105
views
0
recommends
+1 Recommend
0 collections
    0
    shares
      • Record: found
      • Abstract: found
      • Article: not found

      U/Pb Zircon Geochronology and Tempo of the End-Permian Mass Extinction

      Read this article at

      ScienceOpenPublisherPubMed
      Bookmark
          There is no author summary for this article yet. Authors can add summaries to their articles on ScienceOpen to make them more accessible to a non-specialist audience.

          Abstract

          The mass extinction at the end of the Permian was the most profound in the history of life. Fundamental to understanding its cause is determining the tempo and duration of the extinction. Uranium/lead zircon data from Late Permian and Early Triassic rocks from south China place the Permian-Triassic boundary at 251.4 ± 0.3 million years ago. Biostratigraphic controls from strata intercalated with ash beds below the boundary indicate that the Changhsingian pulse of the end-Permian extinction, corresponding to the disappearance of about 85 percent of marine species, lasted less than 1 million years. At Meishan, a negative excursion in δ 13 C at the boundary had a duration of 165,000 years or less, suggesting a catastrophic addition of light carbon.

          Related collections

          Most cited references32

          • Record: found
          • Abstract: not found
          • Article: not found

          A low-contamination method for hydrothermal decomposition of zircon and extraction of U and Pb for isotopic age determinations

          T.E Krogh (1973)
            Bookmark
            • Record: found
            • Abstract: not found
            • Article: not found

            Intercalibration of standards, absolute ages and uncertainties in 40Ar/39Ar dating

              Bookmark
              • Record: found
              • Abstract: found
              • Article: not found

              A blast of gas in the latest Paleocene: simulating first-order effects of massive dissociation of oceanic methane hydrate.

              Carbonate and organic matter deposited during the latest Paleocene thermal maximum is characterized by a remarkable -2.5% excursion in delta 13C that occurred over approximately 10(4) yr and returned to near initial values in an exponential pattern over approximately 2 x 10(5) yr. It has been hypothesized that this excursion signifies transfer of 1.4 to 2.8 x 10(18) g of CH4 from oceanic hydrates to the combined ocean-atmosphere inorganic carbon reservoir. A scenario with 1.12 x 10(18) g of CH4 is numerically simulated here within the framework of the present-day global carbon cycle to test the plausibility of the hypothesis. We find that (1) the delta 13C of the deep ocean, shallow ocean, and atmosphere decreases by -2.3% over 10(4) yr and returns to initial values in an exponential pattern over approximately 2 x 10(5) yr; (2) the depth of the lysocline shoals by up to 400 m over 10(4) yr, and this rise is most pronounced in one ocean region; and (3) global surface temperature increases by approximately 2 degrees C over 10(4) yr and returns to initial values over approximately 2 x 10(6) yr. The first effect is quantitatively consistent with the geologic record; the latter two effects are qualitatively consistent with observations. Thus, significant CH4 release from oceanic hydrates is a plausible explanation for observed carbon cycle perturbations during the thermal maximum. This conclusion is of broad interest because the flux of CH4 invoked during the maximum is of similar magnitude to that released to the atmosphere from present-day anthropogenic CH4 sources.
                Bookmark

                Author and article information

                Journal
                Science
                Science
                American Association for the Advancement of Science (AAAS)
                0036-8075
                1095-9203
                May 15 1998
                May 15 1998
                : 280
                : 5366
                : 1039-1045
                Affiliations
                [1 ]S. A. Bowring, M. W. Martin, and K. Davidek are in the Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02319, USA. D. H. Erwin is in the Department of Paleobiology, National Museum of Natural History, Washington, DC 20560, USA. Y. G. Jin and W. Wang are at the Laboratory of Paleobiology and Stratigraphy, Nanjing Institute of Geology and Paleontology, Academia Sinica, Nanjing, 210008, People's Republic of China.
                Article
                10.1126/science.280.5366.1039
                9582110
                43ad92cc-34e5-4e32-91e7-3ed53145feeb
                © 1998
                History

                Comments

                Comment on this article