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It has been argued that power plants should make use of off-peak hours (such as late at night) to generate mechanical energy and store it until it is needed during peak load times, such as the middle of the day. One suggestion has been to store the energy in large flywheels spinning on nearly frictionless ball bearings. Consider a flywheel made of iron (density 7800 kg/m\(^3\)) in the shape of a 10.0-cm-thick uniform disk. (a) What would the diameter of such a disk need to be if it is to store 10.0 megajoules of kinetic energy when spinning at 90.0 rpm about an axis perpendicular to the disk at its center? (b) What would be the centripetal acceleration of a point on its rim when spinning at this rate?

Short Answer

Expert verified
(a) Diameter is approximately 5.56 m. (b) Centripetal acceleration is approximately 49.5 m/sĀ².

Step by step solution

01

Understand the Problem

The exercise involves calculating the dimensions and physical properties of a flywheel required to store a specific amount of kinetic energy (10.0 megajoules) when rotating at a specific speed (90.0 rpm). We need to find the diameter of the disk and the centripetal acceleration of a point on its rim.
02

Find the Moment of Inertia

The kinetic energy stored in a rotating object is given by the formula \( K = \frac{1}{2} I \omega^2 \), where \( I \) is the moment of inertia and \( \omega \) is the angular velocity. For a solid disk, \( I = \frac{1}{2} m r^2 \), where \( m \) is the mass and \( r \) is the radius of the disk.
03

Relate Mass to Volume and Density

The mass \( m \) of the disk can be expressed in terms of volume \( V \) and density \( \rho \): \( m = \rho V \). The volume of the disk is \( V = \pi r^2 t \), where \( t \) is the thickness of the disk (0.10 m).
04

Calculate Angular Velocity

Convert the rotational speed from rpm to radians per second. \( \omega = 90 \cdot \frac{2\pi}{60} \approx 9.42 \) rad/s.
05

Set Up Energy Equation

Substitute \( I \) and \( \omega \) into the kinetic energy equation: \( 10 \times 10^6 = \frac{1}{2} \times \frac{1}{2} \times \rho \times \pi \times r^2 \times t \times r^2 \times (9.42)^2 \). Solving this will give us the disk's radius \( r \).
06

Solve for Radius

Rearrange and solve the equation for \( r \) to get \( r^4 = \frac{20 \times 10^6}{\rho \pi t \times (9.42)^2} \). Substitute the known values (\( \rho = 7800 \) kg/mĀ³, \( t = 0.10 \) m) to find \( r \).
07

Calculate Diameter

Once \( r \) is found, the diameter \( D \) is simply \( 2r \). Substitute \( r \) to find \( D \).
08

Calculate Centripetal Acceleration

The centripetal acceleration \( a_c = \omega^2 \times r \). Using the value of \( \omega \) calculated earlier and \( r \), find \( a_c \).

