Host star — TOI-2257
- Spectral type
- M3
- Temperature
- 3,430 K
- Radius
- 0.31 R☉
- Mass
- 0.33 M☉
- Luminosity
- 0.014 L☉
- Distance
- 57.8 pc (188 ly)
Red dwarf — the most common type of star. Cool and small.
Very cool — a faint red dwarf.
Orbits TOI-2257 · 188 light-years from Earth
TOI-2257 b is a super-Earth with 2.19 times Earth's radius and 5.45 Earth masses, orbiting a small, cool M3 star every 35.2 days at a distance of 0.145 AU. Its equilibrium temperature of 256 Kelvin sits well below Earth's average of 288 K—cold enough that the planet likely receives less stellar energy than our home world does. However, the planet's notably high density of 2.84 g/cm³ suggests a rocky composition with a substantial iron core, making it genuinely terrestrial rather than a gaseous world. The most significant complication is the planet's highly eccentric orbit of 0.496, which means its distance from the star swings dramatically, creating potentially extreme seasonal variations in temperature and radiation that could destabilize any developing biosphere. Its habitability score of 87 out of 100 reflects these trade-offs—a solid rocky world in a plausible orbital zone around its host, but with climatic volatility that remains poorly understood. TOI-2257 b's combination of substantial mass, genuine terrestrial character, and moderate distance from Earth (188 light-years) make it an exceptional target for atmospheric characterization with future telescopes.
TOI-2257 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 -17°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 35 days makes the year 10.4× 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.
Highly eccentric — temperatures would swing wildly between closest and farthest approach.
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.