Anatomical and Ecological Constraints on Phanerozoic Animal Diversity in the Marine Realm
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Early Sponge Evolution: a Review and Phylogenetic Framework
Available online at www.sciencedirect.com ScienceDirect Palaeoworld 27 (2018) 1–29 Review Early sponge evolution: A review and phylogenetic framework a,b,∗ a Joseph P. Botting , Lucy A. Muir a Nanjing Institute of Geology and Palaeontology, Chinese Academy of Sciences, 39 East Beijing Road, Nanjing 210008, China b Department of Natural Sciences, Amgueddfa Cymru — National Museum Wales, Cathays Park, Cardiff CF10 3LP, UK Received 27 January 2017; received in revised form 12 May 2017; accepted 5 July 2017 Available online 13 July 2017 Abstract Sponges are one of the critical groups in understanding the early evolution of animals. Traditional views of these relationships are currently being challenged by molecular data, but the debate has so far made little use of recent palaeontological advances that provide an independent perspective on deep sponge evolution. This review summarises the available information, particularly where the fossil record reveals extinct character combinations that directly impinge on our understanding of high-level relationships and evolutionary origins. An evolutionary outline is proposed that includes the major early fossil groups, combining the fossil record with molecular phylogenetics. The key points are as follows. (1) Crown-group sponge classes are difficult to recognise in the fossil record, with the exception of demosponges, the origins of which are now becoming clear. (2) Hexactine spicules were present in the stem lineages of Hexactinellida, Demospongiae, Silicea and probably also Calcarea and Porifera; this spicule type is not diagnostic of hexactinellids in the fossil record. (3) Reticulosans form the stem lineage of Silicea, and probably also Porifera. (4) At least some early-branching groups possessed biminerallic spicules of silica (with axial filament) combined with an outer layer of calcite secreted within an organic sheath. -
Evolutionary Patterns of Trilobites Across the End Ordovician Mass Extinction
Evolutionary Patterns of Trilobites Across the End Ordovician Mass Extinction by Curtis R. Congreve B.S., University of Rochester, 2006 M.S., University of Kansas, 2008 Submitted to the Department of Geology and the Faculty of the Graduate School of The University of Kansas in partial fulfillment on the requirements for the degree of Doctor of Philosophy 2012 Advisory Committee: ______________________________ Bruce Lieberman, Chair ______________________________ Paul Selden ______________________________ David Fowle ______________________________ Ed Wiley ______________________________ Xingong Li Defense Date: December 12, 2012 ii The Dissertation Committee for Curtis R. Congreve certifies that this is the approved Version of the following thesis: Evolutionary Patterns of Trilobites Across the End Ordovician Mass Extinction Advisory Committee: ______________________________ Bruce Lieberman, Chair ______________________________ Paul Selden ______________________________ David Fowle ______________________________ Ed Wiley ______________________________ Xingong Li Accepted: April 18, 2013 iii Abstract: The end Ordovician mass extinction is the second largest extinction event in the history or life and it is classically interpreted as being caused by a sudden and unstable icehouse during otherwise greenhouse conditions. The extinction occurred in two pulses, with a brief rise of a recovery fauna (Hirnantia fauna) between pulses. The extinction patterns of trilobites are studied in this thesis in order to better understand selectivity of the -
Geologic Time Scale Cards
PreCambrian SuperEon (4.6 BYA – 541 MYA) Hadean Eon (4.6 BYA - 4 BYA) Slide # 1 46 feet Earth Forms • Earth is formed from a mass of dust and gas that gravity pulled together. • The process causes a huge amount of radioactive decay and Earth is a boiling ball of lava. • At 4.5 BYA a protoplanet named Theia collides with Earth and a debris ring forms which later becomes our moon. • Earth cools and forms the layers – core, mantel, and outer crust. • Meteors bombard earth bringing frozen droplets of water that later become our oceans. • Volcanic activity continues and Earth’s earliest continental crust forms before 4.03 BYA. The Acasta gneiss is one of the oldest rocks on Earth dating 4.03 billion years.. PreCambrian SuperEon (4.6 BYA – 541 MYA) Archaean Eon (4 BYA – 2.5 BYA) Slide # 2 40 feet Primitive, Simple Life Forms • Earth’s crust cools and plate tectonics forms. • Ancient rock formations form from 4 to 2.5 BYA. • The Primordial soup theory suggests early minerals and compounds from meteors made the perfect recipe for primitive, simple life to form at the thermal vents of the ocean. • Single cell life formed the ocean and over time stromatolites, photosynthesizing colonial bacteria, formed in shallow water and released oxygen. • The oxygen attached to trace iron in the oceans and formed sedimentary layers of banded iron formations (BIFS) that are presently mined for iron ore. Banded iron formations from the late Archaean and early Proterozoic eons Stromatolite fossil image PreCambrian SuperEon (4.6 BYA – 541 MYA) Proterozoic Eon (2.5 BYA – 541 MYA) Slide # 3 25 feet Early life • Photosynthesizing life further establishes and releases oxygen throughout the ocean. -
