On the structure and composition of Uranus and Neptune

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Models, Neptune (Planet), Planetary Composition, Planetary Structure, Uranus (Planet), Abundance, Helium, Hydrogen, Ice, Planetary Rotation, Rocks, Planets, Uranus, Neptune, Structure, Composition, Models, Interior, Rocks, Ice, Hydrogen, Helium, Density, Quadrapole Moments, Data, Rotation, Oblateness, Period, Cooling, Theoretical Studies

Scientific paper

A series of models is presented of Uranus and Neptune in which the relative amounts of (1) rock, (2) ices, and (3) hydrogen and helium are allowed to vary. By fitting the density and the gravitational quadrupole moment, the model composition can be determined. Because of the ambiguity in the rotation periods of these planets, several possible models are presented and discussed.

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