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Europa's differentiated internal structure: inferences from four Galileo encountersRadio Doppler data from four encounters of the Galileo spacecraft with the jovian moon Europa have been used to refine models of Europa's interior. Europa is most likely differentiated into a metallic core surrounded by a rock mantle and a water ice-liquid outer shell, but the data cannot eliminate the possibility of a uniform mixture of dense silicate and metal beneath the water ice-liquid shell. The size of a metallic core is uncertain because of its unknown composition, but it could be as large as about 50 percent of Europa's radius. The thickness of Europa's outer shell of water ice-liquid must lie in the range of about 80 to 170 kilometers.
Document ID
20040172554
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Anderson, J. D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Schubert, G.
Jacobson, R. A.
Lau, E. L.
Moore, W. B.
Sjogren, W. L.
Date Acquired
August 22, 2013
Publication Date
September 25, 1998
Publication Information
Publication: Science
Volume: 281
Issue: 5385
ISSN: 0036-8075
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
ISSN: 0036-8075
Distribution Limits
Public
Copyright
Other
Keywords
unmanned
Flight Experiment
Galileo Project
long duration
Ice
Jupiter
Water
Support, U.S. Gov't, Non-P.H.S
Iron
Extraterrestrial Environment
Silicates
Ferrous Compounds

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