Six new equations can be derived from Equations (G.24)–(G.29)
by multiplying them successively by
,
,
,
,
, and
, and then
summing the resulting equations. The right-hand sides
of the new equations are
![$\displaystyle \frac{\partial {\cal R}}{\partial X}\,\frac{\partial X}{\partial ...
...\,\frac{\partial Z}{\partial c_j}\equiv
\frac{\partial {\cal R}}{\partial c_j}.$](img4684.png) |
(G.30) |
The new equations can be written in a more compact form via
the introduction of Lagrange brackets, which are defined as
![$\displaystyle [c_j,c_k] \equiv \sum_{l=1,3}\left(\frac{\partial X_l}{\partial c...
...ac{\partial X_l}{\partial c_k}\,\frac{\partial \dot{X}_l}{\partial c_j}\right),$](img4685.png) |
(G.31) |
where
,
, and
.
Thus, the new equations become
![$\displaystyle \sum_{k=1,6}[c_j, c_k]\,\frac{dc_k}{dt} = \frac{\partial {\cal R}}{\partial c_j},$](img4689.png) |
(G.32) |
for
.
Note, incidentally, that
Let
![$\displaystyle [p,q] = \sum_{l=1,3}\left(\frac{\partial X_l}{\partial p}\,\frac{...
... \frac{\partial X_l}{\partial q}\,\frac{\partial \dot{X}_l}{\partial p}\right),$](img4694.png) |
(G.35) |
where
and
are any two orbital elements. It follows that
![$\displaystyle \frac{\partial}{\partial t} [p,q] = \sum_{l=1,3}\left(\frac{\part...
...l}{\partial q}\,\frac{\partial^{\,2} \dot{X}_l}{\partial p\,\partial t}\right),$](img4695.png) |
(G.36) |
or
![$\displaystyle \frac{\partial}{\partial t} [p,q]= \sum_{l=1,3}\left[
\frac{\part...
...\partial X_l}{\partial p}\,\frac{\partial \dot{X}_l}{\partial t}\right)\right].$](img4696.png) |
(G.37) |
However, in the preceding expression,
and
stand for
coordinates and velocities of Keplerian orbits calculated with
treated as constants. Thus, we can write
and
, giving
![$\displaystyle \frac{\partial}{\partial t} [p,q]= \sum_{l=1,3}\left[
\frac{\part...
...rac{\partial F_0}{\partial X_l}\,\frac{\partial X_l}{\partial p}\right)\right],$](img4701.png) |
(G.38) |
because
![$\displaystyle \ddot{X}_l = \frac{\partial F_0}{\partial X_l},$](img4702.png) |
(G.39) |
where
.
Expression (G.38) reduces to
![$\displaystyle \frac{\partial}{\partial t}[p,q] = \frac{1}{2}\frac{\partial^{\,2...
...partial q\,\partial p} + \frac{\partial^{\,2} F_0}{\partial q\,\partial p} = 0,$](img4704.png) |
(G.40) |
where
. Hence, we conclude that
Lagrange brackets are functions of the osculating orbital
elements,
, but are not explicit functions of
.
It follows that we can evaluate these brackets at any convenient point in the orbit.