@prefix dbpprop: .
@prefix dbpedia: .
dbpedia:Omega_Men dbpprop:base dbpedia:Vega .
dbpedia:Gliese_721 dbpprop:redirect dbpedia:Vega .
@prefix rdf: .
@prefix ns3: .
dbpedia:Vega rdf:type ns3:WhiteMainSequenceStars ,
ns3:NorthernPoleStars ,
ns3:StarsWithProperNames ,
ns3:BayerObjects ,
ns3:FlamsteedObjects .
@prefix opencyc: .
dbpedia:Vega rdf:type opencyc:Mx4rvVi80ZwpEbGdrcN5Y29ycA ,
ns3:DeltaScutiVariables .
@prefix owl: .
dbpedia:Vega owl:sameAs opencyc:Mx4rwJAH-pwpEbGdrcN5Y29ycA ,
.
@prefix foaf: .
@prefix ns7: .
dbpedia:Vega foaf:page ns7:Vega ;
dbpprop:reference .
@prefix rdfs: .
dbpedia:Vega rdfs:label "Vega"@fi ,
"Wega"@pl ,
"Vega"@cs ,
"Alpha Lyrae"@fr ,
"\u0412\u0435\u0433\u0430"@ru ,
"Vega (stj\u00E4rna)"@sv ,
"Vega (stjerne)"@no ,
"Vega (y\u0131ld\u0131z)"@tr ,
"Vega (estrela)"@pt ,
"Vega"@ca ,
"\u7E54\u5973\u4E00"@zh ,
"Vega"@en ,
"Wega"@nl ,
"Wega"@de ,
"Vega (estrella)"@es ,
"Vega"@it ,
"\u0412\u0435\u0433\u0430"@uk ,
"\u30D9\u30AC"@ja ,
"Vega"@hu ,
"Vega"@ro .
@prefix dbpedia-owl: .
dbpedia:Vega dbpedia-owl:thumbnail ;
dbpprop:abstract "Vega (\u03B1 Lyr / \u03B1 Lyrae / Alpha Lyrae) is the brightest star in the constellation Lyra, the fifth brightest star in the night sky and the second brightest star in the northern celestial hemisphere, after Arcturus. It is a relatively nearby star at only 25 light-years from Earth, and, together with Arcturus and Sirius, one of the most luminous stars in the Sun's neighborhood. Vega has been extensively studied by astronomers, leading it to be termed, \"arguably the next most important star in the sky after the Sun. \" Historically, Vega served as the northern pole star around 12,000 BC and will do so again at 13,727 AD when the declination will be +86°14'. Vega was the first star, other than the Sun, to have its photograph taken and the first to have its spectrum photographed. It was also one of the first stars to have its distance estimated through parallax measurements. Vega has served as the baseline for calibrating the photometric brightness scale, and was one of the stars used to define the mean values for the UBV photometric system. In terms of years, Vega is only about a tenth the age of the Sun, but it is evolving so quickly that it has already approached the midpoint of its life expectancy, as has the Sun. It has an unusually low abundance of the elements with a higher atomic number than that of helium. Vega is also a suspected variable star that may vary slightly in magnitude in a periodic manner. It is rotating rapidly with a velocity of 274 km/s at the equator. This is causing the equator to bulge outward because of centrifugal effects, and, as a result, there is a variation of temperature across the star's photosphere that reaches a maximum at the poles. From the Earth, Vega is being observed from the direction of one of these poles. Based upon an excess emission of infrared radiation, Vega has a circumstellar disk of dust. This dust is likely the result of collisions between objects in an orbiting debris disk, which is analogous to the Kuiper belt in the Solar System. Stars that display an infrared excess because of dust emission are termed Vega-like stars. Irregularities in Vega's disk also suggest the presence of at least one planet, likely to be about the size of Jupiter, in orbit around Vega."@en ,
"Alpha Lyrae (\u03B1 Lyrae / \u03B1 Lyr), plus connue sous son nom traditionnel de V\u00E9ga, est l'\u00E9toile la plus brillante de la constellation de la Lyre. Vue depuis la Terre, il s'agit de la cinqui\u00E8me \u00E9toile la plus brillante du ciel, la deuxi\u00E8me de l'h\u00E9misph\u00E8re nord juste apr\u00E8s Arcturus. C'est une \u00E9toile relativement proche du Soleil, \u00E0 25,3 ann\u00E9es-lumi\u00E8re de celui-ci. C'est aussi, en termes de luminosit\u00E9 intrins\u00E8que l'une des \u00E9toiles les plus brillantes du voisinage solaire avec \u03B1 Bootis (Arcturus) et \u03B1 Canis Majoris (Sirius). Du fait de ses propri\u00E9t\u00E9s, V\u00E9ga fut l'objet de nombreuses \u00E9tudes de la part des astronomes et a ainsi plusieurs fois jou\u00E9 un r\u00F4le important dans l'histoire de l'astronomie. Elle fut par exemple la premi\u00E8re \u00E9toile autre que le Soleil \u00E0 avoir \u00E9t\u00E9 photographi\u00E9e et dont le spectre ait \u00E9t\u00E9 mesur\u00E9. Ce fut aussi une des premi\u00E8res \u00E9toiles dont la distance fut estim\u00E9e par parallaxe. Elle fut par ailleurs utilis\u00E9e pour la calibration des \u00E9chelles de luminosit\u00E9 photom\u00E9triques et fut une des \u00E9toiles qui servirent de r\u00E9f\u00E9rence pour la d\u00E9finition des valeurs moyennes du syst\u00E8me UBV. Incidemment, V\u00E9ga fut l'\u00E9toile polaire autour de 12\u00A0000 av. J. -C. (et le sera de nouveau dans 12\u00A0000 ans), m\u00EAme s'il n'existe aucun document de l'\u00E8re pr\u00E9historique attestant qu'elle ait \u00E9t\u00E9 utilis\u00E9e pour le rep\u00E9rage ou l'orientation. V\u00E9ga est relativement jeune compar\u00E9e au Soleil. Sa m\u00E9tallicit\u00E9 est inhabituellement faible. V\u00E9ga serait une \u00E9toile variable (c'est-\u00E0-dire que son \u00E9clat varierait p\u00E9riodiquement). Elle est en rotation rapide \u00E0 une vitesse de 274 km\u22C5s \u00E0 l'\u00E9quateur. Elle pr\u00E9sente ainsi un renflement \u00E0 l'\u00E9quateur en raison de la force centrifuge et, en cons\u00E9quence, sa temp\u00E9rature varie au sein de sa photosph\u00E8re pour \u00EAtre maximale aux p\u00F4les. Depuis la Terre, elle est observ\u00E9e dans une direction proche de l'axe de ses p\u00F4les. La mesure des radiations infrarouges de V\u00E9ga a permis de d\u00E9terminer que l'\u00E9toile poss\u00E8de un disque de poussi\u00E8res centr\u00E9 sur l'\u00E9toile. Ces poussi\u00E8res sont probablement le r\u00E9sultat de collisions entre objets d'un disque de d\u00E9bris, similaire \u00E0 la ceinture de Kuiper du Syst\u00E8me solaire. Les \u00E9toiles qui pr\u00E9sentent un exc\u00E8s de rayonnement infrarouge en raison des \u00E9missions de poussi\u00E8re sont appel\u00E9es \u00AB \u00E9toiles similaires \u00E0 V\u00E9ga \u00BB (Vega-like stars). Les irr\u00E9gularit\u00E9s du disque de V\u00E9ga sugg\u00E8rent la pr\u00E9sence d'au moins une exoplan\u00E8te, probablement de la taille de Jupiter en orbite autour de l'\u00E9toile."@fr ,
