Bespreking:Kepler se wette
Hierdie bladsy is 'n besprekingsbladsy waar verbeteringe tot die Kepler se wette-artikel bespreek word. Hierdie bladsy is nie 'n forum vir 'n algemene bespreking van die artikel se onderwerp nie. |
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Daaglikse bladtrekke van Kepler se wette
'n Grafiek sou hier vertoon word, maar grafieke is tydelik afgeskakel. Besoek intussen gerus die interaktiewe grafiek by pageviews.wmcloud.org. |
Animations demonstrating Kepler's Second Law of Planetary Motion.[wysig bron]
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):
Low | High |
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(mkwadee) Mkwadee (kontak) 19:36, 17 Desember 2022 (UTC)