One model for a certain planet has a core of radiusR and mass Msurrounded by an outer shell of inner radius R, outer radius 2R, and mass4M. IfM=4.1×1024kgandR=6.0×106m, what is the gravitational acceleration of a particle at points (a)R(b)3Rfrom the center of the planet?

Short Answer

Expert verified

a)Thegravitational acceleration of a particle at points R from the center of the planetis7.6 m/s2.

b)Thegravitational acceleration of a particle at points 3R from the center of the planet is4.2 m/s2

Step by step solution

01

Listing the given quantities

Mass of the planetM=4.1×1024kg

Radius of the planetR=6.0×106m

02

Understanding the concept of the gravitational acceleration

Here, by using the concept of the gravitational acceleration solve the given problem

Formula:ag=GMR2

03

Calculation of the gravitational acceleration of a particle at points from the center of the planet

(a)

The gravitational acceleration is

g=GMR2=7.6 m/s2

Thegravitational acceleration of a particle at points from the center of the planet is7.6 m/s2

04

Calculation of the gravitational acceleration of a particle at points 3R from the center of the planet

(b)

Note thatthetotal mass is5M. Thus,ag

ag=G(5M)(3R)2=4.2 m/s2

Thegravitational acceleration of a particle at pointsfrom the center of the planet is4.2 m/s2

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

An asteroid, whose mass is 2.0×10−4times the mass of Earth, revolves in a circular orbit around the Sun at a distance that is twice Earth’s distance from the Sun.

(a) Calculate the period of revolution of the asteroid in years.

(b) What is the ratio of the kinetic energy of the asteroid to the kinetic energy of Earth?

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  km3 . What is the density (mass per unit volume) of the asteroid? was sent spinning out of control. Just before the collision and in

A spaceship is on a straight-line path between Earth and the Moon. At whatdistance from Earth is the net gravitational force on the spaceship zero?

Figure 13-28 shows three particles initially fixed in place, with Band Cidentical and positioned symmetrically about the yaxis, at distance dfrom A. (a) In what direction is the net gravitational forceF→net on A? (b) If we move Cdirectly away from the origin, doesFnetchange in direction? If so, how and what is the limit of the change?

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.

Sign-up for free