Transformation of the orbits of minor bodies at close encounters with terrestrial planets

Details Transformation of the orbits of minor bodies at close encounters with terrestrial planets Transformation of the orbits of minor bodies at close encounters with terrestrial planets

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991avest..25..177a&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 25, Mar.-Apr. 1991, p. 177-180. In Russian.

Astronomy and Astrophysics

Astronomy

Celestial Bodies, Encounters, Orbit Calculation, Solar Orbits, Terrestrial Planets, Asteroids, Comets, Laplace Equation, Meteoroids

Scientific paper

A computing scheme based on multiple application of the unperturbed problem of two bodies (the Laplace method) is used to show that close encounters of minor bodies with terrestrial planets can result in the formation of short-period orbits in the inner solar system. It is suggested that Geminid- and Arietid-type meteor streams and at least some Amor- and Apollo-type asteroids may be of cometary origin.

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