Physics for scientists and engineers 8th edition solutions manual

(Chapters 1-22)


Student Solutions Manual
and Study Guide
for
S ERWAY

AND

J EWETT ’ S

P H YS I C S
FOR

S CIENTISTS

AND

E NGINEERS

V OLUME O NE
E IGHTH E DITION
Full solutions to text-boxed numbered problems in Chapters 1-22 of textbook.

John R. Gordon
Emeritus, James Madison University

Ralph V. McGrew
Broome Community College

Raymond A. Serway
Emeritus, James Madison University

Australia • Brazil • Canada • Mexico • Singapore • Spain • United Kingdom • United States

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PREFACE
This Student Solutions Manual and Study Guide has been written to accompany the
textbook Physics for Scientists and Engineers, Eighth Edition, by Raymond A. Serway

and John W. Jewett, Jr. The purpose of this Student Solutions Manual and Study Guide is
to provide students with a convenient review of the basic concepts and applications presented in the textbook, together with solutions to selected end-of-chapter problems from
the textbook. This is not an attempt to rewrite the textbook in a condensed fashion. Rather,
emphasis is placed upon clarifying typical troublesome points and providing further practice in methods of problem solving.
Every textbook chapter has in this book a matching chapter, which is divided into
several parts. Very often, reference is made to specific equations or figures in the textbook.
Each feature of this Study Guide has been included to ensure that it serves as a useful supplement to the textbook. Most chapters contain the following components:

•

Equations and Concepts: This represents a review of the chapter, with emphasis
on highlighting important concepts, and describing important equations and formalisms.

•

Suggestions, Skills, and Strategies: This offers hints and strategies for solving typical problems that the student will often encounter in the course. In some sections, suggestions are made concerning mathematical skills that are necessary in the analysis of
problems.

•

Review Checklist: This is a list of topics and techniques the student should master
after reading the chapter and working the assigned problems.

•

Answers to Selected Questions: Suggested answers are provided for approximately
15 percent of the objective and conceptual questions.

•

Solutions to Selected End-of-Chapter Problems: Solutions are shown for approximately 20 percent of the problems from the text, chosen to illustrate the important
concepts of the chapter. The solutions follow the Conceptualize—Categorize—Analyze—Finalize strategy presented in the text.

A note concerning significant figures: When the statement of a problem gives data to
three significant figures, we state the answer to three significant figures. The last digit is
uncertain; it can for example depend on the precision of the values assumed for physical
constants and properties. When a calculation involves several steps, we carry out intermediate steps to many digits, but we write down only three. We “round off” only at the end of
any chain of calculations, never anywhere in the middle.
We sincerely hope that this Student Solutions Manual and Study Guide will be useful
to you in reviewing the material presented in the text and in improving your ability to solve

iii

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iv

Preface

problems and score well on exams. We welcome any comments or suggestions which could
help improve the content of this study guide in future editions, and we wish you success in
your study.
John R. Gordon
Harrisonburg, Virginia
Ralph V. McGrew

Binghamton, New York
Raymond A. Serway
Leesburg, Virginia

Acknowledgments
We are glad to acknowledge that John Jewett and Hal Falk suggested significant
improvements in this manual. We are grateful to Charu Khanna and the staff at MPS Limited
for assembling and typing this manual and preparing diagrams and page layouts. Susan
English of Durham Technical Community College checked the manual for accuracy and suggested many improvements. We thank Brandi Kirksey (Associate Developmental Editor),
Mary Finch (Publisher), and Cathy Brooks (Senior Content Project Manager) of Cengage
Learning, who coordinated this project and provided resources for it. Finally, we express our
appreciation to our families for their inspiration, patience, and encouragement.

Copyright 2010 Cengage Learning, Inc. All Rights Reserved. May not be copied, scanned, or duplicated, in whole or in part.

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Preface

v

Suggestions for Study
We have seen a lot of successful physics students. The question, “How should I study
this subject?” has no single answer, but we offer some suggestions that may be useful to you.
1.

Work to understand the basic concepts and principles before attempting to solve

assigned problems. Carefully read the textbook before attending your lecture on that
material. Jot down points that are not clear to you, take careful notes in class, and ask
questions. Reduce memorization of material to a minimum. Memorizing sections of a
text or derivations would not necessarily mean you understand the material.

2.

After reading a chapter, you should be able to define any new quantities that were
introduced and discuss the first principles that were used to derive fundamental equations. A review is provided in each chapter of the Study Guide for this purpose, and
the marginal notes in the textbook (or the index) will help you locate these topics.
You should be able to correctly associate with each physical quantity the symbol used
to represent that quantity (including vector notation if appropriate) and the SI unit
in which the quantity is specified. Furthermore, you should be able to express each
important formula or equation in a concise and accurate prose statement.

3.

Try to solve plenty of the problems at the end of the chapter. The worked examples
in the text will serve as a basis for your study. This Study Guide contains detailed
solutions to about fifteen of the problems at the end of each chapter. You will be able
to check the accuracy of your calculations for any odd-numbered problems, since the
answers to these are given at the back of the text.

4.

