QZ Puppis
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Puppis |
| Right ascension | 07h 52m 38.64663s |
| Declination | −38° 51′ 46.1305″ |
| Apparent magnitude (V) | 4.47 - 4.54 |
| Characteristics | |
| Spectral type | B2.5V |
| U−B color index | −0.68 |
| B−V color index | -0.20 |
| Variable type | ellipsoidal |
| Astrometry | |
| Radial velocity (Rv) | +29.50 km/s |
| Proper motion (μ) | RA: −8.92 mas/yr Dec.: +3.34 mas/yr |
| Parallax (π) | 5.03±0.19 mas |
| Distance | 650 ± 20 ly (199 ± 8 pc) |
| Absolute magnitude (MV) | −2.00 |
| Details | |
| Mass | 6.0 M☉ |
| Radius | 7.3 R☉ |
| Luminosity | 2,268 L☉ |
| Surface gravity (log g) | 3.5 cgs |
| Temperature | 15,254 K |
| Metallicity [Fe/H] | −0.15 dex |
| Rotational velocity (v sin i) | 151 km/s |
| Age | 24.1 Myr |
| Other designations | |
| b Puppis, QZ Pup, CD−38°3769, GC 10661, GSC 07646-03591, HIP 38455, HR 3084, HD 64503, NSV 3789, SAO 198545 | |
| Database references | |
| SIMBAD | data |
QZ Puppis (QZ Pup, b Pup) is a class B2.5V (blue main-sequence) star in the constellation Puppis. Its apparent magnitude is 4.5 and it is approximately 650 light years away based on parallax.
QZ Puppis was identified as a small-amplitude variable star in 1974, but the nature of the variability was unclear. It was thought to be a spectroscopic binary on the basis of variability in the radial velocity of its spectral lines. As a hot B-class main sequence star with variable spectral lines, it was suspected of being a β Cephei variable but this classification was repeatedly rejected. The short-period sinusoidal variations in brightness with an amplitude of 0.03 magnitudes were interpreted as ellipsoidal variations as the star, distorted by a close companion, rotates with a period of 1.1 days. Later analysis of Hipparcos photometry detected shallow eclipses.
The companion to QZ Puppis is only known from its effect on the visible star as they orbit. The primary shows radial velocity variations of 71 km/s as it orbits every 1.112 days.