HIP 65 A is 202 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this K4 V star; the first was found in 2020 by transit (Transiting Exoplanet Survey Satellite (TESS)).
Fly there in 3DHIP 65 A b goes round its star every 23.5 hours, 90 times as often as Mercury goes round the Sun.
HIP 65 A 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 | K4 V |
| Surface temperature | 4,590 K |
| Mass | 0.781 solar masses |
| Radius | 0.7242 solar radii |
| Luminosity | 0.2099 times the Sun |
| Apparent magnitude | 11 |
| Age | about 4.1 billion years |
| Distance from the Sun | 201.5 light-years (61.8 parsecs) |
| Position (J2000) | RA 0.1856°, Dec -54.8308° |
| Constellation | Phoenix |
HIP 65 B has no spectral type listed of magnitude 16.12, moving through space with it. In 2016 it was 3.8″ from HIP 65 A, at position angle 322° (Washington Double Star Catalog, 00007-5450 KPP2838 AB): 235 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 |
|---|---|---|---|---|---|
| HIP 65 A b | 23.5 hours | 0.0178 AU | 22.754 R⊕ | 1021.2 M⊕ | Transit, 2020 |
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.