TOI-892 is 1,111 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this F star; the first was found in 2020 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DTOI-892 b goes round its star every 10.6 days, 8 times as often as Mercury goes round the Sun.
| Spectral type | F |
| Surface temperature | 6,261 K |
| Mass | 1.28 solar masses |
| Radius | 1.39 solar radii |
| Luminosity | 2.7 times the Sun |
| Apparent magnitude | 11.43 |
| Age | about 2.2 billion years |
| Distance from the Sun | 1110.7 light-years (340.5 parsecs) |
| Position (J2000) | RA 86.7382°, Dec -11.2353° |
| Constellation | Lepus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| TOI-892 b | 10.6 days | 0.0920 AU | 11.994 R⊕ | 301.94 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 6,261 K, 2.7 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.52 to 2.65 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 1,111 years ago, around AD 920.