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<p>in 1915, which describes gravity in terms of the <a href="page.php?w=curvature">curvature</a> of <a href="page.php?w=spacetime">spacetime</a>, caused by the uneven distribution of mass. The most extreme example of this curvature of spacetime is a <a href="page.php?w=black_hole">black hole</a>, from which nothing--not even light--can escape once past the black hole's <a href="page.php?w=event_horizon">event horizon</a>. However, for most applications, gravity is sufficiently well approximated by <a href="page.php?w=Newton%27s_law_of_universal_gravitation">Newton's law of universal gravitation</a>,</p><p>
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