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Chapter 25 Earth’s Moon.

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Presentation on theme: "Chapter 25 Earth’s Moon."— Presentation transcript:

1 Chapter 25 Earth’s Moon

2 25.1 Origin & Properties of the Moon
4 theories of origin: 1) Earth and moon formed simultaneously 2) Fission: Earth spun so fast that a chunk spun off into orbit 3) Capture: moon formed elsewhere and was caught by Earth’s gravity

3 Origin of the Moon 4) Impact Theory – planet sized object collided with Earth and debris settled into orbit, pulled together and formed the moon ** This is the currently accepted theory!

4

5 Features of the Moon Maria: large, dark areas formed from early lava flows Terrae (highlands): older, lighter areas of the moon with more craters Impact Craters: formed from meteorites Weathered and eroded by micrometeorites No atmosphere!

6 25.2 The moon’s motions Orbits the Earth in 27 1/3 days
Orbit shape is elliptical Perigee=nearest to Earth Apogee=farthest from Earth We see the same side of the moon because the Moon’s orbit around Earth takes just as long as one rotation on its axis! Orbital period = rotational period

7 Moon’s Phases

8 Lunar Eclipse Moon enters Earth’s shadow
Can only occur at a full moon phase Umbra=total shadow Penumbra=partial shadow Moon appears orange

9 Solar Eclipse Occurs when moon comes between the sun and Earth
Occurs only at the new moon phase Total time = 7.5 min Moon is dark, but sun’s corona is visible around the moon making a gold ring


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