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Chapter 6: Terrestrial Planets -The Moon Earth’s interior is revealed by seismology, the study of earthquakes. Layers are revealed: A layered object: Inner core Outer core Mantle Crust Hydrosphere Atmosphere Magnetosphere Earth’s Moon: the interior is not as well understood Missing: Hydrosphere Atmosphere Magnetosphere Full Moon, Near Side Far side of the Moon (taken by Apollo 16) Two Faces of the Moon Maria Near Side Impact Basin Cratered Highlands Far Side Apollo and Luna Landing Sites A15 A17 L24 L20 A12 A14 A11 A16 L16 Moon, Close Up, craters, maria, and highlands Meteoroid Impact causes craters and ejecta Lunar Craters, big and small (microscopic, even) Lunar Surface is blanketed in dust from small meteorites. Lunar Tides are due to the gravity of the Moon Solar and Lunar effects on Tides depend on the relative orientations of the Earth, Moon, and Sun The tidal bulge is actually offset somewhat from being directly underneath the Moon. This produces a torque, a kind of twisting force on the Earth. The tides cause the Earth to slow down and the Moon’s orbit to increase in radius (4 cm per century). Also, the Moon’s rotation is synchronous with its orbit. The Moon’s formation is believed to be due to a collision of a massive (Mars-sized) object with the early Earth. Computer simulation show that this could leave a moonsized satellite in the correct orbit. Lunar Evolution: the Moon after the early bombardment Lunar Evolution: the formation of the maria by volcanic eruptions Lunar Evolution: after 3 billion years of cratering Large Lunar Crater (note smaller recent craters)