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・ Beta Herculis
・ Beta Hi Chahiye
・ Beta Ho To Aisa
・ Beta Horologii
・ Beta Hydrae
・ Beta Hydri
・ Beta hydroxy acid
・ Beta Indi
・ Beta integral
・ Beta Island
・ Beta Island, Bermuda
・ Beta Israel
・ Beta Kappa Chi
・ Beta Lacertae
・ Beta Leonis Minoris
Beta Leporis
・ Beta Librae
・ Beta Love
・ Beta Lupi
・ Beta Lyrae
・ Beta Lyrae variable
・ Beta Mensae
・ Beta Microscopii
・ Beta Monkey Music
・ Beta Monocerotis
・ Beta motor neuron
・ Beta movement
・ Beta Mu Sigma
・ Beta Muscae
・ Beta negative binomial distribution


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Beta Leporis : ウィキペディア英語版
Beta Leporis


Beta Leporis (Beta Lep, β Leporis, β Lep) is the second brightest star in the constellation of Lepus.〔 It is also known as Nihal,"quenching their thirst". The occasional spelling ''Nibal'' appears to be due to a misreading.〔
Based on parallax measurements from the Hipparcos astrometry satellite,〔 this star is located about from the Earth. It has an apparent visual magnitude of 2.84 and a stellar classification of G5 II. The mass of this star is 3.5 times the mass of the Sun and it is about 240 million years old,〔 which is sufficient time for a star this massive to consume the hydrogen at its core and evolve away from the main sequence, becoming a G-type bright giant.〔
This is a double star system and may be a binary. Using adaptive optics on the AEOS telescope at Haleakala Observatory, the pair was found to be separated by an angle of 2.58 arcseconds at a position angle of 1.4°.〔 Component B has been observed to fluctuate in brightness and is catalogued as suspected variable star NSV 2008.

==References==




抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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