There is a mass-luminosity relationship because stars support their weight by generating energy, and more massive stars have more weight to support.
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Q3: Observing star clusters will give astronomers needed
Q4: Stellar models can easily be accomplished by
Q5: What is the upper limit of a
Q6: The age of a star cluster can
Q7: The helium flash stage will always completely
Q9: When the Sun moves off the main
Q10: Brown dwarfs are _.
A) stars with a
Q11: Globular clusters have approximately how many stars?
A)
Q12: As a one-solar-mass star evolves off the
Q13: Giant and supergiant stars are rare because
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