Johannes Kepler: Difference between revisions
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==Laws of Planetary Motion== | ==Laws of Planetary Motion== | ||
[[File:Laws.JPG|left|500px|thumb| | [[File:Laws.JPG|left|500px|thumb|1st and 2nd laws. The sun is located at f1 and is thus a foci of both planets orbits which is the 1st law. The equal areas of A1 and A2 demonstrates the 2nd law. ]] | ||
===1. Law of Orbits=== | ===1. Law of Orbits=== |
Revision as of 12:19, 3 December 2015
Page Claimed by Davis Johnston
Background
What are the mathematical equations that allow us to model this topic. For example [math]\displaystyle{ {\frac{d\vec{p}}{dt}}_{system} = \vec{F}_{net} }[/math] where p is the momentum of the system and F is the net force from the surroundings.
Laws of Planetary Motion
1. Law of Orbits
All planets move in elliptical orbits with the Sun at one of the two foci
2. Law of Areas
A line that connects a planet to the sun sweeps out equal areas in equal times.
3. Law of Periods
The square of the period of any planet is proportional to the cube of the semi major axis of its orbit.
Further reading
Books, Articles or other print media on this topic
External links
References
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