Chapter 5 - Light Flashcards

Test Review for Chapter 5 (37 cards)

1
Q

Absorption lines

A

Black lines seen on a spectrum that occur when an object absorbs light

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2
Q

Amplitude

A

The height of a wave
(peak to trough)

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3
Q

Atomic mass

A

The number of protons and neutrons in an atom

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4
Q

Atomic number

A

The number of protons in an atom

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5
Q

Doppler effect

A

Occurs when light from a moving object appears differently depending on how the object is moving

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6
Q

Emission lines

A

Colored lines on a spectrum that occur when an object emits light

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7
Q

Frequency

A

The number of waves that pass a particular point every second

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8
Q

Ionization energy

A

The amount of energy required for an electron to escape an atom

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9
Q

Intensity

A

The amount of radiation emitted at a particular wavelength

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10
Q

Isotope

A

Atoms of the same element that have different numbers of neutrons

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11
Q

Photon

A

A particle of light

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12
Q

Power

A

Energy per unit time

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13
Q

Redshift

A

Occurs when the light from an object appears to have its wavelengths shifted towards the red end of the spectrum

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14
Q

Blueshift

A

Occurs when the light from an object appears to have its wavelengths shifted towards the blue end of the spectrum

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15
Q

Wavelength

A

The distance from peak-to-peak or trough-to-trough in a wave

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16
Q

What are the ways in which light and matter interact?

A
  1. Light can pass through matter (transmission)
  2. Matter can reflect light
  3. Matter can scatter light
  4. Matter can absorb light
  5. Matter can emit light
17
Q

List the electromagnetic spectrum in order of increasing wavelength.

A

Gamma rays, X rays, ultraviolet, visible light, infrared, microwaves, radio waves

18
Q

List the electromagnetic spectrum in order of increasing frequency.

A

Radio waves, microwaves, infrared, visible light, ultraviolet, X-rays, gamma rays

19
Q

List the electromagnetic spectrum in order of increasing energy.

A

Radio waves, microwaves, infrared, visible light, ultraviolet, X-rays, gamma rays

20
Q

How is the wavelength and frequency of light related to its speed?

A

No relation
Light travels at the same speed regardless of wavelength or frequency

21
Q

How is the energy of a photon related to its frequency?

A

Higher-energy photons have higher frequencies
(directly proportional)

22
Q

What is the approximate wavelength range of visible light?

23
Q

What is the approximate frequency range of visible light?

A

400 - 750 THz

(400 - 750 trillion Hz)

24
Q

Emission spectrum:
What does it show, what does it look like, and how is it produced?

A
  1. It shows the wavelengths of light emitted by atoms/molecules
  2. It is mostly black with a few colored lines
  3. It is produced when a cooler object emits light, such as a cloud of cool gas
25
Absorption spectrum: What does it show, what does it look like, and how is it produced?
1. Shows the complete spectrum of light emitted by an object, minus any blocked by other materials 2. Looks like a complete rainbow with black lines throughout 3. Produced when light from a hot object passes through cooler materials
26
Continuous spectrum: What does it show, what does it look like, and how is it produced?
1. Shows the complete spectrum of colors produced by an object 2. Looks like a full, unbroken rainbow 3. Produced by hot, dense objects (blackbodies)
27
Thermal spectrum: What does it show, what does it look like, and how is it produced?
1. Shows the range of wavelengths of light produced by an object and their relative intensities 2. Looks like a graph of a smooth curve 3. Produced by any hot object emitting light
28
How are electron energy level transitions related to the wavelength/frequency/energy of the absorbed or emitted photon?
The greater the energy transition, the greater the energy of the photon. Higher frequency and shorter wavelength. The smaller the energy transition, the smaller the energy of the photon. Lower frequency and longer wavelength.
29
Describe Wien's Law.
The radiation curve for blackbodies will peak at wavelengths that are inversely proportional to the blackbody's temperature.
30
As an object gets hotter, what happens to the wavelength at which it emits most of its radiation?
They will become shorter
31
As an object gets colder, what happens to the wavelength at which it emits most of its radiation?
They will become longer
32
Describe the Stefan-Boltzmann Law.
For a blackbody, the energy radiated by unit surface area per unit time is proportional to its temperature raised to the fourth power.
33
What happens to the energy emitted by a blackbody as the temperature of that body increases?
It increases
34
If we observe the frequency of light from an object to be higher than the rest frequency, is the object moving towards or away from us?
Towards us (the light is being blueshifted)
35
If we observe the frequency of light from an object to be lower than the rest frequency, is the object moving towards or away from us?
Away from us (the light is being redshifted)
36
If an object is moving towards us, how would the wavelength of its light compare to its wavelength at rest?
The wavelength would be shorter (more blue)
37
If an object is moving away from us, how would the wavelength of its light compare to the wavelength at rest?
The wavelength would be longer (more red)