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Conditions for the onset of plate tectonics on terrestrial planets and moons

✍ Scribed by C. O'Neill; A.M. Jellinek; A. Lenardic

Book ID
116452770
Publisher
Elsevier Science
Year
2007
Tongue
English
Weight
793 KB
Volume
261
Category
Article
ISSN
0012-821X

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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