AS103 Astronomy Final Exam

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193 Terms

1
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how does the use of the word “theory” differ from its everyday use?

science: theory is tested and reliable set of ideas. Everyday: a guess

2
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what does it mean to say that a theory should be “falsifiable” as opposed to being “proveable”

a theory must make testable predictions, which may be wrong. But it cannot “prove” unless all possible solutions have been tested

3
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why do we see things in the night sky as they were in the past, instead of right now and why doesn’t this matter in daily life?

things are light years away and takes a long time for their light to reach us. It doesn’t matter in daily life because the amount of time that has passed is not very significant

4
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how many total constellations are there

88

5
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what do we call the 12 constellations the sun travels through

zodiac constellations

6
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an astronomer thinks of a constellation not as a stick figure but as what?

an area of the sky

7
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what point on the meridian do the constellations rotate around

NCP for us (or Polaris)

8
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which way is the moon’s orbital motion

it orbits in the same sense as the Earth’s rotation

9
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what naked eye observation led to the development of solar system models in the first place

the retrograde motion (or any motion), “wanderers”

10
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Early (Ptolemaic) models put what object at the center

Earth at the center

11
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Later (Copernican) models put what object at the center

Sun at the center

12
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is the celestial sphere we used in lab Ptolemaic or Copernican model?

Ptolemaic (geocentric) model

13
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the same force applied to both the Earth and the Moon produces very different accelerations. What is the reason for this difference?

larger mass = smaller acceleration. (F = ma)

14
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equation that relates the initial and final energies of the system (photon emission)

conservation of energy: E initial = E final (example: E3 = E + E2)

15
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description of an equatorial mount

declination can be fixed, telescope turns to follow objects in the sky.

16
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Advantages of equatorial mount

easier to take pictures and easier to follow objects in the sky

17
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advantages of alt az mount

strong

18
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description of alt az mount

axes parallel/perpendicular and zenith aligne

19
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what is the universality of physical law

physics laws observed on Earth are assumed to be the same everywhere

20
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Why do you see stars in the past

very far distance, light years away.

21
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distance angle formula

D = 2πd(α/360)

22
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time for light to reach somewhere formula

T = d/c

23
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What causes the diurnal motion of the stars and constellations across the night sky?

Earth’s daily rotation

24
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What causes different constellations to appear at night in different seasons?

orbit (revolution) of Earth around the Sun

25
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What causes seasons?

inclination of Earth’s spin (rotation) axis from direction perpendicular to the plane of the orbit (23.5)

26
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why are you more likely to see a lunar eclipse than a solar?

Solar is along a narrow path and lasts a few mins. Lunar is visible for hours from entire night side of the Earth

27
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Why don’t we get an eclipse every new/full moon?

Earth, Moon, Sun must align both in the plane of Earth’s orbit and perpendicular to the plane. (line of nodes) Also: shape, tilt, and orbit are not perfect.

28
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what does it mean to say the moon orbits synchronously with respect to Earth?

The orbital and rotational periods are the same

29
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What is one piece of evidence that ancient astronomers had that the Earth is a sphere?

gradual disappearance of ships hull with distance. Varying height of pole star with geographic location. shadow edge on Moon during lunar eclipse

30
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Solar eclipse diagram

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31
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lunar eclipse diagram

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32
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why don’t we have eclipses all the time (diagram)

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33
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diagram showing synchronously orbits

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34
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horizon label diagram

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35
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diagram showing solstices and equinoxes

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36
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moon phases diagram

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37
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Why do we say that astronomy often deals in extremes?

the universe has extreme temps, distances, energy

38
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Why is it so important to understand the properties of light?

to be able to calculate distances

39
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What force is most important on astronomical scales?

gravity

40
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why the moon always shows the same face to Earth.

synchronous rotation. moon rotates once each time it orbits the Earth

41
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celestial sphere diagram

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42
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what does right ascension correlate with

longitude

43
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what does declination correlate with

latitude

44
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difference between solar and sidereal day

solar is 4 minutes longer. solar based on sun getting from high to high point in day. sidereal based on certain star crossing meridian.

