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Example of a Newton One newton (N) is the force it takes to change the speed of a 1 kg mass by 1 m/s in 1 second. Time 1N Time 1 kg 2 m/s 1 m/s 1N 1 kg Equation for Newton’s Second Law Acceleration (m/s2) F a= m Force (N) Mass (kg) More mass Mass Mass F m F m Less acceleration a= Speed increases faster More acceleration a= Speed increases Acceleration Newton’s Second Law Force More force Force m F Speed increases slower a = Object in Free Fall Start 0 m/s After 1 second 9.8 m/s After 2 seconds 19.6 m/s After 3 seconds 29.4 m/s Newton’s Third Law Reaction force More acceleration Action force Less acceleration Converting Energy +- 120 volts CH4 + 2O2 2H2O + CO2 + energy Chemical energy +- 120 volts 0 volts +- 120 volts 0 volts 0 volts Safety ground (0 volts) Electrical energy Hot steam Heat energy Mechanical energy Some Important Variables in the System g Time Mass on ti Posi ed Spe Angle Systems and Variables System includes: car, ramp, angle, speed, time, mass tion Posi ed Spe Angle Not included: color, light, window, floor or friction (or anything else) Work Work (joules) Force (newtons) W = Fd 1N 1 meter Distance (meters) in the direction of the force Block Lifting the 1 newton block 1 meter requires 1 joule of work. Power Power (watts) Michael seconds P= W t 100 N Work (joules) Time (seconds) Jim 2m 100 N seconds Michael and Jim do the same amount of work but do not have the same power. 2m Power Example Start Work 100 N Power 10 m 10 seconds 60 seconds 1,000 J 100 W 1,000 J 16.7 W Power = Amount of work done time Energy Flow Mechanical Advantage of a Lever Mechanical advantage Li MAlever = Lo Input arm Li Fulcrum Length of input arm (m) Length of output arm (m) Output arm Lo Mechanical Advantage Mechanical advantage Fo MA = Fi Output force (N) Input force (N) Output force Input force 200 kg Input force Output force A small input force can create a large output force for simple machines with a mechanical advantage greater than one. The Three Classes of Levers 1st Class Output force Input force Input force Output force fulcrum Input force 2nd Class Output force Input force fulcrum Output force 3rd Class Input force Input force Output force fulcrum Output force Earth Image: NASA Forming a Planetary System Jupiter NASA photo Mars ESA photo Mercury Image from radar maps, NASA Planet Overview Property Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto Diameter (km) 4,878 12,102 12,756 6,794 142,796 120,660 51,200 49,500 2,200 3.3 × 1023 4.9 × 1024 6.0 × 1024 6.4 × 1023 1.9 × 1027 5.7 × 1026 8.7 × 1025 1.0 × 1026 1.3 × 1022 5.44 5.25 5.52 3.91 1.31 0.69 1.21 1.67 1.75 58 108 150 228 778 1430 2870 4500 5910 Major moons (#) 0 0 1 2 39 30 21 8 1 Strength `of gravity (N/kg) 3.7 8.9 9.8 3.7 23.1 9.0 8.7 11.0 0.6 Surface temperature (°C) -170 to +400 +450 to +480 -88 to +48 -89 to -31 -108 -139 -197 -201 -223 59 243 1 1.03 0.41 0.43 0.72 0.67 6.4 0.24 0.62 1 1.9 12 29 84 165 249 47.89 35.04 29.80 24.14 13.06 9.64 6.80 5.43 4.74 Mass (kg) Density (g/cm3) Average distance from sun (million km) Rotation period (Earth days) Revolution period (Earth years) Orbital speed (km/sec) Planet Size Relative to the Sun Pluto Pluto Image courtesy NASA/JPL-Caltech Saturn NASA photo The Solar System Uranus and Neptune Uranus Neptune Images: NASA Jet Propulsion Labratory Venus Image: NASA Evolution of a Sun-like Star Luminosity Bright Pluto Dim 25,000 10,000 6,000 Temperature (ºC) 3,000 Stars, Color and Temperature Ultraviolet Light output { Infrared Visible light Color Sun Anatomy Types of Galaxies Spiral Barred spiral Lenticular Elliptical