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Search for the 700,000-year-old source crater of the Australasian tektite strewn fieldMany tektite investigations have hypothesized that the impact crater that was the source of the extensive Australasian strewn field lies somewhere in or near Indochina. This is due to variations in abundance and size of tektites across the strewn field, variation of thickness of microtektite layers in ocean cores, nature and ablation characteristics across the field, and, above all, the occurrence of the large, blocky, layered Muong Nong-type tektites in Indochina. A recent study of the location and chemistry of Muong Nong-type and splash-form tektites suggests that the source region can be further narrowed to a limited area in eastern Thailand and southern Loas. Satellite multispectral imagery, a digital elevation dataset, and maps showing drainage patterns were used to search within this area for possible anomalous features that may be large degraded impact craters. Four interesting structures were identified from these datasets, and they are presented.
Document ID
19930000989
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Schnetzler, C. C.
(Maryland Univ. College Park., United States)
Garvin, J. B.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: Lunar and Planetary Inst., International Conference on Large Meteorite Impacts and Planetary Evolution
Subject Category
Geophysics
Accession Number
93N10177
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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