Physical observations of comets: Their composition, origin and evolution

Details Physical observations of comets: Their composition, origin and evolution Physical observations of comets: Their composition, origin and evolution

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991plas.rept...29c&link_type=abstract

In NASA, Washington, Reports of Planetary Astronomy, 1991 p 29-31 (SEE N92-12792 03-89)

Astronomy and Astrophysics

Astronomy

Asteroids, Cometary Atmospheres, Imaging Techniques, Planetary Composition, Planetary Evolution, Stellar Evolution, Stellar Spectra, High Resolution, Imaging Spectrometers, Space Observations (From Earth), Spectrum Analysis

Scientific paper

The composition, origins, and evolution of comets were studied. The composition was studied using spectroscopic observations of primarily brighter comets at moderate and high resolution for the distribution of certain gases in the coma. The origins was addressed through an imaging search for the Kuiper belt of comets. The evolution was addressed by searching for a link between comets and asteroids using an imaging approach to search for an OH coma.

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