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Triton - Do we see to the surface?The quantity and physical state of methane and nitrogen in the atmosphere of Neptune's satellite Triton and on the surface are evaluated by means of new telescopic data and laboratory measurements of these volatiles. Methane ice is seen in some spectral regions, indicating that the atmosphere is sufficiently transparent to permit sunlight penetration to the surface. Some of the molecular nitrogen absorption occurs in the atmosphere, though some must occur in condensed nitrogen (liquid or solid) on Triton's surface, or in a thin cloud of condensed nitrogen. The Voyager spacecraft cameras should see the surface of Triton.
Document ID
19890059227
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Cruikshank, D. P.
(NASA Ames Research Center Moffett Field, CA, United States)
Giver, L. P.
(NASA Ames Research Center Moffett Field, CA, United States)
Brown, R. H.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Tokunaga, A. T.
(Hawaii, University Honolulu, United States)
Date Acquired
August 14, 2013
Publication Date
July 21, 1989
Publication Information
Publication: Science
Volume: 245
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0036-8075
Accession Number
89A46598
Distribution Limits
Public
Copyright
Other

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