Deck 2: A Users Guide to the Sky

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سؤال
<strong>  Figure 2-5 Examine the accompanying figure. Which term would be the correct scientific designation for Polaris in Ursa Minoris?</strong> A) North Star B)   α Ursa Major C) -0.3 Ursa Minoris D) α Ursae Minoris E) β Ursae Minoris <div style=padding-top: 35px> Figure 2-5
Examine the accompanying figure. Which term would be the correct scientific designation for Polaris in Ursa Minoris?

A) North Star
B)   α Ursa Major
C) -0.3 Ursa Minoris
D) α Ursae Minoris
E) β Ursae Minoris
استخدم زر المسافة أو
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سؤال
From which language did the majority of star names originate?

A) Arabic
B) Latin
C) Greek
D) Spanish
E) Italian
سؤال
The constellations are an ancient heritage handed down for thousands of years as ways to tell stories of mythical heroes and monsters.
سؤال
Earth spins completely upright like a giant top.
سؤال
In ancient times, constellation boundaries were well defined.
سؤال
What is an asterism?

A) A legend or folklore association to a grouping of stars
B) Less formally defined group of stars outside the official 88 constellations
C) The council of astronomers who defined the 88 constellations
D) The northern pivot point of the celestial sphere
E) Constellations close enough to a celestial pole that they do not appear to rise from the east and set in the west
سؤال
Which ancient astronomer recorded the magnitude of stars in his star catalog and was used successfully by astronomers for generations?

A) Ptolemy
B) Copernicus
C) Galileo
D) Kepler
E) Aristotle
سؤال
The scale of apparent visual magnitudes extends into negative numbers to represent the faintest objects in the sky.
سؤال
The International Astronomical Union established 88 constellations that represent a defined area of the sky.
سؤال
Which is an example of an asterism?

A) Andromeda
B) Canis Major
C) Ursa Major
D) Big Dipper
E) Pegasus
سؤال
The sky appears to rotate eastward around Earth each day, but that is a consequence of the westward rotation of Earth.
سؤال
What was the purpose of the IAU establishing 88 official constellations?

A) To allow ancient stories of each constellation to be preserved
B) To name all constellations the same across any culture
C) To identify which constellation was created by which culture
D) To define boundaries for constellations including every part of the sky
E) To include additional, fainter stars within a constellation
سؤال
The nadir marks the point of the celestial sphere directly above your head.
سؤال
The seasons are caused by Earth's orbit moving closer to or farther from the Sun.
سؤال
Most individual star names come from Latin and have been altered through passing centuries.
سؤال
Because Earth's axis of rotation is inclined 23.4 degrees from vertical, the Sun moves into the northern sky in the spring and into the southern sky in the fall.
سؤال
Which is an asterism of Pegasus?

A) Great Square
B) Orion
C) Andromeda
D) Scorpio
E) Cassiopeia
سؤال
Astronomers describe the brightness of stars using the brilliance scale.
سؤال
Flux is a measure of the light energy from a star that hits a collecting area of one square meter in one second.
سؤال
What did the IAU establish in 1928?

A) The IAU classified Pluto as a dwarf planet.
B) The IAU published official names of all constellations.
C) The IAU recorded 88 constellations with defined boundaries.
D) The IAU recognized additional orbiting bodies in the Kuiper Belt.
E) The IAU recorded all the mythologies associated with 88 constellations.
سؤال
Within the Northern Hemisphere, the vernal equinox marks the start of ____.

A) winter
B) fall
C) summer
D) spring
E) a new year
سؤال
If two stars have a magnitude difference of 5, what is their flux ratio?

A) 10.0
B) 12.6
C) 100.0
D) 250.0
E) 625.3
سؤال
Even though modern astronomers know that stars are scattered through space at different distances, they still use what scientific model to describe celestial locations in the sky?

A) apparent visual magnitude
B) Copernican revolution
C) celestial sphere
D) scientific orb
E) planetarium dome
سؤال
Which is a unit used to measure angular distance?

A) seconds
B) minutes
C) arc seconds
D) feet
E) kilometers
سؤال
When can Sirius, a favorite star of the Northern Hemisphere, be observed?

