Müzakirə:Kepler qanunları

Animations demonstrating Kepler's Second Law of Planetary Motion.

Son rəy: 2 il öncə1 şərhMüzakirədə 1 nəfər

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

/wiki/File:Circular_orbit_of_planet_with_(eccentricty_of_0.0).gif /wiki/File:Ellipitical_orbit_of_planet_with_an_eccentricty_of_0.2.gif /wiki/File:Ellipitical_orbit_of_planet_with_an_eccentricty_of_0.5.gif /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 (müzakirə) 13:26, 20 dekabr 2022 (UTC)Cavabla

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