Host star — Kepler-283
- Spectral type
- —
- Temperature
- 4,351 K
- Radius
- 0.57 R☉
- Mass
- 0.60 M☉
- Luminosity
- 0.104 L☉
- Distance
- 468.1 pc (1,527 ly)
Cooler than the Sun. Orange or red dwarf.
Orbits Kepler-283 · 1,527 light-years from Earth
Kepler-283 c is a super-Earth roughly 1.82 times Earth's radius with a mass of 3.97 Earth masses, orbiting a cool red dwarf star every 92.7 days at a distance of 0.341 AU. Its equilibrium temperature of 240 Kelvin places it firmly in the frozen zone—substantially colder than Earth's average of 288 Kelvin, though potentially within habitable range if an atmosphere with sufficient greenhouse gases were present. The planet's density of 3.62 grams per cubic centimeter suggests a rocky composition, and its circular orbit offers orbital stability. The major caveat is distance: at 1,530 light-years away, Kepler-283 c remains observationally inaccessible for atmospheric characterization with current technology. Its habitability score of 83 reflects reasonable equilibrium conditions, but we cannot yet determine whether it retains an atmosphere, possesses liquid water, or harbors any geological processes necessary for life. This well-characterized mid-sized world from Kepler's original mission exemplifies the many potentially habitable worlds waiting for future generations of space telescopes to study directly.
Kepler-283 c 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 1.2g — noticeably heavier what you're used to on Earth.
At -33°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 93 days makes the year 3.9× 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.
Nearly circular orbit.
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.