Gravitational Potential Energy: Difference between revisions

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This topic covers Gravitational Potential Energy.
This topic covers Gravitational Potential Energy.
Claimed by Kcrawford38 11/11/2015 6:49 pm
 
==The Main Idea==
==The Main Idea==



Revision as of 13:12, 16 November 2015

This topic covers Gravitational Potential Energy.

The Main Idea

Gravitational Potential energy belongs to a pair of objects in a system (for instance a ball+ Earth system, galaxies of stars interacting gravitationally) and is equal to the work done against gravity. This potential energy is the energy associated within the particles inside a system and is not the same as rest or kinetic energies of the individual particles. Traditionally potential energy is represented by the symbol U and this page describes specific examples in which U is equal to the gravitational energy learned about in earlier pages to be approximately mg near the surface of the Earth or [math]\displaystyle{ F = - G \frac{m_1 m_2}{r^2}\ }[/math]
where:

  • F is the force between the masses;
  • G is the gravitational constant (6.674×10−11 N · (m/kg)2);
  • m1 is the first mass;
  • m2 is the second mass;
  • r is the distance between the centers of the masses.

The latter case is distance dependent and can be derived since force is the negative gradient of U. The negative indicates that potential energy decreases as particles get closer together



A Mathematical Model

[math]\displaystyle{ F = - G \frac{m_1 m_2}{r^2}\ }[/math]
where:

  • F is the force between the masses;
  • G is the gravitational constant (6.674×10−11 N · (m/kg)2);
  • m1 is the first mass;
  • m2 is the second mass;
  • r is the distance between the centers of the masses.


A Computational Model

How do we visualize or predict using this topic. Consider embedding some vpython code here Teach hands-on with GlowScript

Examples

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