HD 75289 is 95.0 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G0 star; the first was found in 1999 by radial velocity (La Silla Observatory).
Fly there in 3DHD 75289 b goes round its star every 3.51 days, 25 times as often as Mercury goes round the Sun.
HD 75289 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 | G0 |
| Surface temperature | 6,117 K |
| Mass | 1.29 solar masses |
| Radius | 1.23 solar radii |
| Luminosity | 2.053 times the Sun |
| Apparent magnitude | 6.35 |
| Age | about 5.6 billion years |
| Distance from the Sun | 95.0 light-years (29.1 parsecs) |
| Position (J2000) | RA 131.9182°, Dec -41.7378° |
| Constellation | Vela |
HD 75289 B is a M5 star of magnitude 11.8, judged a true companion. In 2017 it was 21.3″ from HD 75289, at position angle 77° (Washington Double Star Catalog, 08477-4144 MUG 6 AB): 620 AU on the sky at this distance. The true distance can only be larger.
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HD 75289 b | 3.51 days | 0.0500 AU | 14.2 R⊕ estimated | 155.74 M⊕ minimum | Radial Velocity, 1999 |
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.