Final Flashcards

1
Q

The study of the moon is called

A

Selenologists

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2
Q

Most places on earth experience ____ high ___ and ___ low ___

A

two high tides & two low tides

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3
Q

Tides are created mainly by the influence of this celestial object:

A

moon

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4
Q

The ___ also causes earth’s tides, but it only has about ___ the effect of the moon.

A

sun; 1/2

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5
Q

When the moon is full or new, we experience ___ tides.

A

Spring

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6
Q

When the moon is at quadrature (1st or 3rd Quarters), we experience ___ tides

A

Neap

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7
Q

___ tides are the most exaggerated tides (really high high tides and really low low tides)

A

Spring

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8
Q

We have ___ tides and ___ tides each month

A

Spring; Neap

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9
Q

Explorer 1 discovered these belts of trapped, electromagnetically-charged particles:

A

Van Allen Belts

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10
Q

The moon’s crust, like other terrestrial bodies, is made of these two rocks:

A

granite & basalt

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11
Q

3 principal layers of a terrestrial planet or moon:

A

crust, mantle & core

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12
Q

The Earth’s core is principally made of these metals:

A

magnesium & iron

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13
Q

The arrangement of materials from densest at the core to least dense outward, is caused by this process:

A

chemical differentiation

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14
Q

Lunar maria are made principally of this rock type:

A

dark basalt

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15
Q

How is lunar far side different from its nearside?

A

Twice as thick crust

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16
Q

Why is the lunar far side different from its nearside?

A

Long axis aligned with Earth’s gravitational pull

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17
Q

This process is responsible for the movement of Earth’s surface features:

A

plate techtonics

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18
Q

The margins of tectonic plates are places where these occur:

A

earthquakes & volcanoes

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19
Q

Over 200 million years ago, this “supercontinent” existed:

A

Pangea

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20
Q

This plate boundary, such as in the mid-Atlantic Ocean, is where new crust is being made:

A

Divergent (Iceland)

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21
Q

This plate boundary, such as at Indian and Nepal, is where continental crust collides:

A

Convergent (Himalayas)

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22
Q

This plate boundary, such as at San Andreas, is where two plates run past each other:

A

strike-slip

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23
Q

Geologically speaking, the moon is:

A

dead

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24
Q

Scientific name for lunar soil:

A

regolith

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25
Q

If the moon has no volcanic activity or moonquakes or atmosphere, where does the regolith come from?

A

micrometeriorites from Earth’s atmosphere

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26
Q

All of the planets revolve in this direction:

A

counterclockwise

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27
Q

A planet’s rotational speed is directly related to its distance from the sun: T/F

A

False

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28
Q

The order of the planets outward from the sun:

A

rocky inner, gas giants outer

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29
Q

What are the two classes of planets?

A

Jovians (gas giants) & Terrestrials (rocky planets)

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30
Q

Terrestrials are found in the ___ solar system

A

inner

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31
Q

Jovians are found in the ____ solar system

A

outer

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32
Q

Largest planet in the solar system:

A

Jupiter

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33
Q

2nd largest planet in the solar system:

A

Saturn

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34
Q

The jovian planet’s main constituents:

A

hydrogen, helium, methane, ammonia

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35
Q

Largest terrestrial planet:

A

Earth

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36
Q

2nd largest terrestrial planet:

A

Venus

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37
Q

3rd largest terrestrial planet:

A

Mercury

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38
Q

Liquid water is found only on this planet:

A

Earth

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39
Q

The number of sunspots in the solar photosphere reaches a peak every ___ years

A

11

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40
Q

The suns’s visible surface:

A

photosphere

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41
Q

Large dark spots in the suns photosphere:

A

sunspots

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42
Q

Sunspots are dark because they’re ___ than the surrounding solar photosphere.

A

cooler

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43
Q

Photosphere temperature:

A

11,000 degrees

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44
Q

Sunspot parts - cooler, inner ___; slightly warmer, out ___

A

umbrea; penumbra

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45
Q

Sunspots are permanent features: T/F

A

false

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46
Q

Great glowing jets or clouds of gas int he solar chromosphere:

A

prominences

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47
Q

Outermost layer of the sun containing superheated plasma:

A

chromosphere

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48
Q

Large, powerful sunspots can often release these vast explosion eruptions:

A

flares

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49
Q

Subatomic particles ride the ___, creating ___ in Earth’s atmosphere

A

solar wind; aurora

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50
Q

Three early ideas of how the sun made energy:

A

chemical burning; gravitational contraction; bombardment by asteroids

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51
Q

___ devised the absolute magnitude scale, where 0 degrees - the point where all molecular activity stops

A

Williams Thompson (Lord Kelvin)

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52
Q

“Heat flows from a hotter body to a colder one” is the ___ of thermodynamics.

A

2nd

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53
Q

Besides the Kelvin scale, what are two other commonly used temperature scales:

A

fahrenheit & celsius

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54
Q

Convert to Fahrenheit: 0 degrees Celsius

A

32 degrees (freezes)

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55
Q

Convert to Fahrenheit: 100 degrees Celsius

A

212 degrees (boils)

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56
Q

Convert to Fahrenheit: 0 degrees Kelvin

A

-459 (molecular activity presumably stops)

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57
Q

Why weren’t geologists okay with Kelvin’s 30 million year estimate for the sun’s age?

