Honors Physics Mr. Fedell Chapter 5 Notes – Circular Motion; Gravitation (Student edition) Chapter 5 Questions: 4, 5, 7, 8, 13, 14, 20, 24 Problems: 1, 2, 4, 9, 11, 17, 22, 24, 25, 28, 29, 30, 43, 56, 57, Useful figures: Every single figure and example has something that you can learn from in this chapter. 5.1/5.2 Kinematics/Dynamics of Uniform Circular Motion – the motion of an object traveling at a constant speed on a circular path; magnitude of the velocity is constant while the direction is always changing Tangential Velocity The velocity vector is said to branch from the circular path following a ___________ Magnitude: a) The speed of an object in linear motion uses the formula: π£= π·ππ π‘ππππ (π) ππππ (π ) While… b) Circular motion and speed of an object uses: π£= π·ππ π‘ππππ (π) πΆππππ’ππππππππ (π) 2ο°π = = ππππ (π ) ππππππ (π ) π Period (T) – the time it takes an object to travel the length of the ____________________ Unit: Example #1: A Tire-Balancing Machine The wheel of a car has a radius of r = 0.30 m and is being rotated at 830 revolutions per minute (rpm) on a tire-balancing machine. Determine the speed (in m/s) at which the outer edge of the wheel is moving. Determine the speed halfway to the outer edge (r = 0.15 m) 1 Direction Newton’s First Law: If there is any change in the velocity vector (direction or magnitude) it is due to a ; with circular motion we call this the _______________________ Newton’s Second Law: F = ma; with every force comes an acceleration. With circular motion we use the term acceleration Centripetal (Radial) Acceleration – comes from Latin meaning “center-seeking” Magnitude: An object moving with a speed v on a circular path of radius r has a magnitude ar given by ππ = π£2 π Direction: The vector always points toward the center of the circle and continually changes _____________________as the object moves The linear and centripetal acceleration of an object are related via: Example #2: The Effect of Radius on Centripetal Acceleration The bobsled track at the 1994 Olympics in Lillehammer, Norway, contained turns with radii of 33 m and 24 m. Find the centripetal acceleration at each turn for a speed of 34 m/s, a speed that was achieved in the event. Express the answer in multiples of g = 9.8 m/s 2. 2 The centripetal acceleration vector is inversely proportional to the radius only when v is constant, so… _____ Radius _____ Centripetal acceleration Centripetal Force Magnitude: The force required to keep an object of mass m, moving at a speed v, on a circular path of radius r, and it has a magnitude of πΉπ = π Direction: Always points towards the π£2 π of the circle and continually direction *Important – centripetal force is not a “new” or separate force we must account for, it is the sum of all forces acting on an object pointing towards the center of the circular path* Example #3: The Effect of Speed on Centripetal Force The model airplane from the beginning of our notes we find has a mass of 0.90 kg and moves at a constant speed on a horizontal circular path. Attached to the airplane is a guideline which is taut and allows the plane to follow a circular path. Find the tension T in the guideline (length = 17 m) for speeds of 19 m/s and 38 m/s. *Speed and centripetal force have a direct relationship which indicates as speed ______ centripetal force ______* 5.3 Highway Curves, Banked and Unbanked 3 Circular Motion in the Real-World When you go around a bend in a car you feel as though you are “pushed” into the car door, and this is sometimes referred to as centrifugal force *Centrifugal force is not a real force; it means “_______________” and is incorrect since there is no outward force* Forces acting on the car passenger: Unbanked Curves The force acting on the passenger from the door comes from the car; on unbanked curves, this comes solely from frictional forces made between the __________ and __________ Forces acting on the car: When the wheel is rolling without slipping the road exerts ____________ friction force; when skidding, ____________ friction forces are present. Mr. Fedell’s… why you should buy a car with antilock brakes Example #4: Centripetal Force and Safe Driving What is the maximum speed a car can safely negotiate an unbanked turn with (r = 51m) in dry weather (coefficient of static friction = 0.95) and icy weather (coefficient of static friction = 0.10)? 4 Banked Curves Putting a bank on a curve can reduce tire slippage; the normal force of the vehicle acts to supplement the static friction force exerted on the tires. The angle of a bank can be made such that no friction is required for the car to stay on the road at a certain speed. It is possible to find the angle of the roadway which requires no frictional force at a certain speed. The angle can be found using: π£2 π‘ππ π = ππ Example #5: At the Daytona 500 the track has a radius of r = 316 m and are banked steeply, with θ = 31Μ . Suppose these turns were frictionless. At what speed would the cars have to travel around them? Newton’s Law of Universal Acceleration Newton realized that gravity worked over a distance (the apple?), he proposed that gravity worked over large distances, even from the __________________________________. He proposed his famous law of _________________________________ The direction is toward the two objects. What does this mean? 1. The force never dies out. Every body in the universe feels gravity from every other body in the universe. 2. The larger the ___________, the stronger the _________. 3. The force between two objects is the same (_____________________). The accelerations are different due to their different masses. 4. If the mass of an object doubles, the ______________________. 5. If the distance between two objects is doubled, the force is cut to one quarter of its value. The value of G is G = 6.67 ο΄ο 10-11 N-m2/kg2 We can measure the distance from the center of an object when the object is spherical. 5 Example #6: What is the gravitational force on the moon from the earth? mearth = 6 x 1024 kg mmoon = 7.3x 1022 kg, r = 3.84 x 105 km = is 3.84 x 108 m F = 1.98 x 1020 N This force is a vector, as are all forces, and must be added vectorially, by components. Example #7: What is the magnitude of gravitational force that acts on each particle placed horizontally and at a distance of 1.2 m from each other. The mass of the particles are 12 kg and 25 kg. Gravity Near the Earth What is force of gravity near the surface of the earth? If I am standing on the earth, we have said that the force is mg. That must come from Newton’s law of universal gravitation. Let’s see, how this works. I need to take the distance from the center of the earth when I am standing on the surface of the earth. πΊπππΈ πΉ = ππ = π2 πΊππΈ π= π2 = (6.67 ο΄ο 10-11 N-m2/kg2)(5.97 ο΄ο 1024kg)/(6.38 ο΄ο 106 m)2 = 9.78 m/s2 Example #8: How far above the earth must I go for the force I feel to be 1/2 of what is on the surface of the earth? Large objects near us influence what we perceive as the acceleration of gravity. Near a mountain, there is mass pulling us toward the mountain. Most of the mass is still underneath us, so the difference is very small, but it is there. Also if you go to higher elevations, you are farther from the center of the earth so g goes down very slightly, as well. 6