Besides what you might expect to learn about physics concepts, a very valuable skill
you can take away from your physics course is the ability to solve complicated problems. The way physicists approach complex situations and break them down into
manageable pieces is widely useful. At the end of Chapter 2, the textbook develops
a general problem-solving strategy that guides you through the steps. To help you
remember the steps of the strategy, they are called Conceptualize, Categorize, Analyze, and Finalize.

General Problem-Solving Strategy
Conceptualize
•
The first thing to do when approaching a problem is to think about and understand
the situation. Read the problem several times until you are confident you understand
what is being asked. Study carefully any diagrams, graphs, tables, or photographs that
accompany the problem. Imagine a movie, running in your mind, of what happens in
the problem.
•

If a diagram is not provided, you should almost always make a quick drawing of the
situation. Indicate any known values, perhaps in a table or directly on your sketch.

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vi

Preface

•

Now focus on what algebraic or numerical information is given in the problem. In
the problem statement, look for key phrases such as “starts from rest” (vi = 0), “stops”
(vf = 0), or “falls freely” (ay = –g = –9.80 m/s2). Key words can help simplify the

problem.

•

Next, focus on the expected result of solving the problem. Precisely what is the question asking? Will the final result be numerical or algebraic? If it is numerical, what
units will it have? If it is algebraic, what symbols will appear in the expression?

•

Incorporate information from your own experiences and common sense. What should
a reasonable answer look like? What should its order of magnitude be? You wouldn’t
expect to calculate the speed of an automobile to be 5 × 106 m/s.

Categorize
•
After you have a really good idea of what the problem is about, you need to simplify the
problem. Remove the details that are not important to the solution. For example, you
can often model a moving object as a particle. Key words should tell you whether
you can ignore air resistance or friction between a sliding object and a surface.
•

Once the problem is simplified, it is important to categorize the problem. How does it
fit into a framework of ideas that you construct to understand the world? Is it a simple
plug-in problem, such that numbers can be simply substituted into a definition? If so,
the problem is likely to be finished when this substitution is done. If not, you face
what we can call an analysis problem—the situation must be analyzed more deeply to
reach a solution.

•

If it is an analysis problem, it needs to be categorized further. Have you seen this type
of problem before? Does it fall into the growing list of types of problems that you
have solved previously? Being able to classify a problem can make it much easier to
lay out a plan to solve it. For example, if your simplification shows that the problem
can be treated as a particle moving under constant acceleration and you have already
solved such a problem (such as the examples in Section 2.6), the solution to the new
problem follows a similar pattern. From the textbook you can make an explicit list of
the analysis models.

Analyze
•
Now, you need to analyze the problem and strive for a mathematical solution. Because
you have categorized the problem and identified an analysis model, you can select
relevant equations that apply to the situation in the problem. For example, if your categorization shows that the problem involves a particle moving under constant acceleration, Equations 2.13 to 2.17 are relevant.
•

Use algebra (and calculus, if necessary) to solve symbolically for the unknown variable
in terms of what is given. Substitute in the appropriate numbers, calculate the result,
and round it to the proper number of significant figures.

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Preface

vii

Finalize
•
This final step is the most important part. Examine your numerical answer. Does it
have the correct units? Does it meet your expectations from your conceptualization
of the problem? What about the algebraic form of the result—before you substituted
numerical values? Does it make sense? Try looking at the variables in it to see whether
the answer would change in a physically meaningful way if they were drastically
increased or decreased or even became zero. Looking at limiting cases to see whether
they yield expected values is a very useful way to make sure that you are obtaining
reasonable results.
•

Think about how this problem compares with others you have done. How was it
similar? In what critical ways did it differ? Why was this problem assigned? You
should have learned something by doing it. Can you figure out what? Can you use
your solution to expand, strengthen, or otherwise improve your framework of ideas?
If it is a new category of problem, be sure you understand it so that you can use it as
a model for solving future problems in the same category.

When solving complex problems, you may need to identify a series of subproblems
and apply the problem-solving strategy to each. For very simple problems, you probably
don’t need this whole strategy. But when you are looking at a problem and you don’t know
what to do next, remember the steps in the strategy and use them as a guide.
Work on problems in this Study Guide yourself and compare your solutions to ours.
Your solution does not have to look just like the one presented here. A problem can sometimes be solved in different ways, starting from different principles. If you wonder about
the validity of an alternative approach, ask your instructor.
5.

We suggest that you use this Study Guide to review the material covered in the text

and as a guide in preparing for exams. You can use the sections Review Checklist,
Equations and Concepts, and Suggestions, Skills, and Strategies to focus in on points
that require further study. The main purpose of this Study Guide is to improve the efficiency and effectiveness of your study hours and your overall understanding of physical concepts. However, it should not be regarded as a substitute for your textbook or
for individual study and practice in problem solving.

