Final answer:
The eccentricity of the satellite's orbit, given a perigee radius of 20,000 km and an apogee radius of 150,000 km, is approximately 0.7059.
Step-by-step explanation:
To calculate the eccentricity of an orbit for a satellite, you need to know the perigee and apogee distances. The perigee distance (closest point to Earth) is given to be 20,000 km. The apogee distance (farthest point from Earth) is 150,000 km. The equation for eccentricity (e) is e = (apogee - perigee) / (apogee + perigee). First convert these distances to the distances from the center of the Earth by adding the radius of the Earth (RE) to both the perigee and apogee distances.
Perigee radius = 20,000 km + RE = 20,000 km + 6378 km = 26378 km
Apogee radius = 150,000 km + RE = 150,000 km + 6378 km = 156378 km
Now, plug the values into the eccentricity formula:
e = (156378 km - 26378 km) / (156378 km + 26378 km)
e = 129,000 km / 182,756 km
e = 0.7059
The eccentricity of the satellite's orbit is approximately 0.7059.