Formation of the Solar System

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Created by:

peckensl  on May 11, 2011

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Chapter 28 Section 28.1

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Formation of the Solar System

Planetesimals
objects hundreds of kilometers in diameter. Colliding particles in the early solar system.
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Planetesimals objects hundreds of kilometers in diameter. Colliding particles in the early solar system.
Retrograde Motion The apparant backward movement of a planet
Ellipse Oval Shape that is centered on two points instead of a single point as in a circle
Astronomical Unit a Measurement from a planet to the sun
Eccentricity The ratio of the distance between the foci to the length of the major axis

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