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Survey of the Universe Tom Burbine [email protected] Galileo Galilei (1564-1642) • He was able to figure out answers to these arguments • 1) Things in motion tend to remain in motion. • 2) He used a telescope to see sunspots on the Sun and features on the Moon. • 3) Galileo found that stars were more numerous and more distant than imagined He also • He discovered the moons of Jupiter and saw that they were orbiting Jupiter – – – – Io Europa Ganymede Callisto • Proving that bodies could orbit other bodies besides the Earth Galileo also found that Venus orbited the Sun Difference between mass and weight • Mass is the amount of matter in your body • Weight is the amount of force acting on your body • So on the Moon, you would have the same mass as on Earth but weigh less on the Moon since the Moon is less massive than Earth • Mass in metric system is usually measured in kilograms Isaac Newton (1642-1727) • Supposedly saw an apple fall to the ground • He then understood that gravity was universal, meaning it affected both the planets and us on Earth • Came up with 3 Laws of Motion • Also came up with calculus Force • Force – anything that can cause a body to change velocity • Velocity – a speed in a particular direction Gravity • Gravity is a natural phenomenon by which objects with mass attract one another. Newton • http://www.youtube.com/watch?v=_q6CXni6yTE Newton’s st 1 Law • In the absence of a net (overall) force acting upon it, an object moves with a constant velocity • An object at rest remains at rest • An object in motion tends to remain in motion unless a force is acting upon it Why do things on Earth not remain in motion? Why do things on Earth not remain in motion? • Friction Objects in orbit • Because the planets are moving in elliptical orbits around the Sun and not straight lines, there must be a force acting on the planets • This force is gravity Acceleration • Acceleration is when your velocity is changing • Velocity not changing, no acceleration Acceleration • • • • • a = ∆v/∆t Car is travelling at 10 m/s Increases its speed to 30 m/s over 5 seconds a = (30 m/s – 10 m/s)/5 seconds a = 4 m/s2 Acceleration due to Earth’s gravity • g = 9.8 m/s2 • If something is dropped, it will gain 9.8 m/s in velocity for every second it falls Newton’s nd 2 Law • Force = mass x acceleration • Units of Force kgm/s2 = newton Newton • A Newton is equal to the amount of force required to accelerate a mass of one kilogram at a rate of one meter per second per second How much do you weigh? • • • • So much do you weigh Say your mass is 100 kg F = 100 kg x 9.8 m/s2 F = 980 Newtons • 9.8 m/s2 is the acceleration of gravity on Earth • This is the acceleration due to the Earth’s gravitational field Newton’s rd 3 Law • For any force, there is an equal and opposite reaction force • Gravity is holding you on the ground • The ground is also pushing back up on you with the same amount of force http://www.vshiksha.com/system/files/u1/pslvc6-rocket.jpg Newton’s Universal Law of Gravitation • Every mass attracts every other mass through the force called gravity • Every point mass attracts every single other point mass by a force pointing along the line intersecting both points. • The force is directly proportional to the product of the two masses and inversely proportional to the square of the distance between the point masses Formula • Newton came up with this formula Force is proportional to M1 M2 d2 M1, M2 are the masses of the two objects d is the distance between the objects • If you want to calculate actual forces F = G M1 M2 d2 M1, M2 are the masses of the two objects d is the distance between the objects G = constant = 6.67 x 10-11 m3/(kgs2) So what should you know about this formula F = G M 1 M2 d2 • The force of attraction between any two objects is directly proportional to the product of their masses • The force of attraction between two objects decreases with the square of the distance between their centers • G is a very small number assume all mass is concentrated in the center of a body What is the attraction of two 100 kg people in the same room? F = G M1 M2 d2 • • • • • Say their masses are both 100 kg Their distances are 10 meters apart F = 6.67 x 10-11 m3/(kgs2) * 100*100 kg2/(10*10 m2) F = 6.67 x 10-9 N = 0.0000000067 N Remember the person weighs 980 N F = G M1 M2 d2 • The value of G was determined by Henry Cavendish between 1797-1798 • G = 6.67 x 10-11 m3/(kgs2) • http://blogs.howstuffworks.com/2009/04/13/diycalculate-the-gravitational-constant-like-cavendishdid/ http://www.makingthemodernworld.org.uk/learning_modules/maths/06.TU.02/illustrations/06.IL.09.gif Any Questions?