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Transcript
Seasons activity Explore the causes of the seasons Kit contents: Globe, 2 golf tees (tape to the globe before class), tape, flashlight Key concepts: Science Standards: Student knows that the tilt of the Earth on its own axis as it rotates and revolves around the Sun causes changes in season, length of day and energy available (SC.E.1.2.1). Student knows that a model of something is different from the real thing, but can be used to learn something about the real thing (SC.H.1.2.5). Basic Procedure 1. You’ll need five students for this activity. One student takes the flashlight and plays the Sun. The other four students will play Earth during each of the four seasons of the year. 2. The four season students should evenly space themselves around the Sun students. 3. Using the diagram, the season students should pass the globe around the Sun. 4. As the Earth makes its orbit around the Sun, make sure the tilt always remains the same and that the Earth remains in the same position. For each stop, students should determine what season it is in each hemisphere. 5. Repeat the activity, but have students determine the season for Florida at each of the four positions. Key Knowledge Vocabulary sun - the star at the center of our solar system rotate - spin on an axis axis - imaginary line that passes through the North and South Poles revolve - travel in a path around orbit - the path taken in a revolution equator - imaginary line going all the way around Earth halfway between the North and South Poles Key Concepts The cycle of day and night occurs because the Earth rotates around its axis. A year is the length of time it takes the Earth to revolve around the sun. Seasons are caused by the tilt of the Earth's axis. During the summer, the Northern hemisphere is tilted toward the sun, resulting in more hours of daylight and more direct sun rays. In the winter, the opposite is true. The day when the amount of daylight is the greatest is called the summer solstice (June 20 or 21, in the Northern Hemisphere). The day when the amount of daylight is least is the winter solstice (Dec 21 or 22). The equinoxes are when the hours of daylight and darkness are about equal, and the sun rises in the east and set in the west (September 22 or 23, March 20 or 21). Seasons Data Key: Daylight Hours Across the Globe Time is indicated as number of hours (h) and number of minutes (m) City 1–Jan 1–Feb 1–Mar 1–Apr 1–May 1–Jun 1–Jul 1–Aug 1–Sep 1–Oct 1–Nov 1–Dec Miami, Florida 10h 34m 11h 00m 12h 18m 12h 25m 13h 07m 14h 18m 14h 24m 14h 00m 12h 40m 12h 35m 11h 11m Nome, Alaska 4h 53m 7h 02m 10h 03m 13h 35m 17h 36m 21h 17m 22h 09m 18h 04m 15h 16m 11h 19m 8h 5h 31m 36m Singapore 12h 04m 12h 04m 12h 05m 12h 07m 12h 50m 12h 51m 12h 11m 12h 10m 12h 08m 12h 06m 12h 04m Seattle, Washington 9h 12m 10h 15m 11h 04m 13h 31m 15h 18m 15h 42m 16h 34m 15h 36m 13h 22m 11h 41m 10h 9h 24m 39m Vostok, Antarctica 24h 00m 24h 00m 19h 01m 14h 40m 0h 00m 0h 00m 0h 00m 0h 00m 7h 14m 15h 14m 24h 00m 24h 00m Brisbane, Australia 14h 31m 13h 22m 13h 20m 12h 29m 11h 04m 11h 11m 11h 05m 11h 29m 11h 32m 12h 20m 13h 49m 14h 24m Punta Arenas, Chile 17h 32m 15h 27m 13h 33m 11h 22m 10h 03m 8h 32m 8h 17m 9h 27m 11h 22m 12h 46m 14h 53m 16h 33m Cape Town, South Africa 15h 03m 13h 45m 13h 20m 12h 24m 11h 26m 10h 03m 10h 36m 11h 07m 11h 23m 12h 24m 14h 08m 14h 14m Nairobi, Kenya 12h 12m 12h 10m 12h 08m 12h 06m 12h 04m 12h 03m 12h 03m 12h 04m 12h 05m 12h 07m 12h 09m 12h 09m Axial tilt of major celestial bodies Moon Object Axial tilt (°) 11h 20m 12h 03m 1.5424 Jupiter 3.13 Pluto 119.61 26.73 Eris unknown Mercury ~0.01 Mars 25.19 Saturn Venus 177.36 Ceres ~4 Uranus 97.77 Earth 23.439 Pallas ~60 Neptune 28.32 Monthly Normal and Record High and Low Temperatures for Pensacola Month Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec Rec High °F 80 82 86 96 98 101 106 107 98 92 86 81 Norm High °F 61.2 64.4 70.2 76.2 83.4 89.0 90.7 90.1 87.0 79.3 70.3 63.4 Norm Low °F 42.7 45.4 51.7 57.6 65.8 72.1 74.5 74.2 70.4 59.6 51.1 44.7 Rec Low °F 5 15 22 33 48 56 61 60 43 32 25 11 Rainfall (inches/mm) 5.3/135 4.7/119 6.4/163 3.9/99 4.4/112 6.4/163 8.0/203 6.9/175 5.8/147 4.1/104 4.5/114 4.0/102 Science Background Why does the Earth tilt? No one knows why the Earth's axis