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Mass loss from the region of Mars and the asteroid beltModels of the solar nebula suggest that the mass of solid matter which condensed in the region of Mars and the asteroids was much greater than the amount now present. Bombardment by a primordial population of asteroidal bodies originating near Jupiter's orbit could preferentially remove matter from this region, without significant effects in the earth's zone. A critical velocity exists, for which they can be ejected from the solar system by Jupiter. The minimum perihelion attainable at this velocity lies between the orbits of Mars and the earth. The lifetimes of Mars-crossing bodies are limited by collisions with Jupiter; earth-crossers are ejected on a much shorter time scale. The total bombardment flux was at least two orders of magnitude greater in the zone of Mars than in that of the earth. The flux at Venus and Mercury from this source was negligible.
Document ID
19760032132
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Weidenschilling, S. J.
(MIT Cambridge, Mass., United States)
Date Acquired
August 8, 2013
Publication Date
November 1, 1975
Publication Information
Publication: Icarus
Volume: 26
Subject Category
Lunar And Planetary Exploration
Accession Number
76A15098
Funding Number(s)
CONTRACT_GRANT: NGL-22-009-521
Distribution Limits
Public
Copyright
Other

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