Triple star system in the constellation Cassiopeia
YZ Cas Location of YZ Cassiopeiae (circled)
Observation dataEpoch J2000 Equinox J2000 Constellation Cassiopeia [ 1] A Right ascension 00h 45m 39.0777s [ 2] Declination +74° 59′ 17.063″[ 2] Apparent magnitude (V)5.653[ 3] B Right ascension 00h 45m 42,1503s [ 4] Declination +74° 58′ 43.242″[ 4] Apparent magnitude (V)11.23[ 5] Characteristics A Spectral type A2IV[ 6] (A1Vm + F2V[ 7] ) U−Bcolor index +0.07[ 5] B−Vcolor index +0.05[ 5] Variable type Algol [ 8] B Spectral type F2V[ 9] U−Bcolor index +0.64[ 5] B−Vcolor index +0.94[ 5] Astrometry Radial velocity (Rv )+8.90±0.4[ 10] km/s Proper motion (μ)RA: −15.07[ 2] mas /yr Dec.: −22.17[ 2] mas /yr Parallax (π)11.24± 0.55 mas [ 2] Distance 103.8[ 9] pc Absolute magnitude (MV )+0.251[ 7] Orbit [ 11] Companion TYC 4307-2168-1Period (P)86 580 yr Orbit [ 9] Primary Aa Companion Ab Period (P)4.467 days Semi-major axis (a)17.47 R ☉ [ 12] Eccentricity (e)0.0 Inclination (i)88.332° Details Aa Mass 2.308[ 12] M ☉ Radius 2.547[ 12] R ☉ Luminosity 41.69[ 12] L ☉ Surface gravity (log g )3.988[ 9] cgs Temperature 9,200[ 12] K Rotational velocity (v sin i )29.2[ 9] km/s Ab Mass 1.325[ 13] M ☉ Radius 1.359[ 12] R ☉ Luminosity 3.34[ 12] L ☉ Surface gravity (log g )4.311[ 9] cgs Temperature 6,890[ 13] K Metallicity [Fe/H] +0.10[ 13] dex Rotational velocity (v sin i )15.0[ 9] km/s Age 490 - 550[ 9] Myr Other designations 21 Cassiopeiae,HR 192,BD +74 27,HD 4161,SAO 4216,HIP 3572,GC 891,ADS 624 A,CCDM J00457+7459[ 14] Database references SIMBAD data
YZ Cassiopeiae (21 Cas) is astar system 103.8parsecs (339 ly ) away fromEarth , in the constellationCassiopeia . It comprises three stars: an eclipsingAlgol -type binary and a visually fainter star about 3000AU distant.[ 11] It is faintly visible to thenaked eye under good observing conditions.
Alight curve for YZ Cassiopeiae, plotted fromTESS data[ 15] The primary star in the YZ Cassiopeiae system is a whitesubgiant (main sequence ) star ofspectral type A1Vm and 2.31 solar masses[ 11] (M ☉ ) with a less massive main sequence dwarf star of type F2V[ 3] and 1.35M ☉ .[ 11]
In 1924, Joel Stebbins announced his discovery that the star, then known as 21 Cassiopeiae, is aneclipsing binary .[ 16] It was given itsvariable star designation , YZ Cassiopeiae, in 1925.[ 17] Theapparent magnitude of the eclipsing binary varies from 5.65 to 6.05[ 3] with a period of 4.4672 days.[ 11] Combined, they appear to have a spectral type of A2IV.[ 11]
The binary has a dimmer (magnitude 9.7 according to Norton,[ 18] or 10.5 by SIMBAD) companion of 0.8M ☉ [ 11] orbiting with a period of about 86 580 years.[ 11]
