
K2-18
K2-18 is a red dwarf 124 light-years away in Leo, host to K2-18 b — a habitable-zone sub-Neptune at the centre of the most-watched question in exoplanet science: whether its atmosphere holds water, and possibly a chemical fingerprint of life.
Key facts
Science
Classification
- Type
- Single red-dwarf system
- Central star
- K2-18 — M2.5V red dwarf, ~3457 K, 0.36 M☉
Planets
- Transiting (HZ)
- K2-18 b · the famous biosignature sub-Neptune
- Radial-velocity (inner)
- K2-18 c — shown, disputed
Distance
- Distance
- 124 light-years · in Leo, the Lion
How we know
- Note
- K2-18 b is confirmed and transiting, so its size and density are measured (NASA Exoplanet Archive, checked 2026-07-07). Water vapour (2019) is a real detection; the 2023 hint of dimethyl sulphide (a possible life gas) is CONTESTED and unconfirmed — no claim about life is established. The inner world K2-18 c is a radial-velocity detection (minimum mass, no transit → no measured size): its 9-day signal was disputed as stellar activity in 2018 but independently recovered in 2019 and 2022, though the Archive still flags it controversial — so it IS shown, plainly labelled, as the hot inner sibling (not the biosignature planet). Placed at its real position, 124 light-years away.
Discovery & history
- Name
- A designation from NASA's K2 mission (the repurposed Kepler telescope), the 18th planet-hosting star it confirmed; the star has no proper name.
K2-18 b was found transiting by NASA's K2 mission in 2015. In 2019 Hubble detected water vapour in its atmosphere — the first for a habitable-zone planet — and from 2023 JWST reported carbon-bearing molecules and a contested hint of dimethyl sulphide (DMS), a gas made only by life on Earth. The claim remains hotly debated. A second planet, K2-18 c, was detected by radial velocity in 2017 — challenged as stellar activity in 2018, then independently recovered (2019, 2022), though the NASA Exoplanet Archive still flags it controversial.
Images


Images from open archives · credit shown per image