Fast rotating giant planets such as Jupiter and Saturn possess alternate prograde and retrograde zonal winds which are stable over long periods of time. We consider a compressible model of convection in a spherical shell with rapid rotation, using the anelastic approximation, to explore the paramete
Survival of the Jovian planets with the Sun a Red Giant
β Scribed by Samuel C. Vila
- Publisher
- Springer Netherlands
- Year
- 1985
- Tongue
- English
- Weight
- 121 KB
- Volume
- 33
- Category
- Article
- ISSN
- 1573-0794
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β¦ Synopsis
The survival of the Jovian planets and their satellites as the Sun becomes a Red Giant is considered. It is found that the Jovian planets would not lose any matter -not even hydrogen. The satellites would lose their gaseous or volatile envelopes. Their rocky cores would resist melting and survive. Both the planets and the satellites would be unsuited to support human life.
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