A) during summer
B) during spring
C) all year long
D) during winter
E) during fall
سؤال
<strong>  The Sky Around You - Page 18 (For the following questions) Review the accompanying figure and identify point C.</strong> A) celestial equator B) north celestial pole C) south celestial pole D) zenith E) nadir <div style=padding-top: 35px> The Sky Around You - Page 18 (For the following questions)
Review the accompanying figure and identify point C.

A) celestial equator
B) north celestial pole
C) south celestial pole
D) zenith
E) nadir
سؤال
<strong>  The Sky Around You - Page 19 In the above image, what is the observer measuring?</strong> A) angle B) arc C) distance D) angular distance E) angular momentum <div style=padding-top: 35px> The Sky Around You - Page 19
In the above image, what is the observer measuring?

A) angle
B) arc
C) distance
D) angular distance
E) angular momentum
سؤال
<strong>  Figure 2-6  The star Vega has a magnitude of 0.03. Using the accompanying figure, which object is brighter than Vega?</strong> A) Sun B) Venus C) Sirius D) Polaris E) full moon <div style=padding-top: 35px> Figure 2-6 
The star Vega has a magnitude of 0.03. Using the accompanying figure, which object is brighter than Vega?

A) Sun
B) Venus
C) Sirius
D) Polaris
E) full moon
سؤال
Why is the term  "arc" used to describe units of measure for angular distance?

A) To avoid confusion with the minutes and seconds of time
B) To describe the arc-shaped distance between the stars
C) To distinguish the base unit of 10 per degree
D) To distinguish the difference between northern and southern spheres
E) To describe the placement of the stars within each hemisphere
سؤال
Earth's rapid rotation makes its axis sweep out the shape of a cone, like a heavy top slowing down.  This motion is known as ____.

A) momentum
B) precession
C) revolution
D) precision
E) recession
سؤال
Betelgeuse is the brightest star of which constellation?

A) Orion
B) Ursa Minor
C) Ursa Major
D) Southern Cross
E) Cassiopeia
سؤال
If star A is 14.5 times brighter than star B, then what is their magnitude difference?

A) 1.2
B) 2.9
C) 63.1
D) 800
E) 6.2 x 105
سؤال
What is the flux ratio of two stars whose difference in magnitude is 2.6?

A) 6.3
B) 10.8
C) 21.3
D) 632
E) 1090
سؤال
Due to the cycle of precession, in 12,000 years, which star will replace Polaris as the guiding North Star?

A) Betelgeuse
B) Sirius
C) Vega
D) Rigel
E) Spica
سؤال
Earth's rotation is connected with a very slow celestial motion that can be detected only over _____

A) centuries
B) decades
C) a year
D) a few months
E) short brief periods
سؤال
What is the name of constellations that appear to never rise or set?

A) polar constellations
B) circumference constellations
C) circular constellations
D) celestial polar constellations
E) circumpolar constellations
سؤال
<strong>  The Sky Around You - Page 18 (For the following questions) Review the accompanying figure and identify point A.</strong> A) south point B) nadir C) zenith D) north celestial pole E) south celestial pole <div style=padding-top: 35px> The Sky Around You - Page 18 (For the following questions)
Review the accompanying figure and identify point A.

A) south point
B) nadir
C) zenith
D) north celestial pole
E) south celestial pole
سؤال
<strong>  The Sky Around You - Page 18 (For the following questions) Review the accompanying figure and identify point B.</strong> A) zenith B) north point C) celestial equator D) south celestial pole E) north celestial pole <div style=padding-top: 35px> The Sky Around You - Page 18 (For the following questions)
Review the accompanying figure and identify point B.

A) zenith
B) north point
C) celestial equator
D) south celestial pole
E) north celestial pole
سؤال
<strong>  The Sky Around You - Page 18 (For the following questions) Review the accompanying figure. Where does the celestial equator always meet the horizon?</strong> A) at the north and south celestial poles B) at the north and south poles C) at the east and west points D) at the zenith and nadir E) at the equinox <div style=padding-top: 35px> The Sky Around You - Page 18 (For the following questions)
Review the accompanying figure. Where does the celestial equator always meet the horizon?

