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Kritikon Litterarum, ISSN 0340-9767, 01/2010, Volume 37, Issue 3-4
Journal Article
Nature, ISSN 0028-0836, 08/2019, Volume 572, Issue 7769, pp. 315 - 317
[...]the envelope should be poor in heavy elements. In particular, it needs to be coupled to realistic scenarios for the formation of the Solar System8.... 
Earth | Heavy elements | Jupiter | Solar systems | Extrasolar planets | Embryos
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 09/2010, Volume 520, Issue 18, p. A27
Journal Article
NATURE, ISSN 0028-0836, 08/2019, Volume 572, Issue 7769, pp. 315 - 317
Simulations suggest that Jupiter's dilute core might be the result of a collision between the planet and a Uranus-mass planetary embryo. This finding indicates... 
MULTIDISCIPLINARY SCIENCES | Jupiter | Planets | Earth | Origin | Craters | Jupiter (Planet) | Observations | Structure | Natural history | Core
Journal Article
Science, ISSN 0036-8075, 10/1999, Volume 286, Issue 5437, pp. 72 - 77
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... 
Heavy elements | Jupiter | Planets | Reviews | Saturn | Hydrogen | Average linear density | Gas giants | Chemical composition | Helium | Planetary orbits | Temperature | Solar System | Atmosphere | Astronomical Phenomena | Evolution, Planetary | Metals, Heavy | Extraterrestrial Environment | Pressure | Astronomy | Solar system | Research | Observations | Universe | Astrophysics | Solar systems
Journal Article
2006, ISBN 9783540292166, xii, 451
Book
Astronomy & Astrophysics, ISSN 0004-6361, 02/2018, Volume 610, p. L14
Recent formation and structure models of Jupiter suggest that the planet can have composition gradients and not be fully convective (adiabatic). This... 
Jupiter | Adiabatic flow | Atmospheric models | Planetary evolution | Jupiter atmosphere | Evolution | Planetary composition | Convection | Physics | Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 472, Issue 3, pp. 2590 - 2607
Journal Article
Astrophysical Journal, ISSN 0004-637X, 04/2013, Volume 767, Issue 2, pp. 1 - 7
The accurate determination of Saturn's gravitational coefficients by Cassini could provide tighter constraints on Saturn's internal structure. Also,... 
Heavy elements | Cassini mission | Uncertainty | Gravitation | Hydrostatics | Saturn | Phase separation | Wind velocity | Helium
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2014, Volume 562, pp. A133 - np
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 06/2010, Volume 516, Issue 2, p. A20
Context. The discovery of CoRoT-7b, a planet of a radius 1.68 +/- 0.09 R-circle plus, a mass 4.8 +/- 0.8 M-circle plus, and an orbital period of 0.854 days... 
Planets and satellites: individual: CoRoT-7b | planets and satellites: individual: CoRoT-7b | MIGRATION | HOT JUPITERS | HD 209458B | MODELS | ATMOSPHERIC ESCAPE | GIANT PLANETS | ASTRONOMY & ASTROPHYSICS | MASS | HIGH-PRESSURE EXPERIMENTS | CHEMISTRY | LOWER MANTLE | Physics - Earth and Planetary Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 04/2013, Volume 767, Issue 2, p. 113
The accurate determination of Saturn's gravitational coefficients by Cassini could provide tighter constraints on Saturn's internal structure. Also,... 
planets and satellites: interiors | planets and satellites: composition | planets and satellites: individual (Jupiter, Saturn) | PHASE-SEPARATION | GIANT PLANETS | FIELD | ASTRONOMY & ASTROPHYSICS | ATMOSPHERES | JUPITER | ROTATION | SHAPE | ECLIPSE | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | EQUILIBRIUM | MASS | SATELLITES | HELIUM | SATURN PLANET
Journal Article