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 gravitational parameter 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. |