A) at the north and south celestial poles
B) at the north and south poles
C) at the east and west points
D) at the zenith and nadir
E) at the equinox
سؤال
What is the cause for the slow movement of reference marks, such as the celestial poles and equator, to move across the sky?

A) precession
B) evolution
C) climate change
D) continental drift
E) angular revolution
سؤال
Match between columns
the angle between two lines extending from your eye to two objects in the sky
ecliptic
the angle between two lines extending from your eye to two objects in the sky
flux
the angle between two lines extending from your eye to two objects in the sky
constellation
the angle between two lines extending from your eye to two objects in the sky
magnitude scale
the angle between two lines extending from your eye to two objects in the sky
nadir
the angle between two lines extending from your eye to two objects in the sky
angular diameter
the angle between two lines extending from your eye to two objects in the sky
asterism
the angle between two lines extending from your eye to two objects in the sky
zenith
the angle between two lines extending from your eye to two objects in the sky
celestial sphere
the angle between two lines extending from your eye to two objects in the sky
angular distance
the angular distance across an object, from one edge to another
ecliptic
the angular distance across an object, from one edge to another
flux
the angular distance across an object, from one edge to another
constellation
the angular distance across an object, from one edge to another
magnitude scale
the angular distance across an object, from one edge to another
nadir
the angular distance across an object, from one edge to another
angular diameter
the angular distance across an object, from one edge to another
asterism
the angular distance across an object, from one edge to another
zenith
the angular distance across an object, from one edge to another
celestial sphere
the angular distance across an object, from one edge to another
angular distance
the point of the celestial sphere directly above your head
ecliptic
the point of the celestial sphere directly above your head
flux
the point of the celestial sphere directly above your head
constellation
the point of the celestial sphere directly above your head
magnitude scale
the point of the celestial sphere directly above your head
nadir
the point of the celestial sphere directly above your head
angular diameter
the point of the celestial sphere directly above your head
asterism
the point of the celestial sphere directly above your head
zenith
the point of the celestial sphere directly above your head
celestial sphere
the point of the celestial sphere directly above your head
angular distance
the measure of light energy striking one square meter per second
ecliptic
the measure of light energy striking one square meter per second
flux
the measure of light energy striking one square meter per second
constellation
the measure of light energy striking one square meter per second
magnitude scale
the measure of light energy striking one square meter per second
nadir
the measure of light energy striking one square meter per second
angular diameter
the measure of light energy striking one square meter per second
asterism
the measure of light energy striking one square meter per second
zenith
the measure of light energy striking one square meter per second
celestial sphere
the measure of light energy striking one square meter per second
angular distance
a scientific model of the sky
ecliptic
a scientific model of the sky
flux
a scientific model of the sky
constellation
a scientific model of the sky
magnitude scale
a scientific model of the sky
nadir
a scientific model of the sky
angular diameter
a scientific model of the sky
asterism
a scientific model of the sky
zenith
a scientific model of the sky
celestial sphere
a scientific model of the sky
angular distance
the point of the celestial sphere directly under your feet
ecliptic
the point of the celestial sphere directly under your feet
flux
the point of the celestial sphere directly under your feet
constellation
the point of the celestial sphere directly under your feet
magnitude scale
the point of the celestial sphere directly under your feet
nadir
the point of the celestial sphere directly under your feet
angular diameter
the point of the celestial sphere directly under your feet
asterism
the point of the celestial sphere directly under your feet
zenith
the point of the celestial sphere directly under your feet
celestial sphere
the point of the celestial sphere directly under your feet
angular distance
named group of stars with finite boundaries in the sky
ecliptic
named group of stars with finite boundaries in the sky
flux
named group of stars with finite boundaries in the sky
constellation
named group of stars with finite boundaries in the sky
magnitude scale
named group of stars with finite boundaries in the sky
nadir
named group of stars with finite boundaries in the sky
angular diameter
named group of stars with finite boundaries in the sky
asterism
named group of stars with finite boundaries in the sky
zenith
named group of stars with finite boundaries in the sky
celestial sphere
named group of stars with finite boundaries in the sky
angular distance
provides a measurement range for the brightness of stars
ecliptic
provides a measurement range for the brightness of stars
flux
provides a measurement range for the brightness of stars
constellation
provides a measurement range for the brightness of stars
magnitude scale
provides a measurement range for the brightness of stars
nadir
provides a measurement range for the brightness of stars
angular diameter
provides a measurement range for the brightness of stars
asterism
provides a measurement range for the brightness of stars
zenith
provides a measurement range for the brightness of stars
celestial sphere
provides a measurement range for the brightness of stars
angular distance
a less formally defined grouping of stars
ecliptic
a less formally defined grouping of stars
flux
a less formally defined grouping of stars
constellation
a less formally defined grouping of stars
magnitude scale
a less formally defined grouping of stars
nadir
a less formally defined grouping of stars
angular diameter
a less formally defined grouping of stars
asterism
a less formally defined grouping of stars
zenith
a less formally defined grouping of stars
celestial sphere
a less formally defined grouping of stars
angular distance
the apparent path of the Sun against the background of stars
ecliptic
the apparent path of the Sun against the background of stars
flux
the apparent path of the Sun against the background of stars
constellation
the apparent path of the Sun against the background of stars
magnitude scale
the apparent path of the Sun against the background of stars
nadir
the apparent path of the Sun against the background of stars
angular diameter
the apparent path of the Sun against the background of stars
asterism
the apparent path of the Sun against the background of stars
zenith
the apparent path of the Sun against the background of stars
celestial sphere
the apparent path of the Sun against the background of stars
angular distance
سؤال
If Earth rotated about its axis completely upright, what would we fail to experience?

