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Title: Properties of hydrogen, helium, and silicon dioxide mixtures in giant planet interiors

Abstract

Recent observations of Jupiter and Saturn provided by spacecraft missions, such as Juno and Cassini, compel us to revise and improve our models of giant planet interiors. Even though hydrogen and helium are by far the dominant species in these planets, heavy elements can play a significant role in the structure and evolution of the planet.

Authors:
ORCiD logo [1];  [1];  [1]; ORCiD logo [1]
  1. Univ. of California, Berkeley, CA (United States)
Publication Date:
Research Org.:
Univ. of California, Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1465731
Alternate Identifier(s):
OSTI ID: 1373965
Grant/Contract Number:  
SC0010517; SC0016248
Resource Type:
Accepted Manuscript
Journal Name:
Physics of Plasmas
Additional Journal Information:
Journal Volume: 24; Journal Issue: 4; Journal ID: ISSN 1070-664X
Publisher:
American Institute of Physics (AIP)
Country of Publication:
United States
Language:
English
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY

Citation Formats

Soubiran, François, Militzer, Burkhard, Driver, Kevin P., and Zhang, Shuai. Properties of hydrogen, helium, and silicon dioxide mixtures in giant planet interiors. United States: N. p., 2017. Web. doi:10.1063/1.4978618.
Soubiran, François, Militzer, Burkhard, Driver, Kevin P., & Zhang, Shuai. Properties of hydrogen, helium, and silicon dioxide mixtures in giant planet interiors. United States. doi:10.1063/1.4978618.
Soubiran, François, Militzer, Burkhard, Driver, Kevin P., and Zhang, Shuai. Wed . "Properties of hydrogen, helium, and silicon dioxide mixtures in giant planet interiors". United States. doi:10.1063/1.4978618. https://www.osti.gov/servlets/purl/1465731.
@article{osti_1465731,
title = {Properties of hydrogen, helium, and silicon dioxide mixtures in giant planet interiors},
author = {Soubiran, François and Militzer, Burkhard and Driver, Kevin P. and Zhang, Shuai},
abstractNote = {Recent observations of Jupiter and Saturn provided by spacecraft missions, such as Juno and Cassini, compel us to revise and improve our models of giant planet interiors. Even though hydrogen and helium are by far the dominant species in these planets, heavy elements can play a significant role in the structure and evolution of the planet.},
doi = {10.1063/1.4978618},
journal = {Physics of Plasmas},
number = 4,
volume = 24,
place = {United States},
year = {2017},
month = {3}
}

Journal Article:
Free Publicly Available Full Text
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Cited by: 9 works
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