Works matching Uranus's interior
Results: 21
The interior of Uranus: Thermal profile, bulk composition, and the distribution of rock, water, and hydrogen and helium.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450698
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- Article
A semiclassical model of the interior of Uranus.
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- High Pressure Research, 1990, v. 5, n. 1-6, p. 693, doi. 10.1080/08957959008246229
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- Article
Monte Carlo interior models for Uranus and Neptune.
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- Journal of Geophysical Research. Planets, 1995, v. 100, n. E11, p. 23349, doi. 10.1029/95JE02362
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- Article
Post Voyager comparisons of the interiors of Uranus and Neptune.
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- Geophysical Research Letters, 1990, v. 17, n. 10, p. 1737, doi. 10.1029/GL017i010p01737
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- Article
Atmospheric confinement of jet streams on Uranus and Neptune.
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- Nature, 2013, v. 497, n. 7449, p. 344, doi. 10.1038/nature12131
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- Article
Thermodynamics of diamond formation from hydrocarbon mixtures in planets.
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- Nature Communications, 2023, v. 14, n. 1, p. 1, doi. 10.1038/s41467-023-36841-1
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- Article
Volatile Transport on Ariel and Implications for the Origin and Distribution of Carbon Dioxide on Uranian Moons.
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- Journal of Geophysical Research. Planets, 2024, v. 129, n. 7, p. 1, doi. 10.1029/2024JE008376
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- Article
In Search of Subsurface Oceans Within the Uranian Moons.
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- Journal of Geophysical Research. Planets, 2021, v. 126, n. 12, p. 1, doi. 10.1029/2021JE006956
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- Article
Uranus and Neptune are key to understand planets with hydrogen atmospheres.
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- Experimental Astronomy, 2022, v. 54, n. 2/3, p. 1027, doi. 10.1007/s10686-021-09812-x
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- Article
Laser-driven shock compression of "synthetic planetary mixtures" of water, ethanol, and ammonia.
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- Scientific Reports, 2019, v. 9, n. 1, p. N.PAG, doi. 10.1038/s41598-019-46561-6
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- Article
Interior and Evolution of the Giant Planets.
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- Remote Sensing, 2023, v. 15, n. 3, p. 681, doi. 10.3390/rs15030681
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- Article
Geodigest.
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- Geology Today, 2000, v. 16, n. 1, p. 16, doi. 10.1046/j.1365-2451.2000.1601004.x
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- Article
Does metallic ammonium exist?
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- Nature, 1975, v. 258, n. 5532, p. 222, doi. 10.1038/258222a0
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- Article
Heat and charge transport in H2O at ice-giant conditions from ab initio molecular dynamics simulations.
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- Nature Communications, 2020, v. 11, n. 1, p. 1, doi. 10.1038/s41467-020-17275-5
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- Article
Formation of ammonia–helium compounds at high pressure.
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- Nature Communications, 2020, v. 11, n. 1, p. 1, doi. 10.1038/s41467-020-16835-z
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- Article
Formation and Composition of Planetesimals.
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- Space Science Reviews, 2005, v. 116, n. 1/2, p. 25, doi. 10.1007/s11214-005-1946-2
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- Article
Laser-shock compression of diamond and evidence of a negative-slope melting curve.
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- 2007
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- Letter
Convective-region geometry as the cause of Uranus' and Neptune's unusual magnetic fields.
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- Nature, 2004, v. 428, n. 6979, p. 151, doi. 10.1038/nature02376
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- Article
Diamond formation from methane hydrate under the internal conditions of giant icy planets.
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- Scientific Reports, 2021, v. 11, n. 1, p. 1, doi. 10.1038/s41598-021-87638-5
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- Article
Double superionicity in icy compounds at planetary interior conditions.
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- Nature Communications, 2023, v. 14, n. 1, p. 1, doi. 10.1038/s41467-023-42958-0
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- Article
Liquid methane at extreme temperature and pressure: Implications for models of Uranus and Neptune.
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- JETP Letters, 2013, v. 97, n. 4, p. 184, doi. 10.1134/S0021364013040127
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- Article