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Earth Part 1 The Habitability of Earth
Outline I. The Early History of Earth A. Four Stages of Planetary Development B. Earth as a Planet II. The Solid Earth A. Earth's Interior B. The Magnetic Field C. Earth's Active Crust III. The Atmosphere A. Origin of the Atmosphere B. Human Effects on Earth's Atmosphere
The Early History of Earth Earth formed 4.6 billion years ago from the inner solar nebula. Four main stages of evolution: Most traces of bombardment (impact craters) now destroyed by later geological activity  Two sources of heat in Earth’s interior: ,[object Object],[object Object]
Earth’s Interior Direct exploration of Earth’s interior (e.g. drilling) is impossible.  Earth’s interior can be explored through  seismology:   earthquakes produce  seismic waves .  Two types of seismic waves: P ressure  waves: Particles vibrate back and forth S hear  waves: Particles vibrate up and down
Seismology Seismic waves do not travel through Earth in straight lines or at constant speed. They are bent by or bounce off transitions between different materials or different densities or temperatures. Such information can be analyzed to infer the structure of Earth’s interior.
Earth’s Interior (2) Basic structure : Earth’s interior gets hotter towards the center. Earth’s core is as hot as the sun’s surface; metals are liquid. Melting point = temperature at which an element melts (transition from solid to liquid) Melting point increases with increasing pressure towards the center => Inner core becomes solid Solid crust Solid mantle Liquid core Solid inner core
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Earth’s Magnetic Field ,[object Object],[object Object]
The Role of Earth’s Magnetic Field Earth’s magnetic field protects Earth from high-energy particles coming from the sun (solar wind). Surface of first interaction of solar wind with Earth’s magnetic field =  Bow shock Region where Earth’s magnetic field dominates =  magnetosphere Some high-energy particles leak through the magnetic field and produce a belt of high-energy particles around Earth:  Van Allen belts
The Aurora (Polar Light) As high-energy particles leak into the lower magnetosphere, they excite molecules near the Earth’s magnetic poles, causing the  aurora
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
The Active Earth About 2/3 of Earth’s surface is covered by water. Mountains are relatively rapidly eroded away by the forces of water.
Tectonic Plates Earth’s crust is composed of several distinct tectonic plates, which are in constant motion with respect to each other     Plate tectonics Evidence for plate tectonics can be found on the ocean floor …  and in geologically active regions all around the Pacific
Plate Tectonics Tectonic plates move with respect to each other. Where plates move toward each other, plates can be pushed upward and downward     formation of mountain ranges, some with volcanic activity, earthquakes Where plates move away from each other, molten lava can rise up from below     volcanic activity
Active Zones Resulting from Plate Tectonics Volcanic hot spots due to molten lava rising up at plate boundaries or through holes in tectonic plates
Earth’s Tectonic History
History of Geological Activity Surface formations visible today have emerged only very recently compared to the age of Earth.
The Rock Cycle
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Geology of Earth ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Earth’s Atmosphere ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
The Atmosphere Atmospheric composition severely altered (    secondary atmosphere)  through a combination of two processes: 1) Outgassing: Release of gasses bound in compounds in the Earth’s interior through volcanic activity Earth had a primeval atmosphere from remaining gasses captured during formation of Earth 2) Later bombardment with icy meteoroids and comets
The Structure of Earth’s Atmosphere The ozone layer is essential for life on Earth since it protects the atmosphere from UV radiation Composition of Earth’s atmosphere is further influenced by: ,[object Object],[object Object],[object Object],The temperature of the atmosphere depends critically on its albedo = percentage of sun light that it reflects back into space Depends on many factors, e.g., abundance of water vapor in the atmosphere
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Structure of the Atmosphere
Circulation in our atmosphere results from convection and the Earth’s rotation ,[object Object]
Winds ,[object Object],[object Object],[object Object]
Weather Producers ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
An idealized cold front
An idealized warm front
Weather Forecasting ,[object Object],[object Object],[object Object],[object Object],[object Object]
Climate ,[object Object],[object Object],[object Object],[object Object],[object Object]
The principal climate zones
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Ocean currents influence temperatures and climates
The hydrologic cycle Tidal forces help power the motion of the oceans ,[object Object],[object Object]
Distribution of the Water
Watersheds of three rivers
The path of groundwater
Oceanography ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
A wave passing in the open ocean
A wave becoming breaking onshore
Ocean Conveyor Belt - Major Climate Control
Human Effects on Earth’s Atmosphere 1) The Greenhouse Effect Earth’s surface is heated by the sun’s radiation. Heat energy is re-radiated from Earth’s surface as infrared radiation. CO 2 , but also other gases in the atmosphere, absorb infrared light     Heat is trapped in the atmosphere. This is the Greenhouse Effect. The Greenhouse Effect occurs naturally and is essential to maintain a comfortable temperature on Earth, but human activity, in particular CO 2  emissions from cars and industrial plants, is drastically increasing the concentration of greenhouse gases.
Global Warming ,[object Object],[object Object],[object Object],[object Object]
The Greenhouse Effect ,[object Object],[object Object]
 
