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Tektite-like bodies at Lonar Crater, India - Implications for the origin of tektitesHomogeneous dense glass bodies (both irregular and splash form) with high silica contents (about 67 pct SiO2) occur in the vicinity of Lonar Crater, India. Their lack of microlites and mineral remnants and their uniform chemical composition virtually preclude a volcanic origin. They are similar to tektites reported in the literature. While such a close association of tektite-like bodies with impact craters is already known (Aouelloul Crater, Mauritania; Zhamanshin Crater, U.S.S.R.), the tektite-like bodies at Lonar Crater are unique in that they occur in an essentially basaltic terrain. Present geochemical data are consistent with these high silica glass bodies being impact melt products of two-thirds basalt and one-third local intertrappean sediment (chert). The tektite-like bodies of the impact craters Lonar, Zhamanshin, and Aouelloul are generally similar. Strong terrestrial geochemical signatures reflect the target rock REE patterns and abundance ratios and demonstrate their terrestrial origin resulting from meteorite impact, as has been suggested by earlier workers.
Document ID
19870046817
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Murali, A. V.
(NASA Johnson Space Center; Lunar and Planetary Institute Houston, TX, United States)
Zolensky, M. E.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Blanchard, D. P.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 13, 2013
Publication Date
March 30, 1987
Publication Information
Publication: Journal of Geophysical Research
Volume: 92
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
87A34091
Funding Number(s)
CONTRACT_GRANT: NSF INT-81-05600
CONTRACT_GRANT: NASW-4066
Distribution Limits
Public
Copyright
Other

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