"\u0412\u0435\u0301\u0491\u0430 (\u0430\u0440\u0430\u0431. \u0432\u0430\u043A\u0456 \u00AB\u043F\u0430\u0434\u0430\u044E\u0447\u0430\u00BB) (\u03B1 \u041B\u0456\u0440\u0438) \u2014 \u043D\u0430\u0439\u044F\u0441\u043A\u0440\u0430\u0432\u0456\u0448\u0430 \u0417\u0456\u0440\u043A\u0430 \u0443 \u0441\u0443\u0437\u0456\u0440'\u0457 \u041B\u0456\u0440\u0438, \u043F'\u044F\u0442\u0430 \u0437\u0430 \u044F\u0441\u043A\u0440\u0430\u0432\u0456\u0441\u0442\u044E \u0417\u0456\u0440\u043A\u0430 \u043D\u0456\u0447\u043D\u043E\u0433\u043E \u043D\u0435\u0431\u0430, \u0434\u0440\u0443\u0433\u0430 \u043F\u0456\u0441\u043B\u044F \u0410\u0440\u043A\u0442\u0443\u0440\u0430 \u0432 \u043F\u0456\u0432\u043D\u0456\u0447\u043D\u0456\u0439 \u043F\u0456\u0432\u043A\u0443\u043B\u0456. \u0426\u0435 \u2014 \u0432\u0456\u0434\u043D\u043E\u0441\u043D\u043E \u0431\u043B\u0438\u0437\u044C\u043A\u0430 \u0437\u0456\u0440\u043A\u0430 (25 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432 \u0432\u0456\u0434 \u0417\u0435\u043C\u043B\u0456), \u0456, \u0440\u0430\u0437\u043E\u043C \u0437 \u0410\u0440\u043A\u0442\u0443\u0440\u043E\u043C \u0456 \u0421\u0456\u0440\u0456\u0443\u0441\u043E\u043C, \u043E\u0434\u043D\u0430 \u0437 \u043D\u0430\u0439\u044F\u0441\u043A\u0440\u0430\u0432\u0456\u0448\u0438\u0445 \u0437\u0456\u0440\u043E\u043A. \u0412\u0435\u0433\u0430 \u0431\u0443\u043B\u0430 \u043F\u043E\u043B\u044F\u0440\u043D\u043E\u044E \u0437\u0456\u0440\u043A\u043E\u044E \u0431\u043B\u0438\u0437\u044C\u043A\u043E 12,000 \u0434\u043E \u043D. \u0435. \u0456 \u0441\u0442\u0430\u043D\u0435 \u043F\u043E\u043B\u044F\u0440\u043D\u043E\u044E \u0437\u043D\u043E\u0432\u0443 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u043D\u043E \u0447\u0435\u0440\u0435\u0437 12000 \u0440\u043E\u043A\u0456\u0432 \u0443 \u0440\u0435\u0437\u0443\u043B\u044C\u0442\u0430\u0442\u0456 \u043F\u0440\u0435\u0446\u0435\u0441\u0456\u0457. \u0412\u0435\u0433\u0430 \u0431\u0443\u043B\u0430 \u043F\u0435\u0440\u0448\u043E\u044E \u0437\u0456\u0440\u043A\u043E\u044E \u043F\u0456\u0441\u043B\u044F \u0421\u043E\u043D\u0446\u044F, \u0432 \u044F\u043A\u043E\u044E \u0444\u043E\u0442\u043E\u0433\u0440\u0430\u0444\u0443\u0432\u0430\u043B\u0438 \u0441\u043F\u0435\u043A\u0442\u0440. \u0414\u043E \u0442\u043E\u0433\u043E \u0436, \u0412\u0435\u0433\u0430 \u0431\u0443\u043B\u0430 \u043E\u0434\u043D\u0456\u0454\u044E \u0437 \u043F\u0435\u0440\u0448\u0438\u0445 \u0437\u0456\u0440\u043E\u043A, \u0432\u0456\u0434\u0441\u0442\u0430\u043D\u044C \u044F\u043A\u043E\u0457 \u0432\u0438\u0437\u043D\u0430\u0447\u0438\u043B\u0438 \u0447\u0435\u0440\u0435\u0437 \u043F\u0430\u0440\u0430\u043B\u0430\u043A\u0441 \u0432\u0438\u043C\u0456\u0440\u044E\u0432\u0430\u043D\u043D\u044F. \u0412\u0435\u0433\u0430 \u0441\u043B\u0443\u0436\u0438\u043B\u0430 \u0434\u043B\u044F \u043A\u0430\u043B\u0456\u0431\u0440\u0443\u0432\u0430\u043D\u043D\u044F \u0444\u043E\u0442\u043E\u043C\u0435\u0442\u0440\u0438\u0447\u043D\u043E\u0433\u043E \u043C\u0430\u0441\u0448\u0442\u0430\u0431\u0443 \u044F\u0441\u043A\u0440\u0430\u0432\u043E\u0441\u0442\u0456. \u0423\u043A\u0440\u0430\u0457\u043D\u0441\u044C\u043A\u0430 \u043D\u0430\u0440\u043E\u0434\u043D\u0430 \u043D\u0430\u0437\u0432\u0430 \u0412\u0435\u0433\u0438 \u2014 \u0422\u043A\u0430\u043B\u044F. \u0412 \u043D\u0456\u0447 \u043D\u0430 \u0406\u0432\u0430\u043D\u0430 \u041A\u0443\u043F\u0430\u043B\u0430, \u0432\u043E\u043D\u0430 \u0437\u0443\u0441\u0442\u0440\u0456\u0447\u0430\u0454\u0442\u044C\u0441\u044F \u0437 \u0410\u043B\u044C\u0442\u0430\u0457\u0440\u043E\u043C \u2014 \u041F\u0430\u0441\u0442\u0443\u0445\u043E\u043C."@uk ,
"\u30D9\u30AC\uFF08\u30F4\u30A7\u30AC\u3001Vega\uFF09\u306F\u3053\u3068\u5EA7\u306Eα\u661F\u3067\u3001\u3053\u3068\u5EA7\u3067\u6700\u3082\u660E\u308B\u3044\u3002\u5168\u5929\u3067\u306F5\u756A\u76EE\u306B\u660E\u308B\u3044\u3002\u4E03\u5915\u306E\u304A\u308A\u3072\u3081\u661F\uFF08\u7E54\u5973\u661F\uFF09\u3068\u3057\u3066\u3088\u304F\u77E5\u3089\u308C\u3066\u3044\u308B\u3002\u308F\u3057\u5EA7\u306E\u30A2\u30EB\u30BF\u30A4\u30EB\u3001\u306F\u304F\u3061\u3087\u3046\u5EA7\u306E\u30C7\u30CD\u30D6\u3068\u3068\u3082\u306B\u3001\u590F\u306E\u5927\u4E09\u89D2\u3092\u5F62\u4F5C\u3063\u3066\u3044\u308B\u3002 \u7D14\u767D\u306EA\u578B\u4E3B\u7CFB\u5217\u661F\u3067\u3042\u308A\u3001\u300C\u7D14\u767D\u300D\u3068\u8A00\u3046\u8A00\u8449\u306E\u5B9A\u7FA9\u3068\u3055\u308C\u3066\u3044\u308B\u3002\u6A19\u6E96\u7684\u306A0\u7B49\u661F\u3060\u304C\u30010.19\u65E5\u306E\u5468\u671F\u3067\u50C5\u304B\u306B\u5909\u5149\u3059\u308B\u305F\u3066\u5EA7δ\u578B\u5909\u5149\u661F\u3067\u3042\u308B\u3002\u5909\u5149\u7BC4\u56F2\u304C0.01\u7B49\uFF5E0.04\u7B49\u3068\u5C0F\u3055\u3044\u305F\u3081\u3001\u773C\u8996\u89B3\u6E2C\u3067\u306F\u5909\u5149\u306F\u308F\u304B\u3089\u306A\u3044\u3002\u592A\u967D\u304B\u3089\u306E\u8DDD\u96E2\u306F25.3\u5149\u5E74\u3067\u3001\u6BCE\u79D213.5\u30AD\u30ED\u30E1\u30FC\u30C8\u30EB\u3067\u63A5\u8FD1\u3057\u3066\u3044\u308B\u3002 2003\u5E74\u306B\u306F\u3001\u60D1\u661F\u7CFB\u304C\u5F62\u6210\u3055\u308C\u3064\u3064\u3042\u308B\u3053\u3068\u304C\u5206\u304B\u3063\u305F\u3002\u5F53\u6642\u7D04100\u500B\u307B\u3069\u767A\u898B\u3055\u308C\u3066\u3044\u305F\u60D1\u661F\u7CFB\u306E\u307B\u3068\u3093\u3069\u304C\u3001\u4E3B\u661F\u306E\u8FD1\u304F\u3092\u6728\u661F\u578B\u60D1\u661F\u304C\u9AD8\u901F\u3067\u516C\u8EE2\u3057\u3066\u3044\u308B\u3082\u306E\uFF08\u30DB\u30C3\u30C8\u30FB\u30B8\u30E5\u30D4\u30BF\u30FC\u3068\u547C\u3070\u308C\u308B\uFF09\u3060\u304C\u3001\u3053\u306E\u60D1\u661F\u7CFB\u306F\u592A\u967D\u7CFB\u306B\u8FD1\u4F3C\u306E\u3082\u306E\u3067\u3042\u308B\u53EF\u80FD\u6027\u304C\u3042\u308B\u3002 2006\u5E74\u306B\u306F\u3001\u81EA\u8EE2\u5468\u671F\u304C12.5\u6642\u9593\u3068\u3044\u3046\u9AD8\u901F\u3067\u81EA\u8EE2\u3057\u3066\u304A\u308A\u3001\u305D\u306E\u901F\u3055\u306F\u9060\u5FC3\u529B\u3067\u30D9\u30AC\u304C\u81EA\u58CA\u3059\u308B\u901F\u5EA6\u306E94%\u306B\u9054\u3057\u3066\u3044\u308B\u3053\u3068\u304C\u5224\u660E\u3057\u305F\u3002\u3053\u306E\u305F\u3081\u3001\u6975\u4ED8\u8FD1\u3068\u8D64\u9053\u4ED8\u8FD1\u3067\u306F\u5927\u304D\u306A\u6E29\u5EA6\u5DEE\u304C\u751F\u3058\u3066\u3044\u308B\u3002 \u5730\u7403\u306E\u6B73\u5DEE\u904B\u52D5\u306B\u3088\u308A\u3001\u304A\u3088\u305D12000\u5E74\u5F8C\u306B\u306F\u5317\u6975\u661F\u306B\u306A\u308B\u3002\u305D\u306E\u9803\u306B\u306F\u30D9\u30AC\u307E\u3067\u306E\u8DDD\u96E2\u304C24.7\u5149\u5E74\u306B\u306A\u308B\u3068\u63A8\u7B97\u3055\u308C\u3066\u3044\u308B\u3002"@ja ,
"Wega (Alpha Lyrae, \u03B1 Lyr) - najja\u015Bniejsza gwiazda w gwiazdozbiorze Lutni, pi\u0105ta co do jasno\u015Bci gwiazda nieba, a trzecia na niebie p\u00F3\u0142nocnym. Odleg\u0142a od S\u0142o\u0144ca o 25,3 lat \u015Bwietlnych. Wraz z Deneb i Altair tworzy tzw. tr\u00F3jk\u0105t letni."@pl ,
