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What is the amount of energy emitted in the form of neutrinos, during a supernova explosion,compared to the amount of energy radiated as electromagnetic radiation?


A) only .007 as much
B) about equal amounts
C) about twice as much
D) ten times more
E) 100 times more

F) A) and E)
G) A) and D)

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Because they all involve the detonation of a carbon-rich white dwarf at Chandrasekhar's limit,all Type I supernovae are equally luminous.

A) True
B) False

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What made supernova 1987A so useful to study?


A) We saw direct evidence of nickel to iron decay in its light curve.
B) Its progenitor had been observed previously.
C) In the Large Magellanic Cloud, we already knew its distance.
D) It occurred after new telescopes, such as Hubble, could observe it very closely.
E) All of the above are correct.

F) B) and E)
G) B) and C)

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As a star evolves, heavier elements tend to form by various processes. Which of thefollowing is NOT one of these processes?


A) proton capture and neutron capture
B) fusion of like nuclei
C) helium capture
D) the s process
E) neutronization

F) B) and C)
G) A) and E)

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Which of these is the likely progenitor of a Type II supernova?


A) a mass-transfer binary, with the white dwarf already at 1.3 solar masses
B) a contact binary, with the neutron star at 2.3 solar masses
C) an evolved red giant which is just starting to make silicon in its core
D) two white dwarfs in a contact binary system
E) an evolved blue supergiant that is about to experience the helium flash

F) A) and E)
G) A) and C)

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After reaching its peak luminosity in hours or days, a nova declines in brightness over a periodof a few ________ before returning to its pre-explosion luminosity.

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The heaviest nuclei of all are formed:


A) by neutron capture during a Type II supernova explosion.
B) during a nova explosion.
C) during a carbon detonation supernova.
D) during carbon burning in the giant stage.
E) during the triple alpha process.

F) C) and E)
G) A) and E)

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Of all elements, ________ has the most stable and tightly bound nucleus.

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