The orbital evolution of the Aten asteroids over 11,550 years (9300 BC to 2250 AD)

Details The orbital evolution of the Aten asteroids over 11,550 years (9300 BC to 2250 AD) The orbital evolution of the Aten asteroids over 11,550 years (9300 BC to 2250 AD)

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991avest..25..171z&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 25, Mar.-Apr. 1991, p. 171-176. In Russian.

Astronomy and Astrophysics

Astronomy

Asteroids, Encounters, Orbital Mechanics, Orbital Resonances (Celestial Mechanics), Solar Orbits, Earth Orbits, Mercury (Planet), Planetary Orbits, Secular Variations, Venus (Planet)

Scientific paper

The orbital evolution of five Aten asteroids was monitored by the
Everhart method in the time interval from 9300 BC to 2250 AD. The
closest encounters with large planets in the evolution process are
calculated. Four out of five asteroids exhibit stable resonances with
earth and Venus over the period from 9300 BC to 2250 AD.

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