8.7A Rotation & Revolution

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Science
•
8th Grade
•
Hard
+1
Standards-aligned
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1.
FLASHCARD QUESTION
Front
What is the difference between rotation and revolution in the context of Earth?
Back
Rotation refers to the spinning of Earth on its axis, which takes approximately 24 hours and causes day and night. Revolution refers to Earth's orbit around the Sun, which takes about 365.25 days and causes the seasons.
2.
FLASHCARD QUESTION
Front
What causes day and night on Earth?
Back
Day and night are caused by the rotation of Earth on its axis. When one side of Earth faces the Sun, it experiences day, while the opposite side experiences night.
Tags
NGSS.MS-ESS1-1
3.
FLASHCARD QUESTION
Front
How does the tilt of Earth's axis affect the seasons?
Back
The tilt of Earth's axis (approximately 23.5 degrees) causes different parts of Earth to receive varying amounts of sunlight throughout the year, leading to the changing seasons.
Tags
NGSS.MS-ESS1-1
4.
FLASHCARD QUESTION
Front
What is the equator, and how does it relate to day length?
Back
The equator is an imaginary line that divides Earth into the Northern and Southern Hemispheres. Locations near the equator experience relatively consistent day lengths throughout the year, with minimal variation between seasons.
5.
FLASHCARD QUESTION
Front
What season occurs in the Southern Hemisphere when it is summer in the Northern Hemisphere?
Back
When it is summer in the Northern Hemisphere, it is winter in the Southern Hemisphere.
Tags
NGSS.MS-ESS1-1
NGSS.MS-ESS2-6
6.
FLASHCARD QUESTION
Front
What is the significance of the Earth's revolution in relation to seasons?
Back
Earth's revolution around the Sun, combined with its axial tilt, leads to the changing seasons as different hemispheres tilt toward or away from the Sun at different times of the year.
Tags
NGSS.MS-ESS1-1
7.
FLASHCARD QUESTION
Front
What is the relationship between the position of the Sun in the sky and the seasons?
Back
The position of the Sun in the sky changes with the seasons due to Earth's tilt and revolution, affecting the angle and intensity of sunlight received at different latitudes.
Tags
NGSS.MS-ESS1-1
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