/*! 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} Q38P In deep space, sphere A of mass... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

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?

Short Answer

Expert verified

a. The gravitational potential energy of the two-sphere system just as B is released is-1.7×10-8J

b. The kinetic energy of B when it has moved 0.20mtowards A is 5.6×10-9J.

Step by step solution

01

Step 1: Given

Sphere A,MA=20kgat originx=0mand

Sphere B, MB=10kg at x=0.80m

02

Determining the concept

Using the formula of gravitational potential energy and the principle of conservation of energy, find thegravitational potential energy of the two-sphere system just as B is released and the kinetic energy of B when it has moved towards Arespectively. According to the law ofconservation of energy, energy can neither be created nor be destroyed.

Formulae are as follows:

Ui+Ki=Uf+KfU=GMAMBRK=12mv2

where, MA,  MB, m are masses, R is the radius, v is velocity, G is gravitational constant, K is kinetic energy and U is potential energy.

03

(a) Determining the gravitational potential energy of the two-sphere system just as   is released

Now,

Ui=-GMAMBri

As

MA=20kg, MB=10kg,and ri=0.80mUi=-6.67×10- 11m3s2·kg20kg10kg0.80m=-1.7×10-8J

Hence, the gravitational potential energy of the two-sphere system just as B is released is -1.7×10-8J.

04

(b) Determining the kinetic energy of  B when it has moved  0.20m towards  A

Now,

Ui+Ki=Uf+Kf

As

Ui=-1.7×10-8J,andKi=0ri=0.80m -0.20m=0.60m

-1.7×10-8J=K-6.67×10- 11m3s2·kg20kg10kg0.60m-1.7×10-8J=K-2.22×10-8JK=5.6×10-9J

Hence, the kinetic energy of when it has moved 0.20mtowards A is 5.6×10-9J.

Therefore, using the formula for gravitational potential energy and the law of conservation of energy, kinetic energy 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

Figure 13-43 gives the potential energy functionU(r) of aprojectile, plotted outward from the surface of a planet of radius Rs. If the projectile is launched radially outward from the surfacewith a mechanical energy of -2.0×109J, what are (a) its kineticenergy at radius r=1.25Rsand (b) itsturning point (see Module 8-3)in terms ofRs?

To alleviate the traffic congestion between two cities such as Boston and Washington, D.C, engineers have proposed building a rail tunnel along a chord line connecting the cities (Fig. 13-55). A train, unpropelled by any engine and starting from rest, would fall through the first half of the tunnel and then move up the second half. Assuming Earth is a uniform sphere and ignoring air drag and friction, find the city-to-city travel time.

In 1993 the spacecraft Galileosent an image (Fig. 13-48) of asteroid 243 Ida and a tiny orbiting moon (now known as Dactyl), the first confirmed example of an asteroid–moon system. In the image, the moon, which is 1.5kmwide, is100km from the center of the asteroid, which is role="math" localid="1661157158474" 55kmlong. Assume the moon’s orbit is circular with a period of 27h.

(a) What is the mass of the asteroid?

(b) The volume of the asteroid, measured from the Galileoimages, is14100 â¶Ä‰k³¾3 . What is the density (mass per unit volume) of the asteroid? was sent spinning out of control. Just before the collision and in

The presence of an unseen planet orbiting a distant star can sometimes be inferred from the motion of the star as we see it. As the star and planet orbit, the center of mass of the star-planet system, the star moves toward and away from us with what is called the line of sight velocity, a motion that can be detected. Figure 13-49 shows a graph of the line of sight velocity versus time for the star 14 â¶Ä‰Herculis. The star’s mass is believed to be 0.90 of the mass of our Sun. Assume that only one planet orbits the star and that our view is along the plane of the orbit. Then approximate (a) the planet’s mass in terms of Jupiter’s mass mJand

(b) the planet’s orbital radius in terms of Earth’s orbital radiusrE .

Mile-high building.In 1956, Frank Lloyd Wright proposed the construction of a mile-high building in Chicago. Suppose the building had been constructed. Ignoring Earth’s rotation, find the change in your weight if you were to ride an elevator from the street level, where you weigh600N, to the top of the building.

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.