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TABLE OF CONTENTS
Chapter

Title

Page

1

Physics and Measurement

1

2

Motion in One Dimension

12

3

Vectors

30

4

Motion in Two Dimensions

46

5

The Laws of Motion

68

6

Circular Motion and Other Applications of Newton’s Laws

88

7

Energy of a System

105

8

Conservation of Energy

122

9

Linear Momentum and Collisions

145

10

Rotation of a Rigid Object About a Fixed Axis

166

11

Angular Momentum

193

12

Static Equilibrium and Elasticity

210

13

Universal Gravitation

229

14

Fluid Mechanics

246

15

Oscillatory Motion

261

16

Wave Motion

284

17

Sound Waves

299

18

Superposition and Standing Waves

316

19

Temperature

336

20

The First Law of Thermodynamics

353

21

The Kinetic Theory of Gases

372

22

Heat Engines, Entropy, and the Second Law of Thermodynamics

390

viii

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1
Physics and Measurement
EQUATIONS AND CONCEPTS
The density of any substance is defined as
the ratio of mass to volume. The SI units of
density are kg/m3. Density is an example of
a derived quantity.

r

≡

m
V

(1.1)

SUGGESTIONS, SKILLS, AND STRATEGIES
A general strategy for problem solving will be described in Chapter 2.
Appendix B of your textbook includes a review of mathematical techniques including:

•

Scientific notation: using powers of ten to express large and small numerical values.

•

Basic algebraic operations: factoring, handling fractions, and solving quadratic equations.

•

Fundamentals of plane and solid geometry: graphing functions, calculating areas and volumes, and recognizing equations and graphs of standard figures (e.g. straight line, circle,
ellipse, parabola, and hyperbola).

•

Basic trigonometry: definition and properties of functions (e.g. sine, cosine, and tangent),
the Pythagorean Theorem, and basic trigonometry identities.

REVIEW CHECKLIST
You should be able to:

•

Describe the standards which define the SI units for the fundamental quantities length
(meter, m), mass (kilogram, kg), and time (second, s). Identify and properly use prefixes
and mathematical notations such as the following: ∝ (is proportional to), < (is less than),
≈ (is approximately equal to), Δ (change in value), etc. (Section 1.1)

•

Convert units from one measurement system to another (or convert units within a system).
Perform a dimensional analysis of an equation containing physical quantities whose individual units are known. (Sections 1.3 and 1.4)

•

Carry out order-of-magnitude calculations or estimates. (Section 1.5)

•

Express calculated values with the correct number of significant figures. (Section 1.6)
1

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2

Chapter 1

ANSWER TO AN OBJECTIVE QUESTION
3. Answer each question yes or no. Must two quantities have the same dimensions (a) if
you are adding them? (b) If you are multiplying them? (c) If you are subtracting them?
(d) If you are dividing them? (e) If you are equating them?

Answer. (a) Yes. Three apples plus two jokes has no definable answer. (b) No. One acre
times one foot is one acre-foot, a quantity of floodwater. (c) Yes. Three dollars minus six
seconds has no definable answer. (d) No. The gauge of a rich sausage can be 12 kg divided
by 4 m, giving 3 kg/m. (e) Yes, as in the examples given for parts (b) and (d). Thus we have
(a) yes (b) no (c) yes (d) no (e) yes

ANSWER TO A CONCEPTUAL QUESTION
1. Suppose the three fundamental standards of the metric system were length, density,
and time rather than length, mass, and time. The standard of density in this system is to
be defined as that of water. What considerations about water would you need to address to
make sure the standard of density is as accurate as possible?
Answer. There are the environmental details related to the water: a standard temperature would have to be defined, as well as a standard pressure. Another consideration is
the quality of the water, in terms of defining an upper limit of impurities. A difficulty with
this scheme is that density cannot be measured directly with a single measurement, as can
length, mass, and time. As a combination of two measurements (mass and volume, which
itself involves three measurements!), a density value has higher uncertainty than a single
measurement.

SOLUTIONS TO SELECTED END-OF-CHAPTER PROBLEMS
9.

Which of the following equations are dimensionally correct?
(a) vf = vi + ax

(b) y = (2 m)cos(kx)

where

k = 2 m–1

Solution
Conceptualize: It is good to check an unfamiliar equation for dimensional correctness to
see whether it can possibly be true.
Categorize: We evaluate the dimensions as a combination of length, time, and mass for
each term in each equation.
Analyze:
(a) Write out dimensions for each quantity in the equation
The variables vf and vi are expressed in unts of mրs, so

vf = vi + ax
[vf] = [vi] = LT–1

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Physics and Measurement

The variable a is expressed in units of mրs2 and

[a] = LT–2

The variable x is expressed in meters. Therefore

[ax] = L2T–2

Consider the right-hand member (RHM) of equation (a):

[RHM] = LT–1 + L2T–2

Quantities to be added must have the same dimensions.
Therefore, equation (a) is not dimensionally correct.
(b) Write out dimensions for each quantity in the equation

3

■

y = (2 m) cos (kx)
[y] = L

For y,

[2 m] = L
[kx ] = ⎡⎣ 2 m –1 x ⎤⎦ = L–1L
and for (kx),
Therefore we can think of the quantity kx as an angle in radians, and we can take
its cosine. The cosine itself will be a pure number with no dimensions. For the
left-hand member (LHM) and the right-hand member (RHM) of the equation
we have
for 2 m,

(

[LHM] = [ y] = L

)

[RHM] = [2 m][cos (kx)] = L

These are the same, so equation (b) is dimensionally correct.

■

Finalize: We will meet an expression like y = (2 m)cos(kx), where k = 2 m–1, as the wave
function of a wave.

