Deck 3: Moon Phases and Eclipses

ملء الشاشة (f)
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سؤال
In most months, there are no eclipses.
استخدم زر المسافة أو
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لقلب البطاقة.
سؤال
What is a new moon?

A) The lunar phase in which the first quarter Moon approaches full moon
B) The lunar phase in which Earth's shadow is cast on the Moon
C) The lunar phase in which the Moon's shadow is cast on Earth
D) The lunar phase in which sunlight illuminates only the far side of the Moon
E) The lunar phase in which sunlight illuminates the Earth facing side of the Moon
سؤال
A "larger" Moon on the horizon is an optical illusion.
سؤال
To see a solar eclipse, you have to be in Earth's shadow.
سؤال
As the illuminated part of the Moon grows larger from new to full, it is said to "wane".
سؤال
What does a waning crescent moon mean?

A) The changing Moon between full moon and third quarter
B) The changing Moon between third quarter and new moon
C) The changing Moon between first quarter and full moon
D) The changing Moon between new moon and first quarter
E) The changing Moon between first and third quarters
سؤال
Our calendar divides the year into 30-day periods in recognition of the synodic cycle of the Moon.
سؤال
What happens every 29.5 days?

A) The Moon's Saros cycle
B) The Moon's synodic cycle
C) The Moon's sidereal cycle
D) The Moon's ecliptic season
E) The Moon's chance for a partial eclipse
سؤال
Since the Moon is about 0.5 degrees in angular diameter, about how far does it move in 24 hours across the background of the constellations?

A) 0.5 degrees
B) 1.0 degree
C) 2 degrees
D) 9 degrees
E) 13 degrees
سؤال
Predicting an eclipse is easy because all you have to do is keep track of where the Moon crosses the ecliptic.
سؤال
What produces the lunar phases?

A) The rotation of the Moon
B) The revolution of the Moon
C) The changing direction of sunlight
D) Earth's tilted axis relative to the Moon
E) The changing direction of Earth to the Moon
سؤال
What is the length of time half of the Moon stays in sunlight per full rotation?

A) 29.53 days
B) 27.3 days
C) two weeks
D) one month
E) two months
سؤال
Any location on the Moon is sunlit for three weeks and is in darkness for one week as the Moon rotates.
سؤال
The angular diameters of the Moon and Sun vary slightly because the orbits of the Moon and Earth are slightly elliptical.
سؤال
The Moon moves slowly against the background of the constellations.
سؤال
When the full Moon passes through Earth's shadow, the eclipse is visible from anywhere on Earth's dark side.
سؤال
What does a waxing gibbous moon mean?

A) The changing Moon between full moon and third quarter
B) The changing Moon between third quarter and new moon
C) The changing Moon between first quarter and full moon
D) The changing Moon between new moon and first quarter
E) The changing Moon between first and third quarters
سؤال
What are the two parts of a shadow during an eclipse?

A) total and partial
B) apogee and perigee
C) sidereal and synodic
D) waxing and waning
E) umbra and penumbra
سؤال
The geometry of a solar eclipse is the same as that of a lunar eclipse.
سؤال
When the Moon is totally eclipsed, the Moon is illuminated by some sunlight reflected by Earth's atmosphere.
سؤال
The chromosphere is often marked by eruptions on the solar surface called ____.

A) solar flares
B) prominences
C) solar nodes
D) diamond rings
E) coronal mass ejections
سؤال
Calculate the angular diameter of the Moon with these known facts: Moon's linear diameter = 3480 km
Moon's average distance from Earth = 384,000 km
Number of arc seconds in 1 radian = 2.06 x 105

A) 31 arc seconds
B) 187 arc seconds
C) 1750 arc seconds
D) 1870 arc seconds
E) 1910 arc seconds
سؤال
If the Moon is too far from Earth during a solar eclipse, the _____ does not reach Earth's surface.