Church 18.Pdf (1.785Mb)
Paleontological Contributions Number 18 Efficient Ornamentation in Ordovician Anthaspidellid Sponges Stephen B. Church August 9, 2017 Lawrence, Kansas, USA ISSN 1946-0279 (online) paleo.ku.edu/contributions Ridge-and-trough ornamented outer-wall fragment of the Ordovician anthaspidellid sponge Rugocoelia eganensis Johns, 1994. Paleontological Contributions August 9, 2017 Number 18 EFFICIENT ORNAMENTATION IN ORDOVICIAN ANTHASPIDELLID SPONGES Stephen B. Church Department of Geological Sciences, Brigham Young University, Provo, Utah 84602-3300, [email protected] ABSTRACT Lithistid orchoclad sponges within the family Anthaspidellidae Ulrich in Miller, 1889 include several genera that added ornate features to their outer-wall surfaces during Early Ordovician sponge radiation. Ornamented anthaspidellid sponges commonly constructed annulated or irregularly to regularly spaced transverse ridge-and-trough features on their outer-wall surfaces without proportionately increasing the size of their internal wall or gastral surfaces. This efficient technique of modi- fying only the sponge’s outer surface without enlarging its entire skeletal frame conserved the sponge’s constructional energy while increasing outer-wall surface-to-fluid exposure for greater intake of nutrient bearing currents. Sponges with widely spaced ridge-and-trough ornament dimensions predominated in high-energy settings. Widely spaced ridges and troughs may have given the sponge hydrodynamic benefits in high wave force settings. Ornamented sponges with narrowly spaced ridge-and- trough dimensions are found in high energy paleoenvironments but also occupied moderate to low-energy settings, where their surface-to-fluid exposure per unit area exceeded that of sponges with widely spaced surface ornamentations. Keywords: lithistid sponges, Ordovician radiation, morphological variation, theoretical morphology INTRODUCTION assumed by most anthaspidellids. -
Associated Organisms Inhabiting the Calcareous Sponge Clathrina Lutea in La Parguera Natural
bioRxiv preprint doi: https://doi.org/10.1101/596429; this version posted April 3, 2019. The copyright holder for this preprint (which was not certified by peer review) is the author/funder, who has granted bioRxiv a license to display the preprint in perpetuity. It is made available under aCC-BY-NC-ND 4.0 International license. 1 Associated organisms inhabiting the calcareous sponge Clathrina lutea in La Parguera Natural 2 Reserve, Puerto Rico 3 4 Jaaziel E. García-Hernández1,2*, Nicholas M. Hammerman2,3*, Juan J. Cruz-Motta2 & Nikolaos V. 5 Schizas2 6 * These authors contributed equally 7 1University of Puerto Rico at Mayagüez, Department of Biology, PO Box 9000, Mayagüez, PR 8 00681 9 2University of Puerto Rico at Mayagüez, Department of Marine Sciences, Marine Genomic 10 Biodiversity Laboratory, PO Box 9000, Mayagüez, PR 00681 11 3School of Biological Sciences, University of Queensland, Gehrmann Laboratories, Level 8, 12 Research Road, St Lucia, QLD 4072, Australia 13 14 15 Nikolaos V. Schizas, [email protected], FAX: 787-899-5500 16 17 Running Head: Infauna of the calcareous sponge Clathrina lutea 18 19 20 1 bioRxiv preprint doi: https://doi.org/10.1101/596429; this version posted April 3, 2019. The copyright holder for this preprint (which was not certified by peer review) is the author/funder, who has granted bioRxiv a license to display the preprint in perpetuity. It is made available under aCC-BY-NC-ND 4.0 International license. 21 ABSTRACT 22 Sponges provide an array of ecological services and benefits for Caribbean coral reefs. They 23 function as habitats for a bewildering variety of species, however limited attention has been paid 24 in the systematics and distribution of sponge-associated fauna in the class Calcarea or for that 25 matter of sponges in the Caribbean. -
MARINE FAUNA and FLORA of BERMUDA a Systematic Guide to the Identification of Marine Organisms
