Host star — K2-332
- Spectral type
- —
- Temperature
- 3,315 K
- Radius
- 0.28 R☉
- Mass
- 0.27 M☉
- Luminosity
- 0.009 L☉
- Distance
- 123.2 pc (402 ly)
Very cool — a faint red dwarf.
Orbits K2-332 · 402 light-years from Earth
K2-332 b is a super-Earth — larger than our planet but likely still rocky or ice-rich. Whether it has a thin atmosphere like Mars or a crushing one like Venus remains unknown.
Surface gravity is about 1.1g — noticeably heavier what you're used to on Earth.
With an equilibrium temperature around -7°C, this planet sits in the temperature range where liquid water could potentially exist on the surface — a key ingredient for life as we know it.
An orbital period of 18 days makes the year 20.6× shorter than Earth's. You'd celebrate your birthday more often here.
Logarithmic bars so Jupiter-class planets fit the same scale as Earth-size worlds.
Very cool — a faint red dwarf.
Detected by measuring the tiny dip in starlight as the planet crosses in front of its star.
Low density — probably icy or gas-rich.
A transit photometer watches a star nonstop and measures its brightness to ~0.01%. When a planet passes between us and the star, the star dims briefly — the deeper the dip, the bigger the planet. This is how Kepler and TESS found most known exoplanets.
Where this host star sits among … exoplanet host stars. The main sequence band runs diagonally — giants and supergiants sit above, white dwarfs below.
ESI combines radius similarity and equilibrium temperature similarity. Earth = 100. Mars ≈ 73. Venus ≈ 44. This score reflects two physical parameters only — not atmosphere, water, or magnetic field.