Search results

Jump to navigation Jump to search
  • '''General relativity (GR)''' is a [[theory]] of [[gravitation]] that was developed by [[Albert Einstein]] between 1907 and 1915. Accordin Before the advent of general relativity, [[Newton's law of universal gravitation]] had been accepted for more than two hundred years as a valid description ...
    67 KB (9,914 words) - 21:17, 11 August 2009
  • | interaction = [[Electromagnetism]], [[Gravitation]], [[Strong interaction|Strong]], [[Weak interaction|Weak]] ...eraction]]s, also known as ''fundamental forces'' ([[electromagnetism]], [[gravitation]], [[strong interaction]], and [[weak interaction]]), as well as the only k ...
    61 KB (8,771 words) - 19:12, 19 August 2009
  • ...ysics]]. It unifies [[special relativity]] and [[Newton's law of universal gravitation]], and describes gravity as a geometric property of [[space]] and [[Time in ...general relativity|Golden age of general relativity|Classical theories of gravitation}} ...
    160 KB (21,329 words) - 06:49, 19 August 2009
  • [[Gravitation|Gravitational interactions]] of galaxies with each other and clusters cause ...Charles | coauthors = Thorne, Kip S. and Wheeler, John Archibald | title = Gravitation | location = San Francisco | publisher = W. H. Freeman | year = 1973 | isbn ...
    66 KB (9,812 words) - 01:07, 12 August 2009
  • |journal=[[General Relativity and Gravitation]] |title=Relativity, Gravitation and World Structure ...
    71 KB (10,454 words) - 13:19, 15 March 2011
  • ...idates for the use of the polar coordinate system. These systems include [[gravitation|gravitational fields]], which obey the [[inverse-square law]], as well as s ...
    35 KB (5,187 words) - 09:51, 14 August 2009
  • ...pplication of this extension to the [[sedimentation]] of particles under [[gravitation|gravity]].<ref name="tolman_1918" /> For example, the haze sometimes seen i ...ost stars are spherically symmetric, the total [[Newton's law of universal gravitation|gravitational]] [[Potential_energy#Calculation_of_gravitational_potential_e ...
    84 KB (12,734 words) - 06:55, 8 August 2009
  • ...of [[Minkowski space]]. The latter serves—in the absence of significant [[gravitation]]—as a model of [[space time]] in [[special relativity]].<ref>{{harvard cit ...on | last1=Weinberg | first1=Steven | author1-link=Steven Weinberg | title=Gravitation and Cosmology | publisher=[[John Wiley & Sons]] | location=New York | year= ...
    88 KB (12,980 words) - 01:52, 12 August 2009
  • ...orbit of Uranus led astronomers to deduce that its orbit was subject to [[gravitation]]al [[perturbation (astronomy)|perturbation]] by an unknown planet. Neptune ...known body was [[Perturbation (astronomy)|perturbing]] the orbit through [[gravitation]]al interaction. In 1843, [[John Couch Adams]] calculated the orbit of a hy ...
    83 KB (11,988 words) - 11:30, 20 August 2009
  • ...such as a planet revolving around a sun. For two bodies interacting by [[gravitation|Newtonian gravity]], the LRL vector is a [[constant of motion]], meaning th ...
    61 KB (8,970 words) - 23:12, 23 July 2009
  • ...o have begun 4.6&nbsp;[[1000000000 (number)|billion]] years ago with the [[gravitation]]al collapse of a small part of a giant [[molecular cloud]]. Most of the co ...
    85 KB (12,829 words) - 17:09, 18 August 2009
  • ...lp them in understanding [[general relativity]], a geometrical theory of [[gravitation]] developed mainly by [[Albert Einstein]]. Hilbert had observed that the [[ ...
    97 KB (14,013 words) - 22:11, 13 August 2009