A

Earth was estimated to several hundred million years old

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58
Q

___ devised the laws of special and general relativity.

A

Albert Einstein

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59
Q

This formula explains how matter is converted into energy, is the secret of the sun’s success:

A

E=MC2

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60
Q

In E=MC2, E = ___

A

energy produced

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61
Q

In E=MC2, M = ___

A

mass detroyed

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62
Q

In E=MC2, C = ___

A

speed of light

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63
Q

Temperature of the solar core:

A

27 million degrees

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64
Q

In the solar core, hydrogen is converted into ___

A

helium plus energy

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65
Q

The process fo splitting heavy elements into smaller units is nuclear ___

A

fusion

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66
Q

The combining of light elements into heavier ones is nuclear ___

A

fission

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67
Q

The sun’s nuclear fusion process, whereby hydrogen atoms combine to ultimately form helium and energy is called the ___

A

proton-proton chain

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68
Q

In more massive stars, the nuclear fusion process is called the ___

A

carbon cycle

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69
Q

The sun’s gravity field is so powerful that it can ___ light

A

bend

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70
Q

In 1919, during a ___, the deflection of starlight by the sun’s gravity field was first detected by Sir Arthur Eddington

A

total solar eclipse

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71
Q

These “wrinkle” in the Mercurian crust are the result of shrinkage of the planet:

A

lobate scarps

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72
Q

Impact feature on Mercury, over a thousand miles across:

A

caloris basin

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73
Q

This spacecraft once orbited Mercury, but it recently smashed into it:

A

Mercury Messenger

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74
Q

Compared to its crust and mantle, Mercury’s metal core is comparatively:

A

large

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75
Q

The atmosphere of Mercury is ___

A

non-existent

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76
Q

Venus’ atmosphere is made of:

A

carbon dioxide

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77
Q

Our sister planet:

A

Venus

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78
Q

The air pressure eon Venus is ___ that of Earth’s

A

90 times

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79
Q

The surface temperature on Venus:

A

900 degrees Fahrenheit

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80
Q

This effect has caused Venus’ atmosphere to become superheated:

A

greenhouse effect

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81
Q

With coronae and volcanoes and tectonics, geologically speaking, Venus is ___

A

active

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82
Q

Impact craters on Venus are not generally very big or very small, but mostly ___

A

mid-size

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83
Q

Mars is ___ the size of Earth

A

1/3-1/2

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84
Q

Mars rotation rate compared to Earth’s:

A

24 1/2 (slightly longer)

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85
Q

Mars has these cold polar features that grow and shrink with the seasons:

A

ice caps

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86
Q

Mars ice caps are made up of both water ice and ___

A

dry ice

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87
Q

In 1887, a ___ brought us within 35 million miles of ___

A

perihelic opposition; Mars

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88
Q

At the U.S. Naval Observatory, ___ found Mars’ two small moons.

A

large 26” refractor

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89
Q

Mars two small moons:

A

Phobos; Deimos

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90
Q

___ observed canali (channels) on Mars; the wod was mistranslated as ___.

A

Giovanni Schiaparelli; canals

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91
Q

He advanced the idea of intelligent Martians who built irrigation canals:

A

Percival Lowel

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92
Q

15 mile high volcano on Mars:

A

Olympus Mons

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93
Q

3000 mile long crack in the ground on Mars:

A

Valles Marineris

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94
Q

Dry river valleys, flood zones, alluvial fans and sea or lakebed, as well as hematite “blueberries” on the Meridian plains are a good indicator of ___ in the past on Mars.

A

liquid water

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95
Q

Gaspra, Ida, Mathilde and Eros are all examples of these:

A

Asteroids

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96
Q

Another name for an asteroid:

A

minor asteroids

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97
Q

He found the first asteroid telescopically, and named it Ceres:

A

Father Guiseppi Piazzi

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98
Q

___ Law is a numerical sequence which suggested the existence of the ___ as well as planets beyond the orbit of Uranus

A

Bode’s; asteroids

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99
Q

Bode’s Law is not a law because its is not ___ and it doesn’t always ___

A

universal; work

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100
Q

A popular scientific theory suggests that the dinosaurs were killed off by ___

A

meteors

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101
Q

A streak of light in the night sky is called a ___

A

meteroid

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102
Q

The rock in outer space prior to its burning up in the Earths atmosphere is called a ___

A

meteor

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103
Q

When a meteor hits Earth, it’s call a ___

A

meteorite

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104
Q

A bright meteor is known as a ___

A

fireball

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105
Q

If a meteor loudly explodes, it’s called a ___

A

bolide

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106
Q

Characteristics of meteorites:

A

heavy, magnetic, with fusion crust

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107
Q

This type of meteorite is metallic and readily identifiable as meteoritic in nature:

A

iron-nickel

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108
Q

Iron meteorites, cut, polished and etched, reveal these iron crystals:

A

widmanstatten pattern

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109
Q

These meteorites are made of stony materials, like earth rocks:

A

achondrites

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110
Q

These stony meteorites contain rounded bits of glassy rock:

A

chondrites

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111
Q

This meteorite type is a mixture of stony and iron

A

tektites

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112
Q

Jupiter is 1/2 billion miles from the sun, Saturn is 1 billion miles from the sun, Uranus is ___ billions miles from the sun

A

2

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113
Q

Because of its fast rotation and resulting centrifugal force, the planet Jupiter is wider at the equator than from pole to pole, making it ___

A

oblate

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114
Q

Large hurricane on Jupiter, 2-3x the size of Earth, w/ 400 mph winds:

A

Great Red Spot (GRS)

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115
Q

The GRS has been observed telescopically for ___ years

A

400

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116
Q

These atmospheric phenomena are to be found at Jupiter:

A

storms, lighting, and aurorae

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117
Q

This comet smashed into Jupiter in 1994:

A

Shoemaker-Levy 9

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118
Q

Jupiter’s outer moon - ancient, heavily cratered terrain:

A

Callisto

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119
Q

Largest moon in solar system (Jupiter) featuring ice, grooved terrain:

A

Garymede

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120
Q

Fresh, smooth-surface moon of Jupiter with fine cracks in icy crust and subsurface water:

A

Europa

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121
Q

Tidally heated, sulfur covered Jupiter moon with many active volcanoes:

A

Io

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122
Q

Which of the gas giant planets has rings:

A

Jupiter, Saturn, Neptune, Uranus

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123
Q

Volume of space controlled by a planet’s magnetic field:

A

magnetosphere

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124
Q

What are Saturn’s rings mainly made of:

A

tiny water ice chunks

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125
Q

Saturn’s density is less than:

A

water

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126
Q

Besides the ___ gap, there is also ___ division in Saturn’s rings

A

cassini; enke

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127
Q

Electrostatically charged dust suspended above Saturn’s rings:

A

spokes

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128
Q

Titan possess a thick atmosphere made principally of this gas:

A

nitrogen

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129
Q

This musician discovered the planet Uranus (almost named, “George”) in 1781:

A

William Herschel

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130
Q

What may have caused Uranus’ sideways tilt?

A

Collision, or planets may tip time to time

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131
Q

Of Uranus’ dozens of moons, this one has ice cliffs several miles high:

A

Miranda

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132
Q

This Earth-sized Neptunian feature has recently disappeared:

A

The great dark spot

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133
Q

This Neptunian moon orbits backwards or retrograde

A

Triton

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134
Q

These eruptive features are found on Triton:

A

Cryovolcanoes

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135
Q

Besides promoting Martian canals, Lowell postulated a ninth planet known at the time as ___

A

Planet X

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136
Q

Planet X was discovered in 1930 by ___

A

Clyde Tombaugh

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137
Q

Tombaugh discovered the planet one night while looking through a telescope: T/F

A

False

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138
Q

Planet X was soon named:

A

Pluto

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139
Q

Because Pluto’s orbit is more elliptical and offset from the others, it sometimes slips inside ___ orbit.

A

Neptunes

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140
Q

Besides Charon, Pluto has four more moons discovered only recently;

A

Nix, Hydra, Styx and Kerberos

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141
Q

The amount of reflectivity of a planet:

A

albedo

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142
Q

Kuiper belt objects such as Quaor, Sedna and Eris are classified as ___

A

ice dwarfs

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143
Q

Short-period comets may come from this belt outside Neptune’s orbit:

A

Kuiper belt

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144
Q

This spherical cloud of comets surrounds our solar system:

A

Oort Cloud

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145
Q

In 1682 he saw the comet that would later be named for him:

A

Edmund Halley

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146
Q

Haley thought that the comets did not travel in straight lines, but instead had ___

A

elliptical orbits

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147
Q

The orbits of many comets are highly ___

A

elliptical

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148
Q

Recent apparitions of Halley’s Comet:

A

1682, 1759, 1835, 1920 (142 years)

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149
Q

Halley’s Comet reappears in:

A

2052

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150
Q

Comet Hale-Bopp is a good example of a ___ period comet

A

long

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151
Q

Halley’s comet is a ___ period comet

A

short

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152
Q

Comet tails always point ___ from the sun due to the pressure of solar radiation and flow of subatomic particles outward - the solar wind.

A

away

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153
Q

Parts of a comet: the atmospheric head, called a ___

A

Coma

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154
Q

Parts of a comet: the dust and gas blown off the coma by the solar wind:

A

tail

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155
Q

The ___ tail of a comet extends out in a straight line

A

iron or gas

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156
Q

The ___ tail curves away from a comet in an arc

A

dust

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157
Q

Spacecraft have flown past comet tails, struck comets, and brought back comet tail material to Earth: T/F

A

True

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158
Q

The dense worlds are found in the ___ solar system

A

inner

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159
Q

The gas giants are located in the ___ solar system

A

outer

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160
Q

This kind of material boils at fairly low temperatures:

A

volatile

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161
Q

This kind of material remains solid at high temperatures:

A

refractory

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162
Q

This hypothesis best explains the moon’s origin:

A

large impact theory

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163
Q

The ___ suggested that a passing star pulled material from the sun to form planets

A

planetismal theory

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164
Q

The ___ suggested that hot gas blew off the sun to form planets

A

tidal theory

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165
Q

The ___ suggested the sun was a binary, but the companion blew up making planets.

