
Moon Phases, Eclipses, and Tides
Authored by Tammy Rall
Science
8th Grade
NGSS covered
Used 43+ times

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17 questions
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1.
MULTIPLE CHOICE QUESTION
2 mins • 1 pt
Which statement best explains why different portions of the Moon are visible at different times of the month?
As Earth moves along its orbit, it blocks different parts of the Moon.
As the Moon moves along its orbit, it passes through Earth's shadow.
As the Moon moves along its orbit, only a fraction of it is visible from Earth.
As Earth moves along its orbit, its shadow falls on different parts of the Moon.
Tags
NGSS.MS-ESS1-1
2.
MULTIPLE CHOICE QUESTION
2 mins • 1 pt
In the fourth century BC, Aristotle observed a phenomenon in which he saw a circular shadow on the Moon. He argued that Earth was a sphere based on this observation. What phenomenon caused the shadow on the Moon?
a solar eclipse
a lunar eclipse
a spring equinox
a summer solstice
Tags
NGSS.MS-ESS1-1
3.
MULTIPLE CHOICE QUESTION
1 min • 1 pt
If the Moon did not rotate at the same rate that it revolved, which of the following would be true?
There would be no more tides.
We would no longer see eclipses.
We would be able to see all sides of the Moon.
The cycle of the Moon's phases would repeat faster.
Tags
NGSS.MS-ESS1-1
4.
MULTIPLE CHOICE QUESTION
2 mins • 1 pt
An observer at location A on Earth views the Moon when it is at position M1. Which phase of the Moon will the observer see?
full moon
new moon
third quarter
waxing gibbous
Tags
NGSS.MS-ESS1-1
5.
MULTIPLE CHOICE QUESTION
1 min • 1 pt
At which Moon position could a solar eclipse be seen from Earth?4
M1
M2
M3
M4
Tags
NGSS.MS-ESS1-1
6.
MULTIPLE CHOICE QUESTION
1 min • 1 pt
At which Moon position could a lunar eclipse be seen from Earth?
M1
M2
M3
M4
Tags
NGSS.MS-ESS1-1
7.
MULTIPLE CHOICE QUESTION
2 mins • 1 pt
Noel built a stationary three-dimensional scale model of the Earth-Sun-Moon system for a presentation to his science class. What kind of information will his model NOT be able to demonstrate?
the relative sizes of the celestial bodies
the relative distances among the celestial bodies
the relative appearance of the Moon during each phase
the relative locations of the celestial bodies during an eclipse
Tags
NGSS.MS-ESS1-1
NGSS.MS-ESS1-3
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