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Two blocks, each of mass m, are attached to the ends of a massless rod which pivots as shown in Fig. 8–43. Initially the rod is held in the horizontal position and then released. Calculate the magnitude and direction of the net torque on this system when it is first released.

Short Answer

Expert verified

The net torque on the system is \(\sum {\tau = mg} \left( {{l_2} - {l_1}} \right)\) in the clockwise direction.

Step by step solution

01

Definition of torque

Torque is defined as the measure of the force that causes an object to rotate about an axis. It is also called the rotational equivalent of linear force.

Mathematically, torque is represented as follows:

\(\begin{align}\vec \tau &= \vec r \times \vec F\\\left| \tau \right| &= rF\sin \theta \end{align}\) … (i)

Here, F is the applied force, and r is the perpendicular distance between the point about which the torque is calculated and the point of application of force.

02

Determination of the net torque on the system

There is a torque due to the force of gravity (weight) on the left block that will accelerate the rod anti-clockwise. Similarly, there will be a clockwise torque due to the weight of the right block.

Suppose the clockwise direction is positive. The net torque acting on the system will be given as follows:

\(\begin{align}\sum \tau &= mg{l_2} + \left( { - mg{l_1}} \right)\\ &= mg{l_2} - mg{l_1}\\ &= mg\left( {{l_2} - {l_1}} \right)\end{align}\)

Thus, the net torque is \(mg\left( {{l_2} - {l_1}} \right)\) in the clockwise direction.

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Most popular questions from this chapter

Most of our Solar System’s mass is contained in the Sun, and the planets possess almost all of the Solar System’s angular momentum. This observation plays a key role in theories attempting to explain the formation of our Solar System. Estimate the fraction of the Solar System’s total angular momentum that is possessed by planets using a simplified model which includes only the large outer planets with the most angular momentum. The central Sun (mass\(1.99 \times {10^{30}}\;{\rm{kg}}\), radius\(6.96 \times {10^8}\;{\rm{m}}\)) spins about its axis once every 25 days and the planets Jupiter, Saturn, Uranus, and Neptune move in nearly circular orbits around the Sun with orbital data given in the Table below. Ignore each planet’s spin about its own axis.

Planet

Mean Distance from Sun\(\left( { \times {{10}^6}\;{\rm{km}}} \right)\)

Orbital Period

(Earth Years)

Mass

\(\left( { \times {{10}^{25}}\;{\rm{kg}}} \right)\)

Jupiter

778

11.9

190

Saturn

1427

29.5

56.8

Uranus

2870

84.0

8.68

Neptune

4500

165

10.2

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