HD 204313 is 156 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this G5 V star; the first was found in 2010 by radial velocity (La Silla Observatory).
Fly there in 3DHD 204313 c goes round its star every 35.0 days, 2.5 times as often as Mercury goes round the Sun.
| Spectral type | G5 V |
| Surface temperature | 5,767 K |
| Mass | 1.03 solar masses |
| Radius | 1.1 solar radii |
| Luminosity | 1.258 times the Sun |
| Apparent magnitude | 7.99 |
| Age | about 3.38 billion years |
| Distance from the Sun | 155.9 light-years (47.8 parsecs) |
| Position (J2000) | RA 322.0511°, Dec -21.7274° |
| Constellation | Capricornus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HD 204313 c | 35.0 days | 0.211 AU | 4.31 R⊕ estimated | 17.163 M⊕ minimum | Radial Velocity, 2015 |
| HD 204313 b | 5.6 years | 3.185 AU | 12.9 R⊕ estimated | 1466.8 M⊕ | Radial Velocity, 2010 |
| HD 204313 e | 20.1 years | 7.457 AU | 12.2 R⊕ estimated | 4868.2 M⊕ | Radial Velocity, 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.