TOI-132 is 534 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G8 V star; the first was found in 2020 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-132 b goes round its star every 2.11 days, 42 times as often as Mercury goes round the Sun.
| Spectral type | G8 V |
| Surface temperature | 5,397 K |
| Mass | 0.97 solar masses |
| Radius | 0.9 solar radii |
| Luminosity | 0.6 times the Sun |
| Apparent magnitude | 11.197 |
| Age | about 6.34 billion years |
| Distance from the Sun | 533.9 light-years (163.7 parsecs) |
| Position (J2000) | RA 338.3997°, Dec -43.4369° |
| Constellation | Grus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-132 b | 2.11 days | 0.0260 AU | 3.42 R⊕ | 22.4 M⊕ | Transit, 2020 |
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 5,397 K, 0.60 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.75 to 1.34 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 534 years ago, around 1490.