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词条 Zeta Centauri
释义

  1. References

{{Starbox begin
| name=Zeta Centauri
}}{{Starbox image
| image =

| caption=Location of ζ Centauri (circled)
}}{{Starbox observe
| epoch = J2000.0
| ra = {{RA|13|55|32.38565}}
| dec = {{DEC|−47|17|18.1482}}
| appmag_v = +2.55[3]
| constell = Centaurus
}}{{Starbox character
| class = B2.5 IV[4]
| b-v = −0.22[3]
| u-b = −0.91[3]
| variable =
}}{{Starbox astrometry
| radial_v = +6.5[7]
| prop_mo_ra = −57.37
| prop_mo_dec = −44.55
| parallax = 8.54
| p_error = 0.13
| parallax_footnote =
| absmag_v = −2.79[11]
}}{{Starbox orbit
| reference = [12]
| period_unitless = 8.024 days
| axis_unitless = 0.0014"[13]
| eccentricity = 0.5
| periastron = 2413719.321 JD
| periarg = 290
}}{{Starbox detail
| mass = {{nowrap|7.8 ± 0.1}}[4]
| radius = {{nowrap|5.80 ± 0.53}}[15]
| gravity = {{nowrap|3.84 ± 0.08}}[15]
| metal_fe =
| age_myr = {{nowrap|39.8 ± 5.7}}[4]
| luminosity =
| temperature = {{nowrap|23,561 ± 283}}[15]
| rotational_velocity = 235[19]
}}{{Starbox catalog
| names=Alnair, ζ Cen, CD−46 8949, CP−46 6560, HD 121263, HIP 68002, HR 5231, SAO 224538.[20]
}}{{Starbox reference
| Simbad=HD+121263
}}{{Starbox end}}Zeta Centauri, Latinized from ζ Centauri, is a binary star system in the southern constellation of Centaurus. It has the proper name Alnair, from the scientific-Arabic[21] Nayyir Badan Qanṭūris (نير بطن قنطورس), meaning "The Bright (Star) of the Body of the Centaur".[1] With a combined apparent visual magnitude of +2.55,[3] it is one of the brighter members of the constellation. This system is close enough to the Earth that its distance can be measured directly using the parallax technique. This yields a value of roughly {{Convert|382|ly|pc|abbr=off|lk=on}}, with a 1.6% margin of error.

In Chinese, {{lang|zh|庫樓}} ({{lang|zh-Latn|Kù Lóu}}), meaning Arsenal, refers to an asterism consisting of ζ Centauri, η Centauri, θ Centauri, 2 Centauri, HD 117440, ξ1 Centauri, γ Centauri, τ Centauri, D Centauri and σ Centauri.[2] Consequently, ζ Centauri itself is known as {{lang|zh|庫樓一}} ({{lang|zh-Latn|Kù Lóu yī}}, {{lang-en|the First Star of Arsenal}}.)[3]

ζ Cen is a double-lined spectroscopic binary system,[27] which indicates that the orbital motion was detected by shifts in the absorption lines of their combined spectra caused by the Doppler effect. The two stars orbit each other over a period of slightly more than eight days with an orbital eccentricity of about 0.5.[12] The estimated angular separation of the pair is 1.4 mas.[13]

At an estimated age of 40 million years,[4] the primary component of this system appears to be in the subgiant stage of its evolution with a stellar classification of B2.5 IV.[4] It is a large star with nearly 8[4] times the mass of the Sun and close to 6[15] times the Sun's radius. This star is rotating rapidly with a projected rotational velocity of {{nowrap|235 km s−1}}.[19]

References

1. ^ibid., p.28.
2. ^{{zh icon}} 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}}.
3. ^{{zh icon}} AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 25 日
4. ^{{citation | title=XHIP: An extended hipparcos compilation | last1=Anderson | first1=E. | last2=Francis | first2=Ch. | journal=Astronomy Letters | volume=38 | issue=5 | pages=331 | year=2012 | bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015 | arxiv=1108.4971 | postscript=. }}
5. ^{{citation | last1=Fitzpatrick | first1=E. L. | last2=Massa | first2=D. | title=Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry | journal=The Astronomical Journal | volume=129 | issue=3 | pages=1642–1662 |date=March 2005 | doi=10.1086/427855 | bibcode=2005AJ....129.1642F |arxiv = astro-ph/0412542 }}
6. ^{{citation | last1=Tetzlaff | first1=N. | last2=Neuhäuser | first2=R. | last3=Hohle | first3=M. M. | title=A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun | journal=Monthly Notices of the Royal Astronomical Society | volume=410 | issue=1 | pages=190–200 |date=January 2011 | doi=10.1111/j.1365-2966.2010.17434.x | bibcode=2011MNRAS.410..190T |arxiv = 1007.4883 }}
7. ^{{citation | last=Wilson | first=R. E. | date=1953 | title=General Catalogue of Stellar Radial Velocities | publisher=Carnegie Institute of Washington D.C. | bibcode=1953GCRV..C......0W }}
8. ^{{citation | last1=Bernacca | first1=P. L. | last2=Perinotto | first2=M. | title=A catalogue of stellar rotational velocities | journal=Contributi Osservatorio Astronomico di Padova in Asiago | volume=239 | issue=1 | date=1970 | bibcode=1970CoAsi.239....1B }}
9. ^{{citation | display-authors=1 | last1=Johnson | first1=H. L. | last2=Iriarte | first2=B. | last3=Mitchell | first3=R. I. | last4=Wisniewskj | first4=W. Z. | title=UBVRIJKL photometry of the bright stars | journal=Communications of the Lunar and Planetary Laboratory | volume=4 | issue=99 | date=1966 | bibcode=1966CoLPL...4...99J }}
10. ^{{cite simbad | title=* zet Cen | accessdate=2012-03-01 }}
11. ^{{citation | last1=Kunitzsch | first1=P. | last2=Smart | first2=T. | date = 2006 | title = A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations | edition = 2nd revised | publisher = Sky Pub | location = Cambridge, MA | isbn=978-1-931559-44-7 | page=4 }}
12. ^{{citation | last1=van Rensbergen | first1=W. | last2=De Loore | first2=C. | last3=Jansen | first3=K. | title=Evolution of interacting binaries with a B type primary at birth | journal=Astronomy and Astrophysics | volume=446 | issue=3 | pages=1071–1079 |date=February 2006 | doi=10.1051/0004-6361:20053543 | bibcode=2006A&A...446.1071V }}
13. ^{{citation | first1=A. C. | last1=Maury | date=1922 | title=The Orbit of the Spectroscopic Binary ζ Centauri | journal=Harvard College Observatory Circular | volume=233 | pages=1–4 | bibcode=1922HarCi.233....1M }}
14. ^{{citation | last1=Halbwachs | first1=J. L. | title=List of Estimated Angular Separations of Spectroscopic Binaries | journal=Astronomy and Astrophysics Supplement | volume=44 | page=47 |date=April 1981 | bibcode=1981A&AS...44...47H }}
[4][5][6][7][8][9][10][11][12][13][14]
}}{{Stars of Centaurus}}

8 : Centaurus (constellation)|Bayer objects|Spectroscopic binaries|B-type subgiants|Hipparcos objects|Durchmusterung objects|HR objects|Henry Draper Catalogue objects

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