A

double star theory

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166
Q

The ___ was the basis for our modern ___; suggesting that the sun and planets formed from a cloud created by exploding stars

A

condensation theory; solar nebula

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167
Q

According to the solar nebula theory, the solar system began about ___ billion years ago

A

4.6

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168
Q

How was this age determined? (universe)

A

Radioactive dating of meteorites

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169
Q

Large planet-building objects that formed from the solar nebula:

A

planetesimals

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170
Q

Massive objects destined to become planets:

A

protoplanets

171
Q

If the solar nebula theory is right, then planets should be very ___ in the Universe.

A

common

172
Q

Visual evidence of solar nebulae has been found as protoplanetary discs, or ___ in the ___ and in the spectroscopic wobbles or nearby ___.

A

proplyds; Great Orion Nebula; Stars Spectra

173
Q

The speed of light, symbolized by the letter C, is approximately 186,000 miles per second. Given that there are roughly 33 million seconds in a year (60 X 60 X 24 X 365.25), light can travel about ____in one year.

A

6 trillion miles

174
Q

The speed light can travel in one year:

A

lightyear

175
Q

A “parallax second of arc,” is called a ___

A

parsac

176
Q

A parsec is equal to about ___ light years

A

3.26

177
Q

Objects beyond our solar system, such as stars, nebulae, and galaxies:

A

deep sky objects / deep space objects

178
Q

All of the stars we can see with the naked eye are part of the ___

A

Milky Way Galaxy

179
Q

This French astronomer made a list of a hundred or so fuzzy objects that weren’t comets:

A

Charles Messier

180
Q

When comets are far from the sun, they don’t have ___

A

tails

181
Q

One way to determine if a fuzzy object is a comet is to see if it ___ against the background of stars.

A

moves

182
Q

The first Messier object, M-1, is really the ___ nebula, the exploded remains of a star

A

crab

183
Q

The Messier list objects comprise of ___ star clusters & ___ star clusters

A

nebula, open; globular

184
Q

At 4.3 LY, the nearest star to us after the sun (so far as we know):

A

Alpha Centauri (Rigel)

185
Q

of stars in the Alpha Centauri system

A

3

186
Q

Common center of mass in the Alpha Centauri system:

A

barycenter

187
Q

Of the three stars of Alpha Centrauri, this red dwarf is the closest to us:

A

Proxima

188
Q

The most common kind of star:

A

red dwarf

189
Q

The rarest kind of star:

A

blue giant

190
Q

Stars are formed from the contraction and heating up of ___

A

nebulae

191
Q

Our sun is sometimes designated as a ___

A

yellow dwarf

192
Q

Barnard’s Star and Proxima Centauri are ___

A

red dwarfs

193
Q

The stars we see in the sky at night are predominately the most common - red dwarfs: T/F

A

False - too faint to see

194
Q

Betelgeuse, Aldebaran and Antares are very bright but also very ___

A

cool

195
Q

Stars: ___ and ___ giants

A

red; blue

196
Q

Stars:___ and ___ dwarfs

A

white; red

197
Q

Stars: ___ stars and ___ holes

A

neutron; black

198
Q

Massive stars that blow up:

A

supernovas

199
Q

Blue giant characteristics:

A

massive, hot, bright (Rigel, Vega)

200
Q

Red giant characteristics:

A

big, cool (Betelgeuse, Antares, Aldebaran)

201
Q

White dwarf characteristics:

A

small, hot (Sirius B, Procyon B)

202
Q

Neutron stars are also called ___

A

pulsars

203
Q

Pulsar star characteristics:

A

small, very hot, dense, magnetic, rotate rapidly

204
Q

There is a neutron star in this nebula:

A

crab

205
Q

___ is a good example of a black hole, but it was not discovered until the 1960’s

A

Cygnus X-1

206
Q

Two basic kinds of star cluster: ___ and ___

A

open; globular

207
Q

Open star clusters are also called ___

A

galactic star clusters

208
Q

Two examples of open star clusters: ___ and ___

A

Pleiades; Praesepe

209
Q

___ star clusters are spherical in shape

A

Globular

210
Q

Globular star clusters contain ___ of stars, and they are ___

A

millions; very, very old

211
Q

Two examples of globular star clusters: ___ and ___

A

M13 Hercules, Omega Centauri

212
Q

A large cloud in outer space: ___ and ___

A

nebula; nebulae

213
Q

Nebulae are composed of ___ and ___ and are trillions of miles across.

A

gas; dust

214
Q

A ___ is mainly dust with very little gas, like the nebulosity around the Pleiades

A

reflection nebula

215
Q

A ___, aka a Barnard cloud or Bok globule, has no bright stars within to light it up

A

dark nebula

216
Q

An ___ is the birthplace of new stars; the gas is lit up by the light of stars within.

A

emission nebula

217
Q

Examples of emission nebulae:

A

Lagoon, Eagle, Trifid, Rosette, N. American

218
Q

A ___ is the listed-off outer atmosphere of a dying star.

