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175 Puppis (c Puppis) é uma estrela na dir … 175 Puppis (c Puppis) é uma estrela na direção da Puppis. Possui uma ascensão reta de 07h 45m 15.30s e uma declinação de −37° 58′ 07.0″. Sua magnitude aparente é igual a 3.62. Considerando sua distância de 1387 anos-luz em relação à Terra, sua magnitude absoluta é igual a −4.52. Pertence à classe espectral K4III. −4.52. Pertence à classe espectral K4III.
, c Puppis, also known as HD 63032 and HR 30 … c Puppis, also known as HD 63032 and HR 3017, is a spectroscopic binary star in the constellation Puppis. Its apparent magnitude is 3.61. Located around 347 parsecs (1,130 ly) distant, the primary is an orange-red bright giant or supergiant of spectral type K2.5Ib-IIa or K5IIa, while the secondary, discovered in 1983, is a blue main-sequence star of spectral type B9V. The system is the brightest member of the open cluster NGC 2451, over two magnitudes brighter than every other star in the cluster. As the turnoff point of the cluster is currently around B7, the parameters of the system fit with cluster membership.of the system fit with cluster membership.
, c Puppis(
Ne doit pas être confondu avec ( … c Puppis(
Ne doit pas être confondu avec (= HD 53704) ) Cet article est une ébauche concernant une étoile. Vous pouvez partager vos connaissances en l’améliorant (comment ?) selon les recommandations des projets correspondants. c PuppisHD 63032 C Puppis dans NGC 2451 Autres désignations c Pup, HD 63032, HIP 37819, HR 3017, CD-37 3863, CPD-37 1558, SAO 198398, NSV 3723 c Puppis, également désignée HD 63032 ou HR 3017, est une étoile binaire de la constellation de la Poupe. Sa magnitude apparente visuelle est de 3,62 et elle est distante d'environ ∼810 a.l. (∼248 pc) de la Terre. c Puppis se trouve sur le ciel entre Naos et Nu Puppis. Elle est située dans l'amas ouvert NGC 2451, dont elle est l'étoile la plus brillante de plus de deux magnitudes. Étant donné que le point de sortie de la séquence principale de l'amas est autour du type B7, les paramètres du système sont compatibles avec une appartenance à NGC 2451. c Puppis est un système binaire. Son étoile primaire est classée comme une géante lumineuse orange de type spectral K5IIa, tandis que son compagnon est une étoile bleu-blanc de la séquence principale de type B9V.anc de la séquence principale de type B9V.
, 弧矢三，即船尾座c（英語：c Puppis），又名CD-37 3863、SAO 198398和HR 3017，是一个位于船尾座的光学双星系统。其视星等为3.61，距太阳系347秒差距（1,130光年），双星中的前者为一颗橙红色亮巨星，恒星光谱为K2.5Ib-IIa或K5IIa，后者则在1983年才被发现，是一颗光谱为B9V的B型主序星。虽然后者已低于疏散星团的B7，但因前者过于明亮，故弧矢三仍是NGC 2451中最亮的恒星。
, HD 63032 är en dubbelstjärna belägen i den … HD 63032 är en dubbelstjärna belägen i den mellersta delen av stjärnbilden Akterskeppet, som också har Bayer-beteckningen c Puppis. Den har en skenbar magnitud av ca 3,61 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget enligt Gaia Data Release 2 på ca 2,9 mas, beräknas den befinna sig på ett avstånd på ca 1 110 ljusår (ca 340 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 17 km/s.liocentrisk radialhastighet på ca 17 km/s.
, HD 63032, nota anche come c Puppis, è una stella gigante brillante arancione di magnitudine 3,64 situata nella costellazione della Poppa. Dista 1388 anni luce dal sistema solare.
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c Puppis(
Ne doit pas être confondu avec ( … c Puppis(
Ne doit pas être confondu avec (= HD 53704) ) Cet article est une ébauche concernant une étoile. Vous pouvez partager vos connaissances en l’améliorant (comment ?) selon les recommandations des projets correspondants. c PuppisHD 63032 C Puppis dans NGC 2451 Autres désignations c Pup, HD 63032, HIP 37819, HR 3017, CD-37 3863, CPD-37 1558, SAO 198398, NSV 3723 c Puppis est un système binaire. Son étoile primaire est classée comme une géante lumineuse orange de type spectral K5IIa, tandis que son compagnon est une étoile bleu-blanc de la séquence principale de type B9V.anc de la séquence principale de type B9V.
, HD 63032, nota anche come c Puppis, è una stella gigante brillante arancione di magnitudine 3,64 situata nella costellazione della Poppa. Dista 1388 anni luce dal sistema solare.
, c Puppis, also known as HD 63032 and HR 30 … c Puppis, also known as HD 63032 and HR 3017, is a spectroscopic binary star in the constellation Puppis. Its apparent magnitude is 3.61. Located around 347 parsecs (1,130 ly) distant, the primary is an orange-red bright giant or supergiant of spectral type K2.5Ib-IIa or K5IIa, while the secondary, discovered in 1983, is a blue main-sequence star of spectral type B9V. The system is the brightest member of the open cluster NGC 2451, over two magnitudes brighter than every other star in the cluster. As the turnoff point of the cluster is currently around B7, the parameters of the system fit with cluster membership.of the system fit with cluster membership.
, 弧矢三，即船尾座c（英語：c Puppis），又名CD-37 3863、SAO 198398和HR 3017，是一个位于船尾座的光学双星系统。其视星等为3.61，距太阳系347秒差距（1,130光年），双星中的前者为一颗橙红色亮巨星，恒星光谱为K2.5Ib-IIa或K5IIa，后者则在1983年才被发现，是一颗光谱为B9V的B型主序星。虽然后者已低于疏散星团的B7，但因前者过于明亮，故弧矢三仍是NGC 2451中最亮的恒星。
, HD 63032 är en dubbelstjärna belägen i den … HD 63032 är en dubbelstjärna belägen i den mellersta delen av stjärnbilden Akterskeppet, som också har Bayer-beteckningen c Puppis. Den har en skenbar magnitud av ca 3,61 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget enligt Gaia Data Release 2 på ca 2,9 mas, beräknas den befinna sig på ett avstånd på ca 1 110 ljusår (ca 340 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 17 km/s.liocentrisk radialhastighet på ca 17 km/s.
, 175 Puppis (c Puppis) é uma estrela na dir … 175 Puppis (c Puppis) é uma estrela na direção da Puppis. Possui uma ascensão reta de 07h 45m 15.30s e uma declinação de −37° 58′ 07.0″. Sua magnitude aparente é igual a 3.62. Considerando sua distância de 1387 anos-luz em relação à Terra, sua magnitude absoluta é igual a −4.52. Pertence à classe espectral K4III. −4.52. Pertence à classe espectral K4III.
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HD 63032
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, 弧矢三
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