HIP 14810 is 165 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this G5 star; the first was found in 2005 by radial velocity (W. M. Keck Observatory).
Fly there in 3DHIP 14810 b goes round its star every 6.67 days, 13 times as often as Mercury goes round the Sun.
| Spectral type | G5 |
| Surface temperature | 5,544 K |
| Mass | 1.01 solar masses |
| Radius | 1.07 solar radii |
| Luminosity | 0.9772 times the Sun |
| Apparent magnitude | 8.52 |
| Age | about 5.84 billion years |
| Distance from the Sun | 164.6 light-years (50.5 parsecs) |
| Position (J2000) | RA 47.8093°, Dec 21.0971° |
| Constellation | Aries |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HIP 14810 b | 6.67 days | 0.0696 AU | 13 R⊕ estimated | 1239.5 M⊕ minimum | Radial Velocity, 2005 |
| HIP 14810 c | 147.7 days | 0.549 AU | 13.6 R⊕ estimated | 416.36 M⊕ minimum | Radial Velocity, 2006 |
| HIP 14810 d | 981.8 days | 1.940 AU | 14.1 R⊕ estimated | 187.52 M⊕ minimum | Radial Velocity, 2009 |
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 5,544 K, 0.98 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.95 to 1.69 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 165 years ago, around 1860.