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Entering orbit…
Habitability
16/ 100
Uninhabitable
Wolf 1061 d rendered in TerraForge from its measured mass, orbit and star

Wolf 1061 d

Also written Wolf 1061d

Sub-Neptune14 light years awayFound 2015
Mass
7.70 × Earth
Radius
2.69 × Earth
Gravity
1.06 g
Surface (est.)
131 K
Year
217 days
From Earth
14.1 ly
Mass
7.70 × Earth
Radius
2.69 × Earth
Gravity
1.06 g
Surface (est.)
131 K
Year
217 days
From Earth
14.1 ly

Wolf 1061 system

Type
M-type (Red Dwarf)
Spectral type
M3.5
Temperature
3,342 K
Radius
0.307 ☉
Mass
0.294 ☉
Planets
3
Luminosity
0.0102 ☉

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 12 times as wide as Wolf 1061 d, so only its edge is in view. Orbits spaced as in the star system view.

Estimated: this planet doesn't transit its star, so its size is inferred, not measured

Wolf 1061 d, from the NASA Exoplanet Archive (found 2015). Measured: 7.7 Earth masses, 0.47 AU, a 3342 K M-type star. Composition inferred from a estimated bulk density of 0.40x Earth's, modeled rather than measured since this isn't a transiting planet, too low for bare rock at this size, suggesting a rocky core under roughly a 6% hydrogen/helium envelope by mass, with an assumed 24-hour day — rotation cannot be measured for exoplanets.

Surface. No solid surface - a hydrogen-helium envelope wrapped around a rocky core (a sub-Neptune)

Sub-Neptune
Life unlikely — too cold for liquid waterMagnetic FieldLow Activity
Wolf 1061 d is a sub-Neptune: a 7.7x 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: 7.7x Earth (under 20x, below the giants)✓ A hydrogen-helium envelope over the core

Reading Wolf 1061 d’s atmosphere

Dominant elements: O, Si, Fe, N, C, HThis is what a telescope would measure while Wolf 1061 d 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.Wolf 1061 d sits about 14 light-years away, found by the radial velocity 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
16
Contributing Factors
temperature13
Very cold - water frozen, challenging 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
7.70x Earth (4.60e+25 kg)
Radius
1.97x Earth (12,581 km)
This planet: 1.97× Earth radiusEarth: 1× (baseline)
Surface Gravity
1.97x Earth (19.4 m/s²)
Surface Temperature
131 K (-142 °C / -224 °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.

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