145 G. Canis Majoris

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145 G. Canis Majoris
Observation data
Epoch J2000      Equinox J2000
Constellation Canis Major
Right ascension 07h 16m 36.83456s[1]
Declination −23° 18′ 56.1383″[1]
Apparent magnitude (V) 4.79[2]
Characteristics
Spectral type K3Ib-[3] or K4III[4]
B−V color index 1.710[2]
Distance
2,700 ± 200 ly
(820 ± 70 pc)
Details
If a giant star
Myr
HR 2764, SAO 173349, WDS J07166-2319A[9]
Database references
SIMBADdata

145 G. Canis Majoris (HD 56577) is a single

supergiant star in the southern constellation of Canis Major. This star is Gould's 145th of Canis Major in his Uranometria Argentina. [11] Kostjuk erroneously lists it as simply "145 CMa". SIMBAD follows this error in its object query result as "* 145 CMa – Star".[12]

The properties and evolutionary state of 145 G. CMa are disputed, it being classed either as a young massive supergiant or a somewhat older and less massive giant. It has been given two MK

spectral classifications: K3Ib[3] (corresponding to a supergiant) and K4III[4]
(corresponding to a giant). Tezzlaff et al. gives a large mass of 7.8 

Based on the assumption that it is a

Gaia DR2 parallax, it would have a luminosity of 14,000 L, rather high for a giant.[5] An older measurement based on the Hipparcos distance of 435 parsecs (1,420 ly) give a lower luminosity of 5,960 L.[14]

The star is one component of a close

.[15] The two stars appear to be unrelated and the close alignment accidental, with HD 56578 being a much closer and less luminous Am star.[16]

Notes

  1. ^ a b Applying the Stefan–Boltzmann law with a nominal solar effective temperature of 5,772 K:
    .

References