HD 204941 is 93.7 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this K1/2V star; the first was found in 2011 by radial velocity (La Silla Observatory).
Fly there in 3DHD 204941 b takes 4.7 years to go round its star once.
HD 204941 is one of 2 stars in its system: the other is drawn where the Washington Double Star Catalog measures it on the sky.
| Spectral type | K1/2V |
| Surface temperature | 5,026 K |
| Mass | 0.58 solar masses |
| Radius | 0.78 solar radii |
| Luminosity | 0.31 times the Sun |
| Apparent magnitude | 8.45 |
| Age | about 6.67 billion years |
| Distance from the Sun | 93.7 light-years (28.7 parsecs) |
| Position (J2000) | RA 323.0967°, Dec -20.9580° |
| Constellation | Capricornus |
HD 204941 B is a M0V star of magnitude 11.39, moving through space with it. In 2016 it was 56.1″ from HD 204941, at position angle 219° (Washington Double Star Catalog, 21324-2058 LDS6354): 1,611 AU on the sky at this distance. The true distance can only be larger.
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HD 204941 b | 4.7 years | 2.550 AU | 10.1 R⊕ estimated | 73.101 M⊕ minimum | Radial Velocity, 2011 |
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.