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Gravity Fields and Interiors of the Saturnian SatellitesThis viewgraph presentation reviews the Gravity Science Objectives and accomplishments of the Cassini Radio Science Team: (1) Mass and density of icy satellites (2) Quadrupole field of Titan and Rhea (3) Dynamic Love number of Titan (4) Moment of inertia of Titan (in collaboration with the Radar Team) (5) Gravity field of Saturn. The proposed measurements for the extended tour are: (1) Quadrupole field of Enceladus (2) More accurate measurement of Titan k2 (3) Local gravity/topography correlations for Iapetus (4) Verification/disproof of "Pioneer anomaly".
Document ID
20070032882
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
hdl:2014/39828
Authors
Rappaport, N. J. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Armstrong, J. W. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Asmar, Sami W. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Iess, L. (La Sapienza Univ. Rome, Italy)
Tortora, P. (Bologna Univ. Forly, Italy)
Somenzi, L. (La Sapienza Univ. Rome, Italy)
Zingoni, F. (La Sapienza Univ. Rome, Italy)
Date Acquired
August 23, 2013
Publication Date
July 15, 2006
Subject Category
Lunar And Planetary Science And Exploration
Meeting Information
Meeting: Third Annual Meeting of the Asia--Oceania Geosciences Society
Country: Singapore
Start Date: July 10, 2006
End Date: July 14, 2006
Distribution Limits
Public
Copyright
Other
Keywords
gravity
satellites
Saturn
Rhea
Enceladus
Cassini Mission

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