HD 92788 is 113 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this G6 V star; the first was found in 2000 by radial velocity (Multiple Observatories).
Fly there in 3DHD 92788 c takes 31.8 years to go round its star once.
| Spectral type | G6 V |
| Surface temperature | 5,744 K |
| Mass | 1.15 solar masses |
| Radius | 1.14 solar radii |
| Luminosity | 1.047 times the Sun |
| Apparent magnitude | 7.31637 |
| Age | about 2.55 billion years |
| Distance from the Sun | 113.0 light-years (34.7 parsecs) |
| Position (J2000) | RA 160.7021°, Dec -2.1847° |
| Constellation | Sextans |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HD 92788 b | 325.8 days | 0.970 AU | 13 R⊕ estimated | 1195 M⊕ minimum | Radial Velocity, 2000 |
| HD 92788 c | 31.8 years | 10.500 AU | 13 R⊕ estimated | 1166.4 M⊕ minimum | Radial Velocity, 2019 |
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 5,744 K, 1.0 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.97 to 1.72 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 113 years ago, around 1910.