Boring Billion Earth's
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Integrative and Comparative Biology Integrative and Comparative Biology, Volume 58, Number 4, Pp
Integrative and Comparative Biology Integrative and Comparative Biology, volume 58, number 4, pp. 605–622 doi:10.1093/icb/icy088 Society for Integrative and Comparative Biology SYMPOSIUM INTRODUCTION The Temporal and Environmental Context of Early Animal Evolution: Considering All the Ingredients of an “Explosion” Downloaded from https://academic.oup.com/icb/article-abstract/58/4/605/5056706 by Stanford Medical Center user on 15 October 2018 Erik A. Sperling1 and Richard G. Stockey Department of Geological Sciences, Stanford University, 450 Serra Mall, Building 320, Stanford, CA 94305, USA From the symposium “From Small and Squishy to Big and Armored: Genomic, Ecological and Paleontological Insights into the Early Evolution of Animals” presented at the annual meeting of the Society for Integrative and Comparative Biology, January 3–7, 2018 at San Francisco, California. 1E-mail: [email protected] Synopsis Animals originated and evolved during a unique time in Earth history—the Neoproterozoic Era. This paper aims to discuss (1) when landmark events in early animal evolution occurred, and (2) the environmental context of these evolutionary milestones, and how such factors may have affected ecosystems and body plans. With respect to timing, molecular clock studies—utilizing a diversity of methodologies—agree that animal multicellularity had arisen by 800 million years ago (Ma) (Tonian period), the bilaterian body plan by 650 Ma (Cryogenian), and divergences between sister phyla occurred 560–540 Ma (late Ediacaran). Most purported Tonian and Cryogenian animal body fossils are unlikely to be correctly identified, but independent support for the presence of pre-Ediacaran animals is recorded by organic geochemical biomarkers produced by demosponges. -
Download Download
Dorjnamjaa et al. Mongolian Geoscientist 49 (2019) 41-49 https://doi.org/10.5564/mgs.v0i49.1226 Mongolian Geoscientist Review paper New scientific direction of the bacterial paleontology in Mongolia: an essence of investigation * Dorj Dorjnamjaa , Gundsambuu Altanshagai, Batkhuyag Enkhbaatar Department of Paleontology, Institute of Paleontology, Mongolian Academy of Sciences, Ulaanbaatar 15160, Mongolia *Corresponding author. Email: [email protected] ARTICLE INFO ABSTRACT Article history: We review the initial development of Bacterial Paleontology in Mongolia and Received 10 September 2019 present some electron microscopic images of fossil bacteria in different stages of Accepted 9 October 2019 preservation in sedimentary rocks. Indeed bacterial paleontology is one the youngest branches of paleontology. It has began in the end of 20th century and has developed rapidly in recent years. The main tasks of bacterial paleontology are detailed investigation of fossil microorganisms, in particular their morphology and sizes, conditions of burial and products of habitation that are reflected in lithological and geochemical features of rocks. Bacterial paleontology deals with fossil materials and is useful in analysis of the genesis of sedimentary rocks, and sedimentary mineral resources including oil and gas. The traditional paleontology is especially significant for evolution theory, biostratigraphy, biogeography and paleoecology; however bacterial paleontology is an essential first of all for sedimentology and for theories sedimentary ore genesis or biometallogeny Keywords: microfossils, phosphorite, sedimentary rocks, lagerstatten, biometallogeny INTRODUCTION all the microorganisms had lived and propagated Bacteria or microbes preserved well as fossils in without breakdowns. Bacterial paleontological various rocks, especially in sedimentary rocks data accompanied by the data on the first origin alike natural substances. -
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. -
Gawler Craton: Half a Billion Years Older Than Previously Thought!
