Let us treat a helicopter rotor blade as a long, thin rod, as shown in Fig. 8–49. (a) If each of the three rotor helicopter blades is 3.75 m long and has a mass of 135 kg, calculate the moment of inertia of the three rotor blades about the axis of rotation. (b) How much torque must the motor apply to bring the blades from rest to a speed of 6.0 rev/s in 8.0 s?

FIGURE 8-49

Problem 43

Short Answer

Expert verified
  1. The moment of inertia is \(1.90 \times {10^3}\;{\rm{kg}} \cdot {{\rm{m}}^{\rm{2}}}\).
  2. The required torque is \(8900\;{\rm{m}} \cdot {\rm{N}}\).

Step by step solution

01

Concepts

The torque is the product of the moment of inertia and the square of the distance. For this problem, first, find the total moment of inertia and then find the angular acceleration to find the torque.

02

Given data

The initial angular velocity of the blades is \({\omega _1} = 0\).

The final angular velocity is \({\omega _2} = 6.0\;{\rm{rev/s}} = 6.0 \times 2\pi \;{\rm{rad/s}}\).

The length of the blades is \(L = 3.75\;{\rm{m}}\).

The time is taken by the helicopter to reach the final angular velocity is \(t = 8.0\;{\rm{s}}\).

The mass of each blade is \(m = 135\;{\rm{kg}}\).

You can assume the blades as uniform rods rotating about one end.

Let I be the moment of inertia of the blades, and \(\tau \) is the required torque.

03

Calculation for part (a)

The moment of inertia of one blade is \(\frac{1}{3}m{L^2}\).

The total moment of inertia of the three blades is

\(\begin{align}I &= 3 \times \frac{1}{3}m{L^2}\\ &= 3 \times \frac{1}{3} \times \left( {135\;{\rm{kg}}} \right) \times {\left( {3.75\;{\rm{m}}} \right)^2}\\ &= 1898.44\;{\rm{kg}} \cdot {{\rm{m}}^{\rm{2}}}\\ \approx 1.90 \times {10^3}\;{\rm{kg}} \cdot {{\rm{m}}^{\rm{2}}}\end{align}\).

Hence, the moment of inertia is \(1.90 \times {10^3}\;{\rm{kg}} \cdot {{\rm{m}}^{\rm{2}}}\).

04

Calculation for part (b)

Now, the angular acceleration of the rotor is

\(\begin{align}\alpha &= \frac{{{\omega _2} - {\omega _1}}}{t}\\ &= \frac{{6.0 \times 2\pi \;{\rm{rad/s}} - 0}}{{8.0\;{\rm{s}}}}\\ &= 4.71\;{\rm{rad/}}{{\rm{s}}^{\rm{2}}}\end{align}\)

The required value of the torque is

\(\begin{align}\tau &= I\alpha \\ &= \left( {1898.44\;{\rm{kg}} \cdot {{\rm{m}}^{\rm{2}}}} \right) \times \left( {4.71\;{\rm{rad/}}{{\rm{s}}^{\rm{2}}}} \right)\\ &= 8941.65\;{\rm{m}} \cdot {\rm{N}}\\ &= 8900\;{\rm{m}} \cdot {\rm{N}}\end{align}\).

Hence, the required torque is \(8900\;{\rm{m}} \cdot {\rm{N}}\).

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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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