ESSC 102 Unit 3 Mini Test (Dr.Welch, SELU)

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124 Terms

1
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______ is our ONLY source of information for distant objects (the broader universe)

Light

2
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What is light?

an electromagnetic wave that behave like a particle

3
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Nothing travels faster than the speed of

light

4
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Repeat distance

Wavelength

5
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Visible light has ___ wavelengths

small

6
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Frequency is measured in

Hertz

7
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The speed of light in a vacuum is

300,000 km/s

8
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The formula for speed of light is?

Wavelength x frequency

9
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Colors to which the human eye is sensitive is referred to as the ______ with the color determined by the lights ______

visible light spectrum, wavelength

10
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The longest visible wavelength

Red, 700nm

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The shortest visible wavelength

Violet 400nm

12
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Electromagnetic Spectrum is made up of

radio waves, microwaves, infrared gamma rays, UV rays, x rays

13
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Shortest wavelength in the Electromagnetic Spectrum is

gamma rays

14
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What are ways light interacts with matter?

Emission, Absorption, Transmission, Reflection/Scattering

15
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Stars __ light

emit

16
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An example of lights interaction with matter determining what we see is the answer to "Why is the Earth blue?'

The Earth's atmosphere scatters blue light more effectively than red light because blue wavelengths are shorter

17
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The sun appears red at sunset because?

The sun is at a different angle to the blue light is reflected through space instead of through the earth

18
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Passing light through a prism makes a

Spectrum

19
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The word spectrum means

Phantom in Latin

20
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You can learn more about an object when it has a _____ and ______

emission line and absorption line

21
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When passing light through a prism, you can notice what in the spectrum?

the missing elements

22
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Hot objects produce a

continuous spectrum

23
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What is a continuous spectrum?

light emitted at all wavelengths

24
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What is created when atoms in gas absorb light if certain wavelengths producing lines in the spectrum

absorption line spectrum

25
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What is created when atoms in a gas cloud reemit absorbed light energy at the same wavelengths at which they absorbed it?

Emission line spectrum

26
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We can determine what things from the light of an object?

Chemical composition, temperature, and doppler motion

27
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When matter is heated, electrons move _____ levels

energy

28
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Electrons moving either up or down energy levels creates a unique

spectral fingerprint

29
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A spectral fingerprint is expressed as _____ and _____ lines in an object's spectrum

emission and absorption

30
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Temperature and ____ correlate

color

31
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What color is the coolest?

red

32
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As you increase the temperature of an object the wavelength gets

shorter

33
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Wien's law states

increasing temperature decreases wavelength

34
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Absolute 0 on the Kelvin scale means

the particles have completely quit moving

35
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The sun supposedly can reach up to

15 million Kelvin

36
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When matter becomes so hot, the particles are no longer repulsed by each other because they are moving so fast they can slam into each other and become

one

37
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Short wavelength have a _____ pitch

higher

38
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Long wavelength have a _____ pitches

lower

39
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Redshift occurs when an object is moving ______ from you

away

40
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Blue shift occurs when an object is moving _____ you

toward

41
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If we could see an asteroid crashing into earth it would be

blue shift

42
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If we could see an asteroid moving away from earth it would be

red shift

43
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The light from all other galaxies in the universe outside of the milkyway is red shifted meaning

the galaxies are moving away from us

44
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A light year is a unit of

distance NOT time

45
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Speed of light is

300,000 km/s

46
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The sun is _____ away from earth

8.3 light MINUTES

47
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The moon is _____ away from earth

1.3 light SECONDS

48
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We can only ever see how the sun looked

8 minutes ago

49
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The further we look away from our planet, the further we

travel back in time

50
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We cannot see more than 13.7 billion light years away from earth because we would be looking back to

before the universe was formed

51
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The most important thing a telescope can do is

collect more light than your eyes

52
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Telescopes use _______ or _______ to focus light

mirror, lenses

53
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What is needed for Collecting Power of a telescope?

Light

54
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What is needed for Focusing Power of a telescope?

Mirrors or Lenses

55
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What is needed for Resolving Power of a telescope?

Lenses and Magnification

56
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________ telescopes are better

Reflecting

57
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________ telescopes take light from a distant object and bend in down to your eye piece

Refracting

58
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Refracting telescopes are best for objects that

produce their own light

59
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_________ telescopes collect more light and bounce them down to your eyepiece off of mirrors

Reflecting

60
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Why do we put telescopes in space?

To avoid light pollution, to avoid turbulence/twinkling, and because our atmosphere absorbs most of the electromagnetic spectrum

61
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Light from stars twinkle because

it has to make its way through our moving atmosphere

62
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Telescopes are NOT put in space to be closer to the stars, the whole point is to

get away from our atmosphere

63
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Cold gas clouds radio in the ____ waves

radio

64
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Dust clouds radiate in the _____ waves

infrared

65
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Hot gasses around black holes emit _____ waves

x rays

66
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We can see a lot of the galaxy by being able to detect

the non visible wavelengths

67
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Hubble telescope is pretty much just

a ground base telescope, but better

68
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EVE captures ____ light

UV

69
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Spizer captures

heat/infrared

70
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Chandra captures

X rays

71
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James Webb Telescope 2018 will work in ____ and produce ____

infrared, optical pictures

72
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Hubble telescope has been in space since

the early 2000s

73
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The sun is very similar to

all the other stars in the universe

74
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Our sun is just special to us because

it is closest to us

75
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Our sun is just

a ball of hot gas bound by gravity

76
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Our sun is made of

hydrogen and helium and trace amount of other elements like calcium and potassium

77
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What keeps our sun going?

fusion

78
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Every second our sun converts 600 million tons of Hydrogen into 596 million tons of Helium, that missing 4 million of material

powers and heat ours planet and solar system

79
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Our sun shines not because it is on fire, but because it is powered by

nuclear energy FUSION

80
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Atomic number

number of protons in nucleus

81
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Atomic Mass

number of protons and neutrons in nucleus

82
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Taking protons and neutrons in the nucleus of an item and combining them to make something bigger

Fusion

83
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Splitting the atom

fission

84
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The atomic bomb is

fission

85
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Our sun uses what (fusion or fission)

Fusion

86
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Our sun is a ____ mass star

low

87
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Proton Proton Chain

fusing four hydrogen nuclei into one Helium nuclei

88
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What does the equation of Proton Proton Chain look like?

4H =>1 He + energy

89
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We can figure out the rate of fusion in our sun by counting

neutrinos

90
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CNO cycle

high mass main sequence stars fuse H to He at a higher rate using Carbon, Nitrogen, and Oxygen as catalysts/fuel (runs out of fuel faster)

91
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Our sun is stable because of

fusion which pushes out on the gravity

92
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Gravity and Fusion create ____ with our sun

gravitational equilibrium

93
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A flow of charged particles from the surface of the sun

Solar Wind

94
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Outermost layer of the Sun's atmosphere

Corona

95
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Middle layer of the sun's solar atmosphere that is the first part in the visible light spectrum

Chromosphere

96
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Visible surface of the sun, 5,800K

Photosphere

97
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Why is the sun yellow?

because the surface/Photosphere is 5,800K

98
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Energy is transported upward by rising hot gas

Convection Zone

99
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Energy Transported upward by photons

Radiation Zone

100
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10% most centralized part of the sun and is the hottest, energy generated by nuclear fusion 15 million K

Core