ISSUE 92 Dec 2008 Foundations of South Australia discovered Gawler Craton: half a billion years older than previously thought! Geoff Fraser, Chris Foudoulis, Narelle Neumann, Keith Sircombe (Geoscience Australia) Stacey McAvaney, Anthony Reid, Michael Szpunar (Primary Industries and Resources South Australia) Recent geochronology results obtained using Geoscience Australia’s a billion years older than the Sensitive High Resolution Ion Microprobe (SHRIMP) have identified oldest previously-dated rock from Mesoarchean rocks (about 3150 million years old) in the eastern South Australia, making these Gawler Craton, South Australia. These rocks are approximately half the oldest rocks yet discovered in 136° 137° Australia outside the Pilbara and Port Augusta Yilgarn Craton areas of Western 08GA-G01 Australia. A series of seismic transects are being collected across selected regions of the Australian 33° See Inset below Whyalla continent as part of Geoscience Kimba Australia’s Onshore Energy SOUTH Security Program. One of these AUSTRALIA seismic transects, collected in June 2008, traverses the northern Cowell Eyre Peninsula of South Australia Iron Monarch (figure 1). When processed, the seismic data will provide an east– 23 Mile Wallaroo west cross-section of the eastern 34° margin of the Gawler Craton. Spencer Moonta Gulf This region hosts significant CUMMINS uranium, geothermal, copper- Iron Baron/ TUMBY BAY Iron Prince gold, gold and iron resources. Maitland To assist the interpretation of 08-3449-1 0 50 km the seismic data and the current geological mapping program of Mesoarchean granite NT QLD Primary Industries and Resources WA Seismic survey route SA Road South Australia, a program of NSW VIC Railway geochronology is underway to Mineral occurence TAS Town/locality determine the ages of major rock units crossed by the seismic line. -
Trace Fossils and Substrates of the Terminal Proterozoic–Cambrian Transition: Implications for the Record of Early Bilaterians and Sediment Mixing
Trace fossils and substrates of the terminal Proterozoic–Cambrian transition: Implications for the record of early bilaterians and sediment mixing Mary L. Droser*†,So¨ ren Jensen*, and James G. Gehling‡ *Department of Earth Sciences, University of California, Riverside, CA 92521; and ‡South Australian Museum, Division of Natural Sciences, North Terrace, Adelaide 5000, South Australia, Australia Edited by James W. Valentine, University of California, Berkeley, CA, and approved August 16, 2002 (received for review May 29, 2002) The trace fossil record is important in determining the timing of the appearance of bilaterian animals. A conservative estimate puts this time at Ϸ555 million years ago. The preservational potential of traces made close to the sediment–water interface is crucial to detecting early benthic activity. Our studies on earliest Cambrian sediments suggest that shallow tiers were preserved to a greater extent than typical for most of the Phanerozoic, which can be attributed both directly and indirectly to the low levels of sediment mixing. The low levels of sediment mixing meant that thin event beds were preserved. The shallow depth of sediment mixing also meant that muddy sediments were firm close to the sediment–water interface, increasing the likelihood of recording shallow-tier trace fossils in muddy sed- iments. Overall, trace fossils can provide a sound record of the onset of bilaterian benthic activity. he appearance and subsequent diversification of bilaterian Tanimals is a topic of current controversy (refs. 1–7; Fig. 1). Three principal sources of evidence exist: body fossils, trace fossils (trails, tracks, and burrows of animal activity recorded in the sedimentary record), and divergence times calculated by means of a molecular ‘‘clock.’’ The body fossil record indicates a geologically rapid diversification of bilaterian animals not much earlier than the Precambrian–Cambrian boundary, the so-called Cambrian explosion. -
“Modern-Type Plate Tectonics”?
SILEIR RA A D B E E G D E A O D L Special Session, “A tribute to Edilton Santos, a leader in Precambrian O E I G C I A Geology in Northeastern Brazil”, edited by A.N. Sial and V.P. Ferreira O BJGEO S DOI: 10.1590/2317-4889202020190095 Brazilian Journal of Geology D ESDE 1946 Dawn of metazoans: to what extent was this influenced by the onset of “modern-type plate tectonics”? Umberto G. Cordani1* , Thomas R. Fairchild1 , Carlos E. Ganade1 , Marly Babinski1 , Juliana de Moraes Leme1 Abstract The appearance of complex megascopic multicellular eukaryotes in the Ediacaran occurred just when the dynamics of a cooling Earth allowed establishment of a new style of global tectonics that continues to the present as “modern-type plate tectonics”. The advent of this style was first registered in 620 Ma-old coesite-bearing Ultra-High Pressure eclogites within the Transbrasiliano-Kandi mega-shear zone along the site of the West Gondwana Orogeny (WGO). These eclogites comprise the oldest evidence of slab-pull deep subduction capable of inducing con- tinental collisions and producing high-relief Himalayan-type mega-mountains. Life, prior to this time, was essentially microscopic. Yet with increasing Neoproterozoic oxygenation and intensified influx of nutrients to Ediacaran oceans, resulting from the erosion of these mountains, complex macroscopic heterotrophic eukaryotes arose and diversified, taking the biosphere to a new evolutionary threshold. The repeated elevation of Himalayan-type mega-mountains ever since then has continued to play a fundamental role in nutrient supply and biosphere evolution. Other authors have alluded to the influence of Gondwana mountain-building upon Ediacaran evolution, however we claim here to have identified when and where it began. -
