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CommentFrank et al.'s (1986) suggestion that the earth is impacted by small (100-Mg) comets at the rate of 20/min is reconsidered in the light of recent comet models. The possibility of such a swarm of comets is found to be problematical because of the large number of comets required and because thermal stability arguments, while not excluding such a possibility, imply that it is implausible. In a reply, Frank et al. reaffirm their findings that such small comets, following direct elliptical orbits about the sun, are distributed in a disk centered on the sun and lying near the ecliptic plane at heliocentric radial distances 1-10,000 AU. The presence of these comets in the inner solar system is attributed to the gravitational action of the outer planets, passing stars, or interstellar clouds on comets is more distant orbits.
Document ID
19870030593
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mckay, C. P.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 13, 2013
Publication Date
September 1, 1986
Publication Information
Publication: Geophysical Research Letters
Volume: 13
ISSN: 0094-8276
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0094-8276
Accession Number
87A17867
Funding Number(s)
CONTRACT_GRANT: NGL-16-001-002
CONTRACT_GRANT: N00014-85-K-0404
CONTRACT_GRANT: NAG5-483
Distribution Limits
Public
Copyright
Other

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