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Objectives Describe and define • Work • Energy • Power • Efficiency Mechanics 7 Work, Energy and Power IFP Friday 13th November 2015 Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Objectives Work • What do you already know? • Some key stuff to note down… Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Work Work is done by a force when the force moves its point of application in the direction of the force. e.g. by lifting a weight, one does work Work produced by a force on an object is proportional to the strength of the force and proportional to the distance travelled by the object in the direction of the force. (more simply: W = Fd) Unit of work is the joule (J): this is the work done when a force of 1 N moves its point of application through 1 metre in the direction of the force. Objectives F and S at an angle? • W = Fs cosθ • Work done = force x distance travelled in the direction of the force • Although a scalar, work has a sign! Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Objectives What about a variable force? • Work done is just the area under the graph. • You could just count the squares, or use integration to calculate it. • You won’t be asked to in this course! Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Objectives Energy • What is it? • What can it do? Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words • What forms are there? Put them on the board Objectives Energy • What is it? the capacity to do work. • What can it do? moves things, heat things up, cool them down, make light, make noise, break things, power our electronics etc… Examples of Energy Transfers Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Objectives Kinetic energy Energy of motion: • Ek = ½ m v2 1 J = 1 joule = 1 kg (ms-1)2 =1 kg m2 s-2 Simple example a mass of 1 kg moves at 2 ms-1. Ek= ½ (1 kg) (2 ms-1)2 =2 J Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Objectives Potential energy Potential energy is “stored” energy resulting from any force which depends only on position e.g. gravity, force in a spring, electrostatic attraction/repulsion Gravitational potential energy is only one form of potential energy: It arises from height in a gravitational field Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Objectives Potential Energy • • • • Ep = m g h h: height above the origin level. The origin (h=0) can be freely chosen. Potential energy is always relative to some reference level or position e.g. a 1 kg mass is held 20m above the ground. What is its gravitational potential energy relative to the ground? • U = 1kg 9.8 ms-2 20m= 196 J Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Objectives Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Conservation of energy It’s a Very important principle Has nothing to do with the answer: :“the law of conservation of energy is a law passed by the government to tell us to save energy” (student in a test) • In an isolated system the total energy is conserved. • Isolated system: one where there is no energy transfer into or out of the system. • Energy can only be transformed from one form to the other. • Energy cannot be created or destroyed. • Examples of energy transfers? Power • Power is the rate at which energy is used, or similarly the rate at which a force does work on an object. • power = • • • • energy transferred time taken average: P = ΔW/ Δt, or at a given time: P= dW/dt Units watts(W): 1 watt = 1 joule per second Also horsepower (hp) : 1 hp = 745.6 W Objectives Power We can relate power, force and speed: • P = dW/dt = d (F s cosθ)/dt • for fixed F (both magnitude and angle) • P = F ds/dt cosθ = F v cos θ • or P = F v Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Objectives Efficiency • In many cases (machines) energy is transformed from one form to the other but in the process there is a waste of energy. • E.g. friction in a machine or resistance in wires of electric motors waste energy. • Notion of efficiency of a machine: • Efficiency = useful power delivered /total power supplied (often a %) Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Objectives Examples Example 1 A 500 kg rock slides from rest down a hill 500m long and 300m high. The coefficient of kinetic friction between the rock and the hill is μ=0.25. If the gravitational potential energy is set to 0 at the bottom of the hill, (a) What is the rock’s potential energy just before the slide? (b) How much work is done by the frictional force during the slide? (c) What is the kinetic energy and the speed of the rock when it reaches the bottom of the hill? Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Problem 1 Solution – on handout! • Tricky problem. • Principles… 1. 2. 3. 4. Ep = mgh. This is easy, =1.47 MJ Work done = force * distance moved Force = reaction force * friction coeff Reaction force = component of weight acting perpendicular to slope 5. Work that out first! Then 6. Ep – work done against friction = energy left over 7. Use ½ mv2 to find v Objectives Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Solution 1 (a) U = m g h = 500 kg 9.8 m/s 300m = 1,47 MJ (b) W= - Ff s = -μ m g cosθ s sinθ=h/s cosθ = (s2-h2)1/2/s W= - μ m g (s2-h2)1/2 = -0.49 MJ (c) K = ½ m v2 =U + W = 0.98 MJ v = 62.6 m/s (note – this is a “clever” way to use cos and sin. Might be better just to use pythagoras to get horizonal distance of 400m ) Example 2 A car of mass m=1000 kg travelling at speed vi=30m/s has its speed reduced to vf=10 m/s by a constant breaking force over a distance of 80m. Find: Objectives Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words (a) the car’s initial kinetic energy (b) the final kinetic energy (c) the breaking force Objectives Problem 2 solution • (a) Ei = ½ m vi 2 = 450000 J • (b) Ef = ½ m vf 2 = 50000 J • (c) ΔE=Ef- Ei = (50000 – 450000) J = -400000 J W = F s = ΔE= -400000 kJ F = ΔE/s = -400,000/80 N = 5000 N (the minus sign indicates direction is opposite to direction of motion) Describe and define • Work • Energy • Power • Efficiency Discuss conservation of energy and conservative forces Carry out calculations to demonstrate understanding. Key Words Example 3 Mass m1 with initial velocity v1i collides with mass m2 which is initially at rest. The collision is elastic (energy and momentum are conserved). What are the velocities of the two masses after the collision? • Elastic collision, important information: 1. total momentum before = total momentum after m1 v1i = m1 v1f + m2 v2f (1) 2. total energy before = total energy after ½m1 v1i2 = ½ m1 v1f2 + ½ m2 v2f2 (2) Strategy: solve for v2f Eq (1) and substitute this into (2) then solve the resultant equation for v1f. • v1f = v1i (m1-m2)/(m1+m2) • Then substitute back v1f into equation for v2f and get: • v2f = v1i 2 m1/(m1 + m2) • If m1=m2 then the two masses exchange velocities! • -If m2 is enormous compared to m1 then m1 reverses its velocity and m2 almost at rest. • -What if m1 is enormous compare to m2? • Note – the algebra is tricky. You will NOT be asked to do this!