124 94 98MB
English Pages 936 Year 2015
McFARLAND
HIRSCH
_O’MEARA
SI BASE UNITS There are seven SI base units, one for each of length, mass, time, electric current, temperature, amount of substance, and luminous inten-
sity. The following definitions of the base units were adopted by the Conférence générale des poids et mesures in the years indicated.
owl [Kitogram |ke
“The metre is the length of the path travelled by light in a vacuum during a time interval of 1/(299 792 458) of a second” (adopted in 1983).
“The kilogram is...the mass of the international prototype of the kilogram” (adopted in 1889 and 1901). “The second is the duration of 9 192 631 770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the cesium-133 atom” (adopted in 1967).
ampere
“The ampere is that constant current which, if maintained in two straight parallel conductors of infinite length, of negligible circular cross section, and placed one metre apart in vacuum, would produce between these conductors a force equal to 2 X 10°’ N/m (newtons per metre of length)” (adopted in 1948).
“The kelvin...is the fraction 1/273.16 of the thermodynamic temperature of the triple point of water” (adopted in 1967).
“The mole is the amount of substance of a system which contains as many elementary entities as there are atoms in 0.012 kg of carbon-12” (adopted in 1967). candela
“The candela is the luminous intensity, in a given direction, of a source that emits monochromatic radiation of frequency 5.40 x 10'4 Hz and that has a radiant intensity in that direction of 1/683 watt per steradian” (adopted in 1979).
SOME Si DERIVED UNITS Derived units are formed from products and ratios of the base units. Some derived units are given special names, such as the newton or joule, to honour certain scientists.
Derived Unit
Quantity
Name
Symbol
area volume
speed
m/s or m-s_!
density
kg/m?
acceleration
Es
force
kg-m/s?
newton
energy
kg-m?/s? or N-m
joule
power
J/s
watt
frequency
I/s ors"!
hertz
pressure
N/m?
pascal coulomb
electric charge
electric potential electric resistance
V/A
ohm
electric capacitance
Cry
farad
magnetic field
N-A’!-m"!
tesla
(radio )activity
I/s ors"!
becquerel
PEEP ETP
NEL
S! PREFIXES Factor
| Prefix
10%
| Symbol
|
Origin
yotta
Italian ott(o) — eight (3 X 8 = 24)
zetta
Italian etta — seven (3 X 7 = 21)
peta
Greek peta — spread out
10° 10° 10°
giga mega kilo
Greek gigas — giant Greek mega — great Greek khilioi — thousand
10°
hecto
‘=
deca*
ex
tera
reek hekaton — hundred reek deka — ten
— =)
deci
Latin decimus — tenth
Om
centi
Latin centum — hundred
102
10% 10
milli
Latin mille — thousand
107}5
femto
Greek femten — fifteen
LO
atto
Danish atten — eighteen
105%
zepto
Greek micros — very small
107?
nano
Greek nanos — dwarf
Italian piccolo — small
Z
Greek (h)epto — seven (—3 X 7 = —21)
Greek octo — eight (~3 x 8 = ~24)
“Alternative spelling: deka.
Greek Alphabet Greek Letter | Name
| Equivalent |Sound When Spoken
Reon
eat
ee
[Sa
Bea
aya
a ae Ee
eal
Zeta
N IN 3 i 1m
9)
md
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zay-tah E
ay-tay
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X
Zz iil
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Can
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Web Increased Engagement.
»
Improved Outcomes.
A
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NELSON
PHYSICS
AN ALGEBRA-BASED APPROACH
Digitized by the Internet Archive in 2023 with funding from Kahle/Austin Foundation
https://archive.org/details/physicsalgebraba0000erni
PHYSICS AN ALGEBRA-BASED APPROACH
Ernie McFarland University of Guelph
Alan J. Hirsch
Joanne M. O’Meara University of Guelph
NELSON
NELSON Physics: An Algebra-Based Approach by Ernie McFarland, Alan J. Hirsch, and Joanne M. O'Meara Vice President, Editorial
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Library and Archives Canada Cataloguing in Publication
McFarland, Ernie, author Physics: an algebra-based approach / Ernie McFarland (University of Guelph), Alan J. Hirsch, Joanne M. O'Meara (University of Guelph). — First edition. Includes index. ISBN 978-0-17-653186-7 (bound)
1. Mathematical physics— Textbooks. 2. Algebraic logic— Textbooks. |. Hirsch, Alan J., author Il. O'Meara, Joanne M. QVoanne Michelle), author Ill. Title.
QC20.7.A4M34 2015 530.15 C2014-908371-8 ISBN-13: 978-0-17-653186-7 ISBN-10: 0-17-653186-6
| BRIEF TABLE TABLE OF OFCONTENTS CONTENTS |
Preface for Instructors About the Authors
xiv
xix
CHAPTER 1
Measurement and Types of Quantities
CHAPTER 2
One-Dimensional Kinematics
CHAPTER 3
Vectors and Trigonometry
CHAPTER 4
Two-Dimensional Kinematics
CHAPTER 5
Newton's Laws of Motion
105
CHAPTER 6
Applying Newton's Laws
139°
CHAPTER 7
Work, Energy, and Power
161
CHAPTER 8
Momentum and Collisions
CHAPTER 9
Gravitation
CHAPTER 1Q~
Rotational Motion
CHAPTER 11
Statics, Stability, and Elasticity
CHAPTERI12
Fluid Statics and Dynamics
CHAPTER13
Oscillations and Waves
CHAPTER 14
Soundand Music
CHAPTER 15
‘Reflection, Refraction, and Dispersion of Light
CHAPTER 16
Wave Optics
CHAPTER17
OpticalInstruments
CHAPTER 18
MHeatand Thermodynamics
CHAPTER 19
Electric Charge and Electric Field
CHAPTER 20
Electric Potential Energy, Electric Potential, and Current
CHAPTER 21
‘Electrical Resistance and Circuits
CHAPTER22
Magnetism
CHAPTER 23
Electromagnetic Induction
CHAPTER 24
Nuclear Physics: Theory and Medical Applications
Glossary
1
21
59 73
195
223 255 287
325
373
413 467
509 551 591 627 651
677
705 735 763
807
Appendix A: Answers to Exercises and End-of-Chapter Questions
Index NEL
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|CONTENTS | Preface for Instructors
xiv
2.5
Acceleration Due to Gravity
G
About
the Authors
CHAPTER
xix
Terminal Speed
1
CHAPTER REVIEW
Measurement in the Past
128
3
3.1 3
5
3.2
Conversions within the Metric System
8
oO
60
3.3 13
Sine Law
ScalarsandVectors
14
Cosine Law
16
LOOKING BACK...LOOKING AHEAD
3.4
65
Adding Vectors
Ee
66
Adding and Subtracting Vectors
66
Using Components
17
63
64
Trigonometric Identities
17
62
Vector Subtraction 62 Trigonometry 63 Sine, Cosine, and Tangent
14
Order-of-Magnitude Estimations
67
Subtracting Vectors
69
ee Vien One-Dimensional
a 3 Ba
LOOKING BACK...LOOKING AHEAD te
2.1
Distance andSpeed 22 Instantaneous Speed 24 Uniform Motion 24
ar
CHAPTER 4 Two-Dimensional Kinematics 73
2.2
Position, Displacement, and Velocity Average Velocity 26
Rinomaticcmel
=|
4.2 36
Solving Constant-Acceleration Problems 38 Equations of Kinematics for Constant Acceleration 38 Applying the Kinematics Equations 40
gs ae
74
Velocity in Two Dimensions
34
oO
: 5 Displacement and Velocity in
Instantaneous Velocity
Variable (Non-Constant) Acceleration
NEL
ce
é. 85
Displacement in Two Dimensions 29
70
70
Two Dimensions
32
Constant Acceleration
2.4
4.1
27
Graphing Non-Uniform Motion
Acceleration
