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September 8, 2009 Physics I Lesson 1Dr J. Tison
1
Scientific Discovery( A mystery story)
• Curiosity and inquisitiveness of how natural phenomena occur
• Observe and interpret
• Imagination – Hypothesize meaning of observations– Create models and theories
• Test models and theories: experiments– Modify and retest
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Refine models and theories
• Accepted theories– often proven incorrect by new evidence– create new or improved theories
• Example… – Ptolemy (ca 100AD) taught the earth is center
of solar system – Copernicus, then Galileo (ca 1500AD)
determined that the sun is the center of the solar system.
September 8, 2009 Physics I Lesson 1Dr J. Tison
3
Symmetry in the universe?
• A scientist looks for…– Symmetry or commonality – Applies accepted theories, hypotheses, or models.
• Example…– Newton’s Law of Gravitational Force (2 masses):
• Fg = Gm1m2/r2
– Coulomb’s Law of Electrostatic Force (2 charges): • Fe = Kq1q2/r2
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Expand the range of theories• Newton’s law of motion
– “classical” description of bodies in motion
• Einstein’s theories of relativity – “modern” physics extends to the wider range
of phenomena, in the universe
Newton’s Laws of Motion are used to describe most natural phenomena that are observed in normal everyday situations.
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Who’s on first? Models, Theories, Laws & Principles
• Model: Visual concept of what is observed
• Theory: Detailed description with measurable results to test model
• Law (e.g. Newton’s): Concise, general statements about how nature behaves
• Principle: (e.g. Archimedes) is a less general statement than a law
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Measurement and Uncertainty
Lord Kelvin (1824-1907):
• “… when you can measure what you are speaking about, and express it in numbers, you know something about it;
• … when you cannot express it in numbers, your knowledge is of a meager and unsatisfactory kind;
• … it may be the beginning of knowledge, but you have scarcely, in your thoughts, advanced the stage of Science, whatever the matter may be”
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Measurements
• Some examples…– Distance, speed (and velocity) – Temperature – Time– Weight – And, many others.
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Measurement and Calculations
• Examples...– Speed = (distance)/(time) e.g. mph, ft/sec, etc
• 2 measurements: (1) distance; (2) time
– Momentum = (mass)∙(velocity) = (mass)∙(distance)/time
• 3 measurements: (1) mass; (2) distance; (3) time
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Undefinable Quantities
• Some physical quantities…– length, time, mass, temperature, are
fundamental and are not calculated from others
– International committees (e.g. SI) determine the “standard” for measuring undefinable quantities
September 8, 2009 Physics I Lesson 1Dr J. Tison
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SI Base units: Length
Length: meter (m) – Length of the path traveled by light in a
vacuum, – During the time interval of 1/299 792 458 of a
second
Note: Speed of light is 299,792,458 m/s
September 8, 2009 Physics I Lesson 1Dr J. Tison
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SI Base units: Mass
Mass: kilogram (kg) – Mass of a platinum-iridium cylinder
• (Bureau International des Poids et Mesures (BIPM), Sèvres, Paris (1st CGPM (1889), CR 34-38).
– Only base unit with a prefix (kg); • Gram is derived unit, equal to 1/1000 of a
kilogram;
– Only unit still defined by a physical prototype • (instead of a measurable natural phenomenon )
September 8, 2009 Physics I Lesson 1Dr J. Tison
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SI Base units: Time
Time : second (s)
• Duration of exactly 9,192,631,770 periods of the radiation corresponding to
• Transition between two hyperfine levels of the ground state of the cesium-133 atom– at a temperature of 0º K
September 8, 2009 Physics I Lesson 1Dr J. Tison
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SI Base Unit:Temperature, Kelvin (ºK)
• Thermodynamic temperature, ºK – Absolute temperature – Fraction 1/273.16 (exactly) of the
thermodynamic temperature at the triple point* of water
*Triple Point of Water: water, ice, and water vapour coexisting in a stable equilibrium :0.01 °C; 6.03 x 10-3 atm)
September 8, 2009 Physics I Lesson 1Dr J. Tison
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SI Base Unit: Ampere (A)
• Ampere: Constant current maintained in– Two straight parallel conductors of
• Infinite length and • Negligible cross-section, and• Placed 1 meter apart in a vacuum,
– Produces a force between these conductors
= 2×10 -7 n/m
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Systems of Units
• mks– SI – French Academy of Sciences – meter, kilogram, sec
• cgs– centimeter, gram, sec
• British
– foot, lb, sec
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Conversion between Units
Speed = distance/time– 1 m/s = (1m/s)(100cm/1m) = 100cm/s
– 1 m/s = (1m/s) (1in/2.54cm)(100cm/1m) = 3.94in/s
– 1 m/s = (1m/s) (1in/2.54cm)(100cm/1m (60s/min)
(60min/h)
= 14.2 x 103 in/h
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Uncertainty: Accuracy, Precision
Which has high accuracy? high precision? low accuracy? low precision?
