CoRoT-32 is 1,881 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G0 VI star; the first was found in 2018 by transit (CoRoT).
Fly there in 3DCoRoT-32 b goes round its star every 6.72 days, 13 times as often as Mercury goes round the Sun.
| Spectral type | G0 VI |
| Surface temperature | 5,970 K |
| Mass | 1.08 solar masses |
| Radius | 0.79 solar radii |
| Luminosity | 0.7 times the Sun |
| Apparent magnitude | 13.626 |
| Distance from the Sun | 1880.9 light-years (576.7 parsecs) |
| Position (J2000) | RA 100.1952°, Dec 9.2574° |
| Constellation | Monoceros |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| CoRoT-32 b | 6.72 days | 0.0710 AU | 6.3891 R⊕ | 47.675 M⊕ | Transit, 2018 |
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 5,970 K, 0.70 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.79 to 1.38 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 1,881 years ago, around AD 150.