"\u7E54\u5973\u4E00\uFF0C\u5373\u8457\u540D\u7684\u7E54\u5973\u661F\uFF0C\u56E0\u5728\u4E2D\u570B\u53E4\u4EE3\u300C\u725B\u90CE\u7E54\u5973\u300D\u795E\u8A71\u4E2D\uFF0C\u7E54\u5973\u70BA\u5929\u5E1D\u5B6B\u5973\uFF0C\u6545\u4EA6\u7A31\u5929\u5B6B\u3002 \u7E54\u5973\u661F\u662F\u5929\u7434\u5EA7\u6700\u4EAE\u7684\u6046\u661F\uFF08\u5929\u7434\u5EA7\u03B1\u661F\uFF09\uFF0C\u4E5F\u662F\u5168\u5929\u7B2C\u4E94\u4EAE\u661F\uFF0C\u5728\u5927\u89D2\u661F\u4E4B\u5F8C\u3002\u5728\u5317\u534A\u7403\u7684\u590F\u5929\uFF0C\u7E54\u5973\u661F\u591A\u53EF\u5728\u5929\u9802\u9644\u8FD1\u7684\u4F4D\u7F6E\u898B\u5230\uFF0C\u8DDD\u5730\u740325.3\u5149\u5E74\u3002\u7531\u65BC\u7E54\u5973\u661F\u7684\u8996\u661F\u7B49\u63A5\u8FD1\u96F6\uFF0C\u56E0\u6B64\u4E0D\u5C11\u5C08\u696D\u5929\u6587\u5B78\u5BB6\u6703\u4EE5\u7E54\u5973\u661F\u4F86\u4F5C\u5149\u5EA6\u6E2C\u5B9A\u7684\u6A19\u6E96\u3002 \u7E54\u5973\u661F\u8207\u4F4D\u65BC\u5929\u9DF9\u5EA7\u7684\u6CB3\u9F13\u4E8C\uFF08\u725B\u90CE\u661F\uFF09\uFF0C\u53CA\u5929\u9D5D\u5EA7\u7684\u5929\u6D25\u56DB\uFF0C\u7D44\u6210\u8457\u540D\u7684\u300C\u590F\u5B63\u5927\u4E09\u89D2\u300D\u3002\u5982\u679C\u628A\u5B83\u770B\u4F5C\u662F\u4E00\u500B\u76F4\u89D2\u4E09\u89D2\u5F62\uFF0C\u90A3\u7E54\u5973\u661F\u4FBF\u662F\u69CB\u6210\u76F4\u89D2\u7684\u661F\u661F\u3002 \u7E54\u5973\u661F\u7684\u5149\u8B5C\u5206\u985E\u70BAA0V\uFF0C\u5176\u6EAB\u5EA6\u6BD4\u5929\u72FC\u661F\u7684A1V\u9AD8\u4E00\u9EDE\u3002\u5B83\u4ECD\u65BC\u65BC\u4E3B\u5E8F\u661F\u968E\u6BB5\uFF0C\u4E26\u900F\u904E\u628A\u6838\u5FC3\u5167\u7684\u6C2B\uFF0C\u805A\u8B8A\u6210\u6C26\u4F86\u767C\u5149\u767C\u71B1\u3002\u6B64\u5916\uFF0C\u7E54\u5973\u661F\u7684\u8CEA\u91CF\u70BA\u592A\u967D\u76842.5\u500D\uFF0C\u7531\u65BC\u8CEA\u91CF\u8D8A\u9AD8\u7684\u6046\u661F\uFF0C\u5176\u6D88\u8017\u71C3\u6599\u7684\u901F\u5EA6\u4E5F\u8F03\u5FEB\uFF0C\u6BCF\u79D2\u653E\u51FA\u76F8\u7B49\u65BC\u592A\u967D50\u500D\u7684\u80FD\u91CF\uFF0C\u56E0\u6B64\u7E54\u5973\u661F\u7684\u58FD\u547D\u50C5\u70BA10\u5104\u5E74\uFF0C\u5373\u592A\u967D\u58FD\u547D\u7684\u5341\u4EFD\u4E4B\u4E00\uFF1B\u7D93\u6E2C\u5B9A\u7E54\u5973\u661F\u6BCF12.5\u5C0F\u6642\u81EA\u8F49\u4E00\u5468\uFF0C\u6574\u9846\u6046\u661F\u5448\u6241\u5E73\u72C0\uFF0C\u8D64\u9053\u76F4\u5F91\u6BD4\u5169\u6975\u5927\u4E8623%\u3002 \u7531\u65BC\u5929\u7403\u7684\u5929\u6975\u6703\u56E0\u6B72\u5DEE\u800C\u51FA\u73FE\u79FB\u4F4D\uFF0C\u56E0\u6B64\u7E54\u5973\u661F\u6703\u65BC\u5927\u7D04\u897F\u514314,000\u5E74\u6210\u70BA\u5317\u6975\u661F\u3002"@zh ,
"Alpha Lyrae (α Lyr) mais conhecida como Vega \u00E9 a estrela mais brilhante da constela\u00E7\u00E3o de Lira e a quinta estrela mais brilhante do c\u00E9u, separada do nosso sistema solar por 25 anos-luz o que equivale a 236.520.000.000.000 de quil\u00F4metros da terra (aproximadamente 1.576.800 UA de dist\u00E2ncia), o que a torna uma das estrelas mais pr\u00F3ximas do nosso Sol. Vega tem como di\u00E2metro 4.315.000 km, em compara\u00E7\u00E3o com a Terra (12.756 km) Vega \u00E9 338 vezes maior e 3 vezes maior do que o nosso sol. Considerada uma estrela nova, com pouco mais de 1 milh\u00E3o de anos desde sua forma\u00E7\u00E3o, um d\u00E9cimo do tempo do nosso Sol, tem duas vezes e meia a massa e cinq\u00FCenta vezes mais intensidade de brilho que nossa estrela. Astr\u00F4nomos calcularam a temperatura da estrela em cerca de 10.000 Kelvin nas regi\u00F5es polares e 7.600 Kelvin na linha equatorial. Vega tem um anel de poeira e gases a sua volta, o que na \u00E9poca de sua descoberta, nos anos 80, imaginou-se ser um in\u00EDcio de forma\u00E7\u00E3o planet\u00E1ria, mas estudos mais recentes chegaram a conclus\u00E3o de que mais provavelmente se trata de detritos de massas celestes, devido exatamente a idade relativamente jovem de Vega. Mesmo que ali existam planetas, \u00E9 pouco prov\u00E1vel que exista vida neles, devido ao pouco tempo de forma\u00E7\u00E3o da estrela. O famoso cientista e escritor Carl Sagan, ao escrever um de seus maiores sucessos liter\u00E1rios, Contato - estrelado no cinema pela atriz Jodie Foster \u2013 coloca Vega como ponto de encontro de uma civiliza\u00E7\u00E3o infinitamente mais adiantada que a nossa."@pt ,
"A Vega (\u03B1 Lyrae) a Lant csillagk\u00E9p legf\u00E9nyesebb csillaga, egyben az \u00E9szaki \u00E9gbolton a negyedik. Neve arab eredet\u0171, annyi mint \u201Elecsap\u00F3 sas\u201D, utalva arra, hogy az arab csillag\u00E1szok a Nagy Ny\u00E1ri H\u00E1romsz\u00F6gben h\u00E1rom madarat l\u00E1ttak. Eg\u00E9sz ny\u00E1ron megfigyelhet\u0151, est\u00E9nk\u00E9nt m\u00E1just\u00F3l febru\u00E1rig l\u00E1tszik. 52\u00B0 feletti sz\u00E9less\u00E9geken cirkumpol\u00E1ris. Fiatal, k\u00E9k f\u00E9ny\u0171 csillag, ez\u00E9rt rendk\u00EDv\u00FCl f\u00E9nyes, l\u00E1tsz\u00F3lagos f\u00E9nyess\u00E9ge 0,04, de magnit\u00FAd\u00F3ja krist\u00E1lytiszta \u00E9jjeleken negat\u00EDv \u00E9rt\u00E9keket is felvesz. A Naphoz viszonylag k\u00F6zeli csillag, 26 f\u00E9ny\u00E9v t\u00E1vols\u00E1gra van. Spektr\u00E1lis t\u00EDpusa \u201EA\u201D (feh\u00E9r)."@hu ,
"Vega, \u03B1 Lyrae, je typick\u00E1 hv\u011Bzda hlavn\u00ED posloupnosti. Je nejjasn\u011Bj\u0161\u00ED hv\u011Bzdou souhv\u011Bzd\u00ED Lyry. Je z\u00E1rove\u0148 p\u00E1tou nejjasn\u011Bj\u0161\u00ED hv\u011Bzdou oblohy. Vega tvo\u0159\u00ED spolu s nejjasn\u011Bj\u0161\u00EDmi hv\u011Bzdami souhv\u011Bzd\u00ED Labut\u011B a Orla letn\u00ED troj\u00FAheln\u00EDk. D\u00EDky precesi zemsk\u00E9 osy se kolem roku 14 000 dostane do bl\u00EDzkosti severn\u00EDho nebesk\u00E9ho p\u00F3lu a nahrad\u00ED tak pro \u00FA\u010Dely orientace dne\u0161n\u00ED Pol\u00E1rku. Vzhledem k tomu, \u017Ee jej\u00ED hv\u011Bzdn\u00E1 velikost je bl\u00EDzk\u00E1 hodnot\u011B 0, byla v 18. stolet\u00ED pou\u017E\u00EDv\u00E1na jako kalibra\u010Dn\u00ED hv\u011Bzda pro nastavov\u00E1n\u00ED stupnice hv\u011Bzdn\u00FDch velikost\u00ED, co\u017E ji\u017E dnes neplat\u00ED. Proto\u017Ee v\u0161ak m\u00E1 velice ploch\u00E9 spektrum v oblasti viditeln\u00E9ho a bl\u00EDzk\u00E9ho infra\u010Derven\u00E9ho z\u00E1\u0159en\u00ED, st\u00E1le standardem pro stanovov\u00E1n\u00ED tzv. barevn\u00E9ho indexu v syst\u00E9mu UBVGRI, kde v\u0161echny rozd\u00EDly jsou nastaveny na nulovou hodnotu. Vega je st\u00E1\u0159\u00EDm kolem 300 mili\u00F3n\u016F let pom\u011Brn\u011B mlad\u00E1 hv\u011Bzda. Ji\u017E del\u0161\u00ED dobu se v\u00ED, \u017Ee je obklopena protoplanet\u00E1rn\u00EDm diskem. V roce 2003 vypo\u010D\u00EDtali brit\u0161t\u00ED astronomov\u00E9, \u017Ee se vlastnosti protoplanet\u00E1rn\u00EDho disku daj\u00ED nejl\u00E9pe vysv\u011Btlit planetou, kter\u00E1 se podob\u00E1 Neptunu."@cs ,
"Vega, Lir Tak\u0131my\u0131ld\u0131z\u0131'nda (esk. \"Kanun Tak\u0131my\u0131ld\u0131z\u0131\") yer alan en parlak y\u0131ld\u0131z. Vega, Lyra Tak\u0131my\u0131ld\u0131z\u0131'n\u0131n alfa y\u0131ld\u0131z\u0131 olup, bu tak\u0131my\u0131ld\u0131z\u0131n en parlak [y\u0131ld\u0131z]\u0131d\u0131r. G\u00F6\u011F\u00FCn be\u015Finci parlak y\u0131ld\u0131z\u0131d\u0131r. Kuzey yar\u0131k\u00FCresinde Arcturus\u2019tan sonra ikinci parlak y\u0131ld\u0131zd\u0131r. G\u00FCne\u015F\u2019e 25.3 \u0131\u015F\u0131k y\u0131l\u0131 uzakl\u0131kta oldu\u011Fundan G\u00FCne\u015F\u2019e nispeten yak\u0131n bir y\u0131ld\u0131z say\u0131l\u0131r. Yakla\u015F\u0131k M. \u00D6. 