Physics 231 Topic 1: Introduction, Units, Significant Figures Alex Brown September 2, 2015 MSU Physics 231 Fall 2015 1 Today's Lecture: Key Concepts Syllabus International System of Units (SI) Mass: kilograms (kg) Length: meters (m) Time: seconds (s) Units and conversions Dimensional Analysis Scientific Notation (e.g., 4.3x1012 and 2.3E4) Significant Figures Covers chapter 1 in Rex & Wolfson MSU Physics 231 Fall 2015 2 Textbook & Reading Essential College Physics, Volume 1 • The syllabus lists the relevant chapters for each lecture and homework • Read the material before class • Not everything can be covered in class • Lectures are not a replacement for the textbook MSU Physics 231 Fall 2015 3 MSU Physics 231 Fall 2015 4 MSU Physics 231 Fall 2015 5 MSU Physics 231 Fall 2015 6 MSU Physics 231 Fall 2015 7 MSU Physics 231 Fall 2015 8 MSU Physics 231 Fall 2015 9 Homework Homework is to be done online using LON-CAPA http://msu.lon-capa.org Homework assignments are due Tuesdays at 10 PM The deadline is strict. Being away from a network connection is no excuse. Do not wait until the last minute! Assignments are somewhat unique to each student Discussion board You are encouraged to use the discussion board inside LON-CAPA. If you don't understand a problem, or you need help, just click on the "Post Discussion" link and post your question. If you know the answer to somebody else's question, don't be afraid to post you answer. Don't forget: The best way to learn is to teach. But – to do well in the exams you should try the problem on your own first, and if you use the discussion board, be sure you understand the concepts and the reasoning behind the solution. MSU Physics 231 Fall 2015 10 Extra Credit Quizzes We will be doing in-class quizzes using i>Clickers Quizzes will be given almost everyday You must have in i>Clicker to participate Start to count them on Monday September 14th Be on time, quizzes are sometimes at the beginning of class. There are NO make-ups for quizzes all of the points are for extra credit You must take quizzes in this section. No credit for quizzes in other sections. Quiz points: 3 for correct answers, 1 for incorrect answers Scores will be posted on my website occasionally – check to ensure you're registered You must register your i<Clicker on lon-capa before Monday September 14th Even if you have registered before, you need to re-register for this course! You MUST enter the preceding “A” before your student ID MSU Physics 231 Fall 2015 11 Extra Credit Quizzes You must use your own and ONLY your own i>Clicker in class If you are found to be using another person's i>Clicker, all clickers will be confiscated This will be considered a violation of the rules governing academic dishonesty MSU Physics 231 Fall 2015 12 MSU Physics 231 Fall 2015 13 MSU Physics 231 Fall 2015 14 Information and links Lecture ppt and pdf Grade updates MSU Physics 231 Fall 2015 15 Physics Learning Center (PLC) The Strosacker Physics Learning Center is located in BPS 1248 Details and schedule TBA The PLC is a cooperative learning center, not a help room. TAs will encourage group work and will help groups who get stuck. Group work A very effective learning tool for both strong and weak students You must do your own assignments and must learn how to do problems on your own Do as much as you can of the assignments before group work – PREPARE! MSU Physics 231 Fall 2015 16 How to Suceed in PHY231 Read the book before coming to class. Go to the Physics Learning Center frequently! The TAs are there to help you learn. Always attend the lectures. Recognize that learning physics is different than many other subjects Physics is about understanding concepts and connecting your knowledge with these concepts. Physics is not just about memorizing facts. Some physics concepts will be contrary to your instincts, but not contrary to your intellect. Be willing to think things through! Keep working continuously – do the reading assignments, think about what you learned in lecture, keep thinking AS WE GO. Memorizing facts is not sufficient, so cramming before an exam is not effective. Understanding the concepts helps you set up