A

planetary nebula

219
Q

Examples of planetary nebulae:

A

Hourglass, Eskimo, Ring, Dumbell, Catseye, Spirograph, Helix

220
Q

A ___ nebula is not really a nebula, but a distant galaxy, like the ___ galaxy

A

spiral; Andromeda

221
Q

A star’s ___ tells us its temperature

A

color

222
Q

Cool stars are ___

A

red

223
Q

Hot stars are ___

A

blue

224
Q

Newton used a prism to split the sun’s light into its component colors, a ___ spectrum

A

rainbow

225
Q

The colors of a rainbow spectrum, as noted by Newton

A

red, orange, yellow, green, blue, indigo, violet

226
Q

The light that the human eye can see is called ___

A

visible light

227
Q

The prism separates the colors of visible light by ___ its different wavelengths to various degrees

A

bending

228
Q

A rainbow fringe around an image produced by a lens is called ___

A

chromatic aberration

229
Q

A complete collection of colors caused by splitting light

A

continuous spectrum

230
Q

Name the full spectrum of light from lowest to highest energy:

A

radio, infrared, visible, ultraviolet, x-ray, gamma ray

231
Q

A device that allows us to see absorption lines in a spectrum of light:

A

spectroscope

232
Q

Dark absorption or Fraunhofer lines make up this kind of spectrum:

A

absorption spectrum

233
Q

An absorption spectrum is caused by ___ absorbing select wavelengths of light

A

cool gasses

234
Q

Bunsen and Kirchoff discovered this kind of visible light spectrum:

A

emission (bright light)

235
Q

An emission spectrum is made by causing a low-density ___ to glow and emit select wavelengths of light

A

nebula

236
Q

Each element has its own spectral ___ allowing us to identify the compositions of stars.

A

signature

237
Q

Modern spectral analysis is accomplished not with prisms but with ___

A

diffraction gradings

238
Q

This effect causes blue shifts and red shifts in stars ___

A

doppler

239
Q

A higher frequency of light represents a ___ shift

A

blue

240
Q

A lower frequency of light represents a ___ shift

A

red

241
Q

The star Spica has red-shifted spectral lines; six months later its lines are blue-shifter. What causes this?

A

Earth revolution carries us towards and then away

242
Q

Kind of velocity exhibited by red or blue-shifted stars:

A

radial

243
Q

The greater the Doppler shift , the ___ the radial velocity of the object

A

greater

244
Q

Faint stars without Arabic names, greek or Roman letter designations, have ___

A

Flamsteed numbers

245
Q

He was England’s first royal astronomer and built the Greenwich Observatory:

A

John Flamsteed

246
Q

This Danish astronomer was first to determine the speed of light:

A

Ole Roemer

247
Q

The small shift in a star’s position caused by viewing it from two different locations:

A

stellar parallax

248
Q

Given D=1/p, calculate the distance to Alpha Centauri if its parallax is .75 arc second

A

Divide 1.00 by .75 = 1.33 pc

249
Q

After parallax has been taken into account, stars that change their positions among the other stars over time display what’s called:

A

proper motion

250
Q

Two stars that orbit each other are called ____

A

binary stars

251
Q

A binary where the stars are far enough from each other that the telescope can let you see them visually is called a ___

A

visual binary

252
Q

At first glance, they look like a binary star, but they’re not actually bound gravitationally:

A

optical double

253
Q

It looks like one star, but its spectral lines periodically split and then re-merge, the split again:

A

spectroscopic binary

254
Q

A binary system where two stars pass in front of each other:

A

eclipsing binary

255
Q

This star in Perseus is an eclipsing binary system:

A

Algol

256
Q

The ___ of eclipsing binaries allows us to measure their orbits and velocities, their diameters and their masses and sometimes their share and surface features.

A

light curve

257
Q

When a cool star eclipses a hot star, the system’s brightness drops ___ than when a hot star eclipses a cool one

A

a lot more

258
Q

___ devised the spectral classes of stars

A

Annie Cannon

259
Q

Spectral classes of stars from hot to cool:

A

O, B, A, F, G, K, M

260
Q

Make up a mnemonic to remember the order:

A

Oh boy, a fat gorilla kicked me

261
Q

Each spectral class of star is further subdivided into ___ classes

A

10

262
Q

The ___ law applies to the way light dims with distance.

A

inverse square

263
Q

If Jupiter is 500 million miles from the sun and Uranus is 2 billion miles out, how much less light does Uranus get than Jupiter

A

1/16

264
Q

If star A and star B are the same size and the same temperature, but star B is three times farther away that star A, how much dimmer does star B appear than star A

A

9 times

265
Q

If star A and star B are the same distance away, but star B is much fainter than star A, then star B’s absolute magnitude is much less than star A’s.

A

True

266
Q

If star A and star B are the same size and temperature, but star A appears 100 times brighter than star B, then star A must be ___

A

10 times closer

267
Q

The true measurement of a star’s visual brightness:

A

absolute magnitude

268
Q

___ and ___ devised the Hertzsprung-Russel diagram

A

Hertzrung; Russell

269
Q

The HR diagram plots a star’s ___ or ___ against its ___ or ___

A

temperature, spectral class; absolute magnitude, luminosity

270
Q

The ___ of a star compares its brightness to that of the suns

A

luminosity

271
Q

The absolute magnitude of a star is its apparent magnitude if it were ___ away from us.