25
CHAPTERREVIEW
27
Instantaneous Velocity Graphing Uniform Motion 2.3
60
Adding and Subtracting Vectors Using Scale Diagrams 61 Properties of Vector Addition
10
Calculations Based on Measurements
CHAPTER REVIEW
36 g S
60
Multiplying a Vector by a Scalar
Derived Units 6 Metric Prefixes 8
1.5
General Properties of Vectors
Vector Symbols 60 Directions of Vectors
6
Dimensional Analysis Significant Digits 12
5S
59
Vectors and Trigonometry
Metric Units, Prefixes, and Conversions Base Units in the Metric System 5
Round-off Error
ae
2
Measurement in Science and Physics
1.3. 1.4
52
CHAPTER 3
2
Scientific Notation
51
Kameel4u/Shutterstock
Measurement in Our Daily Lives
1.2
49
LOOKING BACK...LOOKING AHEAD
The Importance of
Measurement
44
Calculations Involving the Acceleration Due to Gravity 46
Measurement and Types of Quantities 1 1.1
44
Measuring the Acceleration Due to Gravity
74
76
77
Acceleration inTwo Dimensions
79
iistamaneous nccele/averier2e
4.3 4.4
Introduction to Projectile Motion 81 Solving Projectile Motion Problems 86 Maximum Horizontal Range 88
Vil
Viil
4.5
CONTENTS
Uniform Circular Motion
90
The Direction of Centripetal Acceleration
The Magnitude of Centripetal Acceleration 4.6
Velocity CHAPTER REVIEW
CHAPTER
91
7.4
Work Done By Friction
176
7.6
OtherTypes of Energy
178
Elastic Potential Energy in Sports
105
Energy Units
7.7
Gravity, Normal Force, Friction, andTension 106 Free-Body Diagrams 107
5.3
Newton’s Second Law of Motion
Schurt/Shutterstock Stefan
7.8
110
5.5
Solving Problems Using Newton’s First and Second Laws 116
CHAPTER REVIEW
114
CHAPTER
The Fundamental Forces
LOOKING BACK...LOOKING AHEAD
8.1
128
188
189
8
132
195
196
133
Average Force
140
198
Conservation of Momentum Dimension 201
Elastic and Inelastic Collisions
8.4
Conservation of Momentum Dimensions 213
LOOKING BACK...LOOKING AHEAD
6.3
Centrifugal “Force”
in One
8.3
Gunn/ Mitch Shutterstock.com
145
Forces in Circular Motion
SurangaSL/Shu
198
Applications of Conservation of Momentum
139
140
6.2
196
Contact Time during a Collision
8.2
Static and Kinetic Friction
Momentum
Momentum, Force, and Time
CHAPTER 6
146
CHAPTER REVIEW
204
207
in Two 217
217
151
Inertial and Noninertial Frames of Reference
Centrifuges and Centrifugal “Force”
152
Earth’s Surface as a Noninertial Frame of Reference 154
LOOKING BACK...LOOKING AHEAD
151
CHAPTER
Work, Energy, and Power
9.1
223
Law of Universal Gravitation
224
Determination of G 227
155
MarcelC/Think
Gravitational Force between Extended Objects 227
9.2
Gravity Due to Planets and Stars Variations ing on Earth
161 9.3
Gravitational Field
228
231
232
Calculating Gravitational Force from Gravitational Field 234
Work Done by a Constant Force 162
Chiyacat/Shutterstock
9.4
Using Vector Components to Determine Work 164 Work Done in Circular Motion
9
Gravitation
155
CHAPTER 7
7.1
186
Momentum and Collisions
134
Applying Newton's Laws
CHAPTER REVIEW
183
186
123
Newton’s Third Law of Motion
Controlling Friction
Efficiency of Energy Conversions
LOOKING BACK...LOOKING AHEAD
112
Newton’s First Law of Motion
Coefficients of Friction
182
Energy Sources and Conservation
5.4
6.1
181
Energy Return on Investment
More Problem-Solving
178
180
Kilowatt-Hour: An Energy Unit
108
Gravitational Acceleration and Force
CHAPTER REVIEW
Power
173
175
7.5
5
170
172
Law of Conservation of Energy Mechanical Energy
100
Adding Forces
5.8
Gravitational Potential Energy
99
5.2
5.7
7.3
Choosing the y = 0 Position
94
Newton's Laws of Motion
5.6
Kinetic Energy and the Work-Energy Theorem 167
Frames of Reference and Relative
LOOKING BACK...LOOKING AHEAD
5.1
7.2 90
Orbits, Kepler’s Laws, and Weightlessness Keplers Laws
166
Weightlessness
235
237 239 NEL
CONTENTS
9.5
Gravitational Potential Energy in General
CHAPTER
12
Fluid Statics and Dynamics 325
Escape Speed 245 Black Holes 247
Einstein’s Theory of Gravity
248
LOOKING BACK...LOOKING AHEAD CHAPTER REVIEW
242
12.1
249
Properties of Fluids Specific Gravity
250
Pressure
CHAPTER
10
326
Rotational Motion
255
328
Pressure in Liquids
Rotational Kinematics
10.2
Relations between Rotational and Linear Quantities 262 Tangential Acceleration
255
U-Tube Manometer TempSport/Corbis lundt/ Dimitri ©
12.2
263
265
Kinetic Energy of Rolling Objects
10.4
270
Angular Momentum
12.4
275
12.5
277
LOOKING BACK...LOOKING AHEAD
279
279
il
Centre of Mass
288
arindambanerjee/ Shutterstock.com
11.3
Stability 300 Stability and the Human Body 300 Other Examples of Stability 301
291
13.1
303
307
Shear and Bulk Stress and Strain;
309
Torsion of Cylinders 310 Bulk Stress and Bulk Strain
312
Stress and Strain in Architecture
313
314
LOOKING BACK...LOOKING AHEAD
NEL
362
363
Drag Force in General
355
316
367
368
13
373
Oscillations and Simple Harmonic Motion 374
StockSh ©
Period, Frequency, and Phase 304
359
365
Oscillations and Waves
Tensile Stress and Strain; Young’s Modulus
317
351
359
Sedimentation
CHAPTER
292
Stress and Strain; Elasticity
CHAPTER REVIEW
349
350
358
Turbulent Flow
CHAPTER REVIEW
Static Equilibrium
Spanning a Space
349
LOOKING BACK...LOOKING AHEAD
291
Elasticity and Plasticity
Viscosity
Poiseuille’s Law
11.2
Architecture
Fluid Dynamics
Newtonian and Non-Newtonian Fluids
Finding Centre of Mass Experimentally
11.5
344
Buoyancy and Archimedes’ Principle 346
Applications of Bernoulli’s Equation
12.6
Centre of Mass and Newton’s Laws of Motion 290
11.4
340
342
Bernoulli's Equation
280
Centre of Gravity
SurfaceTension
Equation of Continuity
Statics, Stability, and Elasticity 287 11.1
336
Streamline Flow and Ideal Fluids
Angular Momentum and Kinetic Energy
CHAPTER
333
Pascal’s Principle; Pressure in the Atmosphere 335
Capillary Action
Torque and Newton’s Second Law for Rotation 272
CHAPTER REVIEW
Measuring Blood Pressure
Measuring Atmospheric Pressure
12.3
Newton’s Second Law for Rotation
10.5
331
332
Pressure in the Atmosphere
Rotational Kinetic Energy and Moment of Inertia 267
329
329
Other Units of Pressure
10.1
10.3
endopac Think
327
Gauge Pressure and Absolute Pressure
Rolling Objects
IX
The Reference Circle
376
376
13.2
The Simple Pendulum
379
13.3
The Sinusoidal Nature of Simple Harmonic Motion 381
13.4
Energy in Simple Harmonic Motion; Damping; Resonance 386 Conservation of Mechanical Energy in SHM 386 Damped Harmonic Motion Resonance
390
389
X
CONTENTS
13.5
13.6
Energy Transfer with Waves 394 Transverse and Longitudinal Waves 394
CHAPTER 15 Reflection, Refraction, and
an Es3 2
Oceanic and Seismic Waves
Dispersion
E§5 F
PeriodicWaves
395
398
15.1
Reflection and Transmission of Waves
399
Diffraction of Waves
CHAPTER REVIEW
468
403 15.2
407
Measuring the Speed of Light
472
Mirrors and Their images
475
Rg ae
408
cele
S
14
14.2
=
413
9 $F
The Nature of Sound
414
Sound Transmission in Air 414 The Speed of Sound in Air 415 The Speed of Sound in G | 416 : eae he gn teal?
