Characterization of the regimes of hydrodynamic escape from low-mass exoplanets

LEO's

Nature Astronomy, Published online: 09 May 2024; doi:10.1038/s41550-024-02269-w

An updated Jeans parameter that includes tidal forces can distinguish the various driving forces, both exogenous and endogenous, of atmospheric escape from low-mass close-in exoplanets. Depending on its value, escape can be dominated by tidal forces, extreme ultraviolet stellar radiation or a combination of the two.

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