A

10pc

272
Q

At a distance of 10 pc, the sun’s apparent magnitude would be ___

A

5th Mv

273
Q

___ stars have a red color

A

M

274
Q

___ stars are orange

A

K

275
Q

___ stars are yellow

A

G

276
Q

___ stars are blue / white

A

O&B

277
Q

In the HR diagram, hot stars are on the ___ side

A

left

278
Q

In the HR diagram, cool stars are on the ___ side

A

right

279
Q

In the HR diagram, bright stars are at the ___

A

top

280
Q

In the HR diagram, dim stars are at the ___

A

bottom

281
Q

90% of all known stars fall along this line on the HR diagram:

A

main sequence line

282
Q

As you go up the main HR sequence, the star temperatures and brightness ___

A

increase

283
Q

Cool dim stars:

A

red dwarf

284
Q

hot, bright stars:

A

blue giants

285
Q

cool, bright stars:

A

red giants

286
Q

hot, dim stars

A

white dwarfs

287
Q

Red giants and white dwarfs are off the main sequence: T/F

A

True

288
Q

Stars are formed out of emission-___

A

nebulae

289
Q

When the hydrogen in the core of a star is used up, the star begins to ___

A

die

290
Q

The less massive the star, the ___ it lives

A

longer

291
Q

The more massive the star, the ___ its lifespan

A

shorter

292
Q

___ have such long lives that some of them started glowing when the universe was young

A

Red dwarfs

293
Q

Our own sun has shone for ___

A

5 billion years

294
Q

Our own sun will shine for another ___

A

5 billion years

295
Q

The only star that typically never becomes a red giant is a ___

A

red dwarf

296
Q

When the sun finally dies, it will explode as a supernova, then collapse to become a black hole: T/F

A

False

297
Q

When the sun’s nuclear furnace shuts down, it will first ___; then ___ will begin to “burn” in a shell surrounding the solar core. About this same time, ___ will begin to burn in the core, making ___. The sun will then ___ and become a ___ giant.

A

contract & heat up; hydrogen; carbon; helium; swell; red

298
Q

When the outer atmosphere of the sun “lifts off” and expands out into space it will make a ___

A

planetary nebula

299
Q

Eventually the sun will burn up its shell hydrogen and core helium and collapse to become a ___

A

white dwarf

300
Q

When the sun becomes a white dwarf, it will be the size of ___

A

Earth

301
Q

A long time after the sun becomes a white dwarf, it will cool to become a ___

A

black dwarf

302
Q

___ are exploding stars

A

Supernova

303
Q

The last nearby supernova seen occurred in ___ in the ___, 160,000 LY away

A

1987; large megellanic cloud

304
Q

A simple ___ is a dying star, but it not an exploding star

A

nova

305
Q

Novae are ___ found in ___

A

white dwarfs; binary systems

306
Q

Novae pull gas from its companion down onto an ___

A

accretion disc

307
Q

White dwarf stars can brighten again and again, often at regular intervals of time: T/F

A

True

308
Q

If a white dwarf pulls enough material to increase its mass sufficiently, it can become a ___

A

supernova

309
Q

Exploding white dwarf stars are ___ supernovae

A

Type 1

310
Q

Solitary massive stars that explode are ___

A

Type 2

311
Q

___ stars result from supernovae

A

Neutron

312
Q

Neutron stars are about ___ across and spin ___

A

10 miles; fast

313
Q

___ proposed mass limits for stars that would either become white dwarfs, neutron stars or black holes

A

Chandrasekhar

314
Q

If a dying star has more than 2.4 times the mass of the sun, it will become a ___

A

black hole

315
Q

At the center of the black hole is a tiny, super-dense point called a ___

A

singularity

316
Q

An ___ surrounds the black hole

A

accretion disc

317
Q

A black holes speed-of-light point of no return is the ___

A

event horizon

318
Q

Although we can’t see black holes directly, we can detect their presence due to their ___

A

gravity fields

319
Q

___ can leak out from around black holes

A

x-rays & radiation

320
Q

The distance from the singularity to the event horizon is known as the ___

A

schwarzschild radius

321
Q

Schwarzchild radius is equal to ___ solar mass.

A

3km

322
Q

if a black hole has 10 times the sun’s mass, its Schwarzschild radius is ___

A

30km

323
Q

Joylen =

A

Pulsar

324
Q

rapidly rotating =

A

Pulsar

325
Q

Hershcel’s star counts led him to conclude that th eMilky Way galaxy was shaped like a ___

A

great disc or millstone

326
Q

According to the Law of ___, matter is fairly evenly distributed throughout the Universe

A

homogeniety

327
Q

Herschel thought we were at the ___ of the galaxy

A

center

328
Q

A dark region in the Milky Way that passes through the Summer Triangle is called the ___

A

great rift

329
Q

William Parsons, the Earl of Rosse, built this, the largest telescope in the world; the ___

A

Irish Leviathon

330
Q

The Leviathan was powerful enough to observe individual stars in ___

A

other galaxies

331
Q

Parsons suggested, as with the Whirlpool Nebula, that spiral nebulae might well be other ___

A

galaxies

332
Q

___ catalogued ___ and found a connection between their absolute magnitudes and their light curve periods

A

Henrietta Leavitt; cepheid variable stars

333
Q

The greater a Cepheid variable’s absolute magnitude, the ___ time it takes to go through a cycle.

