Article · Wikipedia archive · Last revised Jul 20, 2026

S Muscae

S Muscae is a classical (δ) Cepheid variable star in the constellation Musca about 2,800 light years away.

Last revised
Jul 20, 2026
Read time
≈ 3 min
Length
704 w
Citations
26
Source
S Muscae
Location of S Muscae (circled)
Observation data
Epoch J2000      Equinox ICRS
Constellation Musca
Right ascension 12h 12m 47.01834s1
Declination −70° 09′ 06.4363″1
Apparent magnitude (V) 5.89 - 6.492
Characteristics
Spectral type F6Ib (F6-G02) + B5V3
U−B color index +0.664
B−V color index +1.004
Variable type δ Cepheid2
Astrometry
Radial velocity (Rv)−1.915 km/s
Proper motion (μ) RA: −7.791 mas/yr
Dec.: −0.601 mas/yr
Parallax (π)1.99±0.84 mas1
Distance2,798 ± 55 ly
(858±17 pc)6
Absolute magnitude (MV)−4.017
Orbit6
Period (P)506.3±0.5 days
Semi-major axis (a)(2.95±0.09)×10−3"
(2.53±0.09 AU)
Eccentricity (e)0.088±0.006
Inclination (i)144.7±2.8°
Longitude of the node (Ω)99.6±14.4°
Periastron epoch (T)2,457,165.9±4.4 JD
Argument of periastron (ω)
(secondary)
194.8±3.3°
Semi-amplitude (K1)
(primary)
14.85±0.03 km/s
Semi-amplitude (K2)
(secondary)
16.63±3.27 km/s
Details
S Mus A
Mass4.44±0.916 M
Radius65.18 R
Luminosity3,4677 L
Metallicity+0.189
S Mus B
Mass3.98±0.216 M
Temperature17,00010 K
Other designations
S Mus, HR 4645, SAO 251791, CD−69°977, GSC 09231-00752, HD 106111, GC 16679, HIP 59551, AAVSO 1207-69
Database references
SIMBADdata

S Muscae is a classical (δ) Cepheid variable star in the constellation Musca about 2,800 light years away.

A light curve for S Muscae, plotted from TESS data11 source ↗

S Muscae is a yellow supergiant ranging between spectral types F6Ib and G0Ib and magnitudes 5.89 to 6.49 over a period of 9.66 days.2 It is a luminous star around six times as massive as the Sun and 65.1 times the radius of the Sun. It is a binary star with a blue-white main sequence star companion likely to be of spectral type B3V to B5V with a mass of just over five solar masses,12 one of the hottest and brightest companions of a Cepheid known. The two stars orbit each other every 505 days.13

S Muscae has been found to lie within the faint star cluster ASCC 69.14

References

References

  1. Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.
  2. Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
  3. Skiff, B. A. (2014). "VizieR Online Data Catalog: Catalogue of Stellar Spectral Classifications (Skiff, 2009-2014)". VizieR On-line Data Catalog: B/Mk. Originally Published in: Lowell Observatory (October 2014). 1. Bibcode:2014yCat....1.2023S.
  4. Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
  5. Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; Levato, H.; Morrell, N. I.; Torres, G.; Udry, S. (2004). "SB9: The ninth catalogue of spectroscopic binary orbits". Astronomy and Astrophysics. 424 (2): 727–732. arXiv:astro-ph/0406573. Bibcode:2004A&A...424..727P. doi:10.1051/0004-6361:20041213. S2CID 119387088.
  6. Gallenne, A.; Kervella, P.; Borgniet, S.; Mérand, A.; Pietrzyński, G.; Gieren, W.; Monnier, J. D.; Schaefer, G. H.; Evans, N. R.; Anderson, R. I.; Baron, F.; Roettenbacher, R. M.; Karczmarek, P. (February 2019). "Multiplicity of Galactic Cepheids from long-baseline interferometry. IV. New detected companions from MIRC and PIONIER observations". Astronomy and Astrophysics. 622: A164. Bibcode:2019A&A...622A.164G. doi:10.1051/0004-6361/201834614. ISSN 0004-6361.
  7. Remage Evans, Nancy; Bond, Howard E.; Schaefer, Gail H.; Mason, Brian D.; Karovska, Margarita; Tingle, Evan (2013). "Binary Cepheids: Separations and Mass Ratios in 5 M ⊙ Binaries". The Astronomical Journal. 146 (4): 93. arXiv:1307.7123. Bibcode:2013AJ....146...93E. doi:10.1088/0004-6256/146/4/93. S2CID 34133110.
  8. Moskalik, P.; Gorynya, N. A. (2005). "Mean Angular Diameters and Angular Diameter Amplitudes of Bright Cepheids". Acta Astronomica. 55: 247. arXiv:astro-ph/0507076. Bibcode:2005AcA....55..247M.
  9. Klagyivik, P.; Szabados, L. (2009). "Observational studies of Cepheid amplitudes. I. Period-amplitude relationships for Galactic Cepheids and interrelation of amplitudes". Astronomy and Astrophysics. 504 (3): 959. arXiv:0908.3561. Bibcode:2009A&A...504..959K. doi:10.1051/0004-6361/200811464. S2CID 18283579.
  10. Evans, Nancy Remage; Massa, Derck; Fullerton, Alexander; Sonneborn, George; Iping, Rosina (2006). "Cepheid Masses: FUSE Observations of S Muscae". The Astrophysical Journal. 647 (2): 1387–1392. arXiv:astro-ph/0607489. Bibcode:2006ApJ...647.1387E. doi:10.1086/505519. S2CID 119020617.
  11. "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
  12. Bohm-Vitense, Erika; Remage Evans, Nancy; Carpenter, Kenneth; Beck-Winchatz, Bernhard; et al. (1997). "The Mass of the Classical Cepheid S Muscae". The Astrophysical Journal. 477 (2): 916. Bibcode:1997ApJ...477..916B. doi:10.1086/303725.
  13. Evans, Nancy Remage (1990). "The orbit and colors of the Cepheid S MUSCAE". Publications of the Astronomical Society of the Pacific. 102: 551. Bibcode:1990PASP..102..551E. doi:10.1086/132668.
  14. Remage Evans, Nancy; Pillitteri, Ignazio; Wolk, Scott; Guinan, Edward; Engle, Scott; Bond, Howard E.; Schaefer, Gail H.; Karovska, Margarita; Depasquale, Joseph; Tingle, Evan (2014). "X-Ray Detection of the Cluster Containing the Cepheid S Mus". The Astrophysical Journal Letters. 785 (2): L25. arXiv:1403.6939. Bibcode:2014ApJ...785L..25E. doi:10.1088/2041-8205/785/2/L25. S2CID 119113620.