- •Preface
- •Contents
- •1 Introduction
- •1.1 Physics
- •1.2 Mechanics
- •1.3 Integrating Numerical Methods
- •1.4 Problems and Exercises
- •1.5 How to Learn Physics
- •1.5.1 Advice for How to Succeed
- •1.6 How to Use This Book
- •2 Getting Started with Programming
- •2.1 A Python Calculator
- •2.2 Scripts and Functions
- •2.3 Plotting Data-Sets
- •2.4 Plotting a Function
- •2.5 Random Numbers
- •2.6 Conditions
- •2.7 Reading Real Data
- •2.7.1 Example: Plot of Function and Derivative
- •3 Units and Measurement
- •3.1 Standardized Units
- •3.2 Changing Units
- •3.4 Numerical Representation
- •4 Motion in One Dimension
- •4.1 Description of Motion
- •4.1.1 Example: Motion of a Falling Tennis Ball
- •4.2 Calculation of Motion
- •4.2.1 Example: Modeling the Motion of a Falling Tennis Ball
- •5 Forces in One Dimension
- •5.1 What Is a Force?
- •5.2 Identifying Forces
- •5.3.1 Example: Acceleration and Forces on a Lunar Lander
- •5.4 Force Models
- •5.5 Force Model: Gravitational Force
- •5.6 Force Model: Viscous Force
- •5.6.1 Example: Falling Raindrops
- •5.7 Force Model: Spring Force
- •5.7.1 Example: Motion of a Hanging Block
- •5.9.1 Example: Weight in an Elevator
- •6 Motion in Two and Three Dimensions
- •6.1 Vectors
- •6.2 Description of Motion
- •6.2.1 Example: Mars Express
- •6.3 Calculation of Motion
- •6.3.1 Example: Feather in the Wind
- •6.4 Frames of Reference
- •6.4.1 Example: Motion of a Boat on a Flowing River
- •7 Forces in Two and Three Dimensions
- •7.1 Identifying Forces
- •7.3.1 Example: Motion of a Ball with Gravity
- •7.4.1 Example: Path Through a Tornado
- •7.5.1 Example: Motion of a Bouncing Ball with Air Resistance
- •7.6.1 Example: Comet Trajectory
- •8 Constrained Motion
- •8.1 Linear Motion
- •8.2 Curved Motion
- •8.2.1 Example: Acceleration of a Matchbox Car
- •8.2.2 Example: Acceleration of a Rotating Rod
- •8.2.3 Example: Normal Acceleration in Circular Motion
- •9 Forces and Constrained Motion
- •9.1 Linear Constraints
- •9.1.1 Example: A Bead in the Wind
- •9.2.1 Example: Static Friction Forces
- •9.2.2 Example: Dynamic Friction of a Block Sliding up a Hill
- •9.2.3 Example: Oscillations During an Earthquake
- •9.3 Circular Motion
- •9.3.1 Example: A Car Driving Through a Curve
- •9.3.2 Example: Pendulum with Air Resistance
- •10 Work
- •10.1 Integration Methods
- •10.2 Work-Energy Theorem
- •10.3 Work Done by One-Dimensional Force Models
- •10.3.1 Example: Jumping from the Roof
- •10.3.2 Example: Stopping in a Cushion
- •10.4.1 Example: Work of Gravity
- •10.4.2 Example: Roller-Coaster Motion
- •10.4.3 Example: Work on a Block Sliding Down a Plane
- •10.5 Power
- •10.5.1 Example: Power Exerted When Climbing the Stairs
- •10.5.2 Example: Power of Small Bacterium
- •11 Energy
- •11.1 Motivating Examples
- •11.2 Potential Energy in One Dimension
- •11.2.1 Example: Falling Faster
- •11.2.2 Example: Roller-Coaster Motion
- •11.2.3 Example: Pendulum
- •11.2.4 Example: Spring Cannon
- •11.3 Energy Diagrams
- •11.3.1 Example: Energy Diagram for the Vertical Bow-Shot
- •11.3.2 Example: Atomic Motion Along a Surface
- •11.4 The Energy Principle
- •11.4.1 Example: Lift and Release
- •11.4.2 Example: Sliding Block
- •11.5 Potential Energy in Three Dimensions
- •11.5.1 Example: Constant Gravity in Three Dimensions
- •11.5.2 Example: Gravity in Three Dimensions
