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Entering orbit…
Habitability
3/ 100
Uninhabitable
TOI-1442 b rendered in TerraForge from its measured mass, orbit and star

TOI-1442 b

Also written TOI-1442b, TOI 1442b, TOI 1442 b

Rocky Terrestrial134 light years awayFound 2022
Mass
1.71 × Earth
Radius
1.17 × Earth
Gravity
1.25 g
Surface (est.)
905 K
Year
9.8 hrs
From Earth
134 ly
Mass
1.71 × Earth
Radius
1.17 × Earth
Gravity
1.25 g
Surface (est.)
905 K
Year
9.8 hrs
From Earth
134 ly

TOI-1442 system

Type
M-type (Red Dwarf)
Temperature
3,330 K
Radius
0.31 ☉
Mass
0.29 ☉
Planets
1
Luminosity
0.0105 ☉

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 29 times as wide as TOI-1442 b, so only its edge is in view. Orbits spaced as in the star system view.

TOI-1442 b, from the NASA Exoplanet Archive (found 2022). Measured: 1.71 Earth masses, 0.0071 AU, a 3330 K M-type star. Composition inferred from a measured bulk density of 1.07x Earth's, which is rock and iron, with a day locked to its 0.4-day year, as anything orbiting this close would be.

Surface. Rocky surface with impact craters, possible volcanic features

Rocky Terrestrial
Life unlikely — too hot for liquid waterMagnetic FieldModerate Activity
TOI-1442 b is dominated by silicate (24.5%) and iron (12.3%) content, forming a rocky terrestrial body.
Rocky terrestrial planets are primarily composed of silicate rocks and metals. They're the most common type of small planet in the universe.
Classification Criteria:
✓ Silicon: 24.5% + Iron: 12.3% + Magnesium: 3.6%✓ Mass: 1.7x Earth (terrestrial range)

Reading TOI-1442 b’s atmosphere

Dominant elements: O, Si, Fe, N, H, CThis is what a telescope would measure while TOI-1442 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.TOI-1442 b sits about 134 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
3
Contributing Factors
temperature1
Scorching - hot enough to melt lead, though rock stays solid; no chance for life
atmosphere70

Thin CO₂ and nitrogen atmosphere

Nitrogen atmosphere provides protection but not breathable
water8
Limited water content - boiling away, little would be retained
magnetic Field100
Magnetic field provides radiation protection
geology90
Active geology recycles nutrients and drives carbon cycle
Organic Chemistry80
Core organic elements (CHNO) present
rotation60
Fast rotation - strong global wind patterns and weather systems, but manageable

Physical Properties

Mass
1.71x Earth (1.02e+25 kg)
Radius
1.20x Earth (7,619 km)
This planet: 1.20× Earth radiusEarth: 1× (baseline)
Surface Gravity
1.20x Earth (11.7 m/s²)
Surface Temperature
905 K (632 °C / 1,170 °F)
Rotation Period
9.8 hours/day (faster than Earth)
This planet: 10 h/dayEarth: 24 h/day

Time Dilation

Clocks run 14.0 seconds per year slower than deep space — about 19 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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