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Lambda Leporis (λ Lep / 6 Leporis / HD 348 … Lambda Leporis (λ Lep / 6 Leporis / HD 34816 / HR 1756) es una estrella en la constelación de Lepus, la liebre, de magnitud aparente +4,27.De acuerdo con la nueva reducción de los datos de paralaje del satélite Hipparcos, se encuentra a 1150 años luz del Sistema Solar. Lambda Leporis es una subgigante blanco-azulada de tipo espectral B0.5IV.Muy caliente, tiene una temperatura superficial de 26.850 K y una luminosidad bolométrica —que incluye una importante cantidad de energía radiada como luz ultravioleta— 13.480 veces mayor que la luminosidad solar.Su radio es 4,5 ± 1,3 veces más grande que el del Sol y gira sobre sí misma con una velocidad de rotación proyectada de 25 km/s.Es una estrella similar a Becrux (β Crucis) o Dschubba (δ Scorpii), aunque está mucho más alejada que estas. Lambda Leporis posee una masa de 12,2 ± 0,3 masas solares.Tiene una edad estimada de 600.000 años, equivalente a 1/7700 parte de la edad de nuestro Sol; sin embargo, una estrella tan masiva vive una corta vida y, de hecho, Lambda Leporis está ya abandonando la secuencia principal. Su masa supera sobradamente el límite de por encima del cual las estrellas finalizan su vida estallando en forma de supernova. su vida estallando en forma de supernova.
, Lambda Leporis (6 Leporis) é uma estrela n … Lambda Leporis (6 Leporis) é uma estrela na direção da constelação de Lepus. Possui uma ascensão reta de 05h 19m 34.53s e uma declinação de −13° 10′ 36.4″. Sua magnitude aparente é igual a 4.29. Considerando sua distância de 1076 anos-luz em relação à Terra, sua magnitude absoluta é igual a −3.30. Pertence à classe espectral B0.5IV.−3.30. Pertence à classe espectral B0.5IV.
, Lambda Leporis (λ Leporis, förkortat Lambd … Lambda Leporis (λ Leporis, förkortat Lambda Lep, λ Lep) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den nordvästra delen av stjärnbilden Haren. Den har en skenbar magnitud på 4,29 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 3,8 mas, beräknas den befinna sig på ett avstånd på ca 850 ljusår (ca 260 parsek) från solen. ca 850 ljusår (ca 260 parsek) från solen.
, Lambda Leporis, which is the Latinized for … Lambda Leporis, which is the Latinized form of λ Leporis, is a solitary, blue-white hued star in the southern constellation of Lepus. It is visible to the naked eye with an apparent visual magnitude of +4.29. Based upon an annual parallax shift of 3.83 mas, it is estimated to lie roughly 850 light years from the Sun. Relative to its neighbors, this star has a peculiar velocity of 16.3±2.8 km/s. It is a member of the Orion OB1 association (Ori OB1), and it has been identified as a high-velocity runaway star. This is a massive, B-type main-sequence star with a corrected stellar classification of B0.5 V. It is an estimated eight million years old and is spinning with a projected rotational velocity of 30 km/s. This star has around 15 times the mass of the Sun and 4.5 times the Sun's radius. It is radiating 15,488 times the Sun's luminosity from its photosphere at an effective temperature of 30,400 K.e at an effective temperature of 30,400 K.
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rdfs:comment |
Lambda Leporis (λ Lep / 6 Leporis / HD 348 … Lambda Leporis (λ Lep / 6 Leporis / HD 34816 / HR 1756) es una estrella en la constelación de Lepus, la liebre, de magnitud aparente +4,27.De acuerdo con la nueva reducción de los datos de paralaje del satélite Hipparcos, se encuentra a 1150 años luz del Sistema Solar.uentra a 1150 años luz del Sistema Solar.
, Lambda Leporis (λ Leporis, förkortat Lambd … Lambda Leporis (λ Leporis, förkortat Lambda Lep, λ Lep) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den nordvästra delen av stjärnbilden Haren. Den har en skenbar magnitud på 4,29 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 3,8 mas, beräknas den befinna sig på ett avstånd på ca 850 ljusår (ca 260 parsek) från solen. ca 850 ljusår (ca 260 parsek) från solen.
, Lambda Leporis (6 Leporis) é uma estrela n … Lambda Leporis (6 Leporis) é uma estrela na direção da constelação de Lepus. Possui uma ascensão reta de 05h 19m 34.53s e uma declinação de −13° 10′ 36.4″. Sua magnitude aparente é igual a 4.29. Considerando sua distância de 1076 anos-luz em relação à Terra, sua magnitude absoluta é igual a −3.30. Pertence à classe espectral B0.5IV.−3.30. Pertence à classe espectral B0.5IV.
, Lambda Leporis, which is the Latinized for … Lambda Leporis, which is the Latinized form of λ Leporis, is a solitary, blue-white hued star in the southern constellation of Lepus. It is visible to the naked eye with an apparent visual magnitude of +4.29. Based upon an annual parallax shift of 3.83 mas, it is estimated to lie roughly 850 light years from the Sun. Relative to its neighbors, this star has a peculiar velocity of 16.3±2.8 km/s. It is a member of the Orion OB1 association (Ori OB1), and it has been identified as a high-velocity runaway star.dentified as a high-velocity runaway star.
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Lambda Leporis
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