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Voyager 2 at Neptune - Imaging science resultsNeptune's atmosphere is revealed by Voyager 2 images to contain clouds of methane ice above a lower deck of hydrogen sulfide or ammonia ices, and to be dominated by an anticyclonic storm system designated the 'Great Dark Spot'; this bears both similarities and differences to the Great Red Spot of Jupiter. Like the rings of Uranus, those of Neptune are composed of very dark, but in addition very dusty, material. Six new regular satellites have been discovered whose radii range from 25 to 200 km. Triton is noted to be a differentiated body showing evidence of early surface-melting episodes. At least two active plumes are found on Triton, which may be driven by solar heating.
Document ID
19900031372
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Smith, B. A.
(Arizona, University Tucson, United States)
Soderblom, L. A.
(USGS Flagstaff, AZ, United States)
Banfield, D.
(California Institute of Technology Pasadena, United States)
Barnet, C.
(Arizona Univ. Tucson, AZ, United States)
Beebe, R. F.
(New Mexico State University Las Cruces, United States)
Bazilevskii, A. T.
(AN SSSR Institut Geokhimii i Analiticheskoi Khimii, Moscow, Ussr)
Bollinger, K.
(JPL Pasadena, CA, United States)
Boyce, J. M.
(Arizona Univ. Tucson, AZ, United States)
Briggs, G. A.
(NASA Headquarters Washington, DC United States)
Brahic, A.
(Paris Observatoire, Meudon, France)
Date Acquired
August 14, 2013
Publication Date
December 15, 1989
Publication Information
Publication: Science
Volume: 246
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
90A18427
Distribution Limits
Public
Copyright
Other

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