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

Schubert, G.; Limonadi, D.; Anderson, J. D.; Campbell, J. K.; Giampieri, G.

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