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- Q1196515 subject Q7009834.
- Q1196515 subject Q7465903.
- Q1196515 subject Q8293947.
- Q1196515 subject Q8569496.
- Q1196515 subject Q8569500.
- Q1196515 abstract "Beta Arae (β Ara, β Arae) is the brightest star in the constellation Ara, with an apparent visual magnitude of 2.8. Parallax measurements place it at a distance of roughly 650 light-years (200 parsecs) from Earth.The spectrum of this star matches a stellar classification of K3 Ib-IIa, with the luminosity class notation 'Ib-IIa' indicating that the star lies part way between a higher luminosity bright giant (IIa) and a lower luminosity supergiant (Ib). This represents two of the evolutionary stages that a massive star passes through after it has exhausted the hydrogen at its core. Beta Arae is radiating energy from its outer envelope at an effective temperature of 4,582 K, which causes it to take on the orange hue of a K-type star. This enlarged star appears to be rotating slowly with a projected rotational velocity of about 5 km s−1. The abundance of elements other than hydrogen and helium, what astronomer term the star's metallicity, is more than three times the abundance in the Sun.Rarely, this star is called by the name Vasat-ül-cemre in Turkish spelling, derived from Arabic word ﻭﺳﻂ (wasath) and ﺟﻤﻩﺮ (khamra), meaning "middle of fire".REDIRECT Template:Unreliable source?This is a redirect from a page that has been moved (renamed). This page was kept as a redirect to avoid breaking links, both internal and external, that may have been made to the old page name. For more information follow the bold category link. In Chinese, 杵 (Chǔ), meaning Pestle, refers to an asterism consisting of β Arae, σ Arae and α Arae. Consequently, β Arae itself is known as 杵三 (Chǔ sān, English: the Third Star of Pestle.)↑ 1.0 1.1 1.2 1.3 1.4 1.5 ↑ 2.0 2.1 ↑ 3.0 3.1 3.2 3.3 3.4 3.5 ↑ 4.0 4.1 ↑ 5.0 5.1 ↑ 6.0 6.1 6.2 6.3 ↑ ↑ ↑ ↑ ↑ ↑".
- Q1196515 thumbnail Ara_IAU.svg?width=300.
- Q1196515 wikiPageExternalLink betaara.html.
- Q1196515 wikiPageExternalLink AladinPreview?-c=17+25+17.9887-55+31+47.583&ident=*+bet+Ara&submit=Aladin+previewer.
- Q1196515 wikiPageExternalLink VizieR-S?HR%206461.
- Q1196515 wikiPageWikiLink Q1054200.
- Q1196515 wikiPageWikiLink Q111130.
- Q1196515 wikiPageWikiLink Q1145781.
- Q1196515 wikiPageWikiLink Q124313.
- Q1196515 wikiPageWikiLink Q13955.
- Q1196515 wikiPageWikiLink Q165074.
- Q1196515 wikiPageWikiLink Q179600.
- Q1196515 wikiPageWikiLink Q193599.
- Q1196515 wikiPageWikiLink Q2.
- Q1196515 wikiPageWikiLink Q2074757.
- Q1196515 wikiPageWikiLink Q2143996.
- Q1196515 wikiPageWikiLink Q217030.
- Q1196515 wikiPageWikiLink Q2545970.
- Q1196515 wikiPageWikiLink Q256.
- Q1196515 wikiPageWikiLink Q499138.
- Q1196515 wikiPageWikiLink Q555846.
- Q1196515 wikiPageWikiLink Q5881.
- Q1196515 wikiPageWikiLink Q6464.
- Q1196515 wikiPageWikiLink Q6472.
- Q1196515 wikiPageWikiLink Q654182.
- Q1196515 wikiPageWikiLink Q7009834.
- Q1196515 wikiPageWikiLink Q7465903.
- Q1196515 wikiPageWikiLink Q7850.
- Q1196515 wikiPageWikiLink Q8293947.
- Q1196515 wikiPageWikiLink Q845735.
- Q1196515 wikiPageWikiLink Q854050.
- Q1196515 wikiPageWikiLink Q8569496.
- Q1196515 wikiPageWikiLink Q8569500.
- Q1196515 wikiPageWikiLink Q8928.
- Q1196515 wikiPageWikiLink Q9253.
- Q1196515 wikiPageWikiLink Q984158.
- Q1196515 type Place.
- Q1196515 type CelestialBody.
- Q1196515 type Location.
- Q1196515 type Place.
- Q1196515 type Star.
- Q1196515 type Thing.
- Q1196515 comment "Beta Arae (β Ara, β Arae) is the brightest star in the constellation Ara, with an apparent visual magnitude of 2.8. Parallax measurements place it at a distance of roughly 650 light-years (200 parsecs) from Earth.The spectrum of this star matches a stellar classification of K3 Ib-IIa, with the luminosity class notation 'Ib-IIa' indicating that the star lies part way between a higher luminosity bright giant (IIa) and a lower luminosity supergiant (Ib).".
- Q1196515 label "Beta Arae".
- Q1196515 depiction Ara_IAU.svg.
- Q1196515 name "Beta Arae".