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On the origin of interplanetary dust within recorded historyThe possibility of an abrupt origin of interplanetary dust as a result of a collision between asteroids or an extraordinary comet is considered. If all interplanetary dust were produced in one event within recorded history, it would have been visible from the Earth with the unaided eye. The rate, surface area, and brightness of asteroid collision remnants are derived. Ancient Chinese records are searched for extraordinary comets aand bright pointlike objects with small angular motion and concentration to the ecliptic.
Document ID
19930029962
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Reach, William T.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 15, 2013
Publication Date
September 1, 1992
Publication Information
Publication: Meteoritics
Volume: 27
Issue: 4
ISSN: 0026-1114
Subject Category
Astrophysics
Accession Number
93A13959
Funding Number(s)
CONTRACT_GRANT: NSF AST-88-18544
Distribution Limits
Public
Copyright
Other

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