HIP 94235 is 191 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G V star; the first was found in 2022 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DHIP 94235 b goes round its star every 7.71 days, 11 times as often as Mercury goes round the Sun.
HIP 94235 is one of 2 stars in its system. The position of the other star is not catalogued, so only HIP 94235 and its planets are drawn.
| Spectral type | G V |
| Surface temperature | 5,991 K |
| Mass | 1.094 solar masses |
| Radius | 1.08 solar radii |
| Luminosity | 1.373 times the Sun |
| Apparent magnitude | 8.31 |
| Age | about 0.118 billion years |
| Distance from the Sun | 190.8 light-years (58.5 parsecs) |
| Position (J2000) | RA 287.7411°, Dec -60.2726° |
| Constellation | Pavo |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HIP 94235 b | 7.71 days | 0.0787 AU | 3 R⊕ | 379 M⊕ | Transit, 2022 |
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 5,991 K, 1.4 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.10 to 1.93 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 191 years ago, around 1840.