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  1. Newton’s law of gravitation states that the magnitude of the gravitational force between two masses is directly proportional to the product of the masses, and is inversely proportional to the square of the distance between them, (where the distance is measured between the two centres of the masses). Where. Gm. F. = 1 m 2 r2.

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  2. through the Law of Gravitation enunciated by Newton in 1687. Every particle of matter in the universe attracts every other particle with a force that is directly proportional to the product of the masses of the particles and inversely proportional to the square of the distance between them.

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  3. Chapter 13 - Universal Gravitation In Chapter 5 we studied Newton’s three laws of motion. In addition to these laws, Newton formulated the law of universal gravitation. This law states that two masses are attracted by a force given by 2 1 2 r Gm m F = , where G = 6.67 x 10-11 N⋅m2/kg2 (not g = 9.8 m/s2). For spherical masses, r is the distance

  4. Gravitation 1 Newton’s Law of Gravitation Along with his three laws of motion, Isaac Newton also published his law of grav-itation in 1687. Every particle of matter in the universe attracts every other particle with a force that is directly proportional to the product of the masses of the particles and inversely

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  5. The force of gravity is an attractive force that is proportional to the product of the masses of the interacting objects, and inversely proportional to the square of the distance between them. A gravitational interaction involves the attractive force that any object with mass exerts

  6. How Newton’s Law of Universal Gravitation Explains Kepler’s Laws.............................................................11. Kepler’s Third Law (well, for circular orbits)...................................................................................................11.

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  8. Gravity Newton's Universal Law of Gravitation (first stated by Newton): any two masses m 1 and m 2 exert an attractive gravitational force on each other according to 12 2 mm FG r 1 This applies to all masses, not just big ones. G = universal constant of gravitation = 6.67 10–11 N m2 / kg2 (G is very small, so it is very difficult to measure!)

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