TOI-672 is 218 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this M0 V star; the first was found in 2023 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-672 b goes round its star every 3.63 days, 24 times as often as Mercury goes round the Sun.
| Spectral type | M0 V |
| Surface temperature | 3,810 K |
| Mass | 0.54 solar masses |
| Radius | 0.54 solar radii |
| Luminosity | 0.04799 times the Sun |
| Apparent magnitude | 13.576 |
| Distance from the Sun | 218.2 light-years (66.9 parsecs) |
| Position (J2000) | RA 167.9909°, Dec -39.3281° |
| Constellation | Centaurus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-672 b | 3.63 days | 0.0376 AU | 5.31 R⊕ | 50.9 M⊕ | Transit, 2023 |
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 3,810 K, 0.048 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.23 to 0.43 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 218 years ago, around 1810.