45
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Planets’ orbits are

elliptical with the sun at a focus

46
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The line between a planet and the sun sweeps out

equal areas in equal times

47
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A complete orbit has P^2 = a^3, where P and a represent

sidereal orbital motion (yr) and semi major axis (Au) (conservation of angular momentum)

48
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Newton’s first law

an object’s velocity will remain constant if there is no net external force acting on it

49
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Newton’s second law: the acceleration of, mass of, and net force on an object are related as (equation) 

acceleration = net force / mass (F = ma)

50
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Newton’s third law

the action and reaction forces between two bodies are equal in magnitude and opposite in direction. ΣF12 = -F21

51
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Why do we say that an object traveling at constant speed on a circle is accelerated, even though its speed is not changing?

its direction of motion is changing. acceleration is a change in velocity and velocity is speed and direction

52
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SB law says

total emission is proportional to T^4

53
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Wien’s law says

different temperatures peaks at a wavelength is inversely proportional to the temperature

54
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What is special about the Kelvin/absolute scale?

kelvin has zero temperature at minimum molecular kinetic energy. As cold as you can get. Energy is proportional to temperature. (more convenient)

55
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What is conservation of energy

initial energy = final energy

56
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Equation that relates initial and final energy of system (e- jumps from level 3 to level 1)

E1 + E = E3

57
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Why is it possible to use the emission/absorption spectra of atoms to identify what element the atoms are?

the spectra (the photons) are unique to each element or chemical compound

58
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What is the biggest obstacle to Earth-bound viewing in astronomy?

the atmosphere

59
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Why are telescopes placed in high locations?

to get above some of the atmosphere. (less absorption)

60
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Why are telescopes placed in remote locations?

darker, less light pollution (reflection)

61
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What are two main types of telescope mounts

Altitude-azimuth, equatorial

62
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How is alt-az aligned

zenith aligned

63
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How is equatorial mount aligned

polar aligned

64
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Which mount can carry the most weight

altitude-azimuth

65
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Which mount is easier to use for taking pictures

equatorial

66
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Rank eye, photo film, CCD based on sensitivity, linearity, data analysis

poor: eye, good: film, excellent: CCD

67
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If you increase the diameter of telescope 3 times, by what factor does the image brightness change

  1. B α D^2 … B’/B = (3D)^2 / (D)^2 = 9

68
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If you increase the diameter of telescope 3 times, by what factor does the image resolution change

  1. R α D … R’/R = 3D/D = 3

69
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Rank the importance of magnification, brightness, and resolution

brightness=1, resolution=2, magnification=3

70
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Is magnification improved by a larger diameter?

no

71
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Is brightness improved by a larger diameter?

yes

72
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Is resolution improved by a larger diameter?

yes

73
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Mathematical relation to diameter (magnification)

none (D^0)

74
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Mathematical relation to diameter (brightness)

D^2

75
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Mathematical relation to diameter (resolution)

D^1

76
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Which telescope (reflector or refractor) performs better with construction

reflector

77
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Which telescope (reflector or refractor) performs better with spherical aberration

they perform the same

78
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Which telescope (reflector or refractor) performs better with chromatic aberration

reflector

79
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Which telescope (reflector or refractor) performs better with atmospheric transmission

they perform the same (relates to location)

80
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Which telescope (reflector or refractor) performs better with light pollution

they perform the same (relates to location)

81
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Why do we sometimes speak of light as rays and sometimes as "electromagnetic waves"?

they can behave as particle and have magnetic field. Light travels in a straight line

82
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Why do we have to use the absolute temp scale in describing blackbody radiation

because this scale is based on thermal energy

83
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What are the two processes used by lenses and mirrors to focus light and create an image?

reflect and refract

84
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What countermeasures can we employ against things that make for poor viewing

high, dry, and dark places

85
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parts of a wave diagram

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86
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Electromagnetic spectrum diagram

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87
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blackbody diagram

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88
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photon emission/absorption diagram

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89
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equal areas equal times diagram

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90
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object traveling around sun diagram

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91
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object traveling in a circle diagram

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92
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diagram of refractor

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93
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diagram of reflector

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94
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equation relating wave speed (v), frequency (f), and wavelength (lambda)?

v = f * λ

95
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Terrestrial planets location (inner/outer)

inner

96
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Terrestrial planets density (high/low)

high

97
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Terrestrial planets mass (high/low)

low

98
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Terrestrial planets overall composition (light/heavy)

heavy

99
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Terrestrial planets moons (many/few)

few

100
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jovian planets location (inner/outer)

outer