 Star map shows star position on the northern edge of the constellation Crux | |
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Crux |
| Right ascension | 12h 17m 53.191430s[1] |
| Declination | −55° 58′ 31.8904″[1] |
| Apparent magnitude (V) | 7.80[2] |
| Characteristics | |
| Spectral type | F5 V[3] |
| B−V color index | 0.458±0.003[2] |
| Astrometry | |
| Radial velocity (Rv) | +10.2±1.7[2] km/s |
| Proper motion (μ) | RA: −39.014[1] mas/yr Dec.: −12.872[1] mas/yr |
| Parallax (π) | 9.6774 ± 0.0429 mas[1] |
| Distance | 337 ± 1 ly (103.3 ± 0.5 pc) |
| Absolute magnitude (MV) | 2.99[2] |
| Details | |
| Radius | 2.03+0.11 −0.10[1] R☉ |
| Luminosity | 6.56±0.04[1] L☉ |
| Temperature | 6,484+157 −168[1] K |
| Metallicity [Fe/H] | −0.04±0.08[2] dex |
| Age | 13±2[4] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 106906 is a binary star[6] system in the southern constellation of Crux. It is too faint to be visible to the naked eye, having a combined apparent visual magnitude of 7.80.[2] The distance to this system is approximately 337 light years based on parallax, and it is receding from the Sun with a radial velocity of +10 km/s.[2] It is a member of the Lower Centaurus–Crux group of the Scorpius–Centaurus OB association of co-moving stars.[4]
This is a double-lined spectroscopic binary system consisting of two F-type main-sequence stars with similar masses and a matching stellar classification of F5 V.[6] Their orbital period is less than 100 days.[4]
