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Magnetic field signatures near Galileo's closest approach to GaspraTwo large magnetic field rotations were recorded by the spacecraft Galileo 1 minute before and 2 minutes after its closest approach to the asteroid Gaspra. The timing and the geometry of the field changes suggest a connection with Gaspra, and the events can be interpreted as the result of the draping of the solar wind field around a magnetospheric obstacle. Gaspra's surface field is inferred to be within an order of magnitude of Earth's surface field, and its magnetic moment per unit mass is in the range observed for iron meteorites and highly magnetized chondrites. The location of the magnetic signatures suggests that perturbations are carried by waves in the magnetosonic-whistler mode with wavelengths between electron and ion gyro radii.
Document ID
19930067205
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kivelson, M. G.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Bargatze, L. F.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Khurana, K. K.
(California Univ. Los Angeles, United States)
Southwood, D. J.
(Imperial College of Science, Technology, and Medicine London, United Kingdom)
Walker, R. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Coleman, P. J., Jr.
(California Univ. Los Angeles, United States)
Date Acquired
August 16, 2013
Publication Date
July 16, 1993
Publication Information
Publication: Science
Volume: 261
Issue: 5119
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
93A51202
Funding Number(s)
CONTRACT_GRANT: JPL-958694
Distribution Limits
Public
Copyright
Other

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