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Surface ices and the atmospheric composition of PlutoObservations of the 1.4- to 2.4-micrometer spectrum of Pluto reveal absorptions of carbon monoxide and nitrogen ices and confirm the presence of solid methane. Frozen nitrogen is more abundant than the other two ices by a factor of about 50; gaseous nitrogen must therefore be the major atmospheric constituent. The absence of carbon dioxide absorptions is one of several differences between the spectra of Pluto and Triton in this region. Both worlds carry information about the composition of the solar nebula and the processes by which icy planetesimals formed.
Document ID
19930070169
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Owen, Tobias C.
(Hawaii Univ. Honolulu, United States)
Roush, Ted L.
(San Francisco State Univ.; NASA, Ames Research Center Moffett Field, CA, United States)
Cruikshank, Dale P.
(NASA Ames Research Center Moffett Field, CA, United States)
Elliot, James L.
(NASA Ames Research Center Moffett Field, CA, United States)
Young, Leslie A.
(MIT Cambridge, MA, 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)
Geballe, Thomas R.
(Joint Astronomy Center Hilo, HI, United States)
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
93A54166
Distribution Limits
Public
Copyright
Other

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