Why can high-mass stars "burn" helium more easily than low-mass stars?
A) A high-mass star's core is already very hot, so it only needs to compress its core a little to burn helium.
B) High-mass stars are already burning helium on the main sequence.
C) Low-mass stars have proportionately less helium than high-mass stars.
D) This statement is false. It is much harder for high-mass stars to burn helium.
Correct Answer:
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Q51: Stars like the Sun probably do not
Q52: As a star like the Sun evolves
Q53: A star leaves the main sequence when
A)
Q54: When a massive star begins to run
Q55: When a massive star begins to run
Q57: The period-luminosity law of pulsating variable stars
Q58: What makes variable stars useful in determining
Q59: High-mass stars become _ variables when they
Q60: The light curve of a large Cepheid
Q61: What is a "pulsating star"?
A) a rotating
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