Quasi-stationary parameters of small bodies in the solar system

Details Quasi-stationary parameters of small bodies in the solar system Quasi-stationary parameters of small bodies in the solar system

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987avest..21...75k&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 21, Jan.-Mar. 1987, p. 75-83. In Russian.

Astronomy and Astrophysics

Astronomy

Apollo Asteroids, Comets, Meteoroids, Solar System, Astronomical Photography, Meteorite Collisions, Meteoroid Showers, Orbits, Radar Photography, Statistical Distributions

Scientific paper

The following quasistationary parameters of small bodies in the solar system are introduced: P = 0.6/a-[a(1-e2)]cos2i-2, Q = 0.4+(2a-1)(1-e2)cos2i- e2(0.4-sin2ωmsin2i). These are investigated on the basis of data of photographic and radar observations of meteors, comets and Apollo-Amor asteroids. From the quasistationary parameters P and Q one can infer the genetic relations between the bodies studied, specify the probabilities of their encounters with planets and the meteor matter influx on the planets of our solar system.

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