Deck 65: Mass Loss and Death of Low-Mass Stars

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Question
Stars like our sun will leave this type of remnant after they die:

A) neutron star
B) black hole
C) T-Tauri
D) white dwarf
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Question
Helium core fusion in the Sun will last about _____ years.

A) 10 million
B) 1 million
C) 100 million
D) 1000 million
Question
Stars like our sun will in their final phases become

A) RR Lyra variable.
B) Mira variable.
C) Cepheid variable.
D) T-Tauri variable.
Question
The process that generates energy in a white dwarf is

A) the fusion of hydrogen into helium.
B) the fusion of helium into carbon.
C) the helium flash.
D) nonexistent. A white dwarf no longer generates energy.
Question
After our sun dies it will be surrounded by a _______.
Question
Our sun will become a _____ when it dies.
Question
Eventually a white dwarf cools to a black dwarf.
Question
A low mass star is usually less than 12 solar masses.
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Deck 65: Mass Loss and Death of Low-Mass Stars
1
Stars like our sun will leave this type of remnant after they die:

A) neutron star
B) black hole
C) T-Tauri
D) white dwarf
white dwarf
2
Helium core fusion in the Sun will last about _____ years.

A) 10 million
B) 1 million
C) 100 million
D) 1000 million
100 million
3
Stars like our sun will in their final phases become

A) RR Lyra variable.
B) Mira variable.
C) Cepheid variable.
D) T-Tauri variable.
Mira variable.
4
The process that generates energy in a white dwarf is

A) the fusion of hydrogen into helium.
B) the fusion of helium into carbon.
C) the helium flash.
D) nonexistent. A white dwarf no longer generates energy.
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5
After our sun dies it will be surrounded by a _______.
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6
Our sun will become a _____ when it dies.
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7
Eventually a white dwarf cools to a black dwarf.
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8
A low mass star is usually less than 12 solar masses.
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