Size Variations in Foraminifers from the Early Permian to the Late Triassic: Implications for the Guadalupian–Lopingian and the Permian–Triassic Mass Extinctions
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A Geoconservation perspective on the trace fossil record associated with the end – Ordovician mass extinction and glaciation in the Welsh Basin Item Type Thesis or dissertation Authors Nicholls, Keith H. Citation Nicholls, K. (2019). A Geoconservation perspective on the trace fossil record associated with the end – Ordovician mass extinction and glaciation in the Welsh Basin. (Doctoral dissertation). University of Chester, United Kingdom. Publisher University of Chester Rights Attribution-NonCommercial-NoDerivatives 4.0 International Download date 26/09/2021 02:37:15 Item License http://creativecommons.org/licenses/by-nc-nd/4.0/ Link to Item http://hdl.handle.net/10034/622234 International Chronostratigraphic Chart v2013/01 Erathem / Era System / Period Quaternary Neogene C e n o z o i c Paleogene Cretaceous M e s o z o i c Jurassic M e s o z o i c Jurassic Triassic Permian Carboniferous P a l Devonian e o z o i c P a l Devonian e o z o i c Silurian Ordovician s a n u a F y r Cambrian a n o i t u l o v E s ' i k s w o Ichnogeneric Diversity k p e 0 10 20 30 40 50 60 70 S 1 3 5 7 9 11 13 15 17 19 21 n 23 r e 25 d 27 o 29 M 31 33 35 37 39 T 41 43 i 45 47 m 49 e 51 53 55 57 59 61 63 65 67 69 71 73 75 77 79 81 83 85 87 89 91 93 Number of Ichnogenera (Treatise Part W) Ichnogeneric Diversity 0 10 20 30 40 50 60 70 1 3 5 7 9 11 13 15 17 19 21 n 23 r e 25 d 27 o 29 M 31 33 35 37 39 T 41 43 i 45 47 m 49 e 51 53 55 57 59 61 c i o 63 z 65 o e 67 a l 69 a 71 P 73 75 77 79 81 83 n 85 a i r 87 b 89 m 91 a 93 C Number of Ichnogenera (Treatise Part W) -
Guadalupian, Middle Permian) Mass Extinction in NW Pangea (Borup Fiord, Arctic Canada): a Global Crisis Driven by Volcanism and Anoxia
The Capitanian (Guadalupian, Middle Permian) mass extinction in NW Pangea (Borup Fiord, Arctic Canada): A global crisis driven by volcanism and anoxia David P.G. Bond1†, Paul B. Wignall2, and Stephen E. Grasby3,4 1Department of Geography, Geology and Environment, University of Hull, Hull, HU6 7RX, UK 2School of Earth and Environment, University of Leeds, Leeds, LS2 9JT, UK 3Geological Survey of Canada, 3303 33rd Street N.W., Calgary, Alberta, T2L 2A7, Canada 4Department of Geoscience, University of Calgary, 2500 University Drive N.W., Calgary Alberta, T2N 1N4, Canada ABSTRACT ing gun of eruptions in the distant Emeishan 2009; Wignall et al., 2009a, 2009b; Bond et al., large igneous province, which drove high- 2010a, 2010b), making this a mid-Capitanian Until recently, the biotic crisis that oc- latitude anoxia via global warming. Although crisis of short duration, fulfilling the second cri- curred within the Capitanian Stage (Middle the global Capitanian extinction might have terion. Several other marine groups were badly Permian, ca. 262 Ma) was known only from had different regional mechanisms, like the affected in equatorial eastern Tethys Ocean, in- equatorial (Tethyan) latitudes, and its global more famous extinction at the end of the cluding corals, bryozoans, and giant alatocon- extent was poorly resolved. The discovery of Permian, each had its roots in large igneous chid bivalves (e.g., Wang and Sugiyama, 2000; a Boreal Capitanian crisis in Spitsbergen, province volcanism. Weidlich, 2002; Bond et al., 2010a; Chen et al., with losses of similar magnitude to those in 2018). In contrast, pelagic elements of the fauna low latitudes, indicated that the event was INTRODUCTION (ammonoids and conodonts) suffered a later, geographically widespread, but further non- ecologically distinct, extinction crisis in the ear- Tethyan records are needed to confirm this as The Capitanian (Guadalupian Series, Middle liest Lopingian (Huang et al., 2019). -
