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.
Near-infrared spectrophotometry of Titan
1975-04-01
Miscellaneous
No indication
English
Infrared photometry and spectrophotometry of Titan
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