12.000 y\u0131llar\u0131nda Kutup y\u0131ld\u0131z\u0131 oldu ve 12.000 y\u0131llar\u0131nda yeniden kutup y\u0131ld\u0131z\u0131 olacakt\u0131r. G\u00FCne\u015F\u2019ten sonra foto\u011Fraf\u0131 \u00E7ekilen ilk y\u0131ld\u0131zd\u0131r. Vega s\u00F6zc\u00FC\u011F\u00FC Arap\u00E7a en nasr el vak\u00EE (\u0627\u0644\u0646\u0633\u0631 \u0627\u0644\u0648\u0627\u0642\u0639 - av\u0131na \u00E7ullanan kartal) ifadesindeki vak\u00EE (d\u00FC\u015Fen) kelimesinden Latince yoluyla T\u00FCrk\u00E7eye ge\u00E7mi\u015Ftir. \u015Eems\u00FCl \u015F\u00FCmus olarak da bilinir. D\u00FCnya'dan yakla\u015F\u0131k 26 \u0131\u015F\u0131k y\u0131l\u0131 uzakta olan Vega, belirgin bir mavi \u0131\u015F\u0131kla parlar ve 0,03 ile 0,04 aras\u0131nda de\u011Fi\u015Fen g\u00F6r\u00FCn\u00FCr b\u00FCy\u00FCkl\u00FC\u011F\u00FCyle, g\u00F6ky\u00FCz\u00FCn\u00FCn en parlak 5. y\u0131ld\u0131z\u0131d\u0131r. 1840 y\u0131l\u0131nda Vega'n\u0131n paralaks\u0131n\u0131n (Biri D\u00FCnya'n\u0131n merkezinden, di\u011Feri yery\u00FCz\u00FCnde bulunan bir kimsenin g\u00F6z\u00FCnden \u00E7\u0131kan iki do\u011Frunun, bir g\u00F6kcisminin merkezinde birle\u015Ferek olu\u015Fturduklar\u0131 d\u00FC\u015F\u00FCn\u00FClen a\u00E7\u0131. ) Rus g\u00F6kbilimci Friedrich Georg Wilhelm von Struve taraf\u0131ndan bulunmas\u0131, y\u0131ld\u0131zlararas\u0131 uzakl\u0131klar\u0131n hesaplanmas\u0131 bak\u0131m\u0131ndan \u00F6nemli bir olayd\u0131r. Vega ayn\u0131 zamanda, foto\u011Fraf\u0131 \u00E7ekilen ilk y\u0131ld\u0131zd\u0131r. Lir Tak\u0131my\u0131ld\u0131z\u0131'nda yer alan Vega, Kartal Tak\u0131my\u0131ld\u0131z\u0131'ndaki Altair ve Ku\u011Fu Tak\u0131my\u0131ld\u0131z\u0131'ndaki Deneb'le birlikte yaz \u00FC\u00E7geninin k\u00F6\u015Felerini olu\u015Fturan y\u0131ld\u0131zlardan biridir. Vega, bir zamanlar \"Kutup y\u0131ld\u0131z\u0131\"yd\u0131. G\u00FCne\u015F ve Ay'\u0131n \u00E7ekim kuvvetlerinin etkisiyle, D\u00FCnya'n\u0131n ekvator b\u00F6lgesindeki \u015Fi\u015Fkinlik, gezegenin eksensel hareketinde bir teredd\u00FCte yol a\u00E7maktad\u0131r. Buna ba\u011Fl\u0131 olarak 26.000 y\u0131lda bir olu\u015Fan y\u00F6r\u00FCngesel sal\u0131n\u0131m, y\u0131ld\u0131zlar\u0131n g\u00F6ky\u00FCz\u00FCndeki konumlar\u0131n\u0131 da yava\u015F yava\u015F de\u011Fi\u015Ftirmektedir. Bu nedenle Vega, yakla\u015F\u0131k 11.500 y\u0131l sonra tekrar \"kutup y\u0131ld\u0131z\u0131\" konumunda olacakt\u0131r. Tayf t\u00FCr\u00FC A, y\u00FCzey s\u0131cakl\u0131\u011F\u0131 9.500 Kelvin derece olan Vega, G\u00FCne\u015F'ten yakla\u015F\u0131k 50 kat daha parlak bir y\u0131ld\u0131zd\u0131r. K\u00FCtlesi ise G\u00FCne\u015F'in k\u00FCtlesinin 2,5 kat\u0131ndan fazlad\u0131r. Bu nedenle, i\u00E7 yak\u0131t\u0131n\u0131 G\u00FCne\u015F'ten \u00E7ok daha h\u0131zl\u0131 t\u00FCketmektedir. Vega'n\u0131n \u00F6mr\u00FCn\u00FCn G\u00FCne\u015F'in \u00F6mr\u00FCn\u00FCn %10'undan bile k\u0131sa olaca\u011F\u0131 tahmin edimektedir. Buna g\u00F6re Vega, yakla\u015F\u0131k 1 milyar y\u0131l sonra s\u00F6nm\u00FC\u015F bir y\u0131ld\u0131z olacakt\u0131r. 1983 y\u0131l\u0131nda K\u0131z\u0131l\u00F6tesi G\u00F6kbilim Uydusu (\"Infrared Astronomy Satellite\", IRAS), y\u0131ld\u0131z\u0131n k\u0131z\u0131l\u00F6tesi \u0131\u015F\u0131n yayan ve taneciklerden olu\u015Fan b\u00FCy\u00FCk bir haleyle \u00E7evrelendi\u011Fini saptad\u0131. Disk bi\u00E7imindeki bu hale daha \u00E7ok s\u0131cak bir toz bulutuna benzemektedir ve y\u0131ld\u0131z\u0131n merkezinden yakla\u015F\u0131k 815 astronomik birim uza\u011Fa kadar yay\u0131lmaktad\u0131r. Vega'ya benzer pek\u00E7ok ba\u015Fka y\u0131ld\u0131z da benzer bir diske sahiptir. Vega'n\u0131n d\u00F6n\u00FC\u015F ekseninin D\u00FCnya'ya dik oldu\u011Fu, onu \u00E7evreleyen disk bi\u00E7imli toz bulutunun ise y\u00FCz\u00FCn\u00FCn bize d\u00F6n\u00FCk oldu\u011Fu g\u00F6zlenmi\u015Ftir. Yani, y\u0131ld\u0131z\u0131 \u00E7evreleyen disk, G\u00FCne\u015F'i \u00E7evreleyen ve gezegenleri i\u00E7eren ku\u015Fa\u011Fa benzer bi\u00E7imde konumlanm\u0131\u015Ft\u0131r. Bu nedenle, Vega'n\u0131n bir gezegen sistemi olabilece\u011Fi ya da b\u00F6yle bir sistemin olu\u015Fmakta oldu\u011Fu d\u00FC\u015F\u00FCncesi a\u011F\u0131rl\u0131k kazanm\u0131\u015Ft\u0131r. Helen Walker ve ekibinin \u0130ngiltere'deki Rutherford Appleton Laboratuar'\u0131na ba\u011Fl\u0131 K\u0131z\u0131l\u00F6tesi Uzay G\u00F6zlemevi'nde (Infrared Space Observatory) y\u00FCr\u00FCtt\u00FC\u011F\u00FC \u00E7al\u0131\u015Fmalar, Vega'n\u0131n diskinin 200 mikron b\u00FCy\u00FCkl\u00FC\u011F\u00FCnde, yani tipik y\u0131ld\u0131zlararas\u0131 tozdan 200 kat daha b\u00FCy\u00FCk taneciklerden olu\u015Ftu\u011Funu ortaya \u00E7\u0131kard\u0131. 2002 y\u0131l\u0131nda ise g\u00F6kbilimciler, toz bulutunun iki ayr\u0131 noktada yo\u011Funla\u015Farak u\u00E7 verdi\u011Fini duyurdular. Bunlardan biri y\u0131ld\u0131z\u0131n g\u00FCney bat\u0131s\u0131nda, y\u0131ld\u0131zdan 60 astronomik birim uzakta, di\u011Feri de kuzey do\u011Fusunda, y\u0131ld\u0131zdan 75 astronomik birim uzakta yer almaktayd\u0131. Bu duruma, d\u0131\u015Fmerkezli (eksantrik) bir y\u00F6r\u00FCnge \u00E7izen ve g\u00F6r\u00FClemeyen bir gezegenin yol a\u00E7\u0131yor olabilece\u011Fi d\u00FC\u015F\u00FCn\u00FClmektedir. Hesaplamalara g\u00F6re, ancak sarmal bir toz bulutunun i\u00E7inde d\u0131\u015Fmerkezli bir y\u00F6r\u00FCnge \u00E7izmekte olan bir gezegen, y\u0131ld\u0131zdan uzaktaki iki ayr\u0131 noktada bir yo\u011Funla\u015Fmaya neden olabilir. Bu durumun G\u00FCne\u015F Sistemi'nde g\u00F6r\u00FClmemesinin nedeni ise, gezegenlerin y\u00F6r\u00FCngelerinin b\u00F6yle bir etkiyi olu\u015Fturacak \u00F6l\u00E7\u00FCde d\u0131\u015Fmerkezli olmamas\u0131d\u0131r. G\u00FCne\u015F Sistemi d\u0131\u015F\u0131nda bulunan \u00E7ok say\u0131da gezegenin y\u00F6r\u00FCngelerinin d\u0131\u015Fmerkezli oldu\u011Fu bilinmektedir. Bu nedenle, asimetrik toz yo\u011Funla\u015Fmalar\u0131n\u0131n, d\u0131\u015F uzaydaki gezegen sistemlerinin ortak \u00F6zelliklerinden biri oldu\u011Fu d\u00FC\u015F\u00FCn\u00FClmektedir. \u00D6te yandan, bu etkiye bir gezegenin neden oldu\u011Fu varsay\u0131m\u0131 d\u0131\u015F\u0131nda, \u00E7ok b\u00FCy\u00FCk g\u00F6kta\u015Flar\u0131n\u0131n \u00E7arp\u0131\u015Fmalar\u0131n\u0131n da neden oluyor olabilece\u011Fi ileri s\u00FCr\u00FClmektedir. Ancak, her ne kadar eldeki verilerle tersi kan\u0131tlanamasa da, Vega'n\u0131n iki yan\u0131nda, biribirine kar\u015F\u0131t y\u00F6nlerde olu\u015Fan b\u00F6ylesi b\u00FCy\u00FCk \u00E7arp\u0131\u015Fmalar\u0131n ger\u00E7ekle\u015Fme olas\u0131l\u0131\u011F\u0131 olduk\u00E7a d\u00FC\u015F\u00FCkt\u00FCr. E\u011Fer Vega'n\u0131n gezegenleri varsa, bunlarda ya\u015Fam\u0131n geli\u015Fmi\u015F olmas\u0131 olanaks\u0131z gibidir. K\u00FCtlesi G\u00FCne\u015F'in k\u00FCtlesinin 2,5 kat\u0131ndan fazla olan Vega'n\u0131n hen\u00FCz 200 milyon y\u0131ll\u0131k ge\u00E7mi\u015Fi oldu\u011Fu tahmin edilmektedir. Bu s\u00FCrenin, ilkel canl\u0131lar\u0131n geli\u015Fmesi i\u00E7in bile \u00E7ok k\u0131sa oldu\u011Fu s\u00F6ylenebilir."@tr ,