is tilted by 23.5 degrees. Some astronomers think that about 5 billion years ago, when the Earth was still very young, it was struck by a Mars-sized planet. This colossal impact could have tipped our planet over. Whatever the reason, it's a good thing - if the Earth did not tilt, countries near the poles would be cold and dark all year round. If it tilted too much, the seasons would be very extreme – like on the planet Uranus. Here the winter lasts for 42 years in total darkness! Using the sun to determine the size of the Earth In 200 B.C. Eratosthenes was the head librarian in Alexandria, Egypt. He received a letter from a friend in Syene, which lies on the Tropic of Cancer. His friend passed on the remarkable fact that on the summer solstice the sun would climb to be directly overhead at midday. The sun would shine to the bottoms of the deepest wells, and the buildings would have no shadows. In Alexandria, the sun was not directly overhead on the summer solstice. It did not shine to the bottoms of wells and a vertical stick had a shadow. How could this be? Eratosthenes figured that if the earth were flat, shadows would be the same everywhere. So the surface must be curved: a sphere. The next year he went out and measured the midday shadow of a long vertical pole on the summer solstice in Alexandria and it measured 7.2 degrees. There are 360 degrees in a circle. He divided 360 by 7.2 and found that 7.2 degrees was about one-fiftieth of a circle. He then had beatimist, surveyors trained to walk with equal steps, measure the distance between Syene and Alexandria. Multiplying the distance between Syene and Alexandria by 50, his calculated the circumference of the earth to be 24,662 miles. This is only 200 miles off of the actual circumference of the earth Temperature and seasons Summer solstice is called, in temperate climates, the first day of summer. The reason for the delay between maximum heating and maximum heat (temperature) is that it takes time to warm up the ground and water. Differences between temperatures at different places at the same latitude are related to nearby geographic features, particularly water, which exerts a moderating effect, slowly taking up heat and slowly releasing it. Length of day vs angle of sunlight There are two contributors to the warmth of the seasons, the length of the day and the angle that the sunlight hits the Earth. The rays of the summer sun, high in the sky, arrive at a steep angle and heat the land much more than those of the winter sun, which hit at a shallow angle. At steep angles, sunlight hits the ground more directly, concentrating the radiation in a narrower spot. At shallow angles, that same amount of radiation is spread further, resulting in less heating at any given spot. Although the length of the day is an important factor in explaining why summers are hot and winter cold, the angle of sunlight is probably more important. In the arctic summer, even though the sun shines 24 hours a day, it produces only moderate warmth, because it skims around the horizon and its light arrives at a low angle. Greek mythology Persephone is the daughter of Zeus and Demeter, goddess of the harvest. Persephone was such a beautiful young woman that everyone loved her, even Hades wanted her for himself. One day, when she was collecting flowers on the plain of Enna, the earth suddenly opened and Hades rose up from the gap and abducted her. None but Zeus, and the all-seeing sun, Helios, had noticed it. Broken-hearted, Demeter wandered the earth, looking for her daughter until Helios revealed what had happened. Demeter was so angry that she withdrew herself in loneliness, and the earth ceased to be fertile. Knowing this could not continue much longer, Zeus sent Hermes down to Hades to make him release Persephone. Hades grudgingly agreed, but before she went back he gave Persephone a pomegranate (or the seeds of a pomegranate, according to some sources). When she later ate of it, it bound her to underworld forever and she had to stay there one-third of the year. The other months she stayed with her mother. When Persephone was in Hades, Demeter refused to let anything grow and winter began. The Zodiac The signs of the Zodiac represent the constellations that lie in the plane of the ecliptic that the Earth travels as