Chapter 5 Notes Circular Motion and Gravitation. Chapter 5 5-1 Kinematics of Uniform Circular Motion  Uniform circular motion - An object that moves.

Slides:



Advertisements
Similar presentations
Lecture 16 Chapter 6: Circular Motion Please sit in the first six rows.
Advertisements

Circular Motion and Gravitation
Bellringer 11/12 A worker does 25 J of work lifting a bucket, then sets the bucket back down in the same place. What is the total net work done on the.
Section 5-8: Satellites and “Weightlessness”
If the force exerted by a horse on a cart is equal and opposite to the force exerted by a cart on the horse, as required by Newton’s third law, how does.
Circular Motion Level 1 Physics. What you need to know Objectives Explain the characteristics of uniform circular motion Derive the equation for centripetal.
Apparent Weight Riding in a elevator– why does our weight appear to change when we start up (increase) and slow down (decrease)? Our sensation of weight.
Physics 101: Lecture 11, Pg 1 Physics 101: Lecture 11 Centripetal Force l Brief Review of Chapters 1-4 l Textbook Chapter 5 è Uniform circular motion :
Department of Physics and Applied Physics , F2010, Lecture 10 Physics I LECTURE 10 3/3/10.
Chapter 7 Tangential Speed
Circular Motion and Gravitation
Satellite Motion. Low Orbit  A container falls off the space station while in low earth orbit. It will move A) straight down toward Earth. A) straight.
Physics I Honors Specific Forces Centripetal Force.
Chapter 6: Circular Motion and Gravitation
Newton’s Law of Gravitation. Newton concluded that gravity was a force that acts through even great distances Newton did calculations on the a r of the.
Gravity ISCI More Free Fall Free Fall Vertical and Horizontal Components of Free Fall.
What keeps them in orbit?
Free Fall The acceleration of gravity (g) for objects in free fall at the earth's surface is 9.8 m/s2. Galileo found that all things fall at the same rate.
Ch. 7 (Section 7.3) Circular Motion.
Acceleration is equal to Δv/Δt. Velocity is a vector and there are two ways a vector can be changed: by changing magnitude or by changing direction.
Kepler’s laws, Gravitational attraction, and projectile motion.
Advanced Physics Chapter 5 Circular Motion: Gravitation.
Cutnell/Johnson Physics 7th edition Reading Quiz Questions
ROTATIONAL MOTION Uniform Circular Motion
Important situations in circular motion. When accelerating, the feeling you have is opposite the acceleration This is why it feels like there is centrifugal.
Uniform Circular Motion. Motion in a Circle Revolution: If entire object is moving in a circle around an external point. The earth revolves around the.
Circular Motion. Uniform Circular Motion Motion of an object at constant speed along a circular path.
Centripetal Motion Motion towards the center of a circle.
Uniform Circular Motion. What is uniform circular motion? 4 Movement of an object at constant speed around a circle with a fixed radius 4 Can the velocity.
Chapter 7 Rotational Motion and the Law of Gravity
CIRCULAR MOTION. Path of an object in circular motion: The velocity is tangential The acceleration is directed towards the center (centripetal acceleration)
Circular Motion Chapter 9. Circular Motion Axis – is the straight line around which rotation takes place. Internal Axis - is located within the body of.
7-3 Circular Motion. As an object travels in uniform circular motion Its tangential speed remains constant The direction of its velocity is constantly.
Centripetal Acceleration is a vector quantity because it has both direction and magnitude. Centripetal Acceleration is defined as an acceleration experienced.
Circular motion Objectives: understand that acceleration is present when the magnitude of the velocity, or its direction, or both change; understand that.
CIRCULAR MOTION. WHAT IS UNIFORM CIRCULAR MOTION The motion of an object in a circle at constant speed. However, direction and therefore velocity are.
CHAPTER 5 CIRCULAR MOTION AND GRAVITATION Kinetics of Uniform Circular Motion An object moving in circular motion is in constant acceleration, even if.
Chapter 5 Circular Motion; Gravitation. 1. Use Newton's second law of motion, the universal law of gravitation, and the concept of centripetal acceleration.
Uniform Circular Motion. Acceleration When an object moves at a constant speed in a circular path, it is constantly changing direction – accelerating.
Circular Motion Section 7.3
Circular Motion. PhET Lady Bug Motion Think about this Click “Show Both” at the top, and “Circular” at the bottom Watch the following and comment: Which.
Conceptual Physics Notes on Chapter 9 CircularMotion.
Newton’s Second Law of Motion. Newton’s Second Law Newton’s Second Law of Motion- Acceleration depends on the objects mass and the net force acting on.
Law of universal Gravitation Section The force of gravity: All objects accelerate towards the earth. Thus the earth exerts a force on these.
Chapter Uniform Circular Motion  Uniform circular motion is the motion of an object traveling at a constant (uniform) speed on a circular path.
Circular Motion; Gravitation
Sect. 5-2: Uniform Circular Motion. The motion of a mass in a circle at a constant speed. Constant speed  The Magnitude (size) of the velocity vector.
Satellites & “Weightlessness”. “Weightlessness” What keeps a satellite in orbit? The centripetal acceleration is CAUSED by the Gravitational Force! F.
Dynamics of Uniform Circular Motion Uniform Circular Motion Centripetal Acceleration Centripetal Force Satellites in Circular Orbits Vertical Circular.
Circular Motion Centripetal Force Apparent Weight Newtons’ Universal Gravitation Law.
Chapter 9 Circular Motion. Axis – Central point around which rotation occurs (axis) (fulcrum) Rotation – occurs when an object turns about an internal.
Chapter 5 Circular Motion; Gravitation. 5-1 Kinematics of Uniform Circular Motion Uniform circular motion: motion in a circle of constant radius at constant.
Circular Motion: Gravitation Chapter Kinematics of Uniform Circular Motion  Uniform circular motion is when an object moves in a circle at constant.
1. A physics teacher twirls a roll of masking tape in a 2.2 m radius vertical circle. What is the minimum velocity at the top of the circle that will keep.
Uniform circular motion and Universal Gravitation
SENIOR HIGH SCHOOL 1 SLAWI SUBJECT: PHYSIC GRADE: XI SEMESTER: 1/ WRITTEN BY: SETYANINGSIH, SPd NIP:
Circular Motion Lecture 08: l Uniform Circular Motion è Centripetal Acceleration è More Dynamics Problems l Circular Motion with Angular Acceleration è.
Circular Motion Chapter 7.3. Motion & Forces What you already know: –Velocity – a measure of the change in displacement (distance with direction. –Mass.
Do Now Which of the following objects is accelerating: a. A car slowing down. b. A free fall object momentarily stopped at its max height. c. A ball tied.
Rockets and Satellites. How Do Rockets Lift Off? Rockets and space shuttles lift into space using Newton’s third law of motion.
Sect. 6-4 Satellites and “Weightlessness”. Satellites are routinely put into orbit around the Earth. The tangential speed must be high enough so that.
Uniform Circular Motion. 4 dXxQ7o dXxQ7o.
Circular Motion and the Law of Universal Gravitation.
Section 2 Newton’s Law of Universal Gravitation
Weightlessness.
Circular Motion and Gravitation
Chapter 7 Objective Solve problems involving centripetal acceleration.
Rockets and Satellites
Weightlessness.
Chapter 2 Astronomy.
Presentation transcript:

