Astronomy: Explaining Why Stars on Top Left of Main Sequence Spend Less Time

Thread starter vanilla5085
Start date Feb 20, 2014
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Astronomy Stars

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Stars on the top left of the main sequence, typically more massive and hotter, have higher rates of nuclear fusion, leading to faster consumption of their hydrogen fuel. In contrast, stars on the lower right are less massive and cooler, allowing them to sustain hydrogen fusion for a longer duration. The difference in mass and temperature directly influences their lifespans on the main sequence, with more massive stars having significantly shorter lifetimes. This phenomenon is a fundamental aspect of stellar evolution and is well-documented in astrophysics. Understanding these differences is crucial for studying the life cycles of stars.

Feb 20, 2014

vanilla5085

Hi, I was just wondering if anyone could help me with this question. I couldn't find anything on the internet.

Q12 Explain why a star on the top left of the main sequence will spend much less time on the main sequence than another star on the lower right

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Feb 20, 2014

SteamKing

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Nothing at all? How hard did you look?

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