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IRAS serendipitous survey observations of Pluto and CharonOn Aug. 16, 1983, the Infrared Astronomical Satellite made two separate pointed observations of Pluto and its moon Charon. Because of the small angular displacement of the system between the times of measurement, the Pluto-Charon system was identified as a source in the Serendipitous Survey (SSC 14029+0518). Detections were made at 60 and 100 micrometers with color-corrected flux densities of 581 + or - 58 and 721 + or - 123 millijanskys, respectively. Pluto is best described as having a dark equatorial band, and brighter polar caps of methane ice extending to + or - 45 deg latitude, at most. An upper limit of approximately 9 meter-amagats is placed on the column abundance of a methane atmosphere on Pluto, which is comparable to recent upper limits based on independent ground-based spectroscopy.
Document ID
19880024367
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sykes, Mark V.
(Arizona Univ. Tucson, AZ, United States)
Cutri, Roc M.
(Steward Observatory Tucson, AZ, United States)
Lebofsky, Larry A.
(Arizona, University Tucson, United States)
Binzel, Richard P.
(Science Applications International Corp. Planetary Science Institute, Tucson, AZ, United States)
Date Acquired
August 13, 2013
Publication Date
September 11, 1987
Publication Information
Publication: Science
Volume: 237
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
88A11594
Funding Number(s)
CONTRACT_GRANT: NSG-7114
CONTRACT_GRANT: JPL-954601
Distribution Limits
Public
Copyright
Other

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