Discussió:Lleis de Kepler

Corregeixo la tercera llei treient la referència a les unitats astronòmiques ja que la llei es compleix independentment de les unitats que es facin servir.--Pere prlpz 20:00, 24 nov 2006 (CET)

He corregit la llei de Kepler i he afegit una reformulació matemàtica de la 3a Llei de Kepler més ampliada. --62.57.176.118 (discussió) 09:28, 29 jul 2009 (CEST)

Traducció

--Townie (discussió) 16:23, 4 des 2018 (CET)

Animations demonstrating Kepler's Second Law of Planetary Motion.

There is an animated figure on the English version of this page which I made which the shows motion of planets orbiting with various eccentricities around a star and may be of use.

The animated gifs are individually viewable at https://commons.wikimedia.org/wiki/File:Circular_orbit_of_planet_with_(eccentricty_of_0.0).gif https://commons.wikimedia.org/wiki/File:Ellipitical_orbit_of_planet_with_an_eccentricty_of_0.2.gif https://commons.wikimedia.org/wiki/File:Ellipitical_orbit_of_planet_with_an_eccentricty_of_0.5.gif https://commons.wikimedia.org/wiki/File:Ellipitical_orbit_of_planet_with_an_eccentricty_of_0.8.gif The code to produce the table is here (see edit mode):

Orbits of planets with varying eccentricities. The red ray rotates at a constant angular velocity and with the same orbital time period as the planet, $T=1$. S: Sun at the primary focus, C: Centre of ellipse, S': The secondary focus. In each case, the area of all sectors depicted is identical.

Low	High
Planet orbiting the Sun in a circular orbit (e=0.0)	Planet orbiting the Sun in an orbit with e=0.5
Planet orbiting the Sun in an orbit with e=0.2	Planet orbiting the Sun in an orbit with e=0.8

Mkwadee (disc.) 17:37, 20 des 2022 (CET)