Sep 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986georl..13..976m&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 13, Sept. 1986, p. 976-978; Reply, p. 979, 980.
Physics
1
Collision Rates, Comets, Earth Atmosphere, Hypervelocity Impact, Thermal Conductivity, Thermal Stability
Scientific paper
Frank 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.
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