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Asian Paleocene-Early Eocene Chronology and Biotic Events
©Geol. Bundesanstalt, Wien; download unter www.geologie.ac.at Berichte Geol. B.-A., 85 (ISSN 1017-8880) – CBEP 2011, Salzburg, June 5th – 8th Asian Paleocene-Early Eocene Chronology and biotic events Suyin Ting1, Yongsheng Tong2, William C. Clyde3, Paul L.Koch4, Jin Meng5, Yuanqing Wang2, Gabriel J. Bowen6, Qian Li2, Snell E. Kathryn4 1 LSU Museum of Natural Science, Baton Rouge, LA 70803, USA 2 Institute of Vert. Paleont. & Paleoanth., CAS., Beijing 100044, China 3 University of New Hampshire, Durham, NH 03824, USA 4 University of California Santa Cruz, Santa Cruz, CA 95064, USA 5 American Museum of Natural History, New York, NY 10024, USA 6 Purdue University, West Lafayette, IN 47907, USA Biostratigraphic, chemostratigraphic, and magnetostratigraphic studies of the Paleocene and early Eocene strata in the Nanxiong Basin of Guangdong, Chijiang Basin of Jiangxi, Qianshan Basin of Anhui, Hengyang Basin of Hunan, and Erlian Basin of Inner Mongolia, China, in last ten years provide the first well-resolved geochronological constrains on stratigraphic framework for the early Paleogene of Asia. Asian Paleocene and early Eocene strata are subdivided into four biochronological units based on the fossil mammals (Land Mammal Ages). From oldest to youngest, they are the Shanghuan, the Nongshanian, the Gashatan, and the Bumbanian Asian Land Mammal Ages (ALMA). Recent paleomagnetic data from the Nanxiong Basin indicate that the base of the Shanghuan lies about 2/3 the way up Chron C29r. Nanxiong data and recent paleomagnetic and isotopic results from the Chijiang Basin show that the Shanghuan-Nongshanian ALMA boundary lies between the upper part of Chron C27n and the lower part of Chron C26r, close to the Chron C27n-C26r reversal. -
A/L Hcan %Mlsdum
A/LSoxfitateshcan %Mlsdum PUBLISHED BY THE AMERICAN MUSEUM OF NATURAL HISTORY CENTRAL PARK WEST AT 79TH STREET, NEW YORK 24, N.Y. NUMBER 1957 AUGUST 5, 1959 Fossil Mammals from the Type Area of the Puerco and Nacimiento Strata, Paleocene of New Mexico BY GEORGE GAYLORD SIMPSON ANTECEDENTS The first American Paleocene mammals and the first anywhere from the early to middle Paleocene were found in the San Juan Basin of New Mexico. Somewhat more complete sequences and larger faunas are now known from elsewhere, but the San Juan Basin strata and faunas are classical and are still the standard of comparison for the most clearly established lower (Puercan), middle (Torrejonian), and upper (Tiffanian) stages and ages. The first geologist to distinguish clearly what are now known to be Paleocene beds in the San Juan Basin was Cope in 1S74. He named them "Puercan marls" (Cope, 1875) on the basis of beds along the upper Rio Puerco, and especially of a section west of the Rio Puerco southwest of the then settlement of Nacimiento and of the present town of Cuba, on the southern side of Cuba Mesa. Cope reported no fossils other than petrified wood, but in 1880 and later his collector, David Baldwin, found rather abundant mammals, described by Cope (1881 and later) in beds 50 miles and more to the west and northwest of the type locality but referred to the same formation. In the 1890's Wortman collected for the American Museum in the Puerco of Cope, and, on the basis of this work, Matthew (1897) recognized the presence of two quite distinct faunas of different ages. -
Asteroid Impact, Not Volcanism, Caused the End-Cretaceous Dinosaur Extinction
Asteroid impact, not volcanism, caused the end-Cretaceous dinosaur extinction Alfio Alessandro Chiarenzaa,b,1,2, Alexander Farnsworthc,1, Philip D. Mannionb, Daniel J. Luntc, Paul J. Valdesc, Joanna V. Morgana, and Peter A. Allisona aDepartment of Earth Science and Engineering, Imperial College London, South Kensington, SW7 2AZ London, United Kingdom; bDepartment of Earth Sciences, University College London, WC1E 6BT London, United Kingdom; and cSchool of Geographical Sciences, University of Bristol, BS8 1TH Bristol, United Kingdom Edited by Nils Chr. Stenseth, University of Oslo, Oslo, Norway, and approved May 21, 2020 (received for review