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1 Aurigae is the original name for a star … 1 Aurigae is the original name for a star now in the constellation Perseus. It was the first entry in John Flamsteed's catalogue of stars in Auriga. When Eugène Joseph Delporte drew up simplified boundaries for the constellations on behalf of the International Astronomical Union in 1930, 1 Aurigae ended up over the border in Perseus. To avoid confusion, the star may instead be referred to by its Harvard Revised catalogue number, HR 1533. Based upon its parallax measurement of 6.48 mas, this star is located approximately 520 light years from Earth. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.89. 1 Aurigae is moving closer to the Earth with a heliocentric radial velocity of −25 km/s. This is a possible binary star system, based upon the status of the visible component as a mild barium star. The primary is an aging giant star with a stellar classification of K3.5 III Ba0.2:. It is 3.9 billion years old with 1.49 times the mass of the Sun and around 44 times the Sun's radius. This star is radiating 561 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,102 K. The suspected companion star should be a white dwarf that previously transferred s-process elements to the visible member. s-process elements to the visible member.
, 五车增七，即御夫座1（1 Aur， 1 Aurigae），是一个位于英仙座的分光双星系统，距离地球520光年。 它是一颗K-型巨星，视星等为4.88。 虽然五车增七的佛氏命名是御夫座1，但它实际是位于英仙座靠近御夫座的边界处。
, 1 Aurigae, som är stjärnans Flamsteed-bete … 1 Aurigae, som är stjärnans Flamsteed-beteckning, är en ensam stjärna belägen i den västra delen av stjärnbilden, Perseus. Den engelske astronomen John Flamsteed katalogiserade stjärnan som tillhörig Kuskens stjärnbild (latin Auriga) i sin sammanställning av Flamsteedobjekt. När gränserna för stjärnbilderna preciserades på 1930-talet hamnade 1 Aurigae inom Perseus stjärnbild. Stjärnan anges därför ofta numera med sin HR-beteckning, som är HR 1533. Den har en skenbar magnitud på ca 4,89 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 6,5 mas, beräknas den befinna sig på ett avstånd på ca 500 ljusår (ca 150 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet av ca -25 km/s.iocentrisk radialhastighet av ca -25 km/s.
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五车增七，即御夫座1（1 Aur， 1 Aurigae），是一个位于英仙座的分光双星系统，距离地球520光年。 它是一颗K-型巨星，视星等为4.88。 虽然五车增七的佛氏命名是御夫座1，但它实际是位于英仙座靠近御夫座的边界处。
, 1 Aurigae, som är stjärnans Flamsteed-bete … 1 Aurigae, som är stjärnans Flamsteed-beteckning, är en ensam stjärna belägen i den västra delen av stjärnbilden, Perseus. Den engelske astronomen John Flamsteed katalogiserade stjärnan som tillhörig Kuskens stjärnbild (latin Auriga) i sin sammanställning av Flamsteedobjekt. När gränserna för stjärnbilderna preciserades på 1930-talet hamnade 1 Aurigae inom Perseus stjärnbild. Stjärnan anges därför ofta numera med sin HR-beteckning, som är HR 1533. Den har en skenbar magnitud på ca 4,89 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 6,5 mas, beräknas den befinna sig på ett avstånd på ca 500 ljusår (ca 150 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet av ca -25 km/s.iocentrisk radialhastighet av ca -25 km/s.
, 1 Aurigae is the original name for a star … 1 Aurigae is the original name for a star now in the constellation Perseus. It was the first entry in John Flamsteed's catalogue of stars in Auriga. When Eugène Joseph Delporte drew up simplified boundaries for the constellations on behalf of the International Astronomical Union in 1930, 1 Aurigae ended up over the border in Perseus. To avoid confusion, the star may instead be referred to by its Harvard Revised catalogue number, HR 1533.Harvard Revised catalogue number, HR 1533.
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五车增七
, 1 Aurigae
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