perturbation

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perturbation , in astronomy and physics, small force or other influence that modifies the otherwise simple motion of some object. The term is also used for the effect produced by the perturbation, e.g., a change in the object's energy or path of motion. One important effect of perturbations is the advance, or precession, of the perihelion of a planet, which can be described as a slow rotation of the entire planetary orbit. A residual advance in the perihelion of Mercury provided a valuable test of Einstein's general theory of relativity .

In the solar system the dominant force is the gravitational force exerted by the sun on each planet; assuming that this is the only force, the simple elliptical orbits described by Kepler's laws are derived. However, the perturbations caused by the gravitational interaction of the planets among themselves change and complicate the curve of these orbits. The study of perturbations has led to important discoveries in astronomy. Within the solar system, the existence and position of Neptune was predicted because of the deviations of Uranus from its computed path. Likewise, Pluto was discovered by its effect on Neptune. Beyond the confines of the solar system, perturbations in the orbits of stars caused by the gravitational forces of orbiting bodies have led to the discovery of a number of extrasolar planetary systems .

In the atom the dominant force is the electrical force between the nucleus and the electrons; this force determines the characteristic structure, or energy levels, of the atom. The forces exerted by the electrons among themselves are perturbations that slightly modify this structure.

perturbation A change in the orbit of a body, usually due to the gravitational attraction of another body. Thus the planets in their elliptical orbits about the Sun mutually perturb one another, producing changes in their orbital elements. The orbits of satellites are perturbed by their mutual gravitational attractions and also by the Sun. Perturbations also arise in the orbits of satellites that lie close to their planets because the planets are not perfectly spherical in shape. The orbits of some artificial Earth satellites are also perturbed by atmospheric drag. See also periodic perturbation; secular perturbation.