"Vega (α Lyrae, alfa de Lira) \u00E9s l'estel m\u00E9s brillant de la constel\u00B7laci\u00F3 de Lira, culminant al zenit a les latituds mitjanes de l'hemisferi nord, durant l'estiu. \u00C9s un estel proper, a nom\u00E9s 25 anys llum de dist\u00E0ncia del Sol i, juntament amb Arcturus i S\u00EDrius, un dels estels m\u00E9s brillants en la proximitat del Sol. Vega \u00E9s un v\u00E8rtex del Triangle Estival. El seu nom prov\u00E9 del terme \u00E0rab waqi, que significa \u00ABall\u00F2 que cau\u00BB, a trav\u00E9s de la frase \u0627\u0644\u0646\u0633\u0631 \u0627\u0644\u0648\u0627\u0642\u0639 an-nasr al-w\u0101qi\u2018, tradu\u00EFda com a \u00ABl'\u00E0liga que cau en picat\u00BB. En les representacions gr\u00E0fiques de la constel\u00B7laci\u00F3, Vega apareix com una joia incrustada en el cos de la Lira. La seva classificaci\u00F3 espectral \u00E9s A0V (S\u00EDrius, una A1V, \u00E9s lleugerament menys potent) i est\u00E0 dins de la seq\u00FC\u00E8ncia principal, mentre t\u00E9 lloc la fusi\u00F3 d'hidrogen en heli en el seu nucli. Donat que estels m\u00E9s potents usen el seu combustible de fusi\u00F3 m\u00E9s r\u00E0pidament que els petits, la vida de Vega \u00E9s nom\u00E9s de 1.000 milions d'anys, una desena part que la del Sol. Vega tamb\u00E9 \u00E9s tres vegades m\u00E9s massiva que el Sol i crema amb una pot\u00E8ncia cinquanta vegades superior. Vega t\u00E9 un disc de pols i gas al voltant, descobert pel sat\u00E8l\u00B7lit IRAS a mitjan dels anys 1980. Aix\u00F2 significa que hi ha planetes o planetes en formaci\u00F3. El disc protoplanetari \u00E9s, com es pot endevinar pel seu nom, un precursor de la formaci\u00F3 de planetes per\u00F2 pot persistir molt de temps despr\u00E9s de la formaci\u00F3 dels planetes si no hi ha planetes gasosos gegants com J\u00FApiter. Cap a l'any 14.000, Vega ser\u00E0 l'estrella que indicar\u00E0 el Nord, en lloc de l'estrella polar, a causa de la precessi\u00F3 dels equinoccis. Els astr\u00F2noms professionals han usat Vega per a la calibraci\u00F3 d'escales fotom\u00E8triques de brillantor absoluta. Quan la magnitud de l'escala es va fixar, va resultar que Vega estava a prop de la magnitud zero. Aix\u00ED, es va decidir que la magnitud aparent de Vega seria, per definici\u00F3, zero a totes les longituds d'ona. Actualment ja no se segueix aquest patr\u00F3 i Vega ja no est\u00E0 calibrada com a punt de magnitud zero. Vega t\u00E9 un espectre electromagn\u00E8tic relativament pla a la regi\u00F3 visible (longituds d'ona de 350-850 nan\u00F2metres, que l'ull hum\u00E0 pot observar). El flux de Vega decau r\u00E0pidament a l'infraroig."@ca ,
"Wega (ook wel Vega) (alpha Lyrae) is de helderste ster in het sterrenbeeld Lier (Lyra) en een van de helderste van de noordelijke hemel. De ster staat ook bekend als Fidis en \"de harpster\". Door de Arabieren werd Wega Al Nasr al Waki, de Vallende Adelaar van de woestijn genoemd, in bronnen van 4000 jaar oud komt de ster al voor als Ma'at. In 1983 werd door de IRAS satelliet ontdekt dat de ster omgeven wordt door een schijf van stof waaruit in de toekomst misschien planeten kunnen ontstaan. Door de precessie van de aardas stond ongeveer 14000 jaar geleden de noordelijke hemelpool in de buurt van Wega, dit was toen dus de Poolster en niet de ster Polaris."@nl ,
"Vega (α Lyrae) \u00E4r den ljusaste stj\u00E4rnan i stj\u00E4rnbilden Lyran. Namnet kommer fr\u00E5n det arabiska ordet waqi som betyder \"st\u00F6rtande\", fr\u00E5n frasen \"den st\u00F6rtande gamen\". Vega \u00E4r den n\u00E4st ljusaste stj\u00E4rnan p\u00E5 den norra stj\u00E4rnhimlen och den femte ljusaste stj\u00E4rnan p\u00E5 hela stj\u00E4rnhimlen. Avst\u00E5ndet till Vega \u00E4r 25 ljus\u00E5r, d\u00E4rmed \u00E4r Vega en relativt n\u00E4rbel\u00E4gen stj\u00E4rna. Stj\u00E4rnan har en massa som \u00E4r 2,5 g\u00E5nger s\u00E5 stor som solen. Dess effekt \u00E4r 50 g\u00E5nger st\u00F6rre \u00E4n solens, vilket g\u00F6r att den kommer att ha en livsl\u00E4ngd 1 000 000 000 \u00E5r, en tiondel av solens. Runt Vega finns en gasfattig cirkumstell\u00E4r skiva av kollisionsspillror och partiklar, uppt\u00E4ckt av satelliten IRAS p\u00E5 1980-talet. Detta antyder att planeter \u00E4r f\u00E4rdigbildade, om s\u00E5dana n\u00E5gonsin har bildats."@sv ,
"Vega (Alpha Lyrae) er den sterkeste stjernen i stjernebildet Lyren og den femte sterkeste stjernen p\u00E5 stjernehimmelen, m\u00E5lt etter tilsynelatende lysstyrke. Sammen med Deneb og Altair utgj\u00F8r den sommertriangelet, som er godt synlig p\u00E5 den nordlige halvkule. Navnet Vega kommer fra det arabiske ordet waqi, \u00ABfallende\u00BB, etter uttrykket an-nasr al w\u0101qi` (\u0646\u0633\u0631 \u0627\u0644\u0648\u0627\u0642\u0639), som betyr \u00ABden fallende \u00F8rna\u00BB. Vega er en relativt n\u00E6rliggende stjerne, bare 25,3 lys\u00E5r borte. Vega var den f\u00F8rste stjernen som ble fotografert, i 1850, og i 1872 ble det tatt bilde av spekteret. Vega var ogs\u00E5 den f\u00F8rste stjernen man klarte \u00E5 m\u00E5le avstanden til med en rimelig h\u00F8y n\u00F8yaktighetsgrad. Da man fastsatte skalene for en stjernes lysstyrke, valgte man Vega som basis og lot den f\u00E5 relativ lysstyrke 0. Vega er relativt ung og har en uvanlig lav mengde med grunnstoffer med st\u00F8rre atommasse enn helium. Den type stjerne som Vega representerer, har en levetid p\u00E5 bare rundt 1 milliard \u00E5r, alts\u00E5 bare ca tidelen av levealderen til v\u00E5r sol. Man regner med at Vegas alder er mellom 386 og 511 millioner \u00E5r, slik at den er halvveis i livsl\u00F8pet sitt. Vegas masse er omtrent 2 ganger solmassen, og lysstr\u00E5lingen er 37 ganger solens. Den roterer med en fart p\u00E5 274 km/s ved ekvator. Dette f\u00E5r ekvator til \u00E5 bule ut p\u00E5 grunn av sentrifugalkraften. I 1983 fant man at Vega har en skive av st\u00F8v rundt seg. Dette st\u00F8vet er langt vekk fra stjernen og har en temperatur p\u00E5 -180 \u00B0C. Det er beregnet at massen til dette st\u00F8vet er p\u00E5 0,3 % av jordas masse. Det er derfor lite sannsynlig at det vil skje en dannelse av protoplaneter her i dette st\u00F8vlaget. Imidlertid fins det sannsynligvis en stor planet i dette solsystemet, omtrent p\u00E5 Neptuns st\u00F8rrelse. Ogs\u00E5 stjernene Fomalhaut og HR 4796 kan ha planeter omkring seg."@no ,
"Wega, auch bekannt als \u03B1 Lyrae, ist der Hauptstern des Sternbildes Leier (Lyra); der Name leitet sich vom arabischen Ausdruck \u0627\u0644\u0646\u0633\u0631 \u0627\u0644\u0648\u0627\u0642\u0639, an-nasr al-w\u0101qi\u02BF ab, was in \u00DCbersetzung \u201Eherabsto\u00DFender (Adler)\u201C bedeutet."@de ,
"Vega (Wega, \u03B1 Lyr, Alfa Lyrae) on Lyyran t\u00E4hdist\u00F6n p\u00E4\u00E4t\u00E4hti. T\u00E4m\u00E4 kirkas sinert\u00E4v\u00E4nvalkea t\u00E4hti on melko l\u00E4hell\u00E4 meit\u00E4, \"vain\" 25,3 valovuoden p\u00E4\u00E4ss\u00E4. Vega on 3. kirkkain meille Suomeen n\u00E4kyv\u00E4 kiintot\u00E4hti, vain Arcturus ja Sirius ovat kirkkaampia. Vega on niin sanotun Kes\u00E4kolmion k\u00E4rkit\u00E4hti. Kes\u00E4kolmioon kuuluvat my\u00F6s Joutsenen Deneb ja Kotkan Altair. Vega on my\u00F6s viidenneksi kirkkain t\u00E4hti pohjoisella taivaanpallonpuoliskolla. Suomessa Vega n\u00E4kyy aina (on horisontin yl\u00E4puolella), sill\u00E4 kyseinen t\u00E4hti on sirkumpolaarinen eli sen deklinaatio on enemm\u00E4n kuin Suomen leveysaste Maan p\u00E4\u00E4ll\u00E4. Vegaa on k\u00E4ytetty elokuvassa Ensimm\u00E4inen yhteys."@fi ,
