Physics
Scientific paper
Sep 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992metic..27..353r&link_type=abstract
Meteoritics (ISSN 0026-1114), vol. 27, no. 4, p. 353-360.
Physics
3
Asteroids, Comets, Evolution (Development), Interplanetary Dust, Brightness Distribution, Halley'S Comet, Interplanetary Medium
Scientific paper
The 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.
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