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Entering orbit…
Habitability
59/ 100
Marginal

Reading Kepler-1229 b’s atmosphere

Dominant elements: O, Si, H, Fe, N, CThis is what a telescope would measure while Kepler-1229 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-1229 b sits about 864 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.

Kepler-1229 b

Ice WorldMarginal864 light years awayFound 2016

Kepler-1229 b, from the NASA Exoplanet Archive (found 2016). Measured: 2.54 Earth masses, 0.301 AU, a 3784 K K-type star. Composition inferred from a measured bulk density of 0.93x Earth's at this size, suggesting roughly 16% water/ice by mass, with an assumed 24-hour day — rotation cannot be measured for exoplanets.

Host star

Kepler-1229

Type
K-type (Orange)
Temperature
3,784 K
Radius
0.51 ☉
Mass
0.54 ☉
Known planets
1 (this one)
Luminosity
0.0293 ☉

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.

Ice World

No life — too cold for liquid waterMagnetic FieldLow Activity
Why is this a Ice World?Your planet orbits at 0.30 AU from its star, resulting in frigid temperatures of 219K.
Ice worlds form beyond the frost line where temperatures are low enough for water and other volatiles to freeze solid. They may have subsurface oceans beneath thick ice shells.
Classification Criteria:
✓ Distance: 0.30 AU (>3 AU) or Temperature <200K✓ Temperature: 219K✓ Water content: 38.8% for ice formation
Further reading
Imagined LifeJames Trefil & Michael SummersWhat could live on a world like this one: ice shells, supergravity, tidally locked twilight.Envisioning ExoplanetsMichael CarrollWhat these worlds might look like from the ground, painted from the same measurements this page renders.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.
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Habitability ScoreMarginal
59
Contributing Factors
temperature40
Extreme temperature - very difficult for life
atmosphere70
Nitrogen atmosphere provides protection but not breathable
water55
Abundant water - frozen solid, no liquid phase at this temperature
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
2.54x Earth (1.52e+25 kg)
Radius
1.36x Earth (8,693 km)
This planet: 1.36× Earth radiusEarth: 1× (baseline)
Surface Gravity
1.36x Earth (13.4 m/s²)
Surface Temperature
219 K (-54 °C / -65 °F)
Rotation Period
24.0 hours/day
This planet: 24 h/dayEarth: 24 h/day

Orbital Environment

Star Type
K-type (Orange)
Distance from Star
0.30 AU (45 million km)
Orbital Period
72 days

Atmosphere

Thin nitrogen and methane atmosphere

Elemental Composition

O - Oxygen
31.0%
Si - Silicon
21.4%
H - Hydrogen
15.6%

Surface Characteristics

Frozen surface covered in water ice, possible subsurface ocean if tidal heating present
A binary star system's orrery: two suns close together, a red dashed dead-zone boundary, and a debris trail left by a destroyed world

New: Binary Star Systems 🌀

A system can now orbit two suns. Add a companion star when you build one — close, medium, or wide — and the physics decides what survives: a shared center of mass carves out a dead zone where gravity from both stars tears a world apart, leaving it as debris, and every surviving planet's orbit goes elliptical, moving fastest at closest approach and slowest out at aphelion. Push the separation to wide and the dead zone opens tens of AU across, wide enough to gut a system that would have been stable around one star alone. Stand on a world that made it through and you'll watch two suns cross the sky together.

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