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Entering orbit…
Habitability
25/ 100
Extremely Harsh
Kepler-30 d rendered in TerraForge from its measured mass, orbit and star

Kepler-30 d

Also written Kepler-30d, Kepler 30d, Kepler 30 d

Gas Giant2980 light years awayFound 2012
Mass
23.10 × Earth
Radius
8.80 × Earth
Gravity
0.30 g
Surface (est.)
344 K
Year
143 days
From Earth
2,981 ly
Mass
23.10 × Earth
Radius
8.80 × Earth
Gravity
0.30 g
Surface (est.)
344 K
Year
143 days
From Earth
2,981 ly

Kepler-30 system

Type
G-type (Yellow (Sun-like))
Temperature
5,498 K
Radius
0.95 ☉
Mass
0.99 ☉
Planets
3
Luminosity
0.580 ☉

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.

Kepler-30 b0.18 AU11 M⊕
Kepler-30 c0.30 AU640 M⊕
Kepler-30 d0.50 AUYou are here23 M⊕
Habitable zone

Star and planets drawn to scale: the star is 12 times as wide as Kepler-30 d, so only its edge is in view. Orbits spaced as in the star system view.

Kepler-30 d, from the NASA Exoplanet Archive (found 2012). Measured: 23.1 Earth masses, 0.5 AU, a 5498 K G-type star. Composition inferred from a measured bulk density of 0.03x Earth's, which only hydrogen and helium can explain, with an assumed 24-hour day — rotation cannot be measured for exoplanets.

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

Gas Giant
Life unlikely — no phosphorus — DNA and ATP are built on itMagnetic FieldExtreme Activity
Kepler-30 d has 86.0% hydrogen and helium, combined with a mass of 23.1x 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: 23.1x Earth (>10x required)

Reading Kepler-30 d’s atmosphere

Dominant elements: H, He, O, C, NThis is what a telescope would measure while Kepler-30 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.Kepler-30 d sits about 2981 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.
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.Exoplanets: Diamond Worlds, Super Earths, Pulsar PlanetsMichael Summers & James TrefilThe strange end of the catalogue — carbon worlds, molten rock, planets orbiting dead stars.The Little Book of ExoplanetsJoshua WinnHow these worlds are found, and what a measurement can honestly tell us.
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
25
Contributing Factors
temperature37
Hot - near boiling, only heat-loving microbes would thrive
atmosphere30

Hydrogen and helium dominated with trace methane and ammonia

Hydrogen-rich atmosphere typical of gas giants
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
rotation100
Optimal rotation period - balanced day/night cycle, moderate weather, and good heat distribution

Physical Properties

Mass
23.10x Earth (1.38e+26 kg)
Radius
2.85x Earth (18,144 km)
This planet: 2.85× Earth radiusEarth: 1× (baseline)
Surface Gravity
2.85x Earth (27.9 m/s²)
Surface Temperature
344 K (71 °C / 159 °F)
Rotation Period
24.0 hours/day
This planet: 24 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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