Properties of hydrogen, helium, and silicon dioxide mixtures in giant planet interiors
- Univ. of California, Berkeley, CA (United States); Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA
- Univ. of California, Berkeley, CA (United States)
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.
- Research Organization:
- Univ. of California, Berkeley, CA (United States)
- Sponsoring Organization:
- USDOE; USDOE Office of Science (SC)
- Grant/Contract Number:
- SC0010517; SC0016248
- OSTI ID:
- 1465731
- Alternate ID(s):
- OSTI ID: 1373965
- Journal Information:
- Physics of Plasmas, Journal Name: Physics of Plasmas Journal Issue: 4 Vol. 24; ISSN 1070-664X
- Publisher:
- American Institute of Physics (AIP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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