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Nature of the ocean beneath K2-18 b’s H2-rich atmosphere is unknown

Determine the physical nature of the ocean hypothesized beneath K2-18 b’s hydrogen-rich atmosphere, including whether a liquid water ocean exists and, if so, characterize its phase state and composition to evaluate potential habitability.

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Background

The atmospheric composition retrieved for K2-18 b supports Hycean-like conditions and suggests a substantial interior water inventory. In Hycean scenarios, an ocean lies beneath an H2-rich atmosphere, but its properties cannot be directly inferred from current transmission spectra.

Establishing the ocean’s nature is central to assessing K2-18 b’s habitability, as liquid water requires specific thermal and radiative conditions. The authors note that, despite atmospheric evidence, the existence, phase, and characteristics of a putative ocean remain undetermined.

References

While the atmospheric composition is consistent with predictions for hycean conditions and a large water inventory in the interior, the nature of the possible ocean beneath the H$_2$-rich atmosphere is unknown.

New Constraints on DMS and DMDS in the Atmosphere of K2-18 b from JWST MIRI (2504.12267 - Madhusudhan et al., 16 Apr 2025) in Section 1 (Introduction)