next up previous
Next: Perturbations and more on Up: Orbital Elements Previous: Coordinate Transformations

An explicit Example

In this section we will compute the cartesian coordinates of the satellite given as an example in a previous section. The two-line element was given by:

1 20361U 89097A   01154.90156813 -.0000008400000-0  00000-0 0  7462
2 20361 56.2556 342.0793 0127851 179.5306 322.3780 2.00562298 74668

We already calculated $a=26,560.46$ km. Furthermore, we have $e=0.0127851$. From this we get $b=26,558.29$km. The next step is to compute the ecc3entric anomaly from Kepler's equation. The mean anomaly was given by $\nu=322.378^{\circ}$. The numerical solution of Kepler's equation requires that we measure all angles in radians (You cannot do Calculus type operations with degrees ever!!). Transforming it into radians gives us $\nu=5.62639$. We next perform the fixed point iteration with $E_0=\nu=5.62639$. This gives us $E_1=5.63734$, $E_2=5.62767$, $E_3=5.62764$, and $E_4=5.62264$. Since $E_3=E_4$ both are approximations to the eccentric anomaly with 5 valid digits. We will use $E=5.62764$. Using this we can directly compute the $(x''',y''',z''')$ coordinates of the satellite.

\begin{eqnarray*}
x''' &=& a\cos E-ae =20,566.52\\
y''' &=& b\sin E= -16,381.46\\
z''' &=& 0
\end{eqnarray*}

Next we compute the necessary transforms. First a rotation about $z'''$ by $-\omega$. From the two-line elements we get that $\omega=179.53^{\circ}$. Therefore,we have

\begin{eqnarray*}
x''&=& \cos 179.53^{\circ} x'''-\sin 179.53^{\circ} y'''=-20,...
...3^{\circ}x'''+\cos 179.53^{\circ} y'''=16,549.62\\
z''&=&z'''
\end{eqnarray*}

This is clearly a rotation of about $180^{\circ}$. In the nex step we need to rotate by $-i$ about the $x''$ axis. From the two line elements we get $i=56.26^{\circ}$. This gives us:

\begin{eqnarray*}
x'&=&x''=-20,431.45\\
y'&=& \cos 56.26^{\circ}y''-\sin 56.2...
...\
z'&=& \sin 56.26^{\circ}y''+\cos 56.26^{\circ}z''=13,762.11
\end{eqnarray*}

We complete the procedure by rotating about the $z'$ axis by $-\Omega$. The two line elements give $\Omega=342.08^{\circ}$. This yields:

\begin{eqnarray*}
x&=&\cos 342.08^{\circ}x'-\sin 342.08^{\circ}y'=-16,611.96\\ ...
...^{\circ}x'+\cos 342.08^{\circ}y'=15,032.66\\
z&=&z'=13,762.11
\end{eqnarray*}

Hence the cartesian coordinates of this satellite at the given time are $(-16,611,15,032.66,13,762.11)$, where these distances are measured in km. In this example we used an accuracy of 10m for the distances. One may of course need higher accuracy in some applications.
next up previous
Next: Perturbations and more on Up: Orbital Elements Previous: Coordinate Transformations
Werner Horn 2006-06-06