Standard assumptions in astrodynamics 

For most of the problems in astrodynamics involving two bodies m_1\, and m_2\, standard assumptions are usually the following:

{m_2\over{m_1}} \ll 1

Results:

\mu=G{m_1}\simeq{G}(m_1+m_2)

where G\, is a gravitational constant.

The center of the central body can be taken as the origin of an inertial frame of reference for the orbiting body,

Examples where those assumptions do not hold

Two bodies orbiting each other

If A2 is not fulfilled, many results still apply with a small modification; see the two-body problem in astrodynamics.

See also