1. Do Now 4/4 1.Copy down this week’s homework and leave out your planner to be stamped. 2.Grade SEM 4.2 3.Complete your Moon Log for today. MondayTuesdayWednesdayThursdayFriday -No HW-SEM 4.3 #1-5-SEM 4.3 All-CFU for LT A tomorrow - Have a great break!

2. Minute to Win it! 1.As a table group use the iPad app “Planets” and click on “globe” to answer the following questions Where is one country that is experiencing night right now? What part of the Earth is experiencing sunrise right now?

3. SEM: Scientific Principles 84 85 What causes the daily, monthly, and yearly patterns I see on Earth? SEM: Learning Targets SEM 2: The Earth is 4 times the diameter of the moon. The Sun is 109 times the diameter of the Earth. The Earth orbits the sun and the moon orbits the Earth. SEM 3: The Sun is higher in the sky in the summer and lower in the winter at solar noon. Shadows are long in the morning, shorter at solar noon, and long in the evening. SEM 4.1: The side of the Earth facing the sun is day and facing away is night. Seasons are caused by the tilt of the Earth relative to the Sun as it orbits the Sun. Equinox (fall and spring) is when the poles are equal distance from the sun and Solstice (winter and summer) is when one pole is pointed most towards the sun. SEM 4.2: The Earth rotates counter clockwise when viewed from the Northern Hemisphere. We know that the tilt of the Earth does not change through out the year because the North Pole always points towards Polaris.

4. Why do we have seasons? Possible ideas: A.The Earth is closer to the Sun in the Summer and further in the Winter. B.The tilt of the Earth changes through out the year. C.The side of the Earth facing the Sun will have the Sun lower in the sky. The side facing away from the Sun will have the sun higher in the sky. D.The Earth’s orbit around the Sun allows one pole to point more towards the sun and one pole more away from the sun at different points in the orbit.

5. Crash Course

6. Now 1.Trim and tape SEM 4.3 on page 103 2.Learning Target: I can use evidence to infer the causes of day, night, and seasons 3.First thoughts: 4.Table of Contents

7. Click “latitude/longitude” Type in latitude and longitude from your worksheet Go To Location

8. Click on the date. Use the up and down arrows to change the date.

9. 4. Set the “Time Flow Rate” to 3000x. 5. Start time by clicking “Run Time Forward” button. 7. Click “Stop” when the Sun is “rising” above the horizon. 8. What direction is the sun rising in? 9. What time is it?

10. EIS book page 28

11. 10. Start time by clicking “Run Time Forward” button. 11. Click “Stop” when the Sun is at solar noon. 12. What is the angle of separation? 13. What time is it?

12. 14. Start time by clicking “Run Time Forward” button. 15. Click “Stop” when the Sun is “setting” below the horizon. 16. What direction is the sun setting in? 17. What time is it?

13. Easiest way to complete data. Click down arrow by Date

14. Record the times of: Sunrise Solar Noon Sunset You can click on each time to go to that time.

15. If time says “UT” instead of “AM or PM”, uncheck “Display Universal Time”

16. If the Sun does not fit in the same screen as your horizon at solar noon...

17. RSQ #1 p101: On May 18, th Cairo, Egypt (30° N) has 14 Hours of day light. Using the map on my homepage and Goggle Map, what city would have 10 hours of day light on May 18 th ? Explain. Cairo, Egypt 14 hrs daylight 10 hrs night30° N Unknown… 10 hrs daylight 14 hrs night30° S

18. HW: No HW PUSH IN YOUR CHAIR!!! Reminder

19. Do Now 4/5 1.Complete Moon Log

20. Computers Left-hand elbow partners get computers – Table 1 – computers #1 and #9 – Table 2 – computers #2 and lab station computer – Table 3 – computers #3 and #10 – Table 4 – computers #4 and lab station computer – Table 5 – computers #5 and #11 – Table 6 – computers #6 and lab station computer – Table 7 – Computers #7 and #12 – Table 8 – Computers #8 and lab station computer

21. Double-check your Cities(s) Table 1: Alaska, Ecuador, Antarctica, Washington Table 2: Alaska, Ecuador, Antarctica, Washington Table 3: Alaska, Ecuador, Antarctica, Washington Table 4: Alaska, Ecuador, Antarctica, Washington Table 5: Alaska, Ecuador, Antarctica, Washington Table 6: Alaska, Ecuador, Antarctica, Washington Table 7: Alaska, Ecuador, Antarctica, Washington Table 8: Alaska, Ecuador, Antarctica, Washington

