Beta Centauri: Difference between revisions
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'''Beta Centauri''' (β Cen, β Centauri) is a [[star]] system in the southern [[constellation]] of [[Centaurus]]. With an [[apparent visual magnitude]] of 0.60, it is the second brightest star in the [[constellation]] [[Centaurus]] and the [[list of brightest stars|tenth brightest star]] in the night sky. It has the traditional names '''Hadar''' and '''Agena'''. The name ''Hadar'' comes from the [[Arabic language|Arabic]] word for " |
'''Beta Centauri''' (β Cen, β Centauri) is a [[star]] system in the southern [[constellation]] of [[Centaurus]]. With an [[apparent visual magnitude]] of 0.60, it is the second brightest star in the [[constellation]] [[Centaurus]] and the [[list of brightest stars|tenth brightest star]] in the night sky. It has the traditional names '''Hadar''' and '''Agena'''. The name ''Hadar'' comes from the [[Arabic language|Arabic]] word for "incline" ie swirling star ( حدر حيدر) , or "ground / soil / earth" (from '''أل أرض''' - ''al ardh'')<ref name=allen1963/> or "civilization" (from '''ألحضارة''' - ''al hidaara''), while the name ''Agena'' comes from [[Latin]] words for "the knee". The Chinese name for the star is 马腹一 ([[Standard Chinese|Mandarin]]: mǎ fù yī, ''the First Star of the Horse's Abdomen'').<ref>{{zh icon}} [http://aeea.nmns.edu.tw/2006/0607/ap060729.html AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 29 日]</ref> |
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==Properties== |
==Properties== |
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Revision as of 22:21, 6 December 2013
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| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Centaurus |
| Right ascension | 14h 03m 49.40535s[1] |
| Declination | –60° 22′ 22.9266″[1] |
| Apparent magnitude (V) | 0.60[2] |
| Astrometry | |
| Radial velocity (Rv) | +5.9[3] km/s |
| Proper motion (μ) | RA: –33.27[1] mas/yr Dec.: –23.16[1] mas/yr |
| Parallax (π) | 9.35 ± 0.50 mas[1] |
| Distance | 350 ± 20 ly (107 ± 6 pc) |
| Characteristics | |
| Spectral type | B1 III[4] |
| U−B color index | –0.98[2] |
| B−V color index | –0.22[2] |
| Variable type | β Cep |
| Details | |
| Mass | 10.7 ± 0.1[5] / 10.3 ± 0.1[5] M☉ |
| Luminosity | 41,700[4] L☉ |
| Surface gravity (log g) | 3.5 ± 0.4[5] cgs |
| Temperature | 25,000 ± 2,000[5] K |
| Age | (14.1 ± 0.6) × 106[5] years |
| Other designations | |
| Database references | |
| SIMBAD | data |
Beta Centauri (β Cen, β Centauri) is a star system in the southern constellation of Centaurus. With an apparent visual magnitude of 0.60, it is the second brightest star in the constellation Centaurus and the tenth brightest star in the night sky. It has the traditional names Hadar and Agena. The name Hadar comes from the Arabic word for "incline" ie swirling star ( حدر حيدر) , or "ground / soil / earth" (from أل أرض - al ardh)[6] or "civilization" (from ألحضارة - al hidaara), while the name Agena comes from Latin words for "the knee". The Chinese name for the star is 马腹一 (Mandarin: mǎ fù yī, the First Star of the Horse's Abdomen).[8]
Properties
Based upon parallax measurements from the astrometric Hipparcos satellite,[9][10] the distance to this system is about 350 light-years (110 parsecs).[1] The spectrum matches a star with a stellar classification of B1 III,[4] with the luminosity class of III indicating this is a giant star that has exhausted the hydrogen at its core and evolved away from the main sequence. It is a Beta Cephei variable star with a pulsation period of 0.157 days.[4]
In 1935, Joan Voûte identified Beta Centauri as a double star, giving it the identifier VOU 31. The companion is separated from the primary by 1.3 seconds of arc, and has remained so since the discovery, although the position angle has changed slightly. This would indicate that the orbital period is very long, if the pair are actually gravitationally associated.[citation needed]
