Published August 12, 2008
| Published
Journal Article
Open
Metallic helium in massive planets
- Creators
-
Stevenson, David J.
Chicago
Abstract
In this issue of PNAS, Stixrude and Jeanloz (4) show that band closure in pure helium occurs at lower pressures than previously thought, provided the effect of high temperatures is taken into account. This suggests that helium behaves as a metal, at least at the highest pressures encountered in Jupiter and perhaps over a wider range of pressures in the many, often much hotter, planets of Jupiter's mass and larger that are now evidently common in the universe (5). The full thermodynamic and transport properties of the relevant mixtures cannot be deduced from the behavior of the end members (pure hydrogen and pure helium) and are therefore an area of ongoing research.
Additional Information
© 2008 by the National Academy of Sciences. PNAS published ahead of print August 6, 2008, doi:10.1073/pnas.0806430105. Author contributions: D.J.S. wrote the paper. The author declares no conflict of interest. See companion article PNAS 103:11071.Attached Files
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Additional details
- PMCID
- PMC2516209
- Eprint ID
- 11362
- Resolver ID
- CaltechAUTHORS:STEpnas08
- Created
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2008-08-07Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)