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The Hotspots
 Volcanoes on Mars are much wider and taller than
  Earths, but have similar ratios of height to base radius
Formation and Eruption of Martian
Volcanoes
 Mars no longer has active tectonic plate activity
 Due to no movement of crustal drifting, the volcanic
  hot spot remains under the same mountain resulting
  in extremely large mountains, such as Olympus Mons
 On Mars, shield volcanoes form above volcanic hot
  spots
Crustal
Magnetism
on Mars
•Red areas shows
the North
magnetic fields
•Blue areas shows
the South
magnetic fields
Shield Volcanoes on Mars
                    Olympus Mons
                      The caldera




                    Tharsis Ridge
                       Ascaraeus Mons
                       Pavonis Mons
                       Arsia Mons
Tectonic Plate Movement and
Formation of Earth Volcanoes
 Most of Earths volcanoes form near convergent plate
  boundaries, such as the Pacific Ring of Fire (68% of
  Earth’s Volcanoes)
 Earth’s hot spot theory on volcano formation
   Oceanic divergent plate boundaries
   Continental convergent plate boundaries
   Earths “hotspots”
 Statovolcanoes
Stratovolcanoes on Earth
                Stratovolcanoes are known
                 for their steep profile and
                 fluctuations of explosive
                 and quiet eruptions
                Mount Krakatoa exploded
                 killing nearly 40,000
                 people in 1883
                Mount Vesuvius erupted in
                 79 A.D. The city of Pompeii
                 and Herculaneum were
                 destroyed by large amounts
                 of ash and pumice
Citations
• Hamilton, C. (1995). Martian volcanoes.
  Retrieved from
  http://www.solarviews.com/eng/marsvolc.htm
• Tayfun Oner, A. (1997). Retrieved from
  http://www.solarviews.com/cap/mars/voly1.htm
• Greetings from mars. (n.d.). Retrieved from
  http://abyss.uoregon.edu/~js/ast121/lectures/lec
  12.html

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Mikes pp

  • 1. The Hotspots  Volcanoes on Mars are much wider and taller than Earths, but have similar ratios of height to base radius
  • 2. Formation and Eruption of Martian Volcanoes  Mars no longer has active tectonic plate activity  Due to no movement of crustal drifting, the volcanic hot spot remains under the same mountain resulting in extremely large mountains, such as Olympus Mons  On Mars, shield volcanoes form above volcanic hot spots
  • 3. Crustal Magnetism on Mars •Red areas shows the North magnetic fields •Blue areas shows the South magnetic fields
  • 4. Shield Volcanoes on Mars  Olympus Mons  The caldera  Tharsis Ridge  Ascaraeus Mons  Pavonis Mons  Arsia Mons
  • 5. Tectonic Plate Movement and Formation of Earth Volcanoes  Most of Earths volcanoes form near convergent plate boundaries, such as the Pacific Ring of Fire (68% of Earth’s Volcanoes)  Earth’s hot spot theory on volcano formation  Oceanic divergent plate boundaries  Continental convergent plate boundaries  Earths “hotspots”  Statovolcanoes
  • 6. Stratovolcanoes on Earth  Stratovolcanoes are known for their steep profile and fluctuations of explosive and quiet eruptions  Mount Krakatoa exploded killing nearly 40,000 people in 1883  Mount Vesuvius erupted in 79 A.D. The city of Pompeii and Herculaneum were destroyed by large amounts of ash and pumice
  • 7. Citations • Hamilton, C. (1995). Martian volcanoes. Retrieved from http://www.solarviews.com/eng/marsvolc.htm • Tayfun Oner, A. (1997). Retrieved from http://www.solarviews.com/cap/mars/voly1.htm • Greetings from mars. (n.d.). Retrieved from http://abyss.uoregon.edu/~js/ast121/lectures/lec 12.html