A model of the heliocentric orbits of a stream of Earth-impacting interstellar meteoroids

Details A model of the heliocentric orbits of a stream of Earth-impacting interstellar meteoroids A model of the heliocentric orbits of a stream of Earth-impacting interstellar meteoroids

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...382.1118b&link_type=abstract

Astronomy and Astrophysics, v.382, p.1118-1124 (2002)

Astronomy and Astrophysics

Astrophysics

10

Meteors, Meteoroids, Ism: Kinematics And Dynamics

Scientific paper

We consider the influx of a collinear stream of interstellar particles (ISPs) into the Solar System for the case where non-gravitational forces are negligible (particle size ga 20 mu m) and model their Keplerian trajectories to yield the expected heliocentric orbits on impact with the Earth. The heliocentric orbital characteristics of such a stream of ISPs undergo cyclic seasonal variations allowing the determination of the stream inflow direction and far-Sun speed the orbit element signatures.

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