HD 76728

Suspected binary star system in the constellation Carina From Wikipedia, the free encyclopedia

HD 76728 is a suspected astrometric binary[7] star system in the constellation Carina. It has the Bayer designation c Carinae; HD 76728 is the identifier from the Henry Draper catalogue. The visible component has a blue-white hue and is visible to the naked eye with an apparent visual magnitude of +3.84.[1] The system is located at a distance of approximately 320 light years from the Sun based on parallax,[2] and it is drifting further away with a radial velocity of around +25 km/s.[1] It is a candidate member of the Volans-Carina Association of co-moving stars.[8]

Right ascension08h 55m 02.82822s[2]
Declination−60° 38 40.5998[2]
Quick facts Constellation, Right ascension ...
HD 76728
Location of c Carinae (circled in red)
Observation data
Epoch J2000.0      Equinox ICRS
Constellation Carina[1]
Right ascension 08h 55m 02.82822s[2]
Declination −60° 38 40.5998[2]
Apparent magnitude (V) +3.84[1]
Characteristics
Spectral type B8/9II[3]
B−V color index −0.104±0.006[1]
Variable type Constant[4]
Astrometry
Radial velocity (Rv)+25.0±4.1[1] km/s
Proper motion (μ) RA: −28.18[2] mas/yr
Dec.: +41.48[2] mas/yr
Parallax (π)10.20±0.10 mas[2]
Distance320 ± 3 ly
(98.0 ± 1.0 pc)
Absolute magnitude (MV)−1.12[1]
Details
Radius4.057[5] R
Luminosity446[5] L
Temperature13,180[5] K
Other designations
c Car, CPD−60°1243, FK5 336, GC 12359, HD 76728, HIP 43783, HR 3571, SAO 250374, CCDM J08550-6039, WDS J08550-6039A[6]
Database references
SIMBADdata
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The visible component is an aging bright giant star with a stellar classification of B8/9II.[3] The spectrum of the star displays metallic lines of magnesium.[9] The Volans-Carina Association to which it belongs has an age of 90 million years.[8] The star has four times the radius of the Sun and is radiating 450 times the Sun's luminosity from its photosphere at an effective temperature of 13,180 K.[5]

References

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