00:01
Now, in this problem, we can consider the gravitational force acting on the satellite is given by newton's law of gravitation.
00:27
Hence we could write force is equivalent to g times m1 m2 divided by r square, where g is equivalent to gravitational constant, m1 and m2 is equivalent to the mass of the earth and the satellite, while r is the distance between the centers.
01:12
Next, we can say that the gravitational field at the location of the satellite is defined as the force per its unit mass, which is g is equivalent to f divided by m2, where m2 is the mass of the satellite.
01:50
So, we could write this as g m1 divided by r square.
01:55
Next, satellite's acceleration is determined by newton's second law as equivalent to m2 a, so where a is nothing but the acceleration of the satellite.
02:30
Now we can solve for the acceleration of the satellite and say that a is ratio of force upon the mass, which is m2...