13. A rectangular building lot has a width of 75.0 ft and a length of 125 ft. Determine the
area of this lot in square meters.
Solution
Conceptualize: We must calculate the area and convert units. Since a meter is about
3 feet, we should expect the area to be about A ≈ (25 m)(40 m) = 1 000 m2.
Categorize: We will use the geometrical fact that for a rectangle Area = Length × Width;
and the conversion 1 m = 3.281 ft.
Analyze:

⎛ 1m ⎞
⎛ 1m ⎞
A = ᐉ × w = (75.0 ft) ⎜
(125 ft) ⎜
= 871 m 2
⎟
⎝ 3.281 ft ⎠
⎝ 3.281 ft ⎟⎠

■

Finalize: Our calculated result agrees reasonably well with our initial estimate and has
the proper units of m2. Unit conversion is a common technique that is applied to many
problems. Note that one square meter is more than ten square feet.

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4

Chapter 1

15. A solid piece of lead has a mass of 23.94 g and a volume of 2.10 cm3. From these data,
calculate the density of lead in SI units (kilograms per cubic meter).
Solution
Conceptualize: From Table 14.1, the density of lead is 1.13 × 104 kgրm3, so we should
expect our calculated value to be close to this value. The density of water is 1.00 × 103 kg/m3,
so we see that lead is about 11 times denser than water, which agrees with our experience
that lead sinks.
Categorize: Density is defined as ρ = m / V . We must convert to SI units in the calculation.
Analyze:

⎛ 23.94 g ⎞ ⎛ 1 kg ⎞ ⎛ 100 cm ⎞ 3

ρ = ⎜
⎝ 2.10 cm 3 ⎟⎠ ⎜⎝ 1 000 g ⎟⎠ ⎝ 1 m ⎠
⎛ 23.94 g ⎞ ⎛ 1 kg ⎞ ⎛ 1 000 000 cm 3 ⎞
4
3
= ⎜
⎜
⎟⎠ = 1.14 × 10 kg/m
⎝ 2.10 cm 3 ⎟⎠ ⎜⎝ 1 000 g ⎟⎠ ⎝
1 m3

■

Finalize: Observe how we set up the unit conversion fractions to divide out the units
of grams and cubic centimeters, and to make the answer come out in kilograms per cubic
meter. At one step in the calculation, we note that one million cubic centimeters make
one cubic meter. Our result is indeed close to the expected value. Since the last reported
significant digit is not certain, the difference from the tabulated values is possibly due to
measurement uncertainty and does not indicate a discrepancy.

21. One cubic meter (1.00 m3) of aluminum has a mass of 2.70 × 103 kg, and the same
volume of iron has a mass of 7.86 × 103 kg. Find the radius of a solid aluminum sphere that
will balance a solid iron sphere of radius 2.00 cm on an equal-arm balance.
Solution
Conceptualize: The aluminum sphere must be larger in volume to compensate for its
lower density. Its density is roughly one-third as large, so we might guess that the radius is
three times larger, or 6 cm.
Categorize: We require equal masses:
Analyze:

mAl = mFe

or

ρAlVAl = ρFeVFe

We use also the volume of a sphere. By substitution,

ρAl ⎛ 4 π rA13 ⎞ = ρFe ⎛ 4 π (2.00 cm)3 ⎞
⎝3
⎠
⎝3
⎠
Now solving for the unknown,
⎛ 7.86 × 10 3 kg/m 3 ⎞
⎛ρ ⎞
(2.00 cm )3 = 23.3 cm 3
rAl 3 = ⎜ Fe ⎟ (2.00 cm )3 = ⎜
3
3⎟
ρ
⎝ Al ⎠
⎝ 2..70 × 10 kg/m ⎠
Taking the cube root, rAl = 2.86 cm

■

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Physics and Measurement

5

Finalize: The aluminum sphere is only 43% larger than the iron one in radius, diameter,
and circumference. Volume is proportional to the cube of the linear dimension, so this
moderate excess in linear size gives it the (1.43)(1.43)(1.43) = 2.92 times larger volume it
needs for equal mass.

23. One gallon of paint (volume = 3.78 × 10–3 m3) covers an area of 25.0 m2. What is the
thickness of the fresh paint on the wall?
Solution
Conceptualize: We assume the paint keeps the same volume in the can and on the wall.
Categorize: We model the film on the wall as a rectangular solid, with its volume given by
its “footprint” area, which is the area of the wall, multiplied by its thickness t perpendicular to
this area and assumed to be uniform.
Analyze: V = At

gives

–3
3
t = V = 3.78 × 10 2 m = 1.51 × 10 –4 m
A

25.0 m

■

Finalize: The thickness of 1.5 tenths of a millimeter is comparable to the thickness of a
sheet of paper, so it is reasonable. The film is many molecules thick.

25. (a) At the time of this book’s printing, the U.S. national debt is about $10 trillion.
If payments were made at the rate of $1 000 per second, how many years would it take
to pay off the debt, assuming no interest were charged? (b) A dollar bill is about 15.5 cm
long. How many dollar bills, attached end to end, would it take to reach the Moon? The
front endpapers give the Earth-Moon distance. Note: Before doing these calculations, try
to guess at the answers. You may be very surprised.
Solution
(a) Conceptualize: $10 trillion is certainly a large amount of money, so even at a rate of
$1 000րsecond, we might guess that it will take a lifetime (∼100 years) to pay off the debt.
Categorize: The time interval required to repay the debt will be calculated by dividing the total debt by the rate at which it is repaid.
Analyze:

T =

$10 trillion
$10 × 1012
=
= 317 yr
$1000 / s
($1000 / s) ( 3.156 × 10 7 s/yr )

■

Finalize: Our guess was a bit low. $10 trillion really is a lot of money!
(b) Conceptualize: We might guess that 10 trillion bills would reach from the Earth to
the Moon, and perhaps back again, since our first estimate was low.

