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Ocean Tides On Asynchronously Rotating Planets Orbiting Low-mass Stars - Astrobiology

Summary by astrobiology.com
Planets in the liquid-water habitable zone of low-mass stars experience large tidal forces, 103 to 104 times those on Earth, due to the small distance between the habitable zone and the host stars. Therefore, interior solid tides, ocean tides and atmospheric tides on these planets could be much stronger than that on Earth, but rare […] The post Ocean Tides On Asynchronously Rotating Planets Orbiting Low-mass Stars appeared first on Astrobiology.
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astrobiology.com broke the news in on Saturday, July 12, 2025.
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