Orbital Dynamics

Orbital dynamics is the study of the motion of objects in the presence of gravitational forces of other bodies. All bodies provide a gravitational pull on other bodies surrounding it. The force exerted by two bodies on each other is given by

<math>F = \frac{Gm_{1}m_{2}}{r^{2}}</math>

where G is the Universal Gravitational Constant whose value is 'insert value here', <math>m_1</math> is the mass of the first body, <math>m_2</math> is the mass of the second body, and r is the distance between them.

This article is a stub. You can help Lunarpedia by expanding it or sorting it into the correct stub subcategory.

Work on this article has outpaced copyediting on it. You can help Lunarpedia by formatting, editing, or tidying it.