On the orbital decay of the gas giant Kepler-1658b

15. 11. 2023 (accepted)

On the orbital decay of the gas giant Kepler-1658b

Star system: Kepler-1658 | Distance from the Sun: 2629 light years

Gas giant Kepler-1658 b is slowly spiraling inward due to tidal interactions with its host star. The observed rate of orbital decay cannot be explained by tidal dissipation in the star alone, but it can be explained if the planet rotates non-synchronously

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On the orbital decay of the gas giant Kepler-1658b external link

Stars mentioned

Kepler-1658

Subgiant

mass: 1.45 M☉

radius: 3 R☉

distance: 2629 ly

stars in the system: 3

exoplanets: 0

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