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K2-18 b

A temperate sub-Neptune studied through atmospheric spectroscopy.

classification
Sub-Neptune exoplanet
system
K2-18
overview //

K2-18 b is larger than Earth and unlike any Solar System planet. Tentative 2023-2025 JWST hints of dimethyl sulfide (DMS), a potential biosignature gas, remain low-confidence and contested by independent reanalyses; this is a disputed, tentative claim, not a confirmed detection, and atmospheric interpretations more broadly remain model-dependent and actively debated.

technical data //
Class
Sub-Neptune exoplanet
Location / system
K2-18
Distance
About 120 light-years from Earth

Only values with an established scientific consensus are listed. Where a quantity is uncertain or model-dependent, it is discussed in the sections below rather than stated as data.

what we know //
01

Overview (starter entry, expanded review pending)

K2-18 b is larger than Earth and unlike any Solar System planet. Tentative 2023-2025 JWST hints of dimethyl sulfide (DMS), a potential biosignature gas, remain low-confidence and contested by independent reanalyses; this is a disputed, tentative claim, not a confirmed detection, and atmospheric interpretations more broadly remain model-dependent and actively debated.

how do we know? //

Transit photometry and spectroscopy

K2-18 b is not resolved as a surface. Its listed properties come from changes in host-star light or motion; atmospheric claims, where attempted, depend on instrument sensitivity and retrieval models.

methods archive →
open questions //
  • What remains least constrained about K2-18 b?Composition, internal structure, formation history or local environment can require different observations and may remain model-dependent.

Items above are unresolved. Hypotheses are labelled as such and are not presented as confirmed findings.

sources / data //editorial standard →
  1. NASA/IPAC // verified 28 September 2026

    NASA Exoplanet Archive ↗

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