MARINE FAUNA AND FLORA OF BERMUDA A Systematic Guide to the Identification of Marine Organisms Edited by WOLFGANG STERRER Bermuda Biological Station St. George's, Bermuda in cooperation with Christiane Schoepfer-Sterrer and 63 text contributors A Wiley-Interscience Publication JOHN WILEY & SONS New York Chichester Brisbane Toronto Singapore ANTHOZOA 159 sucker) on the exumbrella. Color vari many Actiniaria and Ceriantharia can able, mostly greenish gray-blue, the move if exposed to unfavorable condi greenish color due to zooxanthellae tions. Actiniaria can creep along on their embedded in the mesoglea. Polyp pedal discs at 8-10 cm/hr, pull themselves slender; strobilation of the monodisc by their tentacles, move by peristalsis type. Medusae are found, upside through loose sediment, float in currents, down and usually in large congrega and even swim by coordinated tentacular tions, on the muddy bottoms of in motion. shore bays and ponds. Both subclasses are represented in Ber W. STERRER muda. Because the orders are so diverse morphologically, they are often discussed separately. In some classifications the an Class Anthozoa (Corals, anemones) thozoan orders are grouped into 3 (not the 2 considered here) subclasses, splitting off CHARACTERISTICS: Exclusively polypoid, sol the Ceriantharia and Antipatharia into a itary or colonial eNIDARIA. Oral end ex separate subclass, the Ceriantipatharia. panded into oral disc which bears the mouth and Corallimorpharia are sometimes consid one or more rings of hollow tentacles. ered a suborder of Scleractinia. Approxi Stomodeum well developed, often with 1 or 2 mately 6,500 species of Anthozoa are siphonoglyphs. Gastrovascular cavity compart known. Of 93 species reported from Ber mentalized by radially arranged mesenteries. -
End-Permian Mass Extinction in the Oceans: an Ancient Analog for the Twenty-First Century?
EA40CH05-Payne ARI 23 March 2012 10:24 End-Permian Mass Extinction in the Oceans: An Ancient Analog for the Twenty-First Century? Jonathan L. Payne1 and Matthew E. Clapham2 1Department of Geological and Environmental Sciences, Stanford University, Stanford, California 94305; email: [email protected] 2Department of Earth and Planetary Sciences, University of California, Santa Cruz, California 95064; email: [email protected] Annu. Rev. Earth Planet. Sci. 2012. 40:89–111 Keywords First published online as a Review in Advance on ocean acidification, evolution, isotope geochemistry, volcanism, January 3, 2012 biodiversity The Annual Review of Earth and Planetary Sciences is online at earth.annualreviews.org Abstract This article’s doi: The greatest loss of biodiversity in the history of animal life occurred at the 10.1146/annurev-earth-042711-105329 end of the Permian Period (∼252 million years ago). This biotic catastro- Annu. Rev. Earth Planet. Sci. 2012.40:89-111. Downloaded from www.annualreviews.org Copyright c 2012 by Annual Reviews. phe coincided with an interval of widespread ocean anoxia and the eruption All rights reserved of one of Earth’s largest continental flood basalt provinces, the Siberian by Stanford University - Main Campus Robert Crown Law Library on 06/04/12. For personal use only. 0084-6597/12/0530-0089$20.00 Traps. Volatile release from basaltic magma and sedimentary strata dur- ing emplacement of the Siberian Traps can account for most end-Permian paleontological and geochemical observations. Climate change and, per- haps, destruction of the ozone layer can explain extinctions on land, whereas changes in ocean oxygen levels, CO2, pH, and temperature can account for extinction selectivity across marine animals. -
PERMIAN BASIN PROVINCE (044) by Mahlon M
PERMIAN BASIN PROVINCE (044) By Mahlon M. Ball INTRODUCTION The Permian Basin is one of the largest structural basins in North America. It encompasses a surface area in excess of 86,000 sq mi and includes all or parts of 52 counties located in West Texas and southeast New Mexico. Structurally, the Permian Basin is bounded on the south by the Marathon-Ouachita Fold Belt, on the west by the Diablo Platform and Pedernal Uplift, on the north by the Matador Arch, and on the east by the Eastern Shelf of the Permian (Midland) Basin and west flank of the Bend Arch. The basin is about 260 mi by 300 mi in area and is separated into eastern and western halves by a north-south trending Central Basin Platform. In cross section, the basin is an asymmetrical feature; the western half contains a thicker and more structurally deformed sequence of sedimentary rock. The Permian Basin has been characterized as a large structural depression formed as a result of downwarp in the Precambrian basement surface located at the southern margin of the North American craton. The basin was filled with Paleozoic and, to a much lesser extent, younger sediments. It acquired its present structural form by Early Permian time. The overall basin is divisible into several distinct structural and tectonic elements. They are the Central Basin Platform and the Ozona Arch, which separate the Delaware and Val Verde Basins on the south and west from the Midland Basin on the north and east, the Northwestern Shelf on the southern extremity of the Pedernal Uplift and Matador Arch, and the Eastern Shelf on the western periphery of the Bend Arch. -
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. -
The Parallels Between the End-Permian Mass Extinction And
