TOI-3629 is 424 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this M1 star; the first was found in 2022 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-3629 b goes round its star every 3.94 days, 22 times as often as Mercury goes round the Sun.
| Spectral type | M1 |
| Surface temperature | 3,870 K |
| Mass | 0.63 solar masses |
| Radius | 0.6 solar radii |
| Luminosity | 0.075 times the Sun |
| Apparent magnitude | 14.639 |
| Age | about 7 billion years |
| Distance from the Sun | 424.3 light-years (130.1 parsecs) |
| Position (J2000) | RA 359.7934°, Dec 39.3143° |
| Constellation | Andromeda |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-3629 b | 3.94 days | 0.0430 AU | 8.2946 R⊕ | 82.635 M⊕ | Transit, 2022 |
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 3,870 K, 0.075 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.28 to 0.54 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 424 years ago, around 1600.