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Cryogenian Glaciation and the Onset of Carbon-Isotope Decoupling” by N
CORRECTED 21 MAY 2010; SEE LAST PAGE REPORTS 13. J. Helbert, A. Maturilli, N. Mueller, in Venus Eds. (U.S. Geological Society Open-File Report 2005- M. F. Coffin, Eds. (Monograph 100, American Geophysical Geochemistry: Progress, Prospects, and New Missions 1271, Abstracts of the Annual Meeting of Planetary Union, Washington, DC, 1997), pp. 1–28. (Lunar and Planetary Institute, Houston, TX, 2009), abstr. Geologic Mappers, Washington, DC, 2005), pp. 20–21. 44. M. A. Bullock, D. H. Grinspoon, Icarus 150, 19 (2001). 2010. 25. E. R. Stofan, S. E. Smrekar, J. Helbert, P. Martin, 45. R. G. Strom, G. G. Schaber, D. D. Dawson, J. Geophys. 14. J. Helbert, A. Maturilli, Earth Planet. Sci. Lett. 285, 347 N. Mueller, Lunar Planet. Sci. XXXIX, abstr. 1033 Res. 99, 10,899 (1994). (2009). (2009). 46. K. M. Roberts, J. E. Guest, J. W. Head, M. G. Lancaster, 15. Coronae are circular volcano-tectonic features that are 26. B. D. Campbell et al., J. Geophys. Res. 97, 16,249 J. Geophys. Res. 97, 15,991 (1992). unique to Venus and have an average diameter of (1992). 47. C. R. K. Kilburn, in Encyclopedia of Volcanoes, ~250 km (5). They are defined by their circular and often 27. R. J. Phillips, N. R. Izenberg, Geophys. Res. Lett. 22, 1617 H. Sigurdsson, Ed. (Academic Press, San Diego, CA, radial fractures and always produce some form of volcanism. (1995). 2000), pp. 291–306. 16. G. E. McGill, S. J. Steenstrup, C. Barton, P. G. Ford, 28. C. M. Pieters et al., Science 234, 1379 (1986). 48. -
Assembly, Configuration, and Break-Up History of Rodinia
Author's personal copy Available online at www.sciencedirect.com Precambrian Research 160 (2008) 179–210 Assembly, configuration, and break-up history of Rodinia: A synthesis Z.X. Li a,g,∗, S.V. Bogdanova b, A.S. Collins c, A. Davidson d, B. De Waele a, R.E. Ernst e,f, I.C.W. Fitzsimons g, R.A. Fuck h, D.P. Gladkochub i, J. Jacobs j, K.E. Karlstrom k, S. Lu l, L.M. Natapov m, V. Pease n, S.A. Pisarevsky a, K. Thrane o, V. Vernikovsky p a Tectonics Special Research Centre, School of Earth and Geographical Sciences, The University of Western Australia, Crawley, WA 6009, Australia b Department of Geology, Lund University, Solvegatan 12, 223 62 Lund, Sweden c Continental Evolution Research Group, School of Earth and Environmental Sciences, University of Adelaide, Adelaide, SA 5005, Australia d Geological Survey of Canada (retired), 601 Booth Street, Ottawa, Canada K1A 0E8 e Ernst Geosciences, 43 Margrave Avenue, Ottawa, Canada K1T 3Y2 f Department of Earth Sciences, Carleton U., Ottawa, Canada K1S 5B6 g Tectonics Special Research Centre, Department of Applied Geology, Curtin University of Technology, GPO Box U1987, Perth, WA 6845, Australia h Universidade de Bras´ılia, 70910-000 Bras´ılia, Brazil i Institute of the Earth’s Crust SB RAS, Lermontova Street, 128, 664033 Irkutsk, Russia j Department of Earth Science, University of Bergen, Allegaten 41, N-5007 Bergen, Norway k Department of Earth and Planetary Sciences, Northrop Hall University of New Mexico, Albuquerque, NM 87131, USA l Tianjin Institute of Geology and Mineral Resources, CGS, No. -
Sea Level and Global Ice Volumes from the Last Glacial Maximum to the Holocene
Sea level and global ice volumes from the Last Glacial Maximum to the Holocene Kurt Lambecka,b,1, Hélène Roubya,b, Anthony Purcella, Yiying Sunc, and Malcolm Sambridgea aResearch School of Earth Sciences, The Australian National University, Canberra, ACT 0200, Australia; bLaboratoire de Géologie de l’École Normale Supérieure, UMR 8538 du CNRS, 75231 Paris, France; and cDepartment of Earth Sciences, University of Hong Kong, Hong Kong, China This contribution is part of the special series of Inaugural Articles by members of the National Academy of Sciences elected in 2009. Contributed by Kurt Lambeck, September 12, 2014 (sent for review July 1, 2014; reviewed by Edouard Bard, Jerry X. Mitrovica, and Peter U. Clark) The major cause of sea-level change during ice ages is the exchange for the Holocene for which the direct measures of past sea level are of water between ice and ocean and the planet’s dynamic response relatively abundant, for example, exhibit differences both in phase to the changing surface load. Inversion of ∼1,000 observations for and in noise characteristics between the two data [compare, for the past 35,000 y from localities far from former ice margins has example, the Holocene parts of oxygen isotope records from the provided new constraints on the fluctuation of ice volume in this Pacific (9) and from two Red Sea cores (10)]. interval. Key results are: (i) a rapid final fall in global sea level of Past sea level is measured with respect to its present position ∼40 m in <2,000 y at the onset of the glacial maximum ∼30,000 y and contains information on both land movement and changes in before present (30 ka BP); (ii) a slow fall to −134 m from 29 to 21 ka ocean volume. -
