Kepler’s Laws of Planetary Orbits: All deduced from observations 1. Orbits are ellipses 2. Plane Velocity Varies as it orbits 3. P 2 = A 3. Ptolemy. Copernicus – doesn’t quite get it right – still needs epicycles. Tycho’s Insane Model. Kepler’s Ultimate Resolution. An Ellipse:.
Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.
Kepler’s Laws of Planetary Orbits:All deduced from observations1. Orbits are ellipses2. Plane Velocity Varies as it orbits3. P2 = A3
Eccentricity of Mars orbit means variations in Earth-Mars distance at opposition
Kepler’s Second Law – Equal areas in Equal Times
This requires the planet to move fastest when its closest to the sun
P = orbital period measured in units of years
A = orbital distance, measured in units of AU (1 AU = 1
Astronomical Unit = distance from the Earth to the Sun
Kepler’s Laws are a purely empirical and precise description of the orbits of the planets
But, he has no dynamical basis for understanding why these laws exist.