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Earths Dynamic Systems Hamblin

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Composition is unique in solar system. 78% nitrogen. 21% oxygen (not present in ... Layers defined by composition and physical properties. Compositional layers ... – PowerPoint PPT presentation

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Title: Earths Dynamic Systems Hamblin


1
Class website www.sci.uidaho.edu/coslab/ -follow
Teaching link to Geology 101
Textbook Earth An Introduction to Physical
Geology by Tarbuck Lutgens
2
Tests and Grading   3 Exams 600 pts (200
pts each) Final Exam 350 pts
(cumulative) Email Quizzes 50 pts 1000
pts First Exam 7 February Wed.
3
The Earth in Space
You will be here.
4
What makes Geology different from Physics or
Chemistry? Geology is Postdictive.as opposed to
Predictive like Chemistry. Postdictive science
is historical in nature. -it is science with a
story
5
Age of the Earth 4.5 Billion years 4,600,000,00
0 years Age of the Universe 14 Billion years
6
  • Time is measured by change
  • -Deep time
  • -millions billions of years
  • -James Hutton (1726-1797) considered the
    father of geological science.
  • -postulated a very old Earth
  • -formulated concept of Uniformitarianism

7
Uniformitarianism
  • Laws of nature dont change with time
  • Past events explained by modern processes
  • Uniformity of Process not Rate
  • Assumes vast amounts Deep Time

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9
Earth Compared to Other Planets
  • The Solar System
  • The inner planets
  • Rocky planets near the Sun
  • Mercury, Venus, Earth Mars
  • The outer planets
  • Giant gaseous planets
  • Jupiter, Saturn, Uranus, Neptune
  • Pluto, a small icy minor planet

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11
Origin of the Solar System
  • Gravitational collapse of gas dust cloud
    nebula
  • Rotation around a central mass
  • Disk shaped cloud
  • Temperature variations segregated matter
  • Small particles accreted into larger
    planetesimals, planets

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13
How do we Know this?
14
Ordinary Chondritic Meteorite -composition of
asteroids and the early solar system
-pyroxene chondrule in thinsection
-chondrules
15
Iron Meteorites -actually mixture of Fe and
Ni -planetary cores?
16
  • Differences between inner and outer planets
  • Density
  • The rocky inner planetsdensities of
  • 3 g/cm3 more
  • The gaseous outer
  • Planetsdensities
  • of 1.6 g/cm3 or less

17
Earth
  • Internal Heat
  • Produces changes in the Earths features
  • Sources of internal heat
  • Radioactive decay
  • Decay releases heat energy
  • Accretionary heat
  • from Earths formation

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19
Earths Outermost Layers
  • The most dynamic portion of the Earth
  • Atmosphere
  • Thin gaseous envelope surrounding Earth
  • Hydrosphere
  • Water layer dominated by the oceans
  • Biosphere
  • All living things on the planet
  • Lithosphere
  • Rocky outer shell

20
The Atmosphere
  • Composition is unique in solar system
  • 78 nitrogen
  • 21 oxygen (not present in early atmosphere)
  • Minor amounts of carbon dioxide, argon and water
    vapor

21
The Hydrosphere
  • Total mass of water on or near the Earths
    surface
  • Covers 71 of Earths surface
  • 98 in oceans
  • 2 in glaciers, groundwater, lakes and streams
    (fresh water)

22
The Biosphere
  • All life on Earth
  • Animals plants on land, in the sea and air
  • Microorganisms-the most common form of life
  • Evolved within narrow zone near the Earths
    surface

23
Earths Internal Structure
  • Solid Earth has a layered structure
  • Layers defined by composition and physical
    properties
  • Compositional layers
  • crust - mantle - core
  • Physical layers
  • lithosphere - asthenosphere - mesosphere - outer
    core - inner core

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26
Compositional Layers
  • Crust
  • Outermost compositional layer
  • Definite change in composition at the base of the
    crust
  • 2 types
  • Continental crust
  • Oceanic crust

27
Compositional Layers
  • Mantle
  • Largest layer in the Earth
  • 2900 km thick
  • 82 by volume
  • 68 by mass
  • Composed of silicate rocks with abundant iron and
    magnesium
  • Density ranges from 3.2 to 5 g/cm3

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29
Compositional Layers
  • Core
  • Central mass about 7000km in diameter
  • Average density of 10.8 g/cm3
  • 16 by volume, 32 of mass
  • Indirect evidence of composition
  • Metallic iron

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31
Physical Layers
  • Lithosphere
  • Crust upper portion of the mantle
  • Solid rigid
  • Thickness ranges from 10 km beneath oceans to 300
    km in continental areas

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33
  • Crust
  • Continental crust
  • Thick - up to 75 km
  • Lower density - 2.7 g/cm3
  • Strongly deformed
  • Much older - may be billions of years old

34
  • Crust
  • Oceanic crust
  • Thinner - about 8 km
  • More dense - 3.0 g/cm3
  • Comparatively undeformed
  • Much younger - lt 200 million years old

35
Majors Features of the Continents
  • Shields
  • Stable platforms
  • Folded Mountains

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37
Continental Margin San Francisco Monterey Bay
Area
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