The spatial distribution of large cometary meteoroids in the inner solar system

Details The spatial distribution of large cometary meteoroids in the inner solar system The spatial distribution of large cometary meteoroids in the inner solar system

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acm..proc..403m&link_type=abstract

In Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991 p 403-406 (SEE N93-19113 06-90)

Astronomy and Astrophysics

Astronomy

Meteoroids, Quadrantid Meteoroids, Spatial Distribution, Taurid Meteoroids, Astronomical Models, Comets, Density Distribution

Scientific paper

A model of the spatial density distribution of large (m greater than 10-3 g) cometary meteoroids in the inner solar system is obtained assuming that they have orbits closely associated with that of their parent comet. Distributions of the orbital parameters of the Taurid, Quadrantid and Perseid meteoroid streams are used in developing the model.

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