Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

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 is6.33×109 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 kg

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

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=(6.67×1011Nm2/kg2)(5.98×1024kg)(125kg)7.87×106m=6.33×109J

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=(6.67×1011Nm2/kg2)(5.98×1024kg)(125kg)7.87×106m=6.33×109J

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 Vaia!

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

Two dimensions.In the figure, three point particles are fixed in place in anx-yplane. ParticleAhas massmA , particleBhas mass2.00mA, and particleChas mass3.00mA. A fourth particleD, with mass4.00mA, is to be placed near the other three particles. In terms of distanced, at what (a)xcoordinate and (b)ycoordinateshould particle Dbe placed so that the net gravitational force on particle Afrom particles B, C, and Dis zero?

(a) What will an object weigh on the Moon’s surface if it weighs 100Non Earth’s surface? (b) How many Earth radii must this same object be from the centre of Earth if it is to weigh the same as it does on the Moon?

Two neutron stars are separated by a distance of1.0×1010m. They each have a mass of 1.0×1030kgand a radiusof1.0×105m . They are initially at rest with respect to each other.As measured from that rest frame, how fast are they moving when(a) their separation has decreased to one-half its initial value and(b) they are about to collide?

In deep space, sphere Aof mass 20kgis located at the origin of an x-axis and sphere Bof mass10kg is located on the axis atx=0.80m . Sphere Bis released from rest while sphere Ais held at the origin. (a) What is the gravitational potential energy of the two-sphere system just as Bis released? (b) What is the kinetic energy of Bwhen it has moved 0.20mtoward A?

Question: Consider a pulsar, a collapsed star of extremely high density, with a mass equal to that of the Sun (1.98×1030kg), a radiusRof only 12 km , and a rotational period T of 0.041s . By what percentage does the free-fall acceleration gdiffer from the gravitational acceleration agat the equator of this spherical star?

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.

Sign-up for free