A) umbra
B) ecliptic
C) prominence
D) penumbra
E) solar disk
سؤال
Due to the high temperatures of the gas, what color do prominences appear as during a solar eclipse?

A) copper
B) blue
C) pink
D) violet
E) teal
سؤال
At what point is the Moon farthest away from Earth?

A) apogee
B) perigee
C) umbra
D) penumbra
E) prominence
سؤال
What happens during a penumbral lunar eclipse?

A) Earth only partially enters the penumbra.
B) Earth enters the entire penumbra.
C) The Moon partially enters the penumbra.
D) The Moon only partially enters the umbra.
سؤال
Which part of the Sun is observable during a total solar eclipse?

A) core
B) solar disk
C) sun spots
D) photosphere
E) chromosphere
سؤال
Why can't the Moon always pass through the center of the umbra?

A) The Moon's rotation is slightly faster than its revolution around Earth.
B) The Moon's orbit is inclined by 5 degrees to the plane of Earth's orbit.
C) The Moon's synodic cycle changes a few minutes per cycle.
D) The Moon's orbit changes with the seasons.
E) The Moon is not in its full moon lunar phase.
سؤال
What happens during a partial lunar eclipse?

A) Earth only partially enters the penumbra.
B) The Sun only partially enters the umbra.
C) The Moon only partially enters the penumbra.
D) Earth only partially enters the umbra.
E) The Moon only partially enters the umbra.
سؤال
What gives the Moon a coppery glow during a total eclipse?

A) Sunlight refracted through Earth's atmosphere
B) Sunlight reflected from Earth's surface
C) Not all of the sunlight is blocked out
D) The artificial light reflected up from Earth's surface
E) The spectral emissions of the gases that make up Earth's atmosphere.
سؤال
During a total solar eclipse, what part of the Sun is often visible that we normally cannot see?

A) core
B) CMEs
C) corona
D) photosphere
E) solar wind
سؤال
At what point is the Moon closest to Earth?

A) apogee
B) perigee
C) umbra
D) penumbra
E) prominence
سؤال
What creates a total lunar eclipse?

A) The Sun passes completely through Earth's umbra.
B) The Moon passes completely through Earth's umbra.
C) The Moon passes through some of Earth's penumbra.
D) The Earth passes completely through the Moon's umbra.
E) The Earth passes through some of the Moon's penumbra.
سؤال
The ____ of the Moon and Sun vary slightly because the orbits of the Moon and Earth are slightly elliptical.

A) angular distance
B) linear diameter
C) linear distance
D) angular diameter
E) angular momentum
سؤال
The diamond ring effect is a characteristic of which phenomena?

A) full moon
B) new moon
C) lunar eclipse
D) solar eclipse
E) solar prominence
سؤال
If the Moon crosses Earth's shadow at the center of the umbra, how long will the entire eclipse last from start to finish?

A) 2 to 3 minutes
B) 7 minutes
C) 1 hour 45 minutes
D) 2 hours
E) 6 hours
سؤال
Why do prominences appear pink during a solar eclipse?

A) Because of the high temperature of the gases
B) Because the photosphere being blocked out
C) Because of the placement of the lunar disk over the Sun
D) Because the prominences interact with Earth's magnetic field
E) Because different gases are being combined in the chromosphere
سؤال
Between now and 2024, in which year will there be no opportunities for a solar eclipse?

A) 2015
B) 2016
C) 2018
D) 2021
E) 2024
سؤال
What unit would best describe the linear diameter of a planetary body?

A) arc seconds
B) arc minutes
C) degrees
D) kilometers
E) radians
سؤال
How many times does the Moon cross the ecliptic each month?

