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) |
|---|---|
| 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