Evidence of Cosmic Impact at Abu Hureyra, Syria at the Younger Dryas Onset (~12.8 ka): High-temperature melting at >2200 °C

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作者
Andrew M. T. Moore
James P. Kennett
William M. Napier
Ted E. Bunch
James C. Weaver
Malcolm LeCompte
A. Victor Adedeji
Paul Hackley
Gunther Kletetschka
Robert E. Hermes
James H. Wittke
Joshua J. Razink
Michael W. Gaultois
Allen West
机构
[1] Rochester Institute of Technology,College of Liberal Arts
[2] University of California Santa Barbara,Department of Earth Science and Marine Science Institute
[3] College Hill,Armagh Observatory and Planetarium
[4] Armagh BT61 9DG,Geology Division, School of Earth and Sustainability
[5] Northern Arizona University,Wyss Institute for Biologically Inspired Engineering
[6] Harvard University,Department of Natural Sciences
[7] Elizabeth City State University,Institute of Geology, Czech Academy of Science of the Czech Republic and
[8] Center of Excellence in Remote Sensing Education and Research,Center for Advanced Materials Characterization at Oregon (CAMCOR)
[9] Elizabeth City State University,Leverhulme Research Centre for Functional Materials Design, The Materials Innovation Factory, Department of Chemistry
[10] U.S. Geological Survey (USGS),undefined
[11] Charles University,undefined
[12] Faculty of Science,undefined
[13] Czech Republic,undefined
[14] CZE; and University of Alaska Fairbanks,undefined
[15] 903 Koyukuk Drive,undefined
[16] Los Alamos National Laboratory (retired),undefined
[17] University of Oregon,undefined
[18] University of Liverpool,undefined
[19] Comet Research Group,undefined
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摘要
At Abu Hureyra (AH), Syria, the 12,800-year-old Younger Dryas boundary layer (YDB) contains peak abundances in meltglass, nanodiamonds, microspherules, and charcoal. AH meltglass comprises 1.6 wt.% of bulk sediment, and crossed polarizers indicate that the meltglass is isotropic. High YDB concentrations of iridium, platinum, nickel, and cobalt suggest mixing of melted local sediment with small quantities of meteoritic material. Approximately 40% of AH glass display carbon-infused, siliceous plant imprints that laboratory experiments show formed at a minimum of 1200°–1300 °C; however, reflectance-inferred temperatures for the encapsulated carbon were lower by up to 1000 °C. Alternately, melted grains of quartz, chromferide, and magnetite in AH glass suggest exposure to minimum temperatures of 1720 °C ranging to >2200 °C. This argues against formation of AH meltglass in thatched hut fires at 1100°–1200 °C, and low values of remanent magnetism indicate the meltglass was not created by lightning. Low meltglass water content (0.02–0.05% H2O) is consistent with a formation process similar to that of tektites and inconsistent with volcanism and anthropogenesis. The wide range of evidence supports the hypothesis that a cosmic event occurred at Abu Hureyra ~12,800 years ago, coeval with impacts that deposited high-temperature meltglass, melted microspherules, and/or platinum at other YDB sites on four continents.
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