Properties of hydrogen, helium, and silicon dioxide mixtures in giant planet interiors
- 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 Office of Science (SC)
- Grant/Contract Number:
- SC0010517; SC0016248
- OSTI ID:
- 1465731
- Alternate ID(s):
- OSTI ID: 1373965
- Journal Information:
- Physics of Plasmas, Vol. 24, Issue 4; ISSN 1070-664X
- Publisher:
- American Institute of Physics (AIP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Cited by: 26 works
Citation information provided by
Web of Science
Web of Science
Similar Records
AB INITIO EQUATION OF STATE FOR HYDROGEN-HELIUM MIXTURES WITH RECALIBRATION OF THE GIANT-PLANET MASS-RADIUS RELATION
Evidence of hydrogen-helium immiscibility at Jupiter-interior conditions
THE PROPERTIES OF HEAVY ELEMENTS IN GIANT PLANET ENVELOPES
Journal Article
·
Tue Sep 10 00:00:00 EDT 2013
· Astrophysical Journal
·
OSTI ID:1465731
Evidence of hydrogen-helium immiscibility at Jupiter-interior conditions
Journal Article
·
Wed May 26 00:00:00 EDT 2021
· Nature (London)
·
OSTI ID:1465731
+5 more
THE PROPERTIES OF HEAVY ELEMENTS IN GIANT PLANET ENVELOPES
Journal Article
·
Tue Sep 20 00:00:00 EDT 2016
· Astrophysical Journal
·
OSTI ID:1465731