Abstract
We present the case for liquid models of Jupiter and Saturn. We then discuss the information which can be obtained about their interior structure from a knowledge of their gravitational moments, and we discuss the nature of presently available data and data which will be necessary to fully exploit future results.
Original language | English (US) |
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Pages (from-to) | 147-151 |
Number of pages | 5 |
Journal | Icarus |
Volume | 21 |
Issue number | 2 |
DOIs | |
State | Published - Feb 1974 |
Externally published | Yes |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science