SkyTracko

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

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.