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Hyperion - 13-day rotation from Voyager dataThe rotation period of Hyperion is determined here on the basis of a light-curve derived from low-resolution Voyager images taken over a two-month span. The data indicate a coherent 13-day spin period over 61 days, with the spin axis nearly parallel to the orbital plane. Since Hyperion is not in synchronous rotation, it cannot be used to test the hypothesis that dark dust spiralling inward on retrograde orbits causes the pronounced leading side/trailing side albedo asymmetry observed on the surface of Iapetus.
Document ID
19840053934
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Thomas, P.
(Cornell Univ. Ithaca, NY, United States)
Veverka, J.
(Cornell University Ithaca, NY, United States)
Wenkert, D.
(Cornell Univ. Ithaca, NY, United States)
Danielson, G. E.
(California Institute of Technology Pasadena, CA, United States)
Davies, M. E.
(Rand Corp. Santa Monica, CA, United States)
Date Acquired
August 12, 2013
Publication Date
February 23, 1984
Publication Information
Publication: Nature
Volume: 307
ISSN: 0028-0836
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0028-0836
Accession Number
84A36721
Funding Number(s)
CONTRACT_GRANT: NAGW-193
CONTRACT_GRANT: NASW-3602
Distribution Limits
Public
Copyright
Other

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