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Unit 8 Earth in Space Seasons and Tides
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The reasons for the seasons
Fall Equinox Summer Solstice Spring Equinox Winter Solstice
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The reasons for the seasons
Earth’s Tilt Fall Equinox Summer Solstice Spring Equinox Winter Solstice SUN
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Equinox Solstice Ecliptic Plane
When the days and nights are ~ equal length (March and September) When Sun is furthest or closest to the Earth’s poles The plane in which the planets in our solar system orbit the Sun
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Aphelion Perihelion When Earth is furthest from Sun with slowest revolution When Earth is closest to Sun with fastest revolution
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Bell Work: How will precession affect the seasons?
Fall Equinox SUN Summer Solstice Spring Equinox January 2015 January 15,015
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Earth And its Moon The Moon Orbits the Earth once every 27.3 days.
The Moon and Earth orbit about the barycenter
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Lunar Eclipse When the Moon is FURTHEST from the Sun and on the ecliptic plane
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Solar Eclipse When the Moon is CLOSEST to the Sun and on the ecliptic plane
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Earth And its Moon Gravity from the Moon and Sun cause ocean tides on Earth When Sun-Earth-Moon are lined up the tides are the highest and the lowest.
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When Sun-Earth-Moon form a right angle the high tides are at their lowest and the low tides are at their highest.
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Spring Tides: When Earth, Sun and Moon are aligned; during full and new moons
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Neap Tides: When Sun and Moon form right angles to Earth; during quarter moons
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Diurnal Tides 1 high tide and 1 low tide each lunar day. (1 lunar day = 24hrs 50min) Seen in many areas of the Gulf of Mexico
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Semi-diurnal Tides 2 high tides and 2 low tides of equal size each lunar day. Seen along the East Coast of N. America
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Mixed Semi-diurnal Tides
2 high tides and 2 low tides of unequal size each lunar day. Seen along the West Coast of N. America
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First Quarter Moon New Moon Third Quarter Moon
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