The orbital evolution of the Apollo asteroid group over 11,550 years

Details The orbital evolution of the Apollo asteroid group over 11,550 years The orbital evolution of the Apollo asteroid group over 11,550 years

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992avest..26...71z&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 26, no. 4, p. 71-77.

Astronomy and Astrophysics

Astronomy

Apollo Asteroids, Orbital Elements, Orbital Resonances (Celestial Mechanics), Solar Orbits, Terrestrial Planets

Scientific paper

The Everhard method was used to monitor the orbital evolution of 20 Apollo asteroids in the time interval from 2250 A.D. to 9300 B.C. The closest encounters with large planets in the evolution process are calculated. Stable resonances with Venus and Earth over the period from 2250 A.D. to 9300 B.C. are obtained. Theoretical coordinates of radiants on initial and final moments of integration are calculated.

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