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PHY/EGR 321.001

PHY/EGR 321.001. Spring 2008. Harry D. Downing. Professor and Chair Department of Physics and Astronomy. Roll Call. Fill out Student Information Sheets Pass out syllabi then go to next slide Take pictures of each student in lab today. Let’s visit the web for course information.

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PHY/EGR 321.001

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  1. PHY/EGR 321.001 Spring 2008 Harry D. Downing Professor and Chair Department of Physics and Astronomy

  2. Roll Call Fill out Student Information Sheets Pass out syllabi then go to next slide Take pictures of each student in lab today

  3. Let’s visit the webfor course information. Downing’s PHY/EGR 321 Home Page physics.sfasu.edu

  4. Homework Format

  5. Cover Page Staple at 450 NAME PHY/EGR 321.001 Date Problems Grade

  6. Cover Page,Example Staple at 450 Harry Downing PHY/EGR 321.001 1-16-08 Ch 11 – 2, 6, 9, 16 Grade 5, 4, 5, 3 Pass out some example engineering pad paper

  7. CHAPTER 11 Kinematics of Particles

  8. 11.1 INTRODUCTION TO DYNAMICS • Galileo and Newton (Galileo’s experiments led to Newton’s laws) • Kinematics – study of motion • Kinetics – the study of what causes changes in motion • Dynamics is composed of kinematics and kinetics

  9. RECTILINEAR MOTION OF PARTICLES

  10. 11.2 POSITION, VELOCITY, AND ACCELERATION For linear motion x marks the position of an object. Position units would be m, ft, etc. Average velocity is Velocity units would be in m/s, ft/s, etc. The instantaneous velocity is

  11. The average acceleration is The units of acceleration would be m/s2, ft/s2, etc. The instantaneous acceleration is

  12. Notice If v is a function of x, then One more derivative

  13. 32 16 0 6 2 4 12 0 4 6 2 -12 -24 -36 12 4 6 2 0 -12 -24 Plotted Consider the function x(m) t(s) v(m/s) t(s) a(m/s2) t(s)

  14. 11.3 DETERMINATION OF THEMOTION OF A PARTICLE Three common classes of motion

  15. with then get

  16. Both can lead to or

  17. Work Some Example Problems

  18. 11.4 UNIFORM RECTILINEARMOTION

  19. 11.5 UNIFORMLY ACCELERATEDRECTILINEAR MOTION Also

  20. 11.6 MOTION OF SEVERAL PARTICLES When independent particles move along the same line, independent equations exist for each. Then one should use the same origin and time.

  21. Relative motion of two particles. The relative position of B with respect to A The relative velocity of B with respect to A

  22. The relative acceleration of B with respect to A

  23. Let’s look at some dependent motions.

  24. xA xB A E F B G C D Let’s look at the relationships. System has one degree of freedom since only one coordinate can be chosen independently.

  25. xC xA xB C A B System has 2 degrees of freedom. Let’s look at the relationships.

  26. Work Some Example Problems

  27. 11.7 GRAPHICAL SOLUTIONS OF RECTILINEAR-MOTION • Skip this section.

  28. 11.8 OTHER GRAPHICAL METHODS • Skip this section.

  29. y x z CURVILINEAR MOTION OF PARTICLES 11.9 POSITION VECTOR, VELOCITY, AND ACCELERATION P’ P Let’s find the instantaneous velocity.

  30. y y x x z z P’ P

  31. y y y x x x z z z P’ Note that the acceleration is not necessarily along the direction of the velocity. P

  32. 11.10 DERIVATIVES OF VECTOR FUNCTIONS

  33. Rate of Change of a Vector The rate of change of a vector is the same with respect to a fixed frame and with respect to a frame in translation.

  34. 11.11 RECTANGULAR COMPONENTS OF VELOCITY AND ACCELERATION

  35. y x z y P x z

  36. y x z

  37. Velocity Components in Projectile Motion

  38. y y’ x x’ z z’ 11.12 MOTION RELATIVE TO A FRAME IN TRANSLATION B A O

  39. Work Some Example Problems

  40. 11.13 TANGENTIAL AND NORMAL COMPONENTS Velocity is tangent to the path of a particle. Acceleration is not necessarily in the same direction. It is often convenient to express the acceleration in terms of components tangent and normal to the path of the particle.

  41. y x O Plane Motion of a Particle P’ P

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