High-mass stars burn their fuel much more quickly. and smaller stars are denser than high mass stars.
Because they have less fuel to burn and do so more slowly, low mass stars live longer than high mass stars. While they are converting hydrogen into helium, stars remain on the main sequence. They begin moving off the main sequence as soon as this process is finished. When their cores are depleted of hydrogen, stars exit the main sequence. Our own sun is an illustration of a low-mass star that doesn't perish as rapidly as a large star might. In fact, according to astronomers, we have yet to directly detect the demise of one of these extremely low mass stars.
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