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:

Pangaea

One of the earliest attempts to explain formations of landforms was introduced by Alfred Wegener in the early 1900's. Wegener introduced his continental drift hypothesis called Pangaea. He proposed that a super continent called Pangaea began breaking into smaller continents about 200 million years ago. These smaller continent fragments then drifted to their present positions. Certain kinds of evidence were used to prove this chain of reasoning. Among them were the "fit of South America and Africa, fossil evidence, rock types and structures, and ancient climates." (Tarbuck and Lutgens, 507). However, the continental drift hypothesis failed to provide an acceptable mechanism for the movement of continents.

Harry Hess in 1962 formulated the idea of seafloor spreading, which states that new seafloor is being generated at the mid-oceanic ridges and old, dense seafloor is being consumed at the deep ocean trenches. Hess's sea-floor spreading idea was widely accepted "with the discovery of alternating stripes of high-and-low-intensity magnetism that parallel the ridge crests." (Tarbuck and Lutgens, 507).

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