HD 164922 is 71.8 light-years from the Sun. The NASA Exoplanet Archive lists 4 planets around this G9 V star; the first was found in 2005 by radial velocity (W. M. Keck Observatory).
Fly there in 3DHD 164922 d goes round its star every 12.5 days, 7 times as often as Mercury goes round the Sun.
| Spectral type | G9 V |
| Surface temperature | 5,390 K |
| Mass | 0.926 solar masses |
| Radius | 0.946 solar radii |
| Luminosity | 0.71 times the Sun |
| Apparent magnitude | 7.01227 |
| Age | about 9.58 billion years |
| Distance from the Sun | 71.8 light-years (22.0 parsecs) |
| Position (J2000) | RA 270.6305°, Dec 26.3104° |
| Constellation | Hercules |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HD 164922 d | 12.5 days | 0.103 AU | 1.83 R⊕ estimated | 4 M⊕ minimum | Radial Velocity, 2020 |
| HD 164922 e | 41.8 days | 0.229 AU | 3.23 R⊕ estimated | 10.52 M⊕ minimum | Radial Velocity, 2021 |
| HD 164922 c | 75.7 days | 0.341 AU | 3.66 R⊕ estimated | 13 M⊕ minimum | Radial Velocity, 2016 |
| HD 164922 b | 3.3 years | 2.160 AU | 13.3 R⊕ estimated | 116 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.