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 -
Earth: Atmospheric Evolution of a Habitable Planet
Earth: Atmospheric Evolution of a Habitable Planet Stephanie L. Olson1,2*, Edward W. Schwieterman1,2, Christopher T. Reinhard1,3, Timothy W. Lyons1,2 1NASA Astrobiology Institute Alternative Earth’s Team 2Department of Earth Sciences, University of California, Riverside 3School of Earth and Atmospheric Science, Georgia Institute of Technology *Correspondence: [email protected] Table of Contents 1. Introduction ............................................................................................................................ 2 2. Oxygen and biological innovation .................................................................................... 3 2.1. Oxygenic photosynthesis on the early Earth .......................................................... 4 2.2. The Great Oxidation Event ......................................................................................... 6 2.3. Oxygen during Earth’s middle chapter ..................................................................... 7 2.4. Neoproterozoic oxygen dynamics and the rise of animals .................................. 9 2.5. Continued oxygen evolution in the Phanerozoic.................................................. 11 3. Carbon dioxide, climate regulation, and enduring habitability ................................. 12 3.1. The faint young Sun paradox ................................................................................... 12 3.2. The silicate weathering thermostat ......................................................................... 12 3.3. Geological -
38—GEOLOGIC AGE SYMBOL FONT (Stratagemage) REF NO STRATIGRAPHIC AGE SUBDIVISION TYPE AGE SYMBOL KEYBOARD POSITION for Stratagemage FONT
Federal Geographic Data Committee U.S. Geological Survey Open-File Report 99–430 Public Review Draft - Digital Cartographic Standard for Geologic Map Symbolization PostScript Implementation (filename: of99-430_38-01.eps) 38—GEOLOGIC AGE SYMBOL FONT (StratagemAge) REF NO STRATIGRAPHIC AGE SUBDIVISION TYPE AGE SYMBOL KEYBOARD POSITION FOR StratagemAge FONT 38.1 Archean Eon A Not applicable (use Helvetica instead) 38.2 Cambrian Period _ (underscore = shift-hyphen) 38.3 Carboniferous Period C Not applicable (use Helvetica instead) 38.4 Cenozoic Era { (left curly bracket = shift-left square bracket) 38.5 Cretaceous Period K Not applicable (use Helvetica instead) 38.6 Devonian Period D Not applicable (use Helvetica instead) 38.7 Early Archean (3,800(?)–3,400 Ma) Era U Not applicable (use Helvetica instead) 38.8 Early Early Proterozoic (2,500–2,100 Ma) Era R (capital R = shift-r) 38.9 Early Middle Proterozoic (1,600–1,400 Ma) Era G (capital G = shift-g) 38.10 Early Proterozoic Era X Not applicable (use Helvetica instead) 38.11 Eocene Epoch # (pound sign = shift-3) 38.12 Holocene Epoch H Not applicable (use Helvetica instead) 38.13 Jurassic Period J Not applicable (use Helvetica instead) 38.14 Late Archean (3,000–2,500 Ma) Era W Not applicable (use Helvetica instead) 38.15 Late Early Proterozoic (1,800–1,600 Ma) Era I (capital I = shift-i) 38.16 Late Middle Proterozoic (1,200–900 Ma) Era E (capital E = shift-e) 38.17 Late Proterozoic Era Z Not applicable (use Helvetica instead) 38.18 Mesozoic Era } (right curly bracket = shift-right square bracket) 38.19 Middle Archean (3,400–3,000 Ma) Era V Not applicable (use Helvetica instead) 38.20 Middle Early Proterozoic (2,100–1,800 Ma) Era L (capital L = shift-l) 38.21 Middle Middle Proterozoic (1,400–1,200 Ma) Era F (capital F = shift-f) 38.22 Middle Proterozoic Era Y Not applicable (use Helvetica instead) A–38–1 Federal Geographic Data Committee U.S. -
Geologic Time Lesson Guide Lesson Guide | Description
