Gamma Muscae

Star in the constellation Musca From Wikipedia, the free encyclopedia

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.

A light curve for Gamma Muscae, plotted from TESS data[9]
Right ascension12h 32m 28.01343s[1]
Declination−72° 07 58.7597[1]
Quick facts Constellation, Right ascension ...
γ Muscae
Location of γ Muscae (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Musca
Right ascension 12h 32m 28.01343s[1]
Declination −72° 07 58.7597[1]
Apparent magnitude (V) 3.87[2]
Characteristics
Evolutionary stage main sequence[3][4]
Spectral type B5 V[5]
U−B color index −0.61[2]
B−V color index −0.15[2]
Variable type SPB
Astrometry
Radial velocity (Rv)2.5±7.4[6] 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]
Distance325 ± 4 ly
(100 ± 1 pc)
Absolute magnitude (MV)−1.1[7]
Details
Mass5.09[8] M
Radius4.17[8] R
Luminosity790[7] L
Surface gravity (log g)3.87[8] cgs
Temperature15,490[8] K
Rotational velocity (v sin i)205[5] km/s
Age67.7[8] Myr
Other designations
γ Mus, CD−70°997, FK5 487, GC 17672, HD 109026, HIP 61199, HR 4773, SAO 257000
Database references
SIMBADdata
Close

This is a B-type main-sequence star with a stellar classification of B5 V.[5] 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.[10] It is around five times as massive as the Sun.[11] 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.[5]

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.[7]

References

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