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The Life Cycle Of A Star (physics Only) (GCSE Physics)

The following is a GCSE Physics test covering 'The Life Cycle Of A Star (physics Only)' from the broader topic Space Physics. The test is geared towards the AQA exam board style syllabus.
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Which end state is most likely for a star with an initial mass similar to the Sun?
What role do neutrinos play in a core-collapse supernova?
What observational evidence can indicate that a star has recently undergone a supernova?
Why do massive stars undergo successive stages of fusion forming heavier elements up to iron?
What is the Chandrasekhar limit in the context of stellar remnants?
During the red giant phase a star’s outer layers expand and the surface temperature drops. What effect does this have on the star’s observed colour?
Which element’s fusion in stellar cores marks the end of energy-producing fusion in massive stars (i.e., fusion beyond this point absorbs energy rather than releases it)?
Which property of a star most strongly determines its evolutionary path and final fate?
How does a star’s luminosity change as it evolves off the main sequence into a red giant?
What is meant by “nucleosynthesis” in stellar astrophysics?
Which of the following best describes a planetary nebula?