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Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 16 Physics, 4 th Edition James S. Walker

Chapter 16 - PowerPoint Presentation for College Physics

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Page 1: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

Lecture Outline

Chapter 16

Physics, 4th Edition

James S. Walker

Page 2: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

Chapter 16

Temperature and Heat

Page 3: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

Units of Chapter 16

• Temperature and the Zeroth Law of

Thermodynamics

• Temperature Scales

• Thermal Expansion

• Heat and Mechanical Work

• Specific Heats

• Conduction, Convection, and Radiation

Page 4: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-1 Temperature and the Zeroth Law of

Thermodynamics

Definition of heat:

Heat is the energy transferred between objects

because of a temperature difference.

Objects are in thermal contact if heat can flow

between them.

When the transfer of heat between objects in

thermal contact ceases, they are in thermal

equilibrium.

Page 5: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-1 Temperature and the Zeroth Law of

Thermodynamics

The zeroth law of thermodynamics:

If object A is in thermal equilibrium with object B,

and object C is also in thermal equilibrium with

object B, then objects A and C will be in thermal

equilibrium if brought into thermal contact.

That is, temperature is the only factor that

determines whether two objects in thermal

contact are in thermal equilibrium or not.

Page 6: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-1 Temperature and the Zeroth Law of

Thermodynamics

Page 7: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-2 Temperature Scales

The Celsius scale:

Water freezes at 0° Celsius.

Water boils at 100° Celsius.

The Fahrenheit scale:

Water freezes at 32° Fahrenheit .

Water boils at 212° Fahrenheit .

Page 8: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

Converting between Celsius and Fahrenheit:

16-2 Temperature Scales

Converting between Fahrenheit and Celsius :

Page 9: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-2 Temperature Scales

The pressure in a gas is proportional to its

temperature. The proportionality constant is

different for different gases, but they all reach

zero pressure at the same temperature, which

we call absolute zero:

Page 10: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-2 Temperature Scales

The Kelvin scale is similar to the Celsius scale,

except that the Kelvin scale has its zero at

absolute zero.

Conversion between a Celsius temperature and

a Kelvin temperature:

Page 11: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-2 Temperature Scales

The three temperature scales compared:

Page 12: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-3 Thermal Expansion

Most substances expand when heated; the

change in length or volume is typically

proportional to the change in temperature.

The proportionality constant is called the

coefficient of linear expansion.

Page 13: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-3 Thermal Expansion

Some typical coefficients of thermal expansion:

Page 14: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-3 Thermal Expansion

A bimetallic strip consists of two metals of

different coefficients of thermal expansion, A

and B in the figure. It will bend when heated or

cooled.

Page 15: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-3 Thermal Expansion

The expansion of an area of a flat substance is

derived from the linear expansion in both

directions:

Holes expand as well:

Page 16: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-3 Thermal Expansion

The change in volume of a solid is also derived

from the linear expansion:

For liquids and gases, only the coefficient of

volume expansion is defined:

Page 17: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-3 Thermal Expansion

Some typical coefficients of volume expansion:

Page 18: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-3 Thermal Expansion

Water also expands when it is

heated, except when it is close

to freezing; it actually expands

when cooling from 4° C to 0° C.

This is why ice floats and

frozen bottles burst.

Page 19: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-4 Heat and Mechanical Work

Experimental work has shown that heat is

another form of energy.

James Joule used a

device similar to this

one to measure the

mechanical equivalent

of heat:

Page 20: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-4 Heat and Mechanical Work

One kilocalorie (kcal) is defined as the amount

of heat needed to raise the temperature of 1 kg

of water from 14.5° C to 15.5° C.

Through experiments such as Joule’s, it was

possible to find the mechanical equivalent:

Page 21: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-4 Heat and Mechanical Work

Another unit of heat is the British thermal unit

(Btu). This is the energy required to heat 1 lb of

water from 63° F to 64° F.

Page 22: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-5 Specific Heats

The heat capacity of an object is the amount of

heat added to it divided by its rise in

temperature:

Q is positive if ΔT is positive; that is, if heat is

added to a system.

Q is negative if ΔT is negative; that is, if heat is

removed from a system.