A) holidays
B) seasons
C) weather
D) day and night
E) a 365 day year
سؤال
What is the apparent path of the Sun against the background of stars?

A) ecliptic
B) zenith
C) nadir
D) elliptic
E) shadow
سؤال
Earth _______________ once a year around the Sun.
سؤال
Explain why we have seasons and compare/contrast the cycle of seasons for both hemispheres.
سؤال
What is the Milankovitch hypothesis and what evidence is there to support this hypothesis?
سؤال
Why can someone in the United States almost always be able to observe the constellations such as Ursa Major, Cassiopeia, and Perseus?
سؤال
Which planet is often called our most brilliant "morning star"?

A) Venus
B) Jupiter
C) Mars
D) Mercury
E) Saturn
سؤال
What date is the autumnal equinox for the Southern hemisphere?

A) December 21
B) September 22
C) June 22
D) March 20
E) December 25
سؤال
In 1928, the International Astronomical Union (IAU) established _______________ official constellations with carefully defined boundaries that together include every part of the sky.
سؤال
Day and night cycles are caused by the ____ of Earth.

A) revolution
B) location
C) axis tilt
D) rotation
E) boundaries
سؤال
The eastward rotation of Earth causes the Sun, Moon, planets, and stars to move _______________ in the sky.
سؤال
Astronomers use the _______________ alphabet to identify the bright stars in a constellation in approximate order of brightness.
سؤال
During which event does the Sun reach its most southern point in the celestial sphere within the Northern hemisphere?

A) nadir
B) summer solstice
C) vernal equinox
D) autumnal equinox
E) winter solstice
سؤال
The Milankovitch hypothesis suggests that the shape of Earth's orbit, its precession, and tilted axis can influence climatic changes and thus cause _____.

A) hurricanes
B) ice ages
C) season shift
D) longer days
E) warmer weather
سؤال
Earth's axis is tilted at an angle of _______________ degrees.
سؤال
Why do many people think stars are not in the sky during the daytime?
سؤال
Why is Earth's orbit often referred to be a "nearly perfect circle" and not a true ellipse?
سؤال
The ecliptic is often called the _______________ of Earth's orbit on the sky.
سؤال
Arc seconds are _______________th of an arc minute.
سؤال
Astrology is an example of _______________.
سؤال
Scientists constructed a history of ocean temperatures using deep ocean cores that convincingly matched the predictions of the _______________, describing the cause of multiple ice ages on Earth.
سؤال
Explain why it is difficult to see Mercury in the night sky.
سؤال
Describe the process of precession.
سؤال
On the day of the _______________ in late June, Earth's Northern Hemisphere is inclined toward  the Sun.
سؤال
On the day of summer solstice, explain the position of Earth and the light received by each of the hemispheres.
سؤال
Describe the magnitude scale and compare the ancient method to the current methodology used today.
سؤال
Many of the ancient astronomers applied astrology alongside astronomy, but that no longer holds true for modern astronomers. Explain why astrology is no longer considered useful to the modern scientist.
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Deck 2: A Users Guide to the Sky
1
<strong>  Figure 2-5 Examine the accompanying figure. Which term would be the correct scientific designation for Polaris in Ursa Minoris?</strong> A) North Star B)   α Ursa Major C) -0.3 Ursa Minoris D) α Ursae Minoris E) β Ursae Minoris Figure 2-5
Examine the accompanying figure. Which term would be the correct scientific designation for Polaris in Ursa Minoris?

