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36 Serpentis is a binary star system in the equatorial constellation of Serpens. It has the Bayer designation b Serpentis, while 36 Serpentis is the Flamsteed designation. The system is visible to the naked eye as a dim, white-hued point of light with a combined apparent visual magnitude of 5.09. It is located 162 light years away from the Sun based on parallax, and is moving closer with a radial velocity of −8 km/s. The cooler secondary component, a G0 star, is the source for the X-ray emission that has been detected coming from this system. It has a visual magnitude of 7.8.

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  • 36 Serpentis (en)
  • 36 Serpentis (pt)
  • 36 Serpentis (sv)
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  • 36 Serpentis (b Serpentis) é uma estrela na direção da Serpens. Possui uma ascensão reta de 15h 51m 15.65s e uma declinação de −03° 05′ 25.5″. Sua magnitude aparente é igual a 5.09. Considerando sua distância de 159 anos-luz em relação à Terra, sua magnitude absoluta é igual a 1.65. Pertence à classe espectral A3Vn. (pt)
  • 36 Serpentis, som är stjärnans Flamsteed-beteckning, är en dubbelstjärna i den södra delen av stjärnbilden Ormen, som också har Bayer-beteckningen b Serpentis. Den har en kombinerad skenbar magnitud på ca 5,09 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 20,1 mas, beräknas den befinna sig på ett avstånd på ca 162 ljusår (ca 50 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet av ca -8 km/s (sv)
  • 36 Serpentis is a binary star system in the equatorial constellation of Serpens. It has the Bayer designation b Serpentis, while 36 Serpentis is the Flamsteed designation. The system is visible to the naked eye as a dim, white-hued point of light with a combined apparent visual magnitude of 5.09. It is located 162 light years away from the Sun based on parallax, and is moving closer with a radial velocity of −8 km/s. The cooler secondary component, a G0 star, is the source for the X-ray emission that has been detected coming from this system. It has a visual magnitude of 7.8. (en)
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absmag v
age myr
appmag v
b-v
  • +0.12 (en)
class
  • (en)
  • A3Vn or A2IV-Vn (en)
component
constell
epoch
  • J2000.0 (en)
gravity
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