- •11.5.3 Example: Non-conservative Force Field
- •11.6 Energy Conservation as a Test of Numerical Solutions
- •12 Momentum, Impulse, and Collisions
- •12.2 Translational Momentum
- •12.3 Impulse and Change in Momentum
- •12.3.1 Example: Ball Colliding with Wall
- •12.3.2 Example: Hitting a Tennis Ball
- •12.4 Isolated Systems and Conservation of Momentum
- •12.5 Collisions
- •12.5.1 Example: Ballistic Pendulum
- •12.5.2 Example: Super-Ball
- •12.6 Modeling and Visualization of Collisions
- •12.7 Rocket Equation
- •12.7.1 Example: Adding Mass to a Railway Car
- •12.7.2 Example: Rocket with Diminishing Mass
- •13 Multiparticle Systems
- •13.1 Motion of a Multiparticle System
- •13.2 The Center of Mass
- •13.2.1 Example: Points on a Line
- •13.2.2 Example: Center of Mass of Object with Hole
- •13.2.3 Example: Center of Mass by Integration
- •13.2.4 Example: Center of Mass from Image Analysis
- •13.3.1 Example: Ballistic Motion with an Explosion
- •13.4 Motion in the Center of Mass System
- •13.5 Energy Partitioning
- •13.5.1 Example: Bouncing Dumbbell
- •13.6 Energy Principle for Multi-particle Systems
- •14 Rotational Motion
- •14.2 Angular Velocity
- •14.3 Angular Acceleration
- •14.3.1 Example: Oscillating Antenna
- •14.4 Comparing Linear and Rotational Motion
- •14.5 Solving for the Rotational Motion
- •14.5.1 Example: Revolutions of an Accelerating Disc
- •14.5.2 Example: Angular Velocities of Two Objects in Contact
- •14.6 Rotational Motion in Three Dimensions
- •14.6.1 Example: Velocity and Acceleration of a Conical Pendulum
- •15 Rotation of Rigid Bodies
- •15.1 Rigid Bodies
- •15.2 Kinetic Energy of a Rotating Rigid Body
- •15.3 Calculating the Moment of Inertia
- •15.3.1 Example: Moment of Inertia of Two-Particle System
- •15.3.2 Example: Moment of Inertia of a Plate
- •15.4 Conservation of Energy for Rigid Bodies
- •15.4.1 Example: Rotating Rod
- •15.5 Relating Rotational and Translational Motion
- •15.5.1 Example: Weight and Spinning Wheel
- •15.5.2 Example: Rolling Down a Hill
- •16 Dynamics of Rigid Bodies
- •16.2.1 Example: Torque and Vector Decomposition
- •16.2.2 Example: Pulling at a Wheel
- •16.2.3 Example: Blowing at a Pendulum
- •16.3 Rotational Motion Around a Moving Center of Mass
- •16.3.1 Example: Kicking a Ball
- •16.3.2 Example: Rolling down an Inclined Plane
- •16.3.3 Example: Bouncing Rod
- •16.4 Collisions and Conservation Laws
- •16.4.1 Example: Block on a Frictionless Table
- •16.4.2 Example: Changing Your Angular Velocity
- •16.4.3 Example: Conservation of Rotational Momentum
- •16.4.4 Example: Ballistic Pendulum
- •16.4.5 Example: Rotating Rod
- •16.5 General Rotational Motion
- •Index
Chapter 3
Units and Measurement
In physics we study nature quantitatively—we describe nature with numbers. But not with numbers alone. We need to relate numbers to the physical world using measurement units. For example, you could measure the width of your desk using a pencil as in Fig. 3.1, finding that the width is 6 times the length of your pencil and 2.73 times the length of your shoe. The number alone, 6 or 2.73, does not make any sense in the physical world without the unit: a pencil or a shoe. Using a pencil or a shoe may be practical for you, but not if you want to communicate your result to someone else. Therefore we need standardized units.
