/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Q60P In Fig. 13-50, two satellites, A... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

In Fig. 13-50, two satellites, A and B, both of mass m=125kg , move in the same circular orbit of radius r=7.87×106maround Earth but in opposite senses of rotation and therefore on a collision course.

(a) Find the total mechanical energy role="math" localid="1661161625366" EA+EBof thetwosatellites+Earth system before the collision.

(b) If the collision is completely inelastic so that the wreckage remains as one piece of tangled material ( mass=2m), find the total mechanical energy immediately after the collision.

(c) Just after the collision, is the wreckage falling directly toward Earth’s center or orbiting around Earth?

Short Answer

Expert verified
  1. The total mechanical energy EA +EB of the two satellites + Earth system before the collision is−6.33×109 J.
  2. The total mechanical energy immediately after the collision is-6.33×109 J.
  3. Just after the collision, the wreckage will fall directly toward the Earth’s center.

Step by step solution

01

Step 1: Given

The mass of each satellite A and B isM=125 k²µ

The radius of the orbit of satellites around the Earth isR=7.87×106″¾

02

Determining the concept

Using the formula for the total mechanical energy of an orbiting satellite around the Earth, findthe total mechanical energy of the two satellites + Earth system before the collision and after the collision. From the velocity of the wreckage, interpret its direction of motion.

The formula is as follows:

E=−GMEm2r

where E is total mechanical energy, G is gravitational constant, ME, m are masses and r is the radius.

03

(a) Determining the total mechanical energy EA +EB of the two satellites + Earth system before the collision

The total mechanical energy of an orbiting satellite around the Earth is,

E=−GMEm2r

The total mechanical energy of the two satellites + Earth system before the collision is,

EA+EB=−GMEm2r+−GMEm2r

EA+EB=−GMEmr

EA+EB=−(6.67×10−11 N⋅m2/kg2)(5.98×1024 kg)(125 kg)7.87×106 m=−6.33×109 J

Hence,the total mechanical energy EA +EB of the two satellites + Earth system before the collision is −6.33×109J.

04

(b) Determining the total mechanical energy immediately after the collision

The total mechanical energy immediately after the collision is,

E=−GME(2m)2r

E=−GMEmr

E=−(6.67×10−11 N⋅m2/kg2)(5.98×1024 kg)(125 kg)7.87×106 m=−6.33×109 J

Hence, the total mechanical energy immediately after the collision is −6.33×109 J.

05

(c) Determining whether the wreckage is falling directly toward the earth’s center or orbiting around earth just after the collision 

Just after the collision, the wreckage has zero velocity. So, it will fall towards the Earth’s center.

Therefore, using the formula for the total mechanical energy of an orbiting satellite around the Earth, the total mechanical energy before and after the collision of satellites can be found.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91Ó°ÊÓ!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

In the figure, three 5.00kgspheres are located at distancesd1=0.300 mandd2=0.400 m. What are the (a) magnitude and (b) direction (relative to the positive direction of thexaxis) of the net gravitational force on sphereBdue to spheresAandC?

In Figure (a), particleAis fixed in place atx=-0.20m on thexaxis and particleB, with a mass of 1.0 kg, is fixed in place at the origin. ParticleC(not shown) can be moved along thexaxis, between particleBandx=∞.Figure (b)shows thexcomponentFnet,xof the net gravitational force on particleBdue to particlesAandC, as a function of positionxof particleC. The plot actually extends to the right, approaching an asymptote of−4.17×1010Nas→∞. What are the masses of (a) particleAand (b) particleC?

The radius Rhand mass Mhof a black hole are related by Rh=2GMh/c2, wherecis the speed of light. Assume that the gravitational acceleration agof an object at a distance r0=1.001Rhfrom the center of a black hole is given byag=GMr2(it is, for large black holes). (a) In terms of Mh, findagat.r0 (b) Doesagatr0 increase or decrease asMhincreases? (c) What isagatr0for a very large black hole whose mass is1.55×1012times the solar mass of1.99×1030kg? (d) If an astronaut of height1.70mis atr0with her feet down, what is the difference in gravitational acceleration between her head and feet?(e) Is the tendency to stretch the astronaut severe?

What multiple of the energy needed to escape from Earth givesthe energy needed to escape from (a) the Moon and (b) Jupiter?

Figure 13-44 shows four particles,each of mass 20.0 g, that form a square with an edge length of d =0.600 m. Ifdis reduced to0.200 m, what is the change in the gravitational potential energy of the four-particle system?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.