Gamma Muscae

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Template:Short description

γ Muscae
Template:Location mark
Location of γ Muscae (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Musca
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 3.87[2]
Characteristics
Spectral type B5 V[3]
U−B Template:Engvar −0.61[2]
B−V Template:Engvar −0.15[2]
Variable type SPB
Astrometry
Radial velocity (Rv)Script error: No such module "val".[4] km/s
Proper motion (μ) RA: −51.34[1] mas/yr
Dec.: −5.40[1] mas/yr
Parallax (π)10.04±0.13 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−1.1[5]
Details
Mass5.09[6] Template:Solar mass
Radius4.17[6] Template:Solar radius
Luminosity790[5] Template:Solar luminosity
Surface gravity (log g)3.87[6] cgs
Temperature15,490[6] K
Rotational velocity (v sin i)205[3] km/s
Age67.7[6] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist
Database references
SIMBADdata

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γ Muscae, Latinised as Gamma Muscae, is a blue-white hued star in the southern circumpolar constellation of Musca, the Fly. It can be seen with the naked eye, having an apparent visual magnitude of 3.87.[2] Based upon an annual parallax shift of 10.04 mas as seen from Earth, it is located about 325 light years from the Sun.

File:GammaMusLightCurve.png
A light curve for Gamma Muscae, plotted from TESS data[7]

This is a B-type main-sequence star with a stellar classification of B5 V.[3] It is a variable star that ranges between magnitudes 3.84 and 3.86 over a period of 2.7 days, and is classed as a slowly pulsating B star.[8] It is around five times as massive as the Sun.[9] The star is spinning rapidly with a projected rotational velocity of 205 km/s. This is giving it an oblate shape with an equatorial bulge that is 7% larger than the polar radius.[3]

Gamma Muscae is a proper motion member of the Lower Centaurus–Crux sub-group in the Scorpius–Centaurus OB association, the nearest such association of co-moving massive stars to the Sun.[5]

References

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