Abstract
We present an efficient numerical self-consistent field method for calculating a gravitational model of a rotating liquid planet to spherical harmonic degree ∼30 and a precision ∼10-12 in the external gravity field. The method's accuracy is validated by comparing results, for Jupiter rotation parameters, with the exact Maclaurin constant-density solution. The method can be generalized to non-constant density.
| Original language | English (US) |
|---|---|
| Article number | L15 |
| Journal | Astrophysical Journal Letters |
| Volume | 756 |
| Issue number | 1 |
| DOIs | |
| State | Published - 2012 |
Keywords
- planets and satellites: interiors
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science