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Origin of impact melt rocks in the Bununu howarditeThe Bununu howardite is a polymict regolith breccia which contains impact melt that is largely restricted to a 1-cm thick intrusion containing residual glass. As in Malvern, the melt rock contains melt with meteoritic Ni-Co contents. The cooling rate, interpreted for forming glass from this composition, is a few tenths of a degree per minute. The intrusive melts rock, which is a feature unique to Bununu, may indicate that Bununu was consolidated at the time of impact melting.
Document ID
19800039446
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Klein, L. C.
(Rutgers - The State Univ. Piscataway, NJ, United States)
Hewins, R. H.
(Rutgers University Piscataway, N.J., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1979
Subject Category
Geosciences (General)
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Start Date: March 19, 1979
End Date: March 23, 1979
Accession Number
80A23616
Funding Number(s)
CONTRACT_GRANT: NSG-9065
CONTRACT_GRANT: NSG-7327
Distribution Limits
Public
Copyright
Other

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