"Vega \u00E8 la stella pi\u00F9 brillante della costellazione della Lira, la quinta pi\u00F9 luminosa del cielo notturno, nonch\u00E9 la seconda pi\u00F9 luminosa nell'emisfero celeste boreale, dopo Arturo. Vertice nord-occidentale dell'asterismo del Triangolo Estivo, Vega \u00E8 una stella piuttosto vicina, posta a soli 25 anni luce di distanza, la pi\u00F9 luminosa in termini assoluti entro un raggio di 30 anni luce dal sistema solare. Si tratta di una stella bianca di sequenza principale di classe spettrale A0 V, che possiede una massa circa due volte quella solare ed una luminosit\u00E0 circa 37 volte superiore. L'astro \u00E8 caratterizzato da un'altissima velocit\u00E0 di rotazione sul proprio asse, che gli conferisce l'aspetto di uno sferoide oblato. Questa rapida rotazione, a causa di un fenomeno noto come oscuramento gravitazionale, si riflette sulla temperatura effettiva fotosferica, che varia a seconda della latitudine presa in esame: infatti, si \u00E8 notato che la temperatura all'equatore \u00E8 di circa 2000 K pi\u00F9 bassa rispetto a quella rilevata ai poli, ed \u00E8 proprio in direzione di uno di essi che la stella risulta visibile dalla Terra. \u00C8 inoltre una sospetta variabile Delta Scuti, che manifesta pulsazioni nella luminosit\u00E0 di pochi centesimi di magnitudine ogni 0,19 giorni (circa 4,56 ore). Vega, definita dagli astronomi \"la stella pi\u00F9 importante nel cielo dopo il Sole\", riveste una grande importanza nell'astronomia, dal momento \u00E8 stata impiegata per calibrare gli strumenti osservativi e come riferimento per la misurazione di alcuni parametri comuni a tutte le stelle; inoltre, circa 12 000 anni fa, a causa della precessione dell'asse terrestre, ha svolto il ruolo di stella polare, e lo ricoprir\u00E0 nuovamente tra altri 13 700 anni. A met\u00E0 degli anni ottanta il satellite IRAS ha scoperto, che la stella presenta un eccesso di emissione infrarossa, attribuito alla presenza in orbita di un disco di polveri circumstellare. Queste polveri sarebbero il risultato di collisioni plurime tra gli oggetti orbitanti all'interno di una cintura asteroidale, assimilabile alla fascia di Kuiper nel sistema solare. Alcune irregolarit\u00E0 riscontrate nel disco suggerirebbero la presenza in orbita di almeno un pianeta, per massa simile a Giove. Il nome Vega deriva dalla seconda parte del nome in arabo della stella \u0627\u0644\u0646\u0633\u0631 \u0627\u0644\u0648\u0627\u0642\u0639 an-nasr al-w\u0101qi\u2018, Avvoltoio che plana."@it ,
"\u0412\u0435\u0301\u0433\u0430 (\u03B1 \u041B\u0438\u0440\u044B)\u00A0\u2014 \u0441\u0430\u043C\u0430\u044F \u044F\u0440\u043A\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u041B\u0438\u0440\u044B, \u043F\u044F\u0442\u0430\u044F \u043F\u043E \u044F\u0440\u043A\u043E\u0441\u0442\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 \u043D\u043E\u0447\u043D\u043E\u0433\u043E \u043D\u0435\u0431\u0430 \u0438 \u0432\u0442\u043E\u0440\u0430\u044F\u00A0\u2014 \u0432 \u0421\u0435\u0432\u0435\u0440\u043D\u043E\u043C \u043F\u043E\u043B\u0443\u0448\u0430\u0440\u0438\u0438, \u0442\u0440\u0435\u0442\u044C\u044F \u043F\u043E \u044F\u0440\u043A\u043E\u0441\u0442\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 (\u043F\u043E\u0441\u043B\u0435 \u0421\u0438\u0440\u0438\u0443\u0441\u0430 \u0438 \u0410\u0440\u043A\u0442\u0443\u0440\u0430), \u043A\u043E\u0442\u043E\u0440\u0430\u044F \u043C\u043E\u0436\u0435\u0442 \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0442\u044C\u0441\u044F \u0432 \u0420\u043E\u0441\u0441\u0438\u0438 \u0438 \u0431\u043B\u0438\u0436\u043D\u0435\u043C \u0437\u0430\u0440\u0443\u0431\u0435\u0436\u044C\u0435. \u0412\u0435\u0433\u0430 \u043E\u0442\u0441\u0442\u043E\u0438\u0442 \u043D\u0430 25,3 \u0441\u0432\u0435\u0442\u043E\u0432\u044B\u0445 \u043B\u0435\u0442 \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430 \u0438 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u043E\u0434\u043D\u043E\u0439 \u0438\u0437 \u044F\u0440\u0447\u0430\u0439\u0448\u0438\u0445 \u0437\u0432\u0451\u0437\u0434 (\u043D\u0430\u0440\u044F\u0434\u0443 \u0441 \u0410\u0440\u043A\u0442\u0443\u0440\u043E\u043C \u0438 \u0421\u0438\u0440\u0438\u0443\u0441\u043E\u043C) \u0432 \u0435\u0433\u043E \u043E\u043A\u0440\u0435\u0441\u0442\u043D\u043E\u0441\u0442\u044F\u0445 (\u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 \u0434\u043E 10 \u043F\u0430\u0440\u0441\u0435\u043A). \u041D\u0430\u0437\u0432\u0430\u043D\u0438\u0435 \u00AB\u0412\u0435\u0433\u0430\u00BB \u043F\u0440\u043E\u0438\u0437\u043E\u0448\u043B\u043E \u043E\u0442 \u043F\u0440\u0438\u0431\u043B\u0438\u0437\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0439 \u0442\u0440\u0430\u043D\u0441\u043B\u0438\u0442\u0435\u0440\u0430\u0446\u0438\u0438 \u0430\u0440\u0430\u0431\u0441\u043A\u043E\u0433\u043E \u0441\u043B\u043E\u0432\u0430 waqi (\u00AB\u043F\u0430\u0434\u0430\u044E\u0449\u0438\u0439\u00BB) \u0438\u0437 \u0444\u0440\u0430\u0437\u044B \u0627\u0644\u0646\u0633\u0631 \u0627\u0644\u0648\u0627\u0642\u0639 (an-nasr al-w\u0101qi\u2018, \u00AB\u043F\u0430\u0434\u0430\u044E\u0449\u0438\u0439 \u043E\u0440\u0451\u043B\u00BB), \u0442\u0430\u043A \u043A\u0430\u043A \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0435 \u041B\u0438\u0440\u044B \u0432 \u0434\u0440\u0435\u0432\u043D\u0435\u043C \u043C\u0438\u0440\u0435 \u0438\u0437\u043E\u0431\u0440\u0430\u0436\u0430\u043B\u043E\u0441\u044C \u0432 \u0432\u0438\u0434\u0435 \u043F\u0438\u043A\u0438\u0440\u0443\u044E\u0449\u0435\u0433\u043E \u043E\u0440\u043B\u0430 \u0438\u043B\u0438 \u0433\u0440\u0438\u0444\u0430."@ru ,
"Vega sau \u03B1 Lyrae este cea mai str\u0103lucitoare stea a constela\u0163iei Lira, a cincea cea mai str\u0103lucitoare stea de pe cer \u015Fi a doua cea mai str\u0103lucitoare din emisfera celestial\u0103 nordic\u0103. Are o magnitudine de 0.03 \u015Fi se afl\u0103 la o distanta de 25.31 ani-lumin\u0103 de P\u0103m\u00E2nt."@ro ,
"Vega (Alfa Lyrae / \u03B1 Lyr) es una estrella de primera magnitud (en la clasificaci\u00F3n de Ptolomeo) de la constelaci\u00F3n de la Lira y la principal de la misma. Su nombre proviene de la latinizaci\u00F3n medieval de su denominaci\u00F3n \u00E1rabe, waqi (\u0624\u0627\u0642\u0639) que significa que cae. Para un observador ubicado en una latitud norte central, se aproxima al cenit durante el verano boreal. A tan s\u00F3lo 25 a\u00F1os luz, se cuenta como una de las al Sistema Solar, y como una de las del Sol junto con Sirio y Arturo. Es la del cielo nocturno. Seg\u00FAn an\u00E1lisis espectrogr\u00E1ficos, Vega est\u00E1 en la etapa de secuencia principal, es decir, est\u00E1 convirtiendo hidr\u00F3geno en helio en su n\u00FAcleo. Puesto que las estrellas m\u00E1s masivas y brillantes consumen su combustible m\u00E1s r\u00E1pidamente, la vida de Vega se estima solamente en mil millones de a\u00F1os, un d\u00E9cimo de la de nuestro Sol. Vega es dos veces y media m\u00E1s masiva que el Sol y arde con una luminosidad treinta y siete veces la de \u00E9ste. Vega posee un disco de polvo y gas a su alrededor que fue descubierto por el sat\u00E9lite IRAS a mediados de la d\u00E9cada de los 80. Esto puede significar que o bien