© 2010 Cengage Learning. All Rights Reserved. May not be scanned, copied or duplicated, or posted to a publicly accessible website, in whole or in part.

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6

Chapter 1

Categorize: The number of bills is the distance to the Moon divided by the length
of a dollar.
Analyze:

N=

D 3.84 × 108 m
=
= 2.48 × 10 9 bills
ᐉ
0.155 m

■

Finalize: Ten trillion dollars is larger than this twoand-a-half billion dollars by four thousand times. The
ribbon of bills comprising the debt reaches across the
cosmic gulf thousands of times, so again our guess was
low. Similar calculations show that the bills could span
the distance between the Earth and the Sun ten times.
The strip could encircle the Earth’s equator nearly
40 000 times. With successive turns wound edge to edge without overlapping, the
dollars would cover a zone centered on the equator and about 2.6 km wide.

27. Find the order of magnitude of the number of table-tennis balls that would fit into a
typical-size room (without being crushed). [In your solution, state the quantities you measure or estimate and the values you take for them.]
Solution
Conceptualize: Since the volume of a typical room is much larger than a Ping-Pong ball,
we should expect that a very large number of balls (maybe a million) could fit in a room.
Categorize: Since we are only asked to find an estimate, we do not need to be too concerned about how the balls are arranged. Therefore, to find the number of balls we can
simply divide the volume of an average-size living room (perhaps 15 ft × 20 ft × 8 ft) by
the volume of an individual Ping-Pong ball.
Analyze:

Using the approximate conversion 1 ft = 30 cm, we find
VRoom = (15 ft)(20 ft)(8 ft)(30 cmրft)3 ≈ 6 × 107 cm3

A Ping-Pong ball has a diameter of about 3 cm, so we can estimate its volume as a cube:
Vball = (3 cm)(3 cm)(3 cm) ≈ 30 cm3
The number of Ping-Pong balls that can fill the room is
N≈

VRoom
≈ 2 × 10 6 balls ∼ 10 6 balls

Vball

■

Finalize: So a typical room can hold on the order of a million Ping-Pong balls. This
problem gives us a sense of how large a quantity “a million” really is.

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Physics and Measurement

7

29. To an order of magnitude, how many piano tuners reside in New York City? The
physicist Enrico Fermi was famous for asking questions like this one on oral Ph.D. qualifying
examinations.
Solution
Conceptualize:
Categorize:

Don’t reach for the telephone book! Think.

Each full-time piano tuner must keep busy enough to earn a living.

Analyze: Assume a total population of 107 people. Also, let us estimate that one person
in one hundred owns a piano. Assume that in one year a single piano tuner can service
about 1 000 pianos (about 4 per day for 250 weekdays), and that each piano is tuned once
per year.
Therefore, the number of tuners
⎛ 1 tuner ⎞ ⎛ 1 piano ⎞ 7
=⎜
10 people ∼ 100 tuners
⎝ 1 000 pianos ⎟⎠ ⎜⎝ 100 people ⎟⎠

(

)

■

Finalize: If you did reach for an Internet directory, you would have to count. Instead,
have faith in your estimate. Fermi’s own ability in making an order-of-magnitude estimate
is exemplified by his measurement of the energy output of the first nuclear bomb (the Trinity test at Alamogordo, New Mexico) by observing the fall of bits of paper as the blast wave
swept past his station, 14 km away from ground zero.

43. Review. A pet lamb grows rapidly, with its mass proportional to the cube of its length.
When the lamb’s length changes by 15.8%, its mass increases by 17.3 kg. Find the lamb’s
mass at the end of this process.
Solution
Conceptualize: The little sheep’s final mass must be a lot more than 17 kg, so an order
of magnitude estimate is 100 kg.
Categorize: When the length changes by 15.8%, the mass changes by a much larger
percentage. We will write each of the sentences in the problem as a mathematical equation.

Analyze: Mass is proportional to length cubed: m = kᐉ3 where k is a constant. This model
of growth is reasonable because the lamb gets thicker as it gets longer, growing in threedimensional space.
mi = kᐉi3

At the initial and final points,
Length changes by 15.8%:
Thus

ᐉi + 0.158 ᐉi = ᐉf

Mass increases by 17.3 kg:

and

mf = kᐉf3

Long ago you were told that 15.8% of ᐉ means
0.158 times ᐉ.
and

ᐉf = 1.158 ᐉi

mi + 17.3 kg = mf

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8

Chapter 1

Now we combine the equations using algebra, eliminating the unknowns ᐉi, ᐉf , k, and mi
by substitution:
From

