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Ices on the surface of TritonThe near-infrared spectrum of Triton reveals ices of nitrogen, methane, carbon monoxide, and carbon dioxide, of which nitrogen is the dominant component. Carbon dioxide ice may be spatially segregated from the other more volatile ices, covering about 10 percent of Triton's surface. The absence of ices of other hydrocarbons and nitriles challenges existing models of methane and nitrogen photochemistry on Triton.
Document ID
19930070168
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Cruikshank, Dale P.
(NASA Ames Research Center Moffett Field, CA, United States)
Roush, Ted L.
(San Francisco State Univ.; NASA, Ames Research Center Moffett Field, CA, United States)
Owen, Tobias C.
(Hawaii Univ. Honolulu, United States)
Geballe, Thomas R.
(Joint Astronomy Center Hilo, HI, United States)
De Bergh, Catherine
(Paris Observatoire, Meudon, France)
Schmitt, Bernard
(CNRS Lab. de Glaciologie et de Geophysique de l'Environnement, Saint-Martin-d'Heres, France)
Brown, Robert H.
(JPL Pasadena, CA, United States)
Bartholomew, Mary J.
(Sterling Software, Inc., Palo Alto; NASA, Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 16, 2013
Publication Date
August 6, 1993
Publication Information
Publication: Science
Volume: 261
Issue: 5122
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
93A54165
Distribution Limits
Public
Copyright
Other

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