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Epsilon Muscae
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Epsilon Muscae
Location of ε Muscae (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Musca[1]
Right ascension 12h 17m 34.27564s[2]
Declination −67° 57′ 38.6525″[2]
Apparent magnitude (V) 4.0 – 4.3[3]
Characteristics
Evolutionary stage asymptotic giant branch[4]
Spectral type M5 III[5]
Variable type SRb[3]
Astrometry
Radial velocity (Rv)7.1±0.7[6] km/s
Proper motion (μ) RA: −230.607±0.187 mas/yr[2]
Dec.: −26.206±0.263 mas/yr[2]
Parallax (π)9.9915±0.2 mas[2]
Distance326 ± 7 ly
(100 ± 2 pc)
Absolute magnitude (MV)−0.77[1]
Details
Mass2±0.3[7] M
Radius116±9[7] R
Luminosity1,738[2] L
Surface gravity (log g)0.6±0.02[7] cgs
Temperature3,470±125[7] K
Other designations
ε Mus, CD−67 1216, CPD−67 1931, HD 106849, HIP 59929, HR 4671, SAO 251830
Database references
SIMBADdata

Epsilon Muscae, Latinized from ε Muscae, is a red giant star of spectral type M5III in the constellation Musca.[5] It is a 4th magnitude star, visible to the naked eye under good observing conditions. It is about 330 light-years from the Earth.[2]

A light curve for Epsilon Muscae, plotted from Hipparcos data[8]

Originally a main-sequence star of around 2 solar masses,[7] Epsilon Muscae is now on the asymptotic giant branch[4] and has expanded to 117 times the Sun's diameter and 1,700 its luminosity.[7] It is a semiregular variable, varying between visual magnitudes 4.0 and 4.3[3] in eight distinct periods ranging from a month to over half a year in length.[5] Its distance from the Earth is about the same as the Lower Centaurus–Crux subgroup of the Scorpius–Centaurus association, although it is moving much faster at around 100 km/s and does not share a common origin.[9]

References

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