Expected distribution of orbital elements of interstellar particles in the solar system

Details Expected distribution of orbital elements of interstellar particles in the solar system Expected distribution of orbital elements of interstellar particles in the solar system

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986avest..19..206b&link_type=abstract

(Astronomicheskii Vestnik, vol. 19, July-Sept. 1985, p. 206-210) Solar System Research (ISSN 0038-0946), vol. 19, no. 3, Jan. 19

Astronomy and Astrophysics

Astronomy

1

Interstellar Matter, Orbital Elements, Solar System, Density Distribution, Perihelions, Velocity Distribution

Scientific paper

The distribution of the eccentricities and perihelion distances for interstellar particles and their concentration in the solar system are calculated under the assumption that the distribution of their heliocentric velocities outside the sun's sphere of gravitational action is the same as the velocity distribution of the nearest stars of late spectral class. At a distance of 1 AU from the sun more than 75 percent of the orbits have an eccentricity of less than 1.1, while the particle concentration is nine times higher than in interstellar space.

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