When helium fusion begins in a one solar mass main star, it begins gradually, with this rateslowly increasing over time.
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Q4: Modern astronomers have observed the complete life
Q5: The age of a star cluster can
Q6: A ten billion year old globular cluster
Q7: For binary star systems where the stars
Q8: While more massive than most of its
Q10: A star cluster of age 100 million
Q11: While none yet exist, in the very
Q12: For our Sun, the production of carbon
Q13: As a star begins to evolve away
Q14: When a star becomes a red giant,
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