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A 1000 kg satellite and a 2000 kg satellite follow exactly the same orbit around the earth.
a. What is the ratio F1/F2 of the gravitational force on the first satellite to that on the second satellite?
b. What is the ratio a1/a2 of the acceleration of the first satellite to that of the second satellite?

Short Answer

Expert verified

a) The ratio F1/F2 = ½

b) Ratio a1/a2 =1

Step by step solution

01

Part(a) Step 1: Given information

Mass of satellite 1 = 1000 kg

Mass of satellite 2 = 2000 kg

Follow exactly the same orbit around the earth.

02

Part(a) Step 2 Explanation

Calculate gravitation force on each satellite and find the ratio

Gravitational force on Satellite 1

F1= m1g = 1000 kg x g --------------------------(1)

Gravitational force on Satellite 2

F2= m2g = 2000 kg x g --------------------------(2)

Divide equation (1) and (2) we get

F1 /F2 = 1/2

03

Part(b) Step 1 : Given Information

Mass of satellite 1 = 1000 kg

Mass of satellite 2 = 2000 kg

Follow exactly the same orbit around the earth.

04

Part(b) Step 2: Explanation

Find a for each satellite and find the ratio

Force on Satellite 1

F1=m1a∣F1=1000×a1….....................(4)

Similarly on satellite 2

F2=m2a2F2=2000×a2….......................(5)F1F2=1000×a12000×a212=12×a1a2a1a2=1

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Most popular questions from this chapter

FIGURE P13.57 shows two planets of mass m orbiting a star of mass M. The planets are in the same orbit, with radius r, but are always at opposite ends of a diameter. Find an exact expression for the orbital period T. Hint: Each planet feels two forces.

Let’s look in more detail at how a satellite is moved from one circular orbit to another. FIGURE CP13.71shows two circular orbits, of radii localid="1651418485730" r1and localid="1651418489556" r2, and an elliptical orbit that connects them. Points 1and 2are at the ends of the semimajor axis of the ellipse.

a. A satellite moving along the elliptical orbit has to satisfy two conservation laws. Use these two laws to prove that the velocities at points localid="1651418503699" 1and localid="1651418499267" 2are localid="1651418492993" v1′=2GMr2/r1r1+r2and localid="1651418509687" v2′=2GMr1/r2r1+r2The prime indicates that these are the velocities on the elliptical orbit. Both reduce to Equation 13.22if localid="1651418513535" r1=r2=r.

b. Consider a localid="1651418519576" 1000kgcommunications satellite that needs to be boosted from an orbit localid="1651418573632" 300kmabove the earth to a geosynchronous orbit localid="1651418578672" 35,900kmabove the earth. Find the velocity localid="1651418584351" v1on the inner circular orbit and the velocity localid="1651418590277" v=1at the low point on the elliptical orbit that spans the two circular orbits.

c. How much work must the rocket motor do to transfer the satellite from the circular orbit to the elliptical orbit?

d. Now find the velocity localid="1651418596735" v=2at the high point of the elliptical orbit and the velocity v2 of the outer circular orbit.

e. How much work must the rocket motor do to transfer the satellite from the elliptical orbit to the outer circular orbit?

f. Compute the total work done and compare your answer to the result of Example localid="1651418602767" 13.6.

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