it revolves around the sun. If we could turn off the sun in its fixed position, then the constellation behind it determines the particular Zodiac "sign" of that time of year. The shapes and order of the constellations are available at http://www.jb.man.ac.uk/distance/strobel/nakedeye/nakedeya_files/zodiac.gif. Script Idea What we are going to talk about today -- seasons! What are seasons? While we might think there is a "correct" answer to this question, in actuality it is a vague question. In addition to winter, spring, summer and fall, here we also have hurricane season. Tropical climates typically have a wet and a dry season. People have paid attention to seasons for as long as we have known. They just haven't understood why. Many cultures have had myths about the reason for the seasons. Share the story of Persephone. Even with this myth, many Greeks still continued making scientific observations. Share the story of Eratosthenes. We have some materials here for modeling the seasons. Using the globe and the flashlight, each group should come up with a model that accounts for the seasons, the annual cycle, and the daily cycle. Explain that the Earth is tilted slightly with respect to the Earth-Sun axis. Pass out the materials and let the groups create their model. Ask the groups as you go around what season they are showing, what ideas they have on why it is a particular season. Make sure that they can demonstrate the equinoxes and solstices. Attract the students' attention. Ask them what ideas they had about what causes the seasons. They should note the length of sunlight as well as the angle of sunlight. To demonstrate the angle of sunlight effect, shine the flashlight on a piece of graph paper (or the chalkboard) at different angles. Explain that the flashlight is giving off constant energy, but at different angles that energy is distributed over different amounts of surface area. Point out that the arctic regions get 24 hours of sunlight during the solstices, but you wouldn't expect them to be hotter than Florida. Ask the students if they know about astrology, what sign they are. Explain the history of the zodiac. What might be the purpose of the zodiac? To mark the months. Present poster boards (or big post-it paper) with the zodiacs on them. Ask the students where you should place them so that they can be incorporated into the sun-Earth model. They should be placed on the walls around the room. Ask the students to demonstrate using their model why there are some stars that you see in summer and some in winter. Other challenge questions might be: Why do you see Venus at evening or dawn but never at night but you see Mars, Saturn, and Jupiter at night? Where is the moon in the model; can they account for moon phases? Where is the North Star in our model? What would the seasons be on a planet with a different tilt? Collect the globe and flashlights. Pass out the solar motion demonstrator materials (precut) and glue. Instruct the students on the assembly. Explain to the students that the solar motion demonstrator is a way of determining when and where the sun will appear to rise and set. Stress that it is not the sun travelling in the sky but rather the Earth turning. (By holding the area that says "Months" steady and turning the rest, they can more accurately reflect this.) Tell the students that we live at approximately 30 degrees north. What can they tell about the sunrise and sunset during different months? What about at different latitudes? Refer to the idea of solstice and equinox. Explain when they fall. What can the students tell about them using their demonstrator? They should find that the sun is at its highest point in June, that all latitudes have sunrise and sunset in the due east and west at the equinox, that the North Pole doesn't have its sun set at the summer solstice, among other things. Present the daylight hours table. Ask the students to predict the approximate latitudes of the different cities. Ask the students why July and August are hotter than June when the longest day is June. Alternate Ideas Make a Solar Motion Demonstrator. Note that Pensacola is at 30 degrees N. Consider precutting the materials with an xacto knife to save time. Printing the materials on cardstock is adequate for strength. Signs of the Zodiac