Host star — K2-72
- Spectral type
- —
- Temperature
- 3,360 K
- Radius
- 0.33 R☉
- Mass
- 0.27 M☉
- Luminosity
- 0.015 L☉
- Distance
- 66.4 pc (217 ly)
Very cool — a faint red dwarf.
Orbits K2-72 · 217 light-years from Earth
K2-72 e is a rocky world roughly 1.3 times Earth's radius with a mass of 2.21 Earth masses, orbiting a cool, dim red dwarf star 217 light-years away. Its equilibrium temperature of 286 Kelvin—just above the freezing point of water—places it squarely in the habitable zone, making it one of the more promising candidates for potentially hosting liquid water on its surface. The planet completes an orbit every 24.2 days at a distance of 0.106 AU, similar to Venus's proximity to our Sun but receiving far less energy because its host star is so much cooler and dimmer than ours. With a density of 5.66 grams per cubic centimeter, slightly denser than Earth, the planet likely has a substantial iron core and rocky composition. The main unknowns are whether K2-72 e has retained an atmosphere, what its surface conditions actually are, and whether the modest eccentricity of 0.11 causes significant climate swings. Discovered in 2016 via the transit method and boasting a habitability score of 81, this world deserves closer study to constrain its atmospheric composition and surface environment.
K2-72 e 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.
With an equilibrium temperature around 13°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 24 days makes the year 15.1× 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.
Very cool — a faint 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.
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.