3.1 Standardized Units
Here we use the standard units provided by SI1—the Systeme International—that provide a few precisely defined base units. For example, the standard unit for length in the SI system is called 1 m. To ensure that this standard is the same everywhere there is a standard meter bar, made of platinum-iridium, which is kept at the International Bureau of Weights and Measures outside Paris. Accurate copies of this bar have been sent to various national standards laboratories around the world.
All other units are derived from the base units in Table 3.1. For example, the unit for force is Newton and the unit for energy is Joule. Both are defined as combinations of the base units in the SI system:
1 Newton = 1 N = 1 kg m s−2 , |
(3.1) |
1 Joule = 1 J = 1 N m = 1 kg m s−2 m = 1 kg m2 s−2 . |
(3.2) |
1http://en.wikipedia.org/wiki/International_System_of_Units. |
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© Springer International Publishing Switzerland 2015 |
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A. Malthe-Sørenssen, Elementary Mechanics Using Python, |
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Undergraduate Lecture Notes in Physics, DOI 10.1007/978-3-319-19596-4_3 |
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3 Units and Measurement |
Fig. 3.1 Measuring the width of a table with a pencil and a shoe
Table 3.1 SI units and standard prefixes
SI units |
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Standard prefixes |
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Quantity |
Unit |
Symbol |
Factor |
Prefix |
Symbol |
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Length |
meter |
m |
1012 |
tera- |
T |
Time |
second |
s |
109 |
giga- |
G |
Mass |
kilogram |
kg |
106 |
mega- |
M |
Amount of |
mole |
mol |
103 |
kilo- |
k |
substance |
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Electric |
ampere |
A |
10−1 |
deci- |
d |
current |
|
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|
|
Temperature |
kelvin |
K |
10−2 |
centi- |
c |
Luminous |
candela |
cd |
10−3 |
milli- |
m |
intensity |
|
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10−6 |
micro- |
µ |
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10−9 |
nano- |
n |
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10−12 |
pico- |
p |
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10−15 |
femto- |
f |
This high level of precision may seem unnecessary, but units were no joke for the NASA teams responsible for the safe landing of the Mars Climate Orbiter.2 The Orbiter was launched in December 1998, and NASA lost contact with it on September 23rd, 1999. The Orbiter was last heard from as it approached Mars way too close to the surface. It turned out that the two groups in NASA working on the approach of the Orbiter used different measurement units. One group used English units (feet and pounds) and the other group used metric units (meters and kilograms), and they had not communicated this difference clearly. The result was devastating for the Orbiter and now serves as a warning for all of us: Keep track of your units!
2http://en.wikipedia.org/wiki/Mars_Climate_Orbiter.
3.1 Standardized Units |
33 |
Numerical Notation
Measured quantities in the SI system may be very large or very small. For example, the velocity of light in the SI system is:
c = 299792458 m/s , |
(3.3) |
and the length of the E. coli bacteria is
l = 0.000001 m . |
(3.4) |
A more practical way to represent these numbers is to use scientific notation, where we use a base of 10. The velocity of light is then:
c = 2.9979248 × 108 m/s , |
(3.5) |
and the length of the E. coli bacteria is
l = 1 × 10−6 m . |
(3.6) |
We no longer need to count the number of digits to see the order of magnitude of the number. This notation is also used by Python where we give a number by a decimal
number followed by E and the number x of tens, corresponding to the exponent x in 10x :
>>>L = 0.000001
>>>L
9.9999999999999995E-07
(Notice also the problem with numerical representation of numbers in this example). Similarly, we use scientific notation when we input numbers in Python
>>>U = 1.25E6
>>>U
1250000.0
Prefixes
To make life simpler, there are prefixes for various standard factors so that we do not have to write out the power of tens each time. Instead of writing
0.001 m = 1.0 × 10−3 m , |
(3.7) |
we write |
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0.001 m = 1 millimeter = 1 mm . |
(3.8) |
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3 Units and Measurement |
Similarly, we write |
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1 nm = 1 × 10−9 m , |
(3.9) |
and the well-known kilometer: |
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1 km = 1 × 103 m = 1000 m . |
(3.10) |
We need a large span of prefixes because our physical world spans over a large range of scales.