A) none
B) once
C) twice
D) three times
E) four times
سؤال
Match between columns
The closest point in the Moon's orbit
waxes
The closest point in the Moon's orbit
apogee
The closest point in the Moon's orbit
nodes
The closest point in the Moon's orbit
synodic period
The closest point in the Moon's orbit
totality
The closest point in the Moon's orbit
wanes
The closest point in the Moon's orbit
umbra
The closest point in the Moon's orbit
sidereal period
The closest point in the Moon's orbit
penumbra
The closest point in the Moon's orbit
perigee
The orbital period with respect to the stars of about 27 days
waxes
The orbital period with respect to the stars of about 27 days
apogee
The orbital period with respect to the stars of about 27 days
nodes
The orbital period with respect to the stars of about 27 days
synodic period
The orbital period with respect to the stars of about 27 days
totality
The orbital period with respect to the stars of about 27 days
wanes
The orbital period with respect to the stars of about 27 days
umbra
The orbital period with respect to the stars of about 27 days
sidereal period
The orbital period with respect to the stars of about 27 days
penumbra
The orbital period with respect to the stars of about 27 days
perigee
The illuminated portion of the Moon decreases
waxes
The illuminated portion of the Moon decreases
apogee
The illuminated portion of the Moon decreases
nodes
The illuminated portion of the Moon decreases
synodic period
The illuminated portion of the Moon decreases
totality
The illuminated portion of the Moon decreases
wanes
The illuminated portion of the Moon decreases
umbra
The illuminated portion of the Moon decreases
sidereal period
The illuminated portion of the Moon decreases
penumbra
The illuminated portion of the Moon decreases
perigee
A complete cycle of lunar phases of 29.53 days
waxes
A complete cycle of lunar phases of 29.53 days
apogee
A complete cycle of lunar phases of 29.53 days
nodes
A complete cycle of lunar phases of 29.53 days
synodic period
A complete cycle of lunar phases of 29.53 days
totality
A complete cycle of lunar phases of 29.53 days
wanes
A complete cycle of lunar phases of 29.53 days
umbra
A complete cycle of lunar phases of 29.53 days
sidereal period
A complete cycle of lunar phases of 29.53 days
penumbra
A complete cycle of lunar phases of 29.53 days
perigee
A completely eclipsed moon
waxes
A completely eclipsed moon
apogee
A completely eclipsed moon
nodes
A completely eclipsed moon
synodic period
A completely eclipsed moon
totality
A completely eclipsed moon
wanes
A completely eclipsed moon
umbra
A completely eclipsed moon
sidereal period
A completely eclipsed moon
penumbra
A completely eclipsed moon
perigee
The two points at which the Moon's orbit crosses the ecliptic
waxes
The two points at which the Moon's orbit crosses the ecliptic
apogee
The two points at which the Moon's orbit crosses the ecliptic
nodes
The two points at which the Moon's orbit crosses the ecliptic
synodic period
The two points at which the Moon's orbit crosses the ecliptic
totality
The two points at which the Moon's orbit crosses the ecliptic
wanes
The two points at which the Moon's orbit crosses the ecliptic
umbra
The two points at which the Moon's orbit crosses the ecliptic
sidereal period
The two points at which the Moon's orbit crosses the ecliptic
penumbra
The two points at which the Moon's orbit crosses the ecliptic
perigee
The illuminated portion of the Moon increases
waxes
The illuminated portion of the Moon increases
apogee
The illuminated portion of the Moon increases
nodes
The illuminated portion of the Moon increases
synodic period
The illuminated portion of the Moon increases
totality
The illuminated portion of the Moon increases
wanes
The illuminated portion of the Moon increases
umbra
The illuminated portion of the Moon increases
sidereal period
The illuminated portion of the Moon increases
penumbra
The illuminated portion of the Moon increases
perigee
The region of partial shadow where sunlight is dimmed
waxes
The region of partial shadow where sunlight is dimmed
apogee
The region of partial shadow where sunlight is dimmed
nodes
The region of partial shadow where sunlight is dimmed
synodic period
The region of partial shadow where sunlight is dimmed
totality
The region of partial shadow where sunlight is dimmed
wanes
The region of partial shadow where sunlight is dimmed
umbra
The region of partial shadow where sunlight is dimmed
sidereal period
The region of partial shadow where sunlight is dimmed
penumbra
The region of partial shadow where sunlight is dimmed
perigee
The region of total shadow
waxes
The region of total shadow
apogee
The region of total shadow
nodes
The region of total shadow
synodic period
The region of total shadow
totality
The region of total shadow
wanes
The region of total shadow
umbra
The region of total shadow
sidereal period
The region of total shadow
penumbra
The region of total shadow
perigee
The farthest point in the Moon's orbit
waxes
The farthest point in the Moon's orbit
apogee
The farthest point in the Moon's orbit
nodes
The farthest point in the Moon's orbit
synodic period
The farthest point in the Moon's orbit
totality
The farthest point in the Moon's orbit
wanes
The farthest point in the Moon's orbit
umbra
The farthest point in the Moon's orbit
sidereal period
The farthest point in the Moon's orbit
penumbra
The farthest point in the Moon's orbit
perigee
سؤال
Because the _______________ of the Moon and the Sun vary slightly, the disk of the Moon is sometimes too small to cover the disk of the Sun.
سؤال
After one _______________. of 18 years 11 1/3 days, the pattern of eclipses repeats.
سؤال
Eclipses can occur only when, viewed from Earth, the Sun is near one of the _______________. of the Moon's orbit.
سؤال
A lunar eclipse can only occur when the Moon is ____

