Modeling the distribution of meteoroid matter in the solar system

Details Modeling the distribution of meteoroid matter in the solar system Modeling the distribution of meteoroid matter in the solar system

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986avest..20..134z&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 20, Apr.-June 1986, p. 134-141. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Meteoroid Concentration, Solar System, Distance, Kepler Laws, Mass Distribution, Meteoritic Composition, Orbital Elements, Spatial Distribution

Scientific paper

The problem of modeling the distribution of meteoroid matter in the solar system is formulated and solved using the phase-density distribution function determined in the space of Keplerian elements. The proposed models describe the interplanetary cloud of sporadic meteoroids. The dependences of space density and flux density on heliocentric distance are ascertained on the basis of McCrosky-Posen catalog data for the ecliptic plane.

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