Ocean Tides on Asynchronously Rotating Planets Orbiting Low-mass Stars
Planets in the liquid-water habitable zone of low-mass stars experience large tidal forces, 10 ^3 –10 ^4 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 s...
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| Main Authors: | , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
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| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adeb83 |
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