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Orbital-scale climate change and glacioeustasy during the early Late Ordovician (pre-Hirnantian) determined from δ18O values in marine apatite
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  • journal_title:Geology
  • Contributor:M. Elrick ; D. Reardon ; W. Labor ; J. Martin ; A. Desrochers ; M. Pope
  • Publisher:Geological Society of America
  • Date:2013-07-01
  • Format:text/html
  • Language:en
  • Identifier:10.1130/G34363.1
  • journal_abbrev:Geology
  • issn:0091-7613
  • volume:41
  • issue:7
  • firstpage:775
  • section:Articles
摘要

This study focuses on the ∼10 m.y. before the latest Ordovician (Hirnantian) glaciation; we test whether orbital-scale climatic fluctuations controlled the growth and melting of continental glaciers, resulting in glacioeustatic sea-level changes and the development of widespread marine sedimentary cycles. δ18O values of conodont apatite from 14 Late Ordovician (Katian) cycles range from ∼17‰ to 21‰. Isotopic values decrease and are lowest in the deepest water facies and increase and are highest in shallow-water facies, supporting the hypothesis that glacioeustasy was the dominant control on water-depth changes. Measured intracycle δ18O changes of 0.7‰–2.5‰ were controlled by changes in ice volume (<60 m sea-level changes), sea-surface temperatures (<5 °C), and potentially local increases in seawater evaporation during drier and/or windier glacial stages. These interpreted orbital-scale climate changes and resultant large glacial ice-volume changes support recent interpretations of a dynamic and prolonged Ordovician greenhouse to icehouse transition.

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