True/False
Once the core of a low-mass main-sequence star runs out of hydrogen, fusion in the star stops until the core temperature is high enough for helium fusion to begin.
Correct Answer:
Verified
Correct Answer:
Verified
Related Questions
Q5: How can the core of a star
Q45: If there were mixing processes in a
Q46: The Ring Nebula is a planetary nebula
Q48: A white dwarf star has a
Q49: Using the data in the table below,
Q50: Consider a red giant star with
Q51: A 10M <sub> <span class="ql-formula" data-value="\odot"><span
Q52: A low-mass red giant star's energy comes
Q71: If a main-sequence star were gaining mass
Q95: Explain the two different forms of pressure