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  2. Gravitational potential - Wikipedia

    en.wikipedia.org/wiki/Gravitational_potential

    Gravitational potential. In classical mechanics, the gravitational potential is a scalar field associating with each point in space the work ( energy transferred) per unit mass that would be needed to move an object to that point from a fixed reference point. It is analogous to the electric potential with mass playing the role of charge.

  3. Gravitational energy - Wikipedia

    en.wikipedia.org/wiki/Gravitational_energy

    Gravitational energy or gravitational potential energy is the potential energy a massive object has due to its position in a gravitational field. It is the mechanical work done by the gravitational force to bring the mass from a chosen reference point (often an "infinite distance" from the mass generating the field) to some other point in the ...

  4. Virial theorem - Wikipedia

    en.wikipedia.org/wiki/Virial_theorem

    Virial theorem. In statistical mechanics, the virial theorem provides a general equation that relates the average over time of the total kinetic energy of a stable system of discrete particles, bound by a conservative force (where the work done is independent of path) with that of the total potential energy of the system.

  5. Two-body problem - Wikipedia

    en.wikipedia.org/wiki/Two-body_problem

    The most prominent example of the classical two-body problem is the gravitational case (see also Kepler problem), arising in astronomy for predicting the orbits (or escapes from orbit) of objects such as satellites, planets, and stars. A two-point-particle model of such a system nearly always describes its behavior well enough to provide useful ...

  6. Potential energy - Wikipedia

    en.wikipedia.org/wiki/Potential_energy

    e. In physics, potential energy is the energy held by an object because of its position relative to other objects, stresses within itself, its electric charge, or other factors. [ 1][ 2] The term potential energy was introduced by the 19th-century Scottish engineer and physicist William Rankine, [ 3][ 4][ 5] although it has links to the ancient ...

  7. Gravitational binding energy - Wikipedia

    en.wikipedia.org/wiki/Gravitational_binding_energy

    The gravitational binding energy of a system is the minimum energy which must be added to it in order for the system to cease being in a gravitationally bound state. A gravitationally bound system has a lower ( i.e., more negative) gravitational potential energy than the sum of the energies of its parts when these are completely separated ...

  8. Jeans instability - Wikipedia

    en.wikipedia.org/wiki/Jeans_instability

    v. t. e. The Jeans instability is a concept in astrophysics that describes an instability that leads to the gravitational collapse of a cloud of gas or dust. [ 1] It causes the collapse of interstellar gas clouds and subsequent star formation. It occurs when the internal gas pressure is not strong enough to prevent the gravitational collapse of ...

  9. Geopotential height - Wikipedia

    en.wikipedia.org/wiki/Geopotential_height

    Geopotential is the gravitational potential energy per unit mass at elevation : where is the acceleration due to gravity, is latitude, and is the geometric elevation. [ 1] Geopotential height may be obtained from normalizing geopotential by the acceleration of gravity: where = 9.80665 m/s 2, the standard gravity at mean sea level. [ 4]