteryx. There were two important groups of reptiles that lived in the sea, the dolphinlike ichthyosaurs and the long-necked plesiosaurs. Both of these groups had streamlined bodies and limbs beautifully adapted to marine life. Turtles and crocodiles are also found as fossils in Jurassic deposits.  See also: Archaeopteryx; Pterosauria

    Jurassic mammals, known mainly from their teeth alone, were small and obviously did not compete directly with the dinosaurs. They included a number of biologically primitive groups such as the triconodonts, docodonts and multituberculates. The fish faunas were dominated by the holosteans, characterized by heavy rhombic scales. Their evolutionary successors, the teleosts, probably appeared shortly before the end of the period.  See also: Docodonta; Holostei; Multituberculata; Teleostei; Eutriconodonta (Triconodonta)

     

    Invertebrate fauna

     

    Because they are far more abundant, the invertebrate fossil faunas of the sea are of more importance to stratigraphers and paleoecologists than are the vertebrates. By far the most useful for stratigraphic correlation are the ammonites, a group of fossil mollusks related to squids. They were swimmers that lived in the open sea, only rarely braving the fluctuating salinity and temperature of inshore waters. They are characteristically more abundant in marine shales and associated fine-grained limestones. From a solitary family that recovered from near extinction at the close of the Triassic, there radiated an enormous diversity of genera. Many of these were worldwide in distribution, but increasingly throughout the period these was a geographic differentiation into two major realms. The Boreal Realm occupied a northern region embracing the Arctic, northern Europe, and northern North America. The Tethyan Realm, with more diverse faunas, occupied the rest of the world.  See also: Limestone; Shale

    In most facies the bivalves, which flourished in and on shallow, muddy sea bottoms, are the most abundant and diverse of the macrofauna. They included many cemented forms such as Ostrea, recliners such as Gryphaea, swimmers such as the pectinids and limids, and rock borers such as Lithophaga. However, the majority were burrowers: either relatively mobile, shallow burrowers or forms occupying deep permanent burrows and normally still found in their positions of growth.  See also: Bivalvia; Facies (geology)

    Brachiopods were much more abundant and diverse than they are today. The range of depths below the sea surface that they occupied is far wider than for the bivalves, and a definite depth zonation can be established in Europe, just as with the ammonites.  See also: Brachiopoda

    Echinoderms are best represented as fossils by the crinoids and echinoids, and were all inhabitants of shallow seas, unlike some of the modern representatives of this class. The echinoids include both primitive regular forms, such as the cidaroids, and irregular forms, such as Clypeus and Pygaster.  See also: Echinodermata; Pygasteroida

    Corals belonged to the still extant Scleractinia group and included reef builders such as Isastrea and Thamnasteria. Calcareous and siliceous sponges are also common locally, even forming reefs. It seems likely that the siliceous sponges inhabited somewhat deeper water than the corals.  See also: Scleractinia; Sclerosponge

    The invertebrate microfaunas are represented by abundant foraminifera, ostracods, and radiolaria. Foraminifera and ostracods are of great value to oil companies in correlation studies.  See also: Ostracoda; Radiolaria

    Not all Jurassic invertebrates lived in the sea. Some lived in continental environments such as lakes and rivers; they include a few genera of bivalves, gastropods, and arthropods. These faunas are far less diverse than their marine counterparts.  See also: Arthropoda; Gastropoda; Paleontology

     

    Flora

     

    With regard to the plant kingdom, the Jurassic might well be called the age of gymnosperms, the nonflowering “naked seed” plants, forests of which covered much of the land. They included the conifers, gingkos, and their relatives, the cycads. Ferns and horsetails made up much of the remainder of the land flora. These and others of the Jurassic flora are still extant in much the same forms.  See also: Cycadales; Ginkgoales

    Remains of calcareous algae are widely preserved in limestone. Besides the laminated sedimentary structures produced by what have traditionally been regarded as blue-green algae but are actually cyanobacteria, and known as oncolites and stromatolites, there are skeletal secretions of other groups. Some of these are benthic forms, but many pelagic limestones are seen under the electron microscope to be composed largely of tiny plates of calcite, known as coccoliths, which are secreted by certain planktonic algae also called coccoliths.  See also: Algae; Cyanobacteria; Stromatolite

    It seems likely that the Late Jurassic saw the emergence of the flowering plants, the angiosperms, since well-developed forms of this group existed in the Early Cretaceous. However, it is not quite understood how they emerged, and a satisfactory direct evolutionary ancestor has yet to be identified with certainty.

     

    Economic geology

     

    Jurassic source rocks in the form of organic-rich marine shale and associated rocks contain a significant proportion of the world's petroleum reserves. A familiar example is the Upper Jurassic Kimmeridge Clay of the North Sea, and its stratigraphic equivalents in western Siberia. Some of the source rocks of the greatest petroleum field of all, in the Middle East, are also of Late Jurassic age.  See also: Mesozoic; Petroleum geology

     

    A. Hallam

     

    Bibliography

     

     

        • W. J. Arkell, Jurassic Geology of the World, 1956
    • J. W. C. Cope et al., Jurassic, pts. 1 and 2, Geol. Soc. Lond. Spec. Rep. 14 and 15, 1980
    • A. Hallam, Jurassic climates as inferred from the sedimentary and fossil record, Phil. Trans. Roy. Soc. Lond., B 341:287–296, 1993
    • A. Hallam, Jurassic Environments, 1975
    • A. Hallam, A review of the broad pattern of Jurassic sea-level changes and their possible causes in the light of current knowledge, Palaeogeog., Palaeoclimatol., Palaeoecol.,

    Triassic

     

     

    The oldest period of the Mesozoic Era, encompassing an interval between about 248 and 206 million years ago (Ma). It was named in 1848 by F. A. von Alberti for the threefold division of rocks at its type locality in central Germany, where continental redbeds and evaporites of the older Buntsandstein and younger Keuper formations are separated by marine limestones and marls of the Muschelkalk formation. These carbonates were laid down in a shallow tongue of the Tethys seaway that extended from the Himalayas through the Middle East to the Pyrenees, where more than 10,000 ft (3000 m) of carbonate were deposited. The German section was an unfortunate choice because it is atypical of other Triassic sections and carries a sparsely preserved fossil record. It was subsequently replaced by a marine carbonate sequence in the Alps as the standard for global Triassic reference and correlation. The North American standard marine section is in the western Cordilleras of British Columbia and the Sverdrup Basin of the Arctic.  See also: Mesozoic

     

    Major events

     

    Triassic strata record profound paleontologic changes that reflect major physical changes in Earth history. Two of the five most catastrophic extinctions of the Phanerozoic Eon mark the beginning and end of the Triassic. More than 50% of all Permian families died out at the beginning of the period, including 85–90% of all marine species and 75% of land species; and more than 50% of all marine genera became extinct at the end of the period. The Triassic was also when many new families of plants and animals evolved, including the earliest known mammals.

    As a very brief interval of geologic time (about 40 million years), the Triassic Period uniquely embraces both the final consolidation of Pangaea and the initial breakup of the landmass, which in the Middle Jurassic led to the opening of the Central Atlantic Ocean and formation of modern-day continental margins. The Triassic marks the beginning of a new Wilson cycle of ocean-basin opening through lithospheric extension and oceanic closing through subducting oceanic lithospheres along continental margins. The cycle was named for J. Tuzo Wilson, a pioneer of modern plate tectonic theory. The initial breakup of Pangaea occurred in the western Tethys (precursor of the Mediterranean Sea) between Baltica and Africa and in eastern Greenland between Baltica and the North American craton. Rifting then proceeded into the Central Atlantic, separating the North American and African cratons that led to the separation of Laurasia from Gonwanaland (Fig. 1). Rifting also occurred in Argentina, east Africa, and Australia. In the central Atlantic region, extensional tectonics was accompanied by a huge outpouring of continental flood basalts, forming the Central Atlantic magmatic province (CAMP), whose remnants are now found as feeder dikes and flood basalts on four circum-Atlantic continents, separated by thousands of miles of younger basalts of the oceanic crust (Fig. 2a).  See also: Lithosphere; Plate tectonics

     

     

    Fig. 1  Paleogeography of the Late Triassic Period: after the accretion of south China and Cimmeria (Turkey, Iran, and Tibet) to Laurasia; during the Incipient rifting of Pangaea in eastern North America and northwest Africa along the Allegheny-Mauritanide-Variscan orogeny; and concurrent with oceanic subduction and formation of deep-sea trenches and magmatic arc along the western plate boundary of North America. (After R. K. Bambach, C. R. Scotese, and A. M. Zlegler, Before Pangea: The geographics of the Paleozoic world, Amer. Sci. 68:26–38, 1980)

     

     

     

    fig 1

     

     

     

     

    Fig 2. 

     

    fig 2

     

     

    Final consolidation of Pangaea

     

    The initial consolidation of Pangaea, which was marked by the formation of the Allegheny-Mauritanide-Variscan mountain chain in the middle Carboniferous (320 Ma), resulted from the collision of Gondwanaland and the combined Laurasia-Baltica-Siberian-Kazakhstania landmass (Fig. 1). Major plate accretion continued into the Middle-to-Late Triassic (230 ± 5 Ma), when southern China and Cimmeria (Asia Minor) were sutured to the northern margin of the Tethys seaway. Smaller terranes, called suspect or exotic, were also accreted to the western margin of North America at this time. Disconnected patches of Triassic strata occur from California through western British Columbia into Alaska, where they appear to be displaced island-arc terranes, microcontinents, and ocean-ridge segments, as inferred from paleomagnetic data in the lavas and by the exotic character of their Permian faunas.  See also: Paleogeography; Paleomagnetism

     

    Pangaean supercontinent

     

    The final phase of deformation produced a broadly convex continental plate that extended from the north to the south paleo poles, covered about 25% of the Earth's surface, and was surrounded by a global ocean called Panthalassa. It had a central arch standing about 1 mi (1.6 km) high and an average elevation of more than 4300 ft (1300 m) above the early Mesozoic sea level (Fig. 1). Because of its size, location, and pronounced orographic peaks that probably rivaled the Himalayas, the Pangaea landmass had a major impact on global climates. During the Middle Triassic, Florida lay about 5° south of the Equator, whereas Grand Banks (now off southeastern Newfoundland) was located about 20°N. Pangaea's climatic zones ranged from tropical savanna along its extensive coasts to arid and semiarid across its vast interior.  See also: Desert; Savanna; Supercontinent

    As the plate migrated north, transgressing about 10° of latitude between the Middle Triassic and Middle Jurassic, the plate was subjected to increased aridity as it moved under the influence of the subtropical high-pressure cell. Because of its large size, the landmass must have been subjected to monsoon circulation. Winters along the future central Atlantic probably were dominated by subtropical high-pressure cells bringing in cool dry air from aloft, whereas summers were dominated by equatorial low-pressure systems bringing in warm moist air from the Tethys seaway to the east. As moist air was uplifted almost 1.2 mi (2 km) over the Alleghenian-Variscan chain, it would have cooled adiabatically, yielding rainwater that fed major rivers (for example, the Congo River) flowing thousands of miles away from the axis of uplift across broad alluvial plains to the coastal regions of Alaska, Patagonia, India, and Siberia.  See also: Monsoon meteorology

    With the onset of rifting in the Late Triassic and subsequent topographic changes, small ephemeral streams flowed into the rift valleys, creating huge lakes that may have been comparable in size to present Lake Tanganyika of the East African rift system. Where air masses descended into low-lying rift basins, along the Central Atlantic axis, they warmed adiabatically, causing evaporation and precipitation of evaporite minerals (for example, halite, gypsum, and anhydrite) in marginal epicontinental seas and in continental lacustrine basins. The Triassic and Lower Jurassic lake deposits show a pervasive cyclical pattern of wetting and drying, wherein lakes expanded and contracted with periodicities of 21,000, 42,000, 100,000, and 400,000 years. These intervals agree with the Holocene Milankovitch astronomical theory of climates that are related to small variations in the Earth's orbit and rotation.  See also: Basin; Jurassic; Rift valley; Saline evaporites

     

    Crustal extension

     

    The most important tectonic event in the Mesozoic Era was the rifting of the Pangaea craton, which began in the Late Triassic, culminating in the Middle Jurassic with the formation of the Central Atlantic ocean basin and the proto-Atlantic continental margins [Fig. 2(b)]. Rifting began in the Tethys region in the Early Triassic, and progressed from western Europe and the Mediterranean into the Central Atlantic off Morocco and eastern North America by the Late Triassic. As crustal extension continued throughout the Triassic, the Tethys seaway spread farther westward and inland. Although marine palynomorphs from deep wells on Georges Bank indicate that epicontinental seas, from Tethys on the east or Arctic Canada (through eastern Greenland) on the north, transgressed the craton to the coast of Massachusetts in the Late Triassic, an ocean sea floor did not form in this region until the Middle Jurassic. By that time, rifting and sea-floor spreading extended into the Gulf of Mexico, separating North and South America. Africa and South America did not separate until the Early Cretaceous, when sea- floor spreading created the South Atlantic ocean basin, the great flood basalts of the Amazon and Karoo (Africa), and those of Transarctic and Tasmania record that Gondwanaland had begun to break up by the Triassic Period.  See also: Basalt; Cretaceous; Palynology

     

    Atlantic rift basins

     

    Continental rift basins, passive continental margins, and ocean basins form in response to divergent stresses that extend the crust. Crustal extension, as it pertains to the Atlantic, embraces a major tectonic cycle marked by Late Triassic–Early Jurassic rifting and Middle Jurassic to Recent (Holocene) drifting. The rift stage, involving heating and stretching of the crust, was accompanied by uplift, faulting, basaltic igneous activity, and rapid filling of deep elongate rift basins. The drift stage, involving the slow cooling of the lithosphere over a broad region, was accompanied by thermal subsidence with concomitant marine transgression of the newly formed plate margin. The transition from rifting to drifting, accompanied by sea-floor spreading, is recorded by the postrift unconformity (Fig. 3). Late Triassic Proto-Atlantic rift basins occur in eastern North America, Greenland, the British Isles, north and central West Africa, and South America.  See also: Continental drift; Continental margin; Holocene; Unconformity

     

     

    Fig. 3  Diagrammatic cross section of the Atlantic-type continental passive margine of North America and North Africa, taken at the beginning of the Middle Jurassic with the onset of sea-floor spreading that resulted from crustal thinning and mantie upwelling Note the setting of the Late Triassio-Early Jurassic continental and marine rift basins and their relation to the future passive margins, the postrift unconformity, and the overtying Middle Jurassic drift sequence. (After W. Manapelzer, ed., Triassic-Jurassic Rifting: Continental Breakup and the Origin of the Atlantic Ocean and Passive Margins, pt. A, Elsevier, 1988)

     

     

     

    fig 3

     

     

     