Hearing and the Intensity of Sound
ee A The Human Audible Range 423 Intensity and Loudness a Sound
14.4
The Doppler Effect and Subsonic and Supersonic Speeds in Sound 432
Snell’s Law of Refraction
Dispersion of Light Mirages 489
487
488
: Total Internal Reflection ET nanoee 1c
490
Diamonds and Other Jewels Fibre Optics 493
493
428
15.5
Lenses andTheir Images
432
Wena Aberrations
500
Subsonic and Supersonic Speeds
437
LOOKING BACK..LOOKING AHEAD
Diffraction, Interference, and Resonance : inSound 439
439
CHAPTER
Tonal Quality
14.8
Musical Instruments and Resonance in Stringed and Wind Instruments 447
442
er
Stringed Instruments
16.1
Acoustics
455
CHAPTER REVIEW
:
456
}
i
514
516
S17
Single-Slit Diffraction and Resolution A Qualitative Look at Single-Slit Diffraction
461
:E ZS
Interference Far from the
Measuring the Wavelengths of Visible Light
16.3
459
2
Double-Slit Interference of
Sources
457
462
;
=
509
Diffraction of Light and Huygens’ Principle 510
Two-Source
455
LOOKING BACK...LOOKING AHEAD
16
Light 511 Coherence of Light 514 Analyzing Two-Source Interference Patterns
447
Electrical and Electronic Instruments Virtual Music
16.2
452
Percussion Instruments The Human Voice
502
503
Wave Optics
441
14.6
Wind Instruments
CHAPTER REVIEW
a500
439
Resonance in Sound hc ee ~cales
495
Ray Diagrams for Lenses 496 The Thin-Lens Equation 498 Gradientindex Lenses
Diffraction of Sound
14.9
s=z
g Oe
484
486
436
Beats and Beat Frequency
re fee
Index of Refraction
Applications of the Doppler Effect
ye
’
Refraction and Dispersion of Light
eee
15.4
483
pac Apeicationsanaon
infrasonics, Ultrasonics, and Echgocation
14.5
15.3
423
14.3
Calculating the Observed Frequency
481
Applications of Curved Mirrors
coo
421
476
479
The Mirror Equation
oe
Sound and Music 14.1
eh
Images in Plane MUFOTS Curved Mirrors
CHAPTER
ceae
Light as Energy 468 Transmission of Light 470
406
LOOKING BACK...LOOKING AHEAD
Sources and Propagation of
Light
Interference of Waves 402 Interference in One Dimension 402 Standing Waves in One Dimension
13.8
467
a § 5 ra
The Universal Wave Equation
13.7
of Light
396
519 519
Quantitative Analysis of a Single-Slit Diffraction Pattern 521 NEL
CONTENTS. 16.4
Diffraction Gratings and Spectroscopy Spectroscopy
18.2
Heat, Specific Heat, and Latent Heat
18.3
Thermal Expansion
527
Latent Heats
Diffraction in Two and Three Dimensions
16.5
525
Thin-Film Interference Air-Wedge Interference
528
530
18.4
534
16.6
The Electromagnetic Spectrum
16.7
Polarization of Light
536
Convection
Polarization of Transverse Waves
Light Polarization by Selective Absorption
Light Polarization by Reflection Light Polarization by Scattering
CHAPTER REVIEW
543
First and Second Laws of Thermodynamics
18.5 544
Heat Engines and Entropy
18.6
CHAPTER 17
= 551
ge
552
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Vision Defects and Their Corrections
17.3
The Simple Magnifier
17.4
The Compound Light Microscope
17.5
Telescopes
Space Telescopes
573
Other Telescopes
17.6
564
556
19
19.1
Electric Charge and Atoms
628
19.2
Transfer of Electric Charge
628
19.3
Coulomb’s Law
19.5
Electric Field
631
576
638 639
Electric Field Due to More than One Point Charge
19.6
632
634
Electric Field Due to a Single Charge
580
Electric Field Lines
640
641
Discovery of the Elementary Charge—The Millikan Experiment 643
581 583
Motion of a Charged Particle in a Uniform Electric Field 644
586
LOOKING BACK...LOOKING AHEAD
587
646
647
18
Heat and Thermodynamics
591 &
592
Temperature and Kinetic Energy Internal Energy
CHAPTER 20
Electric Potential Energy, Electric Potential, and cowardlion/Shutterstock Current 651
Temperature and Internal Energy 592 Temperature
NEL
630
Conductors and Insulators
CHAPTER REVIEW
18.1
629
19.4 575 577
LOOKING BACK...LOOKING AHEAD
CHAPTER
Dave Massey/ Shutt
Charging by Contact (Conduction) and by Induction
5/74
Lasers and Holography
CHAPTER REVIEW
621
Static Electricity
571
Controlling Camera Variables Using Lasers
619
620
Electric Charge and Electric Field 627
570
Cameras and Photography
Holography
CHAPTER REVIEW
Electric Force
Structure and Operation of the Camera
17.7
Air Conditioners and Heat Pumps
567
Limiting Factors of a Telescope 573
618
561
567
Radio Telescopes
617
LOOKING BACK...LOOKING AHEAD
CHAPTER
17.2
Reflecting Telescopes
612
613
m
Distance from Sun to nearest star
4 x 10m
Average distance from Earth to Sun
1.5 X 10'"'m
Diameter of Earth
1.3 X 10’ m
Diameter of red blood cell
Sx
Diameter of typical bacteria (Figure 1-9)
mironov/
Figure 1-8 The Andromeda Galaxy, which consists of millions of stars, is similar in shape to our own Milky Way Galaxy. The distance from our solar system to the Andromeda Galaxy is 2 x 10° m. There are thousands of galaxies in the known universe.