Permian (Artinskian to Wuchapingian) Conodont Biostratigraphy in the Tieqiao Section, Laibin Area, South China
Permian (Artinskian to Wuchapingian) conodont biostratigraphy in the Tieqiao section, Laibin area, South China Y.D. Suna, b*, X.T. Liuc, J.X. Yana, B. Lid, B. Chene, D.P.G. Bondf, M.M. Joachimskib, P.B. Wignallg, X.L. Laia a State Key Laboratory of Biogeology and Environmental Geology, China University of Geosciences, Wuhan, 430074, China b GeoZentrum Nordbayern, Universität Erlangen-Nürnberg, Schlossgarten 5, 91054 Erlangen, Germany c Key Laboratory of Marine Geology and Environment, Institute of Oceanology, Chinese Academy of Sciences, Qingdao, 266071, China d Key Laboratory of Marine Mineral Resources, Guangzhou Marine Geological Survey, Ministry of Land and Resources, Guangzhou, 510075, China e State Key Laboratory of Palaeobiology and Stratigraphy, Nanjing Institute of Geology and Palaeontology, 39 East Beijing Road, Nanjing, 210008, R.P. China f School of Environmental Sciences, University of Hull, Hull HU6 7RX, UK g School of Earth and Environment, University of Leeds, Leeds LS2 9JT, UK *Corresponding authors Email: [email protected] (Y.D. Sun) © 2017, Elsevier. Licensed under the Creative Commons Attribution- NonCommercial-NoDerivatives 4.0 International http://creativecommons.org/ licenses/by-nc-nd/4.0/ 1 Abstract Permian strata from the Tieqiao section (Jiangnan Basin, South China) contain several distinctive conodont assemblages. Early Permian (Cisuralian) assemblages are dominated by the genera Sweetognathus, Pseudosweetognathus and Hindeodus with rare Neostreptognathodus and Gullodus. Gondolellids are absent until the end of the Kungurian stage—in contrast to many parts of the world where gondolellids and Neostreptognathodus are the dominant Kungurian conodonts. A conodont changeover is seen at Tieqiao and coincided with a rise of sea level in the late Kungurian to the early Roadian: the previously dominant sweetognathids were replaced by mesogondolellids. -
Proposal of Guadalupian and Component Roadian, Wordian And
Permophiles Issue #34 1999 REPORTS Proposal of Guadalupian and Component morphoclines, absolute dates, and paleomagnetics. Roadian, Wordian and Capitanian Stages as International Standards for the Middle Permian Historic Preamble Prolonged deliberation of SPS members culminated in the man- Series dated formal postal vote by Titular (voting) Members that approved subdivision of the Permian System into three series, in ascending Brian F. Glenister order Cisuralian, Guadalupian and Lopingian (Report of Presi- University of Iowa dent Jin Yugan, Permophiles #29, p. 2). The “——usage of the Department of Geology Guadalupian Series and constituent stages, i.e. the Roadian, the Iowa City, IA 52242, USA Wordian and the Capitanian Stage for the middle part of the Per- mian.” was approved unanimously by 15 voting members. Pro- Bruce R. Wardlaw posal of the Guadalupian as a chronostratigraphic unit of series U. S. Geological Survey rank (Girty, 1902) predates any potential competitors by decades 926A National Center (Glenister et al., 1992). Of the three component stages currently Reston, VA 22092-0001, USA recognized, the upper two (Wordian and Capitanian) enjoy com- parable priority. Capitanian was first employed in a Lance L. Lambert lithostratigraphic sense by Richardson (1904) for the massive reef Department of Physics limestones of the Guadalupe Mountains of New Mexico and West Southwest Texas State University Texas, and the Word was used by Udden et al. (1916) for the San Marcos, TX 78666-4616, USA interbedded clastic/carbonate sequence in the adjacent Glass Moun- tains. Both were used in a strictly chronostratigraphic sense first Claude Spinosa by Glenister and Furnish (1961) as substages of the Guadalupian Stage, referenced by their nominal formations and recognized else- Permian Research Institute where through “ammonoid and fusuline faunas”. -