    Within the proto-Atlantic, off eastern North America and Morocco, lie about 50 northeast- to southwest-trending elongate rift basins, called the Newark rift basins, whose trend follows the fabric of the Alleghenian-Variscan orogen (Fig. 2). Some of these basins are exposed on the land, while others occur beneath the Coastal Plain and under the continental shelf. Almost all of them have developed along reactivated late Paleozoic thrust faults (Fig. 3). Seismic reflection surveys of both the onshore and offshore rift basins show that they are asymmetric half-grabens, bounded on one side by a system of major high-angle normal faults, and on the other side by a gently sloping basement with sedimentary overlap. These basins contain Late Triassic to Early Jurassic strata, which comprise the Newark Supergroup. At the end of the Triassic and into the Early Jurassic, the Newark strata of the Atlantic region were uplift, tilted, faulted, and intruded by tholeiitic sills and dikes. Subsequently, they were eroded and unconformably overlain by younger Jurassic post rift or drift strata. This episode of deformation, known as the Palisade disturbance, is most evident by the postrift unconformity in the offshore basins.  See also: Fault and fault structures; Graben

    Figure 2, showing a predrift paleogeographic reconstruction of the circum-Atlantic region, outlines the major Triassic basins and lithofacies. Two major basin types are recognized (Fig. 3): Newark-type detrital basins, which are exposed onshore as half-grabens and contain a thick (approximately 2.5–5 mi or 4–8 km) sequence of fluvial-lacustrine strata and border fanglomerates; and evaporite basins, which occur seaward of the string of detrital basins and contain a thick evaporite facies with interbeds of red mudstones and carbonates. As more than 3300 ft (1000 m) of salt was concentrated, these basins must have acted as huge evaporating pans. The Triassic-Jurassic systemic boundary, throughout the broad region of the Atlantic, typically is marked by tholeiitic lava flows and intrusives that are dated about 200 Ma (Early Jurassic), or only slightly older than the oldest dated crust of the Atlantic Ocean.  See also: Facies (geology)

     

    Central Atlantic magmatic province

     

    The breakup of Pangaea was accompanied by the most extensive outpouring of continental basaltic lava known, covering an area estimated to be about 4 million mi2 (10 million km2). Basaltic remnants (flood basalts and feeder dikes) of this igneous province, named the Central Atlantic Magmatic Province (CAMP), are found on the rifted margins of four circum-Atlantic continents, particularly eastern North America, South America, western Africa, and southwestern Europe [Fig. 2(a)]. Almost all of CAMP rocks are mafic tholeoiites that were intruded into or extruded onto clastic rocks in Newark-type rift basins. The Palisades Sill, along the west shore of the lower Hudson River in Northern New Jersey, is an example of this magmatic event. It is thought that the immensely thick and widespread seaward-dipping basaltic wedges, manifested by the East Coast magnetic anomaly, are linked to CAMP.  See also: Geomagnetism

    Recent multidisciplinary studies in stratigraphy, palynology, geochronology, paleomagnetism, and petrography indicate CAMP formed as a singular episodic event in Earth's history, occurring during a very brief interval of geologic time, perhaps no longer than 4 million years. Importantly, this event occurred about 200 Ma and was contemporaneous with widespread mass extinction at the Triassic-Jurassic boundary. A causal relationship is postulated by many scientists to climate change that was forced by emission of huge quantities of volcanic gasses, estimated by researchers to be in the order of from 1–5 × 1012 metric tons. Radical shifts in climate due to the ejection of aerosols into the atmosphere and destruction of environments by lava flows, ash falls, fires, and toxic pollution of soil and streams are suggested consequences of this event. A similar explanation has been offered for the mass extinctions that occurred at the end of the Paleozoic and Mesozoic Eras, with major volcanic eruptions of the Siberian Traps and Deccan Traps, respectively.

     

    Western North America

     

    Permian-to-Triassic consolidation of Pangaea in western North America led to the Sonoma orogeny (mountain building), which resulted from overthrusting and suturing of successive island-arc and microcontinent terranes to the western edge of the North American Plate. However, toward the end of the Triassic Period, as crustal extension was occurring in the Central Atlantic region, the plate moved westward, overriding the Pacific Plate along a reversed subduction zone. This created, for the remainder of the Mesozoic Era, an Andean-type plate edge with a subducting sea floor and associated deep-sea trench and magmatic arc. These effects can be studied in the Cordilleran mountain belt, from Alaska to California, where great thicknesses of volcanics and graywackes were derived from island arcs to the west, and in Idaho and eastern Nevada, where thick Lower Triassic marine limestones and sandstones were laid down adjacent to the rising Cordilleras on the west and interfinger with continental redbeds derived from the stable interior to the east.  See also: Cordilleran belt; Limestone; Orogeny; Redbeds; Sandstone

    As the epicontinental seas regressed westward, nonmarine fluvial, lacustrine, and windblown sands were deposited on the craton. Today many of these red, purple, ash-gray, and chocolate-colored beds are some of the most spectacular and colorful scenery in the American West. For example, the Painted Desert of Arizona, known for its petrified logs of conifer trees, was developed in the Chinle Formation, and the windblown sands of the Wingate and Navajo formations are exposed in the walls of Zion National Park in southern Utah.  See also: Petrified forests

     

    Life

     

    The Triassic is bracketed by two major biotic crises that terminated many groups of organisms. Triassic marine faunas can be distinguished from their predecessors by the absence of groups that flourished in the Permian, such as the fusulinid foraminiferans, the tabulate and rugose corals, the trepostome and cryptostome bryozoans, the productid and other brachiopod groups, the trilobites, and certain groups of echinoderms. Owing to a very low stand of sea level, Early Triassic marine faunas are not common, and show very small diversity except for ammonites. This is partly ecologic. The reef community, for example, is not known from the Early Triassic deposits; yet when it reappeared in mid-Triassic time, it contained sponges that were major members of Permian reefs, and that must have survived in settings that have not been found.  See also: Brachiopoda; Bryozoa; Echinodermata; Foraminiferida; Fusulinacea; Permian; Rugosa; Tabulata; Trilobita

    Triassic faunas are also distinguished from earlier ones by newly evolved groups of plants and animals. In marine communities, molluscan stocks proliferated vigorously. Bivalves diversified greatly and took over most of the niches previously occupied by brachiopods; ammonites proliferated rapidly from a few Permian survivors. The scleractinian (modern) corals appeared, as did the shell-crushing placodont reptiles and the ichthyosaurs. In continental faunas, various groups of reptiles appeared, including crocodiles and crocodilelike forms, the mammallike reptiles, and the first true mammals, as well as dinosaurs.  See also: Cephalopoda; Crocodylia; Dinosauria; Mammalia; Mollusca; Placodontia; Scleractinia

    The Jurassic faunas lack numerous stocks lost in the Rhaeto-Liassic faunal crises. These include survivors of the Permian crises, such as the orthoceratid cephalopods and the conodonts. However, stocks that had flourished greatly in the Triassic also became extinct (phytosaurs, placodonts) or nearly extinct: ammonites were reduced to one or two surviving lineages, which then underwent no other great evolutionary surge in Jurassic time. Furthermore, new groups such as the plesiosaurs and pterosaurs appeared. Triassic land plants contain survivors of many Paleozoic stocks, but the gymnosperms became dominant and cycads appeared. The Permo-Triassic and Rhaeto-Liassic crises record a severe stressing of the biosphere, but the nature and origin of these stresses have not been established.  See also: Conodont; Cycadeoidales; Extinction (biology); Index fossil; Paleobotany; Paleoecology; Paleontology; Pinophyta; Pterosauria

    Warren Manspeizer

     

     

     

    Bibliography

     

     

    • A. Hallam, The end-Triassic bivalve extinction event, Paleogeo. Paleoclimatol. Paleoecol., vol. 35, pp. 1–44, 1981
    • W. E. Hames et al. (eds.), The Central Atlantic Magmatic Province: Insights from Fragments of Pangea, American Geophysical Union, Washington, D.C., 2003
    • G. D. Klein (ed.), Pangea: Paleoclimate, Tectonics, and Sedimentation During Accretion, Zenith, and Breakup of a Supercontinent (Spec. Pap. No. 288), The Geological Society of America, Boulder, Colorado, 1994
    • P. M. Letournea and P. E. Olsen (eds.), The Great Rift Valleys of Pangea in Eastern North America, vol. 1: Tectonics, Structure and Volcanism, Columbia University Press, New York, 2003
    • W. Manspeizer (ed.), Triassic-Jurassic Rifting: Continental Breakup and the Origin of the Atlantic Ocean and Passive Margins, pt. A, Elsevier Science, Amsterdam, 1988
    • D. R. Prothero and R. H. Dott, Evolution of the Earth, 7th ed., McGraw-Hill, New York, 2004
    • S. M. Stanley, Earth System History, Freeman, New York, 1999 

    Additional Readings

     

     

    • Paleomap Project
    • Permian-Triassic Extinction
    • Triassic Period
    • Triassic-Jurassic Working Group
    • Ecology of the Triassic

     

    Ordovician

    The second-oldest period in the Paleozoic Era. The Ordovician is remarkable because not only did one of the most significant Phanerozoic radiations of marine life take place (early Middle Ordovician), but also one of the two or three most severe extinctions of marine life occurred (Late Ordovician). The early Middle Ordovician radiation of life included the initial colonization of land. These first terrestrial organisms were nonvascular plants. Vascular plants appeared in terrestrial settings shortly afterward.  See also: Geologic time scale

    The rocks deposited during this time interval (these are termed the Ordovician System) overlie those of the Cambrian and underlie those of the Silurian. The Ordovician Period was about 7 × 107 years in duration, and it lasted from about 5.05 × 108 to about 4.35 × 108 years ago.

    The British geologist Charles Lapworth named the Ordovician in 1879, essentially as a resolution to a long-standing argument among British geologists over division of the Lower Paleozoic. Until that time, one school of thought, that of R. I. Murchison and his followers, had maintained that only a Silurian Period encompassed the lower part of the Paleozoic. Adam Sedgwick and his followers advocated that two intervals, the Cambrian and the Silurian, could be recognized in the Lower Paleozoic. By 1879 Lapworth observed that “three distinct faunas” had been recorded from the Lower Paleozoic, and he pointed out that each was as “marked in their characteristic features as any of those typical of the accepted systems of later age.”

    To the stratigraphically lowest and oldest of the three, Lapworth suggested in 1879 that the appellation Cambrian be restricted. To the highest and youngest, Lapworth stated that the name Silurian should be applied. To the middle or second of three, Lapworth gave the name Ordovician, taking the name from an ancient tribe renowned for its resistance to Roman domination.

    The type area for the Ordovician System is those parts of Wales and England that include rocks bearing the fossils that composed the second of the three major Lower Paleozoic faunas cited by Lapworth. The Ordovician System in Britain was divided into six major units called series, each distinguished by a unique fossil fauna. The time intervals during which each series formed are epochs. From oldest to youngest, the epochs and series of the British Ordovician are Tremadoc, Arenig, Llanvirn, Llandeilo, Caradoc, and Ashgill. Each of them has a type area in Britain where their characteristic faunas may be collected.

    Intervals of shorter duration than those of the epoch are recognized as well in Britain. One set of such intervals is based on the evolutionary development of the fossils called graptolites. These intervals are the graptolite zones recognized by Lapworth and his associates Ethel M. R. Wood and Gertrude Elles. Each graptolite zone was about 3 × 106 to 5 × 106 years in duration. The boundary between the Ordovician and superjacent Silurian System has been designated as the base of the Parakidograptus acuminatus graptolite zone by international agreement. The type locality for that boundary is at Dob's Linn, near Moffat, southern Scotland. Black, graptolite-bearing shales are exposed there.

    The Ordovician System is recognized in nearly all parts of the world, including the peak of Mount Everest, because the groups of fossils used to characterize the system are so broadly delineated. The British epochs and zones may not be recognized in all areas where Ordovician rocks are found because the fossils used to characterize them are limited to certain geographic areas. Biogeographic provinces limited the distribution of organisms in the past to patterns similar to those of modern biogeographic provinces. Three broadly defined areas of latitude—the tropics, the midlatitudes (approximately 30–60°S), and the Southern Hemisphere high latitudes—constitute the biogeographic regions. Provinces may be distinguished within these three regions based upon organismal associations unique to each province. Epochs and zones are limited to a single region, and consequently each region has a unique set of epochs and zones for the Ordovician. 

     

    Dynamic interrelationships

     

    The Earth's crust is essentially a dynamic system that is ceaselessly in motion. Plate positions and plate motions are linked closely with, and potentially exert a primary driving force that underlies, ocean circulation, ocean-atmosphere interactions, climates and climate change, and expansion and reduction of environments. Life responds to these physical aspects of the Earth's crust.

    Several lines of evidence, including remanent magnetism, distributions of reefs and other major accumulations of carbonate rocks, positions of shorelines, and sites of glacial deposits, may be used to deduce many aspects of Ordovician paleogeography and paleogeographic changes. The Ordovician configuration of land and sea was markedly different from today. Much of the Northern Hemisphere above the tropics was ocean. The giant plate Gondwana was the predominant feature of the Southern Hemisphere. Modern Africa and South America were joined and occupied most the Southern Hemisphere high latitudes. The South Pole lay approximately in north-central Africa. A massive lobe of the plate extended northward from eastern Africa into the tropics. The modern Middle East, Turkey, India, Antarctica, and Australia constituted much of that huge lobe. A number of small plates lay on the margins of Gondwana. Certain of them may have been joined to Gonwana, and others were close to it. Some of these high-latitude plates included Perunica (modern Czech Republic); Avalonia (possibly in two parts, an eastern and a western), which included parts of Wales, southern Britain, Newfoundland, and Maritime Canada; and a number of plates that today make up southern Europe, including those found in the Alps, those that constitute the Iberian Peninsula, and those that made up Armorica (much of France). Plates that were within about 30–55°S latitude included Baltica (modern Scandinavia and adjacent eastern Europe east to the Urals), the Argentine Precordillera, South China, Tarim (in Asiatic China), the Exploits, and perhaps similar small plates. Parts of the Andes within modern northern Argentina, Peru, and Bolivia were within this midlatitudinal interval. Plates in tropical latitudes included Laurentia (modern North America, Greenland, Scotland, and some of northern Ireland), North China, Siberia, one or more plates that made up the Kazakh plate, and several plates that were close to or attached to northern or tropical Gondwana (these make up modern southeastern Asia and southeastern China).  See also: Paleogeography; Paleomagnetism; Plate tectonics

    During the early part of the Ordovician (Tremadoc-Arenig), prior to a significant number of plate movements, siliclastic materials (sand, silts, muds) spread northward from a Gondwana landmass into river, delta, and nearshore marine environments on the Gondwana plate and on those plates close to it, especially those in high latitudes. Coeval tropical environments were sites of extensive carbonate accumulations. Most midlatitude plates were sites of siliclastic and cool-water carbonate deposition.

    Extensive plate motions and major volcanic activity at the margins of many plates characterize the Arenig-Llanvirn boundary interval of the early Middle Ordovician. Many plates on the Gondwanan margins began a northward movement that continued for much of the remainder of the Paleozoic. In addition, Laurentia bulged upward to such an extent that marine environments, which had covered most of the plate early in the Ordovician, were driven to positions on the plate margins. The Avalonian plates joined and moved relatively quickly northward to collide with the eastern side of Laurentia near the end of the Ordovician. Prior to that collision, the Popelogan or Medial New England plate collided with the Laurentian plate at about the position of modern New England. That collision, which occurred about 455 million years ago, classically has been called the Taconic orogeny. Baltica not only moved northward relatively rapidly, but also rotated about 90° during the latter part of the Ordovician. The Argentine Precordillera plate moved southward across a midlatitudinal interval of ocean to collide with what is today the western side of Argentina in the Middle Ordovician. Africa shifted northward during the Ordovician with the result that northern Africa and the regions adjacent to the Middle East shifted into cool-temperate conditions.

