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Last updated 12:33 PM on 9/22/26
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150 Terms

1
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When light slows down entering a new medium, it bends __.

toward the normal.

2
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When light speeds up entering a new medium, it bends __.

away from the normal.

3
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What does the law of reflection state?

Angle of incidence equals angle of reflection.

4
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Diffuse reflection is the __ of light from a rough surface.

scattering

5
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Fermat’s Principle states that light takes the __.

path of least time.

6
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Why does the Sun appear higher at sunrise and sunset?

Atmospheric refraction bends sunlight.

7
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Why do stars twinkle?

Turbulent air refracts starlight unpredictably.

8
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The cause of a mirage is __.

total internal reflection in hot, less dense air.

9
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Total internal reflection occurs when the angle is greater than the __.

critical angle going from dense to less dense.

10
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The index of refraction formula is __.

n = c / v.

11
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The sky appears blue because __.

short wavelengths scatter most.

12
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Why are sunsets red?

Blue light scatters away over long paths; red survives.

13
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Clouds appear white because __.

water droplets scatter all visible wavelengths.

14
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The cause of a rainbow involves __ and internal reflection inside raindrops.

dispersion

15
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Thin film interference is caused by __.

interference between reflections from top and bottom surfaces of a thin film.

16
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Why do soap bubbles show colors?

Thin film interference.

17
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What determines the colors in thin films?

Film thickness and wavelength of light.

18
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Fluorescence occurs when __ excites electrons which emit visible light.

UV light

19
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Fluorescent lamps use phosphor to __.

convert UV light to visible light.

20
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The main difference between fluorescence and phosphorescence is that phosphorescence emits light __.

slowly due to metastable states.

21
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What is an emission spectrum?

Bright lines emitted by excited atoms.

22
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An absorption spectrum is characterized by __ where atoms absorb specific wavelengths.

dark lines

23
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Alpha radiation is a __.

helium nucleus (2 protons, 2 neutrons).

24
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What changes occur during alpha decay?

Atomic number –2, mass number –4.

25
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Beta minus decay changes the atomic number by __.

+1, mass number unchanged.

26
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Gamma emission results in __.

no change in atomic or mass number.

27
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The highest penetrating radiation is __.

gamma radiation.

28
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The strong nuclear force is the __ force and binds nucleons.

strongest and short-range

29
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Why are large nuclei unstable?

Strong force weakens at long distances; proton repulsion increases.

30
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A free neutron behavior results in __.

beta decay into proton, electron, and antineutrino.

31
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Radioactivity is the __ of unstable nuclei.

spontaneous decay

32
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Half-life is the time for __ of a radioactive sample to decay.

half

33
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The type of radiation used in smoke detectors is __.

alpha radiation.

34
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Nuclear fission is the __ of a heavy nucleus into smaller ones with energy release.

splitting

35
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The main source of fission energy comes from __.

kinetic energy of fission fragments.

36
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A condition necessary for a chain reaction is __.

critical mass.

37
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The function of a moderator in nuclear reactions is to __ neutrons.

slow.

38
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Control rods function to __ neutrons.

absorb.

39
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The function of a coolant in a reactor is to __.

transfer heat from the reactor core.

40
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A breeder reactor produces __ by converting U-238 into Pu-239.

plutonium

41
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Nuclear fusion involves the __ of light nuclei into heavier nuclei with energy release.

joining

42
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In the Sun, hydrogen fuses into __.

helium.

43
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Fusion releases energy because __ decreases.

mass per nucleon.

44
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In both fission and fusion, what is conserved?

The number of nucleons.

45
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The fastest-moving radiation is __.

gamma.

46
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Who explained nuclear fission?

Lise Meitner.

47
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Mass-energy equivalence is represented by the equation __.

E = mc².

48
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The photon energy equation is __.

E = hf.

49
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The wave speed formula is __.

v = fλ.

50
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Absorption lines are caused by __ of specific frequencies of light.

atoms absorbing.

51
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When light slows down entering a new medium

It bends toward the normal.

52
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When light speeds up entering a new medium

It bends away from the normal.

53
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Law of reflection

Angle of incidence equals angle of reflection.

54
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Diffuse reflection

Scattering of light from a rough surface.

55
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Fermat’s Principle

Light takes the path of least time.

56
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Why the Sun appears higher at sunrise/sunset

Atmospheric refraction bends sunlight.

57
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Why stars twinkle

Turbulent air refracts starlight unpredictably.

58
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Cause of a mirage

Total internal reflection in hot, less dense air.

59
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Total internal reflection

Occurs when angle > critical angle going dense to less dense.

60
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Index of refraction formula

n=cvn = \frac{c}{v}

61
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Why the sky is blue

Short wavelengths scatter most.

62
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Why sunsets are red

Blue light scatters away over long paths; red survives.

63
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Why clouds are white

Water droplets scatter all visible wavelengths.

64
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Cause of a rainbow

Dispersion + internal reflection inside raindrops.

65
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Cause of thin film interference

Interference between reflections from top and bottom surfaces of a thin film.

66
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Why soap bubbles show colors

Thin film interference.

67
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What determines thin film colors

Film thickness and wavelength of light.

68
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Fluorescence

UV excites electrons which emit visible light.

69
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Why fluorescent lamps use phosphor

Converts UV light to visible light.

70
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Difference between fluorescence and phosphorescence

Phosphorescence emits light slowly due to metastable states.

71
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Emission spectrum

Bright lines emitted by excited atoms.

72
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Absorption spectrum

Dark lines where atoms absorb specific wavelengths.

73
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Alpha radiation

Helium nucleus (2 protons, 2 neutrons).

74
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Alpha decay changes

Atomic number −2-2, mass number −4-4.

75
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Beta minus decay changes

Atomic number +1+1, mass number unchanged.

76
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Gamma emission changes

No change in atomic or mass number.

77
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Highest penetrating radiation

Gamma radiation.

78
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Strong nuclear force

Short-range but strongest force; binds nucleons.

79
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Why large nuclei are unstable

Strong force weakens at long distances; proton repulsion increases.

80
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Free neutron behavior

Beta decays into proton, electron, and antineutrino.

81
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Radioactivity

Spontaneous decay of unstable nuclei.

82
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Half-life

Time for half the radioactive sample to decay.

83
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Radiation used in smoke detectors

Alpha radiation.

84
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Nuclear fission

Splitting a heavy nucleus into smaller ones with energy release.

85
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Main source of fission energy

Kinetic energy of fission fragments.

86
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Condition for chain reaction

Critical mass.

87
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Moderator function

Slows neutrons.

88
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Control rods function

Absorb neutrons.

89
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Coolant function

Transfers heat from the reactor core.

90
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Breeder reactor production

Converts U-238\text{U-238} into Pu-239\text{Pu-239}.

91
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Nuclear fusion

Joining light nuclei into heavier nuclei with energy release.

92
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Fusion in the Sun

Hydrogen fuses into helium.

93
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Why fusion releases energy

Mass per nucleon decreases.

94
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What is conserved in fission and fusion

Number of nucleons.

95
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Fastest-moving radiation

Gamma.

96
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Scientist who explained nuclear fission

Lise Meitner.

97
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Mass–energy equivalence

E=mc2E = mc^2

98
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Photon energy equation

E=hfE = hf

99
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Wave speed formula

v=fλv = f\lambda

100
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Cause of absorption lines

Atoms absorb specific frequencies of light.