Giant molecular clouds and the solar system comets

Details Giant molecular clouds and the solar system comets Giant molecular clouds and the solar system comets

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982jrasc..76..303v&link_type=abstract

Journal of the Royal Astronomical Society of Canada, vol. 76, Oct. 1982, p. 303-308.

Astronomy and Astrophysics

Astronomy

17

Comets, Molecular Clouds, Solar System, Interstellar Gas, Oort Cloud

Scientific paper

The interaction of the sun with giant molecular clouds (GMC) will result in the loss of comets from the Oort cloud. It is shown that regeneration of the Oort cloud cannot occur by the capture of interstellar cometesimals. It is also shown, in an examination of the total density of matter near the sun, that the chemical evolution of the galactic disk was not significantly influenced by heavy elements locked up in interstellar cometesimals.

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