Because they all involve the detonation of a carbon-rich white dwarf at Chandrasekhar's limit,all Type I supernovae are equally luminous.
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Q13: A carbon-detonation supernova starts out as a
Q14: The spectra of the youngest stars show
Q15: Unlike supernovae, novae can explode more than
Q16: Type II supernovae have little hydrogen in
Q17: Except for hydrogen and most of the
Q19: Most of the energy released during a
Q20: A massive star can fuse only up
Q21: For a nova to occur, the system
Q22: An iron core cannot support a star
Q23: Where was supernova 1987A located?
A)in the Orion
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