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definition | During the main sequence stage, a star burns the hydrogen in its core and transforms it into helium. When the helium mass amounts to about 10% of the initial stellar mass, the star can no longer maintain the hydrostatic equilibrium in its core; the star increases its volume and leaves the main sequence in order to become a red giant. | |||||||
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scope note | Not to be confused with the Chandrasekhar limit. | |||||||
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contributor | AAS_Frey.Katie_Admin original | |||||||
creator | AAS_Frey.Katie original |