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  2. Newton's law of universal gravitation - Wikipedia

    en.wikipedia.org/wiki/Newton's_law_of_universal...

    The equation for universal gravitation thus takes the form: F = G m 1 m 2 r 2 , {\displaystyle F=G{\frac {m_{1}m_{2}}{r^{2}}},} where F is the gravitational force acting between two objects, m 1 and m 2 are the masses of the objects, r is the distance between the centers of their masses , and G is the gravitational constant .

  3. General relativity - Wikipedia

    en.wikipedia.org/wiki/General_relativity

    Newton's law of universal gravitation, which describes classical gravity, can be seen as a prediction of general relativity for the almost flat spacetime geometry around stationary mass distributions. Some predictions of general relativity, however, are beyond Newton's law of universal gravitation in classical physics.

  4. Fundamental interaction - Wikipedia

    en.wikipedia.org/wiki/Fundamental_interaction

    Isaac Newton's law of Universal Gravitation (1687) was a good approximation of the behaviour of gravitation. Present-day understanding of gravitation stems from Einstein's General Theory of Relativity of 1915, a more accurate (especially for cosmological masses and distances) description of gravitation in terms of the geometry of spacetime.

  5. History of physics - Wikipedia

    en.wikipedia.org/wiki/History_of_physics

    The curvature of space-time replaced Newton's universal law of gravitation. According to Einstein, gravitational force in the normal sense is an illusion caused by the geometry of space. The presence of a mass causes a curvature of space-time in the vicinity of the mass, and this curvature dictates the space-time path that all freely-moving ...

  6. Mass - Wikipedia

    en.wikipedia.org/wiki/Mass

    Newton's books on universal gravitation were published in the 1680s, but the first successful measurement of the Earth's mass in terms of traditional mass units, the Cavendish experiment, did not occur until 1797, over a hundred years later. Henry Cavendish found that the Earth's density was 5.448 ± 0.033 times that of water. As of 2009, the ...

  7. History of gravitational theory - Wikipedia

    en.wikipedia.org/wiki/History_of_gravitational...

    The resulting net force is exactly what is known as universal gravitation, in which the speed of gravity is that of light. Lorentz calculated that the value for the perihelion advance of Mercury was much too low. [109] In the late 19th century, Lord Kelvin pondered the possibility of a theory of everything. [110]

  8. New details emerge in CEO's slaying - AOL

    www.aol.com/news/details-emerge-ceos-slaying...

    The New York City Police Department released these images of “a person of interest” in the killing of UnitedHealthcare CEO Brian Thompson.

  9. Traité de mécanique céleste - Wikipedia

    en.wikipedia.org/wiki/Traité_de_mécanique_céleste

    Newton laid the foundations of Celestial Mechanics, at the close of the seventeenth century, by the discovery of the principle of universal gravitation. Even in his own hands, this discovery led to important consequences, but it has required a century and a half, and a regular succession of intellects the most powerful, to fill up the outline ...