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Entering orbit…
Habitability
9/ 100
Uninhabitable
TOI-880 Ad rendered in TerraForge from its measured mass, orbit and star

TOI-880 Ad

Also written TOI 880 Ad

Sub-Neptune198 light years awayFound 2025
Mass
13.10 × Earth
Radius
3.40 × Earth
Gravity
1.13 g
Surface (est.)
678 K
Year
14.3 days
From Earth
198 ly
Mass
13.10 × Earth
Radius
3.40 × Earth
Gravity
1.13 g
Surface (est.)
678 K
Year
14.3 days
From Earth
198 ly

TOI-880 system

Type
K-type (Orange)
Spectral type
K0V
Temperature
5,050 K
Radius
0.83 ☉
Mass
0.87 ☉
Planets
3
Luminosity
0.404 ☉

Published by the Extrasolar Planets Encyclopaedia. This world’s temperature and habitability score are computed from its star’s published radius and temperature.

Habitable zone

Star and planets drawn to scale: the star is 27 times as wide as TOI-880 Ad, so only its edge is in view. Orbits spaced as in the star system view.

exoplanet.euListed by the Extrasolar Planets Encyclopaedia; not yet in NASA's confirmed catalogue.View on exoplanet.eu

TOI-880 Ad, from the Extrasolar Planets Encyclopaedia (found 2025). Measured: 13.1 Earth masses, 0.11 AU, a 5050 K K-type star. Composition inferred from a measured bulk density of 0.33x Earth's, too low for bare rock at this size, suggesting a rocky core under roughly a 12% 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 hot for liquid waterMagnetic FieldLow Activity
TOI-880 Ad is a sub-Neptune: a 13.1x 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: 13.1x Earth (under 20x, below the giants)✓ A hydrogen-helium envelope over the core

Reading TOI-880 Ad’s atmosphere

Dominant elements: O, Si, Fe, N, C, HThis is what a telescope would measure while TOI-880 Ad 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-880 Ad sits about 198 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
9
Contributing Factors
temperature4
Scorching - hot enough to melt lead, though rock stays solid; no chance 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
13.10x Earth (7.82e+25 kg)
Radius
2.36x Earth (15,019 km)
This planet: 2.36× Earth radiusEarth: 1× (baseline)
Surface Gravity
2.36x Earth (23.1 m/s²)
Surface Temperature
678 K (405 °C / 761 °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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