FINAL EXAM Flashcards

1
Q

Imagine a line going through Earth, connecting the North and
South Poles. Earth rotates about
this line.

A

Earths Axis

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2
Q

If we extend the Earth’s axis what are the points where it connects with the celestial sphere?

A

North & South celestial pole

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3
Q

the equator of the celestial sphere is called the

A

Ecliptic

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4
Q

Planetary orbits are ellipses, with the Sun at one focus

A

Keplers First Law

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5
Q

path of an object
through space

A

orbit

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6
Q

one of the two
foci

A

focus

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7
Q

The imaginary line connecting Sun and planet sweeps out
equal areas in equal times.

A

Keplers Second Law

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8
Q

the speed of an orbiting planet (or moon or satellite) will change depending where it is in the orbit is called what

A

consequence

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9
Q

Square of period of planet’s orbital motion is proportional to cube of semi-major axis.

A

Keplers Third Law

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10
Q

the time it takes a
planet to travel once around
the Sun

A

Period

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11
Q

the average distance between
Earth and the Sun

A

1 AU

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12
Q

an excitation that propagates through space or a medium

A

wave

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13
Q

sound waves, water waves governed by Newton’s laws exist with a medium

A

Mechanical waves

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14
Q

light, radio waves, microwaves can travel in a vacuum (don’t need a medium to propagate) travel with velocity c = 2.99x108 m/s, which is the speed of light

A

Electromagnetic waves

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15
Q

maximum departure of a wave from the undisturbed state

A

Amplitude

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16
Q

number of meters needed for the wave to repeat itself at a given
moment in time

A

Wavelength

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17
Q

number of seconds needed for a wave to repeat itself at some point
in space

A

period

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18
Q

number of crests passing a given point per unit time

A

frequency

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19
Q

frequency = ?

A

1 / Period

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20
Q

The energy ux from a blackbody at temperature T is proportional to the
fourth power of its absolute temperature. This relationship is known as the

A

Stefan-Boltzmann law

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21
Q

The location of the spectral peak (or maximum) in the power curve of each star
can tell us its temperature

A

Wiens Law

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22
Q

______ allow us to collect
the radiation and focus it on
detectors where we can store
and analyze it

A

Telescopes

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23
Q

Types of telescopes

A

Radio, Infrared, optical, UV, x-ray, gamma rays

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24
Q

____ needs two optically acceptable surfaces, _____ only needs one: easier to make mirrors

A

Lens; Mirror

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25
Q

_______’s use mirrors or lenses to collect light

A

Optical Telescopes

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26
Q

Because this array of colors is a spectrum of light, the instrument used to
disperse the light and form the spectrum is called a

A

spectrometer

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27
Q

____ is the building block of all matter

A

atom

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28
Q

Surrounding the nucleus, there are ____ negatively charged

A

electrons

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29
Q

_______ are due to the discrete (quantum) spacing of an atom’s electron
energy levels

A

spectral lines

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30
Q

What event emits a photon of a discrete energy equal to the difference of the energy levels

A

Electron de-excites

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31
Q

an array of all wavelengths or colors of the
rainbow.

A

Continuous spectrum

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32
Q

appears as a pattern or series of bright lines; it consists of light in which only certain discrete wavelengths are present

A

emission spectrum

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33
Q

If a continuous spectrum passes through a
cool gas, atoms of the gas will absorb the same frequencies they emit
when excited describes what?

A

Absorption Spectrum

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34
Q

From sun (source of continuous spectrum) to a cloud of gas with few absorption lines results in _____. From cloud of gas with predominantly absorption lines results in ___. Straight from sun to _____ spectrum with no absorption lines

A

Absorption spectrum, emission spectrum, continuous spectrum

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35
Q

To measure stellar parallax use position of Earth in January (A)/July(B)

A

Parsec

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36
Q

Referring to parsecs: d (distance) =

A

s / angle

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37
Q

d(parsec) =

A

1 / (angle * arcseconds)

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38
Q

The magnitude equation is:

A

apparent magnitude - absolute magnitude = 5log(distance / (10pc)

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39
Q

What is the difference between apparent and absolute magnitude of a star 100 pc away?

A

5

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40
Q

A star has an apparent magnitude 10.0 and an absolute magnitude 2.5.
How far away is it?

