Near-infrared spectrophotometry of Titan

Details Near-infrared spectrophotometry of Titan Near-infrared spectrophotometry of Titan

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icar...24..443t&link_type=abstract

(International Astronomical Union, Colloquium on Planetary Satellites, Cornell University, Ithaca, N.Y., Aug. 18-21, 1974.) Icar

Astronomy and Astrophysics

Astronomy

6

Infrared Spectroscopy, Methane, Near Infrared Radiation, Planetary Atmospheres, Titan, Abundance, Atmospheric Composition, Molecular Spectra, Saturn (Planet), Spectrophotometry

Scientific paper

Several unusual features in the near-IR spectrum of Titan are examined. Observations during four apparitions establish the reality of the S(1) absorption at 8150.7 A, but the existence of the S(O) absorption at 8272.7 A will require further sightings to become definitively established. These two features are particularly important, as they bear on the abundance of H2 in Titan's atmosphere.

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