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Galileo Gravity Results and the Internal Structure of IoDoppler data generated with the Galileo spacecraft's radio carrier wave were used to measure Io's external gravitational field. The resulting triaxial field is consistent with the assumption that Io is in tidal and rotational equilibrium. The inescapable conclusion is that it has a large metallic core. If the core is a eutectic mixture of iron and iron sulfide, it comprises 20.2 +/- 7.4 percent of the satellite's total mass with a radius that is about 52 percent of lo's mean radius of 1821.3 kilometers; if the core is pure iron, it comprises 10.5 +/- 3.7 percent of the total mass with a radius of about 36 percent of the mean radius.
Document ID
19990099707
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
Authors
Anderson J. D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Sjogren, W. L.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Schubert, G.
(California Univ. Los Angeles, CA United States)
Date Acquired
August 19, 2013
Publication Date
May 3, 1996
Publication Information
Publication: Science
Publisher: American Association for the Advancement of Science
Volume: 272
Subject Category
Lunar And Planetary Exploration
Distribution Limits
Public
Copyright
Other

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