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
Kepler-520 b rendered in TerraForge from its measured mass, orbit and star

Kepler-520 b

Also written Kepler-520b, Kepler 520b, Kepler 520 b

Sub-Neptune2034 light years awayFound 2016
Mass
3.39 × Earth
Radius
1.66 × Earth
Gravity
1.23 g
Surface (est.)
990 K
Year
19.7 days
From Earth
2,035 ly
Mass
3.39 × Earth
Radius
1.66 × Earth
Gravity
1.23 g
Surface (est.)
990 K
Year
19.7 days
From Earth
2,035 ly

Kepler-520 system

Type
F-type (White)
Temperature
6,112 K
Radius
1.09 ☉
Mass
1.1 ☉
Planets
2
Luminosity
3.24 ☉

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-520 c0.060 AU1.2 M⊕
Kepler-520 b0.15 AUYou are here3.4 M⊕
Habitable zone

Star and planets drawn to scale: the star is 72 times as wide as Kepler-520 b, so only its edge is in view. Orbits spaced as in the star system view.

Sub-Neptune, likely · its density could also fit a rocky world

Kepler-520 b, from the NASA Exoplanet Archive (found 2016). Measured: 3.39 Earth masses, 0.146 AU, a 6112 K F-type star. Composition inferred from a measured bulk density of 0.74x Earth's, too low for bare rock at this size, suggesting a rocky core under roughly a 0.8% hydrogen/helium envelope by mass, with an assumed 24-hour day — rotation cannot be measured for exoplanets. Note: TerraForge comes out at 990 K against the archive's 711 K, because it models stars by spectral class, and Kepler-520 is not an average F-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 waterMagnetic FieldLow Activity
Kepler-520 b is a sub-Neptune: a 3.4x 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: 3.4x Earth (under 20x, below the giants)✓ A hydrogen-helium envelope over the core

Reading Kepler-520 b’s atmosphere

Dominant elements: O, Si, Fe, N, C, HThis is what a telescope would measure while Kepler-520 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.Kepler-520 b sits about 2035 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
0
Contributing Factors
temperature0
Scorching - hot enough to melt lead, though rock stays solid; no chance for life
atmosphere30

Deep hydrogen-helium envelope with photochemical haze

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
geology60
Some geological activity provides slow nutrient cycling
Organic Chemistry80
Core organic elements (CHNO) present
rotation100
Optimal rotation period - balanced day/night cycle, moderate weather, and good heat distribution

Physical Properties

Mass
3.39x Earth (2.02e+25 kg)
Radius
1.50x Earth (9,571 km)
This planet: 1.50× Earth radiusEarth: 1× (baseline)
Surface Gravity
1.50x Earth (14.7 m/s²)
Surface Temperature
990 K (717 °C / 1,323 °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.

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