A) full
B) new
C) waxing
D) waning
E) rising
سؤال
Why can't a lunar eclipse happen at every full moon?
سؤال
If eclipses occur in repeatable patterns, then explain why an eclipse is not visible from the same place on Earth after one Saros cycle.
سؤال
Explain why "the dark side of the Moon" is an incorrect statement.
سؤال
What are three common misconceptions about the Moon and how would you provide the correct explanation for those misconceptions?
سؤال
During the _______________ phase, sunlight illuminates the far side of the Moon, and the side you see is in darkness.
سؤال
Eclipses can occur only when, viewed from Earth, the Sun is near one of the ____ of the Moon's orbit.

A) nodes
B) points
C) phases
D) paths
E) ecliptics
سؤال
A(n) _______________ can occur only at a full Moon if the Moon's path carries it through the shadow of Earth.
سؤال
What astronomical period takes 18 years 11 1/3 days to complete?

A) synodic cycle
B) lunar phase cycle
C) eclipse season
D) sidereal period
E) Saros cycle
سؤال
If the Moon passes only partially into the umbra, we witness a(n) _______________.
سؤال
Why does the Moon appear reddish during a total lunar eclipse and not go completely dark?
سؤال
The sidereal period is _______________ days long, the time it takes the Moon to circle the sky once and return to the same position relative to the stars.
سؤال
A solar eclipse can only occur when the Moon is ____

A) full
B) new
C) waning
D) waxing
E) rising
سؤال
A(n) _______________ is the changing phase the week between first quarter and full moon.
سؤال
How many Saros cycles does it take for the same eclipse to occur at about the same location on Earth?

A) one cycle
B) three cycles
C) 18 cycles
D) 22 cycles
E) 54 cycles
سؤال
What is the safest way or method to observe a solar eclipse?

A) using a telescope
B) wearing  sunglasses
C) by observing with your naked eyes
D) through a pinhole projection
E) through a UV filter held up to the sky
سؤال
A(n) _______________ occurs when the Moon moves between Earth and the Sun.
سؤال
The _______________ formula expresses the relationship of the linear (true) diameter, the angular (apparent) diameter, and the distance, of any object.
سؤال
What are the two conditions for an eclipse?
سؤال
The safest and simplest way to observe the partial phases of a solar eclipse is to use _______________  projection .
سؤال
What is an eclipse season?
سؤال
How would you explain to your friend, who knows nothing about astronomy, the way to predict the next eclipse of the Sun?
سؤال
Total lunar eclipses tend to be darkest when the Moon's orbit carries it through the center of the _______________.
سؤال
Describe all that you would see during a total eclipse of the Sun.
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Deck 3: Moon Phases and Eclipses
1
In most months, there are no eclipses.
True
2
What is a new moon?

