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Introduction to Volcanology May 2008 Chapter 1
Content ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
VOLCANO
Volcano ,[object Object]
Origin of Volcanos ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Volcano Mount Saint Helen Eruption, May 18th 1980
Magma chamber conduit mantle Parasitic   Cone Ash   Cloud/Gases Vent Lava Flow Crater Parts of a Volcano
“ Ring of Fire” Volcanic arcs and oceanic trenches partly encircling the Pacific Basin form the so-called , a zone of frequent earthquakes and volcanic eruptions.
Volcanoes and earthquakes ,[object Object]
Volcanology ,[object Object]
VOLCANISM
Volcanism ,[object Object],[object Object]
Origin of Volcanism ,[object Object],[object Object],[object Object],[object Object],[object Object]
Heat Source ,[object Object],When a volcano erupts, the steam and ash is caused by lava that is forcing its way toward the surface of the earth.
Isotopes ,[object Object],Therefore, isotopes have different mass numbers, which give the total number of nucleons—the number of protons plus neutrons.  Hydrogen Deiterium Tritium
U 235 –  U 238   ,[object Object],U238   is the most common isotope of uranium found in nature. In a nuclear reactor, it can be used to breed plutonium-239, which itself can be used in a nuclear weapon or as a reactor fuel source.
Th 232  – K 40 ,[object Object],K40 , which has a radioactive half-life of about 1.2 billion years, could be an important source of heat in the Earth’s core but this has never been unambiguously confirmed in an experiment.
Accretional Heating ,[object Object],By accounting for all energy transfer for every cratering event it is theoretically possible to determine the thermal state of newly- formed planets
Tidal Heating In some other planents is too small to have left over accretional heat, and radioactive decay could not generate the tremendous energy required to power all of the volcanic activity that exists on the moon.
Core Formation ,[object Object],Near the end of accretion, core formation evidently ceased as upper mantle conditions became oxidizing. The accumulation of the oceans is a consequence of the change to oxidizing conditions.
Meteorits ,[object Object]

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Introduction to Volcanology Chapter 1 - Volcanoes, Magma, Earthquakes

  • 1. Introduction to Volcanology May 2008 Chapter 1
  • 2.
  • 4.
  • 5.
  • 6. Volcano Mount Saint Helen Eruption, May 18th 1980
  • 7. Magma chamber conduit mantle Parasitic Cone Ash Cloud/Gases Vent Lava Flow Crater Parts of a Volcano
  • 8. “ Ring of Fire” Volcanic arcs and oceanic trenches partly encircling the Pacific Basin form the so-called , a zone of frequent earthquakes and volcanic eruptions.
  • 9.
  • 10.
  • 12.
  • 13.
  • 14.
  • 15.
  • 16.
  • 17.
  • 18.
  • 19. Tidal Heating In some other planents is too small to have left over accretional heat, and radioactive decay could not generate the tremendous energy required to power all of the volcanic activity that exists on the moon.
  • 20.
  • 21.