ASTM 101WW - Unit II
The Solar System, Its Origin and Terrestrial Planets


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Purpose:

In this unit you will explore the processes that astronomers use in developing theories. In the case of the origin of the solar system, since no one was around 4.6 billion years ago when the solar system formed, astronomers have to play "detective". Like a detective who must recreate a crime from the available evidence, so too, an astronomer must develop a theory of the origin of the solar system from evidence available today. In addition to exploring how the solar system formed, you will also learn how astronomers determine the age of the solar system.

After developing an understanding of the origin of the solar system, you will explore in detail the evolution of the terrestrial planets. You will be most involved in exploring the evolution of their atmospheres and their tectonic past and present. Enjoy!!!

Objectives:

  1. Be able to describe the different types of "solar systems" and efforts to locate other planetary systems. Be able to list the different members of our solar system
  2. Be able to list the planets in order from the Sun
  3. Be able to describe two approaches to developing a theory of the origin of our solar system.
  4. Be able to describe the basic properties of the solar system.
  5. Be able to describe the describe the two types of planets.
  6. Be able to describe the the terrestrial and jovian planets.
  7. Be able to summarize the solar nebular hypothesis of the origin of the solar system.
  8. Be able to summarize the theory behind radiometric dating and how it can be used to detemine the age of the solar system.
  9. Be able to summarize the factors that are important in the evolution of planetary atmospheres. Be able to distinguish between primary and secondary atmospheres.
  10. Venus has sometimes been referred to as the Earth's twin. Be able to write an essay comparing and contrasting Venus and the Earth. Your purpose is to either support or reject this claim.(30-point essay question for the Unit 2 Exam)
  11. Describe some of the unique properties of the planet Mars. (30-point essay question for the Unit 2 Exam)
  12. Be able to describe Mercury in terms of its atmosphere, tectonic properties and temperature.
  13. Be able to summarize the theory of plate tectonics. Be able to state the significance of the following terms: subduction, sea-floor spreading, divergent plate boundary, convergent plate boundary, trench, mid-ocean ridge, San Andreas fault, convection, lithosphere and asthenosphere.
Unit Two Bulletin Board Discussion Topic: Why is life able to exist abundantly on the Earth and not on any of the other terrestrial planets? How does tectonic activity on the Earth differ from that on any other terrestrial planet?

Unit Review: March 16, 2003 - Unit 2 homework and participation in the bulletin board/chat room discussions should be competed by this date.


Fred Hickok
Updated: January 27, 2003
CCBC Catonsville Campus
800 South Rolling Road
Catonsville, Maryland 21228