15-16 Flashcards

1
Q

Most of the light that makes the hazy band of the “milky way” visible in the night sky comes from
reflection and emission nebulae

A

False

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2
Q

William and Caroline Herschel attempted to make a map of the Milky Way galaxy by counting the
number of stars visible in different directions

A

true

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3
Q

Harlow Shapley used observations of globular clusters to determine the position of the center of the galaxy.

A

true

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4
Q

Globular clusters are used as spiral tracers.

A

false

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5
Q

Stars in the central bulge of the galaxy follow elongated orbits tipped steeply to the plane of the disk

A

true

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6
Q

The central bulge and the galactic disk of the Milky Way are often referred to as its spherical
component

A

false

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7
Q

Spiral arms are clearly visible features of galaxies because most sun-like stars in the disk are found
there

A

false

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8
Q

O and B stars are important spiral tracers

A

True

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9
Q

A “grand-design” galaxy contains clear spiral arms with few spurs

A

true

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10
Q

The center of the galaxy has been studied extensively using visible light

A

false

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11
Q

The mass of the black hole in the center of the galaxy has been determined by observing the motion of stars orbiting it

A

True

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12
Q

The black hole at the center of our galaxy is too large to be the remnant of a single star

A

True

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13
Q

The first stars formed in the Universe were composed of 90% hydrogen, 10% helium, and very little
else

A

true

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14
Q

Stars that formed in the very early stages of our galaxy’s formation have high amounts of “metals.”

A

False

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15
Q

Population I stars are younger than Population II stars

A

True

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16
Q

William and Caroline Herschel’s map included four of the following hypotheses in their model of the
galaxy. Which one was the exception?

A

They provided accurate measurements of the distances to stars.

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17
Q

What property of a Cepheid variable can you determine if you know its period

A

absolute magnitude

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18
Q

Based on Shapley’s determination of the center of the galaxy, the Sun is located ____

A

in the middle portion of the galactic disk

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19
Q

The accompanying graph above clearly shows that ____

A

Type I Cepheid variables are always brighter than Type II Cepheids

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20
Q

Examine the accompanying graph. Harlow Shapley did not know that there are two categories of Cepheid variables; he was only familiar with those such as δ Cepheii. Because of this, some of the
Cepheid variables he observed ____

A

were dimmer than expected

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21
Q

Which object would be absent in the galactic halo?

A

emission nebula

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22
Q

The Sun orbits the center of the galaxy about once every ____

A

200,000,000 years

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23
Q

In which area of the galaxy would you find stars with fairly circular orbits about the galactic center

A

disk

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24
Q

Almost all of the gas and dust in the Milky Way is located in the ____

A

disk

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25
Q

The mass of the Milky Way galaxy is a few ___

A

hundreds of billions of solar masses

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26
Q

The following objects are found in a spiral arm of a galaxy. Which is the exception

A

population II stars

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27
Q

O stars must be formed in spiral arms because _____.

A

they do not live long enough to move out of the arm

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28
Q

When you plot the position of sun-like stars, you will find that __

A

Sun-like stars are found in and out of spiral arms

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29
Q

When you plot the position of sun-like stars, you will find that __

A

Sun-like stars are found in and out of spiral arms

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30
Q

“Spurs” are probably the result of ____

A

self-sustaining star formation

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31
Q

Why is it surprising that spiral arms are stable structures, lasting billions of years

A

Differential rotation should tear the arms apart.

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32
Q

Spiral density wave theory and self-sustaining star formation are ways to explain why ____

A

molecular clouds are compressed forming young stars along spiral arms

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33
Q

The center of the Milky Way galaxy is in the direction of the constellation ____

A

Sagittarius

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34
Q

. The center of our galaxy contains a very intense source of radio and X-ray radiation named Sgr A*.
What is it about this source that supports the idea that the radiation comes from a black hole

A

The radiation is coming from an incredibly small object.

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35
Q

Why is it so difficult to study the center of our galaxy

A

​Interstellar dust blocks almost all light before it reaches Earth.

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36
Q

. The best explanation for the activity at the center of the galaxy is a(n) ____.

A

​black hole with a mass several million times the Sun’s

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37
Q

. Which statement about stellar populations is correct

A

Population I stars are found in the disk; Population II stars are found in the bulge and halo.

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38
Q

Elements above hydrogen and helium come from _____.

A

the last phases of stellar evolution and stellar “death

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39
Q

What is the correct ordering of galactic components using the new bottom-up hypothesis starting from
oldest to youngest

A

galactic halo, average globular clusters, galactic disk

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40
Q

One of the most important features that must be explained by models during the formation of the
galaxy is the ____.

A

differences in age and metallicity of stars, especially in the hal

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41
Q

What is the monolithic collapse hypothesis unable to explain?