     

    Life and environments

     

    As plate motions took place, environments changed significantly, as well as life in them. Both oceanic and terrestrial settings became the sites of significant radiations.

    Early Ordovician (Tremadoc-Arenig) environmental conditions in most areas were similar to those of the Late Cambrian. Accordingly, Early Ordovician life was similar to that of the latter part of the Cambrian. Trilobites were the prominent animal in most shelf sea environments. Long straight-shelled nautiloids, certain snails, a few orthoid brachiopods, sponges, small echinoderms, algae, and bacteria flourished in tropical marine environments. Linguloid brachiopods and certain bivalved mollusks inhabited cool-water, nearshore environments.

    Middle Ordovician plate motions were acompanied by significant changes in life. On land, nonvascular, mosslike plants appeared in wetland habitats. Vascular plants appeared slightly later in riverine habitats. The first nonvascular plants occurred in the Middle East on Gondwanan shores. The Middle Ordovician radiation of marine invertebrates is one of the most extensive in the record of Phanerozoic marine life. Corals, bryozoans, several types of brachiopods, a number of crinozoan echiniderms, conodonts, bivalved mollusks, new kinds of ostracodes, new types of trilobites, and new kinds of nautiloids suddenly developed in tropical marine environments. As upwelling conditions formed along the plate margins, oxygen minimum zones—habitats preferred by many graptolites—expanded at numerous new sites. Organic walled microfossils (chitinozoans and acritarchs) radiated in mid- to high-latitude environments. Ostracoderms (jawless, armored fish) radiated in tropical marine shallow-shelf environments. These fish were probably bottom detritus feeders.  See also: Paleoecology

     

    Glaciation

     

    When the Avalon plate collided with the Laurentian, a major mountain chain developed in a tropical setting. Vast quantities of siliclastic materials were shed from that land to form what is called the Queenston delta in the present-day Appalachians. As the Queenston delta grew, glaciation commenced at or near the South Pole. Continental glaciation spread from its North African center for a 1–2-million-year interval late in the Ordovician. Glacially derived materials (including many drop-stones) occurred in the Late Ordovician strata in Morocco, Algeria, southern France, Germany, Spain, Portugal, and the Czech Republic. Sea level dropped by at least 70 m at the glacial maximum. As a result, most shallow to modest-depth marine environments were drained. Karsts formed across many carbonates that had accumulated in the shallow marine settings. Upwelling along many platform margins ceased or became quite limited. As a consequence, former extensive oxygen minimum zones were markedly diminished. The loss of wide expanses of shallow marine environments and extensive oxygen minimum zones led to massive extinctions of benthic marine organisms, as well as those graptolites living near oxygen minimum zones. These extinctions took place over a 1–2-million-year interval as environments shifted, diminished, or eventually were lost. Oxygen isotope studies on brachiopod shells suggest that tropical sea surface temperatures dropped by as much as 4°C.  See also: Geomorphology; Paleoceanography

    The latest Ordovician stratigraphic record suggests that the ice melted relatively quickly, accompanied by a relatively rapid sea-level rise in many areas. Some organisms—certain conodonts, for example—did not endure significant extinctions until sea levels began to rise and shelf sea environments began to expand.  See also: Stratigraphy

     

    Ocean surface circulation

     

    Surface circulation in Ordovician seas was controlled in the tropics by the several platforms and in the Southern Hemisphere by Gondwanaland. Equatorial surface currents flowed east to west, but they were deflected by the shallow shelf environments. The tropical or warm-water faunal provinces were influenced by these deflections. Homogeneity of the tropical faunas was maintained by the surface water currents. Southern Hemisphere currents were influenced by the relatively long west coast of Gondwanaland and of the Baltoscanian Plate. Upwelling conditions would have been generated along these coasts. Location, size, and relief on Gondwanaland probably led to monsoonal seasonal reversals in surface ocean currents near what is today South China. Absence of lands or shallow shelf seas north of the Northern Hemisphere tropics would permit oceanic surface circulation to be zonal; that is, currents flowed from east to west north of 30° north latitude, and they flowed from west to east between 30 and 60° north latitude.

     

    Economic resources

     

    Ordovician shelf and shelf margin rock sequences in areas where there has been little post-Ordovician volcanic activity or severe deformation have yielded petroleum and natural gas. Quartzites interbedded with carbonates formed in shelf sea environments have been used as a source of silica for glass manufacture. Ordovician carbonates are hosts for lead-zinc-silver ores mined in the western United States, including Missouri and Washington. Significant quantities of gold were recovered from Ordovician graptolite-bearing strata in eastern Australia in the late 1800s. Gold-bearing Ordovician rocks occur in Nevada (western United States) where they are part of one of the most prolific gold-producing areas in 

     

     

     

    • J. D. Cooper, M. I. Droser, and S. C. Finney (eds.), Ordovician Odyssey: Short Papers for the 7th International Symposium on the Ordovician System, Pacific Section, Society for Sedimentary Geology, 1995
    • P. Kraft and O. Fatka (eds.), Quo Vadis Ordovician?, Acta Universitatis Carolinae Geologica, vol. 43, no. 1/2, 1999
    • C. Lapworth, On the tripartite classification of the Lower Palaeozoic rocks, Geol. Mag., 6:1–15, 1879
    • T. H. Torsvik, Palaeozoic palaeogeography: A North Atlantic viewpoint, GFF, 120:109–118, 1998

    Cambrian

    An interval of time in Earth history (Cambrian Period) and its rock record (Cambrian System). The Cambrian Period spanned about 60 million years and began with the first appearance of marine animals with mineralized (calcium carbonate, calcium phosphate) shells. The Cambrian System includes many different kinds of marine sandstones, shales, limestones, dolomites, and volcanics. Apart from the occurrence of an alkaline playa containing deposits of trona (hydrated basic sodium carbonate) in the Officer Basin of South Australia, there is very little provable record of nonmarine Cambrian environments.

    The concept that great systems of rocks recorded successive periods of Earth history was developed in England in the early nineteenth century. The Cambrian, which was one of the first systems to be formally named, was proposed by the Reverend Adam Sedgwick in 1835 for a series of sedimentary rocks in Wales that seemed to constitute the oldest sediments in the British Isles. At that time, there was no real idea of the antiquity of Cambrian rocks. They were recognized by distinctive fossils and by their geologic relations to other systems. In the early part of the twentieth century, radiometric techniques for obtaining the ages of igneous and metamorphic rocks evolved. Because of the difficulty of finding rocks that can be dated radiometrically in association with rocks, usually zircon bearing volcanic ashes, that can be dated empirically by fossils, the age in years of most Cambrian deposits is only approximate. The best present estimates suggest that Cambrian time began about 545 million years ago (Ma; earliest date close to the base of the Cambrian is 543 ± 0.2 Ma) and ended at about 485 Ma (latest date in the Upper Cambrian is 491 ± 1 Ma, but this is not terminal Cambrian). It is the longest of the Paleozoic periods and the fourth long est of the Phanerozoic periods.

     

    Geography

     

    Knowledge of Cambrian geography and of the dynamic aspects of evolution and history in Cambrian time is derived from rocks of this age that have been exposed by present-day erosion or penetrated by borings into the Earth's surface. Despite the antiquity of Cambrian time, a surprisingly good record of marine rocks of Cambrian age has been preserved at many localities throughout the world. Each of the different rock types contains clues about its environment of deposition that have been derived from analogy with modern marine environments. From this information, together with knowledge gained from fossils of about the same age within the Cambrian and information about the present geographic distribution of each Cambrian locality, a general picture of world geography and its changes through Cambrian time is available.

     

    Plate tectonics

     

    The theory of plate tectonics has provided criteria whereby ancient continental margins can be identified. By using these criteria and the spatial information about marine environments derived from study of the rocks, the Cambrian world can be resolved into at least four major continents that were quite different from those of today (Fig. 1). These were (1) Laurentia, which is essentially North America, minus a narrow belt along the eastern coast from eastern Newfoundland to southern New England that belonged to a separate microcontinent, Avalonia. This microcontinent, which also included present-day England, and another microcontinent now incorporated in South Carolina were originally marginal to Gondwana; (2) Baltica, consisting of present-day northern Europe north of France and west of the Ural Mountains but excluding most of Scotland and northern Ireland, which are fragments of Laurentia; (3) Gondwana, a giant continent whose present-day fragments are Africa, South America, India, Australia, Antarctica, parts of southern Europe, the Middle East, a nd Southeast Asia; and (4) Siberia, including much of the northeastern quarter of Asia. Unfortunately, there is not enough reliable information to accurately locate these continents relative to one another on the Cambrian globe. Current Cambrian reconstructions rely on similarities of fossil faunas and on studies of magnetic polarity reversals in rock sequences through time (magnetostratigraphy). These have mostly been concentrated across the Precambrian-Cambrian boundary in Australia, Morocco, Siberia, and south China, and across the Cambrian-Ordovician boundary in Australia, North America, Kazakhstan, and north China.  See also: Continental margin; Continents, evolution of; Plate tectonics

     

     

    Fig. 1  Reconstruction of the Lower Cambrian world. (After W. S. McKerrow, C. R. Scotese, and M. D. Brasier, Early Cambrian continental reconstructions. J. Geol. Soc., 149:599–606, 1992)

     

     

     

    fig 1

     

     

     

     

    Time divisions

     

    For most practical purposes, rocks of Cambrian age are recognized by their content of distinctive fossils. On the basis of the successive changes in the evolutionary record of Cambrian life that have been worked out during the past century, the Cambrian System has been divided globally into three or four series, each of which has been further divided on each continent into stages, each stage consisting of several zones (Fig. 2). Despite the amount of work already done, precise intercontinental correlation of series and stage boundaries, and of zones, is still difficult, especially in the Early Cambrian due to marked faunal provinciality. Refinement of intercontinental correlation of these ancient rocks is a topic of research.

     

     

    Fig. 2  North American divisions of the Cambrian S ystem. Asterisks denote levels of major trilobite extinctions.

     

     

     

     

     

     

     

    Life

     

    The record preserved in rocks indicates that essentially all Cambrian plants and animals lived in the sea. The few places where terrestrial sediments have been preserved suggest that the land was barren of major plant life, and there are no known records of Cambrian insects or of terrestrial vertebrate animals of any kind.

     

    Plants

     

    The plant record consists entirely of algae, preserved either as carbonized impressions in marine black shales or as filamentous or blotchy microstructures within marine buildups of calcium carbonate, called stromatolites, produced by the actions of these organisms. Cambrian algal stromatolites were generally low domal structures, rarely more than a few meters high or wide, which were built up by the trapping or precipitation of calcium carbonate by one or more species of algae. Such structures, often composed of upwardly arched laminae, were common in regions of carbonate sedimentation in the shallow Cambrian seas.  See also: Stromatolite

     

    Animals

     

    The animal record is composed almost entirely of invertebrates that had either calcareous or phosphatic shells (Fig. 3). The fossils of shell-bearing organisms include representatives of several different classes of arthropods, mollusks, echinoderms, brachiopods, and poriferans. Coelenterates, radiolarians, and agglutinated foraminiferans are extremely rare, and bryozoans are unknown from Cambrian rocks. Rare occurrences of impressions or of carbonized remains of a variety of soft-bodied organisms, including worms and a group of soft-bodied trilobites, indicate that the fossil record, particularly of arthropods, is incomplete and biased in favor of shell-bearing organisms. Some widespread fossil groups, such as Archaeocyatha, are known only from Cambrian rocks, and several extinct groups of Paleozoic organisms, such as hyolithids and conodo nts, first appear in Cambrian rocks. Conodonts are thought by some specialists to have affinity with vertebrates, but others prefer to relate them to cephalochordates. Dermal plates recovered from the Late Cambrian of North America and Australia are considered to represent the earliest fish remains.  See also: Arthropoda; Conodont; Porifera

     

     

    Fig. 3  Representative Cambrian fossils: (a–c) trilobites; (d–f) brachiopods; (g) hyolithid; (h–i) mollusks; (j–l) echinoderms; and (m, n) archaeocyathids.

     

     

     

    fig 3

     

     

     

     

    Diversity

     

    Although the record of marine life in the Cambrian seems rich, one of the dramatic differences between Cambrian marine rocks and those of younger periods is the low phyletic diversity of most fossiliferous localities. The most diverse faunas of Cambrian age have been found along the ocean-facing margins of the shallow seas that covered large areas of the Cambrian continents. Because these margins were often involved in later geologic upheavals, their rich record of Cambrian life has been largely destroyed. Only a few localities in the world remain to provide a more accurate picture of the diversity of organisms living in Cambrian time. These are known as Konservat Lagerstätten—conservation deposits containing occurrences of extraordinary preservation, particularly of soft body parts. Globally, they are known from more than 35 localities to date if the “Orsten”-type preservation in the Swedish Alum Shale and elsewhere are considered as Lagerstätten. Orsten is an organic-rich, anthraconitic, concretionary limestone in which phosphatized cuticle-bearing organisms are exquisitely preserved in three dimensions. In Laurentia, the richest localities are in the Kinzers Formati on of southeastern Pennsylvania, the Spence Shale of northern Utah, the Wheeler Shale and Marjum Formation of western Utah, the Buen Formation of northern Greenland, and the Burgess Shale of British Columbia. The last is the largest such deposit, containing about 152 mostly monospecific genera of Middle Cambrian age. Equally spectacular is the Chengjiang fauna found at Maotianshan in Yunnan, southwest China, which contains in excess of 70 arthropod-dominated species of Early Cambrian age. However, for extremely fine morphological detail, Orsten-type preservation in the Lower Cambrian of England, the Middle Cambrian of Russia and Australia, and the Upper Cambrian of Poland and Sweden is unsurpassable.

