The evolutionary cutoff between low- and high-mass stars occurs at approximately:

Name: The evolutionary cutoff between low- and high-mass stars occurs at approximately:
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The evolutionary cutoff between low- and high-mass stars occurs at approximately 3 solar masses. This is because at this mass, a star is able to sustain nuclear fusion of helium in its core and continue to burn heavier elements, leading to a longer overall lifespan and different evolutionary path than lower mass stars.

The Evolutionary Cutoff Between Low- and High-Mass Stars Occurs at Approximately