A

The elongated bar shape of the central bulge

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42
Q

_______________ variable stars are useful in measuring the distance to globular clusters.

A

Cepheid

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43
Q

In the late 18th century, two astronomers, both with the last name of _______________, were the first
to attempt to map the shape of the galaxy.

A

Herschel

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44
Q

An astronomer named _______________ used globular clusters to locate the center of the galaxy.
(enter last name only

A

shapley

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45
Q

The galactic _______________ contains very little gas and dust, old stars, and globular clusters.

A

halo

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46
Q

Stars at different distances from the galactic center revolve with different periods, an effect called
_______________ rotation

A

differential

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47
Q

O and B stars only occur in the galactic_____

A

disk

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48
Q

Objects used to map spiral arms are called spiral _______________.

A

tracers

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49
Q

. A partial, or detached, segment of a spiral arm is referred to as a(n) “ _______________.

A

spur

50
Q

Sgr A* has been heavily studied using _______________ interferometry.

A

radio

51
Q

Astronomers refer to elements heavier than helium as _______________

A

metals

52
Q

Elliptical galaxies contain a mix of old and young stars

A

false

53
Q

When spiral nebulae were first discovered, astronomers quickly identified them as distant groupings of stars

A

false

54
Q

Spiral and irregular galaxies have active star formation

A

true

55
Q

The diameter and luminosity of a galaxy do not determine its type

A

true

56
Q

A standard candle is an object with a known luminosity

A

true

57
Q

Globular clusters can be used to measure the distance of nearby galaxies

A

true

58
Q

Hubble’s Law is only effective in measuring the distance to nearby galaxies.

A

false

59
Q

All elliptical galaxies are more massive than the largest spiral galaxies

A

false

60
Q

Galaxies contain 10 times as much dark matter as visible matter

A

true

61
Q

Giant spirals are the largest galaxies in the Universe.

A

false

62
Q

Gravitational lensing can be used to detect the presence of dark matter

A

true

63
Q

Starburst” events are a common outcome of galactic collisions

A

true

64
Q

The Milky Way galaxy has collided with several other large galaxies in its lifetime

A

false

65
Q

Gentle gravitational tidal forces appear to be necessary to create spiral arms.

A

true

66
Q

The farthest galaxies that astronomers have seen are all elliptical galaxies

A

false

67
Q

The identification of “spiral nebulae” as large groupings of stars outside of our own galaxy was proven
by ____

A

photographic plates made by Edwin Hubble showing stars and Cepheid variables

68
Q

In which of the following types of galaxies would you expect to find active star formation

A

spiral and irregular

69
Q

Which types of galaxies lack an ordered structure of stellar orbits

A

irregular galaxies only

70
Q

Which types of galaxies would contain very little gas and dust

A

elliptical galaxies

71
Q

NASA’s Hubble Deep Field images and GOODS program observations have shown that ____

A

​the entire sky is thickly covered with galaxies.

72
Q

The structure of most galaxies is most apparent using near-infrared images that show the locations of
____

A

cool-low luminosity stars

73
Q

in general

A

​most cataloged galaxies are spiral, but elliptical galaxies are the most common.

74
Q

Cepheid variables are useful in measuring the distance to ____

A

galaxies that are within 30 megaparsecs, a relatively short distance

75
Q

Globular clusters can be used to estimate the distance to galaxies by measuring the clusters’ ____.

A

angular diameter

76
Q

An astronomer would find a type Ia supernova in a distant galaxy useful as a(n) ____

A

standard candle

77
Q

Cepheids and globular clusters are limited in their ability to measure the distance to galaxies because
they ____.

A

are not bright enough to detect at large distance

78
Q

Edwin Hubble and Milton Humason discovered that there was a linear relationship between a galaxy’s
____.

A

velocity and distance

79
Q

The Hubble law is one of the most important relations in modern astronomy because it ____

A

allows astronomers to measure the distance to very distant galaxies using only their
spectrum

80
Q

Because the Hubble constant has a value of 70 km/s/Mpc, a galaxy 100 Mpc away would have a
recession velocity of ____

A

7,000 kms

81
Q

Because the Hubble constant equals 70 km/s/Mpc, a galaxy with a recession velocity of 4,900 km/s
would be a distance of ____ Mpc from Earth.

A

70

82
Q

In order to calculate the size and luminosity of a galaxy, you must first determine its ____

A

distance

83
Q

Compared to other spiral galaxies, the Milky Way is ____

A

larger and brighter than most spirals

84
Q

The range of diameters and luminosities displayed by elliptical galaxies is ____

A

​wider than the range for spirals

85
Q

The rotation curve of a galaxy is important in determining the galaxy’s ____

A

mass

86
Q

The ____ depend(s) on the assumption that the mass of a galaxy or galactic cluster is large enough to
keep moving matter bound to the main structure

A

velocity dispersion and cluster methods

87
Q

Dark matter is detectable in the coronae of ____

A

all galaxies

88
Q

A key piece of evidence that leads astronomers to conclude that most galaxies include a supermassive
black hole in the center is that ____

A

stars near the center of other galaxies are orbiting more rapidly than expected

89
Q

A supermassive black hole in the center of a galaxy typically represents ____ of the galaxy’s total
mass.