     

    Trilobites

     

    The most abundant remains of organisms in Cambrian rocks are of trilobites (Fig. 3a–c). They are present in almost every fossiliferous Cambrian deposit and are the principal tools used to describe divisions of Cambrian time and to correlate Cambrian rocks. These marine arthropods ranged from a few millimeters to 20 in. (50 cm) in length, but most were less than 4 in. (10 cm) long. Although some groups of trilobites such as the Agnostida (Fig. 3a) were predominantly pelagic in habitat, most trilobites seem to have been benthic or nektobenthic and show a reasonably close correlation with bottom environments. For this reason, there are distinct regional differences in the Cambrian trilobite faunas of the shallow seas of different parts of the Cambrian world.  See also: Trilobita

     

    Brachiopods

     

    The next most abundant Cambrian fossils are brachiopods (Fig. 3d–f). These bivalved animals were often gregarious and lived on the sediment surface or on the surfaces of other organisms. Brachiopods with phosphatic shells, referred to the Acrotretida (Fig. 3f), are particularly abundant in many limestones and can be recovered in nearly perfect condition by dissolving these limestones in acetic or formic acids. Upper Cambrian limestones from Texas, Oklahoma, and the Rocky Mountains yield excellent silicified shells of formerly calcareous brachiopods when they are dissolved in dilute hydrochloric acid.  See also: Brachiopoda

     

    Archaeocyathids

     

    Limestones of Early Cambrian age may contain large reeflike structures formed by an association of algae and an extinct phylum of invertebrates called Archaeocyatha (Fig. 3m and n). Typical archeocyathids grew conical or cylindrical shells with two walls separated by elaborate radial partitions. The walls often have characteristic patterns of perforations.  See also: Archaeocyatha

     

    Mollusks and echinoderms

     

    The Cambrian record of mollusks and echinoderms is characterized by many strange-looking forms (Fig. 3g–l). Some lived for only short periods of time and left no clear descendants. Representatives of these phyla, such as cephalopods, clams, and true crinoids, which are abundant in younger rocks, are rare in Cambrian rocks; but rostroconch mollusks are known from the Early, Middle, and Late Cambrian at various times in Laurentia, Australia, Siberia, north China, and Korea. Snails, however, are found throughout the Cambrian. Discoveries of primitive clams have been made in Early Cambrian beds, but they are apparently absent from the later record of life for tens of millions of years until post-Cambrian time.  See also: Echinodermata; Mollusca

     

    Corals

     

    Except for rare jellyfish impressions, the Coelenterata were thought to be unrepresented in Cambrian rocks. Corals have now been discovered in early Middle Cambrian rocks in Austral ia. However, like clams, they are not seen again as fossils until Middle Ordovician time, many tens of millions of years later.  See also: Cnidaria

     

    Extinction

     

    The stratigraphic record of Cambrian life in Laurentia (North America) shows perhaps five major extinctions of most of the organisms living in the shallow seas. These extinction events form the boundaries of evolutionary units called biomeres (Fig. 2). Their cause, and their presence in the Cambrian records of other continents, is under investigation. At least one of these extinction events, that at the Marjuman-Steptoean boundary, coincides with a large positive carbon isotope anomaly in Laurentia, Australia, south China, and Kazakhstan. However, perhaps it was these periodic disasters that prevented clear continuity in the evolutionary records of many groups and which led, particularly, to the discontinuous records of the echinoderms, corals, and mollusks.  See also: Animal evolution; Extinction (biology)

     

    Faunal origin

     

    One major unsolved problem is the origin of the entire Cambrian fauna. Animal life was already quite diverse before Cambrian time. The earliest Cambrian beds contain representatives of more than 20 distinctly different invertebrate groups. All of these have calcified shells, but none of the Precambrian organisms have any evidence of shells. There is still no clear evidence to determine whether shells evolved in response to predation or to environmental stress, or as the result of some change in oceanic or atmospheric chemistry.  See also: Precambrian

     

     

    History

     

    At the beginning of Cambrian time, the continents were largely exposed, much as they are now. Following some still-unexplained event, the seas were suddenly populated by a rich fauna of shell-bearing invertebrates after 3 billion years of supporting only simple plants and perhaps 100 million years with shell-less invertebrates.  See also: Precambrian

    Belts of volcanic islands comparable to those of the western Pacific Ocean today fringed eastern Laurentia, the Australian and western Antarctic margins of Gondwana, and southern Siberia. These belts suggest that crustal plates analogous to those of the present day were in motion at that time. Thick evaporites in Siberia and the Middle Eastern and Indian parts of Gondwana suggest regions of warm temperature and high evaporation rate. Absence of significant development of limestones around Baltica suggest that it was a cool region, probably at high latitudes. Near the continental margins of eastern and western Laurentia, on and around Siberia, and on the western Antarctic, eastern Australian, northwestern African, and southern European margins of Gondwana, archaeocyathid bioherms developed and flourished. By the end of Early Cambrian time, archaeocyathids had become extinct, and shell-bearing organisms capable of building bioherms did not reappear until Middle Ordovician time, at least 45 million years later.

    Volcanism and evaporitic conditions continued into the Middle Cambrian in Siberia and parts of Gondwana, and evaporites of this age are also known from northern Canada. However, a dramatic change took place in the southern European and northwestern African parts of Gondwana. Carbonate sedimentation virtually ceased throughout that region as those parts of Gondwana reached areas of cooler water and probably higher latitudes. Sea level was rising over much of the world throughout Middle Cambrian time, flooding the interiors of most continents.

    In the Late Cambrian, parts of western Baltica and eastern Laurentia began to show signs of crustal deformation suggesting that Iapetus, the ocean between Laurentia, Gondwana, and Baltica, was beginning to close. Crustal deformation was also taking place in southern Siberia, eastern Australia, and western Antarctica. In the broad, shallow seas over all of the contin ents except Baltica and the southern European and northwestern African parts of Gondwana, extensive areas of carbonate sediments developed. At least five times in the shallow seas covering Laurentia, large parts of the animal populations became extinct and had to be replenished from the oceanic regions. The last of these extinction events marks the end of Cambrian time in Laurentia.

    Throughout Cambrian time, terrestrial landscapes were stark and barren. Life in the sea was primitive and struggling for existence. Only in post-Cambrian time did the shallow marine environment stabilize and marine life really flourish. Only then did vertebrates evolve and plants and animals invade the land.

     

     

    C. H. Holland (ed.), Cambrian of the British Isles, Norden and Spitzbergen, 1974

    C. H. Holland (ed.), Cambrian of the New World, 1971

    C. H. Holland (ed.), Lower Paleozoic of the Middle East, Eastern and Southern Africa, and Antarctica, 1981

    W. S. McKerrow, C. R. Scotese, and M. D. Brasier, Early continental reconstructions, J. Geol. Soc., 149:559–606, 1992

    M. A. McMenamin and D. L. McMenamin, The Emergence of Animals: The Cambrian Breakthrough, 1990

    A. R. Palmer, A proposed nomenclature for stages and series for the Cambrian of Laurentia, Can. J. Earth Sci., 35(4):323–328, 1998

    A. R. Palmer, Search for the Cambrian world, Amer. Sci., 62:216–224, 1974

    R. A. Robison and C. Tiechert (eds.), Treatise on Invertebrate Paleontology, pt. A: Biogeography, 1979

    J. A. Secord, Controversy in Victorian Geology: The Cambrian-Silurian Dispute, 1986

    H. B. Whittington, The Burgess Shale, 1985

     

    Additional Readings

     

     

    M. D. Brasier, The basal Cambrian transition and Cambrian bio-events (from terminal Proterozoic extinctions to Cambrian biomeres), in O. H. Walliser (ed.), Global Events and Event Stratigraphy in the Phanerozoic, Springer, Berlin, 1995

    M. D. Brasier, Towards a carbon isotope stratigraphy of the Cambrian System: Potential of the Great Basin succession, in E. A. Hailwood and R. B. Kidd (eds.), High Resolution Stratigraphy, Geol. Soc. Spec. Publ., no. 70, 1992

    S. Conway Morris and H. B. Whittington, The animals of the Burgess Shale, Sci. Amer., 241(1):122–133, 1979

    P. J. Cook and J. H. Shergold (eds.), Phosphate Deposits of the World, 1. Proterozoic and Cambrian Phosphorites, Cambridge University Press, Melbourne, 1986

    J. W. Cowie and M. D. Brasier (eds.), The Precambrian-Cambrian Boundary, Oxford Monogr. Geol. Geophy., no. 12, Clarendon Press, Oxford, 1989

    S. J. Gould, Wonderful Life, W. W. Norton, New York, 1989

    Hou Xianguang, L. Ramsköld, and J. Bergström, Composition and preservation of the Chengjiang fauna: A Lower Cambrian soft-bodied biota, Zoologica Scripta, 20(4):395–411, 1991

    C. E. Isachsen et al., New constraint on the division of Cambrian time, Geology, 22:496–498, 1994

    P. Janvier, Vertebrate origins: Conodonts join the club, Nature, 374:761–762, 1995

    E. Landing et al., Duration of the Early Cambrian: U-Pb ages of volcanic ashes from Avalon and Gondwana, Can. J. Earth Sci., 35(4):329–338, 1998

    D. Walossek and K. J. Müller, Cambrian “Orsten”-type arthropods and the phylogeny of Crustacea, in R. A. Fortey and R. H. Thomas (eds.), Arthropod Relationships, Systematics Ass. Spec. Vol. Ser., no. 55, 1997

    H. B. Whittington, Trilobites, Boydell Press, Woodbridge, 1992

    G. C. Young and J. R. Laurie (eds.), An Australian Phanerozoic Time-scale, Oxford University Press, Melbourne, 1996

    International Union of Geological Sciences, Commission on Stratigraphy, Subcommission on Cambrian Stratigraphy

    Cenozoic

     

     

    Cenozoic (Cainozoic) is the youngest and the shortest of the three Phanerozoic geological eras. It represents the geological time (and rocks deposited during that time) extending from the end of the Mesozoic Era to the present day.

    The geological concept of the Cenozoic, as the youngest era of the Phanerozoic, was introduced by J. Phillips in 1941. He considered it to be a unit equivalent to the Tertiary, a term that was still in use from G. Arduino's classification of Primary, Secondary, and Tertiary rocks, introduced in Italy in 1759. Arduino based his subdivision on physical attributes, such as older magmatic and metamorphic rocks as Primary; limestone, marl, and clay with fossils as Secondary; and youngest, fossil-rich rocks as Tertiary. This classification is now largely obsolete, with the exception of the term Tertiary that is still in use in a modified sense. A. Brogninart first modified the concept of Tertiaire in 1810, applying it to the strata deposited above the Cretaceous chalk in the Paris Basin. The term Quaternary (the second and younger period of the Cenozoic) was introduced by M. Morlot in 1854.  See also: Quaternary; Tertiary

    Modern time scales include all of the past 65 million years of geological history in the Cenozoic Era. The distinction of the Cenozoic Era from older eras has been traditionally based on the occurrence of fossils showing affinities to modern organisms, and not on any particular lithostratigraphic criteria.  See also: Index fossil; Paleontology

     

    Subdivisions

     

    Traditional classifications subdivide the Cenozoic Era into two periods (Tertiary and Quaternary) and seven epochs (from oldest to youngest): Paleocene, Eocene, Oligocene, Miocene, Pliocene, Pleistocene, and Holocene. The older five epochs, which together constitute the Tertiary Period, span the time interval from 65 to 1.8 million years before present. The Tertiary is often separated into two subperiods, the Paleogene (Paleocene through Oligocene epochs, also collectively called the Nummulitic in older European literature) and the Neogene (Miocene and Pliocene epochs). These subperiods were introduced by M. Hornes in 1853. The Quaternary Period, which encompasses only the last 1.8 million years, includes the two youngest epochs (Pleistocene and Holocene). Holocene is also often referred to as the Recent, from the old Lyellian classification. Recent stratigraphic opinions are leaning toward abandoning the use of Tertiary and Quaternary (which are seen as the unnecessary holdovers from obsolete classifications) and in favor of retaining Paleogene and Neogene as the prime subdivisions of Cenozoic.  See also: Eocene; Holocene; Miocene; Oligocene; Paleocene; Pleistocene; Pliocene

     

    Tectonics

     

    Many of the tectonic events (mountain-building episodes or orogenies, changes in the rates of sea-floor spreading, or tectonic plate convergences) that began in the Mesozoic continued into the Cenozoic. The Laramide orogeny that uplifted the Rocky Mountains in North America, which began as early as Late Jurassic, continued into the Cretaceous and early Cenozoic time. In its post-Cretaceous phase the orogeny comprised a series of diastrophic movements that deformed the crust until some 50 million years ago, when it ended abruptly. The Alpine orogeny, which created much of the Alps, also began in the Mesozoic, but it was most intense in the Cenozoic when European and African plates converged at an increased pace.  See also: Cretaceous; Jurassic; Mesozoic; Orogeny

    In the Pacific Ocean the most significant tectonic event in the Cenozoic may have been the progressive consumption of the East Pacific Rise at the Cordilleran Subduction Zone and the concomitant development of the San Andreas Fault System some 30 million years ago. See also: Cordilleran belt; Fault and fault structures; Subduction zones

    In the intracontinental region of the Tethys between Europe and Africa, the Cenozoic tectonic history is one of successive fragmentation and collision of minor plates and eventual convergence of the African and European plates. Africa's motion was counterclockwise relative to Europe, which began sometime in the early Mesozoic. By mid-Cenozoic, however, the motion between the two plates was largely convergent. The convergence caused a complex series of events that closed the Tethys Seaway between the two continents. In the late Cenozoic (Pliocene) the final collision of the Arabian plate with the Asian plate along Iran produced the Zagros Mountains, and partially or completely isolated the Caspian and Black seas.  See also: Continental drift

    In the Indian Ocean, perhaps the most significant event during the Cenozoic was rapid movement of the Indian plate northward and its collision with Asia. India had already broken loose from the eastern Gondwana in the late Cretaceous, but around 80 million years ago its motion accelerated, and then increased further in the early Cenozoic. This movement, however, slowed down considerably around 50 million years ago when the Indian plate plowed into the Asian mainland. The first encounter of the two plates caused the initial uplift of the Himalayas. The major phase of the Himalayan orogeny, however, extends from the Miocene to the Pleistocene, when much of the high Himalayas were raised and the Tibetan Plateau was fully uplifted. The encounter also caused major reorganization of the crust both north and south of the collision zone. In the Indian Ocean the plates were reorganized, and spreading was initiated on the Central Indian Ridge system. The collision had important repercussions for the Asian mainland as well. Over 1500 km (900 mi) of crustal shortening has occurred since the collision began. The effects of diastrophism associated with this event extend some 3000 km (1800 mi) northeast of the Himalayas. This includes major strike-slip faults in China and Mongolia, which may account for a major portion of the crustal shortening, which continues to the present day. The present convergence between the Indian and Asian plates is at the rate of about 0.5 cm (0.2 in.) per year.

    Another major long-term affect of the tectonic uplift of Tibetan Plateau, which is dated to have been significant by 40 million years ago, may have been the initiation of the general global cooling trend that followed this event. The uplifted plateau may have initiated a stronger deflection of the atmospheric jet stream, strengthening of the summer monsoon, and increased rainfall and weathering in the Himalayas. Increased weathering and dissolution of carbonate rock results in greater carbon dioxide (CO2) drawdown from the atmosphere. The decreased partial pressure of carbon dioxide (pCO2) levels may have ultimately led to the Earth entering into a renewed glacial phase.

    The convergence between India and Asia and between Africa and Europe in the mid-Cenozoic destroyed the ancestral Tethys Seaway, leaving behind smaller remnants that include the Mediterranean, Black, and Caspian seas.  See also: Plate tectonics

     

    Oceans and climate

     

    The modern circulation and vertical structure of the oceans and the predominantly glacial mode that the Earth is in at present was initiated in the mid-Cenozoic time. The early Cenozoic was a period of transition between the predominantly thermospheric circulation of the Mesozoic and the thermohaline circulation that developed in the mid-Cenozoic. By the mid-Cenozoic the higher latitudes had begun to cool down, especially in the Southern Hemisphere due to the geographic isolation of Antarctica, leading to steeper latitudinal thermal gradients and accentuation of seasonality. The refrigeration of the polar regions gave rise to the cold high-latitude water that sank to form cold bottom water. The development of the psychrosphere (cold deeper layer of the ocean) and the onset of thermohaline circulation are considered to be the most significant events of Cenozoic ocean history, which ushered the Earth into its modern glacial-interglacial cyclic mode.

