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23 Андромеды (лат. 23 Andromedae, HD 905) … 23 Андромеды (лат. 23 Andromedae, HD 905) — предположительно одиночная звезда в созвездии Андромеды на расстоянии приблизительно 122 световых лет (около 37 парсеков) от Солнца. Видимая звёздная величина звезды — +5,71m. Возраст звезды определён как около 759 млн лет.ст звезды определён как около 759 млн лет.
, 23 Andromedae, abbreviated 23 And, is a pr … 23 Andromedae, abbreviated 23 And, is a presumed single star in the constellation Andromeda, although it has been a suspected spectroscopic binary. 23 Andromedae is the Flamsteed designation. Its apparent visual magnitude is 5.71, which indicates it is dimly visible to the naked eye under good viewing conditions. The distance to 23 And, as determined from its annual parallax shift of 26.8 mas, is 121.6 light years. The star is moving further from the Earth with a heliocentric radial velocity of −27 km/s. It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.191″ per year. The stellar classification of 23 And is F0 IV, matching an F-type subgiant star that is in the process of evolving into a red giant. It displays a slight microvariability with a frequency of 0.85784 d−1 and an amplitude of 0.0062 magnitude. The star is around 759 million years old with a projected rotational velocity of 36 km/s. It has 1.43 times the mass of the Sun and is radiating 50 times the Sun's luminosity from its photosphere at an effective temperature of 7,089 K.re at an effective temperature of 7,089 K.
, 23 Andromedae (23 And), som är stjärnans F … 23 Andromedae (23 And), som är stjärnans Flamsteedbeteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Andromeda, men har varit misstänkt att vara en spektroskopisk dubbelstjärna. Den har en skenbar magnitud på ca 5,71 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 26,8 mas, beräknas den befinna sig på ett avstånd på ca 122 ljusår (ca 37 parsek) från solen. Stjärnan rör sig närmare solen med en heliocentrisk radiell hastighet av –27 km/s. Den har en relativt stor egenrörelse och förflyttar sig över himlavalvet med hastigheten 0,191 bågsekunder per år. med hastigheten 0,191 bågsekunder per år.
, 仙女座23，又名BD+40 29，HD 905、SAO 36173、HR 41，是仙女座的一颗恒星，视星等为5.72，位于銀經115.27，銀緯-21.27，其B1900.0坐标为赤經0h 8m 19s，赤緯+40° -21.27′ 0″。
, 23 d'Andròmeda (23 Andromedae) és una estrella de la constel·lació d'Andròmeda. Té una magnitud aparent de 5,71 i una massa d'1,43 masses solars.
, 23 Andromedae è una stella nana bianco-gialla nella sequenza principale di magnitudine 5,72 situata nella costellazione di Andromeda. Dista 114 anni luce dal sistema solare.
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23 Andromedae (23 And), som är stjärnans F … 23 Andromedae (23 And), som är stjärnans Flamsteedbeteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Andromeda, men har varit misstänkt att vara en spektroskopisk dubbelstjärna. Den har en skenbar magnitud på ca 5,71 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 26,8 mas, beräknas den befinna sig på ett avstånd på ca 122 ljusår (ca 37 parsek) från solen. Stjärnan rör sig närmare solen med en heliocentrisk radiell hastighet av –27 km/s. Den har en relativt stor egenrörelse och förflyttar sig över himlavalvet med hastigheten 0,191 bågsekunder per år. med hastigheten 0,191 bågsekunder per år.
, 23 Andromedae è una stella nana bianco-gialla nella sequenza principale di magnitudine 5,72 situata nella costellazione di Andromeda. Dista 114 anni luce dal sistema solare.
, 23 Андромеды (лат. 23 Andromedae, HD 905) … 23 Андромеды (лат. 23 Andromedae, HD 905) — предположительно одиночная звезда в созвездии Андромеды на расстоянии приблизительно 122 световых лет (около 37 парсеков) от Солнца. Видимая звёздная величина звезды — +5,71m. Возраст звезды определён как около 759 млн лет.ст звезды определён как около 759 млн лет.
, 23 d'Andròmeda (23 Andromedae) és una estrella de la constel·lació d'Andròmeda. Té una magnitud aparent de 5,71 i una massa d'1,43 masses solars.
, 23 Andromedae, abbreviated 23 And, is a pr … 23 Andromedae, abbreviated 23 And, is a presumed single star in the constellation Andromeda, although it has been a suspected spectroscopic binary. 23 Andromedae is the Flamsteed designation. Its apparent visual magnitude is 5.71, which indicates it is dimly visible to the naked eye under good viewing conditions. The distance to 23 And, as determined from its annual parallax shift of 26.8 mas, is 121.6 light years. The star is moving further from the Earth with a heliocentric radial velocity of −27 km/s. It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.191″ per year.ial sphere at the rate of 0.191″ per year.
, 仙女座23，又名BD+40 29，HD 905、SAO 36173、HR 41，是仙女座的一颗恒星，视星等为5.72，位于銀經115.27，銀緯-21.27，其B1900.0坐标为赤經0h 8m 19s，赤緯+40° -21.27′ 0″。
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23 d'Andròmeda
, 23 Andromedae
, 23 Андромеды
, 天廄增一
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