HD 143183

Star in the constellation Norma From Wikipedia, the free encyclopedia

HD 143183 is a red supergiant variable star of spectral type M3Ia[6] or K2[3] in the constellation Norma. It is a member of the Norma OB1 association, at a distance of about 2 kiloparsecs. It is one of the most luminous red supergiants with a luminosity over 250,000 times greater than the Sun (L), and is as well one of the largest stars with a radius more than a thousand times that of the Sun (R).[4] Older studies frequently calculated higher luminosities, which would correspond to larger radii.[9][14] It has an estimated mass loss rate of 5×10−5 M per year[9] and has been once described as a cool hypergiant.[5] It is surrounded by a dozen early-type stars and a circumstellar nebula which extends 0.12 parsecs (0.39 ly).

Right ascension16h 01m 22.2226s[2]
Declination−54° 08 35.607[2]
Quick facts Constellation, Right ascension ...
HD 143183

HD 143183 (brightest star in the image) as seen from the Rutherfurd Observatory.
Observation data
Epoch J2000      Equinox J2000
Constellation Norma[1]
Right ascension 16h 01m 22.2226s[2]
Declination −54° 08 35.607[2]
Apparent magnitude (V) 7.3 - 8.6[3]
Characteristics
Evolutionary stage Red supergiant[4] or hypergiant[5]
Spectral type M3 Ia[6] or K2[3]
U−B color index +0.75[7]
B−V color index +2.10[7]
Variable type LB[3]
Astrometry
Radial velocity (Rv)−39.67±0.66[2] km/s
Proper motion (μ) RA: −1.1[8] mas/yr
Dec.: +13.1[8] mas/yr
Parallax (π)0.5559±0.1021 mas[2]
Distance6,850±650[9] ly
(2,100±200[9] pc)
Absolute magnitude (MV)−7.5[10]
Details
Mass20[9] M
Radius1,261[4] R
Luminosity254,000[4] L
Surface gravity (log g)−0.6[9] cgs
Temperature3,443[11]  3,605[6] K
Other designations
V558 Nor, CD−53 6947, HD 143183, IRAS 15576−5400, 2MASS J16013621−5408356[12]
Database references
SIMBADdata
Close
A visual band light curve for V558 Normae, plotted from ASAS data[13]

HD 143183 is catalogued with the variable star designation V558 Normae as its brightness varies irregularly between apparent magnitudes 7.3 and 8.6.[3]

It is possible that HD 143183 is a spectroscopic binary with an OB+ companion, but this is considered doubtful.[9] HD 143183 lies approximately 1' from the 10th-magnitude O-class bright giant CD−53 6363, the second-brightest star in the cluster.

References

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