HIP 67522
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Centaurus |
| Right ascension | 13h 50m 06.280s |
| Declination | −40° 50′ 08.88″ |
| Apparent magnitude (V) | 9.80±0.03 |
| Characteristics | |
| Evolutionary stage | Main sequence |
| Spectral type | G0V |
| Astrometry | |
| Radial velocity (Rv) | 8.26±2.19 km/s |
| Proper motion (μ) | RA: −28.907 mas/yr Dec.: −22.248 mas/yr |
| Parallax (π) | 8.0170±0.0182 mas |
| Distance | 406.8 ± 0.9 ly (124.7 ± 0.3 pc) |
| Details | |
| Mass | 1.22±0.05 M☉ |
| Radius | 1.38±0.06 R☉ |
| Luminosity | 1.75±0.09 L☉ |
| Temperature | 5,675±75 K |
| Rotation | 1.418±0.016 days |
| Rotational velocity (v sin i) | 54.2±0.7 km/s |
| Age | 17±2 Myr |
| Other designations | |
| CD−40 8189, HD 120411, HIP 67522, TOI-6551, TIC 166527623 | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
HIP 67522 is a G-type main sequence star located at a distance of 407 light-years (125 parsecs) away in the constellation of Centaurus. Its visual magnitude of 9.8 makes it much too faint to be seen by the unaided eye. It is slightly larger than the Sun (1.38 R☉) but cooler (5,675 K versus 5,772 K for the Sun). It is also very young being only around 17 million years old. It has two exoplanets orbiting it.