ᐉf = 1.158 ᐉi,

Then

mf = kᐉf3 = k(1.553) ᐉi3 = 1.553 kᐉi3 = 1.553 mi

Next,

mi + 17.3 kg = mf

Solving,

17.3 kg = mf – mf ր1.553 = mf (1 – 1ր1.553) = 0.356 mf
and

we have

ᐉf3 = 1.1583 ᐉi3 = 1.553 ᐉi3

becomes

and

mi = mf ր1.553

mf ր1.553 + 17.3 kg = mf

mf = 17.3 kgր0.356 = 48.6 kg

■

Finalize: Our 100-kg estimate was of the right order of magnitude. The 15.8% increase
in length produces a 55.3% increase in mass, which is an increase by a factor of 1.553. The
writer of this problem was thinking of the experience of a young girl in the Oneida community of New York State. Before the dawn of a spring day she helped with the birth of lambs.
She was allowed to choose one lamb as her pet, and braided for it a necklace of straw to
distinguish it from the others. Then she went into the house, where her mother had made
cocoa with breakfast. Many years later she told this story of widening, overlapping circles
of trust and faithfulness, to a group of people working to visualize peace. Over many more
years the story is spreading farther.

51. The diameter of our disk-shaped galaxy, the Milky Way, is about 1.0 × 105 light-years (ly).
The distance to the Andromeda galaxy (Fig. P1.51 in the text), which is the spiral galaxy
nearest to the Milky Way, is about 2.0 million ly. If a scale model represents the Milky
Way and Andromeda galaxies as dinner plates 25 cm in diameter, determine the distance
between the centers of the two plates.
Solution
Conceptualize: Individual stars are fantastically small compared to the distance between
them, but galaxies in a cluster are pretty close compared to their sizes.
Categorize: We can say that we solve the problem “by proportion” or by finding and

using a scale factor, as if it were a unit conversion factor, between real space and its
model.
Analyze: The scale used in the “dinner plate” model is
S=

1.0 × 10 5 light-years
ly
= 4.00 × 10 3
25 cm
cm

The distance to Andromeda in the dinner plate model will be
D=

2.00 × 10 6 ly
= 5.00 × 10 2 cm = 5.00
3
4.00 × 10 ly/cm

■

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Physics and Measurement

9

Finalize: Standing at one dinner plate, you can cover your view of the other plate with
three fingers held at arm’s length. The Andromeda galaxy, called Messier 31, fills this same
angle in the field of view that the human race has and will always have.

53. A high fountain of water is located at the center of a circular pool as shown in Figure
P1.53. A student walks around the pool and measures its circumference to be 15.0 m. Next,
the student stands at the edge of the pool and uses a protractor to gauge the angle of elevation of the top of the fountain to be f = 55.0°. How high is the fountain?
Solution
Conceptualize: Geometry was invented to
make indirect distance measurements, such as
this one.
Categorize: We imagine a top view to figure
the radius of the pool from its circumference.
We imagine a straight-on side view to use trigonometry to find the height.
Analyze: Define a right triangle whose legs
represent the height and radius of the fountain.
From the dimensions of the fountain and the
triangle, the circumference is C = 2πr and the
angle satisfies tan φ = hրr .
Then by substitution
h = r tan φ =

( 2Cπ ) tan φ
Figure P1.53

Evaluating,

h=

15.0 m
tan 55.0 ο = 3.41 m
2π

■

Finalize: When we look at a three-dimensional system from a particular direction, we
may discover a view to which simple mathematics applies.

57. Assume there are 100 million passenger cars in the United States and the average
fuel consumption is 20 mi/gal of gasoline. If the average distance traveled by each car is
10 000 mi/yr, how much gasoline would be saved per year if average fuel consumption
could be increased to 25 mi/gal?

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10

Chapter 1

Solution

Conceptualize: Five miles per gallon is not much for one car, but a big country can save
a lot of gasoline.
Categorize: We define an average national fuel consumption rate based upon the total
miles driven by all cars combined.
Analyze:

In symbols,
fuel consumed =

total miles driven
average fuel consumption rate

or
f = s
c
For the current rate of 20 miրgallon we have

(100 × 10 cars)(10 (mi/yr)/car ) = 5 × 10
f =
6

4

10

20 mi/gal

gal/yr

Since we consider the same total number of miles driven in each case, at 25 miրgal we have

(100 × 10 cars)(10 (mi/yr)/car ) = 4 × 10
f =
6

4

10

25 mi/gal

Thus we estimate a change in fuel consumption of

gal/yr

Δ f = –1 × 1010 gal/yr

■

The negative sign indicates that the change is a reduction. It is a fuel savings of ten billion
gallons each year.
Finalize:

Let’s do it!

63. The consumption of natural gas by a company satisfies the empirical equation V = 1.50t +
0.008 00t2, where V is the volume of gas in millions of cubic feet and t is the time in months.
Express this equation in units of cubic feet and seconds. Assume a month is 30.0 days.
Solution
Conceptualize: The units of volume and time imply particular combination-units for the

coefficients in the equation.
Categorize: We write “millions of cubic feet” as 106 ft3, and use the given units of time
and volume to assign units to the equation:
Analyze:

(

) (

)

