HR Carinae

HR Car

HR Carinae and its nebula in Hydrogen-alpha with MUSE
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Carina
Right ascension 10h 22m 53.84301s
Declination −59° 37′ 28.3636″
Apparent magnitude (V) 6.95–8.80
Characteristics
Spectral type LBV + RSG
U−B color index −0.22
B−V color index +0.92
Variable type LBV
Astrometry
Proper motion (μ) RA: –6.319 mas/yr
Dec.: +2.332 mas/yr
Parallax (π)0.2032±0.0166 mas
Distance16,000 ± 1,000 ly
(4,900 ± 400 pc)
Absolute magnitude (MV)−9.4
Orbit
Period (P)4557.5±21.0 days
Semi-major axis (a)3.324±0.026"
(18 AU)
Eccentricity (e)0.4±0.2
Inclination (i)119.2±0.7°
Details
LBV
Mass25–40 M
Radius220±60 (100–350) R
Luminosity416,000–790,000 L
Temperature7,900–21,900 K
Rotational velocity (v sin i)150 km/s
RSG
Mass9–20 M
Radius500±150 R
Temperature3,600–4,000 K
Other designations
HR Car, HD 90177, HIP 50843, SAO 238005, CD-59 3044, GC 14276, MWC 202, AAVSO 1019-59
Database references
SIMBADdata

HR Carinae is a luminous blue variable star located in the constellation Carina. It is surrounded by a vast nebula of ejected nuclear-processed material because this star has a multiple shell expanding atmosphere. This star is among the most luminous stars in the Milky Way. It has very broad emission wings on the Balmer lines, reminiscent from the broad lines observed in the spectra of O and Wolf–Rayet stars. A distance of 5 kpc and a bolometric magnitude of −9.4 put HR Car among the most luminous stars of the galaxy.