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TOI-2257 b

Orbits TOI-2257 · 188 light-years from Earth

Super-EarthTransit2021ESI 87 · Very Earth-like
Earth2.19 R⊕
Radius
2.19×
Earth
Mass
5.5×
Earth
Year
35d
Temp
256 K
-17°C
Gravity
1.1×
Earth
Distance
188
ly

Could life exist here?

AI analysis

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.

What it would be like

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.

Earth comparison

Logarithmic bars so Jupiter-class planets fit the same scale as Earth-size worlds.

Radius2.19R⊕
1/25×Earth = 125×
Mass5.45M⊕
1/10000×Earth = 110000×
Surface gravity1.13g
1/100×Earth = 1100×
Equilibrium temp256 K(-17°C)
0 KEarth 255 K2500 K

Side-by-side with Earth

Radius
2.19 R⊕
1.00 R⊕
Mass
5.45 M⊕
1.00 M⊕
Surface gravity
1.13g
1.00g
Year length
35.19 days
365.25 days
Eq. temperature
256 K (-17°C)
255 K (−18°C)
Orbital eccentricity
0.4960
0.0167
Semi-major axis
0.145 AU
1.000 AU

Temperature in context

Liquid N₂Mars avgEarth eq.Earth sfc.Boiling H₂OVenus

Host star — TOI-2257

Spectral type
M3

Red dwarf — the most common type of star. Cool and small.

Temperature
3,430 K

Very cool — a faint red dwarf.

Radius
0.31 R☉
Mass
0.33 M☉
Luminosity
0.014 L☉
Distance
57.8 pc (188 ly)

Discovery & orbit

Method
Transit

Detected by measuring the tiny dip in starlight as the planet crosses in front of its star.

Year
2021
Facility
Transiting Exoplanet Survey Satellite (TESS)
Semi-major axis
0.1450 AU
Period
35.19 days
Eccentricity
0.4960

Highly eccentric — temperatures would swing wildly between closest and farthest approach.

Density
2.84 g/cm³

Low density — probably icy or gas-rich.

Discovered via · Transit

Tiny dip in starlight as the planet crosses in front of its star

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.

Overall share
~75% of all confirmed worlds
Best for
Earth-to-Neptune-sized planets on short orbits

Orbital Animation

TOI-2257TOI-2257 bOrbitHabitable zone
Drag to rotate · scroll to zoom
Semi-major axis: 0.145 AUEccentricity: 0.4960Period: 35.2 days

Hertzsprung–Russell Diagram

Where this host star sits among exoplanet host stars. The main sequence band runs diagonally — giants and supergiants sit above, white dwarfs below.

OBAFGKMCurrent star

How far is 188 light-years?

  • A light beam leaving Earth right now would arrive in 188 years.
  • At Voyager 1's speed (17 km/s), the trip would take approximately 3.3 million years.
  • A radio signal sent today would arrive in 188.5 years — and the reply wouldn't come back for twice that.

Earth Similarity Index

87/100
0 — Nothing like Earth100 — Identical to Earth

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.