A

316pc

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41
Q

Name the categories of stellar spectra:

A

O B A F G K M (Oh Be A Funny Goat, Kick Me)

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42
Q

Intrinsic Variable Stars Used for Distance are _____ & ________

A

Cepheid & RR Lyrae stars

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43
Q

____ stars have
essentially the same luminosity curve, with
periods from 0.5 to 1 day.

A

RR Lyrae

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44
Q

________ periods range from about 1 to 100
days.

A

Cepheid Variables

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45
Q

______ all have about the same
luminosity; knowing their apparent
magnitude allows us to calculate the
distance

A

RR Lyrae Stars

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46
Q

______ have a luminosity that is
strongly correlated with the period of
their oscillations; once the period is
measured, the luminosity is known and
we can proceed as above

A

Cepheids

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47
Q

___ gas is found in Emission
nebulae: hot, glowing area associated with the
formation of large stars.

A

ionized hydrogen(H*)

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48
Q

Found in cold regions
without stars between dust clouds

A

atomic hydrogen(H)

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49
Q

Found in cold dark
dust clouds

A

Molecular hydrogen(H2)

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50
Q

______ are composed of atomic
hydrogen gas that is ionized by near-by stars and are located in which region

A

emission nebulae; HII

51
Q

____ plots stellar luminosity versus surface temperature

A

HR Diagram

52
Q

This region is
where star formation occurs

A

molecular hydrogen

53
Q

The darkened curve on the HR Diagram is called the ____, as this is where most stars are

A

Main sequence

54
Q

these stars are hot but not very luminous, as they are quite small

A

White Dwarfs

55
Q

the brightest stars in the sky appear bright because of their

A

enormous luminosities and not their proximity

56
Q

____ giants are toward the start of the main sequence

57
Q

____ giants are above the end of the main sequence

58
Q

____ percent of stars lie on
the main sequence

59
Q

___ percent of stars are red giants

60
Q

___ percent of stars are white dwarves

61
Q

_____ lie under the main sequence

A

White dwarfs

62
Q

On the HR diagram, The shape of the paths is similar, but they wind up in
different places on the main
sequence depending on their

63
Q

____ causes a star to burn hydrogen in the surrounding shell.The core contracts and heats; the outer atmosphere expands and cools.

A

Once hydrogen is gone

64
Q

Helium begins to fuse in the core & The star expands into a red giant as the core
continues to collapse describes what

A

Helium Flash

65
Q

Only stars with a end life mass of less than 1.4 times the mass of the Sun (called
_____________) will end their cycle as white dwarfs

A

Chandrasekhar limit

66
Q

The collapsing core can reach a stable state as a crushed ball made mainly of neutrons, which astronomers call a

A

neutron star

67
Q

loose, irregular cluster, found mainly
in the plane of the Milky Way

A

open cluster

68
Q

spherical cluster of stars with the
absence of massive main-sequence stars, and the heavily
populated red giant region. Found away from the galactic
plane.

A

globular cluster

69
Q

________ Galaxies - no spiral arms and no disk

A

Elliptical

70
Q

____ galaxies show various degrees of flattening, ranging from systems that
are approximately spherical to those that approach the flatness of spirals.

A

Elliptical

71
Q

Star classification that have a disk and bulge, but no spiral arms, no interstellar gas. In between
ellipticals and spirals.

72
Q

______ galaxies have a wide variety of shapes. Undergoing interactions with other galaxies.

73
Q

very powerful and compact sources of energy at the centers of distant galaxies

74
Q

_____ type galaxies are generally elliptical and lenticular (S0) galaxies

75
Q

____ type galaxies are spiral and irregular galaxies

76
Q

Name the equation: v = H * d

A

Hubbles Law

77
Q

Age of the Universe of about

A

13.8 billion years

78
Q

Name the principle: the Universe is both homogeneous and isotropic

A

Cosmological

79
Q

The fate of the universe (the old theory)

A

slow expansion or decelerate back to the beginning

80
Q

The fate of the universe (the new theory)

A

The universe is expanding rapidly due to dark energy

81
Q

Arno Penzias and Robert Wilson observed the big bang known as the

A

Cosmic background Radiation

82
Q

____ percent of stuff in the universe is made of dark matter and dark energy

83
Q

The reciprocal of the Hubble constant (1/H) is a rough measure of the

A

age of the universe

84
Q

T OR F: If the expansion of the universe were accelerating, it would mean that distant Type Ia supernovae would look fainter than we would expect from measuring their redshifts and applying Hubble’s law.