    The overall history of the Cenozoic oceans is marked by a long-term withdrawal of the seas from epicontinental and coastal oceans and the accretion of ice on the polar regions. The ice buildup may have been partly favored by the more poleward position of the landmasses and the eventual thermal isolation of the Antarctic continent.

    In the early Paleogene, for the first time a deep connection between the North and South Atlantic was developed to allow deeper water penetration into the southern basin that intermittently led to extensive erosion on the ocean floor. However, the most likely source area for deep waters in the early Cenozoic was still in the temperate and low-latitude shelves. Farther north, in the Norwegian Sea area there is magnetic evidence of initiation of sea-floor spreading in the late Paleocene. By the middle Eocene, this area may have become a site for the formation of cold bottom waters. Erosional events on the sea floor indicate that North Atlantic Deep Water may have begun to flow southward at approximately the same time as the initial subsidence of the Greenland-Faeroe Ridge below sea level in the late Eocene. Later on, in the Miocene, the ridge subsided more actively, resulting in greater outflow of higher-salinity water to intermediate and abyssal depths of the Central Atlantic. Evidence also points to vigorous bottom waters in the late Eocene, which increased in intensity through Oligocene and Miocene time.

    The most prominent feature of the surface circulation in the early Cenozoic was the westward flowing circumglobal Tethys Current, which dominated the oceanic scene in the tropical latitudes. As the Indian plate approached the Asian mainland in the early Cenozoic, it progressively restricted the flow of Tethys Current to its north. In the middle Eocene, when the general drop in global sea level and the first encounter of the Indian plate with Asia reduced the northern passage, the main flow moved to the west of the Indian plate. By Oligocene time the westward flow in the Tethys had become intermittent and severely restricted to a narrow western passage. The Tethyan passage had essentially closed by the dawn of the Neogene.

    A paleogeographic event of major import for the overall Cenozoic oceanic patterns was the breaching of the straits between Antarctica and South America at the Drake Passage in the Oligocene. This event led to the development of the circum-Antarctic Current, eventual thermal isolation of Antarctica, and further enhancement of the ice cap on the continent by mid-Oligocene. Winter ice accumulation on the Arctic, which lacks a continent in the polar position, may have also begun by the Oligocene. The increased sequestration of water on ice caps may be responsible for a major global sea-level drop in the mid-Oligocene evidenced along most of the world's continental margins. By late Oligocene time the global surface circulation patterns had essentially evolved the major features of the modern oceans.  See also: Paleoceanography; Paleogeography

    All climatic indicators point to a general warming trend through the Paleocene, culminating in a period of peak global temperatures at the close of Paleocene. The warm climates continued into the early Eocene interval. The latitudinal and vertical thermal gradients in the late Paleocene–early Eocene were low, and mean surface temperature was around 10°C (50°F) in the higher latitudes and 20°C (70°F) in the tropics. Terrestrial flora and fauna also corroborate the peak warming of this interval. For example, the Arctic island of Ellesmere has yielded a rich warm-blooded vertebrate fauna that indicates a range of temperature between 10 and 20°C (50 and 70°F).

    Studies have revealed a prominent carbon-isotopic shift in global carbonate reservoir that coincides with the latest Paleocene peak warming. This has been ascribed to the breakdown of deposits of methane hydrates on continental margins and catastrophic release of methane into the water and atmosphere due to rapid warming of the bottom waters. In the latest Paleocene, bottom water temperature increased rapidly (in less than 10,000 years) by as much as 4°C (7.2°F), with a coincident prominent enrichment of 12C isotope of the global carbon reservoir. The isotopic changes are accompanied by important biotic changes in the oceanic microfauna and are synchronous in the oceans and on land. This rapid and prominent isotopic shift cannot be explained by increased volcanic emissions of carbon dioxide, changes in oceanic circulation, or terrestrial and marine productivity alone. Increased flux of methane from gas-hydrate sources into the ocean-atmosphere system and its subsequent oxidation to carbon dioxide is held responsible for this isotopic excursion in the inorganic carbon reservoir. High-resolution data support the gas-hydrate connection to latest Paleocene abrupt climate change. Evidence from two widely separated sites from the low- and high-latitude Atlantic Ocean indicates multiple injections of methane with global consequences during the relatively short interval at the end of the Paleocene.

    The Eocene time is also characterized by higher global sea levels and increased oceanic productivity and carbonate deposition on the shelves and banks. The climate became more extreme in the late Eocene and through the Oligocene, when the latitudinal contrast increased due to development of ice in the polar regions. Himalayan uplift that produced the obstruction of the Tibetan Plateau in the path of the jet stream in the late Eocene may have been an important contributory factor to the cooling trend of the mid and late Cenozoic. Vertical thermal gradients also steepened once the cold bottom waters outflow began from the higher latitudes.

    The late Cenozoic is characterized by further accentuation of the oceanographic and climatic patterns that were initiated in the early Cenozoic. By Miocene time the Tethyan connection between the Indian Ocean and the Mediterranean Sea had been broken. This event modified the circulation patterns in the North Atlantic and the Mediterranean, which for the first time began to resemble their modern analogs. Neogene climatic proxies (such as stable isotopes in cores and glacial records on land) show evidence of considerable climatic fluctuations. Six major climatic deterioration events have been identified in the Miocene-Pliocene record. These events were also associated with enhanced surface circulation, bottom erosion, and aridity on land over North Africa. The cooler early Miocene climates were followed by a climatic optimum in mid-Miocene, to be in turn followed by a significant deterioration in climate, which has been ascribed to a major enlargement of the ice sheets on Antarctica.

    In the late Miocene, the Mediterranean suffered a salinity crisis following a sea-level fall and the isolation of the basin. The growth of ice caps in the Miocene eventually led to the fall of sea level below the depth of Gibraltar Sill, isolating the Mediterranean Basin. The lack of connection to the open Atlantic and excess evaporation led to high salinities and deposition of voluminous quantities of evaporites in a relatively short time. The Mediterranean was reconnected to the Atlantic in the early Pliocene, allowing cold deep waters to suddenly spill over the subsided Gibraltar Sill. The Black Sea was also converted into an alkaline lake during the salinity crisis when the Mediterranean inflow was cut off. The early Pliocene reconnection with the Mediterranean was once again followed by isolation of the Black Sea, this time as a fresh-water lake. These conditions lasted into the Quaternary, when the reconnection to the Mediterranean was established through the Bosporus Straits around 7000 years ago, ushering in the present-day conditions.  See also: Saline evaporites

    Another important threshold event of the late Cenozoic was the closing of the connection between the Central Atlantic and Pacific oceans at the Isthmus of Panama. The connection was operative until the mid-Pliocene, when tectonic events led to its closure some 3 million years ago. The closure most likely led to more vigorous Gulf Stream flow due to deflected energy, displacing the stream northward to its present-day position. The modern circulation patterns in the Caribbean also date back to this event. Another major climatic-oceanographic event of the Cenozoic was the development of an extensive ice cap on the Arctic. Although there is some evidence of ice cover in the Arctic since the Oligocene, evidence of a significant amount of ice accumulation is only as old as mid-Pliocene, some 3 million years ago, coincident with the closing of the Panama isthmus. The deflection of the Gulf Stream northward due to the latter event may have provided the excess moisture needed for this accumulation.

    The Quaternary climatic history is one of repeated alternations between glacial and interglacial periods. At least five major glacial cycles have been identified in the Quaternary of northwestern Europe. The most recent glacial event occurred between 30,000 and 18,000 years ago when much of North America and northern Europe was covered with extensive ice sheets. The late Pliocene and Pleistocene glacial cyclicity led to repeated falls in global sea level as a result of sequestration of water as ice sheets in higher latitudes during the glacial intervals. For example, the sea level is estimated to have risen some 110 m (360 ft) since the end of the last glacial maximum. As a by-product of these repeated drops in sea level and movement of the shorelines toward the basins, large deltas developed at the mouths of the world's major drainage systems during the Quaternary. These bodies of sand and silt constitute ideal reservoirs for hydrocarbon accumulation.  See also: Delta; Paleoclimatology

     

    Life

     

    At the end of the Cretaceous a major extinction event had decimated marine biota and only a few species survived into the Cenozoic. The recovery, however, was relatively rapid. During the Paleocene through middle Eocene interval, the overall global sea-level rise enlarged the ecospace for marine organisms, and an associated climatic optimum led to increased speciation through the Paleocene, culminating in high marine diversities during the early and middle Eocene. Limestone-building coral reefs were also widespread in the tropical-temperate climatic belt of the early Cenozoic, and the tropical Tethyan margins were typified by expansive distribution of the larger foraminifera known as Nummulites (giving the Paleogene its informal name of the Nummulitic period).  See also: Nummulites

    The late Eocene saw a rapid decline in diversities of marine phyto- and zooplankton due to a global withdrawal of the seas from the continental margins and the ensuing deterioration in climate. Marine diversities reached a new low in the mid-Oligocene, when the sea level was at its lowest, having gone through a major withdrawal of seas from the continental margins. The climates associated with low seas were extreme and much less conducive to biotic diversification. The late Oligocene and Neogene as a whole constitute an interval characterized by increasing partitioning of ecological nichesinto tropical, temperate, and higher-latitude climatic belts,and greater differentiation of marine fauna and flora.

    The terminal Cretaceous event had also decimated the terrestrial biota. Dinosaurs, which had dominated the Mesozoic scene, became extinct. Only a few small shrewlike mammalian species survived into the Paleocene. In the absence of dinosaurian competition, mammals evolved and spread rapidly to become dominant in the Cenozoic. The evolution of grasses in the early Eocene and the wide distribution of grasslands thereafter may have been catalytic in the diversification of browsing mammals. Marsupials and insectivores as well as rodents (which first appeared in the Eocene) diversified rapidly, as did primates, carnivores, and ungulates. The ancestral horse first appeared in the early Eocene in North America, where its lineage evolved into the modern genus Equus,only to disappear from the continent in the late Pleistocene. A complete evolution of the horse can be followed in North America during the Cenozoic. Increase in overall size, reduction in the number of toes, and increasing complexity of grinding surface of the molars over time are some of the obvious trends. Hominoid evolution began during the Miocene in Africa. Modern hominids are known to have branched off from the hominoids some 5 million years ago. Over the next 4.5 million years the hominids went through several evolutionary stages to finally evolve into archaic Homo sapiens about 1 million years ago. Truly modern Homosapiens do not enter the scene until around 100 thousand years ago.  See also: Dinosauria; Fossil humans; Mammalia; Organic evolution

      

     

    • B. U. Haq and F. W. B van Eysinga, Geological Time Table, Elsevier, Amsterdam 1998
    • K. J. Hsü (ed.), Mesozoic and Cenozoic Oceans, 1986
    • C. Pomerol, The Cenozoic Era: Tertiary and Quaternary, 1982
    • M. E. Raymo and W. F. Ruddiman, Tectonic forcing of late Cenozoic climate, Nature, 359:117–122, 1992

    Mesozoic

     

     

    The middle era of the three major divisions of the Phanerozoic Eon (Paleozoic, Mesozoic, and Cenozoic eras) of geologic time, encompassing an interval from 251 to 65 million years ago (Ma) based on various isotopic-age dates. The Mesozoic Era is known also as the Age of the Dinosaurs and the interval of middle life. The Mesozoic Erathem (the largest recognized time-stratigraphic unit) encompasses all sedimentary rocks, body and trace fossils of organisms preserved, metamorphic rocks, and intrusive and extrusive igneous rocks formed during the Mesozoic Era.  See also: Geochronometry

    The Mesozoic Era was originally named for one of three principal divisions of the fossil record, or history of life, that was bounded before and after by significant mass extinctions that dramatically changed the biotic composition of the world. In England during the early 1840s, geologist John Phillips introduced the terms Mesozoic Era and Cenozoic Era, in conjunction with geologist Adam Sedwick's term Paleozoic Era, proposed in 1838, to denote the widespread observation that three successive and distinct biotic assemblages were preserved in the fossil record. The Mesozoic Era comprises life intermediate in kind between ancient life-forms (Paleozoic Era) and recent life-forms (Cenozoic Era).  See also: Cenozoic; Paleozoic

    The Mesozoic Era records dramatic changes in the geologic and biologic history of the Earth. At the beginning of the Mesozoic Era, all the continents were amassed into one large supercontinent, Pangaea. Both the marine and continental biotas were impoverished from the mass extinction that marked the boundary between the Permian and Triassic periods, and the end of the Paleozoic Era. This mass extinction was responsible for the loss of over 90% of the species on Earth. During the Mesozoic Era, many significant events were recorded in the geologic and fossil record of the Earth, including the breakup of Pangaea and the evolution of modern ocean basins by continental drift, the rise of the dinosaurs, the ascension of the angiosperms (flowering plants), the diversification of the insects and crustaceans, and the appearance of the mammals and birds. The end of the Mesozoic Era is marked by a major mass extinction at the Cretaceous-Tertiary boundary that records several meteorite impacts, the extinction of the dinosaurs, the rise to dominance of the mammals, and the beginning of the Cenozoic Era and the life-forms dominant today.  See also: Continental drift; Plate tectonics

    The Mesozoic Era comprises three periods of geologic time: the Triassic Period (251–200 Ma), the Jurassic Period (200–146 Ma), and the Cretaceous Period (146–65 Ma) [Fig. 1]. These periods are each subdivided into epochs, formal designations of geologic time described as Early, Middle, and Late (except for the Cretaceous, which has no middle epoch designated yet). The packages of rock themselves are subdivided into series designated Lower, Middle, and Upper (except for Cretaceous). Each epoch is subdivided into ages. Likewise, each series is subdivided into stages, which are time-stratigraphic units whose boundaries are based on unconformities, hiatuses, or erosional surfaces, on correlations to a type section (where rocks are first described), or preferably on changes in the biota that depict true measurable time (for example, evolutionary changes).  See also: Unconformity

     

     

    Fig. 1  Subdivisions of the Mesozoic Era, including the best age estimates and the eustatic sea-level curve depicted as relative change in coastal onlap as the shoreline moved landward (sea-level rise) or seaward (sea-level fall).

     

     

     

    fig 1

     

     

     

    The correlations of time equivalency and age dating in the Mesozoic Era have been accomplished by utilizing biostratigraphic zones based on individual fossil groups or by an acme or composite zonal assemblage based on numerous fossil groups. Marine and continental fossil groups used to describe chronologically Mesozoic rocks include marine foraminifera and nannofossils (shelled protozoa), ammonites (cephalopods), and inoceramids (mollusks); continental plant spores and pollen (palynology); dinosaurs; and mammals. Correlations based on these and other organisms in the Mesozoic Era depend on the faunal and floral succession through origination and extinction of species.  See also: Cephalopoda; Foraminiferida; Mollusca; Palynology

    The organization of subdivisions based on physical and biological evidence allows geologists and paleontologists to describe both rocks and fossils in specific intervals of time and space. Thus, earth scientists can communicate effectively with one another and characterize more precisely the physical and biotic changes during the Mesozoic Era, as well as the other eras in geologic history.  See also: Paleontology; Stratigraphy

     

    Triassic

     

    The Mesozoic Era begins with the Triassic Period, which constitutes nearly one-third the total time of the era and is well exposed especially in Europe and North America, with other important outcrops in India, China, Argentina, and South Africa. The Triassic Period was named originally the Trias in Germany in 1834 by Friedrich August von Alberti for its unique fauna and natural division into three distinct stratigraphic units.

