Host star — TOI-715
- Spectral type
- M4
- Temperature
- 3,075 K
- Radius
- 0.24 R☉
- Mass
- 0.23 M☉
- Luminosity
- 0.005 L☉
- Distance
- 42.4 pc (138 ly)
Red dwarf — the most common type of star. Cool and small.
Very cool — a faint red dwarf.
Orbits TOI-715 · 138 light-years from Earth
TOI-715 b is a super-Earth roughly 1.55 times Earth's radius and three times Earth's mass, orbiting an M-dwarf star 138 light-years away. Its equilibrium temperature of 234 Kelvin—roughly 39 Kelvin colder than Earth—places it in the habitable zone of its small, cool host star, where liquid water could theoretically persist on the surface. The planet's density of 4.46 grams per cubic centimeter suggests a rocky composition similar to Earth's. However, serious uncertainties remain: we do not know whether TOI-715 b has retained an atmosphere capable of trapping heat, or whether it has a magnetic field to shield against stellar wind erosion. Its 19.3-day orbit around a low-mass star may also increase the likelihood of tidal locking, which could create extreme temperature swings between day and night sides. With a habitability score of 83 out of 100, this world ranks among the most promising exoplanet candidates for habitability, making it a prime target for future atmospheric characterization with next-generation telescopes.
TOI-715 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 1.3g — noticeably heavier what you're used to on Earth.
At -39°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 19 days makes the year 18.9× 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.
Red dwarf — the most common type of star. Cool and small.
Very cool — a faint red dwarf.
Detected by measuring the tiny dip in starlight as the planet crosses in front of its star.
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.