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Entering orbit…
Habitability
33/ 100
Extremely Harsh
K2-72 c rendered in TerraForge from its measured mass, orbit and star

K2-72 c

Also written K2-72c, K2 72c, K2 72 c

Rocky Terrestrial216 light years awayFound 2016
Mass
1.65 × Earth
Radius
1.16 × Earth
Gravity
1.23 g
Surface (est.)
352 K
Year
15.2 days
From Earth
217 ly
Mass
1.65 × Earth
Radius
1.16 × Earth
Gravity
1.23 g
Surface (est.)
352 K
Year
15.2 days
From Earth
217 ly

K2-72 system

Type
M-type (Red Dwarf)
Temperature
3,360 K
Radius
0.331 ☉
Mass
0.271 ☉
Planets
4
Luminosity
0.0146 ☉

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 31 times as wide as K2-72 c, so only its edge is in view. Orbits spaced as in the star system view.

K2-72 c is the third of four planets around K2-72, a red dwarf about 220 light-years away. It crosses in front of its star every 15.2 days, and the NASA Exoplanet Archive lists its radius as about 1.16 times Earth's. It was found by NASA's K2 mission, the second phase of the Kepler space telescope, which spotted the small dips in starlight as each of the four planets passed in front of the star.

Surface. Rocky surface with impact craters, possible volcanic features

Rocky Terrestrial
Life unlikely — too hot for liquid waterModerate Activity
K2-72 c 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: 1.6x Earth (terrestrial range)

Reading K2-72 c’s atmosphere

Dominant elements: O, Si, Fe, N, H, CThis is what a telescope would measure while K2-72 c 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.K2-72 c sits about 217 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 ScoreExtremely Harsh
33
Contributing Factors
temperature31
Hot - near boiling, only heat-loving microbes would thrive
atmosphere42

Thin CO₂ and nitrogen atmosphere

Nitrogen atmosphere provides protection but not breathable (partially stripped by slow rotation)
water50
Limited water content
magnetic Field30
No magnetic field - vulnerable to solar radiation
geology90
Active geology recycles nutrients and drives carbon cycle
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
1.65x Earth (9.85e+24 kg)
Radius
1.18x Earth (7,528 km)
This planet: 1.18× Earth radiusEarth: 1× (baseline)
Surface Gravity
1.18x Earth (11.6 m/s²)
Surface Temperature
352 K (79 °C / 174 °F)
Rotation Period
364.8 hours/day (slower than Earth)
This planet: 365 h/dayEarth: 24 h/day

Elemental Composition

How TerraForge built this world

K2-72 c, from the NASA Exoplanet Archive (found 2016). Measured: 1.65 Earth masses, 0.078 AU, a 3360 K M-type star. Composition inferred from a measured bulk density of 1.06x Earth's, which is rock and iron, with a day locked to its 15.2-day year, as anything orbiting this close would be.

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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