aim: what is the reason for the seasons? seasons animation seasons animation

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  • Aim: What is the reason for the seasons? Seasons animation Seasons animation
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  • Seasons diagram in Northern Hemisphere
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  • A: Two Reasons: 1. The tilt of the Earths axis a. When a hemisphere is tilted toward the Sun, the season is summer b. When a hemisphere is tilted away from the Sun, the season is winter. 2. The revolution of the Earth around the Sun The hemisphere that points toward the Sun changes as the Earth revolves around the Sun = causes seasons to change.
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  • B. Earths tilt creates uneven heating The earth is tilted 23.5 o in relation to the sun. The tilt causes the sun to hit the earth at different angles.causing different temperatures. This is called the angle of insolation. Higher angles=stronger sunlight
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  • PlanetsPeriod of Revolution Around the Sun Mercury87.96 Earth days Venus224.68 Earth days Earth365.25 days Mars686.98 Earth days Jupiter11.862 Earth years Saturn29.456 Earth years Uranus84.07 Earth years Neptune164.81 Earth years Pluto (dwarf planet)247.7 years ESRT periods of revolution Which planet is going: Fastest? Slowest? The farther the planetthe faster the orbital speed!
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  • Questions If the Earths orbit is a 360o ellipse, and it takes 365.25 Earth days to revolve. Approximately how many degrees per day does the Earth travel in its revolution? A) 1B) 3C)10D)30
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  • C. Definitions 1. Revolution: The movement of a planet in its orbit around the Sun. 2. Orbit: The path a planet takes around the Sun. 3. Path is slightly oval shaped called an ellipse. An oval shaped orbit is referred to as elliptical. The farther away the planet, the longer the period of revolution. 4. Season: The change in temperature caused by the earths tilt as it revolves around the sun.
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  • D. Seasons have nothing to do with distance the N.H. is in summer when Earth is farther away from the sun.
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  • E. Animations of the The Earths Orbit seasons animation Earths Orbit
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  • Label Seasons diagram.
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  • The Tropics
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  • F. What is a solstice? When the Suns direct rays (strongest) reach farthest north or farthest south of the equator. 1. Summer Solstice in N.H. June 21 2. First Day of Summer, longest daylight hours 3. Strongest (direct) rays hit north of equator at the tropic of cancer (noon sun directly overhead) Sunrise: N of E Sunset: N of W
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  • 1.Winter Solstice in N.H. December 22 2.First Day of Winter, shortest daylight hours. 3.Strongest (direct) rays hit south of the equator at the tropic of capricorn (noon sun directly overhead) Sunrise: S of E Sunset: S of W
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  • G. What is an Equinox? 1. The direct rays of the Sun are striking at the equator (noon sun directly overhead) 2. All places on Earth have equal hours of daylight and night Autumnal Equinox First Day of Fall in N.H., September 21 Vernal Equinox First Day of Spring in N.H., March 21 Sunrise: due E Sunset: due W
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  • Varying daylight hours.
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  • Summer in the Arctic rWMNE rWMNE
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  • Seasons animation sun at solstice in north pole
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  • Summary effects of Earths tilt Seasons (Angle if insolation) Higher angle = warmer season Lower angle = cooler season Little change at the equator = no seasons Different amounts of daylight hours (duration of insolation) Longer duration = warmer days Shorter duration = cooler days
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  • Insolation Chart Intensity of Insolation (season) Date it OccursAngle of Insolation (Highest arc of the sun) Duration of Insolation ( # daylight hours) Location of the Direct Rays (Latitude) Diagram Maximum insolation (most) Summer Average Insolation Spring -------------------------- Autumn ------------------- - ---------------------------------------------------------- - ---------------------------------------------------- - Minimum insolation (least) Winter
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  • Apparent Path of the Sun Aim: Why do we get differing amounts of daylight hours during the year?
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  • A. Why do we get different amounts of daylight hours during the year? 1. The tilt of the Earths axis makes the sun appear to rise to different heights during different seasons. 2. Summer sun rises higher, takes longer to set, longer daylight hours, shorter shadows, more intensity and duration of insolation. 3. Winter sun rises lower, takes less time to set, shorter daylight hours, longer shadows, less intensity and duration of insolation.
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  • View of Sun in N. H. at noon
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  • At the equator.
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  • Noon sun at different latitudes EQUATORS. HemiN. PoleN. Hemi KNOW THESE DIAGRAMS!
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  • Factors Affecting Insolation Intensity (strength): Atmosphere (clouds) Latitude Seasons Time of Day Duration (length): Latitude Season
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  • Surface temperatures. The Earths surfaces take time to absorb and heat the airso the warmest time of the day is late afternoon, even though the strongest intensity of insolation is at noon. Same applies for seasons.strongest intensity is in June when the sun is most direct overhead, but it takes a couple of months to heat the oceans and landso the warmest month tends to be August.
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  • Climate change in history Milaknovitch cycles Earth wobbles like a top every 26000 yrs. Earths orbit becomes more elliptical every 100,000 yrs. Tilt changes from 23.5 to 24.5 every 41000 yrs. Milankovitch cycles on four different periods: 19,000, 23,000, 41,000 and 100,000 years. Thought to trigger ice ages
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