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Europa's Differentiated Internal Structure: Inferences from Four Galileo Encounters

Anderson, J. D., Schubert, G., Jacobson, R. A., Lau, E. L., Moore, W. B., Sjogren, W. L.·1998·Science

Abstract

Radio 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.

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Metadata

Authors
Anderson, J. D., Schubert, G., Jacobson, R. A., Lau, E. L., Moore, W. B., & Sjogren, W. L.
Venue
Science
Published
1998-09-25
Volume
281
Issue
5385
Pages
2019-2022
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W4247443114
Cited by
413
References
0
FWCI
7.69
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Europa's Differentiated Internal Structure: Inferences from Four Galileo Encounters. https://app.cochat.ai/papers/10.1126/science.281.5385.2019
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Anderson, J. D., Schubert, G., Jacobson, R. A., Lau, E. L., Moore, W. B., & Sjogren, W. L. (1998). Europa's Differentiated Internal Structure: Inferences from Four Galileo Encounters. Science. https://doi.org/10.1126/science.281.5385.2019

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