MO ei
If SOP? rant
Diameter of hydrogen atom
XX
Diameter of proton
Ie S< 10” tay
Or
rea
Estimated age of universe
Age of solar system
53%
H Time since start of human existence
1X
Age of Egyptian pyramids
10% s
LALS< 10)!"s
One year (approximate value)
3.16 X 10's
Time interval between heartbeats
ls
: Duration of nerve impulse —
OP's
of typical radio waves
| Shortest pulse oflight in laboratory
1X
107s
eS
10nes
Lom
Lifetime of a W particle (a boson)
3
Library Photo Gaugler Gary
3.0 pm ————>
ks
Figure 1-9 This scanning electron microscope image shows rod-shaped Salmonella bacteria with a
ils
diameter of about 1 um and a length of about 3 um.
Masses Known universe (estimated)
aOr
ke:
Milky Way Galaxy
8 X 10" kg
Sun
2 X 10° kg
Earth
6 X 10% kg
| Small mountain
1 xX 10° kg
Ocean liner
8 X 10’kg
Car
1 X 10° kg
| Mosquito
wel
PX H0r ke
| Speck of dust
DO MO ONes
Bacterium
1 x 10°’ kg
_ |Uranium atom
4X 10 *kg
| |Electron
9X SS SSI APE
NEL
When manipulating numbers containing exponents, remember to apply the exponent laws where appropriate:
I
OEE ESE DTI EOE RSE EEO IIL EEE
10" kg LE AIOE APE LID IE Ses
se sje =
7% m+n
x™ alg x
=
Tee
(Ey
=
x™
(xy)" —
x y
Dr.
8
CHAPTER1
Measurement and Types of Quantities
Metric Prefixes Use your calculator to perform the calculation in Sample Problem 1-1 to be sure you are using the EE or EXP key correctly. Avoid the error made by some students who try to enter a number like 10” and get 10° instead because they enter 10 EE 24 instead of the correct entry, 1 EE 24.
Although all lengths could be stated using the base unit of the metre, it is sometimes more convenient to state lengths in larger or smaller units, such as the kilometre, the centimetre, or the very tiny nanometre. The metric prefixes, such as “centi,” “kilo,”
and “nano” are based on multiples of 10, a feature of the metric system that is a great advantage. The inside front cover of this book lists the 20 metric prefixes as well as their symbols, meanings, and origins.
Conversions within the Metric System Measurements to be added or subtracted must have a common unit. For example, you cannot add centimetres to metres without first converting to a common unit. Skill in converting one metric unit to another will assist you in analyzing physical situations and solving physics problems. In general, when converting from one metric unit to another, multiply by a conversion ratio such as (100 cm)/(1 m) in which the numerator and denominator are equivalent. Such a ratio equals, effectively, one; multiplying by one does not change the quantity. To determine the ratio either rely on your memory, which will improve with practice, or refer to the list of metric prefixes on the inside front cover.
SAMPLE PROBLEM | 1-2 | Convert 47.5 mm to metres. Solution
The conversion ratio is either (1 m)/(1000 mm) or (10°* m)/(1 mm). The “mm” must be in the denominator to cancel the “mm” in 47.5 mm. are) ion = 4
lm DS io) X< — 1000 mm
= 0.0475 m Thus, the length is 0.0475 m.
SAMPLE PROBLEM | 1-3 | Add 34 cm and 4.20 m. Solution
Before adding, the measurements must be expressed in the same units. In this case, we will use metres. DID YOU KNOW? Measurement errors can be very serious. In July, 1983, Air Canada Flight 143 from Montreal to Edmonton ran out of fuel before reaching Edmonton and was forced to crash land near
34 cm + 4.20 m = 0.34 m + 4.20 m = Al 4s iin
Thus, the sum is 4.54 m (or 454 cm).
Gimli, Manitoba, thus earning the nickname
“the Gimli Glider.” The crew responsible for fuel made an error in calculating the number of litres of fuel per kilogram required. In 1999, a space mission to Mars failed because the rocket manufacturer listed quantities in British Imperial units but the NASA scientists thought the quantities were in metric units.
SAMPLE PROBLEM |1-4| Convert 3.07 X 10" ps to megaseconds. Solution
From the inside front cover, pico =
10°" and mega =
10°. To avoid errors, the best
way to perform this conversion is to proceed in two steps, first converting picoseconds NE
1.2
to seconds, and then seconds to megaseconds. Both these steps can be carried out in one line:
OMA 3.07 < 10” ps = 3.07 X 10” ps X 1 ps
x
Metric Units, Prefixes, and Conversions
DID YOU KNOW? The world’s smallest lengths in an electron developed in Canada Council. Its divisions
TE 10°s
= 3.07 X 10°° Ms
9
ruler used for measuring microscope was for the National Research are only 18 atoms apart.
Thus, the time is 3.07 X 10° Ms. Notice how the ratios were arranged so that “ps” cancelled “ps,” and “s” cancelled “s,” leaving Ms.
SAMPLE PROBLEM |1-5| Convert the density measurement of 5.3 kg/cm’ to kilograms per cubic metre. Solution
The conversion relating centimetres and metres is 100 cm = | m. Since the denominator contains cm’, which represents cm-cm-cm, we must apply the factor three times, that is, we must cube it: (100 cm)’ = (1 m)’. Hence, we have
k Fes cm
k
100
cm:
= 5.3.
cm)" DID YOU KNOW?
lm
kg
For many people, their height and arm span are essentially the same value. Leonardo da Vinci and other Renaissance artists codified this observation.
le rs ee
Thus, the answer is 5.3 X 10° kg/m’.
©] rerrs Applying Estimation Skills Using your hand span (Figure 1-10), arm span, shoe length, and average walking pace is a skill that will help you estimate a great variety of measurements. Use a metre stick or metric tape to determine the following measurements in the unit stated: ¢ your hand span (in centimetres)
* your arm span (in metres) ¢ the sole of your shoe (in centimetres) ¢ the length of your natural pace (in metres)
Practise using the quantities you determined above to calculate, as accurately as possible, (a) the surface area of a desk or lab bench (b) the surface area of the floor of a room
(c) the distance you travel in 1.0 min while walking at a comfortable speed
EEO
+i
a
ae
te
Figure 1-10 Measuring your hand span.
EXERCISES 1-8
List reasons why the original definitions of the metre and second were unsatisfactory.
1-9
Use the values from Table 1-1 to calculate the approximate value of these ratios: (a) largest length to smallest length (b) longest time to shortest time
NEL
(c) greatest mass to least mass Which quantity has by far the greatest range of values?
1-10 If you could count one dollar each second, how long would it take to count to one billion (10°) dollars? Express your answer in seconds and years.
10
CHAPTER1
Measurement and Types of Quantities
1-11 Determine an estimate for the number of stars in our Milky Way Galaxy by assuming that the mass of the average star is the same as the Sun’s mass, and the masses of other bodies, such as planets,
are insignificant (Reference: Table 1-1).
1-12 The mass of a hydrogen atom is about 1.7 < 10” kg. If the Sun consists only of hydrogen atoms (actually, it is about 95% hydrogen), how many such atoms are in the Sun? (Use Table 1-1 as reference.)
(b) Each bristle of a carbon nanotube is 30 nm in diameter.
(c) At 1.23 X 10° km, the Hudson Bay shoreline is the longest bay shoreline in the world. (d) Each day, Voyageur | spacecraft travels another 10 *Tm away from Earth.
1-18 Perform the following unit conversions, showing Express the final answer in scientific notation. (a)
1-13 Simplify
1.486
x
your work.
