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Earth’s Interior
0Made up of 3 major compositional zones
 and 5 structural zones.
Layers of the Earth
Compositional Zones
0Crust: outermost layer
 0Makes up 1% of Earth’s mass
 0Oceanic (5-10km) & continental
  (15-80km)
 0Moho: lowest layer of crust
Compositional Zone
0Mantle: denser than crust
 02,900 km thick (2/3 of Earth’s
  mass)
0Core: center of the Earth
 0Made of iron and nickel
Structural Zones
0 3 compositional zones are divided into 5
  structural zones.
0 Lithosphere: Part of the mantle & crust above it.
  0 Cool & brittle
0 Asthenosphere: Solid rock is able to flow.
  0 Very hot and has high pressure
0 Mesosphere: Layer of solid mantle rock
0 Outer core (liquid)
0 Inner core (solid)
Earth as a Magnet
0Has 2 magnetic
 poles
0Motions in the
 core produce
 electric currents
 that create
 magnetic field.
0Shaped by solar
 winds
Earth’s Rotation
0 The spinning of Earth around its axis is called
  rotation.
0 1 full rotation = 24 hours
  0 Evidence
     0 Foucault Pendulum – Large pendulum that shifts 11 ̊ every
       hour in a clockwise direction.
     0 Coriolis Effect – Winds are deflected to the right in N.
       Hemisphere and to the left in the S. Hemisphere.
Effects of Rotation
0 Sun appears to rise in the east and set in the west.
0 Standard Time Zones
   0 Based upon the rate in which the sun appears to move
     across the sky.
   0 Starting point for the standard time zone is the prime
     meridian.
   0 Passes through Greenwich, England (longitude 0 ̊)
0 International Date Line
   0 Longitude where the date changes.
   0 180th meridian
Standard Time Zones




 Every 15 degrees of longitude
    equals one hour of time
International Date Line




Moving from left to right…subtract one day
  Moving from right to left…add one day
Earth’s Revolution
0The Earth’s orbit around the sun.
0It takes about 365 days to complete one
 full revolution.
Ellipse
0 The shape the earth’s orbit takes around the
  Sun is called an ellipse; an elongated closed
  curve
0 The sun is not in the center of the ellipse
0 Thus, the distance between the sun and earth
 changes.
Ellipse
The Northern Hemisphere’s summer   The Northern Hemisphere’s winter
Equinox
0 When the sun is directly above the Earth’s
  equator.
  0 Daylight = night time in both hemispheres.
  0 Spring equinox and Autumnal equinox
Solstice
0The sun’s direct rays reach their greatest
 distance north or south of the equator.
023.5 ̊N and 23.5 ̊S.
0Winter and Summer solstice
Credits
0 Spaulding, Namowitz (2003). Earth Science.   Evanston, IL:
  McDougal Littell Inc.
0 Photos
   0 http://www.theozonehole.com/coriolis.htm
   0 http://oceanexplorer.noaa.gov/explorations/05galapagos/log
     s/dec22/media/magfield_600.html
   0 http://oceansjsu.com/105d/exped_commotion/5.html
   0 http://en.wikipedia.org/wiki/File:Pendule_de_Foucault.jpg
   0 http://en.wikipedia.org/wiki/File:Earth-lighting-
     equinox_EN.png

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Chapter 4: Earth's Structure and Motioin

  • 1.
  • 2. Earth’s Interior 0Made up of 3 major compositional zones and 5 structural zones.
  • 4. Compositional Zones 0Crust: outermost layer 0Makes up 1% of Earth’s mass 0Oceanic (5-10km) & continental (15-80km) 0Moho: lowest layer of crust
  • 5. Compositional Zone 0Mantle: denser than crust 02,900 km thick (2/3 of Earth’s mass) 0Core: center of the Earth 0Made of iron and nickel
  • 6. Structural Zones 0 3 compositional zones are divided into 5 structural zones. 0 Lithosphere: Part of the mantle & crust above it. 0 Cool & brittle 0 Asthenosphere: Solid rock is able to flow. 0 Very hot and has high pressure 0 Mesosphere: Layer of solid mantle rock 0 Outer core (liquid) 0 Inner core (solid)
  • 7. Earth as a Magnet 0Has 2 magnetic poles 0Motions in the core produce electric currents that create magnetic field. 0Shaped by solar winds
  • 8. Earth’s Rotation 0 The spinning of Earth around its axis is called rotation. 0 1 full rotation = 24 hours 0 Evidence 0 Foucault Pendulum – Large pendulum that shifts 11 ̊ every hour in a clockwise direction. 0 Coriolis Effect – Winds are deflected to the right in N. Hemisphere and to the left in the S. Hemisphere.
  • 9. Effects of Rotation 0 Sun appears to rise in the east and set in the west. 0 Standard Time Zones 0 Based upon the rate in which the sun appears to move across the sky. 0 Starting point for the standard time zone is the prime meridian. 0 Passes through Greenwich, England (longitude 0 ̊) 0 International Date Line 0 Longitude where the date changes. 0 180th meridian
  • 10. Standard Time Zones Every 15 degrees of longitude equals one hour of time
  • 11. International Date Line Moving from left to right…subtract one day Moving from right to left…add one day
  • 12. Earth’s Revolution 0The Earth’s orbit around the sun. 0It takes about 365 days to complete one full revolution.
  • 13. Ellipse 0 The shape the earth’s orbit takes around the Sun is called an ellipse; an elongated closed curve 0 The sun is not in the center of the ellipse 0 Thus, the distance between the sun and earth changes.
  • 15. The Northern Hemisphere’s summer The Northern Hemisphere’s winter
  • 16. Equinox 0 When the sun is directly above the Earth’s equator. 0 Daylight = night time in both hemispheres. 0 Spring equinox and Autumnal equinox
  • 17. Solstice 0The sun’s direct rays reach their greatest distance north or south of the equator. 023.5 ̊N and 23.5 ̊S. 0Winter and Summer solstice
  • 18. Credits 0 Spaulding, Namowitz (2003). Earth Science. Evanston, IL: McDougal Littell Inc. 0 Photos 0 http://www.theozonehole.com/coriolis.htm 0 http://oceanexplorer.noaa.gov/explorations/05galapagos/log s/dec22/media/magfield_600.html 0 http://oceansjsu.com/105d/exped_commotion/5.html 0 http://en.wikipedia.org/wiki/File:Pendule_de_Foucault.jpg 0 http://en.wikipedia.org/wiki/File:Earth-lighting- equinox_EN.png