Lopingian, Permian) of North China
Foss. Rec., 23, 205–213, 2020 https://doi.org/10.5194/fr-23-205-2020 © Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License. The youngest occurrence of embolomeres (Tetrapoda: Anthracosauria) from the Sunjiagou Formation (Lopingian, Permian) of North China Jianye Chen1 and Jun Liu1,2,3 1Key Laboratory of Vertebrate Evolution and Human Origins of Chinese Academy of Sciences, Institute of Vertebrate Paleontology and Paleoanthropology, Chinese Academy of Sciences, Beijing 100044, China 2Chinese Academy of Sciences Center for Excellence in Life and Paleoenvironment, Beijing 100044, China 3College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China Correspondence: Jianye Chen ([email protected]) Received: 7 August 2020 – Revised: 2 November 2020 – Accepted: 16 November 2020 – Published: 1 December 2020 Abstract. Embolomeri were semiaquatic predators preva- 1 Introduction lent in the Carboniferous, with only two species from the early Permian (Cisuralian). A new embolomere, Seroher- Embolomeri are a monophyletic group of large crocodile- peton yangquanensis gen. et sp. nov. (Zoobank Registration like, semiaquatic predators, prevalent in the Carboniferous number: urn:lsid:zoobank.org:act:790BEB94-C2CC-4EA4- and early Permian (Cisuralian) (Panchen, 1970; Smithson, BE96-2A1BC4AED748, registration: 23 November 2020), is 2000; Carroll, 2009; Clack, 2012). The clade is generally named based on a partial right upper jaw and palate from the considered to be a stem member of the Reptiliomorpha, taxa Sunjiagou Formation of Yangquan, Shanxi, China, and is late that are more closely related to amniotes than to lissamphib- Wuchiapingian (late Permian) in age. It is the youngest em- ians (Ruta et al., 2003; Vallin and Laurin, 2004; Ruta and bolomere known to date and the only embolomere reported Coates, 2007; Clack and Klembara, 2009; Klembara et al., from North China Block. -
Paleogeographic Maps Earth History
History of the Earth Age AGE Eon Era Period Period Epoch Stage Paleogeographic Maps Earth History (Ma) Era (Ma) Holocene Neogene Quaternary* Pleistocene Calabrian/Gelasian Piacenzian 2.6 Cenozoic Pliocene Zanclean Paleogene Messinian 5.3 L Tortonian 100 Cretaceous Serravallian Miocene M Langhian E Burdigalian Jurassic Neogene Aquitanian 200 23 L Chattian Triassic Oligocene E Rupelian Permian 34 Early Neogene 300 L Priabonian Bartonian Carboniferous Cenozoic M Eocene Lutetian 400 Phanerozoic Devonian E Ypresian Silurian Paleogene L Thanetian 56 PaleozoicOrdovician Mesozoic Paleocene M Selandian 500 E Danian Cambrian 66 Maastrichtian Ediacaran 600 Campanian Late Santonian 700 Coniacian Turonian Cenomanian Late Cretaceous 100 800 Cryogenian Albian 900 Neoproterozoic Tonian Cretaceous Aptian Early 1000 Barremian Hauterivian Valanginian 1100 Stenian Berriasian 146 Tithonian Early Cretaceous 1200 Late Kimmeridgian Oxfordian 161 Callovian Mesozoic 1300 Ectasian Bathonian Middle Bajocian Aalenian 176 1400 Toarcian Jurassic Mesoproterozoic Early Pliensbachian 1500 Sinemurian Hettangian Calymmian 200 Rhaetian 1600 Proterozoic Norian Late 1700 Statherian Carnian 228 1800 Ladinian Late Triassic Triassic Middle Anisian 1900 245 Olenekian Orosirian Early Induan Changhsingian 251 2000 Lopingian Wuchiapingian 260 Capitanian Guadalupian Wordian/Roadian 2100 271 Kungurian Paleoproterozoic Rhyacian Artinskian 2200 Permian Cisuralian Sakmarian Middle Permian 2300 Asselian 299 Late Gzhelian Kasimovian 2400 Siderian Middle Moscovian Penn- sylvanian Early Bashkirian -
