HD 102350 is a single star in the constellation Centaurus. It has a yellow hue and is visible to the naked eye with an apparent visual magnitude of 4.11. The distance to this star is approximately 390 light years based on parallax, but it is drifting closer with a radial velocity of −3 km/s. It has an absolute magnitude of −1.51. HD 102350 is listed in the Washington Double Star Catalog as having a 13th magnitude companion about 25″ away, but it is a distant background object unrelated to HD 102350.
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| - إتش دي 102350 (ar)
- HD 102350 (fr)
- HD 102350 (en)
- HD 102350 (pt)
- HD 102350 (sv)
- HD 102350 (zh)
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| - إتش دي 102350 (بالإنجليزية: HD 102350) هو نجم واحد في كوكبة قنطورس. لونه أصفر ويمكن رؤيته بالعين المجردة بقدر ظاهري واضح يبلغ 4.11. تبلغ المسافة إلى هذا النجم حوالي 390 سنة ضوئية بناءً على اختلاف المنظر، لكنه ينجرف أقرب بسرعة شعاعية تبلغ 3 كم/ثانية. و قدره المطلق −1.51. (ar)
- HD 102350, également désignée HR 4522, est une étoile de la constellation australe du Centaure. Elle est visible à l'œil nu et sa magnitude apparente est de 4,11. Il s'agit d'une étoile géante lumineuse ou supergéante jaune distante d'environ 390 années-lumière de la Terre. (fr)
- HD 102350 är en ensam stjärna belägen i den södra delen av stjärnbilden Kentauren. Den har en skenbar magnitud av ca 4,11 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 8,4 mas, beräknas den befinna sig på ett avstånd på ca 390 ljusår (ca 119 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca –3,5 km/s. (sv)
- HD 102350，又名CP-60 3325，SAO 251579、HR 4522，是一颗恒星，视星等为4.11，位于銀經295.19，銀緯0.71，其B1900.0坐标为赤經11h 41m 40.4s，赤緯-60° 0.71′ 21″。 (zh)
- HD 102350 is a single star in the constellation Centaurus. It has a yellow hue and is visible to the naked eye with an apparent visual magnitude of 4.11. The distance to this star is approximately 390 light years based on parallax, but it is drifting closer with a radial velocity of −3 km/s. It has an absolute magnitude of −1.51. HD 102350 is listed in the Washington Double Star Catalog as having a 13th magnitude companion about 25″ away, but it is a distant background object unrelated to HD 102350. (en)
- HD 102350 é uma estrela na constelação de Centaurus. Tem uma magnitude aparente visual de 4,09, sendo visível a olho nu em locais sem muita poluição luminosa. Com base em medições de paralaxe pelo satélite Hipparcos, está localizada a uma distância de 390 anos-luz (119 parsecs) da Terra. É um dos sistemas observados pela sonda Hipparcos com a menor variação de magnitude, com amplitude não maior que 0,01, e é listada como uma estrela não variável, apesar de classificações anteriores sugerirem que seja uma variável Cefeida. (pt)
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| - إتش دي 102350 (بالإنجليزية: HD 102350) هو نجم واحد في كوكبة قنطورس. لونه أصفر ويمكن رؤيته بالعين المجردة بقدر ظاهري واضح يبلغ 4.11. تبلغ المسافة إلى هذا النجم حوالي 390 سنة ضوئية بناءً على اختلاف المنظر، لكنه ينجرف أقرب بسرعة شعاعية تبلغ 3 كم/ثانية. و قدره المطلق −1.51. (ar)
- HD 102350 is a single star in the constellation Centaurus. It has a yellow hue and is visible to the naked eye with an apparent visual magnitude of 4.11. The distance to this star is approximately 390 light years based on parallax, but it is drifting closer with a radial velocity of −3 km/s. It has an absolute magnitude of −1.51. This is an aging bright giant star with a stellar classification of G0II. It is a candidate Cepheid variable, but Hipparcos photometry found its brightness to be constant. The star has expanded to 22 times the radius of the Sun and is radiating 283 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 5,051 K. It has a magnitude 13.0 visual companion at an angular separation of 24.3″ along a position angle of 313° relative to the brighter component, as of 2000. HD 102350 is listed in the Washington Double Star Catalog as having a 13th magnitude companion about 25″ away, but it is a distant background object unrelated to HD 102350. (en)
- HD 102350, également désignée HR 4522, est une étoile de la constellation australe du Centaure. Elle est visible à l'œil nu et sa magnitude apparente est de 4,11. Il s'agit d'une étoile géante lumineuse ou supergéante jaune distante d'environ 390 années-lumière de la Terre. (fr)
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