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Published byDoris Fleming Modified over 9 years ago
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Motions of the Solar System
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Earth’s Motions Earth has Three Motions 1. Daily 2. Yearly 3. Cyclic
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Earth’s Motions Rotation Causes Day and Night Two types of Day Sidereal Sidereal Time it takes for the Earth to make one Complete rotation Time it takes for the Earth to make one Complete rotation 23 hrs and 56 minutes23 hrs and 56 minutes Solar Solar Time it takes to go from one Noon to the NextTime it takes to go from one Noon to the Next 24 hours24 hours Earth has a tilt of 23.5 Degrees One cause of the seasons One cause of the seasons
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How Fast are We Moving?
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Earth’s Motions Revolution Earth’s Yearly Journey around the Sun 365 days One Cause of the Seasons Changes the Amount of solar radiation reaching the earth Changes the Amount of solar radiation reaching the earth Aphelion Furthest point away from the sun Furthest point away from the sun Perihelion Closest point to the sun Closest point to the sun
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Annual Motion of the Earth Earth’s Annual Motion around the Sun is an ellipse Ellipse An Elongated Closed Circle An Elongated Closed Circle Sun is not at Center Sun is not at Center
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Earth’s Motions
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Precession
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The Cause of the Seasons
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Sun Position Relative to Earth Event Degrees in Latitude DateSeason Vernal Equinox 0 or Equator March 21 st Spring Summer Solstice 23.5 0 N or Tropic of Cancer June 21 st Summer Autumnal Equinox 0 or Equator September 21 st Fall Winter Solstice 23.5 0 S or Tropic of Capricorn December 21 st Winter
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No Tilt, No Seasons
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Height of Sun in Sky
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Angle of Insolation
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Length of Day and Latitude
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Latitude and Amt. of Solar Radiation
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