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Chapter 5 Earth and Moon
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What do you think? Will the ozone layer, which is now being depleted, naturally replenish itself? Does the Moon have a dark side, where it is forever night? Does the Moon rotate, and if so, how fast? What causes the ocean tides? When does the spring tide occur?
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Why might this planet be called the blue planet?
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The Earth’s atmosphere has evolved over billions of years Earth’s early atmosphere was primarily hydrogen and helium left over from the formation of the solar system Earth’s second atmosphere was primarily CO2 and released from Earth’s interior by volcanoes Earth’s current atmosphere is a 4-to-1 mixture of nitrogen and oxygen which was created by biological activity.
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Earth’s atmospheric layers are defined by temperature ranges Earth’s protecting ozone layer
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Earth’s Ozone Layer Ozone is O 3 Protects the surface from hazardous UV radiation from the Sun Can be destroyed by synthetic chlorofluorocarbons (CFCs) Slowly replenishes itself as it is created from sunlight and lightning Earth’s protective ozone layer had to form before early life could move from the oceans onto dry land
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Plate tectonics produced major changes to the Earth’s surface over the past 200 million years
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Pangea
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SEA FLOOR SPREADING The sea floor between the North America and Europe is spreading apart
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Earth’s surface is composed of about nine major plates which slowly move relative to one another separation Collision of two plates forms mountains
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Plate tectonics is driven by convective currents in Earth’s mantle
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Earth’s interior consists of a rocky mantle and an iron rich core
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The Earth’s magnetic field is caused by dynamo movements in Earth’s core
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The Earth’s magnetic field shield us from the stream of charged particles from the Sun called the solar wind
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Relevance of Earth’s protective magnetosphere Solar Flares - violent explosions on the Sun releasing charged particles into the solar system Solar wind - dangerous stream of charged particles coming from the Sun Van Allen radiation belts - hazardous reservoir of charged particles surrounding Earth Northern Lights (Aurora Borealis)
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Aurora as seen from space
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Aurora surrounding the north geomagnetic pole as seen from space
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The Moon’s surface is covered with craters, plains, and mountains
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Mare Imbrium
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Visits to the Moon yielded invaluable information about its history
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Lunar Soil is called Regolith
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Mare Basalt Mare basalt is solidified lava similar to what composes rocks on Earth’s sea floor.
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Anorthsite Anorthsite is material from the original lunar crust sometimes called the genesis rock and is more than 4 billion years old
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Impact Breccias Impact Breccias are rocks formed from combining debris during a violent impact event
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Likely interior of the Moon
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The Moon probably formed from debris cast into space when a huge planetesimal struck the young Earth
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Gravitation al forces produce the tides and keep the same side of the Moon always facing the Earth Synchronous rotation
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The gravitational force between Earth and Moon results in tides Large spring tides occur when the Sun and Moon are aligned such that they BOTH pull on the Earth’s water. Smaller neap tides occur when the Sun and Moon are misaligned such that they pull on the Earth’s water in different directions.
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Bouncing laser beams off the Moon demonstrates that it slowly moving away from the Earth
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What did you think? Will the ozone layer, which is now being depleted, naturally replenish itself? Yes, the ozone is created from normal oxygen molecules by the Sun’s ultraviolet radiation. Does the Moon have a dark side, where it is forever night? Half of the Moon is always dark, but that half is continually changing as the Moon orbits the Earth. Does the Moon rotate, and if so, how fast? The Moon rotates at the same rate that it revolves around the Earth. If the Moon didn’t rotate, then as it revolved we would see different sides of it, which we don’t. What causes the ocean tides? The tides are caused by gravitational forces, primarily from the Moon and Sun. When does the spring tide occur? Spring tides occur during each full and new Moon.
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Self-Check 1: Describe the chemical evolution of the Earth’s atmosphere. 2: Describe the basic characteristics of plate tectonics on the Earth, including the observational evidence and the underlying cause. 3: List the major divisions of the Earth’s interior and describe the chemical composition and relative physical conditions in each. 4: Describe the relationship of the Van Allen belts and the northern lights to the Earth’s magnetic field. 5: List the various layers in the Earth’s atmosphere and describe the physical characteristics by which they differ. 6: List and describe the nature and probable origin of lunar surface features visible in photographs. 7: Indicate the range in ages of lunar rocks taken from different areas on the lunar surface and explain what they indicate about the stages in the formation of the moon. 8: Describe the key elements of the collisional ejection theory and summarize the evidence that might support it.
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