nous of main sequence stars, having masses 0.1-0.5 times the mass of the Sun. The habitable zones around such stars Planets within the habitable zones of M dwarfs are likely to are therefore very close, being typically between 0.03 and be synchronous rotators; in other words, one side is permanently
Simulations of Superrotation on Slowly Rotating Planets: Sensitivity to Rotation and Initial Condition
β Scribed by Anthony D. Del Genio; Wei Zhou
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 393 KB
- Volume
- 120
- Category
- Article
- ISSN
- 0019-1035
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