A note on the cosmogony of the asteroidal belt

Details A note on the cosmogony of the asteroidal belt A note on the cosmogony of the asteroidal belt

Nov 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..45..235i&link_type=abstract

Astrophysics and Space Science, vol. 45, Nov. 1976, p. 235-241.

Astronomy and Astrophysics

Astrophysics

1

Asteroids, Cosmology, Mass Distribution, Planetary Evolution, Solar Corona, Astronomical Models, Eccentric Orbits, Orbital Elements, Orbital Velocity, Solar Orbits, Solar System, Spatial Distribution

Scientific paper

Several arguments based on the orbital dynamics of the asteroids are used to support the idea that the original solar nebula might not necessarily be the Laplacian type of thin disk-like structure. The orbital distribution of the large asteroids is suggested to be a direct result of their accretions of condensed grains in eccentric orbits via the jet stream process.

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