Host star — Kepler-61
- Spectral type
- K7 V
- Temperature
- 4,017 K
- Radius
- 0.62 R☉
- Mass
- 0.64 M☉
- Luminosity
- 0.107 L☉
- Distance
- 335.1 pc (1,093 ly)
Orange dwarf, cooler and longer-lived than the Sun.
Cooler than the Sun. Orange or red dwarf.
Orbits Kepler-61 · 1,093 light-years from Earth
Kepler-61 b orbits a cool K-type star about 1,090 light-years away, and its equilibrium temperature sits at a temperate 273 Kelvin—right at Earth's freezing point. The planet itself is a super-Earth with 2.15 times our planet's radius and 5.27 Earth masses, giving it a density of 2.91 g/cm³ that suggests a rocky composition with a modest atmosphere. Its 59.9-day orbit places it within the habitable zone, though the moderate eccentricity of 0.25 means temperature swings across its year. The major caveat is distance: at over a thousand light-years away, we cannot directly observe its atmosphere or surface conditions, leaving open critical questions about whether any water persists as liquid, whether toxic volcanic outgassing dominates, or whether the atmosphere has escaped entirely. The habitability score of 80 reflects these tantalizing indicators, but ground truth requires future atmospheric spectroscopy that remains decades away. Kepler-61 b's discovery via the transit method in 2013 makes it an enduring benchmark for how temperate super-Earths challenge our definitions of habitability.
Kepler-61 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 0°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 60 days makes the year 6.1× 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.
Noticeably elliptical. Seasons (if any) would vary in intensity.
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.