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Compare the amount of time a 20 solar mass star will stay on the main sequence to the lengthof time its iron core can exist.

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A 20 solar mass star will stay...

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The core of a highly evolved high mass star is a little larger than:


A) our solar system.
B) our Sun.
C) Jupiter.
D) Earth.
E) a white dwarf.

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

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The total energy emitted by the brightest nova explosions is about:


A) 1,000 Suns.
B) 50,000 Suns.
C) a million Suns.
D) a billion Suns.
E) a trillion Suns.

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

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An iron core will collapse in approximately one ________ in a Type II supernova event.

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Most of the energy released during a supernova is emitted as neutrinos.

A) True
B) False

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What is the only element in your body that was formed during the Big Bang, and not in coresof stars? Explain how you know this.

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Hydrogen was formed during the...

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As a star's evolution approaches the Type II supernova, we find:


A) the heavier the element, the less time it takes to make it.
B) the heavier the element, the higher the temperature to fuse it.
C) helium to carbon fusion takes at least 100 million K to start.
D) photodisintegration of iron nuclei begins at 10 billion K to ignite the supernova.
E) All of the above are correct.

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

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Why does conversion of its core to iron have to mark the end of a star's life? Which stars canend up with iron cores?

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Stars with a total mass of 8 solar masse...

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In a nova, there is a white dwarf, an evolving companion star, and a(n)________ surroundingthe white dwarf's equator.

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The Crab Nebula is a bright, long-lasting supernova remnant that was made by a ________supernova.

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The Chandrasekhar Limit is:


A) the upper mass limit for a white dwarf.
B) the temperature at which hydrogen fusion starts.
C) the temperature at which helium fusion starts.
D) the point at which a planetary nebula forms.
E) the lower mass limit for a Type II supernova.

F) A) and B)
G) B) and D)

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An iron core cannot support a star because:


A) iron is the heaviest element, and sinks upon differentiation.
B) iron has poor nuclear binding energy.
C) iron cannot fuse with other nuclei to produce energy.
D) iron supplies too much pressure.
E) iron is in the form of a gas, not a solid, in the center of a star.

F) B) and D)
G) C) and D)

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For a nova to occur, the system must have already been a(n) :


A) astrometric binary.
B) detached binary.
C) spectroscopic binary.
D) mass-transfer binary.
E) eclipsing binary.

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

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Stellar nucleosynthesis is responsible for the existence of all elements except hydrogen.

A) True
B) False

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What do X-ray observations tell us about conditions around a potential nova?

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The mass transfer causes an accretion di...

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What is the CNO cycle and how is it different from hydrogen fusion via the proton-protonchain?

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The CNO cycle is a kind of hydrogen fusi...

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Why are neutrinos from a Type II supernova detected before photons?


A) Neutrinos travel faster than photons.
B) Neutrinos are easier to detect than photons.
C) Neutrinos are produced in the explosion before photons.
D) Neutrinos are emitted from the outer part of the star; photons come from the core.
E) Neutrinos escape from the star quickly because they hardly interact with matter; photons aredelayed by interactions with matter.

F) B) and E)
G) B) and D)

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Except for hydrogen and most of the helium, all the elements have been formed throughstellar nucleosynthesis.

A) True
B) False

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The supernova that formed M-1, the Crab Nebula, was observed in:


A) 1572 AD by Tycho Brahe.
B) 1604 AD by Johannes Kepler.
C) 1054 AD by Chinese and Middle Eastern astronomers.
D) 1006 by observers in the southern hemisphere.
E) about 9,000 BC by all our ancestors.

F) A) and D)
G) A) and C)

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A carbon-detonation supernova starts out as a white dwarf in a close binary system.

A) True
B) False

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