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The average density of neutron stars approaches


A) a million times that of normal matter.
B) a million times that of even a white dwarf.
C) about 10¹⁷ kg/m³, similar to the density of atomic nuclei.
D) about 10¹⁸ times that of water.
E) infinity.

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Neutron stars and black holes are formed by


A) the star formation process.
B) mass transfer in binary star systems.
C) novae.
D) type I supernovae.
E) type II supernovae.

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Can our Sun ever become a nova? Why?

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No, ours is a single star, wit...

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Short duration gamma-ray bursts are explained as the merger of two neutron stars.

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How does the death of one very massive star give birth to perhaps hundreds of smaller ones soon thereafter?

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The more massive the star, the faster it...

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What is stellar nucleosynthesis?


A) The formation of heavier elements inside stars
B) The formation of planetary nebulae by red giants
C) The formation of stars from a nucleus of contracting material
D) The formation of white dwarfs, neutron stars, and black holes from stars
E) The process by which stars form interstellar dust

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Why should the youngest stars be made of the heaviest elements?

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With each generation of supern...

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Nearly all the elements found in nature were formed inside stars, EXCEPT for


A) carbon and silicon.
B) hydrogen and helium.
C) helium and carbon.
D) silver and technetium.
E) uranium and radium.

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

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

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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.

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

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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.

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The remains of type II supernovae (massive star, core collapse supernovae) are seen in the sky as


A) nebulae that are shrinking as the central mass pulls them in.
B) nebulae that are expanding at thousands of kilometers per hour.
C) nebulae that are stellar nurseries.
D) white dwarfs.
E) white holes.

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Astronomers believe that gamma-ray bursters emit radiation equally in all directions.

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Type II supernovae have little hydrogen in their spectra; it had been used up already.

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Novae are more closely related to type II than to type I supernovae.

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Which statement about young stars is FALSE?


A) They contain a larger fraction of heavy elements than previous generations.
B) They are born in a dustier environment than earlier generations.
C) They are more likely to have planets forming with them than earlier generations.
D) The high mass stars will be more likely to produce heavier elements as they evolve.
E) Being young, they will have more pure hydrogen than earlier generations.

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What is the importance of 1.4 solar masses in stellar evolution?

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1.4 solar masses is the Chandrasekhar Li...

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The vast majority of pulsars are known only from their pulses in


A) X-rays.
B) gamma-rays.
C) visible light.
D) microwaves.
E) radio waves.

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A massive star can fuse only up to the element silicon in its core.

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