1112
Text Assignments:
Phy 201: Chapter 5, problems 3, 8, 10, 15, 18, 30, 36, 40, 48, 50
University Physics: Chapter 12, problems 41, 44, 49, 51, 56, 58, 60, 61, 67
Using the gravitational field simulation at
and do the following Simulation Experiment:
[G:=6.67*10^-11,M:=6*10^24,R_earth:=6.4*10^6]
v(r):=sqrt(G M / r)
Enter in v(R_earth), click on Simplify, Approximate and Approximate.
Angular Velocities
Set a satellite in a circular orbit at a distance of 2 Earth radii and determine the angular speed of the simulated orbit in radians per second. Do this in two ways.
First send out seven straight 'shots' at angles of 0, 1, 2, 3, 4, 5 and 6 radians.
Find the time necessary to go through each radian, using Time Factor 100 instead of the default 1000 (this will slow the simulation by a factor of 10 so you can time it with reasonable accuracy).
Second, time the simulation for 1 complete orbit.
Also, observe the 'realtime interval' necessary to complete an orbit at this radius.
Repeat the above for an orbit at 3 Earth radii.
Repeat once more for the elliptical orbit that goes from your initial radius of the original gravitation experiment to 3 Earth radii.
Analysis:
For each orbit:
According to your observations between the 1-radian lines, what was the average angular velocity, in radians / second, for each interval?
There are 2 pi radians in a circle. According to your timing for the orbit, what was the average angular velocity of the simulation for the entire orbit?
What is the actual average angular velocity of a satellite in this orbit about the Earth (note your 'realtime interval').
Also for the elliptical orbit:
What was your approximate average distance from the center of the planet for each 1-radian interval?
How is the average distance related to the angular velocity?