astro ch 14 Flashcards

1
Q

What color does this wavelength correspond to in the visible-light spectrum?

A

Green

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2
Q

Why do you think the Sun appears white or yellow to our eyes?

A

Because the Sun radiates in other colors, and because the atmosphere scatters blue light stronger than red light.

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3
Q

What two physical processes balance each other to create the condition known as gravitational equilibrium in stars?
View Available Hint(s)

A

gravitational force and outward pressure

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4
Q

According to modern science, approximately how old is the Sun?

A

4.5 billion years

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5
Q

If the Sun suddenly stopped emitting neutrinos, what might we infer (after checking that our neutrino detectors were still operational)?

A

Fusion reactions in the Sun have ceased within the past few minutes

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6
Q

The light radiated from the Sun’s surface reaches Earth in about 8 minutes, but the energy of that light was released by fusion in the solar core about

A

a few hundred thousand years ago

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7
Q

What causes the cycle of solar activity?

A

changes in the organization of the Sun’s magnetic field

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8
Q

What is the solar wind?

A

a stream of charged particles flowing outward from the surface of the Sun

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9
Q

In the late 1800s, Kelvin and Helmholtz suggested that the Sun stayed hot because of gravitational contraction. What was the major drawback to this idea?

A

It predicted that the Sun could shine for about 25 million years, but geologists had already found that Earth is much older than this

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10
Q

Every second, the Sun converts about 600 million tons of hydrogen into 596 million tons of helium. The remaining 4 million tons of mass is

A

converted to an amount of energy equal to 4 million tons times the speed of light squared

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11
Q

The Sun’s surface seethes and churns with a bubbling pattern. Why?

A

We are seeing hot gas rising and cool gas falling as a result of the convection that occurs beneath the surface

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12
Q

What color does this wavelength correspond to in the visible-light spectrum?

A

Infrared, and thermal radiation with such a peak will be red.

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13
Q

How does this color compare with that of the Sun?

A

Sunspots seem to be dark spots because the surface of the Sun is much brighter.

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14
Q

Which of the following changes would cause the fusion rate in the Sun’s core to increase?

A

an increase in the core temperature
a decrease in the core radius

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15
Q

Which of the following must occur for a star’s core to reach equilibrium after an initial change in fusion rate?

A

If the fusion rate initially increases, then the core expands.
If the fusion rate initially decreases, then the core contracts

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16
Q

What would happen if the fusion rate in the core of the Sun were increased but the core could not expand?

A

The Sun’s core would start to heat up, and the rate of fusion would increase even more.

17
Q

In which layer(s) of the Sun does nuclear fusion occur?

A

core

18
Q

Which of the following layers of the Sun can be seen with some type of telescope? Consider all forms of light, but do not consider neutrinos or other particles.

A

chromosphere
photosphere
corona

19
Q

Which of the following best explains why nuclear fusion requires bringing nuclei extremely close together?

A

Nuclei normally repel because they are all positively charged and can be made to stick only when brought close enough for the strong force to take hold.

20
Q

The proton-proton chain is

A

the specific set of nuclear reactions through which the Sun fuses hydrogen into helium

21
Q

What do we mean when we say that the Sun is in energy balance?

A

The amount of energy released by fusion in the Sun’s core equals the amount of energy radiated from the Sun’s surface into space

22
Q

A salesman attempts to convince you to purchase a “solar neutrino shield” to protect you and your family. (It’s even “on sale!”) Why do you turn down this excellent offer?

A

Neutrinos rarely, if ever, interact with other matter.

23
Q

Which of the following is the best answer to the question, “Why does the Sun shine?”

A

As the Sun was forming, gravitational contraction increased the Sun’s temperature until the core become hot enough for nuclear fusion, which ever since has generated the heat that makes the Sun shine.

24
Q

When we say that the Sun is a ball of plasma, we mean that __________.

A

the Sun consists of gas in which many or most of the atoms are ionized (missing electrons)

25
Q

What is the Sun’s approximate composition (by mass)?

A

70% hydrogen, 28% helium, 2% other elements

26
Q

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

A

They are all strongly influenced by magnetic fields on the Sun

27
Q

Satellites in low-Earth orbits are more likely to crash to Earth when the sunspot cycle is near solar maximum because

A

Earth’s upper atmosphere tends to expand during solar maximum, exerting drag on satellites in low orbits

28
Q

Which of the following choices is not a way by which we can study the inside of the Sun?

A

We can send a space probe into the Sun’s photosphere.

29
Q

The dark spots in this photo (such as the one indicated by the arrow) represent what we call

A

sunspots

30
Q

How does the Sun’s mass compare to Earth’s mass?

A

The Sun’s mass is about 300,000 times the mass of the Earth.

31
Q

How is the sunspot cycle directly relevant to us here on Earth?

A

Coronal mass ejections and other activity associated with the sunspot cycle can disrupt radio communications and knock out sensitive electronic equipment.

32
Q

Why do sunspots appear dark in pictures of the Sun?

A

They actually are fairly bright, but appear dark against the even brighter background of the surrounding photosphere.

33
Q

The Sun’s visible surface (that is, the surface we can see with our eyes) is called the

A

photosphere

34
Q

What is the overall fusion reaction that converts mass into other forms of energy in the Sun’s core?

A

4 hydrogen nuclei become 1 helium nucleus

35
Q

When we refer to the solar thermostat, we are referring to the idea that

A

the Sun’s core temperature naturally stays stable

36
Q

The energy balance that contributes to the solar thermostat is a balance between

A

the energy released in the core by fusion and the energy radiated from the Sun’s surface into space