85
Q

T OR F: As the universe expands, the temperature throughout the universe increases regularly

86
Q

T OR F: All the evidence currently suggests that we live in closed universe

87
Q

T OR F: The latest conclusion that astronomers have reached about the expansion of the universe is that the rate at which space is expanding is decelerating – that is, the expansion is slowing down due to the pull of gravity.

88
Q

Recent observations indicate that the universe is expanding faster today than it was a few billion years ago (that, in other words, the expansion of the universe is accelerating.) What kind of observations have led astronomers to this surprising conclusion?

A

the measurement of galaxy distances using white dwarf (type Ia) supernovae

89
Q

According to the Cosmological Principle, the universe is _____ & ______

A

isotropic and homogeneous

90
Q

Roughly how many galaxies make up our Local Group?

A

About 60 or so

91
Q

What cluster is Earth located in

A

Virgo Supercluster

92
Q

Which type of galaxy is observed to contain mostly older stars?

A

Elliptical

93
Q

In which type of galaxy are you likely to observe a significant amount of star formation?

A

Spiral irregular

94
Q

Hubbles constant is around ____ kilometers a second

95
Q

Our Milky Way Galaxy is what type of galaxy?

96
Q

The type of galaxy that consists almost entirely of old stars and is thus less blue (more yellow and reddish) than the other types is:

A

elliptical

97
Q

Edwin Hubble developed a classification scheme for galaxies. By what characteristic did he classify galaxies?

A

their shape

98
Q

Today, astronomers find compelling evidence that the energy source of the quasars and active galaxies is

A

matter falling toward a supermassive black hole at the center of a galaxy

99
Q

Which of the following objects is considered useful to astronomers as a “standard candle” for determining distances?

A

White dwarf

100
Q

Edwin Hubble was able to show that (with the exception of our nearest neighbors) the farther a galaxy is from us, the

A

faster it is moving away from us

101
Q

To calculate the redshift (𝑧) of the quasar, we can use the following formula for redshift:

A

(observed - rest) / rest

102
Q

When a quasar is moving away from us at a significant fraction of the speed of light, we can use the relativistic redshift formula to calculate the redshift (𝑧):

A

sqrt((1+B) / (1-B)) - 1

(B = v/c)

103
Q

gas and dust that lie between stars

A

interstellar matter

104
Q

reflection nebulae have a ____ cast as their interstellar dust grains preferentially reflect _____ starlight (Hint: answer is a color)

105
Q

a zone around a hot star where hydrogen atoms are ionized

A

HII Region

106
Q

The red color we see on a lot of photographs of nebulae comes from which element?

107
Q

Which of the following types of star is the coolest (has the lowest surface temperature)?

108
Q

How to calculate parallax

A

d = 1 / p (parallax angle)

109
Q

T OR F: The amount by which the spectral lines of a star is redshifted tells astronomers how fast the star is moving away from us.

110
Q

The formula relating distance, apparent brightness (also called flux), and luminosity is

A

apparent brightness = luminosity / (4π * distance^2)

111
Q

which planets revolve around the Sun in the same direction

A

All of them

112
Q

T OR F: jovian planets (being larger) rotate significantly more slowly than terrestrials

113
Q

what do all four terrestrial planets have in common?

A

they all have solid surfaces with signs of geological activity on them 

114
Q

The region around the Earth where charged particles are trapped and spiral around is called the ____ sphere

115
Q

T OR F: a comet always has a nice long tail, even when it is far from the Sun

115
Q

what wave has the longest wavelength?

A

radio waves

116
Q

T OR F: For all electromagnetic waves, the frequency multiplied by the wavelength will be the same constant number.

117
Q

Which ancient Greek thinker suggested (long before Copernicus) that the Earth is moving around the Sun?

A

Aristarchus

118
Q

T OR F: At the Earth’s equator, you would see the celestial poles on your horizon.

119
Q

A star is 230 light-years away. The light we see tonight from that star left it

A

230 years ago

120
Q

The point in the sky directly above your head at any given time is called the

121
Q

T OR F: The path that the Sun appears to make in the sky over the course of a year is called the celestial equator.

122
Q

The scientist who first devised experimental tests to demonstrate the validity of the heliocentric model of the solar system was