Other
Scientific paper
Dec 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981rspta.303..351b&link_type=abstract
(Royal Society, Discussion on Planetary Exploration, London, England, Nov. 4, 5, 1980.) Royal Society (London), Philosophical Tr
Other
3
Comets, Cosmology, Interstellar Matter, Molecular Clouds, Nebulae, Solar System, Ambipolar Diffusion, Asteroids, Planetary Evolution, Stellar Evolution, Comets, Solar System, Origin, Formation, Source, Cometesimals, Rotation, Hypotheses, Fragments, Magnetic Properties
Scientific paper
Recent insights into the origin of comets have revived the suggestion that they did not originate in the presolar nebula itself but in a satellite nebula or in other nearby fragments of the same parent interstellar cloud. This provided another way by which material of a somewhat different early history might have been added to that of the planetary system. It is noted that a scheme for the formation of cometesimals exists that is consistent with what is known today on the contraction of a rotating magnetized fragment of an interstellar cloud and its dependence on the given initial conditions, which determine whether a double star, a single star, or cometesimals form.
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