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Lecture:
Eight of the nine planets
fall into two distinctive categories. Mercury, Venus, Earth and Mars share similar
properties and therefore are referred to as the terrestrial planets. Jupiter,
Saturn, Uranus and Neptune share properties that are unique to them; therefore,
they are referred to as the jovian planets. Pluto falls into a category of its
own and is traditionally ignored when discussing the formation of the planets.
The properties of the planets are important in developing a theory which explains the origin of the solar system because any good theory would have to explain the origin of those properties. To better understand the differences between the terrestrial and jovian planets, use the printout of planetary data obtained from the Planetary Data Browser to do this activity. If you no longer have the printout refer to the Properties of the Solar System.
The spacing of the planets' orbits works out so that for most cases the next planet out is about twice as far as the previous planet. A specific numerical sequence was figured out by Johann Titius and popularized by Johann Bode in the late 1700's. A gap between Mars and Jupiter led astronomers to search for a missing planet. Instead they discovered asteroids in that region. Read up about the Titius-Bode Law.
Complete
these Self-check Questions:
None for this lecture.
Homework Questions: (To submit your answers to the homework questions, first copy the questions from this page and paste them into the homework form. Insert your answers below the questions. Fill in the remaining form elements and submit. Your homework will be e-mailed to me. I will return your graded homework to you in the private e-mail of the comm center).
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| Fred
Hickok Updated: January 17, 2001 |
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