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Habitability of Enceladus: Planetary Conditions for Life

โœ Scribed by Christopher D. Parkinson; Mao-Chang Liang; Yuk L. Yung; Joseph L. Kirschivnk

Book ID
106489928
Publisher
Springer Netherlands
Year
2008
Tongue
English
Weight
303 KB
Volume
38
Category
Article
ISSN
1573-0875

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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