22. Double click on the Starry Night Enthusiast 6 icon. Say “Cancel” or “Close” to all popup boxes.

24. Do not view events.

25. Do not set home location.

26. 1. Open Starry Night Enthusiast and choose “Favourites” then “Horizon Shadows”

27. 2. Set the location to your specific location by “Options” then “Viewing Location” and the date 4/5/16

28. Click “latitude/longitude” Type in latitude and longitude from your worksheet Go To Location

29. Click on the date. Use the up and down arrows to change the date.

30. 4. Set the “Time Flow Rate” to 3000x. 5. Start time by clicking “Run Time Forward” button. 7. Click “Stop” when the Sun is “rising” above the horizon. 8. What direction is the sun rising in? 9. What time is it?

31. EIS book page 28

32. 10. Start time by clicking “Run Time Forward” button. 11. Click “Stop” when the Sun is at solar noon. 12. What is the angle of separation? 13. What time is it?

33. 14. Start time by clicking “Run Time Forward” button. 15. Click “Stop” when the Sun is “setting” below the horizon. 16. What direction is the sun setting in? 17. What time is it?

34. Easiest way to complete data. Click down arrow by Date

35. Record the times of: Sunrise Solar Noon Sunset You can click on each time to go to that time.

36. If time says “UT” instead of “AM or PM”, uncheck “Display Universal Time”

37. If the Sun does not fit in the same screen as your horizon at solar noon...

38. Minimize the screen using the edges until you get a circle view

39. When you maximize the screen, your Sun and horizon should fit into the same screen.

40. Now 1.Your graph should show the apparent path of the sun across the sky for all four dates at your location.

41. HW: Study Knowledge Map PUSH IN YOUR CHAIR!!! Reminder

42. Do Now 4/6 1.Complete your moon log for today. 2. Get laptops. 3. RSQ #1 p101: On May 18, th Cairo, Egypt (30° N) has 14 Hours of day light. What city would have 10 hours of day light on May 18 th ? Use Google Earth, the classroom globe, or Map App to answer. Explain.

43. RSQ #1 p101: On May 18, th Cairo, Egypt (30° N) has 14 Hours of day light. Google Earth, the classroom globe, or Map App, what city would have 10 hours of day light on May 18 th ? Explain. Cairo, Egypt 14 hrs daylight 10 hrs night30° N Unknown… 10 hrs daylight 14 hrs night30° S

44. Scientific Explanation Claim: A location at 30⁰ S would have 10 hours of day light on May 18 th. Evidence: If 30⁰ N has 14 hours of day light that means it has 10 hours of night. A place that has 10 hours of day light is the opposite so you are looking for a place on the opposite hempisphere. Reasoning: A location at 30⁰ S would have 10 hours of day light on may 18 th. This is because the Earth is tilted on its axis. On May 18 th the Northern Hemisphere is pointed more towards the Sun. This causes the Sun to be at a lower angle in the Southern Hemisphere causing shorter days and it is higher in the sky in the Northern Hemisphere causing longer days.

45. SEM 4.3 1.Complete OBSERVATIONS for your particular location. 2.Find another pair in the classroom to share/swap data with to answer all the analysis questions.

46. HW: SEM 4.3 (All) PUSH IN YOUR CHAIR, please. Reminder

47. Do Now 4/7 1.Complete your moon log for today. 2.Grade SEM 4.3 3.Take out a correcting pen

48. SEM 4.3 Graphing Your graph should show the apparent path of the sun across the sky for all four dates at your location. (Hint: How do the Spring and Fall Equinoxes compare?) Imagine that you are looking at your graph from this direction…Can you visualize how your data lines describe an arc across the sky?

49. EIS 4.3 6. Describe the pattern of sunrise and sunset times for the equator? Why do you think this is so? The sunrise and sunset times do not change significantly through out the year. This is due to the fact that the Equator is always at the same angle to the Sun.

51. EIS 4.3 7. How do sunrise and sunset times at the Antarctic compare to those in Alaska? They are almost opposite because they are far from the equator in opposite hemispheres. Alaska is not as extreme because it is closer to the equator than Antarctica is.

52. Summer on the North Pole

53. EIS 4.3 8. How does the apparent path of the Sun across the sky during summer change as you move closer to the North Pole? The Sun is lower in the sky at solar noon as you move closer the North Pole in the summer.

54. Solar Noon - Equator

55. Solar Noon - Anchorage

56. Solar Noon - North Pole

57. EIS4.3 9. How might the apparent height of the Sun in the sky and the length of daylight affect the temperature for a particular latitude? The lower the Sun is in the sky the cooler the temperature. This is because the Sun’s rays have to travel through more atmosphere when it is lower in the sky thereby losing more energy. The shorter the length of daylight hours the cooler it is because the Sun has less time to warm up the surface of the Earth.