tiene planetas, o que se podr\u00EDan formar relativamente pronto. En el a\u00F1o 13.600 ser\u00E1 la estrella Polar (lugar ocupado en estos momentos por Polaris) debido al fen\u00F3meno de la precesi\u00F3n de los equinoccios. Los astr\u00F3nomos profesionales han utilizado a Vega para fijar los baremos absolutos de brillo fotom\u00E9trico, lo que supone que la magnitud visual de Vega es aproximadamente cero en todas las longitudes de onda. La intenci\u00F3n original era que el valor fuera exactamente cero, pero en la pr\u00E1ctica no result\u00F3 as\u00ED. Por ejemplo, en el filtro V de Johnson (el m\u00E1s usado por los astr\u00F3nomos en el rango visible o visual), la magnitud de Vega es 0,026 \u00B1 0,008, y en otros filtros hay tambi\u00E9n desviaciones de unas pocas cent\u00E9simas. Tiene tambi\u00E9n un espectro relativamente plano en la regi\u00F3n visual (un campo de longitud de onda que va desde los 350 a los 850 nan\u00F3metros, la mayor\u00EDa de las cuales son visibles al ojo humano), de modo que las densidades de flujo son aproximadamente iguales, 2000-4000 Jy. La densidad de flujo de Vega se reduce r\u00E1pidamente en el infrarrojo y se acerca a los 100 Jy en 5 micr\u00F3metros). Vega es un ejemplo de estrella que rota a gran velocidad, como Altair (\u03B1 Aquilae) o Regulus (\u03B1 Leonis), por lo que su radio ecuatorial es significativamente mayor que su radio polar. Una velocidad de rotaci\u00F3n alta tambi\u00E9n genera diferencias de temperatura superficial entre el ecuador y los polos. La velocidad de rotaci\u00F3n en el ecuador de Vega es de 275 km/s, lo que hace que los polos est\u00E9n a una temperatura superficial de 10.150 K y el ecuador a una temperatura de 7.900 K."@es ;
rdfs:comment ""@zh ,
"Vega (Alpha Lyrae) er den sterkeste stjernen i stjernebildet Lyren og den femte sterkeste stjernen p\u00E5 stjernehimmelen, m\u00E5lt etter tilsynelatende lysstyrke. Sammen med Deneb og Altair utgj\u00F8r den sommertriangelet, som er godt synlig p\u00E5 den nordlige halvkule. Navnet Vega kommer fra det arabiske ordet waqi, \u00ABfallende\u00BB, etter uttrykket an-nasr al w\u0101qi` (\u0646\u0633\u0631 \u0627\u0644\u0648\u0627\u0642\u0639), som betyr \u00ABden fallende \u00F8rna\u00BB. Vega er en relativt n\u00E6rliggende stjerne, bare 25,3 lys\u00E5r borte."@no ,
"A Vega (\u03B1 Lyrae) a Lant csillagk\u00E9p legf\u00E9nyesebb csillaga, egyben az \u00E9szaki \u00E9gbolton a negyedik. Neve arab eredet\u0171, annyi mint \u201Elecsap\u00F3 sas\u201D, utalva arra, hogy az arab csillag\u00E1szok a Nagy Ny\u00E1ri H\u00E1romsz\u00F6gben h\u00E1rom madarat l\u00E1ttak. Eg\u00E9sz ny\u00E1ron megfigyelhet\u0151, est\u00E9nk\u00E9nt m\u00E1just\u00F3l febru\u00E1rig l\u00E1tszik. 52\u00B0 feletti sz\u00E9less\u00E9geken cirkumpol\u00E1ris."@hu ,
"Vega sau \u03B1 Lyrae este cea mai str\u0103lucitoare stea a constela\u0163iei Lira, a cincea cea mai str\u0103lucitoare stea de pe cer \u015Fi a doua cea mai str\u0103lucitoare din emisfera celestial\u0103 nordic\u0103. Are o magnitudine de 0.03 \u015Fi se afl\u0103 la o distanta de 25.31 ani-lumin\u0103 de P\u0103m\u00E2nt."@ro ,
"Vega (Alfa Lyrae / \u03B1 Lyr) es una estrella de primera magnitud (en la clasificaci\u00F3n de Ptolomeo) de la constelaci\u00F3n de la Lira y la principal de la misma. Su nombre proviene de la latinizaci\u00F3n medieval de su denominaci\u00F3n \u00E1rabe, waqi (\u0624\u0627\u0642\u0639) que significa que cae. Para un observador ubicado en una latitud norte central, se aproxima al cenit durante el verano boreal. A tan s\u00F3lo 25 a\u00F1os luz, se cuenta como una de las al Sistema Solar, y como una de las del Sol junto con Sirio y Arturo."@es ,
"Wega (Alpha Lyrae, \u03B1 Lyr) - najja\u015Bniejsza gwiazda w gwiazdozbiorze Lutni, pi\u0105ta co do jasno\u015Bci gwiazda nieba, a trzecia na niebie p\u00F3\u0142nocnym. Odleg\u0142a od S\u0142o\u0144ca o 25,3 lat \u015Bwietlnych. Wraz z Deneb i Altair tworzy tzw. tr\u00F3jk\u0105t letni."@pl ,
"Vega (\u03B1 Lyr / \u03B1 Lyrae / Alpha Lyrae) is the brightest star in the constellation Lyra, the fifth brightest star in the night sky and the second brightest star in the northern celestial hemisphere, after Arcturus. It is a relatively nearby star at only 25 light-years from Earth, and, together with Arcturus and Sirius, one of the most luminous stars in the Sun's neighborhood."@en ,
"\u0412\u0435\u0301\u0433\u0430 (\u03B1 \u041B\u0438\u0440\u044B)\u00A0\u2014 \u0441\u0430\u043C\u0430\u044F \u044F\u0440\u043A\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u041B\u0438\u0440\u044B, \u043F\u044F\u0442\u0430\u044F \u043F\u043E \u044F\u0440\u043A\u043E\u0441\u0442\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 \u043D\u043E\u0447\u043D\u043E\u0433\u043E \u043D\u0435\u0431\u0430 \u0438 \u0432\u0442\u043E\u0440\u0430\u044F\u00A0\u2014 \u0432 \u0421\u0435\u0432\u0435\u0440\u043D\u043E\u043C \u043F\u043E\u043B\u0443\u0448\u0430\u0440\u0438\u0438, \u0442\u0440\u0435\u0442\u044C\u044F \u043F\u043E \u044F\u0440\u043A\u043E\u0441\u0442\u0438 \u0437\u0432\u0435\u0437\u0434\u0430 (\u043F\u043E\u0441\u043B\u0435 \u0421\u0438\u0440\u0438\u0443\u0441\u0430 \u0438 \u0410\u0440\u043A\u0442\u0443\u0440\u0430), \u043A\u043E\u0442\u043E\u0440\u0430\u044F \u043C\u043E\u0436\u0435\u0442 \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0442\u044C\u0441\u044F \u0432 \u0420\u043E\u0441\u0441\u0438\u0438 \u0438 \u0431\u043B\u0438\u0436\u043D\u0435\u043C \u0437\u0430\u0440\u0443\u0431\u0435\u0436\u044C\u0435."@ru ,
""@ja ,
"Vega \u00E8 la stella pi\u00F9 brillante della costellazione della Lira, la quinta pi\u00F9 luminosa del cielo notturno, nonch\u00E9 la seconda pi\u00F9 luminosa nell'emisfero celeste boreale, dopo Arturo. Vertice nord-occidentale dell'asterismo del Triangolo Estivo, Vega \u00E8 una stella piuttosto vicina, posta a soli 25 anni luce di distanza, la pi\u00F9 luminosa in termini assoluti entro un raggio di 30 anni luce dal sistema solare."@it ,
"Alpha Lyrae (α Lyr) mais conhecida como Vega \u00E9 a estrela mais brilhante da constela\u00E7\u00E3o de Lira e a quinta estrela mais brilhante do c\u00E9u, separada do nosso sistema solar por 25 anos-luz o que equivale a 236.520.000.000.000 de quil\u00F4metros da terra (aproximadamente 1.576.800 UA de dist\u00E2ncia), o que a torna uma das estrelas mais pr\u00F3ximas do nosso Sol."@pt ,
"Vega (α Lyrae) \u00E4r den ljusaste stj\u00E4rnan i stj\u00E4rnbilden Lyran. Namnet kommer fr\u00E5n det arabiska ordet waqi som betyder \"st\u00F6rtande\", fr\u00E5n frasen \"den st\u00F6rtande gamen\". Vega \u00E4r den n\u00E4st ljusaste stj\u00E4rnan p\u00E5 den norra stj\u00E4rnhimlen och den femte ljusaste stj\u00E4rnan p\u00E5 hela stj\u00E4rnhimlen. Avst\u00E5ndet till Vega \u00E4r 25 ljus\u00E5r, d\u00E4rmed \u00E4r Vega en relativt n\u00E4rbel\u00E4gen stj\u00E4rna. Stj\u00E4rnan har en massa som \u00E4r 2,5 g\u00E5nger s\u00E5 stor som solen."@sv ,
