Physics
Scientific paper
Mar 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cemec..43..113f&link_type=abstract
Celestial Mechanics, Volume 43, Issue 1-4, pp. 113-117
Physics
Minor Planets:Orbital Evolution, Minor Planets:Orbits, Minor Planets:Resonances, Orbital Evolution:Minor Planets, Orbits:Minor Planets, Resonances:Minor Planets
Scientific paper
We integrated numerically, in the frame of the four body problem “Sun-Jupiter-Saturn-asteroid” the orbit of the asteroid 1974 MA, an Earth-crosser, which is located in a region where three resonances overlap: the two secular resonancesυ 5 andυ 16 and the mean motion resonance 5/1. The numerical integration yields a qualitative orbital evolution of this particular region.
Froeschlé Ch.
Scholl Hans
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