Astronomy and Space Sciences

CONTENTS OF CURRICULUM UNIT 05.04.03

  1. Unit Guide
  1. Introduction
  2. Student Population
  3. Objectives
  4. Overview
  5. Teaching Strategies
  6. BackgroundContent
  7. Volcanoes in the Solar System
  8. Volcanoes on Earth
  9. Radioactivity
  10. Pangaea
  11. Plate Tectonics
  12. Volcanic Landforms
  13. Volcanoes in Space
  14. Io and Its Volcanoes
  15. Types of Volcanoes on Io
  16. Comparing Volcanoes: Earth and Io
  17. Lesson Plans
  18. Lesson 1: Radioactive Decay
  19. Lesson 2: A Scissor Cut: Snipping away at the Decay Process
  20. Lesson 3 Making and Mapping a Volcano
  21. Lesson 4: Galilean Satellites
  22. Annotated Bibliography
  23. Appendix

Volcanoes in the Solar System

Mary Jefferson

Published September 2005

Tools for this Unit:

Comparing Volcanoes: Earth and Io

Earth eruptions are very violent, noisy, or somewhat quiet. Io's massive eruptions are much more violent, hotter, and longer lived than those on Earth. Earth's volcanoes are fueled by radioactive decay whereas Io's volcanoes are fueled by tidal heating. Earth volcanic activities are violently- explosive, mild, or moderate. Io's eruptions are always violent, due to high sulfur content.

Earth volcanoes have specific shapes depending on the geologic processes involved. They are broad-gently sloping or small-steep sloping or anywhere in between. Shield, cinder and composite cones are the most popular terrestrial ones. Io's volcanoes are in shapes similar to those on Earth: plumes, shields, calderas and hot spots. They are huge and eject tons of materials into Jupiter's magnetosphere.

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