クリューゲル60
1. Kruger 60Kruger 60 (DO Cephei) is a binary star system located 13.15 light-years from the Sun. These red dwarf stars orbit each other every 44.6 years. The larger, primary star is designated component A, while the secondary, smaller star is labeled component B. Component A has about 27% of the Sun's mass and 35% of the Sun's radius. Component B has about 18% of the Sun's mass and 24% of the Sun's radius. Component B is a flare star and has been given the variable star designation "DO Cephei".
Read “Kruger 60” on English Wikipedia
Read “クリューゲル60” on Japanese Wikipedia
Read “Kruger 60” on DBpedia
Read “Kruger 60” on English Wikipedia
Read “クリューゲル60” on Japanese Wikipedia
Read “Kruger 60” on DBpedia
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