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Chi Andromedae Chi Andromedae Khi d'Andròmeda Chi Andromedae 天大將軍五 Chi Andromedae 안드로메다자리 키 Chi Andromedae Chi Andromedae Хи Андромеды Chi Andromedae
rdfs:comment
χ Andromedae (Chi Andromedae, kurz χ And) ist ein mit dem bloßen Auge gerade noch wahrnehmbarer Stern im nördlichen Sternbild Andromeda. Seine scheinbare Helligkeit beträgt 5,01m. Nach Parallaxen-Messungen der Raumsonde Gaia ist er etwa 264 Lichtjahre von der Erde entfernt. 仙女座χ，又名BD+43 343，HD 10072、SAO 37406、HR 469，是仙女座的一颗恒星，视星等为4.98，位于銀經131.89，銀緯-17.65，其B1900.0坐标为赤經1h 33m 20.9s，赤緯+43° -17.65′ 39″。 Chi Andromedae (χ Andromedae, χ And) is the Bayer designation for a star in the northern constellation of Andromeda. It has an apparent visual magnitude of +5.01, which is relatively faint for a naked-eye star. Based upon parallax measurements made during the Gaia mission, Chi Andromedae is located around 264 light-years (81 parsecs) from Earth. Хи Андромеды (лат. χ Andromedae), 52 Андромеды (лат. 52 Andromedae), HD 10072 — двойная звезда в созвездии Андромеды на расстоянии приблизительно 257 световых лет (около 79 парсеков) от Солнца. Видимая звёздная величина звезды — +5,008. Орбитальный период — около 7581 суток (20,756 лет). 안드로메다자리 키(χ Andromedae / χ And)는 안드로메다자리의 항성이다. 황색 G형 거성으로 겉보기 등급은 +5.01 등급이다. 지구에서 242 광년 떨어져 있다. Chi Andromedae (χ Andromedae / χ And) est une étoile binaire de la constellation boréale d'Andromède. Elle est visible à l'œil nu et sa magnitude apparente combinée est de 5,01. D'après les mesures de sa parallaxe annuelle réalisées par le satellite Gaia, le système est distant d'environ ∼264 a.l. (∼80,9 pc) de la Terre. Il s'éloigne du Système solaire à une vitesse radiale héliocentrique de +7 km/s. Chi Andromedae (52 Andromedae) é uma estrela na direção da constelação de Andromeda. Possui uma ascensão reta de 01h 39m 21.02s e uma declinação de +44° 23′ 10.1″. Sua magnitude aparente é igual a 5.01. Considerando sua distância de 242 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.66. Pertence à classe espectral G8III.... Chi Andromedae (χ Andromedae / χ And) adalah salah satu bintand di rasi Andromeda. Bintang ini bermagnitudo 5.01 dan berada pada jarak 242 tahun cahaya. Bintang ini merupakan bintang raksasa kuning tipe G. Chi Andromedae (χ And / χ Andromedae) è una stella gigante gialla di magnitudine 5,02 situata nella costellazione di Andromeda. Dista 242 anni luce dal sistema solare. Khi d'Andròmeda (χ Andromedae) és una estrella de la constel·lació d'Andròmeda. És coneguda també amb el nom tradicional de Keun Nan Mun, que comparteix amb φ Andromedae. Aquest nom deriva de la frase en mandarí 軍南門 jūnnánmén, que significa "la porta sud del camp". Khi d'Andròmeda és una gegant groga del tipus G de la magnitud aparent +5,01. Està aproximadament a 242 anys llum de la Terra. Chi Andromedae (Chi And, χ Andromedae, χ And), som är stjärnans Bayerbeteckning, är en dubbelstjärna belägen i östra delen av stjärnbilden Andromeda. Den har en skenbar magnitud på ungefär +5,2, vilket är relativt svagt för att kunna ses med blotta ögat. Baserat på parallaxmätningar gjorda under Hipparcosuppdraget befinner den sig på ett avstånd av ca 250 ljusår (77 parsek) från solen.
