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HD 73468 (HR 3417) is a solitary star in the southern circumpolar constellation Volans. It is faintly visible to the naked eye with an apparent magnitude of 6.10, and is estimated to be 420 light years away based on parallax measurements. However, it is approaching the Solar System with a heliocentric radial velocity of −26.5 km/s.

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  • HD 73468 (en)
  • HD 73468 (sv)
  • HD 73468 (zh)
rdfs:comment
  • HD 73468 är en ensam stjärna i den södra delen av stjärnbilden Flygfisken. Den har en skenbar magnitud av ca 6,10 och är mycket svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 7,8 mas, beräknas den befinna sig på ett avstånd på ca 417 ljusår (ca 128 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -26 km/s. (sv)
  • HD 73468,又名CP-72 713,SAO 256524、HR 3417,是一颗恒星,视星等为6.12,位于銀經287.03,銀緯-19.14,其B1900.0坐标为赤經8h 33m 23s,赤緯-73° -19.14′ 50″。 (zh)
  • HD 73468 (HR 3417) is a solitary star in the southern circumpolar constellation Volans. It is faintly visible to the naked eye with an apparent magnitude of 6.10, and is estimated to be 420 light years away based on parallax measurements. However, it is approaching the Solar System with a heliocentric radial velocity of −26.5 km/s. (en)
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  • HD73468 (en)
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absmag v
  • +0.69 (en)
appmag v
b-v
  • +0.95 (en)
class
  • G8 III (en)
constell
epoch
  • J2000 (en)
gravity
luminosity
mass
metal fe
  • −0.09 (en)
p error
parallax
prop mo dec
  • +73.054 (en)
prop mo ra
  • −54.973 (en)
radial v
  • −26.5 (en)
radius
rotational velocity
temperature
type
u-b
  • +0.65 (en)
has abstract
  • HD 73468 (HR 3417) is a solitary star in the southern circumpolar constellation Volans. It is faintly visible to the naked eye with an apparent magnitude of 6.10, and is estimated to be 420 light years away based on parallax measurements. However, it is approaching the Solar System with a heliocentric radial velocity of −26.5 km/s. HD 73468 is a star with a classification of G8 III, indicating that it is a giant star. It is currently on the horizontal branch — generating energy via helium fusion in its core. HD 73468 has twice the mass of the Sun but has expanded to 10.24 times the radius of the Sun. It shines with a luminosity of 59 L☉ from its swollen photosphere at an effective temperature of 5,001 K, giving a yellow hue. HD 73468 is metal deficient with an iron abundance 81% that of the Sun and spins with a projected rotational velocity of about 2.1 km/s. (en)
  • HD 73468 är en ensam stjärna i den södra delen av stjärnbilden Flygfisken. Den har en skenbar magnitud av ca 6,10 och är mycket svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 7,8 mas, beräknas den befinna sig på ett avstånd på ca 417 ljusår (ca 128 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -26 km/s. (sv)
  • HD 73468,又名CP-72 713,SAO 256524、HR 3417,是一颗恒星,视星等为6.12,位于銀經287.03,銀緯-19.14,其B1900.0坐标为赤經8h 33m 23s,赤緯-73° -19.14′ 50″。 (zh)
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