A

more

334
Q

Using Cepheid variable stars, we can calculate their ___ even if no parallex is observable.

A

distances

335
Q

Until the 1920’s, astronomers weren’t sure if ___ nebulae were part of our galaxy, or other galaxies beyond.

A

spiral

336
Q

The Andromeda galaxy is about ___ light years, or ___ miles away

A

2.5 million; 15 million trillion

337
Q

___ argued that the distribution of ___ star clusters was centered on the constellation ___; therefore, that was the center of the galaxy, not here.

A

Harlow Shapley; globular; Sagittarius

338
Q

Shapley also thought the Milky Way was much ___ than most thought.

A

larger

339
Q

____ argued that spiral nebulae were really distant ___

A

Heber Curtis; galaxies

340
Q

Curtis cited this phenomenon, found in the spiral nebulae, to prove they were far away:

A

Novas

341
Q

In 1924 Edwin Hubble cited his observation of a ___ in M31 to priove it was another galaxy

A

Cephid Variable

342
Q

Three basic galaxy types:

A

spiral; ellipticals; irregulars

343
Q

White spiral and elliptical galaxies can be ___ or ___, irregulars are invariably ___

A

small, large; much smaller

344
Q

E0 elliptical galaxies are ___

A

round

345
Q

E7 elliptical galaxies are ___

A

very elliptical

346
Q

E3 elliptical galaxies are ___

A

in-between round and elliptical

347
Q

Sa spiral galaxies have ___ cores and ___ wound arms

A

large; tight wound

348
Q

Sc spiral galaxies have ___ cores and ___ arms

A

small; widely flung

349
Q

Sb spiral galaxies are ___ Sa and Sc spiral galaxies

A

in-between

350
Q

A variant of the spiral galaxy is the ___ spiral that has a bar-shaped nucleus

A

SBa

351
Q

S0 spirals have a ___ shape but no discernible ___

A

lens/spiral; arms

352
Q

Two small companion galaxies to the Milky Way are the Large and Small ___

A

Magellanic Clouds

353
Q

While our galaxy is a spiral, the Megallanic Clouds are ___

A

irregular

354
Q

Our sun is about ___ from the galaxy’s center; we’re in the ___ arm

A

2/3rds out; Orion

355
Q

At the center of the galaxy is a ___. Surrounding it is a flattened ___; surrounding the bulge and the disc is the ___.

A

Nuclear bulge; disc; halo

356
Q

The disc of a galaxy usually contains 2 or 4 ___

A

arms

357
Q

The nuclear bulge and the halo are often referred to as the __

A

spherical component

358
Q

The ___ is gas and dust along the band of the Milky Way that keeps us from receiving visible light from the other side of the galaxy, and beyond our line-of-sight with the disc.

A

zone of avoidance

359
Q

The sun takes ___ million years to make one orbit of the galaxy; this is a ___ year

A

240; galactic

360
Q

___ is a region at the center of the Milky Way, where superheated gas swirls about at fantastic speeds, driven on by a ___ with ___ million times the mass of the sun!

A

Sagittarius; galactic black hole; 4

361
Q

Stars that orbit rapidly in a ___ fashion are being sped up by ___ matter in the galactic ___, which surrounds the disc and hao

A

non-kepleriana; dark; corona

362
Q

Our galaxy may not be a classic spiral shape, but instead a ___

A

barred spiral (SBa)

363
Q

Stars once formed in the Milky Way’s ___ component, now it’s mainly in the ___’s spiral arms

A

disc

364
Q

There are two basic star types: ___ stars are found mainly in the disc; ___ stars are found mainly n the spherical component.

A

Type 1; Type 2

365
Q

Type 1 stars have fairly ___ orbits confined to the plant of the disk

A

tight

366
Q

___ stars weave in and out of the disc, often traveling at right angles to the disc stars

A

Type 2

367
Q

Type 1 stars contain lots of ___ elements

A

heavy

368
Q

Type II stars are ___

A

metal-poor

369
Q

Type 1 stars are relatively ___

A

young

370
Q

Type II stars are relatively ___

A

old

371
Q

The atoms in our bodies came from:

A

cores of stars exploded!

372
Q

Local group stars are ___

A

cluster of galaxies to which the Milky Way belongs

373
Q

Milky Way diameter:

A

100,000 ly

374
Q

Discovering of Andromeda Nebula was by ___

A

Hubble

375
Q

Stars with lowest average metal content found in what part of galaxy?

A

Halo and Nuclear Bridge

376
Q

Shapley thought the sun is located where?

