Host star — Kepler-62
- Spectral type
- K2 V
- Temperature
- 4,925 K
- Radius
- 0.64 R☉
- Mass
- 0.69 M☉
- Luminosity
- 0.210 L☉
- Distance
- 300.9 pc (981 ly)
Orange dwarf, cooler and longer-lived than the Sun.
Cooler than the Sun. Orange or red dwarf.
Orbits Kepler-62 · 981 light-years from Earth
Kepler-62 e 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.
At 13.9g, gravity is crushing by Earth standards. Walking would feel like carrying a 902 kg backpack permanently.
With an equilibrium temperature around -3°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 122 days makes the year 3.0× 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.
Orange dwarf, cooler and longer-lived than the Sun.
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.
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.