September 8, 2009 Physics I Lesson 1Dr J. Tison
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X Y
• X = average value – sometimes written as= <x>
• Y = calculated difference from <x> – Y is measure of “precision”– % = y/x ∙ 100
• Multiple measurements as in a “Gage R&R” – 5 or 10 measurements.– Static or dynamic– 3 days
September 8, 2009 Physics I Lesson 1Dr J. Tison
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All Measurements have Uncertainty
• Random Errors: statistical – Repeatability and reproducibility– Unpredicable fluctuations in temperature or line
voltage– Mechanical vibrations of an experimental setup– Unbiased estimates of measurements by observer
• Systematic Errors: determinate
– Measurement device: – Instrument calibration– Personal error, e.g. parallax reading of a gage
September 8, 2009 Physics I Lesson 1Dr J. Tison
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How to…
• Obtain greater accuracy – Minimize systematic errors
• Obtain greater precision – Minimize random errors
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Significant Figures
• Number of directly read + one estimated number– All non-zero digits– Leading zeros not significant– Zeros (a) between non-zero, and (b) at end, if
measured, are significant – Least count:
• Smallest subdivision on the measurement scale
• “Meter stick is calibrated in cm with a millimeter least count
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Significant Figures: Example
• 12.3 cm– # significant figures = 3
• 0.0123cm – # significant figures = 3
• 12.03 cm– # significant figures = 4
• 12.30 cm– # significant figures = 3 or 4?
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Significant Figures in Calculations
• Calculating with Significant Figures– Use the least # significant figures– 12.3 x 1.2 = 14.76 = 15
• there are 2 s.f. in 1.2
– 12.3 x 1.20 = 14.76 = 14.8• There are 3 s.f. in 1.20 and 12
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Significant Figures in Calculations
• Calculating with Significant Figures– Use the least # significant figures– 12.3 x 1.2 = 14.76 = 15
• there are 2 s.f. in 1.2
– 12.3 x 1.20 = 14.76 = 14.8• There are 3 s.f. in 1.20 and 12
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Scientific Notation
• Powers of 10 – Usually expressed as 1 digit to left of decimal
point– 1,234.0 = 1.234 ∙ 103 – Alternative notation
• Doesn’t require superscripts (simplifies typing)• 1,234.0 = 1.234E3
• Scientific calculator display
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Scientific Notation
Speed of light: – 186,282 mi/s → 1.86282 ∙ 105 mi/s– 299,792,458 m/s → 2.99792458 ∙ 108 m/s
Gravitational constant– Standard format: 0.0000000000667300 m3 kg-
1 s-2
– Scientific notation: 6.67300 ∙ 10-11 m3 kg-1 s-2
–
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Computations in Powers of 10
• Adding/subtracting– All values must be have same “power of ten”
• Multiplying/dividing– Write each number in scientific notation, i.e. x.yz ∙ 10a– Multiply the numbers as standard numbers– Add/subtract the exponents for the “power of ten
term”• 12.3 x 123.0 = • (1.23 ∙ 101) x (1.23 ∙ 102) = • 5.129 ∙ 103 = 5.129E3
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Powers of Ten Prefixes
10-24 to 1024
• See names Table 1-4
• Most common – 10-12 pico – 109 giga– 10-9 nano-– 103 kilo– 106 mega
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Order of Magnitude
Estimate value to approx. “Power of Ten”– Order of Magnitude (OM) of 100 is 102– ≈ is mathematical operator meaning “roughly”
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Dimensions, Dimensional Analysis
Convenient way to • Verify proper mathematical relationships• Check correctness of calculations• Make sure all terms to be added or subtracted
have same ‘units of measure’
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Lesson 1: Summary
• Scientific Discovery– Models, Theories, Laws, Principles
• Physical Quantities– Undefinables, standards, SI
• Mass, Length, Time, Temperature, etc– Definables
• Velocity, Acceleration, Force, Momentum, etc– Systems of Units
• MKS• CGS• British
September 8, 2009 Physics I Lesson 1Dr J. Tison
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Lesson 1: Summary
• Measurements– Accuracy and Precision– Uncertainty
• Random and Statistical Errors• Determinant and indeterminate• % Uncertainty
– Significant Figures• Calculators and reported values
• Calculations– Scientific Notation
• Powers of 10
– Order of Magnitude (OM)– Dimensional Analysis