A

Disc of galaxy (1/2 way out)

377
Q

Spiral arms are found in their part of the galaxy;

A

disc

378
Q

___ is detected via its gravitational exertions on other ___

A

Dark Matter; galaxies

379
Q

Many large galaxies have ___ at their cores

A

black holes

380
Q

Number of stars in the Milky Way:

A

100-200 Billion

381
Q

M31 galaxy has ___ stars and is ___ than the Milky Way

A

over 300 billion; larger

382
Q

1000 pc’s is a kilo parsec, abbreviate as:

A

kpc

383
Q

1,000,000 pc’s is a megaparsec, abbreviated as:

A

mpc

384
Q

The ___ consists of over two dozen nearby galaxies; its two largest members are the ___ galaxy and the ___

A

Local group; Andromeda; Milky Way

385
Q

Most of the galaxies are this type:

A

elliptical

386
Q

The Local group is a ___ galaxy cluster; Virgo, Fornax, Hercules and Coma are all ___ clusters

A

poor; rich

387
Q

Superclusters of galaxies seem to be arranged in a ___ type pattern, with large ___ within them. One of the largest structures seen is the ___

A

soap bubble; voids; great wall

388
Q

Galactic collisions hardly ever happen Star collisions happen frequently; T/F

A

False

389
Q

The ___ (satellite galaxies of the Milky Way) have collided with us before and will eventually be absorbed by our galaxy in an act of ___

A

Megallanic Clouds; galactic cannibalism

390
Q

As a result of galactic collisions and cannibalism, another class of galaxies is the ____

A

Active or Pecular

391
Q

___ are active elliptical galaxies

A

Radio Galaxies

392
Q

___ are active spiral galaxies

A

Seyfert

393
Q

The most distant active galaxies are called ___. They are about the size of our ___

A

quasars; solar systemm

394
Q

Local group diameter?

A

1 mpc

395
Q

Quasars are probably the ___ of active galaxies. They are most likely powered by ___ and they are the ___ things in existence.

A

core; black holes; oldest

396
Q

Quasars have very large ___ shifts

A

red

397
Q

___ can produce distorted or multiple images of more distant objects. And Einstein ___ is actually one quasar whose light has been split into four images that surround the intervening galaxy.

A

Gravitational lenses; cross

398
Q

___ is the branch of Astronomy that’s concerned with the big questions, such as how did it all begin, where are we going, what will the Universe be like in the future.

A

Cosmology

399
Q

___ pardon asks, “Why is the sky dark at night?”

A

Olbers

400
Q

Thick obscuring dark clouds blocking starlight won’t explain why the sky is dark because…

A

eventually the clouds would light up and glow brightly

401
Q

The five assumptions in Olber’s Paradox:

A

1: The universe is homogenous
2: Isotropic
3: Eternal
4: Infinite
5: Static

402
Q

The fairly even distribution of stars through space is an example of the law of ___

A

homogeneity

403
Q

The Universe is ___; it looks about the same no matter where you are

A

Isotropic

404
Q

Which Olber’s assumptions are wrong?

A

Universe is probably not eternal, not static

405
Q

How is the universe not static?

A

It’s expanding

406
Q

If the universe is expanding, then it was once ___. ___ billion years ago, it would have all been in one place.

A

small; 14

407
Q

He and Edwin Hubble convenience Einstein that the Universe was expanding; ___

A

LeMaitre

408
Q

Hubble used the ___ of distant galaxies to infer that they were moving ___ from us, and that they universe was ___, which led to the ___ theory

A

red shifts; away; expanding; Big Bang

409
Q

Using Hubble’s Law, (D=Vr/H), and a value of H=75 km/Mpc, if a galaxy has an observed recessional velocity of 150,000 km/sec, then its distance is ___

A

2,000 Mpc

410
Q

He dislike the Big Bang theory and came up with his Steady State theory instead:

A

Fred Hoyle

411
Q

___% of the universe is apparently made up of ___ matter. Of the matter we can see, the composition is about ___% hydrogen and ___% helium

A

90-95; dark; 75; 25

412
Q

There is no definable ___ to the Universe, therefore there is no ___ to the Universe

A

edge, center

413
Q

The universe is ___ as galaxies move ___ and ___ is created

A

expanding; outward; new space

414
Q

The cosmic ___ is fairly homogeneous, isotropic, and very cold

A

background radiation

415
Q

Quasars move at ___% the speed of light

A

90

416
Q

The farther out in space we look, the farther back in time we look - this is the phenomena of ___

A

look-back time

417
Q

There are quasars nearby that formed recently: T/F

A

False

418
Q

Galactic collisions were more frequent long ago, as the Universe was a smaller place: T/F

A

True

419
Q

The ___ theory, no longer popular, suggests that there was no beginning and there will be no end to the Universe.

A

Steady State

420
Q

The ___ theory says that everything was created out of a singularity, which expanded outward, carrying all of us with it. Evidence that supports this theory is the observed ___

A

Big Bang; Expansion

421
Q

The ___ may happen in the distant future if there is enough mass in the Universe to halt the expansion and bring everything back together again - in this case, the Universe is said to be ___. In the ___ theory, another Big Bang would then occur.

A

Big Crunch; closed; oscillating

422
Q

If the universe is ___ or ___, then it will not collapse back in on itself; If it is open, it will ___ forever. f it is ___ is will slow to a stop but no contract

A

open, flat; open; flat

423
Q

Predicted residual heat cosmic background radiation:

A

George Gamov