Formation of Short-Period Orbits of Minor Bodies of the Mars Family

Details Formation of Short-Period Orbits of Minor Bodies of the Mars Family Formation of Short-Period Orbits of Minor Bodies of the Mars Family

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995em%26p...68..573t&link_type=abstract

Earth, Moon, and Planets, Volume 68, Issue 1-3, pp. 573-577

Physics

Scientific paper

It is shown that the orbits of minor bodies of the Mars family can be
formed as a result of single close encounters with the inner planets
(Venus -Mars) of minor bodies moving along orbits with the aphelion
distanceq' ≤ 4.26 AU. The Laplace method of the unperturbed two-body
problem was applied.

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