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What is the ratio of the sun’s gravitational force on you to the
earth’s gravitational force on you?

Short Answer

Expert verified

Ratio sun's gravitational force on me to earth's gravitational force on me is

Fs/Fe=5.98 x 10-4

Step by step solution

01

Given information

Mass of earth: Me=5.97 x 1024 kg
Mass of sun: Me=1.98 x 1030 kg
Radius of earth: re}=6.37 x 106 m
Distance from sun to earth: rse=1.5 x 1011m

02

Explanation

We can calculate Gravitational force by

F=GMmr2

First find the gravitation force of Earth on you

Fe=GmMere2=Gm5.97×1024kg6.37×106m2............................(1)

now find Sun's gravitational force

FS=GmMsrse2=Gm1.98×1030kg1.5×1011m2.....................(2)

Now find the ratio

we get

FsFe=5.98×10-4

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Most popular questions from this chapter

A projectile is shot straight up from the earth’s surface at a speed of 10,000km/h. How high does it go?

a. What is the free-fall acceleration at the surface of the sun?

b. What is the free-fall acceleration toward the sun at the distance of the earth?

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Hint: You will need to use two conservation laws.

FIGURE CP13.72 shows a particle of mass m at distance x from the center of a very thin cylinder of mass M and length L. The particle is outside the cylinder, so x > L/2.
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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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