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dbo:abstract
Chi Andromedae (χ Andromedae / χ And) adalah salah satu bintand di rasi Andromeda. Bintang ini bermagnitudo 5.01 dan berada pada jarak 242 tahun cahaya. Bintang ini merupakan bintang raksasa kuning tipe G. 안드로메다자리 키(χ Andromedae / χ And)는 안드로메다자리의 항성이다. 황색 G형 거성으로 겉보기 등급은 +5.01 등급이다. 지구에서 242 광년 떨어져 있다. Chi Andromedae (χ Andromedae, χ And) is the Bayer designation for a star in the northern constellation of Andromeda. It has an apparent visual magnitude of +5.01, which is relatively faint for a naked-eye star. Based upon parallax measurements made during the Gaia mission, Chi Andromedae is located around 264 light-years (81 parsecs) from Earth. χ Andromedae is a member of 天大將軍 (Tiān Dà Jiāng Jūn), meaning Heaven's Great General, together with γ Andromedae, φ Persei, 51 Andromedae, 49 Andromedae, θ Andromedae, τ Andromedae, 56 Andromedae, β Trianguli, γ Trianguli and δ Trianguli. Consequently, the Chinese name for χ Andromedae itself is 天大將軍五 (Tiān Dà Jiāng Jūn wǔ, English: the Fifth Star of Heaven's Great General.) This is most likely a spectroscopic binary system with an estimated orbital period of 20.8 years and an eccentricity of 0.37. The primary component has a stellar classification of G8 III, which indicates it is a giant star that has exhausted the supply of hydrogen at its core and evolved away from the main sequence. The outer envelope has expanded to about nine times the radius of the Sun and it is radiating 47 times the luminosity of the Sun at an effective temperature of 5,070 K. This heat gives the star the yellow-hued glow of a G-type star. It appears to be rotating very slowly with no measurable projected rotational velocity. The secondary component seems to be a main-sequence star of the spectral class G or K. χ Andromedae (Chi Andromedae, kurz χ And) ist ein mit dem bloßen Auge gerade noch wahrnehmbarer Stern im nördlichen Sternbild Andromeda. Seine scheinbare Helligkeit beträgt 5,01m. Nach Parallaxen-Messungen der Raumsonde Gaia ist er etwa 264 Lichtjahre von der Erde entfernt. Höchstwahrscheinlich ist χ And ein spektroskopischer Doppelstern. Dies war bereits 1926 von J. H. Moore vermutet worden. Der Begleiter umkreist die Hauptkomponente mit einer Umlaufszeit von etwa 20,8 Jahren auf einem mäßig elliptischen Orbit, dessen Exzentrizität 0,37 beträgt. Der Hauptstern gehört der Spektralklasse G8 III an. Er hat also bereits den Wasserstoff-Vorrat in seinem Inneren mittels Kernfusion zu Helium verbrannt und sich von der Hauptreihe weg zu einem gelb leuchtenden Riesenstern entwickelt. Nach einer Studie der Forschergruppe um Alessandro Massarotti et al. besitzt der Hauptstern rund 9 Sonnendurchmesser und 47 Sonnenleuchtkräfte. Kalkulationen aus Gaias Messdaten ergeben für ihn etwa 2,8 Sonnenmassen, 10,3 Sonnendurchmesser sowie 68 Sonnenleuchtkräfte. Die effektive Temperatur seiner äußeren Atmosphäre beträgt ungefähr 5070 Kelvin und ist somit etwas niedriger als jene der Sonne. Er dreht sich relativ langsam mit einer projizierten Rotationsgeschwindigkeit von etwa 17 km/s um seine eigene Achse. Sein Begleiter ist vermutlich ein Hauptreihenstern der Spektralklasse G oder K. Хи Андромеды (лат. χ Andromedae), 52 Андромеды (лат. 52 Andromedae), HD 10072 — двойная звезда в созвездии Андромеды на расстоянии приблизительно 257 световых лет (около 79 парсеков) от Солнца. Видимая звёздная величина звезды — +5,008. Орбитальный период — около 7581 суток (20,756 лет). Chi Andromedae (52 Andromedae) é uma estrela na direção da constelação de Andromeda. Possui uma ascensão reta de 01h 39m 21.02s e uma declinação de +44° 23′ 10.1″. Sua magnitude aparente é igual a 5.01. Considerando sua distância de 242 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.66. Pertence à classe espectral G8III.... 仙女座χ，又名BD+43 343，HD 10072、SAO 37406、HR 469，是仙女座的一颗恒星，视星等为4.98，位于銀經131.89，銀緯-17.65，其B1900.0坐标为赤經1h 33m 20.9s，赤緯+43° -17.65′ 39″。 Chi Andromedae (χ And / χ Andromedae) è una stella gigante gialla di magnitudine 5,02 situata nella costellazione di Andromeda. Dista 242 anni luce dal sistema solare. Chi Andromedae (Chi And, χ Andromedae, χ And), som är stjärnans Bayerbeteckning, är en dubbelstjärna belägen i östra delen av stjärnbilden Andromeda. Den har en skenbar magnitud på ungefär +5,2, vilket är relativt svagt för att kunna ses med blotta ögat. Baserat på parallaxmätningar gjorda under Hipparcosuppdraget befinner den sig på ett avstånd av ca 250 ljusår (77 parsek) från solen. Chi Andromedae (χ Andromedae / χ And) est une étoile binaire de la constellation boréale d'Andromède. Elle est visible à l'œil nu et sa magnitude apparente combinée est de 5,01. D'après les mesures de sa parallaxe annuelle réalisées par le satellite Gaia, le système est distant d'environ ∼264 a.l. (∼80,9 pc) de la Terre. Il s'éloigne du Système solaire à une vitesse radiale héliocentrique de +7 km/s. Khi d'Andròmeda (χ Andromedae) és una estrella de la constel·lació d'Andròmeda. És coneguda també amb el nom tradicional de Keun Nan Mun, que comparteix amb φ Andromedae. Aquest nom deriva de la frase en mandarí 軍南門 jūnnánmén, que significa "la porta sud del camp". Khi d'Andròmeda és una gegant groga del tipus G de la magnitud aparent +5,01. Està aproximadament a 242 anys llum de la Terra.
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