Luminous variable star in the constellation Carina
AG Carinae
AG Car (Hubble Space Telescope image)
Observation data Epoch J2000 Equinox J2000
Constellation
Carina
Right ascension
10h 56m 11.57814s[1]
Declination
−60° 27′ 12.8107″[1]
Apparent magnitude (V)
6.96[2](5.7–9.0)[3]
Characteristics
Spectral type
LBV[4]
U−B color index
−0.58[2]
B−V color index
+0.61[2]
Variable type
LBV[5]
Astrometry
Proper motion (μ)
RA: −4.808[1] mas/yr Dec.: +1.955[1] mas/yr
Parallax (π)
0.1925 ± 0.0165 mas[1]
Distance
17,000 ± 1,000 ly (5,200 ± 400 pc)
Absolute magnitude (MV)
~−8 (at minimum)[4]
Details
Mass
55[6]M☉
Radius
50[7]–552[8]R☉
Luminosity
600,000–900,000[9][a]L☉
Temperature
8,000–26,000[7] K
Rotation
13±2[10] days
Rotational velocity (v sin i)
220±50[10] km/s
Other designations
CD–59°3430, HD 94910, HIP 53461, SAO 251185, WR 31b, AAVSO 1052–69
Database references
SIMBAD
data
AG Carinae (AG Car) is a star in the constellation Carina. It is classified as a luminous blue variable (LBV) and is one of the most luminous stars in the Milky Way. The great distance (20,000 light-years) and intervening dust mean that the star is not usually visible to the naked eye; its apparent brightness varies erratically between magnitude 5.7 and 9.0.
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AGCarinae (AG Car) is a star in the constellation Carina. It is classified as a luminous blue variable (LBV) and is one of the most luminous stars in...
plus a handful in other local group galaxies. η Carinae P Cygni AGCarinae HR Carinae V432 Carinae (Wray 15-751) V4029 Sagittarii (HD 168607) V905 Scorpii...
energy going into expansion of a substantial portion of the star. AGCarinae and HR Carinae show similar luminosity decreases in some studies, but in the...
AGCarinae in 1914 by H. E. Wood, this object was announced as a candidate variable star. A year later it was determined by R. Innis that it was AG Carinae...
mass is currently being ejected as a nebula around the star (similar to AGCarinae), which was imaged by the Very Large Telescope in 2010. The nebula was...
the disappearance of a bright star of the galaxy. AGCarinae Markarian 177 LBV 1806-20 Eta Carinae Kehrig, C.; Iglesias-Páramo, J.; Vílchez, J. M.; Gil...
iron and P Cygni profiles on some lines. By 1970, HR Carinae and the similar variable AGCarinae were recognised as being related to the P Cygni variables...
distance to WR 31a as well as to its neighbor, the luminous blue variable AGCarinae. It was thought that, if this distance was confirmed by Gaia's second...
S2CID 11978733. Gull, Theodore R.; Damineli, Augusto (November 2009). "JD13 – Eta Carinae in the Context of the Most Massive Stars". Proceedings of the International...
example, since Argo Navis's gamma star went to Vela, there is no Gamma Carinae. List of stars by constellation Gray, R. O.; Garrison, R. F. (1989-02-01)...
scorpion has darkened or granular raised linear ridges, called "keels" or "carinae" on the pedipalp segments and on other parts of the body; these are useful...
large outbursts in the 17th century. Similar events have been seen in Eta Carinae and possibly a handful of extra-galactic objects. P Cygni does show evidence...
example: open star cluster Carraro 1 at 10:37:00 / -58°44'00") (NW of the Eta Carinae Nebula) CBB — (open star clusters) CCCP-Cl — (open star clusters) CCCP-Gp...
of modifiers; e.g., the nasal caputegulae sit atop the nasal bones. carinaeCarinae (singular: carina) are enamel ridges that form the cutting edges on...
1843 – Chile takes possession of the Strait of Magellan. April – Eta Carinae is temporarily the second-brightest star in the night sky. September 23...
Cimicomorpha) from Myanmar, with the analysis of the evolution of hood, carinae and paranota". Zoological Systematics. 43 (3): 283–293. doi:10.11865/zs...