Red supergiant star in the constellation of Puppis From Wikipedia, the free encyclopedia
MZ Puppis is a red supergiant star in the constellation of Puppis. It has a radius of 400 R☉[8] and a mass of 14 solar masses, similar to Betelgeuse.
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Puppis |
Right ascension | 08h 04m 16.19s[2] |
Declination | −32° 40′ 29.4″[2] |
Apparent magnitude (V) | 5.20 - 5.44[3] |
Characteristics | |
Evolutionary stage | Red supergiant |
Spectral type | M1Iab-Ib[4] |
Variable type | LC?[3] |
Astrometry | |
Radial velocity (Rv) | +35.90[5] km/s |
Proper motion (μ) | RA: −5.736[2] mas/yr Dec.: +6.830[2] mas/yr |
Parallax (π) | 0.8126 ± 0.1013 mas[2] |
Distance | approx. 4,000 ly (approx. 1,200 pc) |
Absolute magnitude (MV) | −4.8[6] |
Details | |
Mass | 14[7] M☉ |
Radius | 400[8] R☉ |
Luminosity | 26,550 - 28,580[8] L☉ |
Surface gravity (log g) | −0.92[9] cgs |
Temperature | 3,745±170[8] K |
Age | 25[10] Myr |
Database references | |
SIMBAD | data |
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