Host star — Kepler-438
- Spectral type
- —
- Temperature
- 3,748 K
- Radius
- 0.52 R☉
- Mass
- 0.54 M☉
- Luminosity
- 0.044 L☉
- Distance
- 195.9 pc (639 ly)
Cooler than the Sun. Orange or red dwarf.
Orbits Kepler-438 · 639 light-years from Earth
Kepler-438 b is a rocky world just 12 percent larger than Earth, orbiting a cool red dwarf star 639 light-years away. With an equilibrium temperature of 288 Kelvin—nearly identical to Earth's average surface temperature—and a nearly circular orbit at 0.166 astronomical units from its host star, this planet sits squarely in the habitable zone where liquid water could exist on its surface. Its mass of 1.46 Earth masses and density of 5.71 grams per cubic centimeter suggest a terrestrial composition similar to our own planet, though we cannot yet know if it has an atmosphere to retain heat or protect against radiation. The main unknowns are whether Kepler-438 b has retained a magnetic field and atmospheric shield over billions of years in close proximity to its star, and whether its 35.2-day year allows for climate stability. This planet achieved an exceptional habitability score of 83 out of 100, making it one of the most Earth-like worlds discovered to date via the transit method.
Kepler-438 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 1.2g — noticeably heavier what you're used to on Earth.
With an equilibrium temperature around 15°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 35 days makes the year 10.4× 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.