Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Puppis |
Right ascension | 07h 52m 38.64663s [1] |
Declination | −38° 51′ 46.1305″ [1] |
Apparent magnitude (V) | 4.47 - 4.54 [2] |
Characteristics | |
Spectral type | B2.5V [3] |
U−B color index | −0.68 [4] |
B−V color index | -0.20 [4] |
Variable type | ellipsoidal [2] |
Astrometry | |
Radial velocity (Rv) | +29.50 [5] km/s |
Proper motion (μ) |
RA: −8.92
[1]
mas/
yr Dec.: +3.34 [1] mas/ yr |
Parallax (π) | 5.03 ± 0.19 mas [1] |
Distance | 650 ± 20
ly (199 ± 8 pc) |
Absolute magnitude (MV) | −2.00 [6] |
Details | |
Mass | 6.0 [7] M☉ |
Radius | 7.3 [7] R☉ |
Luminosity | 2,268 [7] L☉ |
Surface gravity (log g) | 3.5 [7] cgs |
Temperature | 15,254 [7] K |
Metallicity [Fe/H] | −0.15 [8] dex |
Rotational velocity (v sin i) | 151 [9] km/s |
Age | 24.1 [10] Myr |
Other designations | |
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. [12] 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. [13] 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. [12] Later analysis of Hipparcos photometry detected shallow eclipses. [14]
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.
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Puppis |
Right ascension | 07h 52m 38.64663s [1] |
Declination | −38° 51′ 46.1305″ [1] |
Apparent magnitude (V) | 4.47 - 4.54 [2] |
Characteristics | |
Spectral type | B2.5V [3] |
U−B color index | −0.68 [4] |
B−V color index | -0.20 [4] |
Variable type | ellipsoidal [2] |
Astrometry | |
Radial velocity (Rv) | +29.50 [5] km/s |
Proper motion (μ) |
RA: −8.92
[1]
mas/
yr Dec.: +3.34 [1] mas/ yr |
Parallax (π) | 5.03 ± 0.19 mas [1] |
Distance | 650 ± 20
ly (199 ± 8 pc) |
Absolute magnitude (MV) | −2.00 [6] |
Details | |
Mass | 6.0 [7] M☉ |
Radius | 7.3 [7] R☉ |
Luminosity | 2,268 [7] L☉ |
Surface gravity (log g) | 3.5 [7] cgs |
Temperature | 15,254 [7] K |
Metallicity [Fe/H] | −0.15 [8] dex |
Rotational velocity (v sin i) | 151 [9] km/s |
Age | 24.1 [10] Myr |
Other designations | |
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. [12] 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. [13] 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. [12] Later analysis of Hipparcos photometry detected shallow eclipses. [14]
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.