HD 101930 is 97.9 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this K1 V star; the first was found in 2005 by radial velocity (La Silla Observatory).
Fly there in 3DHD 101930 b goes round its star every 70.5 days, 1.2 times as often as Mercury goes round the Sun.
HD 101930 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 V |
| Surface temperature | 5,108 K |
| Mass | 0.57 solar masses |
| Radius | 0.86 solar radii |
| Luminosity | 0.49 times the Sun |
| Apparent magnitude | 8.21 |
| Age | about 1 billion years |
| Distance from the Sun | 97.9 light-years (30.0 parsecs) |
| Position (J2000) | RA 175.8756°, Dec -58.0054° |
| Constellation | Centaurus |
HD 101930 B has no spectral type listed of magnitude 10.72, judged a true companion. In 2015 it was 73″ from HD 101930, at position angle 8° (Washington Double Star Catalog, 11435-5800 MUG 9): 2,192 AU on the sky at this distance. The true distance can only be larger. Its colour is estimated from its brightness.
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HD 101930 b | 70.5 days | 0.300 AU | 10.6 R⊕ estimated | 79.457 M⊕ minimum | Radial Velocity, 2005 |
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.