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?

Short Answer

Expert verified
  1. Kinetic energy at radius r=1.25Rsis 2×109J.
  2. Turing point in terms of Rs is r=2.5Rs.

Step by step solution

01

Step 1: Given

Mechanical energy (ME)is -2.0×109J.

02

Determining the concept

Use the formula for mechanical energy to find kinetic energy at a particular point.Mechanical energy is the energy possessed by an object due to its motion or due to its position.

The formula is as follows:

ME=KE+U

whereMEis mechanical energy, KE is kinetic energy and U is potential energy.

03

(a) Determining the kinetic energy at the radius  r=1.25 Rs

Use the formula of mechanical energy to find kinetic energy as follows:

ME=KE+U

From graph,

U at r=1.25Rs is -4.0×109J

So,

-2.0×109J=-4×109J+KEKE=2.0×109J

Hence, kinetic energy at radius r=1.25Rsis 2×109J.

04

(b) Determining the turning point in terms of  Rs

The turning point is the point where mechanical energy is equal to potential energy.

Now,U=-4.0×109J atr=1.25Rs.So, reducing potential energy by a factor of 2, means the r value must be increased by a factor of 2.

Hence,the turning point in terms ofRsisr=1.25Rs.

Gravitational potential energy is inversely proportional to the distance between the objects. If the distance is reduced, the potential energy increases. In this problem, thisconcept can be used to calculatethe change in gravitational potential energy.

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

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?

(a) What is the escape speed on a spherical asteroid whose radius is500 kmand whose gravitational acceleration at the surface is 3.0ms2 ? (b) How far from the surface will a particle go ifit leaves the asteroid’s surface with a radial speed of 1000m/s? (c)With what speed will an object hit the asteroid if it is dropped from1000kmabove the surface?

Question: A satellite is in elliptical orbit with a period of 8.00×104s about a planet of massM=7.00×1024kg . At aphelion, at radius4.5×107m , the satellite’s angular speed is7.158×10-5rads .What is its angular speed at perihelion?

Question: The radius Rh of a black hole is the radius of a mathematical sphere, called the event horizon that is centered on the black hole. Information from events inside the event horizon cannot reach the outside world. According to Einstein’s general theory of relativity,Rh=2GM/c2 , where Mis the mass of the black hole and cis the speed of light.

Suppose that you wish to study a black hole near it, at a radial distance of 50Rh. However, you do not want the difference in gravitational acceleration between your feet and your head to exceed 10 m/s2 when you are feet down (or head down) toward the black hole. (a) As a multiple of our Sun’s mass Ms , approximately what is the limit to the mass of the black hole you can tolerate at the given radial distance? (You need to estimate your height.) (b) Is the limit an upper limit (you can tolerate smaller masses) or a lower limit (you can tolerate larger masses)?

The Sun and Earth each exert a gravitational force on theMoon. What is the ratioFsun/FEarthof these two forces? (The average Sun–Moon distance is equal to the Sun–Earth distance.)

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