A

A tiny fraction of a percent

90
Q

The mass of visible matter in a galaxy can be estimated by measuring its luminosity. When this is
compared with the measured mass of the galaxy, astronomers find that ____.

A

the measured mass is about ten times the estimated mass, due to the effects of dark matter

91
Q

The mass of a galaxy’s central black hole is related to the mass of the galactic bulge. This implies that
____

A

central black holes formed when the galaxy bulges forme

92
Q

Hot, low-density gas can be detected in galactic clusters through X-ray emission. The gas is important
in understanding dark matter because ____

A

dark matter must make the cluster massive enough to hold on to the hot gas

93
Q

Gravitational lensing is caused by ____.

A

bending of light rays due to the curvature of space-time around a mass

94
Q

Rich galactic clusters are ____

A

mostly elliptical galaxies

95
Q

Spiral galaxies are mostly found ____.

A

in poor clusters

96
Q

Galactic collisions ____

A
97
Q

The Milky Way and other spiral galaxies ____.

A
98
Q

. Spiral structures and steady star formation depend on ____.

A

gentle gravitational interactions with other galaxies

99
Q

One of the rare galaxies that is isolated in space is likely to be a(n) ____.

A

flocculent spiral galaxy

100
Q

At the longest look-back times, we see ____

A

redshifted irregular galaxies

101
Q

S0 galaxies have spiral arms, but little to no gas and dust. This is believed to happen because ____.

A

gas and dust have been stripped from the galaxies as they pass through hot, intergalactic
gas

102
Q

A galaxy with randomly oriented elongated star orbits and little gas and dust would be a(n)
_______________ galaxy.

A

elliptical

103
Q

_______________ galaxies have star formation, but no clear shape

A

irregular

104
Q

Because the Hubble constant has a value of 70 km/s/Mpc, a galaxy 50 Mpc away would have a
recession velocity of _______________ km/s. (Round your answer to the nearest 1 km/s).

A

3500

105
Q

Because the Hubble constant has a value of 70 km/s/Mpc, a galaxy 50 Mpc away would have a
recession velocity of _______________ km/s. (Round your answer to the nearest 1 km/s).

A

3500

106
Q

Because the Hubble constant has a value of 70 km/s/Mpc, a galaxy with a recession velocity of 21,000
km/s must be _______________ Mpc from Earth. (Express your answer as a whole number of Mpc)

A

300

107
Q

_______________ are objects of known luminosity used for finding distances

A

standard candles

108
Q

. The _______________ time is the amount of time it took light to travel from a celestial object to
Earth.

A

light travel time

109
Q

. The mass of a galaxy can be determined from its _______________ curve

A

rotation

110
Q

The mass of a galaxy’s central black hole is proportional to the mass of its _______________

A

host galaxy

111
Q

The velocity dispersion method can be used to find the _______________ of a galaxy

A

mass

112
Q

Galactic _______________ describes the process of a large galaxy absorbing a smaller one

A

collision

113
Q

Gravitational _______________ can be used to detect dark matter

A

Lensing

114
Q

A galaxy that has created a large number of young stars all at once is a(n) _______________ galaxy.

A

starburst

115
Q

A galaxy that has gone through many collisions and mergers must be a(n) _______________ galaxy.

A

elliptical

116
Q

Gentle tidal interactions are probably necessary to support the formation of _______________ in a
galaxy

A

spiral arms

117
Q

All of the farthest detectable galaxies are _______________ galaxies

A

irregular

118
Q

Briefly describe the characteristics of an elliptical galaxy

A

Elliptical galaxies have a smooth ellipsoidal or spherical appearance, and they have far less structure than spiral galaxies do. Elliptical galaxies are typically found in galaxy clusters.

119
Q

How are standard candles used to measure distance?

A

If you have two stars of the same type, but one is further away than the other, it looks fainter. Knowing that they should be the same brightness allows us to work out the distances between them.

120
Q

Is dark matter important in other galaxies and galactic clusters

A

yes because they reside in a region where such matter is much denser than average. Scientists believe that the heavier a cluster is, the more dark matter it has in its environment

121
Q

milkly way compared to others

A

larger and brighter than most spirals

122
Q

What is galactic cannibalism?

A

occurs when the gravitational forces from a larger galaxy or group of galaxies slowly tear apart a smaller galaxy. Characteristic features of galactic cannibalism are streams or halos of stars orbiting the larger galaxy, like the halo of red stars seen around NGC 7317