A) The lunar phase in which the first quarter Moon approaches full moon
B) The lunar phase in which Earth's shadow is cast on the Moon
C) The lunar phase in which the Moon's shadow is cast on Earth
D) The lunar phase in which sunlight illuminates only the far side of the Moon
E) The lunar phase in which sunlight illuminates the Earth facing side of the Moon
The lunar phase in which sunlight illuminates only the far side of the Moon
3
A "larger" Moon on the horizon is an optical illusion.
True
4
To see a solar eclipse, you have to be in Earth's shadow.
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5
As the illuminated part of the Moon grows larger from new to full, it is said to "wane".
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6
What does a waning crescent moon mean?

A) The changing Moon between full moon and third quarter
B) The changing Moon between third quarter and new moon
C) The changing Moon between first quarter and full moon
D) The changing Moon between new moon and first quarter
E) The changing Moon between first and third quarters
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7
Our calendar divides the year into 30-day periods in recognition of the synodic cycle of the Moon.
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8
What happens every 29.5 days?

A) The Moon's Saros cycle
B) The Moon's synodic cycle
C) The Moon's sidereal cycle
D) The Moon's ecliptic season
E) The Moon's chance for a partial eclipse
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9
Since the Moon is about 0.5 degrees in angular diameter, about how far does it move in 24 hours across the background of the constellations?

A) 0.5 degrees
B) 1.0 degree
C) 2 degrees
D) 9 degrees
E) 13 degrees
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10
Predicting an eclipse is easy because all you have to do is keep track of where the Moon crosses the ecliptic.
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11
What produces the lunar phases?

A) The rotation of the Moon
B) The revolution of the Moon
C) The changing direction of sunlight
D) Earth's tilted axis relative to the Moon
E) The changing direction of Earth to the Moon
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12
What is the length of time half of the Moon stays in sunlight per full rotation?

A) 29.53 days
B) 27.3 days
C) two weeks
D) one month
E) two months
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13
Any location on the Moon is sunlit for three weeks and is in darkness for one week as the Moon rotates.
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14
The angular diameters of the Moon and Sun vary slightly because the orbits of the Moon and Earth are slightly elliptical.
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15
The Moon moves slowly against the background of the constellations.
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16
When the full Moon passes through Earth's shadow, the eclipse is visible from anywhere on Earth's dark side.
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17
What does a waxing gibbous moon mean?

A) The changing Moon between full moon and third quarter
B) The changing Moon between third quarter and new moon
C) The changing Moon between first quarter and full moon
D) The changing Moon between new moon and first quarter
E) The changing Moon between first and third quarters
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18
What are the two parts of a shadow during an eclipse?

A) total and partial
B) apogee and perigee
C) sidereal and synodic
D) waxing and waning
E) umbra and penumbra
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19
The geometry of a solar eclipse is the same as that of a lunar eclipse.
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20
When the Moon is totally eclipsed, the Moon is illuminated by some sunlight reflected by Earth's atmosphere.
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21
The chromosphere is often marked by eruptions on the solar surface called ____.

A) solar flares
B) prominences
C) solar nodes
D) diamond rings
E) coronal mass ejections
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22
Calculate the angular diameter of the Moon with these known facts: Moon's linear diameter = 3480 km
Moon's average distance from Earth = 384,000 km
Number of arc seconds in 1 radian = 2.06 x 105

A) 31 arc seconds
B) 187 arc seconds
C) 1750 arc seconds
D) 1870 arc seconds
E) 1910 arc seconds
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23
If the Moon is too far from Earth during a solar eclipse, the _____ does not reach Earth's surface.