58. The tilt of the Earth causes the sunlight to come through the atmosphere at different angle

59. Picture from Earth in Space Textbook p55

60. Summer the sun is higher in the sky Winter the sun is lower in the sky

61. SEM: Scientific Principles 84 85 What causes the daily, monthly, and yearly patterns I see on Earth? SEM: Learning Targets SEM 2: The Earth is 4 times the diameter of the moon. The Sun is 109 times the diameter of the Earth. The Earth orbits the sun and the moon orbits the Earth. SEM 3: The Sun is higher in the sky in the summer and lower in the winter at solar noon. Shadows are long in the morning, shorter at solar noon, and long in the evening. SEM 4.1: The side of the Earth facing the sun is day and facing away is night. Seasons are caused by the tilt of the Earth relative to the Sun as it orbits the Sun. Equinox (fall and spring) is when the poles are equal distance from the sun and Solstice (winter and summer) is when one pole is pointed most towards the sun. SEM 4.2: The Earth rotates counter clockwise when viewed from the Northern Hemisphere. We know that the tilt of the Earth does not change through out the year because the North Pole always points towards Polaris. SEM 4.3: The equator recieves 12 hours of day and 12 hours of night year round. As you move north in the summer the hours of day light get longer and the sun gets lower to the horizon causing less energy to reach the surface of the earth.

62. Why do we have seasons? Possible ideas: A.The Earth is closer to the Sun in the Summer and further in the Winter. B.The tilt of the Earth changes through out the year. C.The side of the Earth facing the Sun will have the Sun lower in the sky. The side facing away from the Sun will have the sun higher in the sky. D.The Earth’s orbit around the Sun allows one pole to point more towards the sun and one pole more away from the sun at different points in the orbit.

63. Why do we have seasons? Notes The Earth is tilted on its axis 23.5 degrees. As the Earth orbits the sun the Seasons change. When one pole is pointed most towards the sun it is summer (solstices). When the poles are equal distance from the sun it is fall and spring (equinox). During the summer the days are longer allowing the Earth to heat up more. During the summer the sun comes through the atmosphere at a more direct angle allowing more energy to reach the Earth.

65. Challenge Question Your friend is in Geneva Switzerland, 46 ○ N and 6 ○ E. What would the angle of separation be for your friend to see the North Star when they look into the night sky? The angle of separation = 46 ○

66. HW: CFU Tomorrow PUSH IN YOUR CHAIR, please. Reminder

67. Purpose: To promote student achievement in Earth and Space Science What it is: Tutoring, focused worktime, and assignment support What it isn’t: Supervised discipline sessions or afterschool daycare. What this means: I am not here to MAKE you do missing assignments, or FORCE you to be on-task. If you refuse to be on task, I will refer you to an administrator, and then have you dropped from 7 th Per. PCMS behavior rules are in effect, including as apply to electronic devices. Personal devices may be used to listen to music. No texting, phone calls or other web-based applications during 7 th Period. During Free Time (3:10 – 3:35) you may play school-approved computer games. 7 th Per. Science

68. Do Now 4/8 1.Complete your moon log

69. Do Now 1.Clear your desk for the CFU. 2.Diamonds collect test blinds for everyone in your table group.

70. SEM 5.1 When you are done: 1.Put the CFU in the In Box 2.Put your test blind away. 3.Collect SEM 5.1 and prep it Cut and tape it on page 105 Complete learning target and first thoughts “I can differentiate the phases of the moon and use a model to show why they occur.” Update table of contents

71. First Thoughts? Share your first thoughts in your table group. Each person reads theirs while the other table members give the reader their full attention. Anyone willing to share with the whole class?

72. What’s up with the Moon? 12345 6789101112 171819 141516 212223242526 272829 20 13 29.5 0 NewWaxing Crescent First Quarter Waxing Gibbous Full Waning Gibbous Third Quarter Waning Crescent New

73. So why do phases happen? 1.The Sun Angle Theory –As the Moon orbits, the angle the Sun hits it changes. This causes the Moon to light up more or less depending on the angle. 2.The Earth Shadow Theory –As the Moon orbits, the shadow of the Earth covers more or less of the Moon. 3.The Earth Perspective Theory –Where the Earth is relative to the Moon determines how much of the illuminated side you see.

74. HW: NONE Have a good break! PUSH IN YOUR CHAIR, please! Reminder