ASTRO C10 Midterm #1

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104 Terms

1
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What is light?

Light is electromagnetic radiation—energy that travels as waves of electric and magnetic fields.

2
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What are the main types of electromagnetic waves (from shortest to longest wavelength)?

Gamma rays → X

3
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What determines a light wave’s color or type?

Its wavelength (or equivalently, its frequency).

4
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What is the relationship between wavelength, frequency, and energy?

Shorter wavelength → higher frequency → higher energy.

5
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What is a photon?

A particle of light that carries energy proportional to its frequency (E = h·f).

6
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What is absorption?

When atoms absorb specific wavelengths of light, moving electrons to higher energy levels.

7
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What is emission?

When electrons fall to lower energy levels and emit light at specific wavelengths.

8
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What are absorption and emission spectra?

Absorption: dark lines in a continuous spectrum. Emission: bright lines at specific wavelengths. Each element has a unique spectral “fingerprint.”

9
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What does a continuous spectrum come from?

Hot, dense objects (like incandescent solids or liquids) emitting all wavelengths.

10
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What does an absorption spectrum come from?

A hot light source passing through a cooler gas that absorbs certain wavelengths.

11
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What does an emission spectrum come from?

A thin, hot gas emitting only specific wavelengths.

12
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What is the Doppler effect in astronomy?

The change in wavelength (or frequency) of light from a moving source.

13
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What does redshift mean?

The object is moving away; wavelengths stretch longer (shift toward red).

14
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What does blueshift mean?

The object is moving toward us; wavelengths shorten (shift toward blue).

15
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What does the Doppler effect tell us about stars or galaxies?

Their radial velocity—how fast they’re moving toward or away from us.

16
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What is thermal radiation?

The electromagnetic energy emitted by any object with a temperature above absolute zero.

17
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What does Wien’s Law state?

Hotter objects emit light at shorter peak wavelengths (λmax ∝ 1/T).

18
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What does the Stefan

Boltzmann Law state?

19
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What happens to color as temperature increases?

Objects go from red → orange → yellow → white → blue as they get hotter.

20
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What limits telescope resolution?

Diffraction (depends on wavelength and aperture) and atmospheric turbulence.

21
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Why do astronomers use space telescopes?

To avoid atmospheric distortion and to observe wavelengths (like UV, X

22
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What causes lunar phases?

The Moon’s changing position relative to Earth and the Sun; we see different portions of its illuminated half.

23
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Order of the main lunar phases?

New Moon → Waxing Crescent → First Quarter → Waxing Gibbous → Full Moon → Waning Gibbous → Last Quarter → Waning Crescent.

24
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What causes eclipses?

The alignment of the Sun, Earth, and Moon (in a straight line).

25
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Why don’t eclipses happen every month?

The Moon’s orbit is tilted ~5° relative to Earth’s orbit, so alignment only occurs occasionally.

26
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What are the three main phases of a solar eclipse?

Partial phase → Diamond Ring → Totality.

27
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What is the corona?

The Sun’s faint outer atmosphere, visible only during totality.

28
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What is the diamond ring effect?

A brief flash of sunlight seen just before or after totality when one last bright spot of photosphere is visible.

29
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What is an annular eclipse?

When the Moon is too far from Earth to cover the Sun completely, leaving a “ring of fire.”

30
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Why do total solar eclipses appear so perfect?

The Sun is about 390× larger than the Moon but also about 390× farther away—so they appear the same size.

31
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How often does a total solar eclipse occur at a given location?

Roughly once every 300–400 years.

32
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What causes Earth’s seasons?

The 23.5° tilt of Earth’s axis, not distance from the Sun.

33
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What happens during an equinox?

Day and night are equal everywhere; occurs around March 22 and September 22.

34
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What happens during a solstice?

One hemisphere is maximally tilted toward or away from the Sun, producing the longest or shortest day.

35
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How does the Coriolis effect influence weather?

Causes rotating systems (like hurricanes) to spin counterclockwise in the Northern Hemisphere and clockwise in the Southern.

36
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What is different about the sky between hemispheres?

Star rotation direction, Moon orientation, and visible constellations (e.g., Orion appears upside down).

37
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What is retrograde motion?

The apparent backward motion of planets against the stars, caused by Earth overtaking them in orbit.

38
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Describe Aristotle’s model of the solar system.

Geocentric; planets move in perfect spheres around Earth.

39
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Describe Ptolemy’s model of the solar system

Geocentric; used epicycles and deferents to explain retrograde motion.

40
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Describe Copernicus’ model.

Heliocentric; planets orbit the Sun, naturally explaining retrograde motion.

41
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What is Kepler’s 3rd law (simplified)?

P^2 = a^3

42
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What does Kepler’s 3rd law help determine?

The masses of celestial bodies (e.g., Sun, Earth, Jupiter).

43
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How did the planets form?

Dust → pebbles → planetesimals → planets; leftover gas blown away by solar winds.

44
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What causes tides?

Differential gravitational pull of the Moon (and Sun) across Earth.

45
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Why are there two high tides per day?

One on the side facing the Moon and one on the opposite side.

46
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What causes the Ring of Fire?

Tectonic plate boundaries with high volcanic and earthquake activity.

47
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Why is the Moon heavily cratered while Earth isn’t?

Earth’s erosion and plate tectonics erase old craters; the Moon lacks both.

48
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What are lunar maria?

Dark basaltic plains from ancient lava flows filling impact basins.

49
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How do we determine the relative age of lunar surfaces?

More craters = older surface.

50
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What is the Giant Impact Hypothesis?

