Star in the constellation Sculptor
Mu Sculptoris
Location of μ Sculptoris (circled)
Observation dataEpoch J2000 Equinox J2000
Constellation
Sculptor
Right ascension
23 40 38.14898
Declination
−32° 04′ 23.2478″
Apparent magnitude (V)
5.30 (5.30 – 5.33)
Characteristics
Evolutionary stage
giant
Spectral type
K1 III
U−B color index
+0.69
B−V color index
+0.97
Variable type
suspected
Astrometry Radial velocity (Rv )+15.79±0.12 km/s Proper motion (μ) RA: −91.30 mas /yr Dec.: −53.29 mas /yr Parallax (π)11.6622 ± 0.1228 mas Distance 280 ± 3 ly (85.7 ± 0.9 pc ) Absolute magnitude (MV )0.54
Details Mass 1.32 M ☉ Radius 10.88+0.16 −0.13 R ☉ Luminosity 61.4±0.8 L ☉ Surface gravity (log g )2.50 cgs Temperature 4,899+29 −35 K Metallicity −0.21 dex Rotational velocity (v sin i )2.6 km/s
Other designations μ Scl , NSV 14661, CD −32°17621, FK5 1618, GC 32888, HD 222433, HIP 116820, HR 8975, SAO 214701, GSC 07515-01148
Database references SIMBAD data
μ Sculptoris , Latinized as Mu Sculptoris , is a solitary, orange-hued star in the southern constellation of Sculptor . It is visible to the naked eye as a dim point of light with an apparent visual magnitude of +5.30. This star is located approximately 291 light years from the Sun based on parallax , and it is drifting further away with a radial velocity of +16 km/s.
This object is an aging K-type giant star with a stellar classification of K1 III. Having exhausted the supply of hydrogen at its core , this star expanded and cooled off the main sequence . At present it has 11 times the girth of the Sun. It is a suspected variable star of unknown type, with its brightness measured as varying from magnitude 5.30 down to 5.33. The star has 1.32 times the mass of the Sun and is radiating 61 times the Sun's luminosity from its swollen photosphere at an effective temperature of 4899 K.
References
^ Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters . 38 (5): 331. arXiv :1108.4971 . Bibcode :2012AstL...38..331A . doi :10.1134/S1063773712050015 . S2CID 119257644 . Vizier catalog entry
^ Samus, N. N.; et al. (2017). "General Catalogue of Variable Stars". Astronomy Reports . 5.1. 61 (1): 80–88. Bibcode :2017ARep...61...80S . doi :10.1134/S1063772917010085 . S2CID 125853869 .
^ Hoffleit, D.; Warren, W. H. (1995). "Bright Star Catalogue". VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H . 5050 (5th Revised ed.). Bibcode :1995yCat.5050....0H .
Mermilliod, J. C. (2006). "Homogeneous Means in the UBV System". VizieR On-line Data Catalog: II/168. Originally Published in: Institut d'Astronomie . 2168 . Bibcode :2006yCat.2168....0M . Vizier catalog entry
Mallama, A. (2014). "Sloan Magnitudes for the Brightest Stars". The Journal of the American Association of Variable Star Observers . 42 (2): 443. Bibcode :2014JAVSO..42..443M . Vizier catalog entry
^ 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 . Vizier catalog entry
^ Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures". Astronomy and Astrophysics . 352 : 555–562. arXiv :astro-ph/9911002 . Bibcode :1999A&A...352..555A . Vizier catalog entry
De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (2014). "A catalog of rotational and radial velocities for evolved stars". Astronomy & Astrophysics . 561 : A126. arXiv :1312.3474 . Bibcode :2014A&A...561A.126D . doi :10.1051/0004-6361/201220762 . S2CID 54046583 . Vizier catalog entry
"mu Scl" . SIMBAD . Centre de données astronomiques de Strasbourg .
Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems" . Monthly Notices of the Royal Astronomical Society . 389 (2): 869–879. arXiv :0806.2878 . Bibcode :2008MNRAS.389..869E . doi :10.1111/j.1365-2966.2008.13596.x . S2CID 14878976 .
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Mu Sculptoris
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