A) North Star
B)   α Ursa Major
C) -0.3 Ursa Minoris
D) α Ursae Minoris
E) β Ursae Minoris
α Ursae Minoris
2
From which language did the majority of star names originate?

A) Arabic
B) Latin
C) Greek
D) Spanish
E) Italian
Arabic
3
The constellations are an ancient heritage handed down for thousands of years as ways to tell stories of mythical heroes and monsters.
True
4
Earth spins completely upright like a giant top.
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5
In ancient times, constellation boundaries were well defined.
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6
What is an asterism?

A) A legend or folklore association to a grouping of stars
B) Less formally defined group of stars outside the official 88 constellations
C) The council of astronomers who defined the 88 constellations
D) The northern pivot point of the celestial sphere
E) Constellations close enough to a celestial pole that they do not appear to rise from the east and set in the west
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7
Which ancient astronomer recorded the magnitude of stars in his star catalog and was used successfully by astronomers for generations?

A) Ptolemy
B) Copernicus
C) Galileo
D) Kepler
E) Aristotle
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8
The scale of apparent visual magnitudes extends into negative numbers to represent the faintest objects in the sky.
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9
The International Astronomical Union established 88 constellations that represent a defined area of the sky.
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10
Which is an example of an asterism?

A) Andromeda
B) Canis Major
C) Ursa Major
D) Big Dipper
E) Pegasus
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11
The sky appears to rotate eastward around Earth each day, but that is a consequence of the westward rotation of Earth.
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12
What was the purpose of the IAU establishing 88 official constellations?

A) To allow ancient stories of each constellation to be preserved
B) To name all constellations the same across any culture
C) To identify which constellation was created by which culture
D) To define boundaries for constellations including every part of the sky
E) To include additional, fainter stars within a constellation
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13
The nadir marks the point of the celestial sphere directly above your head.
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14
The seasons are caused by Earth's orbit moving closer to or farther from the Sun.
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15
Most individual star names come from Latin and have been altered through passing centuries.
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16
Because Earth's axis of rotation is inclined 23.4 degrees from vertical, the Sun moves into the northern sky in the spring and into the southern sky in the fall.
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17
Which is an asterism of Pegasus?

A) Great Square
B) Orion
C) Andromeda
D) Scorpio
E) Cassiopeia
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18
Astronomers describe the brightness of stars using the brilliance scale.
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19
Flux is a measure of the light energy from a star that hits a collecting area of one square meter in one second.
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20
What did the IAU establish in 1928?

A) The IAU classified Pluto as a dwarf planet.
B) The IAU published official names of all constellations.
C) The IAU recorded 88 constellations with defined boundaries.
D) The IAU recognized additional orbiting bodies in the Kuiper Belt.
E) The IAU recorded all the mythologies associated with 88 constellations.
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21
Within the Northern Hemisphere, the vernal equinox marks the start of ____.

A) winter
B) fall
C) summer
D) spring
E) a new year
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22
If two stars have a magnitude difference of 5, what is their flux ratio?

A) 10.0
B) 12.6
C) 100.0
D) 250.0
E) 625.3
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23
Even though modern astronomers know that stars are scattered through space at different distances, they still use what scientific model to describe celestial locations in the sky?

A) apparent visual magnitude
B) Copernican revolution
C) celestial sphere
D) scientific orb
E) planetarium dome
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24
Which is a unit used to measure angular distance?

