Quiz 3 Flashcards

1
Q

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

A

It predicted that the sun could last only about 25 million years, which is far less than the age of earth

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2
Q

What do we mean when we say that the sun is in gravitational equilibrium

A

There is a balance within the sun between the outward push of pressure and the inward pull of gravity

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3
Q

What is the approximate composition of the sun

A

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

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4
Q

What are the appropriate units for the suns luminosity

A

Watts

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5
Q

What is the average temp of the surface of the sun

A

6,000 kelvin

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6
Q

Which is closest to the temperature of the core of the sun

A

10 million Kelvin

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7
Q

From the center outward, which of the following lists the layers of the sun in the correct order

A

CRC PCC

Core, radiation zone, convection zone, photosphere, chromosphere, corona

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8
Q

Which layer of the sun do we normally see

A

Photosphere

The one you take pictures of

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9
Q

The core of the sun is

A

Hotter and denser than the surface

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10
Q

Why do sunspots appear dark in pictures of the sun

A

They actually are fairly bright but appears dark against even brighter background of the surrounding sun

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11
Q

How does the sun generate energy today?

A

Nuclear fusion

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12
Q

At the center of the sun, fusion converts hydrogen into

A

Helium, energy, and nutrinos

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13
Q

Suppose you put two protons near each other, because of the electromagnetic force the two protons will

A

Repel each other

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14
Q

The first step in the proton proton chain produces an anti electron or positron. What happens to the positron

A

It is rapidly converted to energy when it meets an ordinary electron resulting in matter antimatter annihilation

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15
Q

The overall fusion reaction by which the sun currently produces energy is

A

4h=1 He+energy

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16
Q

Which statements best describes the solar neutrino problem

A

Solar neutrinos have been detected, but in fewer numbers than predicted by theoretical models

17
Q

Why are neutrinos so difficult to detect

A

Because they rarely interact with matter

18
Q

What is possible solution to the solar neutrino problem

A

The electron neutrinos created in the sun change into another type of neutrino that we do not detect

19
Q

What happens to energy in the convection zone of the sun

A

Energy is transported outward by the rising of hot plasma and the sinking of cooler plasma

20
Q

Most of the energy produced in the sun is released in the form of visible light from the photosphere. However some energy is released from the upper layers of the solar atmosphere. Which of the following best describes where other form of light are released?

A

The chromosphere is the source of ultraviolet light, and the corona is the source of X rays

21
Q

What is the granulation of the sun

A

The bubbling pattern in the photosphere produced by he underlying convection

22
Q

What processes are involved in the sunspot cycle

A

The winding of magnetic field lines due to differential rotation

23
Q

What observations characterize solar maximum

A

We see many sunspots on the surface of the sun