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1 References  














VZ Arietis






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VZ Arietis
Observation data
Epoch J2000      Equinox J2000
Constellation Aries
Right ascension 02h48m 45.90719s[1]
Declination +25° 11′ 16.95410″[1]
Apparent magnitude (V) 5.89[2] (5.82 - 5.89)[3]
Characteristics
Spectral type A0 V[4]
B−V color index −0.033±0.005[2]
Variable type α2 CVn[3]
Astrometry
Radial velocity (Rv)+13.8±2.9[5] km/s
Proper motion (μ) RA: +56.600[1] mas/yr
Dec.: −0.264[1] mas/yr
Parallax (π)5.7743 ± 0.1298 mas[1]
Distance560 ± 10 ly
(173 ± 4 pc)
Absolute magnitude (MV)0.48[2]
Details[6]
Mass2.74±0.09 M
Radius3.1[7] R
Luminosity78.7+15.1
−12.7
 L
Surface gravity (log g)4.10[8] cgs
Temperature10,304+72
−71
 K
Metallicity [Fe/H]+0.1[8] dex
Rotational velocity (v sin i)54 km/s
Other designations

16 Trianguli, VZ Arietis, BD+24°396, FK5 5868, HD 17471, HIP 13121, HR 830, SAO 75588[9]

Database references
SIMBADdata

VZ Arietis is single,[10] white-hued star in the northern zodiac constellationofAries. Varying between magnitudes 5.82 and 5.89,[3] the star can be seen with the naked eye in dark, unpolluted areas. Based upon an annual parallax shiftof5.8 mas,[1] it is located 560 light years from the Sun. It is moving further away with a heliocentric radial velocity of +14 km/s.[5] The star was formerly known as 16 Trianguli, but as the star is no longer in the constellation Triangulum, this designation has fallen out of use.[11]

This is a chemically peculiar star[6] of type CP2 (Ap star),[12] showing an anomalous abundance of silicon in its spectrum.[13] It has a stellar classification of A0 V,[4] which indicates this is an A-type main-sequence star that currently fusing hydrogen into helium in its core. This is an Alpha2 Canum Venaticorum variable[12] with 2.7[6] times the mass of the Sun and about 3.1[7] times the Sun's radius. It is radiating 79 times the Sun's luminosity from its photosphere at an effective temperature of 10,304 K.[6]

References

[edit]
  1. ^ a b c d e f 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.
  • ^ a b c 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.
  • ^ a b c VSX (4 January 2010). "VZ Arietis". AAVSO Website. American Association of Variable Star Observers. Retrieved 15 June 2014.
  • ^ a b Cowley, A.; et al. (April 1969). "A study of the bright A stars. I. A catalogue of spectral classifications". Astronomical Journal. 74: 375–406. Bibcode:1969AJ.....74..375C. doi:10.1086/110819.
  • ^ a b de Bruijne, J. H. J.; Eilers, A.-C. (October 2012). "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project". Astronomy & Astrophysics. 546: 14. arXiv:1208.3048. Bibcode:2012A&A...546A..61D. doi:10.1051/0004-6361/201219219. S2CID 59451347. A61.
  • ^ a b c d Zorec, 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.
  • ^ a b Pasinetti Fracassini, L. E.; et al. (2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)". Astronomy & Astrophysics. 367 (2) (Third ed.): 521–24. arXiv:astro-ph/0012289. Bibcode:2001A&A...367..521P. doi:10.1051/0004-6361:20000451. S2CID 425754.
  • ^ a b Gebran, 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.
  • ^ "HD 17471". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 22 August 2018.
  • ^ 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.
  • ^ Wagman, M. (August 1987). "Flamsteed's Missing Stars". Journal for the History of Astronomy. 18 (3): 222. Bibcode:1987JHA....18..209W. doi:10.1177/002182868701800305. S2CID 118445625.
  • ^ a b Wraight, K. T.; et al. (February 2012). "A photometric study of chemically peculiar stars with the STEREO satellites - I. Magnetic chemically peculiar stars". Monthly Notices of the Royal Astronomical Society. 420 (1): 757–772. arXiv:1110.6283. Bibcode:2012MNRAS.420..757W. doi:10.1111/j.1365-2966.2011.20090.x. S2CID 14811051.
  • ^ Zverko, J. (September 1984), "Classification of Ap-Stars HR 830 and 21 CVn", Bulletin of the Astronomical Institute of Czechoslovakia, 35: 294, Bibcode:1984BAICz..35..294Z

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=VZ_Arietis&oldid=1182272802"

    Categories: 
    A-type main-sequence stars
    Alpha2 Canum Venaticorum variables
    Ap stars
    Aries (constellation)
    Durchmusterung objects
    Flamsteed objects
    Henry Draper Catalogue objects
    Hipparcos objects
    Bright Star Catalogue objects
    Objects with variable star designations
    Hidden categories: 
    Articles with short description
    Short description is different from Wikidata
     



    This page was last edited on 28 October 2023, at 07:26 (UTC).

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