A) seconds
B) minutes
C) arc seconds
D) feet
E) kilometers
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25
When can Sirius, a favorite star of the Northern Hemisphere, be observed?

A) during summer
B) during spring
C) all year long
D) during winter
E) during fall
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26
<strong>  The Sky Around You - Page 18 (For the following questions) Review the accompanying figure and identify point C.</strong> A) celestial equator B) north celestial pole C) south celestial pole D) zenith E) nadir The Sky Around You - Page 18 (For the following questions)
Review the accompanying figure and identify point C.

A) celestial equator
B) north celestial pole
C) south celestial pole
D) zenith
E) nadir
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27
<strong>  The Sky Around You - Page 19 In the above image, what is the observer measuring?</strong> A) angle B) arc C) distance D) angular distance E) angular momentum The Sky Around You - Page 19
In the above image, what is the observer measuring?

A) angle
B) arc
C) distance
D) angular distance
E) angular momentum
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28
<strong>  Figure 2-6  The star Vega has a magnitude of 0.03. Using the accompanying figure, which object is brighter than Vega?</strong> A) Sun B) Venus C) Sirius D) Polaris E) full moon Figure 2-6 
The star Vega has a magnitude of 0.03. Using the accompanying figure, which object is brighter than Vega?

A) Sun
B) Venus
C) Sirius
D) Polaris
E) full moon
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29
Why is the term  "arc" used to describe units of measure for angular distance?

A) To avoid confusion with the minutes and seconds of time
B) To describe the arc-shaped distance between the stars
C) To distinguish the base unit of 10 per degree
D) To distinguish the difference between northern and southern spheres
E) To describe the placement of the stars within each hemisphere
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30
Earth's rapid rotation makes its axis sweep out the shape of a cone, like a heavy top slowing down.  This motion is known as ____.

A) momentum
B) precession
C) revolution
D) precision
E) recession
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31
Betelgeuse is the brightest star of which constellation?

A) Orion
B) Ursa Minor
C) Ursa Major
D) Southern Cross
E) Cassiopeia
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32
If star A is 14.5 times brighter than star B, then what is their magnitude difference?

A) 1.2
B) 2.9
C) 63.1
D) 800
E) 6.2 x 105
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33
What is the flux ratio of two stars whose difference in magnitude is 2.6?

A) 6.3
B) 10.8
C) 21.3
D) 632
E) 1090
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34
Due to the cycle of precession, in 12,000 years, which star will replace Polaris as the guiding North Star?

A) Betelgeuse
B) Sirius
C) Vega
D) Rigel
E) Spica
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35
Earth's rotation is connected with a very slow celestial motion that can be detected only over _____

A) centuries
B) decades
C) a year
D) a few months
E) short brief periods
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36
What is the name of constellations that appear to never rise or set?

A) polar constellations
B) circumference constellations
C) circular constellations
D) celestial polar constellations
E) circumpolar constellations
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37
<strong>  The Sky Around You - Page 18 (For the following questions) Review the accompanying figure and identify point A.</strong> A) south point B) nadir C) zenith D) north celestial pole E) south celestial pole The Sky Around You - Page 18 (For the following questions)
Review the accompanying figure and identify point A.

A) south point
B) nadir
C) zenith
D) north celestial pole
E) south celestial pole
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38
<strong>  The Sky Around You - Page 18 (For the following questions) Review the accompanying figure and identify point B.</strong> A) zenith B) north point C) celestial equator D) south celestial pole E) north celestial pole The Sky Around You - Page 18 (For the following questions)
Review the accompanying figure and identify point B.

A) zenith
B) north point
C) celestial equator
D) south celestial pole
E) north celestial pole
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39
<strong>  The Sky Around You - Page 18 (For the following questions) Review the accompanying figure. Where does the celestial equator always meet the horizon?</strong> A) at the north and south celestial poles B) at the north and south poles C) at the east and west points D) at the zenith and nadir E) at the equinox The Sky Around You - Page 18 (For the following questions)
Review the accompanying figure. Where does the celestial equator always meet the horizon?

A) at the north and south celestial poles
B) at the north and south poles
C) at the east and west points
D) at the zenith and nadir
E) at the equinox
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40
What is the cause for the slow movement of reference marks, such as the celestial poles and equator, to move across the sky?