3.2 Changing Units
There are many different units used to describe real world quantities: We may measure speed in meters per second, kilometers per hour or feet per second. How do we translate between them? Conversion is done by substituting equivalent quantities represented by different units.
The method is best demonstrated by example. For example, the speedometer in your car reports the speed to be 60 kilometers per hour (km/h). How can you convert this to meters per second (m/s)? This is done by replacing km with meters and hours with seconds by rewriting the units: 1 km = 1000 m and 1 h = 3600 s:
km |
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1000 m |
m |
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60 |
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= 60 |
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= 16.6 |
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. |
(3.11) |
h |
3600 s |
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s |
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What about the reverse scheme? If the wind is blowing 20 meters per second (m/s), what does this correspond to in kilometers per hour (km/h)? We use the same technique as above, although we need an intermediate step to write 1 m in terms of km and 1 s in terms of hours:
1 km = 1000 m |
1 |
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km = 1 m ; , |
(3.12) |
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1000 |
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and similarly: |
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1 h = 3600 s |
1 |
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h = 1 s . |
(3.13) |
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3600 |
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We use these expressions to convert from m/s to km/h:
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m |
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1 |
km |
3600 km |
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km |
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20 |
1000 |
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= 20 |
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= 20 |
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= 72 |
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. |
(3.14) |
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1 |
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s |
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h |
1000 h |
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h |
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3600 |
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3.3 Uncertainty and Significant Digits |
35 |
3.3 Uncertainty and Significant Digits |
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Measured quantities are never exact, but have some uncertainty, which depends on the measurement method. We specify the uncertainty of a measurement by giving a range of values for the measured quantity. If a length is given as 25.0 ± 0.5 m, it means that length most probably is between 25.0 − 0.5 m and 25.0 + 0.5 m. (For quantities with a known distribution of values, we typically describe the range by the standard deviation of the measured quantity).
In practice we use an even briefer way of specifying the uncertainty—by only giving the significant digits when we write down the numerical value of a quantity. For a distance of 25.0 ± 0.5 m it does not make sense to provide many more digits for the length. Writing 25.0000 ± 0.5 m clearly overstates the precision, since we do not really know whether the number is 24.5 m or 25.5 m. Instead we use the number of digits to indicate the uncertainty. We only provide the number of digits we are certain of—the significant digits. Instead of writing d = 25.0 ± 0.5 m we write d = 25 m. This would imply the same: we do not really know whether it is 25.5 m or 24.6 m, but we know that it is not 22 m. Standard practice is that the last digit provided may be uncertain. If you write d = 25 m is means that the value could be d = 24 m or d = 26 m, and if you write d = 25.0 m it means that the value could be d = 25.05 m, but is probably not d = 25.15 m.
This implied uncertainty is why you should never report the full numerical values you get from your calculator or your program. Your program returns a lot of digits— as many digits as it stores—but these digits may not be significant. You therefore need to ensure that you report only the number of significant digits. But how do you know that? You know it because the uncertainty of the result of your calculations will depend on the uncertainty of the numbers you put in. Your calculations cannot improve the uncertainty! The results you report must therefore always reflect the number of significant digits in the data you start with. And it is the number with the largest uncertainty that determines the final uncertainty.
You will learn more formally about how to handle uncertainties in complex calculations in your laboratory courses, but for now you can use the following rules of thumb for handling the number of significant digits:
Multiplication: The number with the least number of significant digits determines the number of significant digits of the result
Addition: It is the position of the decimal point in each of the numbers that determines the uncertainty.
For addition, the position of the decimal point and not the number of significant digits determines the uncertainty of the result:
3.4 mm + 10 mm = 13 mm , |
(3.15) |
1000.00 m + 5 m = 1005 m , |
(3.16) |