1. EARTH , SUN, andMoonInteractions

2. How does what happens up there Affect what happens down here

3. Understanding Climate and Weather What?Why and How?

4. Guide Questions Why do we have night and day? How long is a day/a year? How does sunlight hit the Earth’s surface? (equator vspoles) Why is it warmer at the equator and colder at the poles? Why are there seasons? What is climate and what causes different climates? What is longitude and latitude and how are they related to climate?

5. What causes Night and Day?

6. Length of Day: http://www.cs.sbcc.net/~physics/flash/LengthofDay.swf

7. DAY AND YEAR

8. DAY AND YEAR Rotation earth’s spinning on its axis 1,600 km/hr (rate of spin at any point along the equator) Revolution movement of earth around the sun

9. Leap Year It actually takes the Earth a little longer than a year to travel around the Sun — 365 days, 5 hours, 48 minutes, and 46 seconds, to be exact. It was the ancient Egyptians who first figured out that the solar year and the man-made calendar year didn't always match up. It was the Romans who first designated February 29 as leap day That extra day was added to February because February used to be thelast month of the year http://www.chiff.com/a/leap-year.htm

10. When do we have leap years? a leap day happens in years only divisible by four, i.e., 1996, 2000, 2004 Another stipulation ruled that no year divisible by 100 would have a leap year, except if it was divisible by 400. Thus, 1900 was not a leap year ... but 2000 was! Go figure.

11. Leap Years When was the last leap year? 2008 When is the next? 2012

13. Number of Daylight Hours Every part of Earth gets about the same number of hours of daylight per year half a year of full daylight BUT, not received the same way EQUATOR: it is delivered evenly -- exactly half a day, every single day, throughout the year. POLES: it is delivered all at once -- half a year of daylight, and then half a year of darkness. MIDLATITUDES: it is delivered in greater or lesser amounts, throughout the year -- some days having more than half a day of daylight, but others, half a year later, having less than half a day, and the average, throughout the year, being half a day of daylight per day

14. AMOUNT OF SUNSHINE However, although the different regions receive the same number of hours of daylight, they do NOT receive the same amount of sunshine the amount of sunshine which is received over a certain amount of the ground depends upon how high the Sun is in the sky (the angle of the sun’s rays)

15. How sunlight hits the Earth’s surface

16. When sunlight shines from overhead (on left), one square foot of sunlight falls on one square foot of ground. When it shines at a shallow angle (on right), each square foot of sunlight spreads out over many feet of ground. http://cseligman.com/text/sky/climate.htm

17. Effect of How Sun Hits Earth Equator always warmer (tropical) Poles always colder (arctic)

18. REASON FOR THE SEASONS

20. Earth Motions: PRECESSION Precession – Earth’s axis maintains approximately the same angle of tilt, but the direction in which the axis points continually changes. Currently, the axis points toward Polaris. In the year 14,000, it will point toward Vega. By 28,000, it will point toward Polaris again.

21. PRECESSION

22. SEASONS We have seasons because: The Earth’s axis is tilted 23.5o, so different locations receive different amounts of direct sunlight throughout the year.

24. March Equinox June Solstice December Solstice Sun September Equinox

26. SOLSTICE http://members.shaw.ca/len92/geography.htm

27. SOLSTICE http://www.kidsgeo.com/geography-for-kids/0020-solstices-and-equinoxes.php

28. Peralta Colleges, Physical Geography

29. FACTORS THAT AFFECT CLIMATE Axis or tilt of the Earth -length of day & seasons Latitude (sun angle) Elevation Precipitation (rain, snow, hail) Currents (wind, ocean)

30. What patterns do you notice with the colors?

31. Geography basics http://www.youtube.com/watch?v=95TtXYjOEv4 9 mins

33. How sunlight hits the Earth’s surface?

34. Peralta Colleges, Physical Geography

35. The latitude and longitude system Longitude lines run north-south and meet at the North and South Poles; also called meridians. Latitude lines run east-west and don't meet; also called parallels.

37. South Pole - 90° South

38. Paris, France - 48° North

40. Latitude Some important lines of latitude include The Equator – 0° The Tropic of Cancer – 23.5° N The Tropic of Capricorn – 23.5° S The Arctic Circle – 66.5° N The Antarctic Circle – 66.5° S

41. Longitude The longitude of a country is how far around the earth it lies from London = 0 ° (Prime Meridian). For example Manila - 120° East New York - 74° West The time zones follow lines of longitude that are every 15° away from London

42. Longitude London New York

43. TIME ZONES Time zones: Every 15˚, changes by 1 hour

45. day-light hours

46. precipitation levels (rainfall and snowfall)

47. average (and max, min) temperatures

48. crop growth

49. tourism

50. ecosystems

53. Tides Tides are created by the gravitational force of the Sun and Moon. The Moon’s gravity pulls Earth along an imaginary line connecting Earth and the Moon. This creates bulges of ocean water (tides). The bulges remain aligned with the Moon, so that ocean levels rise and fall as the Earth rotates.

55. This creates two tidal bulges…One facing the Moon & the other on the opposite side.

56. Oceans facing Moon bulge because they are being pulled out from the Earth.