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The rotation period of UranusOn 24 January 1986 the spacecraft Voyager 2 transversed the innermost magnetosphere of the planet Uranus, coming as close as 4.2 Uranus radii to the planet. It is pointed out that the magnetic field data provide a direct measure of the rotation period of the planet's interior, where the field is generated. Two period determinations are reported. A combination of the obtained values provides a weighted mean value of P = 17.24 + or - 0.01 h. It is concluded that the 17.24-h rotation period has important consequences for studies of atmospheric dynamics and the internal structure and composition of Uranus. Thus, inferences regarding the internal structure can be drawn from the relationship between the observed planetary oblateness, rotation period, and gravitational moment.
Document ID
19860063709
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Desch, M. D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Connerney, J. E. P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Kaiser, M. L.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 12, 2013
Publication Date
July 3, 1986
Publication Information
Publication: Nature
Volume: 322
ISSN: 0028-0836
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0028-0836
Accession Number
86A48447
Distribution Limits
Public
Copyright
Other

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