The DOI matches its Crossref record; 56 of the 56 references it cites were found in a registry or an index.
Interiors of Giant Planets Inside and Outside the Solar System
Abstract
An understanding of the structure and composition of the giant planets is rapidly evolving because of (i) high-pressure experiments with the ability to study metallic hydrogen and define the properties of its equation of state and (ii) spectroscopic and in situ measurements made by telescopes and satellites that allow an accurate determination of the chemical composition of the deep atmospheres of the giant planets. However, the total amount of heavy elements that Jupiter, Saturn, Uranus, and Neptune contain remains poorly constrained. The discovery of extrasolar giant planets with masses ranging from that of Saturn to a few times the mass of Jupiter opens up new possibilities for understanding planet composition and formation. Evolutionary models predict that gaseous extrasolar giant planets should have a variety of atmospheric temperatures and chemical compositions, but the radii are estimated to be close to that of Jupiter (between 0.9 and 1.7 Jupiter radii), provided that they contain mostly hydrogen and helium.
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Cites
Abundances of the elements: Meteoritic and solar
Anders, E., & Grevesse, N. (1989) · Geochimica et Cosmochimica Acta · doi:10.1016/0016-7037(89)90286-x · Cited by 10,422
A Jupiter-mass companion to a solar-type star
Mayor, M., & Queloz, D. (1995) · Nature · doi:10.1038/378355a0 · Cited by 4,111
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
Pollack, J. B., Hubickyj, O., Bodenheimer, P., Lissauer, J. J., Podolak, M., & Greenzweig, Y. (1996) · Icarus · doi:10.1006/icar.1996.0190 · Cited by 3,127
A Nongray Theory of Extrasolar Giant Planets and Brown Dwarfs
Burrows, A., Marley, M., Hubbard, W. B., Lunine, J. I., Guillot, T., Saumon, D., Freedman, R., Sudarsky, D., & Sharp, C. (1997) · The Astrophysical Journal · doi:10.1086/305002 · Cited by 1,390
Self-citationAn Equation of State for Low-Mass Stars and Giant Planets
Saumon, D., Chabrier, G., & van Horn, H. M. (1995) · The Astrophysical Journal Supplement Series · doi:10.1086/192204 · Cited by 1,274
Orbital migration of the planetary companion of 51 Pegasi to its present location
Lin, D. N. C., Bodenheimer, P., & Richardson, D. C. (1996) · Nature · doi:10.1038/380606a0 · Cited by 1,235
Low-temperature Rosseland opacities
Alexander, D. R., & Ferguson, J. W. (1994) · The Astrophysical Journal · doi:10.1086/175039 · Cited by 1,161
Suess, H. E., & Urey, H. C. (1956) · Reviews of Modern Physics · doi:10.1103/revmodphys.28.53 · Cited by 1,025
Solar models with helium and heavy-element diffusion
Bahcall, J. N., Pinsonneault, M. H., & Wasserburg, G. J. (1995) · Reviews of Modern Physics · doi:10.1103/revmodphys.67.781 · Cited by 873
Metallization of Fluid Molecular Hydrogen at 140 GPa (1.4 Mbar)
Weir, S. T., Mitchell, A. C., & Nellis, W. J. (1996) · Physical Review Letters · doi:10.1103/physrevlett.76.1860 · Cited by 756
Cited by
The interiors of giant planets: Models and outstanding questions.
Guillot, T. (2005) · Annual Review of Earth and Planetary Sciences · doi:10.1146/annurev.earth.32.101802.120325 · Cited by 524
Self-citationColloquium : Nonlinear collective interactions in quantum plasmas with degenerate electron fluids
Shukla, P. K., & Eliasson, B. (2011) · Reviews of Modern Physics · doi:10.1103/revmodphys.83.885 · Cited by 477
The metal-rich nature of stars with planets
Santos, N. C., Israelian, G., & Mayor, M. (2001) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20010648 · Cited by 477
A chemical survey of exoplanets with ARIEL
Tinetti, G., Drossart, P., Eccleston, P., Hartogh, P., Heske, A., Leconte, J., Micela, G., Ollivier, M., Pilbratt, G., Puig, L., et al. (2018) · Experimental Astronomy · doi:10.1007/s10686-018-9598-x · Cited by 445
Stevenson, D. J. (2003) · Earth and Planetary Science Letters · doi:10.1016/s0012-821x(02)01126-3 · Cited by 434
Metadata
- Authors
- Guillot, T.
- Venue
- Science
- Published
- 1999-10
- Volume
- 286
- Issue
- 5437
- Pages
- 72-77
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2072697696
- Cited by
- 566
- References
- 56
- FWCI
- 10.48
- Type
- journal article
- Language
- en
- Open access
- closed
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