Geologic Time Lesson Guide Lesson Guide | Description Instructor: Dr. Michael T. Lewchuk Grade Level: 6 - 12 Subject: Earth & Physical Science Students will investigate the subdivisions of the Geologic Time Scale. Wonder How: Have you ever wondered how scientists and geologists know how old something is? Goal: Students will gather data and use ratios that will help them create a scale model of Geological time using simple materials found at home. Lesson Guide | Lesson Guide Agenda Lesson Guide Agenda: v Vocabulary v Materials List v Geologic Time Scale v Activity Instructions v Challenge! v Additional Resources v Oklahoma Academic Standards Lesson Guide | Vocabulary Eon – An Eon is the fundamental division of time in Geology. The Earth’s 4.6-billion- year history is divided into four Eons: Hadean, Archean, Proterozoic and Phanerozoic. Precambrian Supereon – This is the combination of the Hadean, Archean and Proterozoic Eons. It is subdivided based on the physical properties of the Earth’s surface and atmosphere. Hadean Eon – The Hadean is the oldest Eon. It is generally described as the time when the Earth was so hot that it was all, or mostly all, molten liquid. Archean Eon – The Archean Eon is generally described as the time when solid rock existed on the surface of the Earth, but little or no free oxygen existed in the atmosphere. Proterozoic Eon – The Proterozoic is generally considered the Eon when free oxygen began to appear in the atmosphere. Microscopic life developed during the Proterozoic. Lesson Guide | Vocabulary Phanerozoic Eon – The Phanerozoic Eon is the most recent Eon in geologic history. -
Tectonics and Crustal Evolution
Tectonics and crustal evolution Chris J. Hawkesworth, Department of Earth Sciences, University peaks and troughs of ages. Much of it has focused discussion on of Bristol, Wills Memorial Building, Queens Road, Bristol BS8 1RJ, the extent to which the generation and evolution of Earth’s crust is UK; and Department of Earth Sciences, University of St. Andrews, driven by deep-seated processes, such as mantle plumes, or is North Street, St. Andrews KY16 9AL, UK, c.j.hawkesworth@bristol primarily in response to plate tectonic processes that dominate at .ac.uk; Peter A. Cawood, Department of Earth Sciences, University relatively shallow levels. of St. Andrews, North Street, St. Andrews KY16 9AL, UK; and Bruno The cyclical nature of the geological record has been recog- Dhuime, Department of Earth Sciences, University of Bristol, Wills nized since James Hutton noted in the eighteenth century that Memorial Building, Queens Road, Bristol BS8 1RJ, UK even the oldest rocks are made up of “materials furnished from the ruins of former continents” (Hutton, 1785). The history of ABSTRACT the continental crust, at least since the end of the Archean, is marked by geological cycles that on different scales include those The continental crust is the archive of Earth’s history. Its rock shaped by individual mountain building events, and by the units record events that are heterogeneous in time with distinctive cyclic development and dispersal of supercontinents in response peaks and troughs of ages for igneous crystallization, metamor- to plate tectonics (Nance et al., 2014, and references therein). phism, continental margins, and mineralization. This temporal Successive cycles may have different features, reflecting in part distribution is argued largely to reflect the different preservation the cooling of the earth and the changing nature of the litho- potential of rocks generated in different tectonic settings, rather sphere. -
Proterozoic Ocean Chemistry and Evolution: a Bioinorganic Bridge? A
S CIENCE’ S C OMPASS ● REVIEW REVIEW: GEOCHEMISTRY Proterozoic Ocean Chemistry and Evolution: A Bioinorganic Bridge? A. D. Anbar1* and A. H. Knoll2 contrast, weathering under a moderately oxidiz- Recent data imply that for much of the Proterozoic Eon (2500 to 543 million years ing mid-Proterozoic atmosphere would have 2– ago), Earth’s oceans were moderately oxic at the surface and sulfidic at depth. Under enhanced the delivery of SO4 to the anoxic these conditions, biologically important trace metals would have been scarce in most depths. Assuming biologically productive marine environments, potentially restricting the nitrogen cycle, affecting primary oceans, the result would have been higher H2S productivity, and limiting the ecological distribution of eukaryotic algae. Oceanic concentrations during this period than either redox conditions and their bioinorganic consequences may thus help to explain before or since (8). observed patterns of Proterozoic evolution. Is there any evidence for such a world? Canfield and his colleagues have developed an argument based on the S isotopic compo- n the present-day Earth, O2 is abun- es and forms insoluble Fe-oxyhydroxides, sition of biogenic sedimentary sulfides, 2– dant from the upper atmosphere to thus removing Fe and precluding BIF forma- which reflect SO4 availability and redox the bottoms of ocean basins. When tion. This reading of the stratigraphic record conditions at their time of formation (16–18). O 2– life began, however, O2 was at best a trace made sense because independent geochemi- When the availability of SO4 is strongly 2– Ͻϳ constituent of the surface environment. The cal evidence indicates that the partial pressure limited (SO4 concentration 1 mM, ϳ intervening history of ocean redox has been of atmospheric oxygen (PO2) rose substan- 4% of that in present-day seawater), H2S interpreted in terms of two long-lasting tially about 2400 to 2000 Ma (4–7).