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Quiz #9

Authored by Kian Rexroat

Science

University

Used 3+ times

Quiz #9
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25 questions

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1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Degeneracy pressure is the source of the pressure that stops the crush of gravity in all of the following except

a White dwarf

A brown dwarf

A neutron star

A very massive main sequence star

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

White dwarfs are so called because

They are both very hot and very small

They are supported by electron degeneracy pressure

They are the opposite of black holes

It amplifies the contrast with the red giants

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following is closest in mass to a white dwarf?

The moon

Earth

The sun

Jupiter

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why is there an upper limit to the mass of a white dwarf?

White dwarfs come only from stars smaller than 1.4 solar masses

The upper limit to the masses of white dwarfs was determined through observations of white to worse, but no one know why the limit exists

The more massive the white dwarf, the higher its temperature and hence the greater it’s degeneracy pressure. At about 1.4 solar masses, the temperature become so high that all matter effectively melts, even individual subatomic particles

The more massive the white dwarf, the greater the degeneracy pressure in the faster the speed of its electrons. Near 1.4 solar masses the speed of the electrons approach the speed of light, some more mass cannot be added without breaking the degeneracy pressure

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the ultimate fate of an isolated white dwarf?

As gravity overwhelms the electron degeneracy pressure, it will explode as a supernova

It will cool down and become a cold black dwarf

The electron degeneracy pressure will eventually overwhelm gravity and the white dwarf will slowly evaporate

As gravity overwhelms the electron degeneracy pressure, it will all become a neutron star

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Suppose a white dwarf is gaining mass because of accretion in a binary system. What happens if the mass someday reaches the 1.4 solar mass limit?

A white dwarf can never gain enough mass to reach the limit because a strong stellar wind prevents the material from reaching it in the first place

The white dwarf immediately collapses into a black hole, disappearing from view

The white dwarf, which is made mostly of carbon, suddenly becomes much hotter in temperature and therefore is able to begin fusing the carbon. This turns the white dwarf back into a star supported against gravity by ordinary pressure.

The white dwarf undergoes a catastrophic collapse, leading to a type of supernova that is somewhat different from that which occurs in a massive star but is comparable in energy

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which of the following statements about nova is not true

When I start system undergoes ANOVA, it brightens considerably, but not as much as a star to undergo a supernova

A star system that undergoes a nova may have another nova sometime in the future

The word nova means new start and originally referred to stars that suddenly appeared in the sky, then disappeared again after a few weeks or months

Our son will probably undergo at least one over when it becomes a white dwarf about 5 billion years from now

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