Alphabetical List
LIST E - GEOLOGIC AGE (STRATIGRAPHIC) TERMS - ALPHABETICAL LIST Age Unit Broader Term Age Unit Broader Term Aalenian Middle Jurassic Brunhes Chron upper Quaternary Acadian Cambrian Bull Lake Glaciation upper Quaternary Acheulian Paleolithic Bunter Lower Triassic Adelaidean Proterozoic Burdigalian lower Miocene Aeronian Llandovery Calabrian lower Pleistocene Aftonian lower Pleistocene Callovian Middle Jurassic Akchagylian upper Pliocene Calymmian Mesoproterozoic Albian Lower Cretaceous Cambrian Paleozoic Aldanian Lower Cambrian Campanian Upper Cretaceous Alexandrian Lower Silurian Capitanian Guadalupian Algonkian Proterozoic Caradocian Upper Ordovician Allerod upper Weichselian Carboniferous Paleozoic Altonian lower Miocene Carixian Lower Jurassic Ancylus Lake lower Holocene Carnian Upper Triassic Anglian Quaternary Carpentarian Paleoproterozoic Anisian Middle Triassic Castlecliffian Pleistocene Aphebian Paleoproterozoic Cayugan Upper Silurian Aptian Lower Cretaceous Cenomanian Upper Cretaceous Aquitanian lower Miocene *Cenozoic Aragonian Miocene Central Polish Glaciation Pleistocene Archean Precambrian Chadronian upper Eocene Arenigian Lower Ordovician Chalcolithic Cenozoic Argovian Upper Jurassic Champlainian Middle Ordovician Arikareean Tertiary Changhsingian Lopingian Ariyalur Stage Upper Cretaceous Chattian upper Oligocene Artinskian Cisuralian Chazyan Middle Ordovician Asbian Lower Carboniferous Chesterian Upper Mississippian Ashgillian Upper Ordovician Cimmerian Pliocene Asselian Cisuralian Cincinnatian Upper Ordovician Astian upper -
GSSP) for Base of the Permian System
11 by Vladimir I. Davydov1, Brian F. Glenister2, Claude Spinosa3, Scott M. Ritter4, V. V. Chernykh5, B. R. Wardlaw6, and W. S. Snyder3 Proposal of Aidaralash as Global Stratotype Section and Point (GSSP) for base of the Permian System 1. All Russian Geological Research Institiute (VSEGEI), St. Petersburg, Russia 2. University of Iowa 3. Permian Research Institute, Boise State University, Idaho 82735 4. Brigham Young University 5. Institute of Geology and Geochemistry, Ural Branch of Russian Academy of Sciences, Sverdlovsk, Russia 6. U.S. Geological Survey The base of the Permian System was originally defined of local letter-designated stages for the Permian are still being uti- (Murchison, 1841) in the Ural Mountains of Russia to lized (e.g. Archbold et al., 1993) despite the fact that the Urals inter- coincide with strata marking the initiation of evaporite national standard has served effectively as a Western Australian ref- deposition, now recognized as the Kungurian Stage. erence for over one-half century (e.g. Miller, 1932). Similarly, in Since that time, the base has been lowered repeatedly to China the base of the Permian became stabilized at the unconformity c c c cydcPdddddddddddddddddddddddddddddddddddddddddddddddddddddTfc yPdddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddIfc cddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddddc -
INTERNATIONAL CHRONOSTRATIGRAPHIC CHART International Commission on Stratigraphy V 2020/03
