High resolution observations of the 2.125-micron feature in Io's spectrum during 1975 and 1976

Details High resolution observations of the 2.125-micron feature in Io's spectrum during 1975 and 1976 High resolution observations of the 2.125-micron feature in Io's spectrum during 1975 and 1976

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992icar...95..325l&link_type=abstract

Icarus (ISSN 0019-1035), vol. 95, Feb. 1992, p. 325-328.

Physics

4

Absorption Spectra, Infrared Spectra, Io, Line Spectra, Near Infrared Radiation, Annual Variations, Space Observations (From Earth)

Scientific paper

High resolution observations of a weak absorption feature in the Io spectrum, obtained in 1975-1976 indicate that, if this feature is indicative of the presence of a new class of material, it may be the only diagnostic feature in Io's near-IR spectrum that can be distinguished by terrestrial telescopes. It appears unlikely that the absorber is a gas, or that gaseous CO2 contributes to the line shape.

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