Based on the variable radial velocity of this star, in 1967 it was suggested that the primary is a double-lined spectroscopic binary. This was confirmed in 1999. The primary consists of a pair of stars with nearly identical mass that orbit each other over a period of 357 days with a large eccentricity of about 0.81.[5][11] The pair are separated by a mean distance of roughly 4 astronomical units.[4]
Cultural significance
Beta Centauri is well known in the Southern Hemisphere as the inner of the two "Pointers" to the Southern Cross. A line made from the other pointer, Alpha Centauri, through Beta Centauri leads to within a few degrees of Gacrux, the star at the top of the cross. Using Gacrux, a navigator can draw a line with Acrux to effectively determine south.[12]
The indigenous Boorong people of northwestern Victoria named it as Bermbermgle (together with α Cen),[13] two brothers who were noted for their courage and destructiveness, and who spear and kill Tchingal, "The Emu" (Coalsack Nebula).[14] The two brothers in Wotjobaluk people is Bram-bram-bult.[13]
References
- ^ a b c d e f van 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
{{citation}}: Unknown parameter|month=ignored (help) - ^ a b c Hogg, A. R. (1958), "Photometric observations of 244 bright stars", Mount Stromlo Observatory Mimeogram, 2, Bibcode:1958MtSOM...2....1H
- ^ Evans, D. S. (June 20–24, 1966), The Revision of the General Catalogue of Radial Velocities, University of Toronto: International Astronomical Union, retrieved 2009-09-10
{{citation}}: Unknown parameter|booktitle=ignored (help); Unknown parameter|editors=ignored (|editor=suggested) (help) - ^ a b c d e Raassen, A. J. J.; et al. (2006), "XMM-Newton observations of β Centauri (B1 III): The temperature structure in the hot plasma and the photosphere-wind connection", Astronomy and Astrophysics, 437 (2): 599–609, Bibcode:2005A&A...437..599R, doi:10.1051/0004-6361:20052650
{{citation}}: Unknown parameter|month=ignored (help) - ^ a b c d e f Ausseloos, M.; et al. (2006), "High-precision elements of double-lined spectroscopic binaries from combined interferometry and spectroscopy. Application to the β Cephei star β Centauri", Astronomy and Astrophysics, 455 (1): 259–269, arXiv:astro-ph/0605220, Bibcode:2006A&A...455..259A, doi:10.1051/0004-6361:20064829
{{citation}}: Unknown parameter|month=ignored (help) - ^ a b Allen, R. H. (1963), Star Names: Their Lore and Meaning (Reprint ed.), New York: Dover Publications Inc, p. 154, ISBN 0-486-21079-0, retrieved 2010-12-12
- ^ "V* bet Cen -- Variable Star of beta Cep type", SIMBAD, Centre de Données astronomiques de Strasbourg, retrieved 2011-12-19
- ^ Template:Zh icon AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 29 日
- ^ Perryman, M. A. C.; Lindegren, L.; Kovalevsky, J.; et al. (1997), "The Hipparcos Catalogue", Astronomy and Astrophysics, 323: L49–L52, Bibcode:1997A&A...323L..49P
{{citation}}: Explicit use of et al. in:|last4=(help); Unknown parameter|month=ignored (help) - ^ Perryman, Michael (2010), The Making of History's Greatest Star Map, Heidelberg: Springer-Verlag, doi:10.1007/978-3-642-11602-5
- ^ Ausseloos, M.; Aerts, C.; Uytterhoeven, K. (2002), "A Study of the Orbital and Intrinsic Variability of the Double-Lined Spectroscopic Binary β Centauri", in Aerts, Conny; Bedding, Timothy R.; Christensen-Dalsgaard, Jørgen (eds.), Radial and Nonradial Pulsations as Probes of Stellar Physics, ASP Conference Proceedings, vol. 259, p. 86, Bibcode:2002ASPC..259...86A
- ^ Kyselka, Will; Lanterman, Ray E. (1976), North Star to Southern Cross, University of Hawaii Press, p. 59, ISBN 0-8248-0419-8
- ^ a b Hamacher, Duane W.; Frew, David J. (2010). "An Aboriginal Australian Record of the Great Eruption of Eta Carinae" (PDF). Journal of Astronomical History & Heritage. 13 (3): 220–34.
{{cite journal}}: CS1 maint: multiple names: authors list (link) - ^ Stanbridge, WM (1857). "On the Astronomy and Mythology of the Aboriginies of Victoria" (PDF). Transactions Philosophical Institiute Victoria. 2: 137–140.
External links
- Kaler, James B., "HADAR (Beta Centauri)", Stars, University of Illinois, retrieved 2011-12-19
