/*! 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

A satellite is put in a circular orbit about Earth with a radiusequal to one-half the radius of the Moon’s orbit. What is its periodof revolution in lunar months? (A lunar month is the period of revolution of the Moon)

The figure shows not to scale, a cross section through theinterior of Earth. Rather than being uniform throughout, Earth isdivided into three zones: an outercrust,amantle,and an innercore.The dimensions of these zones and the masses contained within them are shown on the figure. Earth has a total mass of5.98×1024kgand a radius of6370km. Ignore rotation and assumethat Earth is spherical. (a) Calculateat the surface. (b) Suppose that a bore hole (theMohole) is driven to the crust–mantle interface at a depth of25.0km; what would be the value ofat the bottom of the hole? (c) Suppose that Earth were a uniform spherewith the same total mass and size. What would be the value ofat a depth of25.0km? (Precise measurements ofare sensitive probes of the interior structure of Earth, although results can be becloud by local variations in mass distribution.)

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?

One dimension.In the figure, two point particles are fixed on anxaxis separated by distanced. ParticleAhas massmAM and particle Bhas mass3.00mA. A third particle C, of mass750mA, is to be placed on the xaxis and near particles Aand B. In terms of distance d, at what xcoordinate should Cbe placed so that the net gravitational force on particle Afrom particles Band Cis zero?

(a) What is the gravitational potential energy of the two-particle system in Problem 3? If you triple the separation between theparticles, how much work is done (b) by the gravitational force between the particles and (c) by you?

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.