Motions of the Night Sky Stars, Sun, Moon, Planets.
Protoplanetary Disks: The Initial Conditions of Planet Formation Eric Mamajek University of Rochester, Dept. of Physics & Astronomy Astrobio 2010 – Santiago.
Kepler’s Laws. Kepler and the Physics of Planetary Motion Laws of Planetary Motion Law 1 - Law of Ellipses Law 2 - Law of Equal Areas Law 3 - Harmonic.
Modificado de: Earth’s Tides Simulation Craig Brubaker Union College 2/28/04.
A1 05 Sol Sys Formation
Impact of Climate Change and Variability
Our universe is estimated to be at least 156 billion light years in diameter—with a volume of 1.94e+015 cubic light years. To cross this distance, traveling.
Astronomy 1010-H Planetary Astronomy Fall_2015 Day-14.
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.
SEARCHING FOR EXTRA-SOLAR PLANETS John Webb Dept. of Astrophysics UNSW.
Our Solar System Chapter 28. Formation of the Solar System 28.1.
Ptolemy