A) umbra
B) ecliptic
C) prominence
D) penumbra
E) solar disk
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24
Due to the high temperatures of the gas, what color do prominences appear as during a solar eclipse?

A) copper
B) blue
C) pink
D) violet
E) teal
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25
At what point is the Moon farthest away from Earth?

A) apogee
B) perigee
C) umbra
D) penumbra
E) prominence
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26
What happens during a penumbral lunar eclipse?

A) Earth only partially enters the penumbra.
B) Earth enters the entire penumbra.
C) The Moon partially enters the penumbra.
D) The Moon only partially enters the umbra.
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27
Which part of the Sun is observable during a total solar eclipse?

A) core
B) solar disk
C) sun spots
D) photosphere
E) chromosphere
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28
Why can't the Moon always pass through the center of the umbra?

A) The Moon's rotation is slightly faster than its revolution around Earth.
B) The Moon's orbit is inclined by 5 degrees to the plane of Earth's orbit.
C) The Moon's synodic cycle changes a few minutes per cycle.
D) The Moon's orbit changes with the seasons.
E) The Moon is not in its full moon lunar phase.
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29
What happens during a partial lunar eclipse?

A) Earth only partially enters the penumbra.
B) The Sun only partially enters the umbra.
C) The Moon only partially enters the penumbra.
D) Earth only partially enters the umbra.
E) The Moon only partially enters the umbra.
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30
What gives the Moon a coppery glow during a total eclipse?

A) Sunlight refracted through Earth's atmosphere
B) Sunlight reflected from Earth's surface
C) Not all of the sunlight is blocked out
D) The artificial light reflected up from Earth's surface
E) The spectral emissions of the gases that make up Earth's atmosphere.
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31
During a total solar eclipse, what part of the Sun is often visible that we normally cannot see?

A) core
B) CMEs
C) corona
D) photosphere
E) solar wind
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32
At what point is the Moon closest to Earth?

A) apogee
B) perigee
C) umbra
D) penumbra
E) prominence
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33
What creates a total lunar eclipse?

A) The Sun passes completely through Earth's umbra.
B) The Moon passes completely through Earth's umbra.
C) The Moon passes through some of Earth's penumbra.
D) The Earth passes completely through the Moon's umbra.
E) The Earth passes through some of the Moon's penumbra.
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34
The ____ of the Moon and Sun vary slightly because the orbits of the Moon and Earth are slightly elliptical.

A) angular distance
B) linear diameter
C) linear distance
D) angular diameter
E) angular momentum
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35
The diamond ring effect is a characteristic of which phenomena?

A) full moon
B) new moon
C) lunar eclipse
D) solar eclipse
E) solar prominence
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36
If the Moon crosses Earth's shadow at the center of the umbra, how long will the entire eclipse last from start to finish?

A) 2 to 3 minutes
B) 7 minutes
C) 1 hour 45 minutes
D) 2 hours
E) 6 hours
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37
Why do prominences appear pink during a solar eclipse?

A) Because of the high temperature of the gases
B) Because the photosphere being blocked out
C) Because of the placement of the lunar disk over the Sun
D) Because the prominences interact with Earth's magnetic field
E) Because different gases are being combined in the chromosphere
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38
Between now and 2024, in which year will there be no opportunities for a solar eclipse?

A) 2015
B) 2016
C) 2018
D) 2021
E) 2024
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39
What unit would best describe the linear diameter of a planetary body?

A) arc seconds
B) arc minutes
C) degrees
D) kilometers
E) radians
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40
How many times does the Moon cross the ecliptic each month?