A) precession
B) evolution
C) climate change
D) continental drift
E) angular revolution
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41
Match between columns
the angle between two lines extending from your eye to two objects in the sky
ecliptic
the angle between two lines extending from your eye to two objects in the sky
flux
the angle between two lines extending from your eye to two objects in the sky
constellation
the angle between two lines extending from your eye to two objects in the sky
magnitude scale
the angle between two lines extending from your eye to two objects in the sky
nadir
the angle between two lines extending from your eye to two objects in the sky
angular diameter
the angle between two lines extending from your eye to two objects in the sky
asterism
the angle between two lines extending from your eye to two objects in the sky
zenith
the angle between two lines extending from your eye to two objects in the sky
celestial sphere
the angle between two lines extending from your eye to two objects in the sky
angular distance
the angular distance across an object, from one edge to another
ecliptic
the angular distance across an object, from one edge to another
flux
the angular distance across an object, from one edge to another
constellation
the angular distance across an object, from one edge to another
magnitude scale
the angular distance across an object, from one edge to another
nadir
the angular distance across an object, from one edge to another
angular diameter
the angular distance across an object, from one edge to another
asterism
the angular distance across an object, from one edge to another
zenith
the angular distance across an object, from one edge to another
celestial sphere
the angular distance across an object, from one edge to another
angular distance
the point of the celestial sphere directly above your head
ecliptic
the point of the celestial sphere directly above your head
flux
the point of the celestial sphere directly above your head
constellation
the point of the celestial sphere directly above your head
magnitude scale
the point of the celestial sphere directly above your head
nadir
the point of the celestial sphere directly above your head
angular diameter
the point of the celestial sphere directly above your head
asterism
the point of the celestial sphere directly above your head
zenith
the point of the celestial sphere directly above your head
celestial sphere
the point of the celestial sphere directly above your head
angular distance
the measure of light energy striking one square meter per second
ecliptic
the measure of light energy striking one square meter per second
flux
the measure of light energy striking one square meter per second
constellation
the measure of light energy striking one square meter per second
magnitude scale
the measure of light energy striking one square meter per second
nadir
the measure of light energy striking one square meter per second
angular diameter
the measure of light energy striking one square meter per second
asterism
the measure of light energy striking one square meter per second
zenith
the measure of light energy striking one square meter per second
celestial sphere
the measure of light energy striking one square meter per second
angular distance
a scientific model of the sky
ecliptic
a scientific model of the sky
flux
a scientific model of the sky
constellation
a scientific model of the sky
magnitude scale
a scientific model of the sky
nadir
a scientific model of the sky
angular diameter
a scientific model of the sky
asterism
a scientific model of the sky
zenith
a scientific model of the sky
celestial sphere
a scientific model of the sky
angular distance
the point of the celestial sphere directly under your feet
ecliptic
the point of the celestial sphere directly under your feet
flux
the point of the celestial sphere directly under your feet
constellation
the point of the celestial sphere directly under your feet
magnitude scale
the point of the celestial sphere directly under your feet
nadir
the point of the celestial sphere directly under your feet
angular diameter
the point of the celestial sphere directly under your feet
asterism
the point of the celestial sphere directly under your feet
zenith
the point of the celestial sphere directly under your feet
celestial sphere
the point of the celestial sphere directly under your feet
angular distance
named group of stars with finite boundaries in the sky
ecliptic
named group of stars with finite boundaries in the sky
flux
named group of stars with finite boundaries in the sky
constellation
named group of stars with finite boundaries in the sky
magnitude scale
named group of stars with finite boundaries in the sky
nadir
named group of stars with finite boundaries in the sky
angular diameter
named group of stars with finite boundaries in the sky
asterism
named group of stars with finite boundaries in the sky
zenith
named group of stars with finite boundaries in the sky
celestial sphere
named group of stars with finite boundaries in the sky
angular distance
provides a measurement range for the brightness of stars
ecliptic
provides a measurement range for the brightness of stars
flux
provides a measurement range for the brightness of stars
constellation
provides a measurement range for the brightness of stars
magnitude scale
provides a measurement range for the brightness of stars
nadir
provides a measurement range for the brightness of stars
angular diameter
provides a measurement range for the brightness of stars
asterism
provides a measurement range for the brightness of stars
zenith
provides a measurement range for the brightness of stars
celestial sphere
provides a measurement range for the brightness of stars
angular distance
a less formally defined grouping of stars
ecliptic
a less formally defined grouping of stars
flux
a less formally defined grouping of stars
constellation
a less formally defined grouping of stars
magnitude scale
a less formally defined grouping of stars
nadir
a less formally defined grouping of stars
angular diameter
a less formally defined grouping of stars
asterism
a less formally defined grouping of stars
zenith
a less formally defined grouping of stars
celestial sphere
a less formally defined grouping of stars
angular distance
the apparent path of the Sun against the background of stars
ecliptic
the apparent path of the Sun against the background of stars
flux
the apparent path of the Sun against the background of stars
constellation
the apparent path of the Sun against the background of stars
magnitude scale
the apparent path of the Sun against the background of stars
nadir
the apparent path of the Sun against the background of stars
angular diameter
the apparent path of the Sun against the background of stars
asterism
the apparent path of the Sun against the background of stars
zenith
the apparent path of the Sun against the background of stars
celestial sphere
the apparent path of the Sun against the background of stars
angular distance
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42
If Earth rotated about its axis completely upright, what would we fail to experience?