Chapter 5 Notes Circular Motion and Gravitation

Chapter Kinematics of Uniform Circular Motion  Uniform circular motion - An object that moves in a circle at a constant speed (v).  The magnitude of the velocity remains constant, but the direction of the velocity is constantly changing.  Acceleration = change in velocity / change in time  Object revolving in a circle is continuously accelerating

Chapter 5 Review of centripetal acceleration  pg. 113 Fig 5-1 & 5-2  Velocity points tangent to circle  Change in velocity - points to center of circle  Centripetal acceleration - “center seeking” acceleration  Centripetal acceleration = a r

Chapter 5 a r = v 2 /r  An object moving in a circle of radius r with a constant speed v has an acceleration whose direction is toward the center of the circle and whose magnitude is a r = v 2 /r.  Velocity and acceleration vectors are perpendicular to each other at every point in the path for uniform circular motion.

Chapter 5  Frequency (f) - number of revolutions per second  Period (T) - time required to complete one revolution  T = 1/f  For an object revolving in a circle at constant speed v: v=2  r/T  Example 5-1 & 5-2

Chapter Dynamics of Uniform Circular Motion  Newton F=ma  Object moving in a circle must be acted on by a force  F r =ma r =mv 2 /r  Net force must be directed toward the center of the circle.  Centripetal force - force directed towards center of circle

Chapter 5 Centrifugal force vs. centripetal force  pg. 116 Read Paragraph out loud  Examples 5-3,4,5 & 6 pg

Chapter Satellites and Weightlessness  Satellite - put into circular orbit by accelerating tangentially using rockets  too fast - gravity will not confine it  too slow - gravity will cause it to fall back to earth

Chapter 5 What keeps a satellite in space?  High speed, if it stopped moving it would fall to earth  Satellite is falling, but high tangential speed keeps it from falling to earth

Chapter 5  satellite acceleration = a r = v 2 /r  force accelerating object is earth’s gravity  F= ma r  Gmm E /r 2 = mv 2 /r m = mass satellitem = mass satellite r = r E + height satellite r = r E + height satellite  Example 5-15 pg. 130

Chapter 5 Weightlessness  elevator - rest   F= ma W-mg=0 W=mg  for acceleration upward = positive  accelerate upward at a :  F= ma W-mg = ma W=ma +mg  downward a is negative, W is less than mg

Chapter 5 Weightlessness (cont.)  upward a=1/2g W=3/2mg experience 3/2 g’s acceleration  downward a=-1/2g W=1/2mg experience 1/2g acceleration  if downward acceleration = free fall = g  W=mg-ma W=mg-mg=0  therefore, you feel weightless - “apparent weightlessness”  Apparent weightlessness on earth - ski jump, trampoline

Chapter 5  Satellites fall toward earth, only force acting on it is gravity  Out in space far from the earth - true weightlessness occurs  gravity pull from other planets is extremely small due to large distances away  Prolonged weightlessness - red blood cells diminish, bones lose calcium and become brittle, muscles lose their tone.