April 1, 2020) The Cretaceous/Paleogene mass extinction, 66 Ma, included the (17). However, the timing and size of each eruptive event are demise of non-avian dinosaurs. Intense debate has focused on the highly contentious in relation to the mass extinction event (8–10). relative roles of Deccan volcanism and the Chicxulub asteroid im- An asteroid, ∼10 km in diameter, impacted at Chicxulub, in pact as kill mechanisms for this event. Here, we combine fossil- the present-day Gulf of Mexico, 66 Ma (4, 18, 19), leaving a crater occurrence data with paleoclimate and habitat suitability models ∼180 to 200 km in diameter (Fig. 1A). This impactor struck car- to evaluate dinosaur habitability in the wake of various asteroid bonate and sulfate-rich sediments, leading to the ejection and impact and Deccan volcanism scenarios. Asteroid impact models global dispersal of large quantities of dust, ash, sulfur, and other generate a prolonged cold winter that suppresses potential global aerosols into the atmosphere (4, 18–20). These atmospheric dinosaur habitats. -
The Geologic Time Scale Is the Eon
Exploring Geologic Time Poster Illustrated Teacher's Guide #35-1145 Paper #35-1146 Laminated Background Geologic Time Scale Basics The history of the Earth covers a vast expanse of time, so scientists divide it into smaller sections that are associ- ated with particular events that have occurred in the past.The approximate time range of each time span is shown on the poster.The largest time span of the geologic time scale is the eon. It is an indefinitely long period of time that contains at least two eras. Geologic time is divided into two eons.The more ancient eon is called the Precambrian, and the more recent is the Phanerozoic. Each eon is subdivided into smaller spans called eras.The Precambrian eon is divided from most ancient into the Hadean era, Archean era, and Proterozoic era. See Figure 1. Precambrian Eon Proterozoic Era 2500 - 550 million years ago Archaean Era 3800 - 2500 million years ago Hadean Era 4600 - 3800 million years ago Figure 1. Eras of the Precambrian Eon Single-celled and simple multicelled organisms first developed during the Precambrian eon. There are many fos- sils from this time because the sea-dwelling creatures were trapped in sediments and preserved. The Phanerozoic eon is subdivided into three eras – the Paleozoic era, Mesozoic era, and Cenozoic era. An era is often divided into several smaller time spans called periods. For example, the Paleozoic era is divided into the Cambrian, Ordovician, Silurian, Devonian, Carboniferous,and Permian periods. Paleozoic Era Permian Period 300 - 250 million years ago Carboniferous Period 350 - 300 million years ago Devonian Period 400 - 350 million years ago Silurian Period 450 - 400 million years ago Ordovician Period 500 - 450 million years ago Cambrian Period 550 - 500 million years ago Figure 2. -
Making a Timeline Rope
Making a Timeline Rope Background: Your timeline rope invites students to focus on recent periods of geologic time. This rope demonstrates four periods and seven epochs, beginning with the Jurassic Period in the Mesozoic Era, in the Phanerozoic Eon, and ending at the present time, in the Holocene Epoch, in the Quaternary Period of the Cenozoic Era, in the Phanerozoic Eon. Standards: SC.D.1.2.3 SC.D.1.2.5 SC.D.1.3.1 SC.D.1.3.2 SC.D.1.3.3 MA.1.G.5.1 MA.1.G.5.2 MA.2.G.3.4 MA.2.G.3.1 MA.3.G.5.2 MA.4.G.3.3 MA.6.A.5.1 MA.8.A.1.3 SC.912.E.5.3 SC.912.E.6.4 SC.912.E.6.5 SC.912.N.3.1 SC.912.N.3.5 Objectives: − Analyze how specific geological processes and features are expressed in Florida and elsewhere − Describe the geological development of the present day oceans and identify commonly found features − Understand the function of models in science, and identify the wide range of models used. − Compare, contrast, and convert units of measure Vocabulary: Geologists and paleontologists give names to spans of many years. Spans are approximate; they relate more to fossil age ranges than to absolute years. Experts use a common vocabulary. Eon: Largest division of geologic time. Each eon contains several periods and can last for hundreds of millions to billions of years. Some experts identify four eons. (Example: Life on earth has been abundant during the Phanerozoic Eon, as well- preserved fossils prove.) Era: Shorter than an eon. -
