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Entering orbit…
Habitability
5/ 100
Uninhabitable
Kepler-80 c rendered in TerraForge from its measured mass, orbit and star

Kepler-80 c

Also written Kepler-80c, Kepler 80c, Kepler 80 c

Sub-Neptune1203 light years awayFound 2012
Mass
6.74 × Earth
Radius
2.74 × Earth
Gravity
0.90 g
Surface (est.)
644 K
Year
9.5 days
From Earth
1,204 ly
Mass
6.74 × Earth
Radius
2.74 × Earth
Gravity
0.90 g
Surface (est.)
644 K
Year
9.5 days
From Earth
1,204 ly

Kepler-80 system

Type
K-type (Orange)
Spectral type
K5
Temperature
4,540 K
Radius
0.678 ☉
Mass
0.73 ☉
Planets
6
Luminosity
0.170 ☉

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-80 f0.018 AU12,700 M⊕
Kepler-80 d0.037 AU6.8 M⊕
Kepler-80 e0.049 AU4.1 M⊕
Kepler-80 b0.065 AU6.9 M⊕
Kepler-80 c0.079 AUYou are here6.7 M⊕
Habitable zone

Star and planets drawn to scale: the star is 27 times as wide as Kepler-80 c, so only its edge is in view. Orbits spaced as in the star system view.

Kepler-80 c, from the NASA Exoplanet Archive (found 2012). Measured: 6.74 Earth masses, 0.0792 AU, a 4540 K K-type star. Composition inferred from a measured bulk density of 0.33x Earth's, too low for bare rock at this size, suggesting a rocky core under roughly a 6% hydrogen/helium envelope by mass, with a day locked to its 9.5-day year, as anything orbiting this close would be. Note: TerraForge comes out at 644 K against the archive's 495 K, because it models stars by spectral class, and Kepler-80 is not an average K-type.

Surface. No solid surface - a hydrogen-helium envelope wrapped around a rocky core (a sub-Neptune)

Sub-Neptune
Life unlikely — too hot for liquid waterLow Activity
Kepler-80 c is a sub-Neptune: a 6.7x Earth core wrapped in a deep hydrogen-helium envelope, with no solid surface to stand on.
Sub-Neptunes are the most common planets Kepler found, though our own solar system has none. Too light to be a giant, they still hold on to a thick envelope of light gas over a rocky or icy core.
Classification Criteria:
✓ Mass: 6.7x Earth (under 20x, below the giants)✓ A hydrogen-helium envelope over the core

Reading Kepler-80 c’s atmosphere

Dominant elements: O, Si, Fe, N, C, HThis is what a telescope would measure while Kepler-80 c 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-80 c sits about 1204 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 ScoreUninhabitable
5
Contributing Factors
temperature4
Scorching - hot enough to melt lead, though rock stays solid; no chance for life
atmosphere18

Deep hydrogen-helium envelope with photochemical haze

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 Field30
No magnetic field - vulnerable to solar radiation
geology60
Some geological activity provides slow nutrient cycling
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
6.74x Earth (4.03e+25 kg)
Radius
1.89x Earth (12,034 km)
This planet: 1.89× Earth radiusEarth: 1× (baseline)
Surface Gravity
1.89x Earth (18.5 m/s²)
Surface Temperature
644 K (370 °C / 699 °F)
Rotation Period
228.5 hours/day (slower than Earth)
This planet: 228 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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