INTERNATIONAL CHRONOSTRATIGRAPHIC CHART www.stratigraphy.org International Commission on Stratigraphy v 2020/03 numerical numerical numerical numerical Series / Epoch Stage / Age Series / Epoch Stage / Age Series / Epoch Stage / Age GSSP GSSP GSSP GSSP EonothemErathem / Eon System / Era / Period age (Ma) EonothemErathem / Eon System/ Era / Period age (Ma) EonothemErathem / Eon System/ Era / Period age (Ma) Eonothem / EonErathem / Era System / Period GSSA age (Ma) present ~ 145.0 358.9 ±0.4 541.0 ±1.0 U/L Meghalayan 0.0042 Holocene M Northgrippian 0.0082 Tithonian Ediacaran L/E Greenlandian 0.0117 152.1 ±0.9 ~ 635 U/L Upper Famennian Neo- 0.129 Upper Kimmeridgian Cryogenian M Chibanian 157.3 ±1.0 Upper proterozoic ~ 720 0.774 372.2 ±1.6 Pleistocene Calabrian Oxfordian Tonian 1.80 163.5 ±1.0 Frasnian 1000 L/E Callovian Quaternary 166.1 ±1.2 Gelasian 2.58 382.7 ±1.6 Stenian Bathonian 168.3 ±1.3 Piacenzian Middle Bajocian Givetian 1200 Pliocene 3.600 170.3 ±1.4 387.7 ±0.8 Meso- Zanclean Aalenian Middle proterozoic Ectasian 5.333 174.1 ±1.0 Eifelian 1400 Messinian Jurassic 393.3 ±1.2 Calymmian 7.246 Toarcian Devonian Tortonian 182.7 ±0.7 Emsian 1600 11.63 Pliensbachian Statherian Lower 407.6 ±2.6 Serravallian 13.82 190.8 ±1.0 Lower 1800 Miocene Pragian 410.8 ±2.8 Proterozoic Neogene Sinemurian Langhian 15.97 Orosirian 199.3 ±0.3 Lochkovian Paleo- Burdigalian Hettangian proterozoic 2050 20.44 201.3 ±0.2 419.2 ±3.2 Rhyacian Aquitanian Rhaetian Pridoli 23.03 ~ 208.5 423.0 ±2.3 2300 Ludfordian 425.6 ±0.9 Siderian Mesozoic Cenozoic Chattian Ludlow -
Paleozoic–Mesozoic Eustatic Changes and Mass Extinctions: New Insights from Event Interpretation
life Article Paleozoic–Mesozoic Eustatic Changes and Mass Extinctions: New Insights from Event Interpretation Dmitry A. Ruban K.G. Razumovsky Moscow State University of Technologies and Management (the First Cossack University), Zemlyanoy Val Street 73, 109004 Moscow, Russia; [email protected] Received: 2 November 2020; Accepted: 13 November 2020; Published: 14 November 2020 Abstract: Recent eustatic reconstructions allow for reconsidering the relationships between the fifteen Paleozoic–Mesozoic mass extinctions (mid-Cambrian, end-Ordovician, Llandovery/Wenlock, Late Devonian, Devonian/Carboniferous, mid-Carboniferous, end-Guadalupian, end-Permian, two mid-Triassic, end-Triassic, Early Jurassic, Jurassic/Cretaceous, Late Cretaceous, and end-Cretaceous extinctions) and global sea-level changes. The relationships between eustatic rises/falls and period-long eustatic trends are examined. Many eustatic events at the mass extinction intervals were not anomalous. Nonetheless, the majority of the considered mass extinctions coincided with either interruptions or changes in the ongoing eustatic trends. It cannot be excluded that such interruptions and changes could have facilitated or even triggered biodiversity losses in the marine realm. Keywords: biotic crisis; global sea level; life evolution 1. Introduction During the whole Phanerozoic, mass extinctions stressed the marine biota many times. They triggered disappearances of numerous species, genera, families, and even high-order groups of marine organisms, and they were often associated with outstanding environmental catastrophes such as global events of anoxia and euxinia, unusual warming and planetary-scale glaciations, massive volcanism, and extraterrestrial impacts. Mass extinctions were highly complex events, with the intensity amplified by the interplay among atmosphere, oceans, geologic activity, and extraterrestrial influences. The relevant knowledge is huge, and it continues to grow. -
Time-Calibrated Milankovitch Cycles for the Late Permian
