

Solar Energy and Earth's Position
Interactive Video
•
Geography
•
6th - 8th Grade
•
Practice Problem
•
Hard
Patricia Brown
FREE Resource
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7 questions
Show all answers
1.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the significance of the equator in terms of solar energy?
It is where the Sun is directly overhead at noon during the equinoxes.
It is the line where the Sun never sets.
It is the line where the Sun is directly overhead at noon during the solstices.
It marks the boundary between the northern and southern hemispheres.
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
How does the Earth's axial tilt affect solar energy distribution?
It causes the Earth to receive more solar energy at the poles.
It has no effect on solar energy distribution.
It results in varying solar energy distribution across different parts of the Earth.
It causes the Earth to receive equal solar energy everywhere.
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
During the winter solstice, where is the Sun directly overhead?
The Tropic of Cancer
The Equator
The Tropic of Capricorn
The Arctic Circle
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What happens in the Arctic Circle during the winter solstice?
The Sun is directly overhead.
There is 24 hours of daylight.
There is 24 hours of darkness.
Day and night are of equal length.
5.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the significance of the Tropic of Cancer?
It is where the Sun is directly overhead at noon during the winter solstice.
It marks the boundary of the polar circles.
It is the line where day and night are always equal.
It is where the Sun is directly overhead at noon during the summer solstice.
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What occurs at the equator during the spring equinox?
There is 24 hours of daylight.
The Sun is directly overhead at noon.
There is 24 hours of darkness.
The Sun is directly overhead at midnight.
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the phenomenon of polar night?
A period of continuous darkness at the poles.
A period when day and night are of equal length at the poles.
A period of continuous daylight at the poles.
A period when the Sun is directly overhead at the poles.
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