Quiz 3-4 Flashcards

1
Q

How big is the Sun compared to the Earth?

A

The diameter of the Sun is about 109 times the diameter of Earth

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2
Q

How much mass does the Sun have compared to the Earth?

A

300,000 times the mass of Earth

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3
Q

What is the Sun made of?

A

70% Hydrogen, 28% Helium, 2% heavier elements

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4
Q

Describe how the temperature and density of the Sun change from the center to the visible surface of the Sun.

A

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5
Q

What keeps the Sun from collapsing under its own gravity?

A

Gravitational equilibrium: When the outward push of pressure balances the inward pull of gravity. The Sun’s outward push against gravity comes from the internal gas pressure. The Sun’s internal pressure precisely balances gravity at every point within it, thereby keeping the Sun stable in size. Because the weight of overlying layers is greater as we look deeper into the Sun, the pressure must increase with depth. Deep in the Sun’s core, the pressure makes the gas hot and dense enough to sustain nuclear fusion. The energy released by fusion, in turn, heats the gas and maintains the pressure that keeps the Sun in balance against the inward pull of gravity.

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6
Q

What is nuclear fusion and why are high temperatures needed for hydrogen fusion to occur?

A

Nuclear fusion is the process in which light-weight atomic nuclei smash together and stick (or fuse) to make heavier nuclei. High temperatures are needed because the hotter the temperature, the faster the speed of the of nuclei. At high speeds, nuclei come close enough (collide) for the strong force to bind them together.

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7
Q

How long does it take for a photon to escape the radiation zone in the Sun? Why?

A

About a million years because energy gradually leaks out of the radiation zone in the form of randomly bouncing photons (radiative diffusion).

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8
Q

What is the solar corona?

A

The outermost layer of the Sun’s atmosphere which extends several million kilometers above the visible surface of the Sun.

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9
Q

What is the solar wind? What effect does it have on comets?

A

A flow of charged particles from the surface of the Sun. The solar wind helps shape the magnetospheres of planets and blows back the material that forms the plasma tails of comets.

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10
Q

How does the sun rotate? How does this rotation affect the sun’s magnetic field lines?

A

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11
Q

What is a sunspot and how does it form?

A

Sunspots are dark, cooler regions in the visible surface of the sun. They occur where tightly wound magnetic fields poke nearly straight out from the solar interior. These tight magnetic field line suppress convection within the sunspot and prevent surrounding plasma from entering the sunspot. With hot plasma unable to enter the region, the sunspot plasma becomes cooler than the rest of the photosphere.

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12
Q

What do solar prominences, solar flares, and sunspots have in common?

A

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13
Q

What is a coronal mass ejection (CME) and how is the Earth protected from them?

A

CME is when billions of tons of hot gas are blasted into space at hundreds of miles per second. The Earth is protected from them by its magnetosphere (a region around a planet occupied by its magnetic field).

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14
Q

What is the aurora borealis? How is it formed?

A

When the magnetosphere is overloaded by the flow of charged particles from the Sun, they may cascade toward Earth, producing aurorae.

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15
Q

What is the name of the cells in your eyes that allow you to perceive colors? How many types are there, and which colors are each of them most sensitive to?

A

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16
Q

How are wavelength and energy related for photons (“particles of light”)? How is frequency related to wavelength?

A

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17
Q

List the main regions of the electromagnetic spectrum, from shortest wavelength to longest wavelength.

A

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18
Q

What is a molecular cloud?

A

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19
Q

What features of molecular clouds make conditions favorable for star formation?

A

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20
Q

What is interstellar dust?

A

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21
Q

How does dust affect our view of the night sky, and how is that view different in infrared light?

A

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22
Q

Does an orange star emit light of any colors other than orange? Why does it appear to be orange?

A

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23
Q

What is a protostar?

A

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24
Q

Why is it so hard to detect extrasolar planets?

A

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25
Q

How is the Doppler effect used to discover exoplanets?

A

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26
Q

Describe the transit method to detect exoplanets.

A

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27
Q

If you use an infrared telescope, is it easier to observe a warmer or a colder planet? Why?

A

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28
Q

In general, is it easier to discover big or small exoplanets? Explain your answer in detail.

A

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29
Q

What is the purpose of the space telescope named “Kepler”? Has it been successful? If so, explain why.

A

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30
Q

Describe in some detail one of the extrasolar planets that has been discovered.

A

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31
Q

What is the “habitable zone”?

A

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