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Pi Arietis

From Wikipedia, the free encyclopedia
Multiple star system in the constellation Aries
π Arietis
Location of π Arietis (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAries
Right ascension02h 49m 17.55924s[1]
Declination+17° 27′ 51.5168″[1]
Apparent magnitude (V)5.21[2]
Characteristics
Spectral typeB6 V + A0 V + F8 V[3]
U−Bcolor index–0.47[2]
B−Vcolor index–0.06[2]
Astrometry
Radial velocity (Rv)+8.8[4] km/s
Proper motion (μ)RA: +2.60[1]mas/yr
Dec.: –14.10[1]mas/yr
Parallax (π)4.18±0.69 mas[1]
Distanceapprox. 800 ly
(approx. 240 pc)
Absolute magnitude (MV)−1.56[5]
Details
Luminosity538[5] L
Rotational velocity (v sin i)70[6] km/s
Other designations
π Ari, 42 Arietis,BD+16° 355,HD 17543,HIP 13165,HR 836,SAO 93127.[7]
Database references
SIMBADdata

Pi Arietis,Latinized from π Arietis, is theBayer designation for a multiplestar system in the northernconstellation ofAries. Based uponparallax measurements made during theHipparcos mission, this system is approximately 800light-years (250parsecs) distant fromEarth and has anapparent visual magnitude of 5.21. This is bright enough to be faintly seen with the naked eye.

The primary member of this system is a massive,B-type main sequence star with astellar classification of B6 V. It is a closespectroscopic binary with anorbital period of 3.854 days, aneccentricity of 0.04, and a combined visual magnitude of 5.30. At anangular separation of 3.28 arcseconds is a magnitude 8.46A-type main sequence star with a classification of A0 Vp. Finally, a fourth member of the system is a magnitude 11.0F-type main sequence star with a classification of F8V at an angular separation of 25.2 arcseconds from the primary.[3]

Name

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This star, along withδ Ari,ε Ari,ζ Ari, andρ3 Ari, were Al Bīrūnī'sAl Buṭain (ألبطين), the dual ofAl Baṭn, the Belly.[8] According to the catalogue of stars in theTechnical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars,Al Buṭain were the title for five stars :δ Ari asBotein, π Ari asAl Buṭain I,ρ3 Ari asAl Buṭain II,ε Ari asAl Buṭain III danζ Ari asAl Buṭain IV.[9]

InChinese,左更 (Zuǒ Gēng), meaningOfficial in Charge of the Forest, refers to an asterism consisting of π Arietis,ν Arietis,μ Arietis,ο Arietis andσ Arietis.[10] Consequently, theChinese name for π Arietis itself is左更五 (Zuǒ Gēng wu, English:the Fifth Star of Official in Charge of the Forest.)[11]

References

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  1. ^abcdevan 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.
  2. ^abcCrawford, D. L.; Barnes, J. V.; Golson, J. C. (1971), "Four-color, H-beta, and UBV photometry for bright B-type stars in the northern hemisphere",The Astronomical Journal,76: 1058,Bibcode:1971AJ.....76.1058C,doi:10.1086/111220.
  3. ^abEggleton, 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.
  4. ^Wilson, Ralph Elmer (1953), "General Catalogue of Stellar Radial Velocities",Carnegie Institute Washington D.C. Publication, Washington: Carnegie Institution of Washington,Bibcode:1953GCRV..C......0W.
  5. ^abAnderson, 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.
  6. ^Abt, Helmut A.; Levato, Hugo; Grosso, Monica (July 2002), "Rotational Velocities of B Stars",The Astrophysical Journal,573 (1):359–365,Bibcode:2002ApJ...573..359A,doi:10.1086/340590.
  7. ^"pi. Ari".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2012-08-07.
  8. ^Allen, R. H. (1963),Star Names: Their Lore and Meaning (Reprint ed.), New York, NY: Dover Publications Inc, p. 83,ISBN 0-486-21079-0, retrieved2010-12-12.
  9. ^Rhoads, Jack W. (November 15, 1971),"Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars"(PDF),Jet Propulsion Laboratory, California Institute of Technology.
  10. ^(in Chinese)中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005,ISBN 978-986-7332-25-7.
  11. ^(in Chinese)AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 21 日Archived 2011-05-22 at theWayback Machine

External links

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