TOI-1180 is 235 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 4,738 K star; the first was found in 2024 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-1180 b goes round its star every 9.69 days, 9 times as often as Mercury goes round the Sun.
| Surface temperature | 4,738 K |
| Mass | 0.75 solar masses |
| Radius | 0.73 solar radii |
| Luminosity | 0.265 times the Sun |
| Apparent magnitude | 11.017 |
| Age | about 5 billion years |
| Distance from the Sun | 234.9 light-years (72.0 parsecs) |
| Position (J2000) | RA 214.5558°, Dec 82.1938° |
| Constellation | Camelopardalis |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-1180 b | 9.69 days | 0.0808 AU | 3.072 R⊕ | 10 M⊕ | Transit, 2024 |
Values are the NASA Exoplanet Archive’s composite parameters. A radius marked estimated comes from a mass–radius relation; a mass marked minimum is M sin i. Planet sizes and colours in the 3D view are renderings: none of these worlds has been photographed as more than a point of light.
For a star of 4,738 K, 0.27 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.52 to 0.95 AU. None of its known planets orbits inside it. The zone says how much starlight arrives, not whether a planet has water or air. The edges follow Kopparapu et al. (2014), as the 3D view draws them.
The light you see left 235 years ago, around 1790.