    As a result of the unique geography of the single Pangaean landmass, the alteration in oceanic currents produced around one continent, and the monsoonal climatic setting, life changed substantially in both marine and continental ecosystems. The marine ecosystems witnessed the addition of large reptiles and the modern reef-building corals, the reemergence and diversification of the mollusks, and the emergence of pelagic life in the form of planktonic organisms. Ray-finned and bony fishes and sharks dominated the seas. Placodonts and nothosaurs were aquatic marine reptiles that fed on mollusks and other marine invertebrates. Ichthyosaurs appeared in the oceans for the first time. Fresh-water and terrestrial ecosystems were marked by the emergence and diversification of the dinosaurs, flying reptiles, frogs, turtles, terrestrial crocodiles, and birds; the appearance of the mammals, though quite small in size; the emergence of fresh-water and terrestrial crayfish; and the emergence of new insects, such as the Isoptera (termites), Diptera (flies), and the Hymenoptera (bees, wasps, and possibly ants), appearing earlier in the Mesozoic than previously thought. Trace fossil evidence for these new insects indicates the advent of social behavior in termites and in primitive bees, prior to the appearance of angiosperms in the Cretaceous. In terrestrial ecosystems ferns and seed ferns were abundant, but gymnosperm floras continued to dominate the landscape. Therapsids rediversified after the Permo-Triassic extinctions, and thecodonts gave rise to the crocodiles and to the first dinosaurs, which were small in stature.

    During the Triassic Period the continents were amassed tectonically into one great landmass, the supercontinent Pangaea, that was distributed equally across the paleoequator in both the Northern and Southern hemispheres (Fig. 2a). Since the majority of the enormous Pangaean landmass was inland from the influence of the ocean, and its configuration distributed equally across the Equator, a worldwide monsoonal climate pattern dominated during the Triassic that created alternating wet and dry seasons in many regions. Areas landward of the coasts experienced increased continentality of the climate and produced more pronounced wet and dry seasons.  See also: Paleoclimatology; Paleogeography

     

     

    Fig. 2  Schematic reconstruction showing paleogeography of continents, epicontinental seas, and ocean basins (arrows denote ocean currents) on Pangaea in the Mesozoic Era from the (a) Triassic (220 Ma), (b) Jurassic (155 Ma), and (c) Cretaceous (70 Ma) periods.

     

     

     

    fig 2

     

     

     

    At the end of the Triassic, Pangaea began to break apart and the monsoonal climate pattern began to disintegrate. Evidence for the breakup of Pangaea and the eventual formation of the northern Atlantic Ocean is the presence of rift basins along the east coast of North America and the northwest coast of Africa. A mass extinction defines the boundary between the end of the Triassic and the beginning of the Jurassic. This mass extinction was responsible for the loss of about 60% of the species on Earth. The mass extinctions in the marine and continental realms affected the ocean ecosystem by eliminating the marine conodonts and placodont reptiles, and many species of bivalves, ammonoids, plesiosaurs, and ichthyosaurs disappeared. Most of these groups recovered in the Jurassic. Extinction also claimed the large amphibians and mammallike reptiles from fresh-water and terrestrial ecosystems. The cause of these mass extinctions is unknown, though some scientists hypothesize that either a meteorite impact or increasing global aridity caused many genera to go extinct.  See also: Triassic

     

    Jurassic

     

    The middle part of the Mesozoic Era is represented by the Jurassic Period, which constitutes about one-third of the total time of the era. Jurassic rocks are well exposed, especially in North America and Europe, and other important outcrops exist in South America and Asia. In 1839, German geologist Leopold von Buch established the Jurassic as a system for rocks in Switzerland, Germany, and England. The new system was based on descriptions of equivalent rocks made by the German geologist Alexandre von Humboldt (1795) and the English geologist William Smith (1797–1815). They described massive limestones of the Jura Mountains in Switzerland as the Jura-Kalkstein and the Lias-Oolite rock sequences in England and Wales, respectively.  See also: Limestone; Oolite

    During the Jurassic Period the Pangaean landmass continued to separate into two large continental masses, with one in the Northern Hemisphere and the other in the Southern (Fig. 2b). The Northern Hemisphere landmass, Laurasia, was composed of North America and Eurasia, while the Southern Hemisphere landmass, Gondwanda, was composed of South America, Africa, India, Antarctica, and Australia. Continued plate spreading and more rapid sea-level fluctuations late in the Jurassic created the Tethyan Seaway, which extended between Laurasia and Gondwanda, allowing oceans to flow freely between the continents, and caused epicontinental seas to flood large areas of North America and Europe. The opening of the ocean basins and the resulting increased oceanic circulation created a zonal atmospheric climate pattern that ranged from tropical at the Equator to warm temperate near the Poles, with local zones of aridity due to orographic and latitudinal rain shadows.  See also: Continents, evolution of; Rain shadow

    Oceanic and continental biotas shifted in composition during tectonic and climatic transformations of the Jurassic Period. Numerous reef communities of modern reef-building corals flourished in shallow tropical oceans along with bivalves, ammonites, belemnoids, sea urchins, and fishes. Planktonic life began to prosper in the warm, shallow seas with the appearance of calcareous nannoplankton. Marine reptiles included plesiosaurs and ichthyosaurs, and the invasion of the oceans by crocodiles. Terrestrial and fresh-water ecosystems were dominated by plants such as cycads, cycadeoids, conifers, ginkgos, and to a lesser extent ferns. The Jurassic is also known as the age of the cycads. The dinosaurs' greatest rise to dominance occurred with the radiation of large herbivores such as the sauropods Apatosaurus, Diplodocus, Camarasaurus, the plated stegosaurs, and the heavily armored ankylosaurs. The herbivores were pursued by predatory dinosaurs such as Ceratosaurus and Allosaurus. Many flying reptiles speckled the skies, including pterosaurs and the feathered reptilelike bird, Archaeopteryx. Mammals were still small in size but began to increase in diversity.  See also: Dinosauria; Phytoplankton; Reptilia; Zooplankton

    The end of the Jurassic Period was marked by moderate extinctions of biota in both marine and continental ecosystems. In the marine realm, brachiopod diversity declined steadily, other invertebrate faunas varied in diversity, and marine reptiles, such as the ichthyosaur, became nearly extinct. On the continents, the major extinctions eliminated the last of the therapsids and affected the large herbivorous sauropods, stegosaurs, and ankylosaurs, as well as their predators.  See also: Jurassic

     

    Cretaceous

     

    The last part of the Mesozoic is represented by the Cretaceous Period, which constitutes a little less than one-half the total time of the Mesozoic Era. The Cretaceous is represented well by rocks in North America, South America, Europe, Asia, Africa, and Australia. The Cretaceous Period was named in 1822–1823 by French geologist J. J. d'Omalius d'Halloy for exposures at the White Cliffs of Dover, which are composed of marine chalks and can be traced throughout Europe and North Africa. These widespread chalk units are composed predominantly of microscopic plates of calcareous nannoplankton, and had once been an ancient sea floor.  See also: Chalk; Micropaleontology

    During the Cretaceous Period the face of the Earth began to take on an appearance more similar to the present continental and oceanic configuration (Fig. 2c). Early in the Cretaceous, both Laurasian and Gondwanan continental masses separated into the continents still recognizable today. The separation of Gondwana in the Early Cretaceous marked the onset to the formation of the South Atlantic Ocean. Increased sea-floor spreading rates, which opened the oceanic gaps between the continents, resulted in the expansion of shallow epicontinental seaways in North America, Africa, and Northern Europe, along with the flooding of most of southern Eurasia. These variations in sea-floor spreading rates caused the sea level to fluctuate constantly throughout most of the Cretaceous. The Pacific and Atlantic Ocean basins began taking form, and the Tethyan Seaway, between what is now the western Mediterranean and southeastern Asia, persisted throughout most of the period. New, expanded oceanic realms coupled with the changed continental configurations and increased atmospheric carbon dioxide transformed the early Cretaceous climate into a humid zonal climate, warmer than today. The climate began cooling down, beginning near the end of the Mesozoic.

    The biotic composition during the Cretaceous Period contained a mixture of both intermediate and modern forms of life in both marine and continental ecosystems. In the marine realm, modern types of gastropods, bivalves, and modern fishes shared the oceans with marine reptiles such as mosasaurs and plesiosaurs, ammonoids, belemnoids, and other gigantic, coiled oysters and sedentary bivalves. Other marine invertebrates, such as planktonic and benthic foraminifera, flourished together with bryozoans, corals, reef-building rudist bivalves, crabs, lobsters, and other crustaceans. In the continental Cretaceous realm, the greatest change in fresh-water and terrestrial ecosystems occurred with the appearance and diversification of angiosperms or flowering plants that became more diverse over the early and middle Mesozoic gymnosperm floras near the end of the Cretaceous. At the same time, fresh-water and terrestrial insects continued to diversity and exploit new niches and resources provided by the angiosperms. Many groups of vertebrates, including snakes, modern types of turtles, crocodiles, lizards, and amphibians, diversified from ancient stocks during the Cretaceous to coexist with the dinosaurs that continued to rule the Earth. Mammals continued to evolve and diversify, but remained very small in size in comparison with their modern descendants.  See also: Magnoliophyta; Mammalia

    The dinosaurs diversified for the last time in the Cretaceous and formed ecological communities similar to mammal faunas inhabiting the African plains today. Herbivores such as the great horned dinosaur Triceratops and large duck-billed dinosaurs such as Hadrosaurus traveled in herds, roamed the plains, and followed watercourses in seasonally migrating for food. The predators that followed these herds were the largest carnivores of all times, Albertosaurus and Tyrannosaurus, together with other pack and ambush predators such as the velociraptors and crocodiles, respectively. The few flying reptiles that remained were spectacular, one form attaining a wingspan of nearly 11 m (35 ft), and these creatures shared the skies with modern types of shorebirds and wading birds.

    The end of the Cretaceous, and thus the end of the Mesozoic Era, is marked by a mass extinction known as the Cretaceous-Tertiary boundary (Tertiary is the earliest system of the Cenozoic Era, now divided into the Paleogene and Neogene). This mass extinction is widely known for the demise of 60% of the organisms on Earth, including the ammonoids, the rudist corals, marine reptiles, the dinosaurs, and the flying reptiles. There was a large reduction in the diversity of various marine plankton and continental faunas and floras, but they later recovered early in the Cenozoic. There have been many heated debates over the cause of the terminal Mesozoic extinctions, because some of them focus on extraterrestrial causes such as bolide and comet impacts onto the Earth's surface. Intriguing evidence in the form of iridium anomalies comes from marine deposits and continental coal deposits within rocks spanning the Cretaceous and Tertiary boundary worldwide. Iridium is an element that is typically depleted in rocks derived from the Earth's curst but is enriched in extraterrestrial stony meteorites. Some scientists hypothesize that a large 10-km (6-mi) meteorite or comet struck the Earth, exploded on impact, and released a blast greater than all the nuclear weapons on Earth. Such an impact would have thrown enormous volumes of dust and smoke into the atmosphere, blocked a large fraction of sunlight, and thus caused severe hardships to all marine and continental biota by lowering worldwide temperatures and disrupting the food chain. If the impact occurred in the ocean, huge volumes of water would have been vaporized instantly and caused gigantic tsunamis or tidal waves, which could have swept across most of the lowlands of continents. The devastating results of such an impact have been termed nuclear winter, because the effect would be similar to that produced by an all-out nuclear war. Other scientists hypothesize that extensive volcanic outgassing and cooler climates due to plate tectonic movements produced major changes in global climate and environmental disturbances that forced many organisms into extinction. Despite the similarities in global climate change and mass extinction interpreted by both of these hypotheses, other environmentally sensitive and presumably vulnerable groups of organisms were little affected by the mass extinction event. Environmentally sensitive vertebrates, such as crocodiles, lizards, turtles, frogs, and salamanders, were paradoxically spared and made it through the mass extinctions with little loss of species. The birds also persist through the mass extinctions and in fact radiate in the Paleogene and Neogene.  See also: Cretaceous; Extinction (biology); Geologic time scale; Meteorite; Tertiary

     

     

    • M. V. Caputo, J. A. Peterson, and K. J. Franczyk (eds.), Mesozoic Systems of the Rocky Mountain Region, USA, Rocky Mountain Section, Society for Sedimentary Geology, 1994
    • B. U. Haq and F. W. B. van Eysinga, Geologic Time Table Chart, 4th ed., 1994
    • W. B. Harland et al., A Geologic Time Scale, 1989
    • M. Moullade and A. E. M. Nairn (eds.), The Phanerozoic Geology of the World II: The Mesozoic, 1978
    • S. M. Stanley, Earth System History, 2d ed., 1998
    • British Mesozoic Fossils, 6th ed., British Museum of Natural History, no. 872, 1983
    • K. Carpenter, D. J. Chure, and J. I. Kirkland, (eds.), The Upper Jurassic Morrison Formation: An Interdisciplinary Study, Modern Geology Special Issue, vol. 23, no. 1–4, 1997
    • K. Carpenter, K. F. Hirsch, and J. R. Horner (eds.), Dinosaur Eggs and Babies, Cambridge University Press, 1994
    • P. J. Currie and K. Padian, Encyclopedia of Dinosaurs, Academic Press, San Diego, 1997
    • R. F. Dubiel et al., The Pangean megamonsoon—Evidence from the Upper Triassic Chinle Formation, Colorado Plateau, PALAIOS, 6:347–370, 1991
    • P.-C. Graciansky et al. (eds.), Mesozoic and Cenozoic Sequence Stratigraphy of European Basins, SEPM Spec. Publ. no. 60, Tulsa, 1998
    • S. T. Hasiotis, Complex ichnofossils of solitary to social soil organisms: Understanding their evolution and roles in terrestrial paleoecosystems, Palaeogeog. Palaeoclimatol. Palaeoecol., 192:259–320, 2003
    • S. T. Hasiotis, The invertebrate invasion and evolution of Mesozoic soil ecosystems: The ichnofossil record of ecological innovations, in R. Gastaldo and W. Dimichele (eds.), Phanerozoic Terrestrial Ecosystems, Paleontological Society Short Course, vol. 6, pp. 141–169, 2000
    • P. Kearey and F. J. Vine, Global Tectonic, 2d ed., Blackwell Science Limited, Oxford, England, 1996
    • J. A. Long, Dinosaurs of Australia and New Zealand and Other Animals of the Mesozoic Era, Harvard University Press, Cambridge, MA, 1998
    • C. R. Scotese and J. Glonka, Paleogeographic atlas: PALEOMAP Project, Department of Geology, University of Texas at Arlington, 1992
    • A. G. Smith, D. G. Smith, and B. M. Funnell, Atlas of Mesozoic and Cenozoic Coastlines, Cambridge University Press, 1994
    • S. L. Wing and H.-D. Sues, Mesozoic and Early Cenozoic terrestrial ecosystems, in A. K. Behrensmeyer et al. (eds.), Terrestrial Ecosystems through Time: Evolutionary Paleoecology of Terrestrial Plants and Animals, University of Chicago Press, 1992
    • International Commission on Stratigraphy
    • Introduction to the Mesozoic Era
    • Paleogeography of the Southwestern United States
    • Mesozoic Era of the Phanerozoic Eon

    Paleozoic

    Paleozoic

     

    A major division of time in geologic history, extending from about 540 to 250 million years ago (Ma). It is the earliest era in which significant numbers of shelly fossils are found, and Paleozoic strata were among the first to be studied in detail for their biostratigraphic significance. Western Europe, especially the British Isles, was the cradle of historical geology. Early work with rock strata and their fossils was strictly practical; the relative ages of rock units were essential for correlating scattered outcrops to search for natural resources—particularly coal—in the early part of the nineteenth century.

