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Chapter 8 The Moon

Chapter 8 The Moon. Orbital Properties. Distance between Earth and Moon has been measured to accuracy of a 3 cm using lasers. Distance of the moon from earth is 384,000 km or about 240,000 miles. Physical Properties.

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Chapter 8 The Moon

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  1. Chapter 8 The Moon

  2. Orbital Properties Distance between Earth and Moon has been measured to accuracy of a 3 cm using lasers Distance of the moon from earth is 384,000 km or about 240,000 miles

  3. Physical Properties Escape speed-the speed needed for any object to escape forever from its surface.

  4. Rotation Rates Moon’s rotation rate is the same as the time it takes to make one revolution, so the same side of the Moon always faces Earth. Rotational Period: 27.3 days Revolution: 29.5 days

  5. Moon Phases Phases are due to different amounts of sunlit portion being visible from Earth New Moon-no part of the moon is visible from earth Waning Moon-part of the moon that is visible decreases Waxing Moon-part of the moon that is visible increases Crescent Phase-less than half of the moon is visible from earth Gibbous Phase-more than half of the moon is visible from the earth

  6. Surface Features on the Moon • Moon has 3 main surface features: • Maria • Highlands • Carters • Maria- • Large dark flat areas, due to lava flow (early observers thought they were oceans)

  7. Highlands: Highlands on the moon are higher, lighter, older areas on the moon's surface. Altitudes of the moon's highlands can reach 8000 meters! (That's about 3 miles!)

  8. Craters, from meteorite impacts:

  9. Crater impacts are caused by meteoroid strikes that eject material; after impact explosion ejects more material, leaving crater

  10. King crater on the Farside of the moon. The surface of the moon is scarred with millions of impact craters. There is no atmosphere on the moon to help protect it from bombardment. Also, there is no erosion and little geologic activity to wear away these craters, so they remain unchanged until another new impact changes it.

  11. Messier and Messier A Crater 308 on Farside The size, mass, speed, and angle of the falling object determine the size, shape, and complexity of the resulting crater.

  12. Lunar Cratering and Surface Composition • Craters are typically about 10 times as wide as the meteoroid creating them, and twice as deep. • Rock is pulverized to a much greater depth. • Most lunar craters date to at least 3.9 billion years ago; much less bombardment since then.

  13. Regolith: thick layer of dust left by meteorite impacts. It covers the lunar landscape to an average depth of about 20m. Moon is still being bombarded, especially by very small “micrometeoroids”

  14. More than 3 billion years ago, the moon was volcanically active. Rille is formed from an open lava channel

  15. Evolutionary History of the Moon

  16. Meteorites also hit Earth; this crater is in Arizona: Barringer Meteorite Crater Between 20,000 to 50,000 years ago, a small asteroid about 80 feet in diameter impacted the Earth and formed the crater. The crater is the best preserved crater on Earth and measures 1.2 km in diameter.

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