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Chapter 9: Volcanoes

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Title: Chapter 9: Volcanoes


1
Chapter 9 Volcanoes
  • 9.1 How and Where Volcanoes Form
  • 9.2 Magma and Erupted Materials
  • 9.3 Volcanic Landforms
  • 9.4 Extraterrestrial Volcanism

2
9.1 How and Where Volcanoes Form
  • Volcano-Refers to both the opening in Earth's
    crust through which molten rock, gases and ash
    erupt and to the landform that develops around
    this opening.

3
9.1 How and Where Volcanoes Form
  • Magma Formation
  • 1. Three main conditions for magma to form
  • A decrease in pressure can lower melting
    temperatures.
  • An increase in temperature can cause materials in
    the Asthenosphere to melt.
  • An increase in the amount of water can lower
    melting temperatures.

4
9.1 How and Where Volcanoes Form
  • 2. Most volcanoes are found along mid-ocean
    ridges and along Subduction boundaries.
  • 3. Most magma is less dense than the
    surrounding rocks and therefore rises to the
    surface.

5
9.1 How and Where Volcanoes Form
  • At Subduction Boundaries
  • Oceanic-Oceanic and Oceanic-Continental. See
    diagram on page 195.
  • Create Volcanoes.
  • At Divergent Boundaries
  • Plates split apart and magma oozes up, creating
    ridges.
  • Mostly occurs in the middle of oceans.

6
9.1 How and Where Volcanoes Form
  • D. Over Hot Spots
  • Hot spot- Areas of volcanic activity that result
    from plumes of hot solid material that have risen
    from deep with the Earth's mantle.
  • Hot spots stay in the same place as the plates
    continue to move. See page 197.
  • Volcanic islands forming over a hot spot.

7
9-2 Magma and Erupted Materials
  • Types of Magma
  • Viscosity-resistance to flow. Determined by
    silica content. Higher the silica, slower the
    flow.
  • Gases can create explosive volcanoes.
  • See summary on page 199.
  • Lava Flows
  • Lava-Magma that reaches the surface
  • Basaltic lava flows are usually slow and
    non-explosive. There are two main types
    Pahoehoe (ropey) and AA (sharp).
  • Pillow Lava- rounded lumps of lava formed
    underwater.

8
9-2 Magma and Erupted Materials
  • Ash and Rock Fragments
  • Pyroclastic Material- When gases are released
    solid fragments of this material are ejected.
  • These materials are classified by size. Ash is
    less than 2 mm. Lapilli ranges in size from 2-64
    mm and blocks or bombs are greater than 64 mm.
  • Pyroclastic Flow- A dense superheated cloud that
    travels downhill with amazing speed (100 kph).

9
9.3 Volcanic Landforms
  • Shield Volcanoes
  • Low viscosity lava that flows for long distances.
  • Lava builds up in layers and forms broad bases
    and gentle slopes.

10
9.3 Volcanic Landforms
  • B. Cinder Cones
  • The simplest of the volcanoes occurs when lava is
    thrown from the volcano.
  • Lava hardens before it hits the ground and
    accumulates forming a cone shaped mound.

11
9.3 Volcanic Landforms
  • Composite Cone
  • Develops when layers of material from several
    volcanic events accumulate around a vent.
  • The materials include both hardened lava and
    pyroclastic material.
  • Lahar-A fast moving mudflow created by a volcanic
    eruption.

12
9.3 Volcanic Landforms
  • D. Caldera
  • When magma beneath a volcano is released after
    the top of the volcano collapses, forming a large
    crater shaped basin.
  • Examples are Crater Lake in Oregon and
    Yellowstone NP. See page 204.
  • E. Lava Plateaus
  • Basaltic lava pouring from fissures and spreading
    across the land.
  • Volcano
  • Volcanic Landforms

13
9.4 Extraterrestrial Volcanism
  • The Moon
  • Dark areas on the moon are basaltic lava flows.
  • Volcanism began about 3-4 billion years ago.
  • Mars
  • Home to Olympus Mons, the largest volcano in the
    solar system.
  • It measures 600 km across and 27 km above the
    surrounding terrain

14
9.4 Extraterrestrial Volcanism
  • Venus
  • Has 1600 large volcanoes
  • Some volcanoes may still be active

15
9.4 Extraterrestrial Volcanism
  • D. Io (Jupiters 3rd moon)
  • One of the most volcanically active areas in the
    solar system.
  • Io is caught in a tug of war, which creates
    friction and then heat. That heat drives the
    volcanic activity.
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