Drawing Connections: The Parallels Between the End-Permian Mass Extinction and Current Climate Change An undergraduate of East Tennessee State University explains that humans’ current effects on the biosphere are disturbingly similar to the circumstances that caused the worst mass extinction in biologic history. By: Amber Rookstool 6 December 2016 About the Author: Amber Rookstool is an undergraduate student at East Tennessee State University. She is currently an English major and dreams of becoming an author and high school English Teacher. She hopes to publish her first book by the time she is 26 years old. Table of Contents Introduction .................................................................................................................................1 Brief Geologic Timeline ...........................................................................................................2 The Anthropocene ......................................................................................................................3 Biodiversity Crisis ....................................................................................................................3 Habitat Loss .........................................................................................................................3 Invasive Species ..................................................................................................................4 Overexploitation ...................................................................................................................4 -
Lee-Riding-2018.Pdf
Earth-Science Reviews 181 (2018) 98–121 Contents lists available at ScienceDirect Earth-Science Reviews journal homepage: www.elsevier.com/locate/earscirev Marine oxygenation, lithistid sponges, and the early history of Paleozoic T skeletal reefs ⁎ Jeong-Hyun Leea, , Robert Ridingb a Department of Geology and Earth Environmental Sciences, Chungnam National University, Daejeon 34134, Republic of Korea b Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996, USA ARTICLE INFO ABSTRACT Keywords: Microbial carbonates were major components of early Paleozoic reefs until coral-stromatoporoid-bryozoan reefs Cambrian appeared in the mid-Ordovician. Microbial reefs were augmented by archaeocyath sponges for ~15 Myr in the Reef gap early Cambrian, by lithistid sponges for the remaining ~25 Myr of the Cambrian, and then by lithistid, calathiid Dysoxia and pulchrilaminid sponges for the first ~25 Myr of the Ordovician. The factors responsible for mid–late Hypoxia Cambrian microbial-lithistid sponge reef dominance remain unclear. Although oxygen increase appears to have Lithistid sponge-microbial reef significantly contributed to the early Cambrian ‘Explosion’ of marine animal life, it was followed by a prolonged period dominated by ‘greenhouse’ conditions, as sea-level rose and CO2 increased. The mid–late Cambrian was unusually warm, and these elevated temperatures can be expected to have lowered oxygen solubility, and to have promoted widespread thermal stratification resulting in marine dysoxia and hypoxia. Greenhouse condi- tions would also have stimulated carbonate platform development, locally further limiting shallow-water cir- culation. Low marine oxygenation has been linked to episodic extinctions of phytoplankton, trilobites and other metazoans during the mid–late Cambrian. -
(Anthozoa) from the Lower Oligocene (Rupelian) of the Eastern Alps, Austria
TO L O N O G E I L C A A P I ' T A A T L E I I A Bollettino della Società Paleontologica Italiana, 59 (3), 2020, 319-336. Modena C N O A S S. P. I. Scleractinian corals (Anthozoa) from the lower Oligocene (Rupelian) of the Eastern Alps, Austria Rosemarie Christine Baron-Szabo* & Diethard Sanders R.C. Baron-Szabo, Department of Invertebrate Zoology, Smithsonian Institution, NMNH, W-205, MRC 163, P.O. Box 37012, Washington DC, 20013- 7012 USA; Forschungsinstitut Senckenberg, Senckenberganlage 25, D-60325 Frankfurt/Main, Germany; [email protected]; Rosemarie.Baron- [email protected] *corresponding author D. Sanders, Institut für Geologie, Universität of Innsbruck, Innrain 52, A-6020 Innsbruck, Austria; [email protected] KEY WORDS - Scleractinia, taxonomy, paleoecology, paleobiogeography. ABSTRACT - In the Werlberg Member (Rupelian pro parte) of the Paisslberg Formation (Eastern Alps), an assemblage of colonial corals of eleven species pertaining to eleven genera and eleven families was identified:Stylocoenia carryensis, Acropora lavandulina, ?Colpophyllia sp., Dendrogyra intermedia, Caulastraea pseudoflabellum, Hydnophyllia costata, Pindosmilia cf. brunni, Actinacis rollei, Pavona profunda, Agathiphyllia gregaria, and Faksephyllia faxoensis. This is the first Oligocene coral assemblage reported from the Paisslberg Formation (Werlberg Member) of the Eastern Alps, consisting exclusively of colonial forms. The assemblage represents the northernmost fauna of reefal corals reported to date for Rupelian time. The Werlberg Member accumulated during marine transgression onto a truncated succession of older carbonate rocks. The corals grew as isolated colonies and in carpets in a protected shoreface setting punctuated by high-energy events. Coral growth forms comprise massive to sublamellar forms, and branched (dendroid, ramose) forms.