The Cretaceous-Tertiary Boundary Interval in Badlands National Park, South Dakota
The Cretaceous-Tertiary Boundary Interval in Badlands National Park, South Dakota Philip W. Stoffer1 Paula Messina John A. Chamberlain, Jr. Dennis O. Terry, Jr. U.S. Geological Survey Open-File Report 01-56 2001 U.S. DEPARTMENT OF THE INTERIOR Gale A. Norton, Secretary U.S. GEOLOGICAL SURVEY Charles G. Groat, Director The Cretaceous/Tertiary (K-T) boundary study interval at the Rainbow Colors Overlook along Badlands Loop Road, North Unit of Badlands National Park. This report is preliminary and has not been reviewed for conformity with U.S. Geological Survey (USGS) editorial standards or with the North American Stratigraphic Code. Any use of trade, firm, or product names is for descriptive purposes only and does not imply endorsement by the U.S. Government. 1345 Middlefield Road, Menlo Park, CA 94025 http://geopubs.wr.usgs.gov/open-file/of01-056/ ABSTRACT A marine K-T boundary interval has been identified throughout the Badlands National Park region of South Dakota. Data from marine sediments suggest that deposits from two asteroid impacts (one close, one far away) may be preserved in the Badlands. These impact- generated deposits may represent late Maestrichtian events or possibly the terminal K-T event. Interpretation is supported by paleontological correlation, sequence stratigraphy, magnetostratigraphy, and strontium isotope geochronology. This research is founded on nearly a decade of NPS approved field work in Badlands National Park and a foundation of previously published data and interpretations. The K-T boundary occurs within -
Uncorking the Bottle: What Triggered the Paleocene/Eocene Thermal Maximum Methane Release? Miriame
PALEOCEANOGRAPHY, VOL. 16, NO. 6, PAGES 549-562, DECEMBER 2001 Uncorking the bottle: What triggered the Paleocene/Eocene thermal maximum methane release? MiriamE. Katz,• BenjaminS. Cramer,Gregory S. Mountain,2 Samuel Katz, 3 and KennethG. Miller,1,2 Abstract. The Paleocene/Eocenethermal maximum (PETM) was a time of rapid global warming in both marine and continentalrealms that has been attributed to a massivemethane (CH4) releasefrom marine gas hydrate reservoirs. Previously proposedmechanisms for thismethane release rely on a changein deepwatersource region(s) to increasewater temperatures rapidly enoughto trigger the massivethermal dissociationof gas hydratereservoirs beneath the seafloor.To establish constraintson thermaldissociation, we modelheat flow throughthe sedimentcolumn and showthe effectof the temperature changeon the gashydrate stability zone throughtime. In addition,we provideseismic evidence tied to boreholedata for methanerelease along portions of the U.S. continentalslope; the releasesites are proximalto a buriedMesozoic reef front. Our modelresults, release site locations, published isotopic records, and oceancirculation models neither confirm nor refute thermaldissociation as the triggerfor the PETM methanerelease. In the absenceof definitiveevidence to confirmthermal dissociation,we investigatean altemativehypothesis in which continentalslope failure resulted in a catastrophicmethane release.Seismic and isotopic evidence indicates that Antarctic source deepwater circulation and seafloor erosion caused slope retreatalong -
A Fundamental Precambrian–Phanerozoic Shift in Earth's Glacial
