Host star — Kepler-442
- Spectral type
- —
- Temperature
- 4,402 K
- Radius
- 0.60 R☉
- Mass
- 0.61 M☉
- Luminosity
- 0.117 L☉
- Distance
- 366.0 pc (1,194 ly)
Cooler than the Sun. Orange or red dwarf.
Orbits Kepler-442 · 1,194 light-years from Earth
Kepler-442 b is a rocky world, potentially similar in composition to Earth or Mars — a solid surface you could, in theory, stand on.
Surface gravity is about 1.3g — noticeably heavier what you're used to on Earth.
At -32°C, this world is cold — similar to Earth's polar regions or the surface of Mars. Water would likely be frozen, but subsurface liquid isn't ruled out.
An orbital period of 112 days makes the year 3.3× 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.
Cooler than the Sun. Orange or red dwarf.
Detected by measuring the tiny dip in starlight as the planet crosses in front of its star.
Mildly elliptical — similar to most Solar System planets.
Rocky composition likely. Earth is 5.51 g/cm³.
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.