Create your free account

Enter your email and we'll send a 6-digit code — no password needed.
We only keep your email and the username you choose. We never share or sell your email, and we don't send marketing — we use it only to email you a sign-in code. Read our privacy policy.
Entering orbit…
Habitability
6/ 100
Uninhabitable
TOI-2202 b rendered in TerraForge from its measured mass, orbit and star

TOI-2202 b

Also written TOI-2202b, TOI 2202b, TOI 2202 b

Gas Giant769 light years awayFound 2021
Mass
287.00 × Earth
Radius
11.00 × Earth
Gravity
2.37 g
Surface (est.)
715 K
Year
11.9 days
From Earth
770 ly
Mass
287.00 × Earth
Radius
11.00 × Earth
Gravity
2.37 g
Surface (est.)
715 K
Year
11.9 days
From Earth
770 ly

TOI-2202 system

Type
K-type (Orange)
Spectral type
K8 V
Temperature
5,169 K
Radius
0.808 ☉
Mass
0.841 ☉
Planets
2
Luminosity
0.397 ☉

Published by the NASA Exoplanet Archive. This world’s temperature and habitability score are computed from this star’s measured luminosity, not from a stand-in for its class.

Habitable zone

Star and planets drawn to scale: the star is 8.0 times as wide as TOI-2202 b, so only its edge is in view. Orbits spaced as in the star system view.

TOI-2202 b, from the NASA Exoplanet Archive (found 2021). Measured: 287 Earth masses, 0.0956 AU, a 5169 K K-type star. Composition inferred from a mass of 287 Earths, which is giant territory whatever its 0.22x density suggests, with a day locked to its 11.9-day year, as anything orbiting this close would be.

Surface. No solid surface - thick gaseous envelope with possible rocky core deep within

Gas Giant
Magnetic FieldExtreme Activity
TOI-2202 b has 86.0% hydrogen and helium, combined with a mass of 287.0x Earth, which exceeds the gas giant threshold.
Gas giants form when massive cores capture enormous atmospheres of light gases. They typically form beyond the 'frost line' where volatiles can condense.
Classification Criteria:
✓ Hydrogen + Helium: 86.0% (>60% required)✓ Mass: 287.0x Earth (>10x required)

Reading TOI-2202 b’s atmosphere

Dominant elements: H, He, O, C, NThis is what a telescope would measure while TOI-2202 b crosses in front of its star: starlight passes through the atmosphere and spreads into a rainbow band. Each dark line marks a wavelength the atmosphere absorbed.Every element absorbs its own signature wavelengths — hydrogen always darkens the same two spots, calcium another pair, and so on. Astronomers match the lines in a real spectrum against a library of these signatures to say what an atmosphere is made of, light-years away, without ever visiting. A deeper line generally means more of that element is present.TOI-2202 b sits about 770 light-years away, found by the transit method. Most catalogued distances trace back to parallax: as Earth orbits the Sun, a nearby star appears to shift very slightly against the distant background stars, and the size of that shift gives its distance directly.
Habitability ScoreUninhabitable
6
Contributing Factors
temperature4
Scorching - hot enough to melt lead, though rock stays solid; no chance for life
atmosphere18

Hydrogen and helium dominated with trace methane and ammonia

Hydrogen-rich atmosphere typical of gas giants (partially stripped by slow rotation)
water15
No solid surface — any water is locked in a supercritical mantle and hot ice, not oceans
magnetic Field100
Magnetic field provides radiation protection
geology40
Extreme volcanic activity may be hazardous
Organic Chemistry80
Core organic elements (CHNO) present
rotation30
Very slow rotation - days and nights each last several Earth days, bringing extreme temperature swings

Physical Properties

Mass
287.00x Earth (1.71e+27 kg)
Radius
6.60x Earth (42,024 km)
This planet: 6.60× Earth radiusEarth: 1× (baseline)
Surface Gravity
6.60x Earth (64.7 m/s²)
Surface Temperature
715 K (442 °C / 828 °F)
Rotation Period
285.6 hours/day (slower than Earth)
This planet: 286 h/dayEarth: 24 h/day

Elemental Composition

A dark ringed planet hanging over the horizon of a rocky moon, its rings lit by a distant sun

New: Stand on Your Moons 🌒

A planet's surface view isn't the only ground any more. Press the surface button on a planet with moons and it asks where to stand: the planet itself, or any moon still in orbit, each tagged with what it became — ocean, ice, carbon, volcanic. Every moon gets its own ground and sky from its own physics: airless rock under a black sky, ice cracked by geysers over a hidden sea, sulfur plains shaking with eruptions, or orange haze you can't see the sun through. And hanging over the horizon, there's the planet you built.

Create your free account

Enter your email and we'll send a 6-digit code — no password needed.
We only keep your email and the username you choose. We never share or sell your email, and we don't send marketing — we use it only to email you a sign-in code. Read our privacy policy.

Send feedback

We're still building out the best experience we can — and we'd love your input. Tell us about features you enjoy, ideas you'd like to see, or pain points where something feels off, and we'll know where to look next.

Type
Idea
Bug
Pain point
Other