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Kappa Leporis, Latinized from κ Leporis, i … Kappa Leporis, Latinized from κ Leporis, is a binary star system in the southern constellation of Lepus. The pair have apparent visual magnitudes of 4.43 and 7.00, with the former being bright enough to be seen with the naked eye. As of 2000, they had an angular separation of 2.179 arc seconds along a position angle of 357.3°. Based upon an annual parallax shift of 4.48 mas as measured from Earth, the system is located roughly 730 light years from the Sun. The system is travelling away from the Sun with a radial velocity of +20.8 km/s. The brighter, blue-white hued member of the system, component A, is a B-type main-sequence star with a stellar classification of B9 V. It has nearly five times the mass of the Sun and around 2.6 times the Sun's radius. The star is radiating 1,346 times the Sun's luminosity from its photosphere at an effective temperature of 11,588 K. It displays an infrared excess at a wavelength of 12μm, making it a candidate host for a circumstellar debris disk.date host for a circumstellar debris disk.
, Kappa Leporis (κ Leporis, förkortat Kappa … Kappa Leporis (κ Leporis, förkortat Kappa Lep, κ Lep) som är stjärnans Bayerbeteckning, är en dubbelstjärna belägen i den nordvästra delen av stjärnbilden Haren. Den har en skenbar magnitud på 4,43 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 4,5 mas, beräknas den befinna sig på ett avstånd på ca 730 ljusår (ca 220 parsek) från solen. ca 730 ljusår (ca 220 parsek) från solen.
, Kappa Leporis (4 Leporis) é uma estrela na … Kappa Leporis (4 Leporis) é uma estrela na direção da constelação de Lepus. Possui uma ascensão reta de 05h 13m 13.89s e uma declinação de −12° 56′ 28.6″. Sua magnitude aparente é igual a 4.36. Considerando sua distância de 559 anos-luz em relação à Terra, sua magnitude absoluta é igual a −1.81. Pertence à classe espectral B7V. a −1.81. Pertence à classe espectral B7V.
, Kappa Leporis, du latin κ Leporis, est un … Kappa Leporis, du latin κ Leporis, est un système d'étoiles binaires situé à ~728 a.l. de la Terre dans la constellation du Lièvre. L'étoile primaire a une magnitude apparente de 4,43 et le secondaire, une magnitude de 7,00, la première étant suffisamment brillante pour être vue à l'œil nu.amment brillante pour être vue à l'œil nu.
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Kappa Leporis, Latinized from κ Leporis, i … Kappa Leporis, Latinized from κ Leporis, is a binary star system in the southern constellation of Lepus. The pair have apparent visual magnitudes of 4.43 and 7.00, with the former being bright enough to be seen with the naked eye. As of 2000, they had an angular separation of 2.179 arc seconds along a position angle of 357.3°. Based upon an annual parallax shift of 4.48 mas as measured from Earth, the system is located roughly 730 light years from the Sun. The system is travelling away from the Sun with a radial velocity of +20.8 km/s. Sun with a radial velocity of +20.8 km/s.
, Kappa Leporis (κ Leporis, förkortat Kappa … Kappa Leporis (κ Leporis, förkortat Kappa Lep, κ Lep) som är stjärnans Bayerbeteckning, är en dubbelstjärna belägen i den nordvästra delen av stjärnbilden Haren. Den har en skenbar magnitud på 4,43 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 4,5 mas, beräknas den befinna sig på ett avstånd på ca 730 ljusår (ca 220 parsek) från solen. ca 730 ljusår (ca 220 parsek) från solen.
, Kappa Leporis, du latin κ Leporis, est un … Kappa Leporis, du latin κ Leporis, est un système d'étoiles binaires situé à ~728 a.l. de la Terre dans la constellation du Lièvre. L'étoile primaire a une magnitude apparente de 4,43 et le secondaire, une magnitude de 7,00, la première étant suffisamment brillante pour être vue à l'œil nu.amment brillante pour être vue à l'œil nu.
, Kappa Leporis (4 Leporis) é uma estrela na … Kappa Leporis (4 Leporis) é uma estrela na direção da constelação de Lepus. Possui uma ascensão reta de 05h 13m 13.89s e uma declinação de −12° 56′ 28.6″. Sua magnitude aparente é igual a 4.36. Considerando sua distância de 559 anos-luz em relação à Terra, sua magnitude absoluta é igual a −1.81. Pertence à classe espectral B7V. a −1.81. Pertence à classe espectral B7V.
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Kappa Leporis
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