Chapter 6 Flashcards

1
Q

With respect to light production in stars, select all of the correct statements from the following list.

Hotter stars radiate more energy at higher frequencies.
Stars emit light mostly from their surfaces.
Black body radiators are generally cool.
Temperature is a measure of the heat produced by a star.
Hotter stars have a longer maximum intensity wavelength.
The temperature of a star can be roughly estimated from its color.
Heat flows from hot to cool regions.

A

Hotter stars radiate more energy at higher frequencies.

Stars emit light mostly from their surfaces.

The temperature of a star can be roughly estimated from its color.

Heat flows from hot to cool regions.

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2
Q

With respect to atoms, select all of the correct statements from the following list.
Electrons can be found anywhere outside a nucleus.
The number of neutrons determines the isotope of an atom.
Neutral atoms have the same number of protons as electrons.
The nucleus is completely composed of neutrons.
Electrons surround the nucleus.
Protons are positively charged.
Gaining or losing protons produces different ions.

A

The number of neutrons determines the isotope of an atom.

Neutral atoms have the same number of protons as electrons.

Electrons surround the nucleus.

Protons are positively charged.

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3
Q

Based on the interactions of light and matter, select all of the correct statements from the following list.
Bright-line spectra are created by emission.
Hot gases produce emission spectra.
The size of an electron’s orbit depends on its energy.
Absorption spectra have dark lines.
Hot solids emit continuous spectra.
Electrons will move to higher orbits when an atom absorbs enough energy.
Atoms absorb energy by emitting photons.

A

Bright-line spectra are created by emission.

Hot gases produce emission spectra.

The size of an electron’s orbit depends on its energy.

Absorption spectra have dark lines.

Hot solids emit continuous spectra.

Electrons will move to higher orbits when an atom absorbs enough energy.

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4
Q

With resepct to stellar spectra, select all of the correct statements from the following list.
Atoms can absorb or emit any amount of energy.
Every single star has a unique spectrum.
Balmer lines tend to be strong in all stellar spectra.
Stellar spectra are absorption spectra.
Spectra can reveal the chemical composition of stars.
Doppler shifts in spectral lines give clues to the motions of stars.
The Lyman and Paschen series of the hydrogen spectrum are not visible.

A

Stellar spectra are absorption spectra.

Spectra can reveal the chemical composition of stars.

Doppler shifts in spectral lines give clues to the motions of stars.

The Lyman and Paschen series of the hydrogen spectrum are not visible.

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5
Q

What kind of radiation do we (the human body) emit?

A

infrared

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6
Q

If you quadruple the temperature of a black body, by what factor will the total energy radiated per second per square meter increase?

A

256

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7
Q

Which of the following statements is true about the Celsius and Kelvin (absolute) temperature scales?

A

The size of one degree is the same on both scales.

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8
Q

The temperature of a gas is a measure of which of the following?

A

average motion of its atoms

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9
Q

When the sun is high above the horizon in a clear sky, it has a yellowish color. According to the black body radiation curves shown here, the sun’s surface temperature is most nearly which of the following?

A

6,000 K

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10
Q

If the temperature of star B is twice the temperature of star A, what can we say about the energy emitted by the surface of star B compared to the energy emitted by star A?

A

Each square meter emits sixteen times as much energy per second.

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11
Q

Which subatomic particle has a negative charge?

A

electron

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12
Q

The wavelength of maximum intensity that is emitted by a black body is which of the following?

A

inversely proportional to temperature

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13
Q

Of the following, which color represents the lowest surface temperature for a star?

A

red

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14
Q

The amount of electromagnetic energy radiated from every square meter of the surface of a black body each second is which of the following?

A

proportional to temperature to the fourth power

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15
Q

An atom that is ionized must have which of the following?

A

either more electrons than protons or more protons than electrons

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16
Q

Which of the following is true of an atomic nucleus?

A

All of these choices are correct.

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17
Q

A hot hydrogen gas emits which of the following?

A

only three spectral lines in the visible spectrum: red, blue, and violet

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18
Q

hat conditions produce a dark (absorption line) spectrum?

A

light from a continuous spectrum source passing through a cooler low-density gas

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19
Q

Which electron energy level transition corresponds to a hydrogen atom absorbing a visible light photon that has a wavelength of 656 nanometers?

A

he electron makes the transition from energy level 2 to energy level 3.

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20
Q

All stars are composed of mostly hydrogen and helium, yet many stars have no lines for hydrogen or helium in their spectra. What causes this apparent contradiction?

A

The surface temperature is such that the electrons are not at the proper energy levels to produce spectral lines at visible wavelengths.

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21
Q

You research the star Sirius and find that its spectral lines are blue-shifted. What does this tell you about Sirius?

A

It has a radial velocity that is toward us.

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22
Q

Suppose that you take the spectra of several stars and identify the 656 nm line of hydrogen. You then measure against the reference spectrum on the same image and find that some of the 656 nm lines are shifted due to the Doppler effect. Of the following shifted locations of this line, which one is that of a star that is moving away from us at the highest speed?

A

star E at 659 nm

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23
Q

How did ancient blacksmiths judge the temperature of a heated piece of iron?

A

by its color

24
Q

Which piece of iron is hottest?

A

blue

25
Q

What is the color of the hottest stars?

