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If it gains sufficient mass from a binary companion, a white dwarf can become a


A) black dwarf.
B) planetary nebula.
C) Type II supernova.
D) brown dwarf.
E) Type I supernova.

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Like emission nebulae, planetary nebulae glow because hot stars are causing the gases to ionize when exposed to strong ultraviolet radiation.

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Why is our Sun not forming carbon and heavier elements yet?

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It still has plenty of hydrogen in its c...

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What temperature is needed to fuse helium into carbon?


A) 5,800 K
B) 100,000 K
C) 15 million K
D) 100 million K
E) one billion K

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As a 6 solar- mass star leaves the main sequence on its way to becoming a red supergiant, its luminosity


A) first decreases, then increases.
B) first increases, then decreases.
C) remains roughly constant.
D) decreases.
E) increases.

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On the H- R diagram, a star's position on the main sequence depends on the star's .

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Which stars in globular clusters are believed to be examples of mergers?


A) blue stragglers
B) brown dwarfs
C) planetary nebulae cores
D) blue supergiants
E) eclipsing binaries

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Helium fusion requires a higher temperature than hydrogen fusion.

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Paradoxically, while the core of the red giant is contracting and heating up, its radiation pressure causes its photosphere to swell up and cool off.

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The outward pressure in the core of a red giant balances the inward pull of gravity when


A) the electrons and protons have combined to form neutrons.
B) hydrogen begins fusing into helium.
C) iron forms in the inner core.
D) carbon fuses into heavier elements.
E) the electron orbits are compressed so much they are all in contact.

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Will the Sun become a brown dwarf? Explain.

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No, our Sun is massive enough ...

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The number of Type I and Type II supernovae observed are approximately equal.

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Our Sun will fade in luminosity as its supply of hydrogen drops in a billion years.

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

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A recurrent nova could eventually build up to a


A) core composed of iron.
B) Type II supernova.
C) helium flash.
D) planetary nebula.
E) Type I supernova.

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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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Contrast the deaths of low- versus high- mass stars.

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Low- mass stars swell up as red giants, ...

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Solar mass stars eventually become hot enough for carbon nuclei to fuse together.

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Compared to a cluster containing type O and B stars, a cluster with only type F and cooler stars will be


A) younger.
B) further away.
C) older.
D) more obscured by dust.
E) less obscured by dust.

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A small, dense star the size of Earth that shines by only stored heat is a


A) blue straggler.
B) white dwarf.
C) blue dwarf.
D) black dwarf.
E) brown dwarf.

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