A) holidays
B) seasons
C) weather
D) day and night
E) a 365 day year
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43
What is the apparent path of the Sun against the background of stars?

A) ecliptic
B) zenith
C) nadir
D) elliptic
E) shadow
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44
Earth _______________ once a year around the Sun.
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45
Explain why we have seasons and compare/contrast the cycle of seasons for both hemispheres.
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46
What is the Milankovitch hypothesis and what evidence is there to support this hypothesis?
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47
Why can someone in the United States almost always be able to observe the constellations such as Ursa Major, Cassiopeia, and Perseus?
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48
Which planet is often called our most brilliant "morning star"?

A) Venus
B) Jupiter
C) Mars
D) Mercury
E) Saturn
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49
What date is the autumnal equinox for the Southern hemisphere?

A) December 21
B) September 22
C) June 22
D) March 20
E) December 25
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50
In 1928, the International Astronomical Union (IAU) established _______________ official constellations with carefully defined boundaries that together include every part of the sky.
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51
Day and night cycles are caused by the ____ of Earth.

A) revolution
B) location
C) axis tilt
D) rotation
E) boundaries
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52
The eastward rotation of Earth causes the Sun, Moon, planets, and stars to move _______________ in the sky.
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53
Astronomers use the _______________ alphabet to identify the bright stars in a constellation in approximate order of brightness.
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54
During which event does the Sun reach its most southern point in the celestial sphere within the Northern hemisphere?

A) nadir
B) summer solstice
C) vernal equinox
D) autumnal equinox
E) winter solstice
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55
The Milankovitch hypothesis suggests that the shape of Earth's orbit, its precession, and tilted axis can influence climatic changes and thus cause _____.

A) hurricanes
B) ice ages
C) season shift
D) longer days
E) warmer weather
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56
Earth's axis is tilted at an angle of _______________ degrees.
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57
Why do many people think stars are not in the sky during the daytime?
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58
Why is Earth's orbit often referred to be a "nearly perfect circle" and not a true ellipse?
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59
The ecliptic is often called the _______________ of Earth's orbit on the sky.
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60
Arc seconds are _______________th of an arc minute.
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61
Astrology is an example of _______________.
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62
Scientists constructed a history of ocean temperatures using deep ocean cores that convincingly matched the predictions of the _______________, describing the cause of multiple ice ages on Earth.
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63
Explain why it is difficult to see Mercury in the night sky.
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64
Describe the process of precession.
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65
On the day of the _______________ in late June, Earth's Northern Hemisphere is inclined toward  the Sun.
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66
On the day of summer solstice, explain the position of Earth and the light received by each of the hemispheres.
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67
Describe the magnitude scale and compare the ancient method to the current methodology used today.
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68
Many of the ancient astronomers applied astrology alongside astronomy, but that no longer holds true for modern astronomers. Explain why astrology is no longer considered useful to the modern scientist.
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