20 ms to seconds
(b) 8.6 cm to micrometres
(a) (2.1 X 10°) (4.0 X 10”)
(c) 3.28 g to megagrams
() QS
(d)
OY Ox
IO VOX 10>)
105 MHz to kilohertz
(c) (6.4 X 10”) + (8.0 x 10”)
(e) 2.4 x 10 *MW/m*’ to milliwatts per square metre
(dd) G:88 x 107m) = 2.00'X 10°s)
(f) 9.8 m/s* to metres per square microsecond
1-14 State and give examples of the difference between a derived unit and a base unit. 1-15 Many derived units are named after famous scientists. Name four
(g) 4.7 g/cm* to kilograms per cubic metre
(h) 53 people/km’ to people per hectare (ha) (Note: | ha = 10* m*) 1-19 Simplify
of these and, in each case, state what the unit equals in terms of SI
(a) 280 mm
base units. (Reference: inside front cover.)
(b) 9850 mm
1-16 Describe what patterns can be seen in the list of metric prefixes on the inside front cover.
1-17 Write these measurements without using prefixes: (a) The longest cells in the human body are motor neurons at a length of 1.3 X 107' dam.
1.3
+ 37 cm —
1.68 m
1-20 An American tourist driving in Canada decides to convert the speed limit of 100 km/h to miles per hour, with which she is more familiar. She knows that there are 5280 ft in | mi, that | ft contains 12 in, and that | in = 2.54 cm. Using this information
and your knowledge of SI prefixes, determine the speed limit in miles per hour.
Dimensional Analysis
From earlier science courses, you are familiar with the definition of density as mass/ volume or, using symbols, p = m/V, where p is the Greek letter rho. Rearranging this equation to solve for mass, we have mass = density X volume or m = pV. If this equation is used to solve a problem, the unit resulting from the product of density and volume must equal the unit of mass. The equals sign dictates that the units as well as the numbers are equal on both sides of the equation. An example will illustrate this. Let us find the mass of 0.20 m’ of pure aluminum, which has a density of 2.7 X
10° kg/m’. m=
pV
kg
= 2.7 x 10° me= x 0.20 m
,
=5.4X 10°ke Thus, the mass is 5.4 X 10° kg. In this example, both sides of the equation have dimensions of mass. The symbols for the common
dimensions of length, mass, and time are written L, M, and T,
respectively. We use square brackets to indicate the dimensions of a quantity; for instance, [V] means the dimensions of volume V, and since volume is length X length X length, we have [V] = L’. The process of using dimensions to analyze a problem or an equation is called dimensional analysis _ the process of using dimensions, such as length, mass, and time, to analyze a problem or an equation
dimensional analysis. In this process, the quantities are expressed in terms of dimensions, such as length, mass, and time, and then the expressions are simplified algebraic-
ally. If you develop an equation during the solution of a physics problem, dimensional analysis is a useful tool to ensure that both the left-hand and right-hand sides of your
NEL
1.3
Dimensional Analysis
11
equation have the same dimensions. If they do not, you must have made an error in developing the equation. As an example, the dimensional analysis of the density equation, m = pV, involves determining the dimensions of both sides of the equation to ensure that they are equivalent: Dimensions of left-hand side (L.H.S.)
= [m] =M
M Dimensions of right-hand side (R.H.S.) =[p][V] = ia SEARS
Thus, the L.H.S. and R.H.S. of the equation m = pV have the same dimensions.
SAMPLE PROBLEM |1-6| A student reads a test question which asks for a distance d, given a time ¢t of 2.2 s and a constant acceleration a of 4.0 m/s’. Being unaware of the equation to use, the student decides to try dimensional analysis and comes up with the equation d = at’. Is the equation dimensionally correct? Solution The dimensions involved are L for distance, T for time, and, based on the units m/s’,
L/T’ for acceleration. Now, Dimensions of L.H.S = [d] = L
Dimensions of R.H.S = [aj[?] =
eee XT =L 2
Thus, the dimensions are equal on both sides of the equation, and the equation is dimensionally correct. Unfortunately for this student, the equation is not correct from the point of view of physics. The correct equation is d = 4at’, but since the “ye has no dimensions, it does not change the dimensions of the R.H.S. This illustrates a limitation of dimensional analysis; that is, it cannot detect errors involving multiplication or division by dimensionless constants.
EXERCISES 1-21 Write the dimensions of the following measurements: (a) a speed of 6.8 m/s
1-23 Use the information in the inside front cover to write the dimensions of these derived units:
(b) a speed of 100 km/h
(a) newton
(c) an acceleration of 9.8 m/s?
(b) watt
(d) adensity of 1.2 g/cm’
(c) hertz
1-22 Determine the final type of quantity produced (e.g., length, speed, etc.) in the following dimensional operations: @
IL KUT
(b) (LT) X TT
1-24 When a person is jogging at a constant speed, the distance travelled equals the product of speed and time, or d = vt. Show that the dimensions on both sides of this equation are equal.
1-25 Assume that for a certain type of motion, the distance travelled is related to time according to the equation d = kt’, where k is a constant. Determine the dimensions of k.
(CieMec bs GQ(L/Pieet
1-26. Prove that the equation d= v,t + Sat’ is dimensionally correct. (dis a distance, v, is initial velocity, tis time, and a is acceleration.) REN
EPSTEIN
ISSCESSIES DEESIDE ISISDDEABLS TO
IEEE DIE OLE SENDER I SELES ELPA USEIU ALLS BE ELE SEE EDIE
EISELE LEVIED YORI YEEDLEE ABIDE ELAM VASE
CERES LS PP LIEGE DEE PECL POLD SAGA BOIO IEISEN LESSEE SAE TIS
LRA
12
CHAPTER1
Measurement and Types of Quantities
1.4
Significant Digits
Quantities that are counted are exact, and there is no uncertainty about them. Two
examples are found in these statements: There are 27 bones in a human hand.
Ten dimes have the same value as one dollar.
in measurement, the range of values
Measured quantities are much different because they are never exact; every measurement has some uncertainty associated with it. Measurement uncertainty is the
in which the true value is expected to lie; also called peepMeane
range of values in which the true value is expected to lie; it is also called possible error. Uncertainty should accompany a measured value; in fact, the reporting of a measured
significant digits
value is not complete without stating the uncertainty of the measurement. The uncertainty may arise from the measurement device, environmental conditions, properties of the item being measured, or even the skill of thé person doing the measuring. As an example, suppose you are measuring the mass of a-friend in kilograms. You might try a bathroom scale and get 56 kg, then a scale in a physician’s office and get 55.8 kg, and finally a sensitive electronic scale in a scientific laboratory and get 55.778 kg. Not one of these measurements is exact; even the most precise measurement, the last one, has an uncertainty. For the bathroom scale, the reading of 56 kg could mean that the mass is closer to 56 kg than either 55 kg or 57 kg, and the measurement could be written as 56 kg + | kg. However, you may believe that you can read the scale to the closest 0.5 kg, in which case you would record the measurement as 56 kg + 0.5 kg. In many instruments, the uncertainty 1s stated either on the scale or in the owner’s manual. For example, the scale in the physician’s office could have an uncertainty of + 0.2 kg, so the measurement would be recorded as 55.8 kg + ().2 kg, and if the uncertainty of the electronic scale is + 0.001 kg, the measurement is recorded as 55.778 kg + 0.001 kg. In any measurement, the digits that are reliably known are called significant digits.
uncertainty
the digits in any measurement
that are reliably known
These include the digits known for certain and the single last digit that is estimated. Thus, the mass of 56 kg + | kg has two significant digits, and 55.778 kg + 0.001 kg has five significant digits. The number of significant digits can be determined by applying these rules: ¢
Zeroes placed before other digits are not significant: 0.089 kg has 2 significant digits.
