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Entering orbit…
Habitability
0/ 100
Uninhabitable
HD 224018 b rendered in TerraForge from its measured mass, orbit and star

HD 224018 b

Also written HD 224018b

Rocky Terrestrial342 light years awayFound 2025
Mass
4.10 × Earth
Radius
0.91 × Earth
Gravity
4.95 g
Surface (est.)
968 K
Year
10.6 days
From Earth
342 ly
Mass
4.10 × Earth
Radius
0.91 × Earth
Gravity
4.95 g
Surface (est.)
968 K
Year
10.6 days
From Earth
342 ly

HD 224018 system

Type
G-type (Yellow (Sun-like))
Spectral type
G V
Temperature
5,784 K
Radius
1.15 ☉
Mass
1.01 ☉
Planets
4
Luminosity
1.33 ☉

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.

HD 224018 b0.095 AUYou are here4.1 M⊕
HD 224018 c0.22 AU10 M⊕
HD 224018 d0.53 AU4.2 M⊕
HD 224018 e8.60 AU151 M⊕
Habitable zone

Star and planets drawn to scale: the star is 138 times as wide as HD 224018 b, so only its edge is in view. Orbits spaced as in the star system view.

Estimated: this planet doesn't transit its star, so its size is inferred, not measured

HD 224018 b, from the NASA Exoplanet Archive (found 2025). Measured: 4.1 Earth masses, 0.0952 AU, a 5784 K G-type star. Composition inferred from a measured bulk density of 5.44x Earth's, far too high for silicates alone — an iron-rich world, with a day locked to its 10.6-day year, as anything orbiting this close would be.

Surface. Rocky surface with impact craters, possible volcanic features

Rocky Terrestrial
High Activity
HD 224018 b 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: 4.1x Earth (terrestrial range)

Reading HD 224018 b’s atmosphere

Dominant elements: Si, Fe, Mg, Ni, S, AlThis is what a telescope would measure while HD 224018 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.HD 224018 b sits about 342 light-years away, found by the radial velocity 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.
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 ScoreUninhabitable
0
Contributing Factors
temperature0
Scorching - hot enough to melt lead, though rock stays solid; no chance for life
atmosphere6

Minimal or none

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
geology90
Active geology recycles nutrients and drives carbon cycle
Organic Chemistry20
Limited organic chemistry potential
rotation30
Very slow rotation - days and nights each last several Earth days, bringing extreme temperature swings

Physical Properties

Mass
4.10x Earth (2.45e+25 kg)
Radius
1.60x Earth (10,197 km)
This planet: 1.60× Earth radiusEarth: 1× (baseline)
Surface Gravity
1.60x Earth (15.7 m/s²)
Surface Temperature
968 K (694 °C / 1,282 °F)
Rotation Period
254.4 hours/day (slower than Earth)
This planet: 254 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.

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