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Gravitatinal Coefficients and Internal Structures of the Icy Galilean Satellites: An Assessment of the Galileo Orbiter Mission

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dc.contributor.author Schubert, G. en_US
dc.contributor.author Limonadi, D. en_US
dc.contributor.author Anderson, J. D. en_US
dc.contributor.author Campbell, J. K. en_US
dc.contributor.author Giampieri, G. en_US
dc.date.accessioned 2004-10-05T23:48:56Z
dc.date.available 2004-10-05T23:48:56Z
dc.date.issued 1994
dc.identifier.clearanceno 94-0719
dc.identifier.uri http://hdl.handle.net/2014/34373
dc.description.abstract Simulated radio tracking data from one flyby of Europa, two flybys of Ganymede, and two flybys of Callisto by the Galileo Orbiter yield estimates of the standard errors in the gravitational coefficient J*** of 44, 8.5, and 12 (in units of 10***) for Europa, Ganymede, and Callisto, respectively; errors in C***(in units of 10***) are 12, 1.7 and 2.1. en_US
dc.format.extent 1089210 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Galilean satellites en_US
dc.title Gravitatinal Coefficients and Internal Structures of the Icy Galilean Satellites: An Assessment of the Galileo Orbiter Mission en_US


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