Transit timing observations from kepler i. statistical analysis of the first four months
The Inner Planets: Geology Inner planets vs outer planets Making surfaces Sources of heat Interiors, layering and why Surface Area to Volume ratio and.
F. Marzari, Dept. Physics, Padova Univ. The role of migration and planet-planet scattering in shaping planetary systems.
NASA Image MOLA Digital Altimetry Martian Oceans Evidence for a Northern Ocean on Mars.
Earth-Moon System Section 25.2. Earth’s Moon The moon is about 384,000 kilometers away from the Earth Moon’s gravity is too weak to hold onto gas molecules,
Other Science from Microlensing Surveys I or Microlenses as Stellar Probes By Jonathan Devor.
Condensation of the Solar Nebula Composition of the Solar Nebula As the protoplanetary disk cools, materials in the disk condensate into planetesimals.
April 18, 2006Astronomy 20101 Chapter 12: Comets and Asteroids: Debris of the Solar System.
PTYS/ASTR 206Asteroids/Meteorites 4/17/07 Asteroids and Meteorites.
What Is a Planet? Pluto and Its Place in the Solar System Dr. Matthew Tiscareno, Cornell University.
The Basics of Registax 6 David O’Dell Anderson High School Austin, TX.
The Origin of the Solar System. The Great Chain of Origins: Early Hypotheses 1) Catastrophic hypotheses Example: passing star hypothesis: Star passing.