V = 1.50 × 10 6 ft 3 /mo t + 0.008 00 × 10 6 ft 3 /mo2 t 2

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Physics and Measurement

11

To convert the units to seconds, use
24 h ⎞ ⎛ 3600
1 month = 30.0 d ⎛⎜
⎝ 1 d ⎟⎠ ⎜⎝ 1 h

s⎞
6
⎟⎠ = 2.59 × 10 s, to obtain
2

3
⎛
⎛
⎞ 2
⎞
ft 3 ⎞ ⎛
1 mo
1 mo
6 ft ⎞ ⎛
t
+
×
V = ⎜ 1.50 × 10 6
10
t
0.008
00
⎜
2⎟⎜
6 ⎟
6 ⎟
⎜
⎟
mo ⎠ ⎝ 2.59 × 10 s ⎠

⎝
⎝
mo ⎠ ⎝ 2.59 × 10 s ⎠

(

) (

)

V = 0.579 ft 3 / s t + 1.19 × 10 –9 ft 3 /s 2 t 2
or
V = 0.579t + 1.19 × 10 −9 t 2 , where V is in cubic feeet and t is in seconds

■

Finalize: The coefficient of the first term is the volume rate of flow of gas at the beginning of the month. The second term’s coefficient is related to how much the rate of flow
increases every second.

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2
Motion in One Dimension

EQUATIONS AND CONCEPTS
The displacement Δ x of a particle moving from position xi to position xf equals the
f inal coordinate minus the initial coordinate. Displacement can be positive, negative or zero.

Δ x ≡ xf – xi

(2.1)

Δx
Δt

(2.2)

Distance traveled is the length of the path
followed by a particle and should not be
confused with displacement. When xf = xi ,
the displacement is zero; however, if the
particle leaves xi , travels along a path, and
returns to xi, the distance traveled will not
be zero.
The average velocity of an object during
a time interval Δ t is the ratio of the total
displacement Δ x to the time interval during which the displacement occurs.

v x , avg ≡

The average speed of a particle is a scalar quantity defined as the ratio of the total
distance d traveled to the time required
to travel that distance. Average speed has
no direction and carries no algebraic sign.

The magnitude of the average velocity is
not the average speed; although in certain
cases they may be numerically equal.

vavg ≡

The instantaneous velocity v is defined as
the limit of the ratio Δ x րΔ t as Δt approaches
zero. This limit is called the derivative of x
with respect to t. The instantaneous velocity at any time is the slope of the positiontime graph at that time. As illustrated in the
figure, the slope can be positive, negative,
or zero.

vx ≡

d

Δt

lim Δ x dx
=
Δt
dt

Δt →0

(2.3)

(2.5)

12
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Motion in One Dimension

13

The instantaneous speed is the magnitude
of the instantaneous velocity.
The average acceleration of an object is
defined as the ratio of the change in velocity
to the time interval during which the change
in velocity occurs. Equation 2.9 gives the
average acceleration of a particle in onedimensional motion along the x axis.
The instantaneous acceleration a is defined as the limit of the ratio Δvx րΔ t as Δ t
approaches zero. This limit is the derivative of the velocity along the x direction
with respect to time. A negative acceleration does not necessarily imply a decreasing speed. Acceleration and velocity are
not always in the same direction.
The acceleration can also be expressed as the
second derivative of the position with respect
to time. This is shown in Equation 2.12 for
the case of a particle in one-dimensional
motion along the x axis.

ax , avg ≡

Δv x v x f – v xi
=
Δt
t f – ti

(2.9)

dv
lim Δv
ax ≡ Δt→0 x = x
Δt
dt

(2.10)

d 2x
dt 2

(2.12)

The kinematic equations, (2.13–2.17),
can be used to describe one-dimensional
motion along the x axis with constant acceleration. Note that each equation shows
a different relationship among physical
quantities: initial velocity, final velocity,
acceleration, time, and position.
Remember, the relationships stated in Equations 2.13–2.17 are true only for cases in

which the acceleration is constant.

v x f = v xi + ax t

(2.13)

A freely falling object is any object moving under the influence of the gravitational
force alone. Equations 2.13–2.17 can be
modified to describe the motion of freely
falling objects by denoting the motion to
be along the y axis (defining “up” as positive) and setting ay = −g. A freely falling
object experiences an acceleration that is
directed downward regardless of the direction or magnitude of its actual motion.

v y f = v yi − gt

ax =

v x, avg =

v xi + v x f
2

(2.14)

x f = xi + 12 v xi + v x f t

)

(2.15)

x f = xi + v xi t + 12 ax t 2

(2.16)

(

(

v x2 f = v xi2 + 2ax x f – xi

)

(2.17)

y f = yi + 12 (v yi + v y f )t
v y , avg = 12 (v yi + v y f )
y f = yi + v yi t − 12 gt 2
v 2yf = v yi2 − 2 g( y f − yi )

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14

Chapter 2

SUGGESTIONS, SKILLS, AND STRATEGIES
Organize your problem-solving by considering each step of the Conceptualize, Categorize, Analyze, and Finalize protocol described in your textbook and implemented in the
solution to problems in this Student Solutions Manual and Study Guide. Refer to the stepby-step description of the General Problem-Solving Strategy following Section (2.8) of
your textbook, and in the Preface to this Manual.