UC Riverside UC Riverside Electronic Theses and Dissertations
UC Riverside UC Riverside Electronic Theses and Dissertations Title Exploring the Texture of Ocean-Atmosphere Redox Evolution on the Early Earth Permalink https://escholarship.org/uc/item/9v96g1j5 Author Reinhard, Christopher Thomas Publication Date 2012 Peer reviewed|Thesis/dissertation eScholarship.org Powered by the California Digital Library University of California UNIVERSITY OF CALIFORNIA RIVERSIDE Exploring the Texture of Ocean-Atmosphere Redox Evolution on the Early Earth A Dissertation submitted in partial satisfaction of the requirements for the degree of Doctor of Philosophy in Geological Sciences by Christopher Thomas Reinhard September 2012 Dissertation Committee: Dr. Timothy W. Lyons, Chairperson Dr. Gordon D. Love Dr. Nigel C. Hughes ! Copyright by Christopher Thomas Reinhard 2012 ! ! The Dissertation of Christopher Thomas Reinhard is approved: ________________________________________________ ________________________________________________ ________________________________________________ Committee Chairperson University of California, Riverside ! ! ACKNOWLEDGEMENTS It goes without saying (but I’ll say it anyway…) that things like this are never done in a vacuum. Not that I’ve invented cold fusion here, but it was quite a bit of work nonetheless and to say that my zest for the enterprise waned at times would be to put it euphemistically. As it happens, though, I’ve been fortunate enough to be surrounded these last years by an incredible group of people. To those that I consider scientific and professional mentors that have kept me interested, grounded, and challenged – most notably Tim Lyons, Rob Raiswell, Gordon Love, and Nigel Hughes – thank you for all that you do. I also owe Nigel and Mary Droser a particular debt of graditude for letting me flounder a bit my first year at UCR, being understanding and supportive, and encouraging me to start down the road to where I’ve ended up (for better or worse). -
Cretaceous Paleoceanography
GEOLOGIC A CARPATH1CA, 46, 5, BRATISLAVA, OCTOBER 1995 257 - 266 CRETACEOUS PALEOCEANOGRAPHY A v Z XI06ER WILLIAM W. HAY BORE* CRETACEOUS GEOMAR, Wischhofstr. 1-3, D-24148 Kiel, Germany Department of Geological Sciences and Cooperative Institute for Research in Environmental Sciences, Campus Box 250, University of Colorado, Boulder, CO 80309, USA (Manuscript received January 17, 1995; accepted in revised form June 14, 1995) Abstract: The modem ocean is comprised of four units: an equatorial belt shared by the two hemispheres, tropical-subtropi cal anticyclonic gyres, mid-latitude belts of water with steep meridional temperature gradients, and polar oceans characterized by cyclonic gyres. These units are separated by lines of convergence, or fronts: subequatorial, subtropical, and polar. Con vergence and divergence of the ocean waters are forced beneath zonal (latitude-parallel) winds. The Early Cretaceous ocean closely resembled the modem ocean. The developing Atlantic was analogous to the modem Mediterranean and served as an Intermediate Water source for the Pacific. Because sea-ice formed seasonally in the Early Cretaceous polar seas, deep water formation probably took place largely in the polar region. In the Late Cretaceous, the high latitudes were warm and deep waters moved from the equatorial region toward the poles, enhancing the ocean’s capacity to transport heat poleward. The contrast between surface gyre waters and intermediate waters was less, making them easier to upwell, but be cause their residence time in the oxygen minimum was less and they contained less nutrients. By analogy to the modem ocean, ’’Tethyan” refers to the oceans between the subtropical convergences and ’’Boreal” refers to the ocean poleward of the subtropical convergences. -
The History of Ice on Earth by Michael Marshall
The history of ice on Earth By Michael Marshall Primitive humans, clad in animal skins, trekking across vast expanses of ice in a desperate search to find food. That’s the image that comes to mind when most of us think about an ice age. But in fact there have been many ice ages, most of them long before humans made their first appearance. And the familiar picture of an ice age is of a comparatively mild one: others were so severe that the entire Earth froze over, for tens or even hundreds of millions of years. In fact, the planet seems to have three main settings: “greenhouse”, when tropical temperatures extend to the polesand there are no ice sheets at all; “icehouse”, when there is some permanent ice, although its extent varies greatly; and “snowball”, in which the planet’s entire surface is frozen over. Why the ice periodically advances – and why it retreats again – is a mystery that glaciologists have only just started to unravel. Here’s our recap of all the back and forth they’re trying to explain. Snowball Earth 2.4 to 2.1 billion years ago The Huronian glaciation is the oldest ice age we know about. The Earth was just over 2 billion years old, and home only to unicellular life-forms. The early stages of the Huronian, from 2.4 to 2.3 billion years ago, seem to have been particularly severe, with the entire planet frozen over in the first “snowball Earth”. This may have been triggered by a 250-million-year lull in volcanic activity, which would have meant less carbon dioxide being pumped into the atmosphere, and a reduced greenhouse effect. -
