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PHS 111 - Earth Science > Astronomy Test 2 Objectives > Flashcards

Astronomy Test 2 Objectives Flashcards

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1
Q

Relate the color of light to its relative wavelength and energy.

A

red - longer wavelength, less energy

blue - shorter wavelength, more energy

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2
Q

What is the Doppler Effect and what does it reveal about a star?

A

The Doppler Effect is the change in wavelength (and frequency) due to relative motion between the source and the observer. It reveals a star’s motion relative to Earth. -blue shift, red shift; the higher the velocity the greater the shift in position.

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3
Q

Relate the color of a star and the total energy it radiates to its temperature.

A

A hotter star will be brighter with the peak of its radiation toward the blue end of the spectrum. As the temperature increases, more energy is radiated at shorter wavelengths.

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4
Q

If two stars are the same diameter but one is at a temperature of 6,000 K while the other is at 3,000 K, how many times more energy does the hotter star radiate? (Hint: Stefan-Boltzmann Law) If a third star is at a temperature of 9,000 K, how many times more energy does it radiate compared to the 3,000 K star?

A

the total energy radiated by stars goes up a T to the fourth power
2^4=16
3^4=81

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5
Q

Describe stellar parallax and how it can be used to determine the distance to a star.

A

Stellar parallax is the apparent shift in position of the closer stars with respect to the more distant stars due to Earth’s revolution. Photograph a nearby star against the background of distant stars. Then, when Earth has moved halfway around its orbit six months later, the same star is photographed again. Compare the two photos to get the parallax angle which you can use with a base line to calculate the star’s distance.

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6
Q

Describe what is meant by the apparent and absolute magnitude of a star.

A

Apparent magnitude is the brightness of an object as we view it from Earth.
Absolute magnitude is the brightness a star would have at a distance of 32.6 light-years.

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7
Q

What three variables determine the apparent magnitude of a star?

A

distance
temperature
diameter

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8
Q

Given two stars whose magnitudes differ by a factor of 5 (5, 10, 15, etc), determine how many times bright one star is compared to the other.

A

A difference of 5 magnitudes equals 100x difference in brightness.

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9
Q

Describe the difference between apparent magnitude and absolute magnitude and qualitatively describe how they can be used to determine the distance to a star.

A

apparent (m); absolute (M)
If both are known, the distance can be calculated using
d=10(app-abs+5/5) parsecs.

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10
Q

Relate the sizes of the orbits of the stars in a binary system to the stars’ masses.

A

M1d1=m2D2 (like kids on a seesaw)

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11
Q

Given the mass and distance from the barycenter of one star in a binary system and the mass of the second star, calculate the distance of the second star from the barycenter.

A

M1d1=m2D2

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12
Q

List the stellar spectral classes in order and relate them to a star’s temperature and color.

A

Oh Be A Fine Guy Kiss Me
hottest coolest
blue-white yell oran red

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13
Q

Describe the Hertzsprung-Russell diagram.

  • scales
  • giants and supergiants
  • white dwarfs
  • most and least massive stars
  • main sequence stars
  • most luminous stars
  • position of sun on diagram
A

Scales: left y is mag, x is spectral classes, right y is luminosity
Supergiants very top right; giants top right
White dwarfs bottom
most massive top left
least massive bottom right
main sequence stars diagonal
most luminous - giants/supergiants
position of sun - middle of main sequence, luminosity=1, magnitude=4.9

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14
Q

Describe the reasoning used to determine the sizes of giants, supergiants, and dwarf stars from the Hertzsprung-Russell diagram.

A 
Supergiants/giants are very luminous yet have same surface temperature as red stars on main sequence, so they must be large in diameter. 
Dwarf stars are much less luminous than stars in same spectral class on main sequence, so they must be smaller in diameter.
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15
Q

Describe a neutron star and a pulsar.

A

Neutron star is the result of an explosion of a star that was originally more than 8x the mass of the Sun. They are incredibly hot and very dense.
Pulsars are the radio waves emited by the rapidly rotating neutron stars.

