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Entering orbit…
Habitability
23/ 100
Extremely Harsh
SPECULOOS-3 b rendered in TerraForge from its measured mass, orbit and star

SPECULOOS-3 b

Also written SPECULOOS-3b, SPECULOOS 3b, SPECULOOS 3 b

Rocky TerrestrialFound 2024
Mass
0.89 × Earth
Radius
0.98 × Earth
Gravity
0.94 g
Surface (est.)
480 K
Year
17.3 hrs
Day (est.)
17.3 hrs
Mass
0.89 × Earth
Radius
0.98 × Earth
Gravity
0.94 g
Surface (est.)
480 K
Year
17.3 hrs
Day (est.)
17.3 hrs

SPECULOOS-3 system

Type
M-type (Red Dwarf)
Spectral type
M6.5+/-0.5
Temperature
2,800 K
Radius
0.123 ☉
Mass
0.101 ☉
Planets
1
Luminosity
8.35e-4 ☉

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.

SPECULOOS-3 b0.010 AUYou are here0.9 M⊕
Habitable zone

Star and planets drawn to scale: the star is 14 times as wide as SPECULOOS-3 b, so only its edge is in view. Orbits spaced as in the star system view.

SPECULOOS-3 b, from the NASA Exoplanet Archive (found 2024). Measured: 0.894 Earth masses, 0.00733 AU, a 2800 K M-type star. Composition inferred from a measured bulk density of 0.96x Earth's, which is rock and iron, with a day locked to its 0.7-day year, as anything orbiting this close would be.

Surface. Rocky surface with impact craters, possible volcanic features

Rocky Terrestrial
Life unlikely — too hot for liquid waterMagnetic FieldModerate Activity
SPECULOOS-3 b is dominated by silicate (24.6%) and iron (12.3%) content, forming a rocky terrestrial body.
Rocky terrestrial planets are primarily composed of silicate rocks and metals. They're the most common type of small planet in the universe.
Classification Criteria:
✓ Silicon: 24.6% + Iron: 12.3% + Magnesium: 3.7%✓ Mass: 0.9x Earth (terrestrial range)

Reading SPECULOOS-3 b’s atmosphere

Dominant elements: O, Si, Fe, N, H, CThis is what a telescope would measure while SPECULOOS-3 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.For a real planet, distance is usually measured by 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 — the same geometry surveyors use, at an interstellar scale.
Further reading
ExoplanetsSara Seager (editor)The field's standard reference: how planets are found, how they form, and what their atmospheres are made of.The Planet FactoryElizabeth TaskerHow planets are made, and why so few of them come out like Earth.The Little Book of ExoplanetsJoshua WinnHow these worlds are found, and what a measurement can honestly tell us.Exoplanets: Diamond Worlds, Super Earths, Pulsar PlanetsMichael Summers & James TrefilThe strange end of the catalogue — carbon worlds, molten rock, planets orbiting dead stars.
As an Amazon Associate I earn from qualifying purchases — if you buy through these links, TerraForge may receive a small commission at no extra cost to you.
Habitability ScoreExtremely Harsh
23
Contributing Factors
temperature10
Extremely hot - hostile to known life forms
atmosphere70

Thin CO₂ and nitrogen atmosphere

Nitrogen atmosphere provides protection but not breathable
water30
Limited water content - likely as steam
magnetic Field100
Magnetic field provides radiation protection
geology90
Active geology recycles nutrients and drives carbon cycle
Organic Chemistry80
Core organic elements (CHNO) present
rotation100
Optimal rotation period - balanced day/night cycle, moderate weather, and good heat distribution

Physical Properties

Mass
0.89x Earth (5.34e+24 kg)
Radius
0.96x Earth (6,137 km)
This planet: 0.96× Earth radiusEarth: 1× (baseline)
Surface Gravity
0.96x Earth (9.5 m/s²)
Surface Temperature
480 K (207 °C / 405 °F)
Rotation Period
17.3 hours/day (faster than Earth)
This planet: 17 h/dayEarth: 24 h/day

Time Dilation

Clocks run 14.0 seconds per year slower than deep space — about 19 minutes over a lifetime

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.

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