Uniform Circular Motion – Centripetal Force Uniform circular motion –acc7 Uniform circular motion Orbital motion 2 Synchronous orbits 2 Kepler’s Law of Planetary Motion Prob 5.32 For M = mass of the Sun, the relation between r3 and T2 is called Kepler’s Law of Planetary Motion. Note: Planetary Motion Prob 5.32 The planets actually sweep out elliptical orbits such that the speed increases when r is small (“perihelion” for smallest r) and decreases when r is large (“aphelion” for largest r). Note: Planetary Motion Prob 5.32 Kepler’s 2nd Law: The planets sweep out equal areas in equal times. NOTE: We will generally make the approximation that the planetary orbits are circular (ellipses of small “eccentricity”). Prob 5.32 a Prob 5.33 m = 5850 kg R = 4.15x106 m r = 4.1x105 m + 4.15x106 m = 4.56x106 m T = 7200s Prob 5.33 In orbit: On the planet’s surface: We are looking for mgp but we don’t know the planet’s mass, Mp (in order to make use of the 2nd equation on planet’s surface) . m = 5850 kg R = 4.15x106 m r = 4.1x105 m + 4.15x106 m = 4.56x106 m T = 7200s Prob 5.33 In orbit: On the planet’s surface: We can use the 1st equation (orbit) to find Mp . PROBLEM: We don’t know the satellite’s orbital speed, v . m = 5850 kg R = 4.15x106 m r = 4.1x105 m + 4.15x106 m = 4.56x106 m T = 7200s Prob 5.33 In orbit: We DO know the satellite’s orbital speed, v ! Prob 5.33 In orbit: Combine the two boxes on the right: (We’ve re-derived Kepler’s Law!) Prob 5.33 In orbit: On the planet’s surface: Combine the two boxes on the right: Prob 5.33 So, the weight of the satellite is given by: m = 5850 kg R = 4.15x106 m r = 4.1x105 m + 4.15x106 m = 4.56x106 m T = 7200s → mgp = 2.45 x 104 N (gp = 4.2 m/s2 ) Question b Uniform circular motion Apparent weightlessness Apparent weightlessness Artificial gravity NOTE: it’s the normal force exerted by the inner (“floor”) surface of the spaceship which acts on the person to provide a centripetal acceleration. Artificial gravity 2 Artificial gravity What about friction? What about friction? Consider the rotation “starting up”. Artificial gravity From (a) to (b), the person’s speed in the x (“tangential”) direction is changing. This is an acceleration and requires a tangential force – static friction! At (c), the person’s speed is constant, with uniform motion in the tangential direction. No tangential force is required. Prob 5.28 b Uniform circular motion Vertical circular motion Vertical circular motion Vertical circular motion Prob 5.40 a Chapter 6 Work and Energy Work and Energy We define a new kinematic quantity: Kinetic Energy. A moving object of mass m has a kinetic energy: KE = ½mv2 The SI unit of kinetic energy is the Joule (J) 1J = 1kg.m2/s2 Work and Energy Work and Energy 0 We can change the state of motion of an object (change v) by applying a net force: We say that the force “does work” on the object to change its kinetic energy from an initial value: KE0 = ½mv02 to a final value: KE = ½mv2 Work and Energy Work and Energy 1 Using a kinematic equation: v2 - v02 = 2ax mv2 - mv02 = 2max ½mv2 - ½mv02 = Fx KE – KE0 = Fx Work and Energy Work and Energy 2 ½mv2 - ½mv02 = Fx KE – KE0 = Fx = W Fx = W is the “work done by the net force, F in displacing the object by x”. W = KE – KE0 = ∆KE “Work - Energy Theorem” (work done by Net Force) (units: Joule J = N.m = 1kg.m2/s2 ) Work and Energy ½mv2 - ½mv02 = KE – KE0 = ∆KE = Fx = W Work and Energy 2.1 Work and Energy Prob 6.10 x If multiple forces are acting on an object, each force can perform work. The change in kinetic energy is determined by the work done by the net force. Work and Energy Only the component of a force in the direction of the displacement counts. Work and Energy 3 For displacement in the x direction, the component of applied force along the displacement is Fx = Fcos Work and Energy Work and Energy 3.1 If is the angle between the applied force and the displacement: W = Fxcos = the work done by the applied force. Work and Energy Prob 6.10 x If multiple forces are acting on an object, each force performs work: Wi = Fi xcos . The change in kinetic energy is determined by the work done by the net force: ∆KE = Fnet xcos
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