Elliptical, completes one revolution around the sun every 365days,6hours, and 8minutes
Revolution
Movement of the Earth around the sun, due to the Earth'saxisbeingtilted approximately 23.5 degrees
Rotation
One full rotation of the Earth equalsoneday, Earth rotates counterclockwise
Direct rays
Light rays that are hitting the earth at 90degrees, receivingmoreenergy
Indirect rays
Light rays that hit the earth at an angle, receiving lessenergy
The equator is always hit by direct rays of the sun, which is why it is alwayswarm there
The poles are always being hit by indirectrays, which is why it is cold there
Seasons
1. Spring
2. Summer
3. Autumn
4. Winter
Spring
Starts when the day and night are the samelength on March20, weather gets warmer and sunnier, tree and plants start to grow, many animals have their babies
Summer
Begins on the longestday of the year, usually the warmest and sunniest time of the year, fruit grows on trees and plants, young animals grow bigger and stronger
Autumn
Starts when the day and night are the same length again on September21, leaves changecolor and fall from the trees, some animals collect food before winter comes
Winter
Begins on the shortestday of the year, weather is colder and there is lots of snow in some places, plants and trees stop growing, some animals hibernate
Earth has seasons because its axis is tilted
Solstices and Equinoxes
1. December 21/22 (Winter Solstice)
2. March 20/21 (Spring Equinox)
3. June 21/22 (Summer Solstice)
4. September 22/23 (Autumn Equinox)
Subsolar point
Occurs on the equinoxes, when the sun is directly overhead at the equator
Perihelion
When the Earth is nearest to the Sun, happens around January 3rd
Aphelion
When the Earth is farthest from the Sun, happens around July 4th
Direct rays
Sun's rays hit the ground at 90 degrees, each square meter receives more solar energy
Oblique rays
Sun's rays come in at an angle, each square meter receives less solar energy
Latitude
Measurement of distance north or south of the Equator, increases from 0 to 90 degrees
Different parts of the Earth receive different amounts of solar radiation due to the spherical shape of the Earth