^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters .38 (5):331– 346.arXiv :1108.4971 .Bibcode :2012AstL...38..331A .doi :10.1134/S1063773712050015 .eISSN 1562-6873 .ISSN 1063-7737 .S2CID 119257644 . ^a b c d e van Leeuwen, F. (November 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 . ^a b c Jerzy M. Kreiner, Chun-Hwey Kim, Il-Seong Nha.YZ CAS: Atlas of O-C Diagrams of Eclipsing Binary Stars ^a b Hog, E.; Kuzmin, A.; Bastian, U.; Fabricius, C.; Kuimov, K.; Lindegren, L.; Makarov, V. V.; Roeser, S. (1998). "The TYCHO Reference Catalogue".Astronomy and Astrophysics .335 : L65.Bibcode :1998A&A...335L..65H . ^a b c d e Eggen, O. J. (1963). "Three-color photometry of the components in 228 wide double and multiple systems".Astronomical Journal .68 : 483.Bibcode :1963AJ.....68..483E .doi :10.1086/109000 . ^ Grenier, S.; Baylac, M.-O.; Rolland, L.; Burnage, R.; Arenou, F.; Briot, D.; Delmas, F.; Duflot, M.; Genty, V.; Gómez, A. E.; Halbwachs, J.-L.; Marouard, M.; Oblak, E.; Sellier, A. (1999)."Radial velocities. Measurements of 2800 B2-F5 stars for HIPPARCOS" (PDF) .Astronomy and Astrophysics Supplement .137 (3): 451.Bibcode :1999A&AS..137..451G .doi :10.1051/aas:1999489 . ^a b Bilir, S.; Ak, T.; Soydugan, E.; Soydugan, F.; Yaz, E.; Filiz Ak, N.; Eker, Z.; Demircan, O.; Helvaci, M. (2008). "New absolute magnitude calibrations for detached binaries".Astronomische Nachrichten .329 (8): 835.arXiv :0806.1290 .Bibcode :2008AN....329..835B .doi :10.1002/asna.200811002 .S2CID 6131326 . ^ 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 . ^a b c d e f g h Pavlovski, K.; Southworth, J.; Kolbas, V.; Smalley, B. (2014)."Absolute dimensions of detached eclipsing binaries - III. The metallic-lined system YZ Cassiopeiae" .Monthly Notices of the Royal Astronomical Society .438 (1):590– 603.arXiv :1311.3482 .Bibcode :2014MNRAS.438..590P .doi :10.1093/mnras/stt2229 .S2CID 56144135 . ^ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system".Astronomy Letters .32 (11):759– 771.arXiv :1606.08053 .Bibcode :2006AstL...32..759G .doi :10.1134/S1063773706110065 .S2CID 119231169 . ^a b c d e f g h Tokovinin 1997-1999.J/A+AS/124/75 . Multiple star catalogue (MSC) ^a b c d e f g Eker, Z.; Soydugan, F.; Soydugan, E.; Bilir, S.; Yaz Gökçe, E.; Steer, I.; Tüysüz, M.; Şenyüz, T.; Demircan, O. (2015). "Main-Sequence Effective Temperatures from a Revised Mass-Luminosity Relation Based on Accurate Properties".The Astronomical Journal .149 (4): 131.arXiv :1501.06585 .Bibcode :2015AJ....149..131E .doi :10.1088/0004-6256/149/4/131 .S2CID 118740259 . ^a b c Maxted, P. F. L.; Serenelli, A. M.; Southworth, J. (2015). "Bayesian mass and age estimates for transiting exoplanet host stars".Astronomy & Astrophysics .575 : A36.arXiv :1412.7891 .Bibcode :2015A&A...575A..36M .doi :10.1051/0004-6361/201425331 .S2CID 54857801 . ^ "V* YZ Cas" .SIMBAD .Centre de données astronomiques de Strasbourg . Retrieved26 January 2018 .^ "MAST: Barbara A. Mikulski Archive for Space Telescopes" . Space Telescope Science Institute. Retrieved8 December 2021 .^ Stebbins, Joel (1924)."Photo-electric photometry at the Washburn Observatory" .Popular Astronomy .32 :233– 234.Bibcode :1924PA.....32..233S . Retrieved14 January 2025 . ^ Guthnick, P.; Prager, R. (March 1925)."Benennung von neu entdeckten veränderlichen Sternen" .Astronomische Nachrichten .224 (8):129– 148.Bibcode :1925AN....224..129G .doi :10.1002/asna.19252240802 . Retrieved14 January 2025 . ^ Norton, Arthur P. (1973).Norton's Star Atlas . Gall & Inglis. p. 118 .ISBN 0-85248-900-5 .