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General Relativity

... straight line in curved space its path will curve towards a massive object. No force is needed to explain the change of path, the curvature of spacetime is enough to explain the motion. Pretty clever. ...
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... Special Relativity • Einstein’s special theory of relativity has two parts. – All objects moving at constant velocity have the same laws of physics – The speed of light is constant for all observers ...
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... You should know the equation. Be able to describe the relationships in words, with graphs, with calculations, and applications. For orbiting objects (moons, satellites, comets) that have a change in (mass, radius, or velocity) you should be able to tell how (Fg, T, vel, “g”) are affected. This could ...
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... stronger as the masses increase and rapidly become weaker as the distance between the masses increases, F=G(m1m2/d2) • Evaluate the concept that free-fall acceleration near Earth’s surface is independent of the mass of the falling object • Demonstrate mathematically how free-fall acceleration relate ...
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... Inertial mass Relates to how a mass responds to an external force (also called a contact force). If you push a stalled car into motion you are testing its inertial mass. Gravitational mass Relates to how a mass responds to the force of gravity (also called a field force). If you lift up a stalled ca ...
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... The line joining the two bodies (the sun and the revolving object) sweeps equal areas in equal times. The graphic precisely displays Kepler's second law. The area of every triangle formed is exactly the same area. Also notice as the planet or satellite moves closer to the sun, the speed of its orbit ...
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Equivalence principle

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