A) none
B) once
C) twice
D) three times
E) four times
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41
Match between columns
The closest point in the Moon's orbit
waxes
The closest point in the Moon's orbit
apogee
The closest point in the Moon's orbit
nodes
The closest point in the Moon's orbit
synodic period
The closest point in the Moon's orbit
totality
The closest point in the Moon's orbit
wanes
The closest point in the Moon's orbit
umbra
The closest point in the Moon's orbit
sidereal period
The closest point in the Moon's orbit
penumbra
The closest point in the Moon's orbit
perigee
The orbital period with respect to the stars of about 27 days
waxes
The orbital period with respect to the stars of about 27 days
apogee
The orbital period with respect to the stars of about 27 days
nodes
The orbital period with respect to the stars of about 27 days
synodic period
The orbital period with respect to the stars of about 27 days
totality
The orbital period with respect to the stars of about 27 days
wanes
The orbital period with respect to the stars of about 27 days
umbra
The orbital period with respect to the stars of about 27 days
sidereal period
The orbital period with respect to the stars of about 27 days
penumbra
The orbital period with respect to the stars of about 27 days
perigee
The illuminated portion of the Moon decreases
waxes
The illuminated portion of the Moon decreases
apogee
The illuminated portion of the Moon decreases
nodes
The illuminated portion of the Moon decreases
synodic period
The illuminated portion of the Moon decreases
totality
The illuminated portion of the Moon decreases
wanes
The illuminated portion of the Moon decreases
umbra
The illuminated portion of the Moon decreases
sidereal period
The illuminated portion of the Moon decreases
penumbra
The illuminated portion of the Moon decreases
perigee
A complete cycle of lunar phases of 29.53 days
waxes
A complete cycle of lunar phases of 29.53 days
apogee
A complete cycle of lunar phases of 29.53 days
nodes
A complete cycle of lunar phases of 29.53 days
synodic period
A complete cycle of lunar phases of 29.53 days
totality
A complete cycle of lunar phases of 29.53 days
wanes
A complete cycle of lunar phases of 29.53 days
umbra
A complete cycle of lunar phases of 29.53 days
sidereal period
A complete cycle of lunar phases of 29.53 days
penumbra
A complete cycle of lunar phases of 29.53 days
perigee
A completely eclipsed moon
waxes
A completely eclipsed moon
apogee
A completely eclipsed moon
nodes
A completely eclipsed moon
synodic period
A completely eclipsed moon
totality
A completely eclipsed moon
wanes
A completely eclipsed moon
umbra
A completely eclipsed moon
sidereal period
A completely eclipsed moon
penumbra
A completely eclipsed moon
perigee
The two points at which the Moon's orbit crosses the ecliptic
waxes
The two points at which the Moon's orbit crosses the ecliptic
apogee
The two points at which the Moon's orbit crosses the ecliptic
nodes
The two points at which the Moon's orbit crosses the ecliptic
synodic period
The two points at which the Moon's orbit crosses the ecliptic
totality
The two points at which the Moon's orbit crosses the ecliptic
wanes
The two points at which the Moon's orbit crosses the ecliptic
umbra
The two points at which the Moon's orbit crosses the ecliptic
sidereal period
The two points at which the Moon's orbit crosses the ecliptic
penumbra
The two points at which the Moon's orbit crosses the ecliptic
perigee
The illuminated portion of the Moon increases
waxes
The illuminated portion of the Moon increases
apogee
The illuminated portion of the Moon increases
nodes
The illuminated portion of the Moon increases
synodic period
The illuminated portion of the Moon increases
totality
The illuminated portion of the Moon increases
wanes
The illuminated portion of the Moon increases
umbra
The illuminated portion of the Moon increases
sidereal period
The illuminated portion of the Moon increases
penumbra
The illuminated portion of the Moon increases
perigee
The region of partial shadow where sunlight is dimmed
waxes
The region of partial shadow where sunlight is dimmed
apogee
The region of partial shadow where sunlight is dimmed
nodes
The region of partial shadow where sunlight is dimmed
synodic period
The region of partial shadow where sunlight is dimmed
totality
The region of partial shadow where sunlight is dimmed
wanes
The region of partial shadow where sunlight is dimmed
umbra
The region of partial shadow where sunlight is dimmed
sidereal period
The region of partial shadow where sunlight is dimmed
penumbra
The region of partial shadow where sunlight is dimmed
perigee
The region of total shadow
waxes
The region of total shadow
apogee
The region of total shadow
nodes
The region of total shadow
synodic period
The region of total shadow
totality
The region of total shadow
wanes
The region of total shadow
umbra
The region of total shadow
sidereal period
The region of total shadow
penumbra
The region of total shadow
perigee
The farthest point in the Moon's orbit
waxes
The farthest point in the Moon's orbit
apogee
The farthest point in the Moon's orbit
nodes
The farthest point in the Moon's orbit
synodic period
The farthest point in the Moon's orbit
totality
The farthest point in the Moon's orbit
wanes
The farthest point in the Moon's orbit
umbra
The farthest point in the Moon's orbit
sidereal period
The farthest point in the Moon's orbit
penumbra
The farthest point in the Moon's orbit
perigee
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42
Because the _______________ of the Moon and the Sun vary slightly, the disk of the Moon is sometimes too small to cover the disk of the Sun.
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43
After one _______________. of 18 years 11 1/3 days, the pattern of eclipses repeats.
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44
Eclipses can occur only when, viewed from Earth, the Sun is near one of the _______________. of the Moon's orbit.
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45
A lunar eclipse can only occur when the Moon is ____