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16
Q

Beginning with low mass, medium mass, or high mass stars on the main sequence, list the ending stages in each of their life cycles.

A

low - white dwarfs
medium - planetary nebula with a white dwarf in the center (red giants collapse into white dwarfs which create an expanding spherical cloud of gas)
high - (red supergiant which collapses into) supernova which can result in neutron stars or black holes

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17
Q

List two pieces of data, not their implications, that support the Big Bang model of the universe.

A

galaxies moving away from Earth

radiation - 3 degree cosmic microwave background radiation

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18
Q

What do the red shifts of the galaxies imply about the universe?

A

that the universe is uniformly expanding, which in turn meas at an earlier time the universe was smaller

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19
Q

Arcturus verse

A

Job 38:32; 9:9

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20
Q

Scorpius

A

scorpion

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21
Q

Cygnus

A

swan/northern cross

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22
Q

Sagittarius

A

archer

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23
Q

Lyra

A

lyra

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24
Q

Bootes

A

herdsman

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25
Q

terrestrial planets

A

Mercury
Venus
Earth
Mars

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26
Q

Jovian planets

A

Jupiter
Saturn
Uranus
Neptune

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27
Q

inner planets

A

t

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28
Q

rocky planets

A

ter

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29
Q

have the least mass

A

t

30
Q

have lower densities

A

J

31
Q

have rings

A

J

32
Q

rotate the slowest

A

t

33
Q

have large numbers of satellites

A

J

34
Q

have the greatest polar flattening

A

J

35
Q

Has the Great Dark Spot

A

Neptune

36
Q

has the greatest temperature extremes

A

Mercury

37
Q

has a surface like a rocky desert on Earth

A

Mars

38
Q

its moon, Io, is the most volcanically active in the solar system

A

Jupiter

39
Q

has the “Great Red Spot”

A

Jupiter

40
Q

atmosphere is about 1% of earth’s

A

Mars

41
Q

most prominent ring system

A

Saturn

42
Q

rotates the fastest

A

Jupiter

43
Q

one day-night lasts 176 Earth days

A

Mercury

44
Q

is about half the size of the Earth

A

Mars

45
Q

it’s largest moon, Triton, exhibits cryovolcanism

A

Neptune

46
Q

average surface temperature is about 900 degrees Farenheit

A

Venus

47
Q

Uranus’s “twin”

A

Neptune

48
Q

its moon Titan has methane “rain”

A

Saturn

49
Q

has canyons bigger than the Grand Canyon

A

Mars

50
Q

has wind speeds > 1500 mph

A

Neptune

51
Q

has extensive dust storms

A

Mars

52
Q

has a thick atmosphere of carbon dioxide

A

Venus

53
Q

rotates like a rolling ball

A

Uranus

54
Q

has four “Galilean” moons

A

Jupiter

55
Q

a dwarf planet

A

Pluto

56
Q

has Olympus Mons, the largest volcano in the solar system

A

Mars

57
Q

asteroid belt location

A

between Mars and Jupiter

58
Q

largest known object in asteroid belt

A

Ceres

59
Q

There are only _ asteroids larger than 400 km in diameter.

A

5

60
Q

Comets often referred to as

A

dirty snowballs

61
Q

Short period comets orbit beyond Neptune in a region called the

A

Kuiper belt

62
Q

most famous short-period comet

A

Halley’s Comet

63
Q

Long period comets are located in a spherical shell around the solar system called the

A

Oort cloud

64
Q

three parts of a comet

A

nucleus, coma, tail

65
Q

What would be expected if Earth were to pass through the orbit of a comet?

A

Earth would get meteor showers.

66
Q

three most common types of meteorites

A

irons
stony
stony-irons

67
Q

most notable crater in US produced by a meteoroid

A

Meteor Crater in Arizona

68
Q

Tail of comet always points ________ the Sun.

A

away from

69
Q

The moon Charon is a satellite of

A

Pluto

70
Q

Comets (gain, lose) material with every pass around the Sun.

A

lose

71
Q

Terrestrial planets have

Jovian planets have

A

long days, short years

short days, long years

PHS 111 - Earth Science (9 decks)

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