Tectonophysics 375 (2003) 353–385 www.elsevier.com/locate/tecto A fundamental Precambrian–Phanerozoic shift in earth’s glacial style? D.A.D. Evans* Department of Geology and Geophysics, Yale University, P.O. Box 208109, 210 Whitney Avenue, New Haven, CT 06520-8109, USA Received 24 May 2002; received in revised form 25 March 2003; accepted 5 June 2003 Abstract It has recently been found that Neoproterozoic glaciogenic sediments were deposited mainly at low paleolatitudes, in marked qualitative contrast to their Pleistocene counterparts. Several competing models vie for explanation of this unusual paleoclimatic record, most notably the high-obliquity hypothesis and varying degrees of the snowball Earth scenario. The present study quantitatively compiles the global distributions of Miocene–Pleistocene glaciogenic deposits and paleomagnetically derived paleolatitudes for Late Devonian–Permian, Ordovician–Silurian, Neoproterozoic, and Paleoproterozoic glaciogenic rocks. Whereas high depositional latitudes dominate all Phanerozoic ice ages, exclusively low paleolatitudes characterize both of the major Precambrian glacial epochs. Transition between these modes occurred within a 100-My interval, precisely coeval with the Neoproterozoic–Cambrian ‘‘explosion’’ of metazoan diversity. Glaciation is much more common since 750 Ma than in the preceding sedimentary record, an observation that cannot be ascribed merely to preservation. These patterns suggest an overall cooling of Earth’s longterm climate, superimposed by developing regulatory feedbacks -
Small-Scale Post-Noachian Volcanism in the Martian Highlands? Insights from Terra Sirenum P
45th Lunar and Planetary Science Conference (2014) 1104.pdf SMALL-SCALE POST-NOACHIAN VOLCANISM IN THE MARTIAN HIGHLANDS? INSIGHTS FROM TERRA SIRENUM P. Brož1,2 and E. Hauber3 1Institute of Geophysics ASCR, v.v.i., Prague, Czech Republic, [email protected], 2Institute of Petrology and Structural Geology, Charles University, Czech Republic 3Institute of Planetary Research, DLR, Berlin, Germany, [email protected]. Introduction: Volcanism was globally widespread on Mars in the early history of the planet, but focused with ongoing evolution on two main provinces in Tharsis and Elysium [1]. On the other hand, evidence for post-Noachian volcanism in the Martian highlands is rare outside some isolated regions (e.g., Tyrrhena and Hadriaca Montes) and, to our knowledge, few, if any, such volcanic edifices have been reported so far. It is generally thought that highland volcanism oc- curred early in Mars` history and stopped not later than ~1 Ga after planet formation [2, 3]. Several candidate locations were suggested as volcanic centers in western Gorgonum and south-eastern Atlantis basins [4], where extensive accumulations of possible volcanic deposits exist, however, these volcanic centers were not con- firmed by later studies [5, 6]. Based on our observations we report several prom- ising edifices in Terra Sirenum that might change this view. The study area is situated south of Gorgonum Fig. 1: Themis-IR day-time (upper image), night-time (mid- basin and is about 150x50 km wide. It contains two dle), and interpretational map of the study area. The thermal spectacular cones with outgoing flow-like features and contrast between the two upper images suggests the presence 3 dome-like structures (Fig. -
Selandian-Thanetian Larger Foraminifera from the Lower Jafnayn Formation in the Sayq Area (Eastern Oman Mountains)
Geologica Acta, Vol.14, Nº 3, September, 315-333 DOI: 10.1344/GeologicaActa2016.14.3.7 Selandian-Thanetian larger foraminifera from the lower Jafnayn Formation in the Sayq area (eastern Oman Mountains) J. SERRA-KIEL1 V. VICEDO2,* Ph. RAZIN3 C. GRÉLAUD3 1Universitat de Barcelona, Facultat de Geologia. Department of Earth and Ocean Dynamics Martí Franquès s/n, 08028 Barcelona, Spain. 2Museu de Ciències Naturals de Barcelona (Paleontologia) Parc de la Ciutadella s/n, 08003 Barcelona, Spain 3ENSEGID, Bordeaux INP, G&E, EA, 4592, University of Bordeaux III, France 1 allée F. Daguin, 33607 PESSAC cedex, France *Corresponding author E-mail: [email protected] ABS TR A CT The larger foraminifera of the lower part of the Jafnayn Formation outcropping in the Wadi Sayq, in the Paleocene series of the eastern Oman Mountains, have been studied and described in detail. The analysis have allowed us to develop a detailed systematic description of each taxa, constraining their biostratigraphic distribution and defining the associated foraminifera assemblages. The taxonomic study has permitted us to identify each morphotype precisely and describe three new taxa, namely, Ercumentina sayqensis n. gen. n. sp. Lacazinella rogeri n. sp. and Globoreticulinidae new family. The first assemblage is characterized by the presence ofCoskinon sp., Dictyoconus cf. turriculus HOTTINGER AND DROBNE, Anatoliella ozalpiensis SIREL, Ercumentina sayqensis n. gen. n. sp. SERRA- KIEL AND VICEDO, Lacazinella rogeri n. sp. SERRA-KIEL AND VICEDO, Mandanella cf. flabelliformis RAHAGHI, Azzarolina daviesi (HENSON), Lockhartia retiata SANDER, Dictyokathina simplex SMOUT and Miscellanites globularis (RAHAGHI). The second assemblage is constituted by the forms Pseudofallotella persica (HOTTINGER AND DROBNE), Dictyoconus cf. -
