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  1. The divergence of a vector field which is the resultant of radial inverse-square law fields with respect to one or more sources is proportional to the strength of the local sources, and hence zero outside sources. Newton's law of universal gravitation follows an inverse-square law, as do the effects of electric, light, sound, and radiation ...

  2. 10.1: The Inverse-Square Law. Page ID. Julio Gea-Banacloche. University of Arkansas via University of Arkansas Libraries. Up to this point, all I have told you about gravity is that, near the surface of the Earth, the gravitational force exerted by the Earth on an object of mass m is FG = mg.

  3. Newton's law of gravitation resembles Coulomb's law of electrical forces, which is used to calculate the magnitude of the electrical force arising between two charged bodies. Both are inverse-square laws, where force is inversely proportional to the square of the distance between the bodies. Coulomb's law has charge in place of mass and a ...

    • Overview
    • Gravitation
    • Planetary motion
    • Second law
    • Third Law
    • Orbits

    This article is about Kepler's laws of planetary motion which describe the motions of planets in the solar system that were derived by German astronomer Johannes Kepler with later contributions from Sir Isaac Newton for his law of gravitation. It also mentions how these laws apply not only to gravitational but also other inverse-square-law forces.

    The article is about the laws of gravitation.

    Kepler’s three laws describe the motions of planets in the solar system, including elliptical orbits and angular momentum.

    A radius vector joining any planet to the Sun sweeps out equal areas in equal lengths of time.

    The squares of sidereal periods are directly proportional to cubes of mean distances from Sun.

    Laws apply not only to gravitational but also to all other inverse-square-law forces and electromagnetic forces within atom if allowance made for relativistic and quantum effects.

    • The Editors of Encyclopaedia Britannica
  4. Newton proposed the Inverse Square Law. The effect of gravity (and also on forces such as sunlight) works like this. If say we have a half-mass Earth, it would produce a gravity of not half but a quarter (the square of 2). If Earth was three times closer to the Sun it would get not 3 times as much light but 9 times as much (the square of 3 is 9).

  5. Inverse Square Law, General. Any point source which spreads its influence equally in all directions without a limit to its range will obey the inverse square law. This comes from strictly geometrical considerations. The intensity of the influence at any given radius r is the source strength divided by the area of the sphere.

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  7. Jun 15, 2023 · FG12 = Gm1m2 r212. (8.3.1) (8.3.1) F 12 G = G m 1 m 2 r 12 2. Here, r12 r 12 is just the magnitude of the position vector of particle 2 relative to particle 1 (so r12 r 12 is, indeed, the distance between the two particles), and G G is a constant, known as “Newton’s constant” or the gravitational constant, which at the time of Newton ...

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