Two earth satellites, a and b, each of mass m, are to be launched into circular orbits about earth's center. satellite a is to orbit at an altitude of 5920 km. satellite b is to orbit at an altitude of 19600 km. the radius of earth reis 6370 km. (a) what is the ratio of the potential energy of satellite b to that of satellite a, in orbit? (b) what is the ratio of the kinetic energy of satellite b to that of satellite a, in orbit? (c) which satellite (answer a or b) has the greater total energy if each has a mass of 12.0 kg? (d) by how much?

(a) 0.473

The potential energy of a satellite orbiting around Earth is given by

where

G is the gravitational constant

M is the Earth's mass

m is the satellite's mass

R is the Earth's radius

h is the altitude of the satellite above the Earth's surface

So the potential energy of satellite A is

while potential energy of satellite B is

Therefore the ratio of the potential energy of satellite B to that of satellite A is

and using

hA = 5920 km

hB = 19600 km

R = 6370 km

we find

(b) 0.473

The kinetic energy of a satellite orbiting around Earth instead is given by

So the kinetic energy of satellite A is

while kinetic energy of satellite B is

Therefore the ratio of the kinetic energy of satellite B to that of satellite A is

which is identical to before, so it  gives

(c) Satellite B

The total energy of a satellite in orbit is given by

We see that the total energy is:

1) negative (because the satellite is on a bound orbit)

2) inversely proportional to the distance of the satellite from the Earth's center, R+h

So the magnitude of the fraction in the equation is larger for the satellite which is closer to the Earth's surface (satellite A), but since the energy is negative, this means that the total energy of this satellite is smaller than that of satellite B. So, satellite B has a greater total energy.

(d)

We have to calculate the total energy of each satellite.

Given:

m = 12.0 kg

We find:

So the difference in total energy is

jupiter is the largest planet in our solar system, having a mass and radius that are respectively, 318 and 11.2 times that of earth. suppose that an object falls from rest near the surface of each planet and that the acceleration due to gravity remains constant during the fall. each object falls the same distance before striking the ground. determine the ratio of the time of fall on jupiter to that on earth.