Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Musca |
Right ascension | 12h 42m 05.02561s [2] |
Declination | −69° 24′ 27.1966″ [2] |
Apparent magnitude (V) | 5.93 - 6.73 [3] |
Characteristics | |
Spectral type | F7 Ib [4] - G2 [3] |
B−V color index | 0.750±0.020 [5] |
Variable type | δ Cep [3] |
Astrometry | |
Radial velocity (Rv) | +3.8±2.9 [6] km/s |
Proper motion (μ) |
RA: −4.180
[2]
mas/
yr Dec.: −2.127 [2] mas/ yr |
Parallax (π) | 1.0002 ± 0.0291 mas [2] |
Distance | 3,260 ± 90
ly (1,000 ± 30 pc) |
Absolute magnitude (MV) | -3.62 [7] |
Details | |
Radius | 65 [2] R☉ |
Luminosity | 2,541 [2] L☉ |
Surface gravity (log g) | 2.0±0.1 [8] cgs |
Temperature | 5,985±54 [7] K |
Metallicity [Fe/H] | +0.10±0.05 [8] dex |
Other designations | |
Database references | |
SIMBAD | data |
R Muscae is a yellow-white hued variable star in the southern constellation of Musca. It has a nominal apparent visual magnitude of 6.31, [5] which is near the lower limit of visibility to the naked eye. The distance to this star, as determined from its annual parallax shift of 1.00 mas, [2] is around 3,260 light years.
This is an F-type supergiant star with a baseline stellar classification of F7 Ib. [4] It is a Classical Cepheid variable ranging from apparent magnitude 5.93 to 6.73 [10] over 7.51 days, [7] while varying between spectral types F7 Ib and G2. [10] The star was suspected of having a detectable companion, [11] but this finding was later disputed. [12] Gaia and HST observations have shown that there is a companion, a 15th-magnitude star 7 ″ away. [13] [14] There is an X-ray source with a luminosity of 6.3×1029 erg s−1 located at an angular separation of 1.9 ″ from R Muscae. [15]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Musca |
Right ascension | 12h 42m 05.02561s [2] |
Declination | −69° 24′ 27.1966″ [2] |
Apparent magnitude (V) | 5.93 - 6.73 [3] |
Characteristics | |
Spectral type | F7 Ib [4] - G2 [3] |
B−V color index | 0.750±0.020 [5] |
Variable type | δ Cep [3] |
Astrometry | |
Radial velocity (Rv) | +3.8±2.9 [6] km/s |
Proper motion (μ) |
RA: −4.180
[2]
mas/
yr Dec.: −2.127 [2] mas/ yr |
Parallax (π) | 1.0002 ± 0.0291 mas [2] |
Distance | 3,260 ± 90
ly (1,000 ± 30 pc) |
Absolute magnitude (MV) | -3.62 [7] |
Details | |
Radius | 65 [2] R☉ |
Luminosity | 2,541 [2] L☉ |
Surface gravity (log g) | 2.0±0.1 [8] cgs |
Temperature | 5,985±54 [7] K |
Metallicity [Fe/H] | +0.10±0.05 [8] dex |
Other designations | |
Database references | |
SIMBAD | data |
R Muscae is a yellow-white hued variable star in the southern constellation of Musca. It has a nominal apparent visual magnitude of 6.31, [5] which is near the lower limit of visibility to the naked eye. The distance to this star, as determined from its annual parallax shift of 1.00 mas, [2] is around 3,260 light years.
This is an F-type supergiant star with a baseline stellar classification of F7 Ib. [4] It is a Classical Cepheid variable ranging from apparent magnitude 5.93 to 6.73 [10] over 7.51 days, [7] while varying between spectral types F7 Ib and G2. [10] The star was suspected of having a detectable companion, [11] but this finding was later disputed. [12] Gaia and HST observations have shown that there is a companion, a 15th-magnitude star 7 ″ away. [13] [14] There is an X-ray source with a luminosity of 6.3×1029 erg s−1 located at an angular separation of 1.9 ″ from R Muscae. [15]