In Figure 11.26, if rA=3m, and θ=30°, what is the magnitude of the torque about locationAincluding units? If the force in Figure 11.26 were perpendicular to rA but gave the same torque as before, what would be its magnitude?

Short Answer

Expert verified

The magnitude of torque at location A is6N.m.

The magnitude of the force relative to location A is2N .

Step by step solution

01

Definition of Torque

The force that can cause an object to twist along an axis is measured as torque. In linear kinematics, force is what causes an object to accelerate. Torque is also responsible for the angular acceleration. As a result, torque can be defined as the linear force's rotational equivalent.

02

The given data

Given:

Force acting on the ranch,F=4N

Force is at an angle,θ=30°

Length of the ranch,rA=3m

The figure given below shows the direction of the force on the wrench.

03

Find the magnitude of the force relative to location A 

Magnitude of the torque relative to location A is given by formula:

Torque, τ=rAFsinθ

Substitute the values in the above equation

τ=(3m)(4N)sin30°=6N.m

Hence, the magnitude of torque at location A is 6N.m.

To produce the same torque, the amount of the force acting on the torque relative to position A is given by-

F=τrAsinθ

F=(6N.m)(3m)sin90°=2N

Hence, the magnitude of force at location A is 2N.

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

What is the direction of the orbital (translational) angular momentum of the comet shown in the figure relative to the Sun?

A yo-yo is constructed of three disks: two outer disks of mass M, radius R, and thickness d, and an inner disk (around which the string is wrapped) of mass , radius , and thickness d. The yo-yo is suspended from the ceiling and then released with the string vertical (figure).

Calculate the tension in the string as the yo-yo falls. Note that when the center of the yo-yo moves down a distance y, the yo-yo turns through an angley/r,which in turn means that the angular speedωis equal to vCM/r. The moment of inertia of a uniform disk is12MR2.

If an object has a moment of inertia \(19\,\,{\rm{kg}} \cdot {{\rm{m}}^{\rm{2}}}\) and the magnitude of its rotational angular momentum is \(36\,\,\,{\rm{kg}} \cdot {{\rm{m}}^{\rm{2}}}{\rm{/s}},\) what is its rotational kinetic energy?

In Figure 11.95 two small objects each of mass \({m_1}\)are connected by a light weight rod of length \(L.\) At a particular instant the center of mass speed is\({v_1}\) as shown, and the object is rotating counterclockwise with angular speed \({\omega _1}\). A small object of mass \({m_2}\) travelling with speed \({v_2}\) collides with the rod at an angle \({\theta _2}\) as shown, at a distance\(b\)from the center of the rod. After being truck, the mass \({m_2}\) is observed to move with speed \({v_4}\) at angle\({\theta _4}\).All the quantities are positive magnitudes. This all takes place in outer space.

For the object consisting of the rod with the two masses, write equations that, in principle, could be solved for the center of mass speed \({v_3},\) direction \({\theta _3},\) and angular speed \({\omega _3}\)in terms of the given quantities. Sates clearly what physical principles you use to obtain your equations.

Don’t attempt to solve the equations; just set them up.

In Figure 11.96a spherical non-spinning asteroid of mass\(M\)and radius\(R\)moving with speed\({v_1}\)to the right collides with a similar non-spinning asteroid moving with speed\({v_2}\)to the left, and they stick together. The impact parameter is\(d\).Note that\({I_{sphere}} = \frac{2}{5}M{R^2}.\)

After the collision, what is the velocity \({v_{CM}}\) of the center of mass and the angular velocity \(\omega \) about the center of mass? (Note that each asteroid rotates about its own center with this same \(\omega \)).

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