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Entering orbit…
Habitability
0/ 100
Uninhabitable
KELT-1 b rendered in TerraForge from its measured mass, orbit and star

KELT-1 b

Also written KELT-1b, KELT 1b, KELT 1 b

Brown Dwarf874 light years awayFound 2012
Mass
8650.00 × Earth
Radius
12.40 × Earth
Gravity
56.26 g
Surface (est.)
2,421 K
Year
29.3 hrs
From Earth
874 ly
Mass
8650.00 × Earth
Radius
12.40 × Earth
Gravity
56.26 g
Surface (est.)
2,421 K
Year
29.3 hrs
From Earth
874 ly

KELT-1 system

Type
F-type (White)
Temperature
6,516 K
Radius
1.47 ☉
Mass
1.33 ☉
Planets
1
Luminosity
3.51 ☉

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.

Habitable zone

Star and planets drawn to scale: the star is 13 times as wide as KELT-1 b, so only its edge is in view. Orbits spaced as in the star system view.

KELT-1 b, from the NASA Exoplanet Archive (found 2012). Measured: 8650 Earth masses, 0.0247 AU, a 6516 K F-type star. Composition inferred from a mass of 8650 Earths, which is giant territory whatever its 4.54x density suggests, with a day locked to its 1.2-day year, as anything orbiting this close would be.

Surface. No surface: a deuterium-burning sphere the size of Jupiter and dozens of times its mass, glowing dull red from its own heat

Brown Dwarf
Magnetic FieldNone Activity
KELT-1 b has an unusual composition that doesn't fit standard classifications, or lacks the elements needed for complex geological processes.
Barren worlds can form from uncommon element combinations or may be remnants of larger bodies that lost their atmospheres and volatile materials.
Classification Criteria:
Composition doesn't match standard planet typesMass: 8650.0x EarthTemperature: 2421K

Reading KELT-1 b’s atmosphere

Dominant elements: H, He, O, C, NThis is what a telescope would measure while KELT-1 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.KELT-1 b sits about 874 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.
Habitability ScoreUninhabitable
0
Contributing Factors
temperature0
Inferno world - temperatures exceed all possibility of life
atmosphere30

Hydrogen and helium with iron and silicate cloud decks - hot enough to rain molten metal

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 Field20
A strong field, but no surface beneath it — there is nothing here for it to shelter
geology30
Geologically dead - no nutrient recycling
Organic Chemistry80
Core organic elements (CHNO) present
rotation100
Optimal rotation period - balanced day/night cycle, moderate weather, and good heat distribution

Physical Properties

Mass
8650.00x Earth (5.17e+28 kg)
Radius
20.53x Earth (130,781 km)
This planet: 20.53× Earth radiusEarth: 1× (baseline)
Surface Gravity
20.53x Earth (201.4 m/s²)
Surface Temperature
2,421 K (2,148 °C / 3,898 °F)
Rotation Period
29.3 hours/day (slower than Earth)
This planet: 29 h/dayEarth: 24 h/day

Time Dilation

Clocks run 24.6 seconds per year slower than deep space — about 33 minutes over a lifetime

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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