A) full
B) new
C) waxing
D) waning
E) rising
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46
Why can't a lunar eclipse happen at every full moon?
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47
If eclipses occur in repeatable patterns, then explain why an eclipse is not visible from the same place on Earth after one Saros cycle.
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48
Explain why "the dark side of the Moon" is an incorrect statement.
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49
What are three common misconceptions about the Moon and how would you provide the correct explanation for those misconceptions?
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50
During the _______________ phase, sunlight illuminates the far side of the Moon, and the side you see is in darkness.
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51
Eclipses can occur only when, viewed from Earth, the Sun is near one of the ____ of the Moon's orbit.

A) nodes
B) points
C) phases
D) paths
E) ecliptics
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52
A(n) _______________ can occur only at a full Moon if the Moon's path carries it through the shadow of Earth.
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53
What astronomical period takes 18 years 11 1/3 days to complete?

A) synodic cycle
B) lunar phase cycle
C) eclipse season
D) sidereal period
E) Saros cycle
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54
If the Moon passes only partially into the umbra, we witness a(n) _______________.
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55
Why does the Moon appear reddish during a total lunar eclipse and not go completely dark?
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56
The sidereal period is _______________ days long, the time it takes the Moon to circle the sky once and return to the same position relative to the stars.
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57
A solar eclipse can only occur when the Moon is ____

A) full
B) new
C) waning
D) waxing
E) rising
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58
A(n) _______________ is the changing phase the week between first quarter and full moon.
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59
How many Saros cycles does it take for the same eclipse to occur at about the same location on Earth?

A) one cycle
B) three cycles
C) 18 cycles
D) 22 cycles
E) 54 cycles
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60
What is the safest way or method to observe a solar eclipse?

A) using a telescope
B) wearing  sunglasses
C) by observing with your naked eyes
D) through a pinhole projection
E) through a UV filter held up to the sky
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61
A(n) _______________ occurs when the Moon moves between Earth and the Sun.
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62
The _______________ formula expresses the relationship of the linear (true) diameter, the angular (apparent) diameter, and the distance, of any object.
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63
What are the two conditions for an eclipse?
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64
The safest and simplest way to observe the partial phases of a solar eclipse is to use _______________  projection .
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65
What is an eclipse season?
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66
How would you explain to your friend, who knows nothing about astronomy, the way to predict the next eclipse of the Sun?
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67
Total lunar eclipses tend to be darkest when the Moon's orbit carries it through the center of the _______________.
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68
Describe all that you would see during a total eclipse of the Sun.
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