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
0/ 100
Uninhabitable

Reading TOI-789 d’s atmosphere

Dominant elements: Si, Fe, Mg, Ni, S, AlThis is what a telescope would measure while TOI-789 d 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-789 d sits about 142 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.

TOI-789 d

Also written TOI-789d, TOI 789d, TOI 789 d

Rocky TerrestrialUninhabitable141 light years awayFound 2026

TOI-789 d, from the NASA Exoplanet Archive (found 2026). Measured: 6.6 Earth masses, 0.077 AU, a 3471 K M-type star. Composition inferred from a measured bulk density of 2.41x Earth's, far too high for silicates alone — an iron-rich world, with a day locked to its 13.0-day year, as anything orbiting this close would be.

Host star

TOI-789

Type
M-type (Red Dwarf)
Spectral type
M3 V
Temperature
3,471 K
Radius
0.371 ☉
Mass
0.358 ☉
Known planets
3, including this one
Luminosity
0.0178 ☉

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.

Rocky Terrestrial

Extreme Activity
Why is this a Rocky Terrestrial?TOI-789 d is dominated by silicate (36.6%) and iron (24.4%) 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: 36.6% + Iron: 24.4% + Magnesium: 12.2%✓ Mass: 6.6x Earth (terrestrial range)
Habitability ScoreUninhabitable
0
Contributing Factors
temperature40
Extreme temperature - very difficult for life
atmosphere6
No atmosphere - exposed to radiation and temperature extremes (partially stripped by slow rotation)
water0
No water - the recipe has no hydrogen and oxygen to form it
magnetic Field30
No magnetic field - vulnerable to solar radiation
geology40
Extreme volcanic activity may be hazardous
Organic Chemistry20
Limited organic chemistry potential
rotation30
Very slow rotation - extreme temperature swings between eternal day and night sides

Physical Properties

Mass
6.60x Earth (3.94e+25 kg)
Radius
1.88x Earth (11,951 km)
This planet: 1.88× Earth radiusEarth: 1× (baseline)
Surface Gravity
1.88x Earth (18.4 m/s²)
Surface Temperature
366 K (93 °C / 199 °F)
Rotation Period
312.0 hours/day (slower than Earth)
This planet: 312 h/dayEarth: 24 h/day

Orbital Environment

Star Type
M-type (Red Dwarf)
Distance from Star
0.08 AU (11.5 million km)
Orbital Period
14 days

Atmosphere

Minimal or none

Elemental Composition

Si - Silicon
36.6%
Fe - Iron
24.4%
Mg - Magnesium
12.2%

Surface Characteristics

Rocky surface with impact craters, possible volcanic features
A banded gas giant with four moons in different colors: a yellow sulfur moon, two rust-red rock moons and a blue water moon

New: Choose What Your Moons Are Made Of 🌙

Every moon used to be grey rock, white ice or blue ocean, decided for you. Now each one has a "Made of" choice in the builder's Moons tab — silicate rock, iron, water ice, carbon, sulfur, or nitrogen and methane ice — and the physics decides what that becomes. Put water ice too close to the star and it boils off to bare rock. Put sulfur where a neighbouring moon keeps it tidally flexed and it erupts in Io's yellows. Give a Titan-sized moon nitrogen ice far from the sun and it wraps itself in haze. Hang a water moon about the mass of Earth off a giant planet in the habitable zone and it can hold air and open seas — scored for life on the same scale as a planet, with a day as long as its orbit. A tint slider nudges the colour, but only as far as that material could really go.

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