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・ Kappa Leonis
・ Kappa Leporis
・ Kappa Librae
・ Kappa Lyrae
・ Kappa Matsuri
・ Kappa mechanism
・ Kappa Mikey
・ Kappa Mu Epsilon
・ Kappa no Kaikata
・ Kappa Normae
・ Kappa number
・ Kappa Omicron Nu
・ Kappa Ophiuchi
・ Kappa organism
・ Kappa Pavonis
Kappa Pegasi
・ Kappa Persei
・ Kappa Phi
・ Kappa Phi Gamma
・ Kappa Phi Lambda
・ Kappa Phi Lambda (fraternity)
・ Kappa Phoenicis
・ Kappa Pi
・ Kappa Pictoris
・ Kappa Piscium
・ Kappa Psi
・ Kappa Psi Kappa
・ Kappa Publishing Group
・ Kappa Pyxidis
・ Kappa Reticuli


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Kappa Pegasi : ウィキペディア英語版
Kappa Pegasi


Kappa Pegasi is a triple star system in the constellation Pegasus. It has an apparent brightness of +4.13 magnitude and belongs to the spectral class F5IV; a subgiant star.
This system consists of two components, designated Kappa Pegasi A and B, that are separated by an angular distance of 0.235 arcseconds. The binary nature of this pair was discovered by Sherburne W. Burnham in 1880. They orbit around each other every 11.6 years with a semimajor axis of 0.4 arcseconds. The brighter member of the pair, Kappa Pegasi B, is actually a spectroscopic binary, with the components designated Kappa Pegasi Ba and Kappa Pegasi Bb. They orbit about each other every six days. There is a fourth component, Kappa Pegasi C, which may be an optical companion.〔
==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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