NASA NTRS · 19730058534
Asteroidal source of meteorites.
Abstract
An effective mechanism for the placement of asteroidal fragments into earth-crossing orbits is discussed. It is pointed out that an asteroid in an orbit with a semimajor axis of about 3.27 AU, corresponding to the most apparent Kirkwood Gap, has a period almost exactly half that of Jupiter and will experience strong resonant perturbations by Jupiter. In the proposed mechanism, fragments 10 to 500 m in diameter resulting from collisions between asteroids located just outside the region in which libration due to the perturbations takes place are injected into the Kirkwood Gap.
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Zimmerman, P. D., Wetherill, G. W.. 1973-10-05. Asteroidal source of meteorites.. https://ntrs.nasa.gov/citations/19730058534
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