    During its first four decades, natural groupings of strata were studied and named for easy reference. Thus the several subdivisions of the Paleozoic, ultimately the six standard systems, were established. The original basis for establishing sequence was superposition. The operational stratigraphic hypothesis is that, in most instances, the strata at the bottom of a sequence are the oldest and the overlying beds are progressively younger. Thus, the basal system of the Paleozoic, in which primitive shelly fossils are found, is the Cambrian. As younger and younger layers were studied, their fossils collected, and the biological affinities suggested, the concept of evolution from simpler to more complex life forms took shape in the minds of the paleontologists and geologists who were studying the rocks. This process did not take place in an orderly way, from oldest to youngest strata, but rather as a consequence of fulfilling a need of the moment, whether to complete a geologic map or to solve a problem of stratigraphic correlation. Consequently, the first Paleozoic system to be named and studied in some detail was the Carboniferous—the great “coal-bearing” sequence—given that name by W. D. Conybeare and W. Phillips in 1822. These strata were to provide the world's major energy resources during the next century and a half. Most of the Northern Hemisphere's coal fields, and much of its oil and gas as well, were produced from Carboniferous rocks.  See also: Superposition principle

    In the 1830s and 1840s two British geologists, R. Murchison and A. Sedgwick, studied and named the natural groupings of rock strata in the British Isles. Sedgwick named the Cambrian System in 1835, for a sequence of strata that overlies the Primordial (Precambrian) rocks in northwest Wales. Four years later, Murchison gave the name Silurian to the early Paleozoic rocks found in the Welsh borderland. However, there was an almost complete overlap of the Cambrian by Murchison's Silurian. It was not until 1879, when C. Lapworth named the Ordovician System for rocks intermediate between the Cambrian and the “upper” Silurian, that the three early Paleozoic systems were sorted out in the correct order. In the meantime, Murchison and Sedgwick managed to agree on the rocks above the Silurian and, in 1839, they named the Devonian System for rocks exposed in Devonshire, England. The final Paleozoic system, the Permian, was named by Murchison in 1841, after an expedition to Russia, where he recognized the youngest Paleozoic fossil assemblages in the carbonate rocks exposed in the province of Perm. See also: Precambrian

     

    Subdivisions

     

    The Paleozoic Era is divided into six systems; from oldest to youngest they are Cambrian, Ordovician, Silurian, Devonian, Carboniferous, and Permian. The Carboniferous is subdivided into two subsystems, the Mississippian and the Pennsylvanian which, in North America, are considered systems by many geologists. The Silurian and Devonian systems are closer to international standardization than others; all the series and stage names and lower boundaries have been agreed upon, and most have been accepted. Despite continuing revisions, the major subdivisions of the geologic time scale have been relatively stable for nearly a century. See also: Cambrian; Carboniferous; Devonian; Ordovician; Permian; Silurian

     

    Paleotectonics

     

    The Paleozoic oceans, just as those today, surrounded a series of landmasses that formed the cores of ancient plates, always in motion as are their modern counterparts. Sediments were supplied to the seas through a network of river drainage systems and distributed in the oceans, by currents and gravity, very like today. Clastic sediments were supplied by the mountainous regions that were uplifted and eroded in cyclic patterns as the major plates collided and parted; and subduction at the leading edges of some plates produced volcanic highlands. The plate tectonic theory provides a template for sorting out the periods of mountain building during the Paleozoic. Like the discovery of the stratigraphic systems, periods of orogeny, with their concurrent volcanic and intrusive igneous activities, were revealed by field studies. Tectonic effects (folding and faulting) were analyzed by geologic mapping, as were crosscutting igneous relations and unconformities in the sedimentary sequence. Regional orogenic terranes were named and the general time sequence assigned; these were sharpened as the use of isotopic age analyses of the igneous components became possible in the twentieth century.

    Because Alpine and Appalachian mountain chains were among the first studied in detail, orogenies were first named there. In eastern North America, mountain-building effects during the early Paleozoic were ascribed to the Taconic orogeny (Middle and Late Ordovician); middle Paleozoic events were assigned to the Acadian orogeny (Middle and Late Devonian); and late Paleozoic movements were called Appalachian (more accurately Alleghenian) for Permian and, perhaps, Triassic events. Similar, but not precisely correlative, orogenic episodes in western Europe are ascribed to the early Paleozoic Caledonian and the late Paleozoic Variscan (or Hercynian) orogenies. This regionalization, overlapping of timing of events and lack of correlation of intrusive phases, tectonics, and sedimentation cycles emphasize the universality of the ever-moving plates as the global mechanism responsible for all tectonic events. See also: Dating methods; Isotope; Orogeny; Plate tectonics; Unconformity

     

     

    Fig. 1  Paleogeography of the Cambro-Ordovician (Tremadoc) showing most of the northern plates spread east-west in the equatorial regions. (After W. S. McKerrow and C. R. Scotese, eds., Paleozoic Palaeogeography and Biogeography, Geol. Soc. Mem. 12, Geological Society, London, 1990)

     

     

     

    pic 1

     

     

     

     

     

    Fig. 2  Paleogeography of Old Red Sandstone continent (outlined in color) in Late Devonian. (After R. Goldring and F. Langenstrassen, Open shelf and near-shore clastic facies in the Devonian, in M. R. House, C. T. Scrutton, and M. G. Bassett, eds., The Devonian System, Spec. Pap. Palaeont. 23, Palaeontological Association, London, 1979)

     

     

     

    fig 2

     

     

     

     

    Fig. 3  Paleogeography of the Early Carboniferous (Viséan), showing the Euro-American megaplate centered in equatorial region. (After W. S. McKerrow and C. R. Scotese, eds., Paleozoic Palaeogeography and Biogeography, Geol. Soc. Mem. 12, Geological Society, London, 1990)

     

     

     

    fig 3

     

     

     

     

     

    Fig. 4  Paleogeography at the end of the Permian showing the consolidation into Pangaea preparatory to the onset of the Mesozoic tectonic cycle. (After W. S. McKerrow and C. R. Scotese, eds., Paleozoic Palaeogeography and Biogeography, Geol. Soc. Mem. 12, Geological Society, London, 1990)

     

     

     

    fig 4

     

     

     

     

    Lithofacies

     

    The major changes in lithofacies during the Paleozoic were also effected by biotic evolution through the era. Limestone facies became more abundant and more diversified in the shallow warm seas as calcium-fixing organisms became more diverse and more widespread. Sediment input from the land was modified as plants moved from the seas to the low coastal plains and, eventually, to the higher ground during the Devonian. Primitive vertebrates evolved during the Cambro-Ordovician, but true fishes and sharks did not flourish until the Devonian. Amphibians invaded the land during the Late Devonian and early Carboniferous at about the same time that major forests began to populate the terrestrial realm. These changes produced an entirely new suite of nonmarine facies related to coal formation, and the Carboniferous was a time of formation of major coal basins on all continental plates.

    Climate continually influenced depositional patterns and lithofacies both on land and in the seas. In the major carbonate basins and platforms, particularly from the Late Ordovician onward, cyclic climatic changes resulted in changes from calcitic to magnesian carbonates and, ultimately, to various saline deposits as the basins dried up. There were great salt deposits in several systems, but spectacular thicknesses developed in many basins during the Silurian and Permian. Major cycles of cold and warm climates were overlaid on depositional and evolutionary patterns, producing periods of continental glaciation when large amounts of the Earth's water were tied up in ice during the Late Ordovician, the Late Devonian, and the late Permian. During the earliest and latest of these periods, icesheets were concentrated in the Southern Hemisphere on a single large Paleozoic continental mass—Gondwana. See also: Depositional systems and environments; Facies (geology); Paleoclimatology

     

    Paleogeography

     

    Paleogeographic changes naturally followed the shifting of plates on a megacyclic scale during the Paleozoic. In general, the Paleozoic featured a single southern landmass (Gondwana) for most of the era. This megaplate moved relatively sedately northward during this entire time interval (540–250 Ma) and always contained the magnetic and geographic south poles. Consequently, many of the facies and biologic provinces in the Gondwanan region were influenced by the cooler marine realms and continental and mountain glaciers in nearly every Paleozoic period. Most of the tectonic action that produced major periods of collision, mountain building, carbonate platform building, back-arc fringing troughs with their distinctive faunas and lithofaces, and formation of coal basins and evaporites took place in the Northern Hemisphere. These pulsations produced combinations of Laurentian (North American), Euro-Baltic, Uralian, Siberian, and Chinese plates at various times during the Paleozoic; and these combined units, in turn, moved slowly across the latitudes, producing climatic change; lithofacies changed in response to both the climate and the plate tectonics.

     

     

    Fig. 5  Major fossil groups used for detailed biostratigraphy of the Paleozoic and younger strata. These are not total ranges of all groups. (After J. T. Dutro, R. V. Dietrich, and R. M. Foose, eds., AGI Data Sheets, 3d ed., American Geological Institution, 1989)

     

     

     

    fig 5

     

     

     

    Representative geographies that show the range of change have been deduced (Figs. 1–4). The map for the Cambro-Ordovician portrays the general early Paleozoic patterns (Fig. 1); these hold for the entire span of time from the Early Cambrian (about 540 Ma), through the Cambrian, Ordovician, and Silurian, into the early Devonian (about 400 Ma). There were consolidations in the Northern Hemisphere in the Devonian, leading to a northern landmass—the so-called Old Red Continent (Fig. 2)—the forerunner of the Euro-American megaplate of the Carboniferous (Fig. 3), and culminating at the end of the Permian in the Pangaean continental mass (Fig. 4). This, in turn, set the stage for the breakup of Pangaea during the subsequent Mesozoic tectonic megacyle. See also: Paleogeography

     

    Biogeography and biostratigraphy

     

    The complexities of evolution from relatively simple forms at the beginning of the era to more advanced faunas and floras at the beginning of the Mesozoic produced a web of distributions in both time and space during the Paleozoic. In general terms, there were fewer and simpler life forms in the Cambrian—often termed the Age of Trilobites. All groups of invertebrates and plants became more numerous through geologic time. For example, 7 major invertebrate animal groups at the beginning of the Cambrian doubled to 14 by the end of the period, 20 by the end of the Ordovician, 23 at the end of the Devonian, and 25 at the end of the Paleozoic. The pattern for plant diversification, although starting later, is similar. Three simple plant groups became 5 by the end of the Silurian, 7 at the end of the Devonian, and 13 at the end of the Paleozoic. The vertebrates also diversified very slowly. From one or two groups in the Cambro-Ordovician (conodonts are now considered primitive vertebrates), the number of major kinds rose to 6 at the end of the Devonian and 8 at the end of the Paleozoic.

    Biostratigraphic usefulness of fossils varies widely. Certain groups have been shown empirically to be more useful than others, and the abundance and diversity within these groups change from system to system during the Paleozoic. Groups with wide dispersal, occurrences in several facies, and rapid rates of evolution have proved most useful (Fig. 5). In the Paleozoic, trilobites are most valuable in the Cambrian and Ordovician; conodonts are more widely studied and are providing detailed biochronologic control for many system, stage, and zonal boundaries. Graptolites are indispensible in the deeper-water facies of the Ordovician through Early Devonian; goniatite cephalopods provide standards in the Devonian through the Permian; and fusulinids have long been essential for detailed work in the Carboniferous and Permian. Of course, all groups are useful for other kinds of paleobiologic research. Paleoenvironmental, paleoecological, and paleobiogeographic reconstructions use all appropriate biologic, chemical, and physical data in developing models of ancient Paleozoic worlds. See also: Biogeography; Cephalopoda; Conodont; Fusulinacea; Geologic time scale; Graptolithina; Index fossil; Paleoecology; Stratigraphy; Trilobita

     

    • A. F. Embry, B. Beauchamp, and D. J. Glass (eds.), Pangea: Global Environments and Resources, Canadian Society Petroleum Geologists Memoir 17, 1994
    • F. M. Gradstein, J. G. Ogg, A. G. Smith (eds.), A Geological Time Scale 2004, 2005
    • M. R. House, C. T. Scrutton, and M. G. Bassett (eds.), The Devonian System, Spec. Pap. Palaeont. 23, Palaeontological Association, London, 1979
    • E. G. Kauffman and J. E. Hazel (eds.), Concepts and Methods of Biostratigraphy, 1977
    • W. S. McKerrow and C. R. Scotese (eds.), Palaeozoic Palaeogeography and Biogeography, Geol. Soc. Mem. 12, Geological Society, London, 1990
    • R. C. Moore et al., Treatise on Invertebrate Paleontology, Part A, 1979
    • G. C. Young and J. R. Lauries (eds.), An Australian Phanerozoic Time Scale, Oxford University Press, 1996

     

    مقاله به زبان اصلی با عنوان آنالیز گسل

    Fault analysis

    The detection and diagnosis of malfunctions in technical systems. Such systems include production equipment (chemical plants, steel mills, paper mills, and power stations), transportation vehicles (ships, airplanes, automobiles), and household appliances (washing machines, air conditioners). In any of these systems, malfunctions of components may lead to damage of the equipment itself, degradation of its function or product, jeopardy of its mission, and hazard to human life. While the need to detect and diagnose malfunctions is not new, advanced fault detection has been made possible only by the proliferation of the computer. Fault detection and diagnosis actually means a scheme in which a computer monitors the technical equipment to signal any malfunction and determines the components responsible. The detection and diagnosis of the fault may be followed by automatic actions, enabling the fault to be corrected such that the system may operate successfully even under the particular faulty condition.

     

    Diagnostic concepts

     

    Fault detection and diagnosis applies to both the basic technical equipment and the actuators and sensors attached to it. In the case of a chemical plant, the former includes the reactors, distillation columns, heat exchangers, compressors, storage tanks, and piping. Typical faults are leaks, plugs, surface fouling, and broken moving parts. The actuators are mostly valves, together with their driving devices (electric motors and hydraulic or pneumatic drives). The sensors are devices measuring the different physical variables in the plant, such as thermocouples, pressure diaphragms, and flow meters. Actuator and sensor fault detection is very important because these devices are prone to faults.

    The on-line or real-time detection and diagnosis of faults means that the equipment is constantly monitored during its regular operation by a permanently connected computer, and any discrepancy is signaled almost immediately. On-line monitoring is very important for the early detection of any component malfunction before it can lead to more substantial equipment failure. In contrast, off-line diagnosis involves monitoring the system by a special, temporarily attached device, under special conditions (for example, car diagnostics at a service station).

    The diagnostic activity may be broken down into several logical stages. Fault detection is the indication of something going wrong in the system. Fault isolation is the determination of the fault location (the component which malfunctions), while fault identification is the estimation of its size. On-line systems usually contain the detection and isolation stage; in off-line systems, detection may be superfluous. Fault identification is usually less important than the two other stages.