A

blue

26
Q

What controls the color of a star?

A

its temperature

27
Q

which is a difference between a red star and blue star?

A

The blue star’s emissions peak at shorter wavelengths.

28
Q

If a match and a bonfire can both be considered a black body of about the same temperature, which is giving off more energy?

A

the bonfire

29
Q

If a match and a bonfire can both be considered a black body of about the same temperature, the bonfire gives off more energy. What is the reason for this?

A

The bonfire has a larger surface area.

30
Q

You are more likely to get your face scorched near a bonfire than the same distance from a match burning at the same temperature because:

A

The bonfire has a larger surface area.

31
Q

What is true of a neutral atom?

A

It has the same number of protons and electrons.

32
Q

What is true of an ion?

A

It has gained or lost electrons.

33
Q

What is true of an excited atom?

A

It has an electron at a higher energy level.

34
Q

What determines the wavelengths of the photons an atom will absorb or emit?

A

the difference in energy between electron energy levels

35
Q

What kind of spectrum would be observed when observing radiation from a hot solid or gas under high pressure?

A

continuous

36
Q

What kind of spectrum would be observed when observing radiation through a cool gas?

A

absorption

37
Q

What kind of spectrum would be observed when observing radiation from a compressed (thick) hot gas?

A

emission

38
Q

What kind of spectrum would you observe from molten lava?

A

continuous

39
Q

What kind of spectrum would you observe if you looked through gases boiling out of molten lava?

A

absorption

40
Q

What are the Balmer lines?

A

the visible lines of the hydrogen spectrum

41
Q

Doppler shifts in the wavelengths of stellar spectra can tell us about the motions of a star.

If the lines in a stellar spectrum are blueshifted, which of the following is true?

A

The star is moving toward us.

42
Q

Doppler shifts in the wavelengths of stellar spectra can tell us about the motions of a star.

If the lines in a stellar spectrum are redshifted, which of the following is true?

A

The star is moving away from us.

43
Q

Doppler shifts in the wavelengths of stellar spectra can tell us about the motions of a star.

If the lines in a stellar spectrum show no Doppler shift, which of the following is true?

A

The star could be moving perpendicular to a line between Earth and the star.

44
Q

The nebula shown in the figure above will produce a(n) __________ spectrum.

A

emission

45
Q

Which list below has the following types of stellar spectra in order of increasing temperature from left to right:

A

types M0; K5, G0, F5, A1, B0

46
Q

Which of the following colors or wavelength ranges is most intense in an M0 type star:

A

red

47
Q

Which of the following colors (or wavelength ranges) is most intense in an A1 type star:

A

blue

48
Q

Which of the following types of stellar spectra has its intensity peak at the longest wavelength?

A

type G4

49
Q

A Model Atom. What is the mass of a hydrogen atom in grams?

A

A trillionth of a trillionth of a gram

50
Q

Molecules and Atoms. Which is more massive: an atom, a molecule, an isotope, or an ion?

A

Molecule

51
Q

Absolute Zero. Create a chart of temperature on the vertical axis that includes absolute zero. On the horizontal axis, create three categories for Kelvin, Celsius, and Fahrenheit. Draw the range of freezing water to boiling water on Earth for each category to scale, labeling the temperature axes with the appropriate numbers as given in your text. For absolute zero, freezing water, and boiling water, label each with the speed of particles using words such as “slow motion,” “fast motion,” “no motion,” “very fast motion,” or “very slow motion.” Which words would you use to describe the motion of particles at 3000 K, which is the temperature of a red star?

A

Very fast motion

52
Q

Human Radiation II.
Human body temperature is about 310 K (3.10 × 102 K, or 98.6° F). In which EM band do humans emit most of their radiation? (Hint: See Wien’s Law.)

A

Infrared

53
Q

Human Blackbody. Humans are dense, warm objects, and thus they are blackbodies. A human’s body temperature is about 310 K (3.10 × 102 K, or 98.6° F). Add a panel to the figure below and graph to scale the blackbody emission of humans. From your graph, decide how much light humans emit in the visual wavelength band. Choose the best answer. (Hint: remember that hot object radiates more total energy than a cooler object (Stefan-Boltzmann law) and that the wavelength of maximum intensity is shorter for hotter objects than for cooler objects (Wien’s law).)

A

None

54
Q

Blackbodies. You observe three objects: a star whose surface temperature is around 5800 K, a molecular cloud whose surface temperature is around 58 K, and a nearby cluster of stars whose surface temperature is around 58,000 K. All of these objects are blackbodies. Which of the three objects could you see with your eyes in visual images of the objects? (Hint: Draw their blackbody spectra and find the visual band. Also, the figure below might be useful.)

A

The star and the cluster of stars

55
Q

Light Brightness. You observe three objects: a star whose surface temperature is around 5800 K, a molecular cloud whose surface temperature is around 58 K, and a nearby cluster of stars whose surface temperature is around 58,000 K. All of these objects are blackbodies. Find the colors that we would see these objects with our eyes. Find which color emits more light energy per unit surface area. Based on your values, which object emits more light energy per unit surface area?

A

Cluster of stars

56
Q

Star A, Star B Brightness. Star A’s surface temperature is half that of Star B’s. Which object is brighter at its surface and by how much?

A

Star B; 16