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Kepler's First Two Laws
Yazar:
Šárka Voráčová
Simulation of planetary motion applying Kepler's first two laws: (a) elliptical orbits with (2) ray from Sun to planet sweeping out constant area per unit time. Simplified from "Planetary Orbit by Kepler" by Hans Oosting.
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Kvadratická funkcia f: y = ax^2
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