    Fault detection and isolation can never be performed with absolute certainty because of circumstances such as noise, disturbances, and model errors. There is always a trade-off between false alarms and missed detections, with the proper balance depending on the particular application. In professionally supervised large plants, false alarms are better tolerated and missed detections may be more critical, while in consumer equipment (including cars) the situation may be the opposite.

     

    Approaches

     

    A number of different approaches to fault detection and diagnosis may be used individually or in combination.

     

    Limit checking

     

    In this approach, which is the most widely used, system variables are monitored and compared to preset limits. This technique is simple and appealing, but it has several drawbacks. The monitored variables are system outputs that depend on the inputs. To make allowance for the variations of the inputs, the limits often need to be chosen conservatively. Furthermore, a single component fault may cause many variables to exceed their limits, so it may be extremely difficult to determine the source. Monitoring the trends of system variables may be more informative, but it also suffers from the same drawbacks as limit checking.

     

    Special and multiple sensors

     

    Special sensors may be applied to perform the limit-checking function (such as temperature or pressure limit sensors) or to monitor some fault-sensitive variable (such as vibration or sound). Such sensors are used mostly in noncomputerized systems. Multiple sensors may be applied to measure the same system variable, providing physical redundancy. If two sensors disagree, at least one of them is faulty. A third sensor is needed to isolate the faulty component (and select the accepted measurement value) by “majority vote.” Multiple sensors may be expensive, and they provide no information about actuator and plant faults.

     

    Frequency analysis

     

    This procedure, in which the Fourier transforms of system variables are determined, may supply useful information about fault conditions. The healthy plant usually has a characteristic spectrum, which will change when faults are present. Particular faults may have their own typical signature (peaks at specific frequencies) in the spectrum.  See also: Fourier series and transforms

     

    Fault-tree analysis

     

    Fault trees are the graphic representations of the cause-effect relations in the system. On the top of the tree, there is an undesirable or catastrophic system event (top event), with the possible causes underneath (intermediate events), down to component failures or other elementary events (basic events) that are the possible root causes of the top event. Thelogic relationships from bottom up are represented by AND and OR (or more complex) logic gates. Fault trees can be used in system design to evaluate the potential risks associated with various component failures under different design variants (bottom-up analysis). In a fault diagnosis framework, the tree is used top down; once the top event is observed, the potential causes are analyzed by following the logic paths backward.

     

    Parameter estimation

     

    This procedure uses a mathematical model of the monitored system. The parameters of the model are estimated from input and output measurements in a fault-free reference situation. Repeated new estimates are then obtained on-line in the normal course of system operation. Deviations from the reference parameters signify changes in the plant and a potential fault. The faulty component location may be isolated by computing the new physical plant parameters and comparing them with those from the model.  See also: Estimation theory; Model theory

     

    Consistency checking

     

    This is another way of using the mathematical-system model. The idea is to check if the observed plant outputs are consistent with the outputs predicted by the model (Fig. 1). Discrepancies indicate a deviation between the model and the plant (parametric faults) or the presence of unobserved variables (additive faults). This testing concept is also called analytical redundancy since the model equations are used in a similar way as multiple sensors.

     

    In preparation for fault monitoring by analytical redundancy methods, a mathematical model of the plant needs to be established. This may be done from “first principles,” relying on the theoretical understanding of the plant's operation, or by systems identification using experimental data from a fault-free plant.

    The actual implementation of fault monitoring usually consists of two stages (Fig. 1). The first is residual generation, where residuals are mathematical quantities expressing the discrepancy between the actual plant behavior and the one expected based on the model. Residuals are nominally zero and become nonzero by the occurrence of faults. The second stage is residual evaluation and decision making, where the residuals are subjected to threshold tests and logic analysis. Disturbances and model errors may also cause the residuals to become nonzero, leading to false alarms.

    Fault isolation requires specially manipulated sets of residuals. In the most frequently used approach, residuals are arranged so that each one is sensitive to a specific subset of faults (structured residuals). Then in response to a particular fault, only a fault-specific subset of residuals triggers its test, leading to binary fault codes.

     

    Principal component analysis (PCA)

     

    In this approach, empirical data (input and output measurements) are collected from the plant. The eigenstructure analysis of the data covariance matrix yields a statistical model of the system in which the eigenvectors point at the “principal directions” of the relationships in the data, while the eigenvalues indicate the data variance in the principal directions. This method is successfully used in the monitoring of large systems. By revealing linear relations among the variables, the dimensionality of the model is significantly reduced. Faults may be detected by relating plant observations to the normal spread of the data, and outliers indicate abnormal system situations. Residuals may also be generated from the principal component model, allowing the use of analytical redundancy methods in this framework.  See also: Eigenfunction

     

     

    Example of fault-tree analysis

     

    The schematic of a simple electrical circuit in which a light is operated by a pair of three-way switches is shown in Fig. 2. (Such circuits are used in long hallways.) Figure 3 shows the detailed fault tree of the circuit. The tree goes down to subcomponents (contacts of the switches) in order to illustrate more complex logic relations on this simple system. Note that nonfailure events (operating conditions) are also among the basic events because such conditions (the position of each switch) determine whether a particular failure event triggers the top event.

    Example of consistency checking

     

    Traditionally, a few fundamental variables, such as coolant temperature, oil pressure, and battery voltage, have been monitored in automobile engines by using limit sensors. With the introduction of onboard microcomputers, the scope and number of variables that can be considered have been extended. Active functional testing may be applied to at least one actuator, typically the exhaust-gas recirculation valve. Model-based schemes to cover the components affecting the vehicle's emission control system are gradually introduced by manufacturers. One approach (Fig. 4) uses analytical redundancy to monitor two groups of actuators (fuel injectors and exhaust gas recirculation) and four sensors (throttle position, manifold pressure, engine speed, and exhaust oxygen). By the appropriate selection of the model relations, the residuals are insensitive to the load torque and the vehicle's mass. The structured residual technique is used to support fault isolation. The critical issue is to find sufficiently general models so that a single scheme may function well across an entire automobile product line and under widely varying operating conditions.  See also: Automotive engine; Microcomputer; Microprocessor

    Janos J. Gertler

     

    Bibliography

     

     

    • L. H. Chiang, R. D. Braatz, and E. Russel, Fault Detection and Diagnosis in Industrial Systems, Springer, 2001
    • P. L. Clemens, Fault Tree Analysis, 4th ed., Jacobs Sverdrup, 2002
    • J. Gertler, Fault Detection and Diagnosis in Engineering Systems, 1998
    • J. Gertler, Survey of model-based failure detection and isolation in complex plants, IEEE Control Sys. Mag., 8(7):3–11, 1988
    • R. Patton, P. Frank, and R. Clark (eds.), Fault Diagnosis in Dynamic Systems, 1989

     

    Additional Readings

     

     

    • Fault Tree Analysis

    بررسی منطقه هشجين

     

    خلاصه مطالب:
         توده هاي نفوذي حد واسط تا اسيد زون آتشفشاني- رسوبي ترشير منطقه هشجين به عنوان بخشي از زون آتشفشاني – رسوبي ترشير البرز غربي- آذربايجان نهشته هاي آتشفشاني و آذر آواري ائوسن را قطع كرده و توسط نهشته هاي آهكي و مارني ميوسن زيرين ( بورديگالين) با اگر دگر شيبي فرسايشي پوشيده مي شود.
       توده هاي منفرد كوچك بخش شمال خاوري چهار گوش هشجين در يك راستاي NW-SE و در مسير رودخانه قزل اوزن در عمق بيشتري جايگيري كرده و در اطراف آنها دگر سانيگرمايي و كاني سازيهاي وابسته مشاهده مي گردد. توده هاي بخش مركزي و جنوبي محدوده مذكور در تراز بالاتري جايگزين شده و فاقد زونهاي دگر ساني گرمابي وسيع مي باشند.
       اين توده ها ويژگي گرانتيوئيدهاي تيپ I حواشي فعال قاره اي را دارا بوده و از انواع بعد تكتونيك بشمار مي آيند. اين نوار آتشفشاني- رسوبي محصول تصادم قوس- قاره بوده و در يك حوضه كششي پشت قوس در حواشي فعال قاره اي تكوين يافته اند. ( علوي 1996)
      
       پيش گفتار:
         چهار گوش هشجين بين طولهاي جغرافيائي شرقي 48 درجه تا و عرضهاي جغرافيائي شمالي 37درجه تا محدود شده است. بخش عمده رخنمون سنگي اين چهار گوش متعلق به سنگهاي نوار ماگمايي ترشير زون البرز غربي- آذربايجان بوده و در بخش شمال خاوري آن مجموعه اي از سنگهاي رسوبي پائوژن و كرتاسه بر روي واحدهاي آتشفشاني و آذرآواري ائوسن و اليگوسن رانده شده اند. راندگي از شمالشرق به سمت جنوب غرب در نهشته هاي ائوسن و اليگوسن و ساختارهاي تكتونيكي آنها تأثير داشته و سطوح محوري تاقديسهاي موجود در آنها را به سمت NE شيبدار كرده و در نهايت چينهايي با يك يال خوابيده را تشكيل داده است.
       انديسهاي معدني متعدد فلزي و غير فلزي در نقاط مختلف اين چهار گوش و مناطق مجاور، تنوع ماگماتيسم و پتانسيل بالاي منطقه به جهت زايش كانسارهاي تيپ مس يا طلا پورفيري محرك اصلي در تعيين پتروژنز توده هاي نفوذي اين منطقه بوده است.

    بحث:
          نوار آتشفشاني – رسوبي ترشير البرز غربي- آذربايجان با روند عمومي NE-SE محصول فازهاي كششي پيرنه است كه بدنبال فاز فشارشي لاراميد حادث شده است و آتشفشاني ائوسن عمدتاً از تيپ زير دريائي است.
    بدنبال فعاليت زير دريائي ائوسن، نهشته هاي آذرآواري و آتشفشاني با مشخصه حدواسط تا اسيد با دگرشيبي زاويه اي اندك( حدود 20درجه)، واحدهاي ائوسن را پوشانيده اند و هر دو مجموعه توسط توده هاي نفوذي نيمه عميق با تركيبي در حد مونزوديوريت، كوارتز- مونزوديوريت، مونزوگرانيت، كوارتز مونزونيت و كوارتز سينيت مورد تهاجم قرار گرفته اند. توده هاي نفوذي با تركيب و وضعيت زمين شناسي مشابهي در منطقه ساوه توسط (كايا و همكاران 1978) بروش K-Ar سن يابي شده اند كه برابر 2±37 ميليون سال تعيين شده است.
    همبري اين توده ها با سنگهاي درونگير شارپ بوده و دگرگوني مجاورتي در حد رخساره آلبيت – اپيدوت هورنفلس در حاشيه آنها مشاهده مي گردد. آنكلاوهاي موجود در آنها زير دانه مافيك و ندرتاً فلسيك بوده و زينوليتهائي از سنگهاي آتشفشاني و آتشفشاني آواري در بخشهاي حاشيه اي اين توده ها مشاهده مي گردد. اشكال عدسي شكل و تخم مرغي آنكلاوها نشانگر تغيير شكل ناشي از جريان ماگما و به تبع آن اعمال نيروهاي برشي در حين جايگيري مي باشد. بهمين ترتيب آنكلاوهاي زاويه دار انعكاسي از تغيير شكل در حالت جامد و يا در شرايط جريان ماگما با گرانروي بالاست.
    توده هاي نفوذي از انواع ساب سولووس بوده و ويژگيهاي كاني شناسي و بافتي نشانگر وجود فاز بخاري با فشار بالا در ماگماي مولد اين توده ها مي باشد. بررسيهاي ژئوشيميائي اين توده ها نشان مي دهد كه اغلب آنها داراي مشخصه متاآلومين بوده و تعداد محدودي از آنها ويژگي پرآلكالن نشان مي دهند.در دياگرامهاي Sio2-K2o اغلب نمونه ها در محدوده سريهاي با پتانسيم بالا و شوشونيتي قرار مي گيرند و متعلق به انواع I مي باشند. بررسي تغييرات عناصر اصلي و كمياب نشان از آلايش با مواد پوسته اي و اختلاط ماگمائي دارد كه اين امر از طريق مطالعات بافتي نيز به اثبات رسيده است.
    قرابت زماني و مكاني توده هاي نفوذي منطقه هشجين با سنگهاي آتشفشاني همراه و همخون، ويژگي متاآلومين تا پرآلكالين توده ها، وجود زونهاي دگرساني گرمابي وسيع در اطراف آنها و ويژگيهاي بافتي و كاني شناسي اين توده ها نشان مي دهند كه آنها متعلق به گرانيتوئيدهاي تيپ I بوده و در رده بندي گرانيتوئيدها بر اساس اكسيدهاي عناصر اصلي ( مانيار و پيكولي1989) در محدوده گرانيتوئيدهاي قوسهاي حواشي فعال قاره اي و گرانيتوئيدهاي مرتبط با بالا زدگي پوسته قاره اي بعد از تصادم قرار مي گيرند و تطابق جالبي با زير گروه C از گرانيتوئيدهاي مرتبط با قوسهاي آتشفشاني دارند.
    غني شدگي بالا از عناصري نظير Th,Ba,Rb,K انعكاسي از نقش پوسته قاره اي در تحولات ماگمائي بوده و به عنوان تسلط پوسته اي از آن ياد شده است (هاريس و همكاران 1983). آنومالي منفي و مقادير اندك عناصري نظير Hf,Zr,Ce اغلب در توده هاي مناطق تصادمي قاره – قاره وبعد از تكتونيك مشاهده مي گردد كه از ويژگيهاي ژئوشيميائي توده هاي منطقه محسوب مي شود. گرانيتوئيدهاي بعد تكتونيك مناطق تصادمي محصول ذوب پوسته تحتاني دراثر استقرار دياپيرهاي گوشته اي اند كه ويژگيهاي گرانيتوئيدهاي داخل صفحات (WPG) و برخي از انواع قوسهاي آتشفشاني (VAG) را بطور همزمان منعكس مي سازند. دياگرام عنكبوتي رسم شده براي توده هاي نفوذي منطقه تشابه جالب آنها را با انواع قوسهاي آتشفشاني حواشي فعال قاره اي ( نظيرشيلي) و تا حدودي با انواع داخل صفحات بعد از تصادم را نشان مي دهد.

    نتيجه گيري:
         زون ماگمائي مذكور از شمال به فرو افتادگي خزر كه يك حوضه كششي پشت قوس فرض شده ( زونن شاين و لوپيشون 1986) محدود شده و از جنوب غرب به كمان ماگمائي تبريز- بزمان محدود مي شود. اين نوار محصول فرورانش يك حوضه كششي پشت قوسي است كه بين جزاير قوسي تبريز- بزمان و بلوك قاره اي البرز واقع بوده و در اثر فروانش آن به سمت شمال و شمالشرق و احتمالا با يك حركت دوراني ( به علت زاويه موجود بين نوار ماگمائي تبريز- بزمان و زون ماگمائي البرز غربي – آذربايجان) تصادم قوس- قاره انجام شده و برخي از فعاليتهاي جوان اين نوار را نيز مي توان به اتساع و بالا زدگيهاي بعد از تصادم نسبت داد.