Heliocentric Planets: Inferior and Superior

When Copernicus reordered our solar system, epicycles were not longer required to demonstrate retrograde motion of planets. Additionally, the relationships that each planet's motion held with the Sun no longer needed to be included in their planetary models. The models demonstrate the limited elongation of Inferior Planets, the retrograde motion of the Sun, and the connection between Superior Planets' retrograde motion of the Sun as consequences of the Earth's motion around the Sun.

 

Tim Wotherspoon

 
Resource Type
Activity
Tags
Target Group (Age)
3 – 19+
Language
English
 
 
 
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