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Omega Carinae

Omega Carinae
Diagram showing star positions and boundaries of the Carina constellation and its surroundings
Cercle rouge 100%.svg

Location of ω Carinae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Right ascension 10h 13m 44.21739s
Declination –70° 02′ 16.4563″
Apparent magnitude (V) 3.29
Characteristics
Spectral type B8 IIIe
U−B color index –0.285
B−V color index –0.083
Astrometry
Radial velocity (Rv) +7.0 km/s
Proper motion (μ) RA: -36.01 mas/yr
Dec.: +7.09 mas/yr
Parallax (π) 9.54 ± 0.09mas
Distance 342 ± 3 ly
(104.8 ± 1.0 pc)
Details
Surface gravity (log g) 3.581 cgs
Temperature 13,275 K
Rotational velocity (v sin i) 245 km/s
Other designations
HR 4037, HD 89080, CP−69°1178, FK5 385, HIP 50099, SAO 250885.
Database references
SIMBAD data

Omega Carinae (ω Car, ω Carinae) is a star in the constellation Carina. With a declination greater than 70 degrees south of the celestial equator, it is the most southerly of the bright stars of Carina (third-magnitude or brighter), and it is part of a southern asterism known as the Diamond Cross. This star has an apparent visual magnitude of 3.3 and is located at a distance of about 342 light-years (105 parsecs) from Earth.

Omega Carinae has a stellar classification of B8 IIIe, which places it among a category known as Be stars that display emission lines of hydrogen their spectrum. Omega Carinae is a shell star, having a circumstellar disk of gas surrounding its equator. The luminosity class of III indicates it has evolved into a giant star, having exhausted the hydrogen at its core and left the main sequence. The effective temperature of 13,275 K in its outer envelope is what gives this star the blue-white hue that is characteristic of B-type stars.

This star is rotating rapidly with a projected rotational velocity of 245 km s−1, which gives a lower limit to the star's azimuthal velocity along the equator. The critical equatorial velocity, at which the star would begin to break up, is 320 km s−1. The star's axis of rotation is inclined by an estimated angle of 70.8° to the line of sight from the Earth.


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Wikipedia

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