Journal
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA
Volume 117, Issue 3, Pages 1346-1353Publisher
NATL ACAD SCIENCES
DOI: 10.1073/pnas.1904368116
Keywords
Australasian; impact; crater; Lao; tektite
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Funding
- Earth Observatory of Singapore
- National Research Foundation Singapore
- Singapore Ministry of Education under the Research Centers of Excellence initiative
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The crater and proximal effects of the largest known young meteorite impact on Earth have eluded discovery for nearly a century. We present 4 lines of evidence that the 0.79-Ma impact crater of the Australasian tektites lies buried beneath lavas of a long-lived, 910-km(3) volcanic field in Southern Laos: 1) Tektite geo-chemistry implies the presence of young, weathered basalts at the site at the time of the impact. 2) Geologic mapping and 40Ar-39Ar dates confirm that both pre- and postimpact basaltic lavas exist at the proposed impact site and that postimpact basalts wholly cover it. 3) A gravity anomaly there may also reflect the presence of a buried similar to 17 x 13-km crater. 4) The nature of an outcrop of thick, crudely layered, bouldery sandstone and mud-stone breccia 10-20 km from the center of the impact and fractured quartz grains within its boulder clasts support its being part of the proximal ejecta blanket.
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