SVP's Letter to Editors of Journals and Publishers on Burmese Amber And
Society of Vertebrate Paleontology 7918 Jones Branch Drive, Suite 300 McLean, VA 22102 USA Phone: (301) 634-7024 Email: [email protected] Web: www.vertpaleo.org FEIN: 06-0906643 April 21, 2020 Subject: Fossils from conflict zones and reproducibility of fossil-based scientific data Dear Editors, We are writing you today to promote the awareness of a couple of troubling matters in our scientific discipline, paleontology, because we value your professional academic publication as an important ‘gatekeeper’ to set high ethical standards in our scientific field. We represent the Society of Vertebrate Paleontology (SVP: http://vertpaleo.org/), a non-profit international scientific organization with over 2,000 researchers, educators, students, and enthusiasts, to advance the science of vertebrate palaeontology and to support and encourage the discovery, preservation, and protection of vertebrate fossils, fossil sites, and their geological and paleontological contexts. The first troubling matter concerns situations surrounding fossils in and from conflict zones. One particularly alarming example is with the so-called ‘Burmese amber’ that contains exquisitely well-preserved fossils trapped in 100-million-year-old (Cretaceous) tree sap from Myanmar. They include insects and plants, as well as various vertebrates such as lizards, snakes, birds, and dinosaurs, which have provided a wealth of biological information about the ‘dinosaur-era’ terrestrial ecosystem. Yet, the scientific value of these specimens comes at a cost (https://www.nytimes.com/2020/03/11/science/amber-myanmar-paleontologists.html). Where Burmese amber is mined in hazardous conditions, smuggled out of the country, and sold as gemstones, the most disheartening issue is that the recent surge of exciting scientific discoveries, particularly involving vertebrate fossils, has in part fueled the commercial trading of amber. -
Timing and Tempo of the Great Oxidation Event
Timing and tempo of the Great Oxidation Event Ashley P. Gumsleya,1, Kevin R. Chamberlainb,c, Wouter Bleekerd, Ulf Söderlunda,e, Michiel O. de Kockf, Emilie R. Larssona, and Andrey Bekkerg,f aDepartment of Geology, Lund University, Lund 223 62, Sweden; bDepartment of Geology and Geophysics, University of Wyoming, Laramie, WY 82071; cFaculty of Geology and Geography, Tomsk State University, Tomsk 634050, Russia; dGeological Survey of Canada, Ottawa, ON K1A 0E8, Canada; eDepartment of Geosciences, Swedish Museum of Natural History, Stockholm 104 05, Sweden; fDepartment of Geology, University of Johannesburg, Auckland Park 2006, South Africa; and gDepartment of Earth Sciences, University of California, Riverside, CA 92521 Edited by Mark H. Thiemens, University of California, San Diego, La Jolla, CA, and approved December 27, 2016 (received for review June 11, 2016) The first significant buildup in atmospheric oxygen, the Great situ secondary ion mass spectrometry (SIMS) on microbaddeleyite Oxidation Event (GOE), began in the early Paleoproterozoic in grains coupled with precise isotope dilution thermal ionization association with global glaciations and continued until the end of mass spectrometry (ID-TIMS) and paleomagnetic studies, we re- the Lomagundi carbon isotope excursion ca. 2,060 Ma. The exact solve these uncertainties by obtaining accurate and precise ages timing of and relationships among these events are debated for the volcanic Ongeluk Formation and related intrusions in because of poor age constraints and contradictory stratigraphic South Africa. These ages lead to a more coherent global per- correlations. Here, we show that the first Paleoproterozoic global spective on the timing and tempo of the GOE and associated glaciation and the onset of the GOE occurred between ca. -
Assembling Laurentia—Integrated Theme Sessions on Tectonic Turning Points
