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HD 210434，又名BD-04 5625，SAO 145916、HR 8453，是一颗恒星，视星等为6.01，位于銀經56.51，銀緯-45.37，其B1900.0坐标为赤經22h 5m 20.9s，赤緯-4° -45.37′ 31″。
, HD 210434 är en ensam stjärna belägen i de … HD 210434 är en ensam stjärna belägen i den norra delen av stjärnbilden Vattumannen. Den har en skenbar magnitud av ca 5,98 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 9,8 mas, beräknas den befinna sig på ett avstånd på ca 330 ljusår (ca 102 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -18 km/s.iocentrisk radialhastighet på ca -18 km/s.
, HD 210434 è una stella di magnitudine 5,98 situata nella costellazione dell'Aquario. Dista 282 anni luce dal sistema solare.
, HD 210434 is a subgiant star in the equato … HD 210434 is a subgiant star in the equatorial constellation of Aquarius. According to the Bortle scale, an apparent magnitude of six means this star is faintly visible to the naked eye from dark rural skies. It is an estimated 630 million years old with 2.4 times the mass of the Sun.rs old with 2.4 times the mass of the Sun.
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| rdfs:comment |
HD 210434 is a subgiant star in the equato … HD 210434 is a subgiant star in the equatorial constellation of Aquarius. According to the Bortle scale, an apparent magnitude of six means this star is faintly visible to the naked eye from dark rural skies. It is an estimated 630 million years old with 2.4 times the mass of the Sun.rs old with 2.4 times the mass of the Sun.
, HD 210434 è una stella di magnitudine 5,98 situata nella costellazione dell'Aquario. Dista 282 anni luce dal sistema solare.
, HD 210434，又名BD-04 5625，SAO 145916、HR 8453，是一颗恒星，视星等为6.01，位于銀經56.51，銀緯-45.37，其B1900.0坐标为赤經22h 5m 20.9s，赤緯-4° -45.37′ 31″。
, HD 210434 är en ensam stjärna belägen i de … HD 210434 är en ensam stjärna belägen i den norra delen av stjärnbilden Vattumannen. Den har en skenbar magnitud av ca 5,98 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 9,8 mas, beräknas den befinna sig på ett avstånd på ca 330 ljusår (ca 102 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -18 km/s.iocentrisk radialhastighet på ca -18 km/s.
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HD 210434
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