Page 23: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-5 Specific Heats

The heat capacity of an object depends on its

mass. A quantity which is a property only of the

material is the specific heat:

Page 24: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-5 Specific Heats

Here are some

specific heats of

various materials:

Page 25: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-5 Specific Heats

A calorimeter is a lightweight, insulated flask

containing water. When an object is put in, it

and the water come to thermal equilibrium. If

the mass of the flask can be ignored, and the

insulation keeps any heat from escaping:

1.The final temperatures of the object and the

water will be equal.

2. The total energy of the system is conserved.

This allows us to calculate the specific heat of

the object.

Page 26: Chapter 16 - PowerPoint Presentation for College Physics

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16-6 Conduction, Convection, and Radiation

Conduction, convection, and radiation are

three ways that heat can be exchanged.

Conduction is the flow of heat directly through

a physical material.

Page 27: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-6 Conduction, Convection, and Radiation

Experimentally, it is found that the amount of

heat Q that flows through a rod:

• increases proportionally to the cross-

sectional area A

• increases proportionally to the temperature

difference from one end to the other

• increases steadily with time

• decreases with the length of the rod

Page 28: Chapter 16 - PowerPoint Presentation for College Physics

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16-6 Conduction, Convection, and Radiation

Combining, we find:

The constant k is called the thermal

conductivity of the rod.

Page 29: Chapter 16 - PowerPoint Presentation for College Physics

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16-6 Conduction, Convection, and Radiation

Some typical thermal

conductivities:

Substances with high

thermal conductivities

are good conductors of

heat; those with low

thermal conductivities

are good insulators.

Page 30: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-6 Conduction, Convection, and Radiation

Convection is the flow of

fluid due to a difference

in temperatures, such as

warm air rising. The fluid

“carries” the heat with it

as it moves.

Page 31: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-6 Conduction, Convection, and Radiation

All objects give off energy in the form of

radiation, as electromagnetic waves – infrared,

visible light, ultraviolet – which, unlike

conduction and convection, can transport heat

through a vacuum.

Objects that are hot enough will glow – first

red, then yellow, white, and blue. Objects at

body temperature radiate in the infrared, and

can be seen with night vision binoculars.

Page 32: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

16-6 Conduction, Convection, and Radiation

The amount of energy radiated by an object due

to its temperature is proportional to its surface

area and also to the fourth (!) power of its

temperature.

It also depends on the emissivity, which is a

number between 0 and 1 that indicates how

effective a radiator the object is; a perfect

radiator would have an emissivity of 1.

Page 33: Chapter 16 - PowerPoint Presentation for College Physics

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16-6 Conduction, Convection, and Radiation

This behavior is contained in the Stefan-

Boltzmann law:

Here, e is the emissivity, and σ is the Stefan-

Boltzmann constant:

Page 34: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

Summary of Chapter 16

• Heat is the energy transferred between objects

due to a temperature difference.

• Objects are in thermal contact if heat can flow

between them.

• Objects that are in thermal contact without any

flow of heat are in thermal equilibrium.

• Thermodynamics is the study of physical

processes that involve heat.

• If objects A and B are both in thermal

equilibrium with C, they are in thermal

equilibrium with each other.

Page 35: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

Summary of Chapter 16

• Temperature determines whether two

objects will be in thermal equilibrium.

• Celsius scale: water freezes at 0° C, boils at

100° C

• Fahrenheit: water freezes at 32° F, boils at

212° F

• The lowest attainable temperature is

absolute zero.

• Kelvin: absolute zero is 0 K; water freezes at

273.15 K and boils at 373.15 K

Page 36: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

Summary of Chapter 16

• Temperature scale conversions:

• Most substances expand when heated.

• Linear expansion:

• Volume expansion:

• Water contracts when heated from 0° C to

4° C.

Page 37: Chapter 16 - PowerPoint Presentation for College Physics

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Summary of Chapter 16

• Heat is a form of energy:

• Heat capacity of an object:

• Specific heat is heat capacity per unit mass:

• Energy is conserved in heat flow.

Page 38: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

Summary of Chapter 16

• Conduction: heat exchange from one part of a

material to a cooler part, with no bulk motion of

the material.

• Heat exchanged in time t:

• Convection is heat exchange due to the bulk

motion of an unevenly heated fluid.

• Radiation is heat exchange due to

electromagnetic radiation.

Page 39: Chapter 16 - PowerPoint Presentation for College Physics

Copyright © 2010 Pearson Education, Inc.

Summary of Chapter 16

• Radiated power as a function of temperature:

• Stefan-Boltzmann constant: