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Re: [Phys-l] gravitational force



On Oct 31, 2006, at 2:04 PM, Scott Goelzer wrote:

Hi Mike,
Not for real, but still fun.

I use a solar system simulator (such as Gravitation 5.0 (?) for the
Mac) and have the students tweak a planet's velocity and radius until
they achieve circular orbit - its takes students forever to realize
that the velocity must be tangent. Then the local G for the simulator
can be calculated from Newton's synthesis. In many simulators, it's
not the real value of G. Now, with G, they can compute the
velocities and radii for the planets (4 or 5) in a stable solar
system and derive a nice linear T^2 vs r^3 plot from data obtained.

Elliptical orbits can also be set up, allowing the Law of Areas
explored. I do not go too far with this mathematically at the HS level.

It is also a great introduction to perturbation since most initial
student solar system designs accrete into a single blob.

For a fake lab, it makes for a great couple of periods - better than
movies or me drawing spastic ellipses on the board with triangles
inside them.

Scott's message appeared as soon as my was sent. Let me mention that a pendulum trajectories can be filmed from below. This shows elliptical and circular orbits when the bob is initially pushed sidewise.

Ludwik Kowalski
Let the perfect not be the enemy of the good.