ORIGINS 2B03 Lecture 14: Lecture 14
Document Summary
Matter tells spacetime how to curve, spacetime tells matter how to move along with light. Needed to explain small scales in perspective to big things. Differential gravity (tides are caused by tidal force) Stronger gravitational forces on things closer to the mass. The moon pulls the water from the earth causing tides. In real gravitational fields the acceleration is not exactly constant. The difference between a star and planet is nuclear fusion (not larger than 13x the size of jupiter) Special class of objects that burn deuterium are called brown dwarf. Basically extra-solar planets need to be in orbit around a star and not be burning hydrogen (or any nuclear fusion) Finding planets around other stars is very difficult - stars are big and very bright and their planets are small and very dim. Transit method: watch a given star very patiently and continuously. If one of its planets go in front of it, it gets dimmer.