solutions to problems. Equation hunting is not a good strategy. Little is learned by copying or memorizing the solution of another student. MSU Physics 231 Fall 2015 17 DOs and DON'Ts DON'T... ...use LON-CAPA postings from others before you have given a problem a genuine attempt yourself. If you have to frequently look at how others solved the problem, it means you aren't understanding the material well. ...try to memorize LON-CAPA problems; it is unlikely that you will get many problems in exams that are exactly like the homework ...base your entire study routine on LON-CAPA. Bring variation in your studies and practice questions that are not phrased like LON-CAPA (eg, questions in the book) ...wait until the last weeks of the semester to ask for help if you need it (ie, if you're working hard but still are not doing well) ...cheat on exams, quizzes, homework MSU Physics 231 Fall 2015 18 DOs and DON'Ts DON'T... …use your cell phone in class. MSU Physics 231 Fall 2015 19 Why Learn Physics? Example: Tacoma Narrows Bridge Golden Gate BronxWhiteStone Tacoma Narrows Year 1937 1939 1940 Cost $35M $20M $6.4M Length 4200 ft 2300 ft 2800 ft Width 90 ft 74 ft 39 ft Ratio: Width to Length 1 : 47 1 : 31 1 : 72 MSU Physics 231 Fall 2015 20 Why Learn Physics? Example: Mechanics of the Skeleton Key concept for: • Human medicine • Veterinary medicine • Sports training • Ergonomic engineering In other classes, you learn the names of bones, how to treat broken bones, where to drill to replace things. Physics teaches you HOW and WHY it works (and how to understand the system as a whole) Combination is the key to innovation! MSU Physics 231 Fall 2015 21 Why Learn Physics? Example: Dark Matter & Dark Energy Bullet Cluster • Cosmological measurements have told us that our universe is not made the way we thought. • IE, what we see in telescopes corresponds to what we are all made out of: atoms (stars, gases, planets) MSU Physics 231 Fall 2015 22 Why Learn Physics? Example: Dark Matter & Dark Energy • Cosmological measurements have told us that our universe is not made the way we thought. Bullet Cluster • IE, what we see in telescopes corresponds to what we are all made out of: atoms (stars, gases, planets) • But this is only 4% of what’s out there! MSU Physics 231 Fall 2015 23 Système Internationale (SI) Units (ones used for this course) Unit meter kilogram second Kelvin mole (others) ampere candela Abbreviation m kg s K mol A cd Base unit for length mass time temperature amount of substance electric current luminous intensity Also called the MKS unit system Based on powers of 10 relative to base units All other units derive from these (Area: m2, Speed: m/s, etc) MSU Physics 231 Fall 2015 24 Defining Standard Units Original definition of the meter: 1/10,000,000 of earth's arc length Today: 1m = distance light travels in 1/299,272,458 s MSU Physics 231 Fall 2015 25 Defining Standard Units Platinum-Iridium Kilogram Prototype The kilogram defined by a fixed “prototype” of matter Standards are important: when you buy 1kg of gold, you want to get it right! MSU Physics 231 Fall 2015 26 Defining Standard Units Cesium Atomic Clock National Institute of Standards and Technology (NIST) Original definition of the second: 1/86,400 of a solar day 1960: based on a tropical year Since 1967: 9,192,631,770 periods of radiation corresponding to the transition between two hyperfine states of the ground state of 133Cesium MSU Physics 231 Fall 2015 27 Unit Conversion Example Treat conversions as algebraic equivalencies: Convert by multiplying your existing units by a numerical equivalent of 1.0 Jon has walked 3 miles in 1 hour, what is his average speed in m/s? Given: 1 mile = 1609.3 m ie, 1.0 = ( 1609.3 m/ 1 mile ) Velocity (speed) = distance / time = ( 3 miles ) / ( 1 hour ) Equal to 1.0 = ( 3 miles/hr ) x ( 1609.3 m / mile ) = 4827.9 m/hr = ( 4827.9 m/hr ) x (1 hr / 60 min) x (1 min / 60 sec) = ( 4827.9 m/hr ) x (1 hr / 3600 s) = ( 4827.9/3600 ) m/s = 1.341 m/s MSU Physics 231 Fall 2015 28 A Wide Range of Units MSU Physics 231 Fall 2015 29 Very Large and Very Small Numbers 0.000000000000001 = 10-15 = 1E-15 femto (f) 0.000000000001 = 