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Entering orbit…
Habitability
4/ 100
Uninhabitable
Kepler-292 e rendered in TerraForge from its measured mass, orbit and star

Kepler-292 e

Also written Kepler-292e, Kepler 292e, Kepler 292 e

Sub-Neptune3456 light years awayFound 2014
Mass
7.61 × Earth
Radius
2.67 × Earth
Gravity
1.07 g
Surface (est.)
746 K
Year
12.0 days
From Earth
3,457 ly
Mass
7.61 × Earth
Radius
2.67 × Earth
Gravity
1.07 g
Surface (est.)
746 K
Year
12.0 days
From Earth
3,457 ly

Kepler-292 system

Type
G-type (Yellow (Sun-like))
Temperature
5,299 K
Radius
0.826 ☉
Mass
0.865 ☉
Planets
5
Luminosity
0.460 ☉

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-292 b0.035 AU2.3 M⊕
Kepler-292 c0.045 AU2.8 M⊕
Kepler-292 d0.068 AU5.6 M⊕
Kepler-292 e0.097 AUYou are here7.6 M⊕
Kepler-292 f0.14 AU6.1 M⊕
Habitable zone

Star and planets drawn to scale: the star is 34 times as wide as Kepler-292 e, so only its edge is in view. Orbits spaced as in the star system view.

Kepler-292 e, from the NASA Exoplanet Archive (found 2014). Measured: 7.61 Earth masses, 0.097 AU, a 5299 K G-type star. Composition inferred from a measured bulk density of 0.40x Earth's, too low for bare rock at this size, suggesting a rocky core under roughly a 5% hydrogen/helium envelope by mass, with a day locked to its 12.0-day year, as anything orbiting this close would be.

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-292 e is a sub-Neptune: a 7.6x 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: 7.6x Earth (under 20x, below the giants)✓ A hydrogen-helium envelope over the core

Reading Kepler-292 e’s atmosphere

Dominant elements: O, Si, Fe, N, C, HThis is what a telescope would measure while Kepler-292 e 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-292 e sits about 3457 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
4
Contributing Factors
temperature3
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
7.61x Earth (4.54e+25 kg)
Radius
1.97x Earth (12,531 km)
This planet: 1.97× Earth radiusEarth: 1× (baseline)
Surface Gravity
1.97x Earth (19.3 m/s²)
Surface Temperature
746 K (473 °C / 883 °F)
Rotation Period
288.0 hours/day (slower than Earth)
This planet: 288 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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