The Moon formed from debris after a Mars

51
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Why is Mercury’s temperature extreme?

It has almost no atmosphere to distribute or retain heat.

52
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How is Mercury similar to the Moon?

Heavily cratered surface, no tectonic activity, no atmosphere.

53
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Why is Venus the brightest planet?

It’s close to Earth and has highly reflective sulfuric acid clouds.

54
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Why is Venus hotter than Mercury?

Thick CO₂ atmosphere traps heat via a runaway greenhouse effect.

55
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What is the main gas in Venus’s atmosphere?

Carbon dioxide (96%).

56
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What evidence suggests active volcanism on Venus?

Fluctuating sulfur dioxide levels and radar images showing possible lava flows.

57
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Why doesn’t Earth experience a runaway greenhouse effect?

Earth’s CO₂ is mostly stored in oceans and rocks; natural carbon cycles regulate it.

58
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What is the main driver of modern climate change?

Human

59
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How does the greenhouse effect work?

Visible light heats Earth’s surface; infrared radiation is trapped by greenhouse gases, warming the planet.

60
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What is light?

Light is electromagnetic energy that travels in waves at a constant speed (3 × 10⁸ m/s in a vacuum).

61
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What are the main types of electromagnetic radiation?

Radio, microwave, infrared, visible, ultraviolet, X

62
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What determines a light wave’s energy?

Its frequency — higher frequency means higher energy (E = hf).

63
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What is wavelength?

The distance between wave peaks; longer wavelengths have lower energy..

64
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How do astronomers use the Doppler effect?

To measure how fast stars and galaxies move toward or away from us and to detect exoplanets through small periodic shifts in a star’s light.

65
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What is the Doppler wobble method?

Detecting a star’s slight “wobble” caused by an orbiting planet’s gravitational pull.

66
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What is thermal radiation?

Light emitted by any object with a temperature above absolute zero.

67
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What does Wien’s Law tell us?

Hotter objects emit light at shorter (bluer) wavelengths (λₘₐₓ = constant / T).

68
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What does the Stefan

Boltzmann Law tell us?

69
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What is a blackbody?

An idealized object that absorbs all light and emits a predictable spectrum depending only on temperature.

70
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What determines a telescope’s light

gathering power?

71
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What determines a telescope’s resolution?

The ratio λ/D — shorter wavelengths and larger diameters give sharper images.

72
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What limits resolution on Earth?

Atmospheric turbulence blurs images (seeing conditions).

73
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What is a refracting telescope?

Uses lenses to bend (refract) light to a focus; suffers from chromatic aberration.

74
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What is a reflecting telescope?

Uses mirrors to focus light; avoids chromatic aberration and can be built larger.

75
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What does Kepler’s First Law state?

Planets orbit the Sun in ellipses, with the Sun at one focus.

76
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What does Kepler’s Second Law state?

A line from the planet to the Sun sweeps out equal areas in equal times — planets move faster when closer to the Sun.

77
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What does Kepler’s Third Law state?

P^2 = R^3, the farther a planet is from the Sun, the longer its orbital period.

78
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What does Newton’s First Law state?

An object in motion stays in motion unless acted upon by a force.

79
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What does Newton’s Second Law state?

F = ma — force equals mass times acceleration.

80
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What does Newton’s Third Law state?

Every action has an equal and opposite reaction.

81
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What is the Law of Universal Gravitation?

F = Gm₁m₂ / d² — gravitational force increases with mass and decreases with distance squared.

82
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How does gravity produce an orbit?

Gravity constantly pulls an object toward the planet, but its forward motion makes it “fall around” — it keeps missing, forming an orbit.

83
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What are terrestrial planets?

Mercury, Venus, Earth, and Mars — small, rocky, dense, few moons.

84
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What are giant (Jovian) planets?

Jupiter, Saturn, Uranus, Neptune — large, gaseous, low density, many moons and rings.

85
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What is the “snow line”?

The boundary in the early solar nebula beyond which ices could form; separates terrestrial and giant planets.

86
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What is the Roche limit?

The distance within which a moon or object is torn apart by a planet’s tidal forces (explains Saturn’s rings).

87
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What are comets made of?

“Dirty iceballs” of rock and frozen gases that sublimate when near the Sun, forming tails that point away from it.

88
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What is a periodic comet?

A comet that orbits the Sun repeatedly (returns at regular intervals).

89
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Where do most comets come from?

The Kuiper Belt and the distant Oort Cloud.

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What are asteroids?

Rocky remnants mostly found between Mars and Jupiter in the asteroid belt.

91
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What is a meteor?

A “shooting star” — a meteoroid burning up in Earth’s atmosphere.

92
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What is a meteorite?

A fragment of a meteoroid that survives passage through the atmosphere and lands on Earth.

93
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What is an exoplanet?

A planet orbiting a star outside our solar system.

94
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What is the Doppler wobble method?

Detects periodic shifts in a star’s light due to the gravitational pull of an orbiting planet.

95
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What is the transit method?

Detects small dips in starlight when a planet passes in front of its star.

96
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What can spectra during transits reveal?

The composition of an exoplanet’s atmosphere by analyzing which wavelengths are absorbed.

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What did the Kepler Space Telescope discover?

Thousands of exoplanets — found that small, Earth

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What is the “Goldilocks Zone”?

The habitable zone where conditions are just right for liquid water.

99
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Why does the Sun look red at sunset?

Earth’s atmosphere scatters shorter blue light, leaving red/orange light.

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What would happen if Earth had no axial tilt?

There would be no significant seasonal changes.