Mu Muscae

Mu Muscae, Latinized from μ Muscae, is a solitary star in the southern constellation of Musca. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of around 4.75. Based upon an annual parallax shift of 7.21 mas as seen from Earth, it is located about 450 light years from the Sun. The star is drifting further away with a radial velocity of +37 km/s.

Mu Muscae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Musca
Right ascension 11h 48m 14.53282s
Declination −66° 48 53.6712
Apparent magnitude (V) 4.6 - 4.8
Characteristics
Spectral type K4 III
U−B color index +1.89
B−V color index +1.54
Variable type Lb
Astrometry
Radial velocity (Rv)+37.4±2.8 km/s
Proper motion (μ) RA: −31.223 mas/yr
Dec.: −15.938 mas/yr
Parallax (π)7.2113 ± 0.1762 mas
Distance450 ± 10 ly
(139 ± 3 pc)
Absolute magnitude (MV)−0.85
Details
Radius52.92+1.01
−0.95
 R
Luminosity602.0±16.9 L
Temperature3,930+36
−37
 K
Other designations
μ Mus, CD−66° 1114, HD 102584, HIP 57581, HR 4530, SAO 251597
Database references
SIMBADdata

This is an evolved K-type giant star with a stellar classification of K4 III, having exhausted the supply of hydrogen at its core then cooled and expanded to 53 times the Sun's radius. It most likely on the red giant branch, rather than the asymptotic giant branch, and shows no signs of mass loss. Mu Muscae is a type Lb, oxygen-rich irregular variable with a small amplitude that ranges in visual magnitude between 4.71 and 4.76. It is radiating 602 times the luminosity of the Sun from its photosphere at an effective temperature of 3,930 K.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.