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Neptune cloud structure at visible wavelengthsDigital images of Neptune showing cloud structure at visible wavelengths were obtained in July 1988. A discrete bright feature was detected both at 6190 A (a weak methane absorption band in the visible) and at 8900 A (a stronger methane band in the near infrared). The images also revealed that Neptune's southern pole was bright relative to planetary mid-latitudes at 6190 A but not 8900 A. The implications of these findings for atmospheric rotation and structure are discussed. The detection of discrete features at visible wavelengths is of special importance to the upcoming Voyager encounter with Neptune: the wide-angle camera has a 6190 A filter similar to that used for these observations.
Document ID
19890056494
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hammel, H. B.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Date Acquired
August 14, 2013
Publication Date
June 9, 1989
Publication Information
Publication: Science
Volume: 244
ISSN: 0036-8076
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0036-8076
Accession Number
89A43865
Funding Number(s)
CONTRACT_GRANT: NSF AST-85-14575
CONTRACT_GRANT: NSF AST-86-15631
Distribution Limits
Public
Copyright
Other

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