Epsilon Muscae

Epsilon Muscae, Latinized as ε Muscae, is a red giant star of spectral type M5III in the constellation Musca. Originally a main-sequence star of around 1.5 to 2 solar masses, it is now on the asymptotic giant branch and has now expanded to 130 times the Sun's diameter and 1800 to 2300 its luminosity. It is a semiregular variable, varying between visual magnitudes 4.0 and 4.3 in eight distinct periods ranging from a month to over half a year in length. It is located around 300 light-years distant, the same distance 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.

Epsilon Muscae

A light curve for Epsilon Muscae, plotted from Hipparcos data
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Musca
Right ascension 12h 17m 34.27716s
Declination −67° 57 38.6486
Apparent magnitude (V) 4.0 - 4.3
Characteristics
Evolutionary stage asymptotic giant branch
Spectral type M5 III
Variable type SRb
Astrometry
Radial velocity (Rv)7.1±0.7 km/s
Proper motion (μ) RA: −231.04±0.13 mas/yr
Dec.: −26.39±0.13 mas/yr
Parallax (π)10.82 ± 0.17 mas
Distance301 ± 5 ly
(92 ± 1 pc)
Absolute magnitude (MV)−0.77
Details
Mass<1.5-2 M
Radius~130 R
Luminosity1800-2300 L
Temperature3400 K
Other designations
eps Mus, CPD-67 1931, HD 106849, HIP 59929, HR 4671, SAO 251830.
Database references
SIMBADdata
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