Survey
* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Electromagnetism wikipedia , lookup
Coriolis force wikipedia , lookup
Fictitious force wikipedia , lookup
Weightlessness wikipedia , lookup
Lorentz force wikipedia , lookup
Velocity-addition formula wikipedia , lookup
Woodward effect wikipedia , lookup
Matter wave wikipedia , lookup
Negative mass wikipedia , lookup
Moments and Equilibrium Spanners Moment = = = Force 50 N 10 Nm x Distance (at right angles) x 0.2 m Moment Force = = = = Force x Distance (at right angles) Moment Distance (at right angles) 10 Nm 0.25 m 40 N Moment = 0 Nm if the distance at right angles is zero; therefore make the force parallel to the spanner handle. See-saw Left-hand force causes an anti-clockwise moment. Right-hand force causes a clockwise moment. Call the overall clockwise moment M. M = = = = Clockwise moment ( 60N x 2.3m ) 13.8 Nm 0.2 Nm – – – anti-clockwise moment ( 40N x 3.4m ) 13.6 Nm There is a positive clockwise moment of 0.2 Nm, so the see-saw rotates clockwise (down to the right). Crane The pivot is the end corner of the dockside. Counterweight and crane body cause an anti-clockwise moment. Load causes a clockwise moment. Call the overall clockwise moment M. M = = = Clockwise moments – anti-clockwise moment ( 50,000N x 20m ) + ( 5,000N x 4m ) – ( L N x 15m) 1,000,000 Nm + 20,000 Nm – 15L Nm If the crane is just stable, then M will be zero. So … 15L = 1,000,000 Nm + 20,000 Nm L = 1,020,000 Nm 15 m = 68,000 N So the crane is just balanced if lifting a load of 68,000N – any more than this and it will fall into the docks. Bus If the bus is symmetrical, the CofM is 3m up and 1.5m across. The bus falls if this point is outside of the supports (the wheels). (You can calculate what angle this is using trigonometry … 3m tan(angle) Max angle = 1.5 / 3 = 26.6º ) 1.5m It’s better for the passengers to sit on the bottom because this will make the bus heavier at the bottom so its CofM will be less than 3m up. Collisions and Momentum Vectors and Scalars Scalars: mass, length, time, speed, energy, power, frequency, temperature, angle … Vectors: velocity, momentum, acceleration, force … Cars (i) Red car Momentum = = = Mass x Velocity 500 kg x 20 m/s to the right 10,000 kg m/s to the right Blue car Momentum = = = Total = = Mass x Velocity 500 kg x 20 m/s to the left 10,000 kg m/s to the left 10,000 kg m/s left + 10,000 kg m/s right 0 During the crash, momentum is conserved, so it stays at 0. After the crash, both cars must have speed 0. (ii) Red car Momentum = = = Mass x Velocity 500 kg x 30 m/s to the right 15,000 kg m/s to the right Blue car Momentum = = = Mass x Velocity 500 kg x 20 m/s to the left 10,000 kg m/s to the left Total = = 10,000 kg m/s left + 15,000 kg m/s right 5,000 kg m/s to the right After the crash, momentum is still 5,000 kg m/s right. Wreckage Momentum = Velocity = = = Mass Momentum 5,000 kg m/s right 5 m/s to the right Rocket Before firing Momentum = Mass x Velocity = 1,000 kg x 0 m/s x Velocity Mass 1,000 kg = 0 kg m/s After firing it must be the same – zero. Gas Momentum = = = Mass x Velocity 200 kg x 200 m/s left 40,000 kg m/s left Rocket Must be 40,000 kg m/s right so that the total is still zero. Momentum = Velocity = = = Mass Momentum 40,000 kg m/s right 50 m/s right x Velocity Mass 800 kg Advanced The ship will go slower than we worked out because it doesn’t get that much lighter all in one go. The way to do the sum is a little bit at a time; taking steps of say 10kg of fuel, all the way up to 200kg used. To be more accurate, you make the steps smaller, say every 1kg of fuel, but it takes longer to do. Newton worked out a trick to speed up doing the sum even with the tiniest of steps. It’s called calculus. The real final speed in our example would be 44.6 m/s. Energy – Snooker Momentum before collision Red ball = White ball = = 0 kg m/s 100 g x 1 m/s 0.1 kg m/s Momentum after collision Red ball = = 100 g x 0.8 m/s 0.08 kg m/s White ball = = 100 g x 0.2 m/s 0.02 kg m/s Total 0.1 kg m/s same as before = = KE before collision Red ball = White ball = = = 0J ½ x Mass x Speed2 ½ x 100 g x (1 m/s)2 0.05 J KE after collision Red ball = = = ½ x Mass x Speed2 ½ x 100 g x (0.8 m/s)2 0.032 J White ball = = = ½ x Mass x Speed2 ½ x 100 g x (0.2 m/s)2 0.002 J Total = 0.034 J “Lost” = = 0.05 – 0.034 0.016 J “Lost” energy was converted to sound and heat. Force – Seatbelts Momentum = = = Mass x Velocity 50 kg x 32 m/s forwards 1600 kg m/s forwards Seatbelt 1600 kg m/s lost in 1s (i.e. 1.6kN) Windscreen 1600 kg m/s lost in 0.001s so 1,600,000 kg m/s (1600 / 0.001) would be lost in a whole 1s (i.e. 1.6MN) Skull Survives OK with the seatbelt; but busts open on the windscreen. The airbag makes it take even longer to stop you, so the force is reduced. It’s nothing to do with the bag being made of a soft material; the bag could be hard, so long as it has enough ‘give’ in it to slow you down gradually. Force – Saturn V Momentum = = = Mass x Velocity 3 M kg x 1500 m/s 4500 M kg m/s Force Momentum 4500 M kg m/s 30 MN = = = Time taken 150 s It’s only an estimate because this is the average thrust over the 150s; the thrust was probably not really constant over this time. Orbits Moving in a Circle Experiment The factors that affect the orbit radius are the force applied to the string (the weights you attach), the speed of whirling, and the mass of plasticene. You should find that the speed makes a lot more difference than the other factors. For the mathemagically minded, the formula for the force required is … F mv 2 r where m is the mass, v the speed and r the radius. The speed is squared which is why it makes more difference. You could estimate some values from your experiment to confirm the formula – it will be only very approximate. Question The table of data is a red herring. The centripetal force is provided by the Sun’s gravity which is strongest nearest the Sun. Therefore Mercury must need the biggest force! The mathematicians can work it out using the formula above; Mercury’s high speed is much more important than Jupiter’s mass or Pluto’s distance because the speed gets squared. Notes Centripetal force in orbits is provided by gravity. Centripetal force in atoms is provided by electrostatic attraction (a positive nucleus attracting the negative electrons). Geophysics Wegener