Debby Heyes, who attended my open lab this summer,has a quick AP physics 1 question:

**Are Kepler's Laws included in the course?**

Fast answer: no. A search in the curriculum guide for "Kepler" gives no results.

Deeper answer:

**Yes AND No**. Kepler's laws by name are not part of the curriculum, but some of the behavior of planetary orbits described by Kepler's laws*is*part of AP Physics 1.
The "equal areas / equal times" law can be stated as a consequence of angular momentum conservation. An orbiting planet experiences no torque relative to the central star (because the gravitational force always points back to the center of rotation, meaning the distance term in "torque = force * distance" is zero). Therefore, the planet's angular momentum about the central star is conserved. Treating the planet as a point object, its angular momentum is given by

*mvr*, where*r*is the distance to the central star. When*r*goes down -- i.e. when the planet is closer to the sun --*v*goes up, meaning the planet moves faster in its orbit. That's essentially Kepler's law.
The "period proportional to the 3/2 power of the radius" law is merely a consequence of Newton's second law and circular motion, at least if we consider circular orbits only (which we emphatically do in AP Physics 1). Set the gravitataional force equal to

*ma*, where the acceleration in circular motion is*v*^{2}/*r*. Then the speed of an object in circular motion is the circumference divided by the orbital period. Solving for period gives the Kepler's law relationship -- and we should be able to do that and understand it in AP Physics 1.
The law that says "all orbits are ellipses with the sun at one focus" is not in any way on the AP Physics 1 exam that I can tell.

Then, I pull up "my solar system", a phet simulation. Using the "sun and planet" preset, students are asked to change the simulation as described on their paper to see if they get a circular orbit. (Those who told me that changing the satellite's mass changes its orbital speed as well become confused a bit when the simulation doesn't verify their answer.)

**An exercise I'm running...**I'm asking students what happens to the speed necessary to maintain a circular orbit if (a) the central star's mass is doubled, (b) the planet's mass is doubled, or (c) the planet's distance from the central star is doubled. I hand everyone a different half-page of paper with one of these three questions asked; for more variety, some of the papers say "tripled" or "quadrupled" rather than doubled. Students are guided to solve in variables for the speed, then to use semi-quantitative reasoning to see what happens to the speed.Then, I pull up "my solar system", a phet simulation. Using the "sun and planet" preset, students are asked to change the simulation as described on their paper to see if they get a circular orbit. (Those who told me that changing the satellite's mass changes its orbital speed as well become confused a bit when the simulation doesn't verify their answer.)