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Main Sequence - star is stable because of Hydrostatic Equilibrium. Fusing Hydrogen to Helium in core. Stars spends about 90% lifetime as main sequence.

This is were I found the answer - http://www.maa.mhn.de/Scholar/star_evol.html

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In its next main stage of stellar evolution the sun is expected to be?

In its next main stage of stellar evolution, the Sun is expected to enter the red giant phase. As it exhausts hydrogen in its core, the core will contract and heat up, causing the outer layers to expand significantly. This expansion will ultimately engulf the inner planets, including Mercury and Venus, and possibly Earth. Eventually, the Sun will shed its outer layers, leaving behind a white dwarf surrounded by a planetary nebula.


What is the correct sequence for stellar evolution?

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How would you arrange this in order red giant white dwarf and main sequence and why?

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Point in stellar evolution when a star has used up all its fuel?

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What characterizes a star leaving the Main-Sequence?

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What is the next stage in the suns evolution?

The next stage in the Sun's evolution is the red giant phase. This occurs when the Sun runs out of hydrogen fuel in its core and starts burning helium. During this phase, the Sun will expand and become larger, eventually engulfing Mercury, Venus, and possibly Earth.


What is the evolutionary end of the sun?

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Why does water expand instead of increaing?

due to hydrogen bond


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