¢
Zeroes placed between other digits are always significant: 4006 cm has 4 significant digits.
¢
Zeroes placed after other digits behind a decimal are significant: both 5.800 km and 703.0 N have 4 significant digits.
e
Zeroes at the end of a number are significant only if they are indicated to be so using scientific notation to place the zeroes after a decimal. For example, the distance 5 800 000 km may have anywhere from 2 to 7 significant digits. By using scientific notation, we can judge which digit is the estimated one, so we can determine the number of significant digits:
5.8 X 10° km has 2 significant digits
5.800 5.800 000 percent error
the difference between the measured
and accepted values of a measurement expressed as a percentage
10° km has 4 significant digits 10° km has 7 significant digits
If the accepted value of a measurement is known, the percent error of an experimental measurement can be found using
percent error =
|measured value — accepted value| accepted value
X 100%
NEL
1.4 Significant Digits
13
Calculations Based on Measurements Measurements made in experiments or given in problems are often used in calculations. For example, you might be asked to find the average speed of a cyclist given the measurement of the time it takes to travel a certain distance. The final answer of the problem should take into consideration the number of significant digits of each measurement, and it may have to be rounded off. When adding or subtracting measured quantities, the final answer should have no more than one estimated digit.
SAMPLE PROBLEM |1-7 | Add 123 cm + 12.4cm + 5.38 cm
tions were done first then the answer was rounded off. When calculated answers are
Solution
rounded off to the appropriate number of significant digits, the following rules apply:
123 cm (the “3” is estimated) 12.4 cm (the “4” is estimated)
+ 5.38 cm (the “8” is estimated) 140.78 cm (the “0,” the “7,” and the “8” are estimated)
Thus, the answer should be rounded off to one estimated digit, or 141 cm.
When multiplying or dividing measured quantities, the final answer should have the same number of significant digits as the original measurement with the least number of significant digits.
SAMPLE PROBLEM |1-8| A cyclist travels 4.00 X 10° m on a racetrack in 292.4 s. Calculate the average speed of the cyclist. Solution
Average speed (v) is distance (d) divided by time (f):
d_ 4,00 x 10°m
27
2904
0's
= 1.368.. X 10' m/s This answer should be rounded off to three significant digits. Hence, we obtain an average speed of 1.37 X 10' m/s or 13.7 m/s.
Most quantities written in this book have either two or three significant digits, although some quantities require more significant digits. The answers to the numerical problems have been written to the correct number of significant digits after rounding off following the rules given in this section. You will be able to practise the rules of significant digits with every numerical problem.
“In some specialized cases in statistical calculations, the digit preceding a 5 is not changed if it is even, but it is raised by 1 if it is odd; e.g., 1.265 becomes 1.26 and 1.275 becomes 1.28. This rule exists to
avoid the accumulated error that would occur if the 5 were always rounded up.
NEL
¢ If the first digit to be dropped is 4 or less, the preceding digit is not changed; e.g., to three significant digits 3.814 becomes 3.81. If the first digit to be dropped is more than 5, or a 5 followed by digits other than zeroes, or a 5 alone or followed by zeroes, the preceding digit is raised by 1; e.g., to three significant digits 5.476 becomes 5.48; 9.265 221 becomes 9.27;
and 1.265 becomes 1.27.
14
CHAPTER1
Measurement and Types of Quantities
Round-off Error Assume
you are helping a friend choose floor tiles for a room
with a length (/) of
5.17 dm and a width (w) of 3.41 dm. At a price of $2.49/dm?, how much will the tiles cost? You begin by finding the surface area (A) of the floor: A=IxXw
= 55117 Ginn < S42) Gham
= 1207
ahaa
If you follow the rules of rounding off answers, this area becomes 17.6 dm?. Next you calculate the cost: Cost =A X rate =
17/6 cian?
Mo
pay
~
dm:
= $43.824, or $43.80 to three significant digits But if you had simply left the area calculation in your calculator before multiplying by the rate, the calculated cost would have been: Cost —"A ~ rate
$2.49 = {7207 cline S< °: 2
= $43.89795, or $43.90 to three significant digits You can see that, to obtain a final answer valid to three significant digits, it is necessary to keep more than three significant digits in intermediate answers. Rounding off too early introduces error, which is referred to as round-off error. Hence, when doing calculations, remember to keep all the digits in your calculator until the final answer is determined, and then round off this answer to the correct number of significant digits. If it is necessary to write down an intermediate answer, use the correct number of significant digits, but keep the intermediate answer with all its digits in your calculator.
Order-of-Magnitude Estimations
order-of-magnitude estimation
a calculation
based on reasonable assumptions to obtain a value expressed to a power of 10; also called a Fermi question after Enrico Fermi
When solving numerical problems in physics, as well as in everyday experiences, it is good to be able to estimate the value of a quantity. This skill applies when checking that a calculated answer makes sense, but it also can be applied when you are trying to decide if you can believe some advertising or reports in the media. An order-of-magnitude estimation is a calculation based on reasonable assumptions to obtain a value expressed to a power of 10. Often there is only one significant digit in the calculated value. Consider, for example, an estimation of the volume of air in litres inhaled by a person in one year. We begin with two assumptions. First, a person would inhale about one litre (1 L) of air with each breath. (You might find a more
accurate value by
devising a water-displacement experiment.) Second, the number of breaths a person would take per minute would likely be between 10 and 20, let’s say 15. Now we are ready for the calculation. Notice the cancellation of units in this calculation.
volume of air =
8, breath
x
= 8 X 10°L/
15 breaths min
x
60min h
x
24h_ day
x
365d _=—year
year (one significant digit)
Thus the volume of air inhaled by a person is approximately 8 < 10° L/year. Orderof-magnitude estimations are often rounded off to the nearest power of ten. In this example, we would then obtain 10’ L/year.
NEL
1.4
Significant Digits
15
This type of question will be asked from time to time in this text. Such a problem is called a Fermi question, named after Enrico Fermi, a famous physicist and professor who often asked his students to estimate quantities impossible to measure directly.
(2) PROFILES IN PHYSICS Enrico Fermi (1901-1954): Combining Education with Experimental and Theoretical Physics Enrico Fermi was a brilliant physicist who was at the forefront of 20th century science (Figure 1-11). He is celebrated as one of the leaders in understanding nuclear reactions and learning how to control them. He is remembered as a great teacher who used estimation questions, along with many other methods, to inspire his students to “think physics.” He was honoured by having an element named after him (Fermium, atomic number 100) as well as a class of particles called “fermions,” which have a particular characteristic spin. Born in Rome in 1901, Fermi entered higher education at an institute in Pisa, Italy, at age 17. By age 20 he was already publishing articles in scientific journals. He studied at various European universities and became a physics professor at the University of Rome when he was 24. When Fermi began concentrating less on theoretical physics and more on experimental physics, he discovered how to cause neutrons to slow down during a nuclear reaction. This important discovery later led to the
development of controlled nuclear fission reactions and nuclear fission bombs. For this discovery as well as other contributions, Fermi was awarded the Nobel Prize in Physics in 1938. Shortly after receiving this award in Sweden, he and his family moved to the U.S.A. where he later became a U.S. citizen. Once in the U.S.A., Fermi joined other eminent physicists working on the secret “Manhattan Project” in Chicago, where they created the world’s first chain-reaction “atomic pile.” In July 1945, while witnessing a major nuclear explosion test, he performed the type of calculation he often asked his students to do: he estimated the power of the nuclear blast. Not surprisingly, his estimation was “in the ballpark.” Enrico Fermi combined experimental and theoretical physics in a way that no other leading physicist did. He was highly respected and well-liked, and he preferred easier explanations to harder ones. He died at age 53 of cancer, possibly related USA/Alamy Pictures Keystone © to his close work with radioactive nuclear materials.