Assembling Laurentia—Integrated Theme Sessions on Tectonic Turning Points Michael L. Williams, Dept. of Geosciences, University of Massachusetts, Amherst, Massachusetts 01003, USA, [email protected]; Dawn A. Kellett, Geological Survey of Canada–Atlantic Division, Natural Resources Canada/Government of Canada, 1 Challenger Drive, Dartmouth, Nova Scotia B2Y 4A2, Canada, [email protected]; Basil Tikoff*, Dept. of Geoscience, University of Wisconsin– Madison, 1215 W. Dayton Street, Madison, Wisconsin 53706, USA, [email protected]; Steven J. Whitmeyer, Dept. of Geology and Environmental Science, James Madison University, 801 Carrier Drive, MSC 6903, Harrisonburg, Virginia 22807, USA, [email protected] The North American continent records the headlined by a Pardee Symposium, which and the broader implications of, these changes, evolution of tectonic processes and tectonic will provide an overview of the tectonic evo- and to widen the scope of investigation environments from the earliest Archean to lution of Laurentia and an introduction to the beyond a particular boundary or regional geo- modern times. The continent hosts a rich concept of key “Turning Points.” Seven logical event to the scale of Laurentia itself. Archean (and possibly Hadean) record, at related topical sessions, under the general The time slices for the topical sessions are as least three great Proterozoic orogenic belts, heading “Assembling Laurentia,” will span follows (with brief explanations from each and a wide range of Phanerozoic tectonic, the GSA meeting. -
The East Asian Jigsaw Puzzle Pangaea at Risk? from Neville Haile
192 Nature Vol. 293 17 September 1981 ment with the known seismic refraction (Business and Technological Systems, Inc.) pretation of long-wavelength crustal fields and heat flow data. His group believes that magnetization model for the United States, in terms of a geological/geophysical the region is the site of a late Precambrian derived from Magsat scalar data, had much model, promises to contribute significantly rift which was reactivated in the Mesozoic better resolution than that using POGO to our understanding of the Earth's crust. to form an aulacogen and its model data. In the older disciplines of main-field involves thinning of the upper crust and an Although preliminary, the results dis modelling and studies of external fields, increase in density in the lower crust. The cussed at the meeting indicate that sep there are significant new developments in magnetic low is accounted for by either an aration of the measured field into its core, both analytical techniques and in our isotherm upwarp or, less likely, a litho crustal and external 'components' is being understanding of the physics of the field logical variation in the crust. Mayhew's achieved. The newest discipline, inter- sources. 0 The East Asian jigsaw puzzle Pangaea at risk? from Neville Haile UNTIL fairly recently, reconstructions of the world palaeogeography followed Wegener in showing Eurasia, excluding the Indian subcontinent, as a single block, with the Malay Peninsula and part or all of the Indonesian Archipelago depending from it and looking rather vulnerablel ,2. Other world palaeogeo graphical maps simply omit South-east Asia and most of China (see the figure)3,4. -
The U-Series Toolbox for Paleoceanography
The U-series toolbox for paleoceanography Gideon M. Henderson Department of Earth Sciences, Oxford University, South Parks Road, Oxford, OX1 3PR, ENGLAND. e-mail: [email protected] Robert F. Anderson Lamont-Doherty Earth Observatory of Columbia University, Route 9W, Palisades, NY 10964, USA. e-mail: [email protected] Reviews in Mineralogy and Geochemistry "Uranium Series Geochemistry" Revised Version 1 1. Introduction The geochemistry of marine sediments is a major source of information about the past environment. Of the many measurements that provide such information, those of the U-series nuclides are unusual in that they inform us about the rate and timescales of processes. Oceanic processes such as sedimentation, productivity, and circulation, typically occur on timescales too short to be assessed using parent-daughter isotope systems such as Rb-Sr or Sm-Nd. So the only radioactive clocks that we can turn to are those provided by cosmogenic nuclides (principally 14C) or the U-series nuclides. This makes the U-series nuclides powerful allies in the quest to understand the past ocean-climate system and has led to their widespread application over the last decade. As in other applications of the U-series, those in paleoceanography rely on fractionation of the nuclides away from secular equilibrium. In the oceanic setting, this fractionation is generally due to differences in the solubility of the various nuclides. The general behavior of the U-series nuclides in the oceans was widely researched in the middle decades of the twentieth century. This work established knowledge of the concentrations of the nuclides in the various compartments of the ocean system, and of their fluxes between these compartments. -
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