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Corkee t1_itgo9i0 wrote

One more point against habitable planets around M class stars is that they are likely tidally locked due to the close orbits around the star - even in the Goldilocks zone. Maybe the biggest M class star could have a non-tidally locked planet in its GZ, but that would have to be a young star I guess.

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ErrorlessQuaak t1_itgrhxe wrote

Planets orbiting m dwarfs are not necessarily tidally locked. Spin-orbit resonances likely play a big role in compact multi planet systems.

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