EXERCISES 1-27 Three different scales are for sale at three different prices. A potential buyer measures the mass of a box on the scales and obtains these values:
42.40 kg = 0.005 kg 42.4kg + 0.05 kg
424kg + 100g Which scale do you think would be the most expensive? the least expensive? Why? 1-28) State the number of significant digits in each measurement:
(a) 0.04 Tm (b) 400.20 pm (c) 8.10 X 10°kg (d) 0.008 200 ws
1-29 Round off each quantity to three significant digits, and write the answer 1n scientific notation. (a) 38510 Gm (b) 0.000 940 488 MW (c)
55.055 dam
(d) 876.50 kL (e) 0.076 550 pg 1-30 A student performs measurements to determine the density of pure water at 4°C, and obtains an average result of 1.08 X 10° kg/m’. The accepted value is 1.00 < 10° kg/m*. What is the percent error in the experimental measurement? 1-31 A rectangular mirror measures 1.18 m by 0.378 m. Find the perimeter and the surface area of the mirror, expressing your answers to the appropriate number of significant digits.
16
CHAPTER1
Measurement and Types of Quantities
(a) Assume that the mass of an average cell in your body is 1 x 10“ kg. Calculate the number of cells in your body.
1-32 Use the data on the inside back cover to determine the difference in masses between
(b) What is the mass in kilograms of all the hamburger patties consumed in North America in one year?
(a) aneutron and a proton (b) a proton and an electron
(c) Assume that a Ferris wheel at an amusement park were to fall off its support and become a gigantic rolling wheel. How many rotations, travelling in a straight line, would it have to make to travel from Calgary to Winnipeg?
1-33 Assume that the Earth-Sun distance has a constant value of 1.495 988 = 10'' m and the Earth-Moon distance is constant at 3.844 x 10° m. Also assume that all three lie in the same plane. Determine the greatest and least Moon—Sun distances, taking into consideration significant digits.
(d) Canada’s coastline, including along its islands, is the longest in the world at about 2 X 10° km. If Canada’s entire population were lined up side-by-side with outstretched arms just touching, how many total populations would equal the coastline length?
1-34 Find the time it takes light, travelling at 3.00 x 10° m/s, to travel from the Sun to Earth. (Use the distance given in Question 1-33, and remember significant digits.) 1-35 Fermi Question: Determine a reasonable order-of-magnitude estimation in each case. Show your reasoning.
1.5
Scalars and Vectors
A tourist, trying to find a museum scalar quantity
a quantity with magnitude (or
size) but no direction (also called a scalar)
vector quantity
a quantity with both magnitude
and direction (also called a vector)
DID YOU KNOW? Scalar is derived from the Latin word scala,
which means “ladder” or “steps” and implies magnitude. Vector is a copy of the Latin word vector, which means “carrier” and implies something being carried from one place to another in a certain direction. In biology, a vector can be an organism that carries disease or an agent that transfers genetic material.
in an unfamiliar city, asks how to get there and is
told, “All you have to do is walk one-and-a-half kilometres from here.” This information is obviously not very useful without a direction. A measurement of 1.5 km is an example of a scalar quantity, one with magnitude but no direction. (Magnitude means size.) A measurement such as 1.5 km west is an example of a vector quantity, one with both magnitude and direction. Some common scalar quantities and typical examples are Length or distance
A race track is 100 m long.
Mass
The mass of a newborn baby is approximately 3 kg. The time interval between heartbeats is about 1.0 s.
Vector quantities are common study of motion and forces are Displacement
in physics. The ones used most frequently in the
A crane is used to lift a steel beam 40 m upward.
Velocity
A military jet was travelling at 1600 km/h east.
Acceleration
The acceleration due to gravity on the Moon is 1.6 m/s’ downward (toward the centre of the Moon).
A person falling about 50 cm onto a hard surface and landing on a heel experiences a force of about 2 X 10* N upward, enough to fracture a bone.
Scalar quantities, also called scalars, are easy to manipulate algebraically. The ordinary rules of addition, subtraction, multiplication, and division apply. Vector quantities, or vectors, are more complex. They require special symbols and rules of addition, subtraction, and so on. The general nature of scalars and vectors will be considered as you proceed through Chapter 2. However, details regarding vectors are presented in Chapter 3, which prepares you for vector analysis in two-dimensional motion in Chapter 4.
EXERCISES 1-36 List three scalar quantities other than those already given, and give an example of each.
1-37 For motion that you have experienced today, write two specific examples of displacement and two of velocity.
Chapter Review
|LOOKING
WVé
BACK...LOOKING AHEAD AHEAD
This chapter has emphasized the importance of measurement and basic mathematical skills in physics. Details of the SI units were presented; this system will be used throughout the text. The topics of scientific notation, uncertainties, significant digits, and order-of-magnitude estimations were featured. Scalar and vector quantities were introduced and compared.
In the remainder of the text, you will apply and extend your knowledge of measurement and skills in mathematical operations. The next chapter deals with motion in one dimension. Then Chapter 3 describes mathematical details of vectors and trigonometry required for the study of motion in two dimensions in Chapter 4. Displacement, velocity, and acceleration vectors are important there.
| CONCEPTS AND AND SKILLS. SKILLS Having completed this chapter, you should now be able to do the following: ° State the SI base units of length, mass, and time and give examples of derived units. ¢ Convert from one metric unit to another. ¢ Write numbers using scientific notation. e Apply the exponent laws, especially for multiplication and division involving powers.
Poe
e ¢ ¢
Verify that the dimensions of an equation are correct by using dimensional analysis. Write measurements to the appropriate number of significant digits. Calculate the percent error of a measured value knowing the accepted value.
¢
Perform calculations (+,—,x, and +) involving measured quantities
¢
and round off the answer to the appropriate number of significant digits. Develop skill in estimating quantities and calculate order-ofmagnitude estimations.
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You should now be able to define or explain each of the following words or phrases:
SI
significant digits
scientific notation
percent error
qualitative description
nanotechnology
derived unit
order-of-magnitude estimations
quantitative description
standard unit
dimensional analysis
scalar quantity (or scalar)
measurement
base (or fundamental) unit
uncertainty
vector quantity (or vector)
Chapter Review MULTIPLE-CHOICE QUESTIONS 1-38
The mass closest to
of a heavyweight
(a) 10° (b) 10° (c) 10° 1-39
wrestler,
in grams,
is
(d) 10° (e) 10’
(a) DEBNESA (@) IBC. ID)AN
(a) 7
(d) 4
(b) 6
Crs
+
How many significant digits are there in the product 8.005 00 x 0.005 380 1?
(a) 7 (b) 6
(d) 10° nm (e) 10" pm
(d) B,D, A,C (e) none of these
How many significant digits are there in the sum 460.299 390.0008 + 6.123 + 5.07?