Rising Carbon Dioxide
Human Effects on the Atmosphere (2) 2) Destruction of the Ozone Layer Ozone (= O 3 ) absorbs UV radiation, (which has damaging effects on human and animal tissue). Chlorofluorocarbons (CFCs) (used, e.g., in industrial processes, refrigeration and air conditioning) destroy the Ozone layer. Destruction of the ozone layer as a consequence of human activity is proven (e.g., growing ozone hole above the Antarctic); Must be stopped and reversed by reducing CFC use, especially in developed countries!
Industrial chemicals released into the atmosphere have damaged the ozone layer in the stratosphere
Question ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]

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Earth part 1

  • 1. Earth Part 1 The Habitability of Earth
  • 2. Outline I. The Early History of Earth A. Four Stages of Planetary Development B. Earth as a Planet II. The Solid Earth A. Earth's Interior B. The Magnetic Field C. Earth's Active Crust III. The Atmosphere A. Origin of the Atmosphere B. Human Effects on Earth's Atmosphere
  • 3.
  • 4. Earth’s Interior Direct exploration of Earth’s interior (e.g. drilling) is impossible. Earth’s interior can be explored through seismology: earthquakes produce seismic waves . Two types of seismic waves: P ressure waves: Particles vibrate back and forth S hear waves: Particles vibrate up and down
  • 5. Seismology Seismic waves do not travel through Earth in straight lines or at constant speed. They are bent by or bounce off transitions between different materials or different densities or temperatures. Such information can be analyzed to infer the structure of Earth’s interior.
  • 6. Earth’s Interior (2) Basic structure : Earth’s interior gets hotter towards the center. Earth’s core is as hot as the sun’s surface; metals are liquid. Melting point = temperature at which an element melts (transition from solid to liquid) Melting point increases with increasing pressure towards the center => Inner core becomes solid Solid crust Solid mantle Liquid core Solid inner core
  • 7.
  • 8.
  • 9.
  • 10.
  • 11. The Role of Earth’s Magnetic Field Earth’s magnetic field protects Earth from high-energy particles coming from the sun (solar wind). Surface of first interaction of solar wind with Earth’s magnetic field = Bow shock Region where Earth’s magnetic field dominates = magnetosphere Some high-energy particles leak through the magnetic field and produce a belt of high-energy particles around Earth: Van Allen belts
  • 12. The Aurora (Polar Light) As high-energy particles leak into the lower magnetosphere, they excite molecules near the Earth’s magnetic poles, causing the aurora
  • 13.
  • 14. The Active Earth About 2/3 of Earth’s surface is covered by water. Mountains are relatively rapidly eroded away by the forces of water.
  • 15. Tectonic Plates Earth’s crust is composed of several distinct tectonic plates, which are in constant motion with respect to each other  Plate tectonics Evidence for plate tectonics can be found on the ocean floor … and in geologically active regions all around the Pacific
  • 16. Plate Tectonics Tectonic plates move with respect to each other. Where plates move toward each other, plates can be pushed upward and downward  formation of mountain ranges, some with volcanic activity, earthquakes Where plates move away from each other, molten lava can rise up from below  volcanic activity
  • 17. Active Zones Resulting from Plate Tectonics Volcanic hot spots due to molten lava rising up at plate boundaries or through holes in tectonic plates
  • 19. History of Geological Activity Surface formations visible today have emerged only very recently compared to the age of Earth.
  • 21.
  • 22.
  • 23.
  • 24.
  • 25.
  • 26.
  • 27.
  • 28.
  • 29. The Atmosphere Atmospheric composition severely altered (  secondary atmosphere) through a combination of two processes: 1) Outgassing: Release of gasses bound in compounds in the Earth’s interior through volcanic activity Earth had a primeval atmosphere from remaining gasses captured during formation of Earth 2) Later bombardment with icy meteoroids and comets
  • 30.
  • 31.
  • 32. Structure of the Atmosphere
  • 33.
  • 34.
  • 35.
  • 38.
  • 39.
  • 41.
  • 42.
  • 43.
  • 44. Ocean currents influence temperatures and climates
  • 45.
  • 48. The path of groundwater
  • 49.
  • 50. A wave passing in the open ocean
  • 51. A wave becoming breaking onshore
  • 52. Ocean Conveyor Belt - Major Climate Control
  • 53. Human Effects on Earth’s Atmosphere 1) The Greenhouse Effect Earth’s surface is heated by the sun’s radiation. Heat energy is re-radiated from Earth’s surface as infrared radiation. CO 2 , but also other gases in the atmosphere, absorb infrared light  Heat is trapped in the atmosphere. This is the Greenhouse Effect. The Greenhouse Effect occurs naturally and is essential to maintain a comfortable temperature on Earth, but human activity, in particular CO 2 emissions from cars and industrial plants, is drastically increasing the concentration of greenhouse gases.
  • 54.
  • 55.
  • 56.  
  • 58. Human Effects on the Atmosphere (2) 2) Destruction of the Ozone Layer Ozone (= O 3 ) absorbs UV radiation, (which has damaging effects on human and animal tissue). Chlorofluorocarbons (CFCs) (used, e.g., in industrial processes, refrigeration and air conditioning) destroy the Ozone layer. Destruction of the ozone layer as a consequence of human activity is proven (e.g., growing ozone hole above the Antarctic); Must be stopped and reversed by reducing CFC use, especially in developed countries!
  • 59. Industrial chemicals released into the atmosphere have damaged the ozone layer in the stratosphere
  • 60.