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Phases, Eclipses, and Tides

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Unlike a solar eclipse, a lunar eclipse can be seen anywhere on Earth that the moon is visible. Tides Tides, the rise and fall of water, every 12.5 hours or so. – PowerPoint PPT presentation

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Title: Phases, Eclipses, and Tides


1
Phases, Eclipses, and Tides
2
Phases, Eclipses, and Tides
  • As the moon revolves around Earth and Earth
    revolves around the sun, the relative positions
    of all of them change.
  • These positions cause the phases of the moon,
    eclipses, and tides.

3
Motions of the Moon
  • The moon's orbit around Earth is an oval shape.
  • The moon rotates slowly on its own axis once
    every 27.3 days.
  • Because it revolves around Earth every 27.3 days,
    a day and a year on the moon are the same
    length.
  • The same side of the moon, the near side,
    always faces Earth.
  • The far side of the moon always faces away from
    Earth, so you never see it from Earth.

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Motions of the Moon
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Phases of the Moon
  • The moon does not produce the light you see. It
    reflects light from the sun.
  • The different shapes of the moon you see from
    Earth are called phases.
  • The moon goes through all the phases each time it
    revolves around Earth and each shape may change
    every 3-4 days.
  • about once a month.

8
Phases of the Moon
9
What Causes Phases?
  • Phases are caused by changes in the relative
    positions of the moon, Earth, and the sun.
  • The sun lights the moon.
  • The phase of the moon you see depends on how much
    of the sunlit side of the moon faces Earth.

10
The Cycle of the Phases
  • During the new moon, the side of the moon facing
    Earth is not lit.
  • As the moon revolves around Earth, you see more
    and more of the lighted side of the moon every
    day, until the side of the moon you see is fully
    lit.
  • About 29.5 days after the last new moon, the
    cycle is complete, and you see a new moon again.

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Eclipses
  • In most months the moon revolves completely
    around Earth without the moon moving into Earth's
    shadow or the moon's shadow hitting Earth.
  • When the moon's shadow hits Earth or Earth's
    shadow hits the moon, an eclipse occurs.
  • An eclipse occurs when an object in space comes
    between the sun and a third object, and casts a
    shadow on that object.
  • There are two types of eclipses solar eclipses
    and lunar eclipses.

13
The Tilt of the Moon's Orbit
  • The moon's orbit is tilted with respect to
    Earth's orbit.
  • So the moon rarely goes directly between Earth
    and the sun

14
Solar Eclipses
  • A solar eclipse occurs when the moon passes
    between Earth and the sun, blocking the sunlight
    from reaching Earth.
  • The moon's shadow then hits Earth.

15
Solar Eclipses
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Total Solar Eclipses
  • The darkest part of the moon's shadow, the umbra,
    is cone-shaped.
  • From any point in the umbra, light from the sun
    is completely blocked by the moon.
  • The moon's umbra happens to be long enough so
    that the point of the cone can just reach a small
    part of Earth's surface.

17
Lunar Eclipses
  • A lunar eclipse occurs at a full moon when Earth
    is directly between the moon and the sun.
  • During a lunar eclipse, Earth blocks sunlight
    from reaching the moon.
  • The moon is then in Earth's shadow and looks dark
    from Earth.
  • Because the moon is closest to Earth's shadow
    during the full moon, lunar eclipses occur only
    at full moon.

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Lunar Eclipses
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Total Lunar Eclipses  
  • When the moon is in Earth's umbra, you see a
    total lunar eclipse.
  • You can see Earth's shadow on the moon before and
    after the total part of a lunar eclipse.
  • Unlike a solar eclipse, a lunar eclipse can be
    seen anywhere on Earth that the moon is visible.

20
Tides
  • Tides, the rise and fall of water, every 12.5
    hours or so.
  • The force of gravity pulls the moon and Earth
    (including the water on Earth's surface) toward
    each other.
  • As Earth rotates, the moon's gravity pulls water
    toward the point on Earth's surface closest to
    the moon.
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