10-12 = 1E-12 pico (p) 0.000000001 = 10-9 = 1E-9 nano (n) 0.000001 = 10-6 = 1E-6 micro () 0.001 = 10-3 = 1E-3 milli (m) 0.01 = 10-2 = 1E-2 centi (c) 0.1 = 10-1 = 1E-1 deci (d) 1 = 100 = 1E+0 10 = 101 = 1E+1 deca (da) 100 = 102 = 1E+2 hecto (h) 1000 = 103 = 1E+3 kilo (k) 1000000 = 106 = 1E+6 mega (M) 1000000000 = 109 = 1E+9 giga (G) 10000000000 = 1012 = 1E+12 tera (T) MSU Physics 231 Fall 2015 30 Scientific Notation For very large or very small numbers the scientific notation is advantageous. Write number as mantissa x 10Exponent Example: 0.000000001 = 1 × 10-9 34000000 = 3.4 × 107 Alternative notation: 3.4E7 (CAPA, computers) 1 m = 1000 mm = 1E3 mm MSU Physics 231 Fall 2015 31 MSU Physics 231 Fall 2015 32 Significant Figures MSU Physics 231 Fall 2015 33 Significant Figures Two statements: The population of the USA is 294,109,799 The population of the USA is 294,000,000=2.94×108 First statement implies precision that is probably not warranted Second statement claims that the population is somewhere between 293M and 295M. This is reasonable! General Rules: The number of digits we write down in a number specifies the precision with which we can claim to know the number All non-zero figures are signficant (except exponent in scientific notation) Zeros only count when They are between non-zero figures They are to the right of a non-zero figure and there is a decimal point MSU Physics 231 Fall 2015 34 Significant Figures Example An athlete must bicycle around a circular track for a time trial. His coach tells him that the radius of the circular track is 40.2 m. How far does he ride? Formulae: C = π D = 2 π R D = diameter of the circle R = radius of the circle π = 3.14159265..... We know π to many decimal places, but we only know the radius is between 40.2 and 40.3 m (ie, 3 significant figures). Thus we can only know the circumference to 3 significant figures! What is the answer? C = 2 × 3.14159265... × 40.2 m = 253 m MSU Physics 231 Fall 2015 35 How to Solve Problems There are no general rules but here are some pointers: 1) READ the problem carefully! 2) Summarize (throw away unnecessary info) 3) Visualize (drawing can often help) 4) Convert units (consistency) 5) Set up equations: Plug in numbers if not comfortable with solving sets of equations If confident, plug in numbers at last moment 6) Check whether answers (and units) make sense 7) In exams: once you have solved a problem, check calculations one more time at the end of exam. Especially important if you tend to make small mistakes MSU Physics 231 Fall 2015 36 Greek Alphabet We will use some of those… MSU Physics 231 Fall 2015 37 2D Geometrical Objects object surface circumference square Length2 4xlength triangle ½x base x height Side1+side2+side3 circle x radius2 2 x x radius Radius=diameter/2 rectangle Length x height 2xlength + 2xheight oval xr1xr2 - MSU Physics 231 Fall 2015 38 3D Geometrical Objects object surface volume 6xlength2 length3 2hw+2lh+2wh hlw sphere 4r2 (4/3) x r3 cylinder 2rh r2h cube rectangle MSU Physics 231 Fall 2015 39 Solving Quadratic Equations ax 2 bx c 0 a0 b b 2 4ac x 2a In general there are 2 solutions. In physics problems, One of them is usually not realistic and is thrown out. MSU Physics 231 Fall 2015 40 Calculate the length of the shorter of two sides of a rectangle, which has an area of A = 24 m2 and a perimeter of p = 22 m. Example of two equations and two unknowns. h A = wh p = 2w+2h 24 = wh so w = 24/h 22 = 2w + 2h = (2x24/h) + 2h = (48/h) + 2h w -2h2 + 22h - 48 = 0 22 22 4(2)( 48) 22 10 h 2(2) 4 h 8 or 3 w 3 or 8 2 MSU Physics 231 Fall 2015 ax 2 bx c 0 a0 b b 2 4ac x 2a 41 Dimensional Analysis Dimensions should be treated as algebraic quantities If you know the dimensions you want in the end of a calculation, it helps you plan your work and check your math Example: Calculate the distance traveled in 10 seconds by an object starting at rest and traveling at constant acceleration Given : x = (1/2) a t2 What are the units for a (acceleration)? Rearrange to get units for a: [?] = [m] / [s2] )= m/s2 [m] = [?] [s2] Units of acceleration go here Check your math: [m] = [m/s2] [s2] = [m] MSU Physics 231 Fall 2015 42