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Leyes de Kepler

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Leyes de Kepler

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Leyes del movimiento planetario

Created by

Profe Maria Eugenia Richardi
Profe Maria Eugenia Richardi
Argentina

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Leyes de Kepler
 

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Leyes de KeplerOnline version

Leyes del movimiento planetario

by Profe Maria Eugenia Richardi
1

Las leyes de Kepler describen el movimiento de los planetas alrededor del . La primera ley establece que las de los planetas son , con el sol ubicado en uno de sus focos . La segunda ley señala que un radio que une un planeta con el sol barre áreas iguales en tiempos iguales , lo que implica que la velocidad orbital varía . Según la tercera ley , el cuadrado del de un planeta es proporcional al cubo de su semieje mayor . Estas ideas unifican la mecánica celeste y la observación .

2

La velocidad de un planeta se mantiene constante , lo que implica que en el perihelio la velocidad es mientras que en el afelio la velocidad tangencial es

3

Mientras más circular es una órbita planetaria la excentricidad tiende a . Mientras más " achatada " la órbita , la excentricidad se acerca a 1

4

La tercera ley de Kepler hace referencia a la proporcionalidad entre el del periodo de un planeta y el de su radio medio respecto del So l

5

Los planetas tienen un periodo mayor que los , por lo que el año de es menor que 365 días terrestres y el año de mayor que ese tiemp o

 
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