REVIEW CHECKLIST
•

For each of the following pairs of terms, define each quantity and state how each is
related to the other member of the pair: distance and displacement; instantaneous and
average velocity; speed and instantaneous velocity; instantaneous and average acceleration. (Sections 2.1, 2.2, 2.3 and 2.4)

•

Construct a graph of position versus time (given a function such as x = 5 + 3t − 2t2)
for a particle in motion along a straight line. From this graph, you should be able to
determine the value of the average velocity between two points t1 and t2 and the instantaneous velocity at a given point. Average velocity is the slope of the chord between
the two points and the instantaneous velocity at a given time is the slope of the tangent
to the graph at that time. (Section 2.2)

•

Be able to interpret graphs of one-dimensional motion showing position vs. time,
velocity vs. time, and acceleration vs. time. (Section 2.5)

•

Apply the equations of kinematics to any situation where the motion occurs under
constant acceleration. (Section 2.6)

•

Describe what is meant by a freely falling body (one moving under the influence of
gravity––where air resistance is neglected). Recognize that the equations of kinematics
apply directly to a freely falling object and that the acceleration is then given by a = −g
(where g = 9.80 mրs2). (Section 2.7)

ANSWER TO AN OBJECTIVE QUESTION
13. A student at the top of a building of height h throws one ball upward with a speed
of vi and then throws a second ball downward with the same initial speed | vi |. Just
before it reaches the ground, is the final speed of the ball thrown upward (a) larger,
(b) smaller, or (c) the same in magnitude, compared with the final speed of the ball
thrown downward?
Answer (c) They are the same, if the balls are in free fall with no air resistance. After the
first ball reaches its apex and falls back downward past the student, it will have a downward
velocity with a magnitude equal to vi. This velocity is the same as the initial velocity of
the second ball, so after they fall through equal heights their impact speeds will also be the
same. By contrast, the balls are in flight for very different time intervals.

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Motion in One Dimension

15

ANSWERS TO SELECTED CONCEPTUAL QUESTIONS
1. If the average velocity of an object is zero in some time interval, what can you say
about the displacement of the object for that interval?
Answer The displacement is zero, since the displacement is proportional to average
velocity.

9. Two cars are moving in the same direction in parallel lanes along a highway. At some
instant, the velocity of car A exceeds the velocity of car B. Does that mean that the acceleration of A is greater than that of B? Explain.
Answer No. If Car A has been traveling with cruise control, its velocity may be high (say
60 miրh = 27 mրs), but its acceleration will be close to zero. If Car B is just pulling onto the
highway, its velocity is likely to be low (15 mրs), but its acceleration will be high.

SOLUTIONS TO SELECTED END-OF-CHAPTER PROBLEMS
1. The position versus time for a certain particle
moving along the x axis is shown in Figure P2.1. Find
the average velocity in the time intervals (a) 0 to 2 s, (b)
0 to 4 s, (c) 2 s to 4 s, (d) 4 s to 7 s, and (e) 0 to 8 s.
Solution
Conceptualize: We must think about how x is changing with t in the graph.
Categorize: The average velocity is the slope of a secant
line drawn into the graph between specified points.
Analyze: On this graph, we can tell positions to two
significant figures:
(a) x = 0
v x, avg

at t = 0 and x = 10 m at
Δ x 10 m – 0
=
=
= 5.0 m/s
Δt
2 s–0

t = 2 s:

(b) x = 5.0 m
at
t = 4 s:
Δ x 5.0 m – 0
=
= 1.2 m/s
v x, avg =
Δt
4 s–0
(c) v x, avg =

Figure P2.1

Δ x 5.0 m – 10 m
=
= – 2.5 m/s
Δt
4 s–2 s

■

■

■

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16

Chapter 2

(d) v x , avg =

Δ x –5.0 m – 5.0 m
=
= –3.3 m/s
7 s–4 s
Δt

■

(e) v x , avg =

Δ x 0.0 m – 0.0 m
=
= 0 m//s
8s–0s
Δt

■

Finalize: The average velocity is the slope, not necessarily of the graph line itself,
but of a secant line cutting across the graph between specified points. The slope of
the graph line itself is the instantaneous velocity, found, for example, in the following
problem 5 part (b).
Note with care that the change in a quantity is defined as the final value minus the
original value of the quantity. We use this “final-first” definition so that a positive change
will describe an increase, and a negative value for change represents the later value being
less than the earlier value.

A person walks first at a constant speed of 5.00 m /s along a straight line from point
to point B and then back along the line from B to A at a constant speed of 3.00 m /s.
(a) What is her average speed over the entire trip? (b) What is her average velocity over
the entire trip?

3.

A

Solution
Conceptualize:
velocity.

This problem lets you think about the distinction between speed and

Categorize: Speed is positive whenever motion occurs, so the average speed must be
positive. Velocity we take as positive for motion to the right and negative for motion to the
left, so its average value can be positive, negative, or zero.
Analyze:
(a) The average speed during any time interval is equal to the total distance of travel
divided by the total time:
totaldistance d AB + d BA
average speed =
=
totaltime
t AB + t BA
But

dAB = dBA, tAB = d/vAB,

and

tBA = d րvBA

( )( )

2 vAB vBA
d+d
=
v AB + v BA
d / vAB + d / vBA

so

average speed =

and

⎡ (5.00 m/s)(3.00 m/s) ⎤
average speed = 2 ⎢
⎥ = 3.75 m/s
⎣ 5.00 m /s + 3.00 m / s ⎦

(

) (

)

■

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