ARTICLE Received 31 Oct 2012 | Accepted 16 Aug 2013 | Published 13 Sep 2013 DOI: 10.1038/ncomms3452 OPEN Time-calibrated Milankovitch cycles for the late Permian Huaichun Wu1,2, Shihong Zhang1, Linda A. Hinnov3, Ganqing Jiang4, Qinglai Feng5, Haiyan Li1 & Tianshui Yang1 An important innovation in the geosciences is the astronomical time scale. The astronomical time scale is based on the Milankovitch-forced stratigraphy that has been calibrated to astronomical models of paleoclimate forcing; it is defined for much of Cenozoic–Mesozoic. For the Palaeozoic era, however, astronomical forcing has not been widely explored because of lack of high-precision geochronology or astronomical modelling. Here we report Milankovitch cycles from late Permian (Lopingian) strata at Meishan and Shangsi, South China, time calibrated by recent high-precision U–Pb dating. The evidence extends empirical knowledge of Earth’s astronomical parameters before 250 million years ago. Observed obliquity and precession terms support a 22-h length-of-day. The reconstructed astronomical time scale indicates a 7.793-million year duration for the Lopingian epoch, when strong 405-kyr cycles constrain astronomical modelling. This is the first significant advance in defining the Palaeozoic astronomical time scale, anchored to absolute time, bridging the Palaeozoic–Mesozoic transition. 1 State Key Laboratory of Biogeology and Environmental Geology, China University of Geosciences, Beijing 100083, China. 2 School of Ocean Sciences, China University of Geosciences, Beijing 100083, China. 3 Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, Maryland 21218, USA. 4 Department of Geoscience, University of Nevada, Las Vegas, Nevada 89154, USA. 5 State Key Laboratory of Geological Processes and Mineral Resources, China University of Geosciences, Wuhan 430074, China. -
Thresholds of Temperature Change for Mass Extinctions ✉ Haijun Song 1 , David B
ARTICLE https://doi.org/10.1038/s41467-021-25019-2 OPEN Thresholds of temperature change for mass extinctions ✉ Haijun Song 1 , David B. Kemp1, Li Tian 1, Daoliang Chu 1, Huyue Song1 & Xu Dai1 Climate change is a critical factor affecting biodiversity. However, the quantitative relation- ship between temperature change and extinction is unclear. Here, we analyze magnitudes and rates of temperature change and extinction rates of marine fossils through the past 450 1234567890():,; million years (Myr). The results show that both the rate and magnitude of temperature change are significantly positively correlated with the extinction rate of marine animals. Major mass extinctions in the Phanerozoic can be linked to thresholds in climate change (warming or cooling) that equate to magnitudes >5.2 °C and rates >10 °C/Myr. The sig- nificant relationship between temperature change and extinction still exists when we exclude the five largest mass extinctions of the Phanerozoic. Our findings predict that a temperature increase of 5.2 °C above the pre-industrial level at present rates of increase would likely result in mass extinction comparable to that of the major Phanerozoic events, even without other, non-climatic anthropogenic impacts. 1 State Key Laboratory of Biogeology and Environmental Geology, School of Earth Sciences, China University of Geosciences, Wuhan, China. ✉ email: [email protected] NATURE COMMUNICATIONS | (2021) 12:4694 | https://doi.org/10.1038/s41467-021-25019-2 | www.nature.com/naturecommunications 1 ARTICLE NATURE COMMUNICATIONS | https://doi.org/10.1038/s41467-021-25019-2 ive large-magnitude mass extinctions (the “Big Five”) have rate (n = 45, ρ = 0.59, P < 0.001 for ΔT, n = 45, ρ = 0.54, P < Foccurred during the past 450 million years (Myr)1, where 0.001 for R) (Supplementary Table 1), thus providing parallel the estimated extinction of marine animals for each event supporting evidence that the magnitude and rate of climate was over 75% at the species level2.