Solar System Physics I Dr Martin Hendry 5 lectures, beginning Autumn 2007 Department of Physics and Astronomy Astronomy 1X Session 2007-08.
AST 4.1 PPT
Make Up Bellwork Makeup bellwork is for those who are absent and need to make up a day or two of bellwork.
Dynamics of the young Solar system Kleomenis Tsiganis Dept. of Physics - A.U.Th. Collaborators: Alessandro Morbidelli (OCA) Hal Levison (SwRI) Rodney Gomes.
Chapter 8 Review Clickers The Cosmic Perspective Seventh Edition © 2014 Pearson Education, Inc. Formation of the Solar System.
High P and T at center of Solar nebula cause hydrogen atoms to fuse together to form helium Solid particles condense and collide to form planetesimals.
Models of the Solar System Geocentric Model - Earth is considered to be the center and everything else revolves around it.
Our Solar System. Consists of the sun, eight planets, their moons, asteroids, comets, and The planets are all unique and differ in terms of their: –
The Origin of Our Solar System Part 2
SEMESTERCOMPONENTWEIGHTING 1 2 x Common Tasks (research; common test Term 2)60 Practical work e.g. formal reports, experimental design, investigation follow-up.
Other Interesting Aspects of Astronomy
The Origin of Our Solar System Part 1 Survey of the solar system 1.