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distinctive band of stars on Hertzsprung–Russell diagrams

AI overview

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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Wikidata facts

Instance of: stellar evolution
Subclass of: stellar evolution
Part of: Hertzsprung–Russell diagram
Has part: G-type main-sequence star
Followed by: subgiant
Image: HRDiagram.png

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topic's main category: Category:Main-sequence stars
Commons category: Main-sequence stars
on focus list of Wikimedia project: Wikipedia:Vital articles/Level/4

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