Abstract
A theory which is almost fully analytic is used to investigate Jupiter's cooling rate. We find that a simple model of contraction with adiabatic interior structure gives a total cooling time to the present which is in good agreement with the age of the solar system. The interplay between the surface condition and the cooling rate is exhibited and discussed. The current rate of change of the effective temperature is calculated to be -1°K/0.145×109 yr. Discrepancies with fully numerical investigations of the Jovian age and cooling rate are noted.
Original language | English (US) |
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Pages (from-to) | 305-310 |
Number of pages | 6 |
Journal | Icarus |
Volume | 30 |
Issue number | 2 |
DOIs | |
State | Published - Feb 1977 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science