Helium and argon abundance constraints and the thermal evolution of Comet Austin (1989c1)

Details Helium and argon abundance constraints and the thermal evolution of Comet Austin (1989c1) Helium and argon abundance constraints and the thermal evolution of Comet Austin (1989c1)

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992icar...95..157s&link_type=abstract

Icarus (ISSN 0019-1035), vol. 95, Jan. 1992, p. 157-161.

Astronomy and Astrophysics

Astronomy

10

Abundance, Argon, Austin Comet, Evolution (Development), Helium, Thermodynamic Properties, Constraints, Far Ultraviolet Radiation, Rocket-Borne Instruments, Solar System, Ultraviolet Astronomy

Scientific paper

Far-UV rocketborne spectrometer observations have established upper Ar
and He abundance limits on Comet Austin. These limits indicate, relative
to solar abundance, that Comet Austin is depleted in He/O and no more
than 30-times enriched in Ar/O. Implications of these values for thermal
conditions experienced during formation and evolution are discussed.

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