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Subject Item
dbr:HD_56618
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HD 56618 HD 56618 HD 56618 HD 56618
rdfs:comment
HD 56618 è una stella gigante rossa di magnitudine 4,69 situata nella costellazione del Cane Maggiore. Dista 453 anni luce dal sistema solare. HD 56618 is a single star in the southern constellation of Canis Major. It is a red-hued star that is faintly visible to the naked eye with an apparent visual magnitude of 4.66. This object is located at a distance of approximately 390 light years from the Sun based on parallax measurements. It is drifting further away with a radial velocity of +41.5 km/s, having come to within 203 light-years some 2.2 million years ago. Olin J. Eggen listed it as a probable member of the Hyades supercluster. HD 56618，又名CD-27 3852，SAO 173360、HR 2766，是一颗恒星，视星等为4.64，位于銀經240.58，銀緯-7.3，其B1900.0坐标为赤經7h 12m 34.4s，赤緯-27° -7.3′ 16″。 HD 56618 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Stora hunden. Den har en skenbar magnitud av ca 4,66 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 8,3 mas, beräknas den befinna sig på ett avstånd på ca 390 ljusår (ca 120 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 42 km/s. Olin J. Eggen listade den som en trolig medlem av superhopen Hyaderna.
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dbp:absmagV
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dbo:abstract
HD 56618 è una stella gigante rossa di magnitudine 4,69 situata nella costellazione del Cane Maggiore. Dista 453 anni luce dal sistema solare. HD 56618 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Stora hunden. Den har en skenbar magnitud av ca 4,66 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 8,3 mas, beräknas den befinna sig på ett avstånd på ca 390 ljusår (ca 120 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 42 km/s. Olin J. Eggen listade den som en trolig medlem av superhopen Hyaderna. HD 56618，又名CD-27 3852，SAO 173360、HR 2766，是一颗恒星，视星等为4.64，位于銀經240.58，銀緯-7.3，其B1900.0坐标为赤經7h 12m 34.4s，赤緯-27° -7.3′ 16″。 HD 56618 is a single star in the southern constellation of Canis Major. It is a red-hued star that is faintly visible to the naked eye with an apparent visual magnitude of 4.66. This object is located at a distance of approximately 390 light years from the Sun based on parallax measurements. It is drifting further away with a radial velocity of +41.5 km/s, having come to within 203 light-years some 2.2 million years ago. Olin J. Eggen listed it as a probable member of the Hyades supercluster. This is an aging red giant star currently on the asymptotic giant branch with a stellar classification of M2III. It is not longer undergoing core hydrogen fusion and has expanded to 61 times the radius of the Sun. The star is radiating 700 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 3,797 K.
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