Accretion of jet streams and formation of asteroids

Details Accretion of jet streams and formation of asteroids Accretion of jet streams and formation of asteroids

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983cha%26a...7...54h&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 7, Issue 1, p. 54-58.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Our basic view on the formation of asteroids, stated in [1], is that the initial physical and chemical conditions in the asteroid region led to a slow growth of planetesimals in the region and a transfer of accretable matter to the Jupitor region, resulting in the planetesimals stopping at the ``half-finished'' stage, eventually forming only asteroids and not major planets. In this paper, using the conditions of the nebular disk obtained in that paper and the formula for gravitational instability and regarding the rings resulting from gravitational instability as ``jet streams'', we apply the theory of accretion of jet streams to calculate the growth of the planetesimals and discuss the question of the transfer of accretable material, providing further confirmation of our basic view.

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