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鳳凰座μ，又名CD-46 180，HD 3919、SAO 215194、HR 180，是鳳凰座的一颗恒星，视星等为4.59，位于銀經308.31，銀緯-70.94，其B1900.0坐标为赤經0h 36m 36s，赤緯-46° -70.94′ 2″。
, μ Phoenicis, Latinized as Mu Phoenicis, is … μ Phoenicis, Latinized as Mu Phoenicis, is a suspected astrometric binary star system in the southern constellation of Phoenix. It is visible to the naked eye as a faint, yellow-hued star with an apparent visual magnitude of 4.59. This system is located approximately 246 light years distant from the Sun based on parallax, and is drifting further away with a radial velocity of +17.4 km/s. The visible component is an aging G-type giant star with a stellar classification of G8III. Having exhausted the supply of hydrogen at its core, this star cooled and expanded off the main sequence. At present it has 13 times the girth of the Sun. It is 1.4 billion years old with 2.5 times the mass of the Sun. It is radiating 97 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,900 K.re at an effective temperature of 4,900 K.
, Mu Phoenicis (μ Phoenicis) é uma estrela n … Mu Phoenicis (μ Phoenicis) é uma estrela na constelação de Phoenix. Com uma magnitude aparente visual de 4,59, pode ser vista a olho nu em locais sem poluição luminosa excessiva. De acordo com sua paralaxe medida pela sonda Gaia, está a uma distância de aproximadamente 244 anos-luz (75 parsecs) da Terra. Esta estrela é classificada como uma gigante de classe G com um tipo espectral de G8III. No diagrama HR pertence à população do red clump, o que indica que está na fase evolucionária de queima de hélio no núcleo. A partir da média de diferentes modelos de evolução estelar, sua massa foi estimada em 2,5 vezes a massa solar e sua idade em 1,4 bilhões de anos. A estrela expandiu-se para um raio de 13 vezes o raio solar, e está irradiando energia de sua fotosfera com 87 vezes a luminosidade solar a uma temperatura efetiva de aproximadamente 5 000 K. A partir de uma diferença significativa entre seu movimento próprio nos catálogos Hipparcos e , esta estrela é considerada uma possível binária astrométrica, cujo movimento próprio varia devido a perturbações por uma estrela companheira. perturbações por uma estrela companheira.
, Mu Phoenicis adalah bintang kelas G8III yang berada di rasi Phoenix. Bintang ini berada pada jarak 247 tahun cahaya dari Bumi. Bintang ini bermagnitudo 4.59.
, My Phoenicis (μ Phoenicis, förkortat My Ph … My Phoenicis (μ Phoenicis, förkortat My Phe, μ Phe) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Fenix. Den har en skenbar magnitud på 4,59 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 13,3 mas, beräknas den befinna sig på ett avstånd på ca 246 ljusår (ca 75 parsek) från solen.å ca 246 ljusår (ca 75 parsek) från solen.
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My Phoenicis (μ Phoenicis, förkortat My Ph … My Phoenicis (μ Phoenicis, förkortat My Phe, μ Phe) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Fenix. Den har en skenbar magnitud på 4,59 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 13,3 mas, beräknas den befinna sig på ett avstånd på ca 246 ljusår (ca 75 parsek) från solen.å ca 246 ljusår (ca 75 parsek) från solen.
, Mu Phoenicis adalah bintang kelas G8III yang berada di rasi Phoenix. Bintang ini berada pada jarak 247 tahun cahaya dari Bumi. Bintang ini bermagnitudo 4.59.
, μ Phoenicis, Latinized as Mu Phoenicis, is … μ Phoenicis, Latinized as Mu Phoenicis, is a suspected astrometric binary star system in the southern constellation of Phoenix. It is visible to the naked eye as a faint, yellow-hued star with an apparent visual magnitude of 4.59. This system is located approximately 246 light years distant from the Sun based on parallax, and is drifting further away with a radial velocity of +17.4 km/s.away with a radial velocity of +17.4 km/s.
, 鳳凰座μ，又名CD-46 180，HD 3919、SAO 215194、HR 180，是鳳凰座的一颗恒星，视星等为4.59，位于銀經308.31，銀緯-70.94，其B1900.0坐标为赤經0h 36m 36s，赤緯-46° -70.94′ 2″。
, Mu Phoenicis (μ Phoenicis) é uma estrela n … Mu Phoenicis (μ Phoenicis) é uma estrela na constelação de Phoenix. Com uma magnitude aparente visual de 4,59, pode ser vista a olho nu em locais sem poluição luminosa excessiva. De acordo com sua paralaxe medida pela sonda Gaia, está a uma distância de aproximadamente 244 anos-luz (75 parsecs) da Terra. A partir de uma diferença significativa entre seu movimento próprio nos catálogos Hipparcos e , esta estrela é considerada uma possível binária astrométrica, cujo movimento próprio varia devido a perturbações por uma estrela companheira. perturbações por uma estrela companheira.
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My Phoenicis
, Mu Phoenicis
, 火鳥七
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