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Kinetic Energy
Kinetic energy is a form of energy associated with motion. In the context of flywheel energy storage, it's important to understand how kinetic energy works. The energy stored in a rotating object is given by the equation \( K = \frac{1}{2} I \omega^2 \). Here, \( I \) represents the moment of inertia, which is an indicator of how much mass is distributed around the axis of rotation. The term \( \omega \) is the angular velocity, representing how fast the object is spinning.
The goal with flywheels is to maximize the stored kinetic energy, allowing a power plant to store excess energy until it's needed. This approach is useful during off-peak times, when less electricity is required. Flywheels achieve this by converting electrical energy into kinetic energy and storing it within their spinning motions.
Kept in motion by nearly frictionless bearings, these flywheels can retain energy efficiently over long durations, making them ideal for balancing supply and demand in energy grids.
Moment of Inertia
The moment of inertia \( I \) is critical when discussing rotational motion, including that of a flywheel. It's a measurement that reflects how the mass of an object is spread in relation to the axis of rotation. For a solid disk, which is a common shape for flywheels, the moment of inertia is given by \( I = \frac{1}{2} m r^2 \).
Here, \( m \) denotes the mass of the disk, and \( r \) is its radius. For energy storage purposes, a larger moment of inertia implies that more energy can be stored because the distribution of mass allows for more significant rotational kinetic energy.
Designing a flywheel involves balancing mass and size because a larger radius increases the moment of inertia but also requires more material, affecting cost and practicality. Engineers must consider both the energy needs and physical constraints to design an efficient system.
Angular Velocity
Angular velocity \( \omega \) is a measure of how quickly an object rotates or spins. It's expressed in radians per second (rad/s) and is a key factor in calculating a flywheel's kinetic energy.
To convert rotational speeds from revolutions per minute (rpm) to radians per second, a simple conversion is used: \( \omega = \, \text{rpm} \times \frac{2\pi}{60} \). For example, a flywheel that rotates at 90 rpm has an angular velocity of approximately 9.42 rad/s.
This conversion is crucial, as most equations dealing with rotational dynamics, including those for kinetic energy, require angular velocity to be in radians per second. The higher the angular velocity, the greater the kinetic energy stored, assuming the moment of inertia remains constant.
Centripetal Acceleration
Centripetal acceleration \( a_c \) refers to the acceleration directed towards the center of a circular path. It is an important concept when analyzing points on the rim of a spinning flywheel, as these points experience the highest levels of acceleration.
The formula to calculate centripetal acceleration is \( a_c = \omega^2 \times r \), where \( \omega \) is the angular velocity and \( r \) is the radius of the disk. For points on the rim, it illustrates the impact of rotational speed and radius on the acceleration experienced.
In practical terms, ensuring that \( a_c \) does not exceed material limits is crucial to avoid structural failure. High centripetal forces can lead to significant stress on the flywheel material, necessitating careful design to ensure these forces are manageable.

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Most popular questions from this chapter

You are designing a rotating metal flywheel that will be used to store energy. The flywheel is to be a uniform disk with radius 25.0 cm. Starting from rest at \(t =\) 0, the flywheel rotates with constant angular acceleration 3.00 rad/s\(^2\) about an axis perpendicular to the flywheel at its center. If the flywheel has a density (mass per unit volume) of 8600 kg/m\(^3\), what thickness must it have to store 800 J of kinetic energy at \(t =\) 8.00 s?

About what axis will a uniform, balsa-wood sphere have the same moment of inertia as does a thin-walled, hollow, lead sphere of the same mass and radius, with the axis along a diameter?

A frictionless pulley has the shape of a uniform solid disk of mass 2.50 kg and radius 20.0 cm. A 1.50-kg stone is attached to a very light wire that is wrapped around the rim of the pulley (\(\textbf{Fig. E9.43}\)), and the system is released from rest. (a) How far must the stone fall so that the pulley has 4.50 J of kinetic energy? (b) What percent of the total kinetic energy does the pulley have?

An advertisement claims that a centrifuge takes up only \(0.127 \mathrm{~m}\) of bench space but can produce a radial acceleration of \(3000 \mathrm{~g}\) at 5000 rev \(/ \mathrm{min}\). Calculate the required radius of the centrifuge. Is the claim realistic?

The Crab Nebula is a cloud of glowing gas about 10 lightyears across, located about 6500 light-years from the earth (\(\textbf{Fig. P9.86}\)). It is the remnant of a star that underwent a \(supernova\) \(explosion\), seen on earth in 1054 A.D. Energy is released by the Crab Nebula at a rate of about 5 \(\times\) 10\(^3$$^1\) W, about 10\(^5\) times the rate at which the sun radiates energy. The Crab Nebula obtains its energy from the rotational kinetic energy of a rapidly spinning \(neutron\) \(star\) at its center. This object rotates once every 0.0331 s, and this period is increasing by 4.22 \(\times 10^{-13}\) s for each second of time that elapses. (a) If the rate at which energy is lost by the neutron star is equal to the rate at which energy is released by the nebula, find the moment of inertia of the neutron star. (b) Theories of supernovae predict that the neutron star in the Crab Nebula has a mass about 1.4 times that of the sun. Modeling the neutron star as a solid uniform sphere, calculate its radius in kilometers. (c) What is the linear speed of a point on the equator of the neutron star? Compare to the speed of light. (d) Assume that the neutron star is uniform and calculate its density. Compare to the density of ordinary rock (3000 kg/m\(^3\)) and to the density of an atomic nucleus (about 10\(^{17}\) kg/m\(^3\)). Justify the statement that a neutron star is essentially a large atomic nucleus.

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