"Alpha Lyrae (\u03B1 Lyrae / \u03B1 Lyr), plus connue sous son nom traditionnel de V\u00E9ga, est l'\u00E9toile la plus brillante de la constellation de la Lyre. Vue depuis la Terre, il s'agit de la cinqui\u00E8me \u00E9toile la plus brillante du ciel, la deuxi\u00E8me de l'h\u00E9misph\u00E8re nord juste apr\u00E8s Arcturus. C'est une \u00E9toile relativement proche du Soleil, \u00E0 25,3 ann\u00E9es-lumi\u00E8re de celui-ci."@fr ,
"Vega, Lir Tak\u0131my\u0131ld\u0131z\u0131'nda (esk. \"Kanun Tak\u0131my\u0131ld\u0131z\u0131\") yer alan en parlak y\u0131ld\u0131z. Vega, Lyra Tak\u0131my\u0131ld\u0131z\u0131'n\u0131n alfa y\u0131ld\u0131z\u0131 olup, bu tak\u0131my\u0131ld\u0131z\u0131n en parlak [y\u0131ld\u0131z]\u0131d\u0131r. G\u00F6\u011F\u00FCn be\u015Finci parlak y\u0131ld\u0131z\u0131d\u0131r. Kuzey yar\u0131k\u00FCresinde Arcturus\u2019tan sonra ikinci parlak y\u0131ld\u0131zd\u0131r. G\u00FCne\u015F\u2019e 25.3 \u0131\u015F\u0131k y\u0131l\u0131 uzakl\u0131kta oldu\u011Fundan G\u00FCne\u015F\u2019e nispeten yak\u0131n bir y\u0131ld\u0131z say\u0131l\u0131r. Yakla\u015F\u0131k M. \u00D6."@tr ,
"Vega (α Lyrae, alfa de Lira) \u00E9s l'estel m\u00E9s brillant de la constel\u00B7laci\u00F3 de Lira, culminant al zenit a les latituds mitjanes de l'hemisferi nord, durant l'estiu. \u00C9s un estel proper, a nom\u00E9s 25 anys llum de dist\u00E0ncia del Sol i, juntament amb Arcturus i S\u00EDrius, un dels estels m\u00E9s brillants en la proximitat del Sol. Vega \u00E9s un v\u00E8rtex del Triangle Estival."@ca ,
"\u0412\u0435\u0301\u0491\u0430 (\u0430\u0440\u0430\u0431. \u0432\u0430\u043A\u0456 \u00AB\u043F\u0430\u0434\u0430\u044E\u0447\u0430\u00BB) (\u03B1 \u041B\u0456\u0440\u0438) \u2014 \u043D\u0430\u0439\u044F\u0441\u043A\u0440\u0430\u0432\u0456\u0448\u0430 \u0417\u0456\u0440\u043A\u0430 \u0443 \u0441\u0443\u0437\u0456\u0440'\u0457 \u041B\u0456\u0440\u0438, \u043F'\u044F\u0442\u0430 \u0437\u0430 \u044F\u0441\u043A\u0440\u0430\u0432\u0456\u0441\u0442\u044E \u0417\u0456\u0440\u043A\u0430 \u043D\u0456\u0447\u043D\u043E\u0433\u043E \u043D\u0435\u0431\u0430, \u0434\u0440\u0443\u0433\u0430 \u043F\u0456\u0441\u043B\u044F \u0410\u0440\u043A\u0442\u0443\u0440\u0430 \u0432 \u043F\u0456\u0432\u043D\u0456\u0447\u043D\u0456\u0439 \u043F\u0456\u0432\u043A\u0443\u043B\u0456. \u0426\u0435 \u2014 \u0432\u0456\u0434\u043D\u043E\u0441\u043D\u043E \u0431\u043B\u0438\u0437\u044C\u043A\u0430 \u0437\u0456\u0440\u043A\u0430 (25 \u0441\u0432\u0456\u0442\u043B\u043E\u0432\u0438\u0445 \u0440\u043E\u043A\u0456\u0432 \u0432\u0456\u0434 \u0417\u0435\u043C\u043B\u0456), \u0456, \u0440\u0430\u0437\u043E\u043C \u0437 \u0410\u0440\u043A\u0442\u0443\u0440\u043E\u043C \u0456 \u0421\u0456\u0440\u0456\u0443\u0441\u043E\u043C, \u043E\u0434\u043D\u0430 \u0437 \u043D\u0430\u0439\u044F\u0441\u043A\u0440\u0430\u0432\u0456\u0448\u0438\u0445 \u0437\u0456\u0440\u043E\u043A."@uk ,
"Vega (Wega, \u03B1 Lyr, Alfa Lyrae) on Lyyran t\u00E4hdist\u00F6n p\u00E4\u00E4t\u00E4hti. T\u00E4m\u00E4 kirkas sinert\u00E4v\u00E4nvalkea t\u00E4hti on melko l\u00E4hell\u00E4 meit\u00E4, \"vain\" 25,3 valovuoden p\u00E4\u00E4ss\u00E4. Vega on 3. kirkkain meille Suomeen n\u00E4kyv\u00E4 kiintot\u00E4hti, vain Arcturus ja Sirius ovat kirkkaampia. Vega on niin sanotun Kes\u00E4kolmion k\u00E4rkit\u00E4hti. Kes\u00E4kolmioon kuuluvat my\u00F6s Joutsenen Deneb ja Kotkan Altair. Vega on my\u00F6s viidenneksi kirkkain t\u00E4hti pohjoisella taivaanpallonpuoliskolla."@fi ,
"Wega, auch bekannt als \u03B1 Lyrae, ist der Hauptstern des Sternbildes Leier (Lyra); der Name leitet sich vom arabischen Ausdruck \u0627\u0644\u0646\u0633\u0631 \u0627\u0644\u0648\u0627\u0642\u0639, an-nasr al-w\u0101qi\u02BF ab, was in \u00DCbersetzung \u201Eherabsto\u00DFender (Adler)\u201C bedeutet."@de ,
"Wega (ook wel Vega) (alpha Lyrae) is de helderste ster in het sterrenbeeld Lier (Lyra) en een van de helderste van de noordelijke hemel. De ster staat ook bekend als Fidis en \"de harpster\". Door de Arabieren werd Wega Al Nasr al Waki, de Vallende Adelaar van de woestijn genoemd, in bronnen van 4000 jaar oud komt de ster al voor als Ma'at. In 1983 werd door de IRAS satelliet ontdekt dat de ster omgeven wordt door een schijf van stof waaruit in de toekomst misschien planeten kunnen ontstaan."@nl ,
"Vega, \u03B1 Lyrae, je typick\u00E1 hv\u011Bzda hlavn\u00ED posloupnosti. Je nejjasn\u011Bj\u0161\u00ED hv\u011Bzdou souhv\u011Bzd\u00ED Lyry. Je z\u00E1rove\u0148 p\u00E1tou nejjasn\u011Bj\u0161\u00ED hv\u011Bzdou oblohy. Vega tvo\u0159\u00ED spolu s nejjasn\u011Bj\u0161\u00EDmi hv\u011Bzdami souhv\u011Bzd\u00ED Labut\u011B a Orla letn\u00ED troj\u00FAheln\u00EDk. D\u00EDky precesi zemsk\u00E9 osy se kolem roku 14 000 dostane do bl\u00EDzkosti severn\u00EDho nebesk\u00E9ho p\u00F3lu a nahrad\u00ED tak pro \u00FA\u010Dely orientace dne\u0161n\u00ED Pol\u00E1rku. Vzhledem k tomu, \u017Ee jej\u00ED hv\u011Bzdn\u00E1 velikost je bl\u00EDzk\u00E1 hodnot\u011B 0, byla v 18."@cs ;
foaf:depiction .
@prefix skos: .
dbpedia:Vega skos:subject .
@prefix ns11: .
dbpedia:Vega skos:subject ns11:Lyra_constellation ,
ns11:Castor_Moving_Group ,
ns11:Northern_pole_stars ,
ns11:Flamsteed_objects ,
ns11:HR_objects ,
ns11:Bayer_objects ,
ns11:Delta_Scuti_variables ,
ns11:A-type_main_sequence_stars ,
ns11:Hypothetical_planetary_systems ,
ns11:Circumstellar_discs ,
ns11:HIP_objects ,
ns11:HD_and_HDE_objects ,
ns11:Stars_with_proper_names .
@prefix ns12: .
dbpedia:Vega dbpprop:wikiPageUsesTemplate ns12:dec ,
ns12:starbox_observe ,
ns12:starbox_detail ,
ns12:otheruses1 ,
ns12:starbox_image ,
ns12:starbox_character ,
ns12:ra ,
ns12:sky ;
dbpprop:mass 2.11 ;
dbpprop:age "3.86–5.72"@en .
@prefix ns13: .
dbpedia:Vega dbpprop:dec ns13:DEC ;
dbpprop:otheruses1Property "the star"@en ,
"Vega"@en ;
dbpprop:class "A0V"@en ;
dbpprop:epoch ;
dbpprop:raProperty 56.3364 ,
36 ,
6 ;
dbpprop:ra "—use the \"display all measurements\" option to show additional parameters."@en .
@prefix ns14: .
dbpedia:Vega dbpprop:ra ns14:RA ;
dbpprop:bV 0 ;
dbpprop:uB "\u22120.01"@en ;
dbpprop:luminosity "37 \u00B1 3"@en ;
dbpprop:metal "[M/H] = −0.5"@en ;
dbpprop:skyProperty 56.3364 ,
1.291 ,
"+"@en ,
25 ,
18 ,
47 ,
38 ,
36 .
@prefix ns15: .
dbpedia:Vega dbpprop:pronounce ns15:IPA-en1 ,
ns15:IPA-en ,
"or\n"@en .
@prefix ns16: .
dbpedia:Vega dbpprop:relatedInstance ns16:lang4 ,
ns16:lang5 ,
ns16:lang6 ,
ns16:lang1 ,
ns16:lang2 ,
ns16:lang3 ;
dbpprop:caption "Location of Vega in the constellation Lyra."@en ;
dbpprop:gravity "4.1 \u00B1 0.1"@en ;
dbpprop:temperature "9602 \u00B1 180"@en ;
dbpprop:decProperty 1.291 ,
"−38"@en ,
47 ;
dbpprop:appmagV 0.03 ;
dbpprop:rotation 12.5 ;
dbpprop:radius "2.26 \u00D7 2.78"@en ;
dbpprop:constell dbpedia:Lyra ;
dbpprop:variable dbpedia:Delta_Scuti_variable .
@prefix ns17: .
dbpedia:Vega dbpprop:hasPhotoCollection ns17:Vega .
dbpedia:Alpha_Lyra dbpprop:redirect dbpedia:Vega .
dbpedia:HIP_91262 dbpprop:redirect dbpedia:Vega .
dbpedia:SAO_67174 dbpprop:redirect dbpedia:Vega .
dbpedia:Alpha_Lyrae dbpprop:redirect dbpedia:Vega .
dbpprop:redirect dbpedia:Vega .
@prefix yago: .
yago:Vega owl:sameAs dbpedia:Vega .