File:HRDiagram.png · Wikimedia Commons · See Wikimedia Commons
The main sequence is a distinctive band of stars that appears on diagrams plotting stellar brightness against temperature, representing stars that are actively fusing hydrogen in their cores. Most stars, including our Sun, spend the majority of their lifetimes on the main sequence, making it the most important stage in a star's life cycle.
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Within Vinony's link graph, 주계열 is referenced by 2,787 other articles, and connects out to stellar classification, exotic star and giant star.
It sits within the topics Concepts in astronomy, Main-sequence stars and Star types.
Its subject is documented across 68 Wikipedia language editions.
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