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Rotation and Revolution Notes

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Presentation on theme: "Rotation and Revolution Notes"— Presentation transcript:

1 Rotation and Revolution Notes

2 Motion Terminology Rotation – to spin on an axis

3 Motion Terminology Revolution – the motion of a body around another body

4 Motion Terminology Orbit – the path that is followed around another body in space

5 Earth’s rotation The Earth rotates on its axis every 23 hours & 56 minutes. One rotation = one day Day-time – We face the Sun. Night-time - We face away from the Sun. Rotation causes day and night

6 Earth’s revolution It takes the Earth days (or rotations) to travel or revolve around the Sun once. This is called a year. Earth revolves counterclockwise around the Sun. Orbit

7 Why do we have seasons? The Earth’s orbit around the sun is NOT a perfect circle. It is an ellipse. Seasons are NOT caused by how close the Earth is to the sun. In fact, the Earth is closest to the sun around January 3 and farthest away from the sun around July 4. Ellipse

8 Seasons are the result of the tilt of the Earth's axis.
Earth’s axis is tilted 23.5°. The number of daylight hours is greater for the hemisphere, or half of Earth, that is tilted toward the Sun. The number of daylight hours is smaller for the hemisphere tilted away from the sun.

9 Why do we have seasons? Summer is warmer than winter because the Sun's rays hit the Earth at a more direct angle during summer than during winter More daylight hours in the summer

10 Seasons…in a nut shell

11 Solstices Occur twice a year Winter solstice
shortest day of the year (around December 20 or 21) first day of winter Summer Solstice longest day of the year (around June 20 or 21) First day of summer.

12 Equinoxes Occurs twice a year
Number of daylight hours equals number of nighttime hours Equinox literally means "equal night". Sunlight strikes the earth most directly at the equator.

13 Equinox The vernal (spring) equinox occurs March 20.
The autumnal (fall) equinox occurs September 22 or 23.

14 The Earth's seasons are not caused by the Earth’s distance from the Sun throughout the year.

15 Review Look closely at where the Sun’s light is hitting the Earth most directly during each season:

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