Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

48 Cassiopeiae

From Wikipedia, the free encyclopedia
Triple star system in the constellation Cassiopeia
"A Cassiopeiae" redirects here. Not to be confused withα (alpha) Cassiopeiae.
48 Cassiopeiae
Observation data
Epoch J2000      Equinox J2000
ConstellationCassiopeia
Right ascension02h 01m 57.45035s[1]
Declination+70° 54′ 25.2902″[1]
Apparent magnitude (V)4.49[2]
Characteristics
Spectral typeA3 Va[3] (A2 V + F2 V)[4]
B−Vcolor index0.164±0.008[2]
Astrometry
Radial velocity (Rv)−12.4[5] km/s
Proper motion (μ)RA: −55.69[1]mas/yr
Dec.: −8.71[1]mas/yr
Parallax (π)28.36±0.44 mas[1]
Distance115 ± 2 ly
(35.3 ± 0.5 pc)
Absolute magnitude (MV)1.75[2]
Orbit[6]
Primary48 Cas A
Companion48 Cas B
Period (P)61.14±0.05yr
Semi-major axis (a)0.614±0.002
Eccentricity (e)0.355±0.001
Inclination (i)16.7±0.9°
Longitude of the node (Ω)48.2±3.2°
Periastronepoch (T)1964.35±0.09
Argument of periastron (ω)
(secondary)
19.5±3.6°
Details
48 Cas A
Mass1.93[7] M
Luminosity17.8+0.6
−1.2
[8] L
Surface gravity (log g)4.47[9] cgs
Temperature8,538±290[9] K
Metallicity [Fe/H]−0.4[5] dex
Rotational velocity (v sin i)61[8] km/s
Age376[9] Myr
48 Cas B
Mass1.17[7] M
Other designations
A Cassiopeiae,48 Cas,BD+70° 153,HD 12111,HIP 9480,HR 575,SAO 4554,ADS 1598,CCDM J02020+7054,WDS J02020+7054AB[10]
Database references
SIMBADdata

48 Cassiopeiae is atriple star[11][7] system in the northernconstellation ofCassiopeia. It is visible to the naked eye with a combinedapparent visual magnitude of 4.49.[2] With an annualparallax shift of28.36±0.44 mas as seen from Earth's orbit, it is located approximately 115light years away.[1] The system is moving closer with a heliocentricradial velocity of −12.4 km/s.[5]

The primary component, designated48 Cassiopeiae A, is a whiteA-type main-sequence star with astellar classification of A2 V[4] and anapparent magnitude of +4.65.[12] It has a companion, component B, which is anF-type main-sequence star of class F2 V[4] and an apparent magnitude of +6.74.[12] This pair orbit around their commoncentre of mass once every 61.1 years.[6] They have asemimajor axis of 0.614arcseconds and aneccentricity of 0.355.[6] A third companion, component C, is a magnitude 13.20[12] star located at anangular separation of 23.16 arcseconds as of 2014, or at least 816.5 AU away.[7]

48 Cassiopeiae also has theBayer designation A Cassiopeiae, the only star with a Latin letter designation in the constellation.[13]

References

[edit]
  1. ^abcdefvan 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. ^abcdAnderson, 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.
  3. ^Gray, R. O.; Garrison, R. F. (July 1989), "The Late A-Type Stars: Refined MK Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation",Astrophysical Journal Supplement,70: 623,Bibcode:1989ApJS...70..623G,doi:10.1086/191349.
  4. ^abcEdwards, T. W. (1976), "MK classification for visual binary components",The Astronomical Journal,81: 245,Bibcode:1976AJ.....81..245E,doi:10.1086/111879.
  5. ^abcGebran, M.; et al. (2016), "A new method for the inversion of atmospheric parameters of A/Am stars",Astronomy & Astrophysics,589: A83,arXiv:1603.01146,Bibcode:2016A&A...589A..83G,doi:10.1051/0004-6361/201528052,S2CID 118549566.
  6. ^abcHartkopf, W. I.; et al. (June 30, 2006),Sixth Catalog of Orbits of Visual Binary Stars, United States Naval Observatory, archived fromthe original on 2017-08-01, retrieved2018-06-25.
  7. ^abcdDe Rosa, R. J.; et al. (2014), "The VAST Survey - III. The multiplicity of A-type stars within 75 pc",Monthly Notices of the Royal Astronomical Society,437 (2): 1216,arXiv:1311.7141,Bibcode:2014MNRAS.437.1216D,doi:10.1093/mnras/stt1932.
  8. ^abZorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy & Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789.
  9. ^abcDavid, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets",The Astrophysical Journal,804 (2): 146,arXiv:1501.03154,Bibcode:2015ApJ...804..146D,doi:10.1088/0004-637X/804/2/146,S2CID 33401607.
  10. ^"48 Cas".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2018-06-19.
  11. ^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.
  12. ^abcMason, B. D.; et al. (2014),"The Washington Visual Double Star Catalog",The Astronomical Journal,122 (6): 3466,Bibcode:2001AJ....122.3466M,doi:10.1086/323920, retrieved2015-07-22.
  13. ^Kostjuk, N. D. (2004), "VizieR Online Data Catalog: HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index (Kostjuk, 2002)",VizieR On-line Data Catalog: IV/27A. Originally Published in: Institute of Astronomy of Russian Academy of Sciences (2002),4027,Bibcode:2004yCat.4027....0K.
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
NGC
Other
Galaxies
NGC
Other
Astronomical events
Retrieved from "https://en.wikipedia.org/w/index.php?title=48_Cassiopeiae&oldid=1241655358"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp