The main reason that stars evolved off the main sequence is because they are becoming less massive as energy is lost into space from the proton- proton cycle.
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Q4: Once the helium flash occurs at stage
Q5: The initial rise off the main sequence
Q6: All stars have roughly the same luminosity
Q7: About 90% of the star's total life
Q8: The luminosity of the red giant during
Q10: Helium fusion requires a higher temperature than
Q11: The helium flash increases the star's luminosity.
Q12: The least massive red main- sequence stars
Q13: The helium flash stage lasts several thousand
Q14: Low- mass stars may become hundreds of
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