Students will be able to
- know that for an object to move in a circular orbit around a large object of mass at a radial distance , it must have an orbital speed given by ,
- calculate , , or using .
Students should already be familiar with
- the basic terminology of orbits: orbital speed, orbital period, and orbital radius,
- how to use simple formulae to find the basic properties of a circular orbit (i.e., using to find the orbital period from the orbital speed and radius),
- the idea that for an object moving in a circular orbit, the acceleration of the object is given by , where is the linear speed of the object and is the radius of the orbit,
- the idea that the acceleration due to gravity at a point near a massive object is given by .
Students will not cover
- noncircular orbits,
- Kepler’s third law of planetary motion.