Gamma Canis Majoris

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γ Canis Majoris
Template:Location mark
Location of γ Canis Majoris (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Canis Major
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) +4.10[2]
Characteristics
Spectral type B8II[3]
U−B Template:Engvar −0.45[2]
B−V Template:Engvar −0.13[2]
Astrometry
Radial velocity (Rv)+32.0[4] km/s
Proper motion (μ) RA: −0.14[1] mas/yr
Dec.: −11.36[1] mas/yr
Parallax (π)7.38±0.21 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−1.4[5]
Details
Radius5.205[6] Template:Solar radius
Luminosity750[6] Template:Solar luminosity
Surface gravity (log g)3.5[7] cgs
Temperature13,200[6] K
Metallicity [Fe/H]−0.24[8] dex
Rotation6.214[6] days
Rotational velocity (v sin i)30[9] km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Muliphein, Muliphen, 23 Canis Majoris, BD−15°1625, FK5 271, HD 53244, HR 2657, HIP 34045, SAO 152303
Database references
SIMBADdata

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Gamma Canis Majoris (γ Canis Majoris, abbreviated Gamma CMa, γ CMa), also named Muliphein Template:IPAc-en,[10] is a star in the constellation of Canis Major. It is unclear exactly why this relatively faint star was given the 'gamma' designation, but possibly because it is in the same part of the constellation as Sirius (alpha) and Mirzam (beta).

Nomenclature

γ Canis Majoris (Latinised to Gamma Canis Majoris) is the star's Bayer designation.

It bore the traditional name Muliphein,[11] not to be confused with Muhlifain, which is Gamma Centauri; both names derive from the same Arabic root, محلفين muħlifayn. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[12] to catalogue and standardize proper names for stars. The WGSN approved the name Muliphein for this star on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names.[10]

Properties

Gamma Canis Majoris is a blue-white B-type bright giant with a stellar classification of B8II[3] and an apparent magnitude of +4.11. It is approximately 440 light-years from Earth. It is a chemically peculiar Hg–Mg star displaying abnormal lines of mercury and magnesium.[13] This star has 5.2 times the radius of the Sun and the outer atmosphere has an effective temperature of Script error: No such module "val"..[6]

This star is suspected of being a spectroscopic binary system, and there is a candidate companion at an angular separation of 0.332″ along a position angle of 114.8°.[13] It is a member of the Collinder 121 open cluster.[14]

Modern legacy

Muliphein appears on the flag of Brazil, symbolizing the state of Rondônia.[15]

The US Navy cargo ship USS Muliphen (AKA-61) was named after the star.

References

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Template:Stars of Canis Major

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