(@) 3S
1-42
Order the following four masses in descending size: A: 10 *Mg; BatOukeC210/° Ye; Di 107 Ge. (b) A, C, B, D
NEL
male
Which length is the smallest? (a) 10°cm (b) 10° mm (c) 10° mm
1-40
1-41
@)
1-43
(d) 4 (e) 3
5
An airline passenger of mass 78 kg has a 20.7 kg checked bag and a 4.19 kg carry-on bag. The total mass, to the correct number of significant digits, is
(a) 1.0289 X 10° kg (b) 1.029 X 10° kg (c)
1.03 X 10° kg
(d) 1.0 X 10? kg (e)
1 X 10°kg
18
CHAPTER
1
Measurement and Types of Quantities
Review Questions and Problems 1-44
List reasons why measurement is important for use in (a) society
1-53
and (b) physics.
1-45
List the SI base units of length, time, and mass.
1-46
Why is it not necessary to have a base unit for area in the SI?
1-47
A high-rise apartment building is 30 storeys high. Estimate the height of the building in metres and decametres, showing your reasoning.
1-48
Convert each measurement to the units indicated in parentheses. State the answers in scientific notation.
|Force (F) |Energy (E)
|(F)= Mur | l= ML"
|Power (P)
|[P] = [EVT
Pressure (p)
[p] = [FVL?
(a) What do the symbols M, L, and T mean?
(a) Mt. Everestis 8.85 km high. (metres, decimetres, centimetres)
(b) Make a similar list for these quantities: speed (v), accelera-
(b) The biggest animal known was a blue whale with a mass of 1.90 X 10° Mg. (kilograms, grams, centigrams)
tion (a), and area (A).
(c) Express the dimensions of power and pressure in terms of M,
(c) A “cosmic year” is the time our solar system takes to complete one revolution around the centre of the Milky Way Galaxy. It is
L, and T.
;
(d) How can the dimensions of energy be expressed in terms of mass and speed?
about 2.2 X 10° years. (seconds, microseconds, and exaseconds)
1-49
The list below shows the symbols and dimensions of some quantities used in physics.
(e)
Determine the ratio of each of the following masses to your own mass:
How can the dimensions of power be expressed in terms of mass, speed, and acceleration?
(a) The world’s largest erratic boulder (1.e., one moved by a glacier), located in Alberta, has a mass of 16 Mg.
1-54
If two measurements have different dimensions, can they be added? multiplied? Give an example to illustrate each answer.
(b) The lightest human birth on record is 0.26 kg.
1-55
Before a wooden metre stick is imprinted with millimetre and centimetre markings, it 1s important that the wood be cured (..e., properly dried). Explain why.
1-56
An experiment is used to determine the speed of light in a transparent material. The measured value is 1.82 < 10° m/s and the accepted value is 1.86 X 10° m/s. What is the percent error in the measurement?
1-57
A customer buys three 120 cm pieces of rope from a new roll that is 500 m long. Assume both measurements have three significant digits. What length of rope is left on the roll? (Don’t forget significant digits.)
1-58
The official diameter of the discus for women is 182 mm and for men it is 22] mm. If each discus is rolled along the ground like
(c) The heaviest mass D2. 10 kg:
supported
(d) A prize winning pumpkin (Figure 1-12).
by a person’s
had a mass
shoulders
of 6.7 X
is
10° dg
(e) A recipe calls for 28 g of sea salt.
a wheel for 25.0 revolutions, how much farther does the men’s
discus travel? swisshippo/Fotolia.com ©
1-59
A soccer goal is 7.32 m wide and 2.44 m high. Calculate the area of the goal opening.
1-60
The equation for the volume of a cylinder is V = rh, where r is the radius and / is the height. Find the volume in cubic centimetres of a solid cylinder of gold that is 8.4 cm in diameter and 22.8 cm in height. Write your answer in scientific notation with the appropriate number of significant digits.
1-61
Figure 1-12 A typical prize-winning pumpkin (Question 1-49(d)).
1-50
The larva of a certain moth consumes 86 000 times its own mass at birth within its first 48 h. How much would a human with a mass at birth of 3.0 kg have to consume in the first 48 h to compete with this phenomenal eater? Express your answer in kilograms, then in a unit that requires a number between | and 1000.
1-51
Simplify
Fermi Question: Determine an order-of-magnitude estimation for each quantity. (Show your reasoning.)
1-52
(a) 2.00 X 10° km — 3.0 X 10°m
(a) the number of your normal paces it would take to walk 1.6 km
(b) (4.4 X 10? m) + (2.0 X 10° s’)
(b) the number of kernels of corn in a container that holds 1.0 L
(c) (4.4 X 10’ m) + (2.0 x 10° s)’
(Hint: It may help you to know that a cube 1.0 dm (= 10 cm) on a side has a capacity of 1.0 L.)
The equation for the area of a circle is A = mr’, and the equation for the area of a right-angled triangle is A = bh/2. (a) What do the symbols r, b, and h represent?
(b) Determine the dimensions of the right side of each equation. What do you conclude?
(c) volume of water (in litres) in a typical above-ground backyard swimming pool (See the hint in (b) above.) (d wa the number of times your heart has beat in your lifetime to date
(e) the number of people in the world who are sleeping at the time you are answering this question
NEL
Applying Your Knowledge
1-62
Classify each of the following as either scalar or vector.
(d) the reading on a car’s speedometer
(a) the force exerted by your biceps on your forearm as you hold a weight in your hand
(e) the gravitational force of the Moon on Earth
19
(f) the age of the universe
(b) the number of cars in a parking lot (c) the reading on a car’s odometer
Applying Your Knowledge 1-63
Do the prefixes kilo, mega, and giga when used in connection with computers (e,g., kilobyte) have the same meaning as in SI? Explain your answer.
1-64
Fermi Question: Determine an estimate for the number of cells in your index finger. Assume that the cells are spherical and have
a diameter of about 10 um.
1-65
Fermi Question: The heart of an average adult pumps about 5 L of blood per minute. Estimate the volume of blood your heart will pump from now until the end of your own life expectancy.
1-66
Determine the approximate time it takes a fingernail to grow 1 nm. State your assumptions and show your calculations.
DID YOU KNOW? The answer to Question 1-66 indicates how quickly layers of atoms are assembled in the process of protein synthesis. It took many years to grow the longest fingernails in the world, a world record of 8.65 m in total for all ten fingernails.
falconhy/Fotolia.c ©
Figure 1-13 A peregrine falcon in flight (Question 1-69(b)).
1-70
Recent
measurements
have caused
scientists to state that the
length of a mean solar day increases by | ms each century. (a) How much longer would a day be 3000 years from now?
1-67
one microcentury. Determine how close his estimate was.
1-68
(b) How long will it take from now for the day to be one minute
At one time, Enrico Fermi stated that his 50 min lecture lasted If volume were a base dimension (V) in the SI, what would be the
longer?
1-71
Show mathematically why the stars in the photograph appear to move at the rate of 15° every hour.
dimensions of length? of area?
1-69
NEL
(a) In Canada, the speed limit on many highways is 100 km/h. Convert this measurement to metres per second. (b) The fastest measured speed of any animal is 97 m/s, recorded as a peregrine falcon was diving (Figure 1-13). Convert the measurement to kilometres per hour. (c) Suggest a convenient way of changing metres per second to kilometres per hour and vice versa.
Refer to Figure 1-3(b) on page 3.
Determine approximately how long the time-exposure photograph lasted.
1-72
Fermi Question: Imagine that you are able to cover a typical football field with $10 bills laid out flat. Determine an estimate of the height to which those bills would reach if stacked tightly flat on top of each other.
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