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Why is it so hot here in the summer?

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Presentation on theme: "Why is it so hot here in the summer?"— Presentation transcript:

1 Why is it so hot here in the summer?

2 The Earth in Space TEK 8.7A – the student knows the effects resulting from cyclical movements of the Sun, Earth, and Moon. The student is expected to model and illustrate how the tilted Earth rotates on its axis, causing day and night, and revolves around the sun causing changes in seasons.

3 Rotation - Earth spinning on its axis
Earth’s rotation on its axis causes day and night It takes 24 hours for Earth to rotate once on its axis Earth rotates in a counter- clockwise direction Earth rotates at about 1,600 kilometers per hour Rotation Animation Day and Night Song

4 The movement of one object around another object
Revolution The movement of one object around another object Earth travels (revolves) around the sun One complete revolution around the sun equals a year It is a curved path (elliptical) followed by Earth as it moves around the Sun Earth’s orbit is about 365 ¼ days (Leap year every four years)

5 Revolution

6 Now You Try! Stand in place, and make one complete turn (You have just rotated) Take a trip around your chair (You have just revolved Do you think you can rotate and revolve at the same time? Try it now!

7 Think about what a spinning top, a race car on an oval track, and a globe have in common

8 Turn to your neighbor and explain…
What is the difference between Earth’s rotation and Earth’s revolution?

9 Earth in Space Earth revolves rotates On its axis Around the sun
causing Years Day and night

10 So now you understand day and night – What about seasons?
A Year in 40 seconds

11 Tilt A Whirl! Earth has seasons because its axis is tilted as it revolves around the sun If Earth’s axis were straight up and down, temperatures would remain constant year round (no seasons)

12 Seasons Seasons are caused by the tilt in Earth’s axis
The tilt causes uneven heating by the sun (seasons)

13 Why is it warmer near the equator than near the poles?
At the equator - sunlight hits Earth’s surface more directly Near the north and south poles - sunlight hits Earth’s surface at an angle (energy from the sun is spread out over a greater area)

14 The Earth's axis is tilted by 23.5°
The Earth’s Tilt The Earth's axis is tilted by 23.5°

15 Earth’s axis always points in same direction (towards Polaris - the North Star)

16 Earth’s Tilted Axis Earth’s axis is tilted away from the sun for part of the year and toward the sun for part of the year When tilted toward the sun – summer When tilted away from the sun - winter Note: Summer and winter are not affected by changes in Earth’s distance from the sun.

17

18 Summer in the Northern Hemisphere
Axis is pointing towards the sun

19 Winter in the Northern Hemisphere

20 As the Earth moves around the Sun, this axis always stays pointing in the same direction.

21 Look at the direction of the axis during each season.

22 Direct vs. Indirect Light

23 When the northern hemisphere is leaning away from the sun, the rays coming from it hits this part of the Earth at a smaller (slanted) angle compared to other parts of the world These are called indirect rays Indirect rays - same amount of energy spread over a larger area of the earth therefore it receives less energy (heat)

24 Winter Sun (Indirect) Summer Sun (Direct)
Teacher demos with a flashlight Winter Sun (Indirect) Summer Sun (Direct)

25 Winter Sun (Indirect) Summer Sun (Direct)
Teacher demos with flashlight and globe

26 Seasons Direct sunlight gets more heating
Indirect sunlight gets less heating

27 Misconception Alert! Seasons are NOT caused by the changing distance the Earth is from the Sun. The Earth travels in an elliptical orbit, so the distance does vary – but not enough to cause the change in temperature associated with seasons!

28 When the southern hemisphere is experiencing summer, the northern hemisphere has winter (what do you know about Australia?)

29 6 months later, the situation reverses, and it is now winter in the southern hemisphere since that part of the earth is now leaning away from the sun

30 The energy that hits the Earth by the Sun changes over of the year
The angle the Sun is above the horizon determines how much heat and light strike each square meter of ground

31 This means that in summer, the ground receives more energy (more heat) per square meter than in the winter.  More energy is received by the ground during the summer (high temperatures) and less energy during the winter (lower temperatures).

32 Sun’s Angle Analogy If you had $ to divide among 50 people what would each person get? If you had the same $ to divide among 100 people what would each person get? If you had the same $ to divide among 200 people, what would each person get?

33 Sun’s Angle = money Think of the money as the sun’s power
The sun always shines with the same amount of power, just like the $ If you had to spread the power over a larger area, there would be less power (heating) to go around on that area on Earth. Just like there is less money for each person if the number of people grows.

34 Changes in the Sun’s Angle
Summer Sun is more directly overhead Sun’s energy is concentrated Winter The sun is less directly overhead Sun’s energy is less concentrated

35 Seasons and Earth’s Tilt

36 Seasons Question… The amount of energy is always the same, so why do we have seasons? First reason: the earth is tilted, what’s the second reason?

37 Big Idea: The seasons are the result of: 1) the tilt of the Earth's axis, and 2) revolution around the sun If the tilt of the Earth's axis was 0° there would be no difference in how the rays from the sun hit its different regions (there would be no seasons)

38 Review Look closely at where the Sun is hitting the Earth during each season:
Point out summer solstice and winter solstice

39 Solstice Solstice: Either of the two times in the year, the summer solstice and the winter solstice, when the sun reaches its highest or lowest point in the sky at noon, marked by the longest and shortest days.

40 Make a quick T chart in your notes
Winter Solstice Summer Solstice

41 Winter Solstice The northern hemisphere is pointed furthest away from the sun The sun is directly over the Tropic of Capricorn The shortest day of the year in the northern hemisphere

42 Summer Solstice The northern hemisphere is pointed furthest toward the sun The sun is directly over the Tropic of Cancer The longest day of the year in the northern hemisphere

43 Solstices On two days each year, the noon sun is overhead at either ° S or 23.5° N – solstices. Winter Solstice 23.5° S in the northern hemisphere December 21st shortest day of the year Summer Solstice 23.5° N June 21st Longest day of the year

44 Equinox Equinox: the date (twice each year) at which the sun crosses the equator, therefore day and night are of equal length (about September 22 and March 20).

45 Make a quick T chart in your notes
Spring Equinox Fall Equinox

46 Spring and Fall Equinox
Vernal (spring) and autumnal (fall) equinox - the sun is directly over the equator Days and nights are equal in length

47 Earth in March and September
Equinox (means - Equal night) Halfway between the solstices, neither hemisphere is tilted toward or away from the sun The noon sun is directly overhead at the equator

48 Vernal (Spring) Equinox
March 21st Marks the beginning of spring in the northern hemisphere

49 Autumnal Equinox September 23rd
Marks the beginning of fall in the northern hemisphere

50 Equinoxes and Solstices

51 Videos Seasons Animation


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