Clay Minerals at the Paleocene–Eocene Thermal Maximum: Interpretations, Limits, and Perspectives
minerals Review Clay Minerals at the Paleocene–Eocene Thermal Maximum: Interpretations, Limits, and Perspectives Fabio Tateo Istituto di Geoscienze e Georisorse, Consiglio Nazionale delle Ricerche (IGG-CNR) Padova, c/o Dipartimento di Geoscienze, Università di Padova, Via Gradenigo 6, I-35131 Padova, Italy; [email protected] Received: 20 October 2020; Accepted: 26 November 2020; Published: 30 November 2020 Abstract: The Paleocene–Eocene Thermal Maximum (PETM) was an “extreme” episode of environmental stress that affected the Earth in the past, and it has numerous affinities concerning the rapid increase in the greenhouse effect. It has left several biological, compositional, and sedimentary facies footprints in sedimentary records. Clay minerals are frequently used to decipher environmental effects because they represent their source areas, essentially in terms of climatic conditions and of transport mechanisms (a more or less fast travel, from the bedrocks to the final site of recovery). Clay mineral variations at the PETM have been studied by several authors in terms of climatic and provenance indicators, but also as tracers of more complicated interplay among different factors requiring integrated interpretation (facies sorting, marine circulation, wind transport, early diagenesis, etc.). Clay minerals were also believed to play a role in the recovery of pre-episode climatic conditions after the PETM exordium, by becoming a sink of atmospheric CO2 that is considered a necessary step to switch off the greenhouse hyperthermal effect. This review aims to consider the use of clay minerals made by different authors to study the effects of the PETM and their possible role as effective (simple) proxy tools for environmental reconstructions. -
Geology and Vertebrate Paleontology of Western and Southern North America
OF WESTERN AND SOUTHERN NORTH AMERICA OF WESTERN AND SOUTHERN NORTH PALEONTOLOGY GEOLOGY AND VERTEBRATE Geology and Vertebrate Paleontology of Western and Southern North America Edited By Xiaoming Wang and Lawrence G. Barnes Contributions in Honor of David P. Whistler WANG | BARNES 900 Exposition Boulevard Los Angeles, California 90007 Natural History Museum of Los Angeles County Science Series 41 May 28, 2008 Paleocene primates from the Goler Formation of the Mojave Desert in California Donald L. Lofgren,1 James G. Honey,2 Malcolm C. McKenna,2,{,2 Robert L. Zondervan,3 and Erin E. Smith3 ABSTRACT. Recent collecting efforts in the Goler Formation in California’s Mojave Desert have yielded new records of turtles, rays, lizards, crocodilians, and mammals, including the primates Paromomys depressidens Gidley, 1923; Ignacius frugivorus Matthew and Granger, 1921; Plesiadapis cf. P. anceps; and Plesiadapis cf. P. churchilli. The species of Plesiadapis Gervais, 1877, indicate that Member 4b of the Goler Formation is Tiffanian. In correlation with Tiffanian (Ti) lineage zones, Plesiadapis cf. P. anceps indicates that the Laudate Discovery Site and Edentulous Jaw Site are Ti2–Ti3 and Plesiadapis cf. P. churchilli indicates that Primate Gulch is Ti4. The presence of Paromomys Gidley, 1923, at the Laudate Discovery Site suggests that the Goler Formation occurrence is the youngest known for the genus. Fossils from Member 3 and the lower part of Member 4 indicate a possible marine influence as Goler Formation sediments accumulated. On the basis of these specimens and a previously documented occurrence of marine invertebrates in Member 4d, the Goler Basin probably was in close proximity to the ocean throughout much of its existence.