しゅけいれつせい
主系列星
1. main sequence star; main sequence stars
2. Main sequenceThe main sequence is a continuous and distinctive band of stars that appears on plots of stellar color versus brightness. These color-magnitude plots are known as Hertzsprung–Russell diagrams after their co-developers, Ejnar Hertzsprung and Henry Norris Russell. Stars on this band are known as main-sequence stars or "dwarf" stars. After a star has formed, it creates energy at the hot, dense core region through the nuclear fusion of hydrogen atoms into helium.
Read “Main sequence” on English Wikipedia
Read “主系列星” on Japanese Wikipedia
Read “Main sequence” on DBpedia
Read “Main sequence” on English Wikipedia
Read “主系列星” on Japanese Wikipedia
Read “Main sequence” on DBpedia
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