Interiors of the giant planets

Research output: Contribution to journalArticle

109 Scopus citations

Abstract

Unlike the terrestrial planets, the giant planets-Jupiter, Saturn, Uranus, and Neptune-have retained large amounts of the carbon, nitrogen, and oxygen compounds that were present in their zone of formation. A smaller fraction of the available hydrogen and helium was retained. The distribution and relative amounts of these components in the interiors of the Jovian planets can be inferred from theoretical and experimental data on equations of state and from the planets' hydrostatic equilibrium response to rotation.

Original languageEnglish (US)
Pages (from-to)145-149
Number of pages5
JournalScience
Volume214
Issue number4517
DOIs
StatePublished - Jan 1 1981

ASJC Scopus subject areas

  • General

Fingerprint Dive into the research topics of 'Interiors of the giant planets'. Together they form a unique fingerprint.

  • Cite this