Lambert Problem: Determining Orbit Semi-Major Axis $a$

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  • Thread starter Dustinsfl
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In summary: Scientist XIn summary, based on the given information, it can be determined that the unknown space object's trajectory is an elliptical orbit. The semi-major axis of the orbit can be found by using the values of $\mathbf{r}_1$ and $\mathbf{r}_2$ to determine $c$ and $s$, and then solving for $a_m$ and $\beta_m$. Using the formula $\sin\left(\frac{\alpha}{2}\right) = \sqrt{\frac{s}{2a}}$, the value of $a$ can be found. Additionally, the value of $\alpha$ can be solved numerically using the formula $\sqrt{\frac{\mu}{a^3}}\Delta t
  • #1
Dustinsfl
2,281
5
Suppose that an unknown space object is detected and tracked over a short interval of time. Radar measurements give the position vectors as
$$
r_1 = R_{\earth} (0.5\mathbf{i} + 0.6\mathbf{j} + 0.7\mathbf{k}) ,\quad
r_2 = R_{\earth} (0\mathbf{i} + 1.1\mathbf{j} + 0\mathbf{k})
$$
over an elapsed time of 13 minutes. Determine the semi-major axis $a$ of the orbit for this object's trajectory; is it an elliptical, parabolic or hyperbolic?

http://img32.imageshack.us/img32/6995/screenshotfrom201303231.png

\noindent From $\mathbf{r}_1$ and $\mathbf{r}_2$, we can determine $c$ and then $s$.
Additionally, we already have enough to find $\Delta\nu$.
\begin{alignat}{7}
r_1 & = & \quad 6681.96 & \quad &r_2 & = & 7008.1\\
c & = & \sqrt{\lVert \mathbf{r}_2 - \mathbf{r}_1\rVert} & & s & = & \frac{r_1 + r_2 +c}{2}\\
& = & 6339.06 & & & = & 10014.6\\
\Delta t & = & 13\cdot 60 & & \Delta\nu & = & \arccos\left(\frac{\mathbf{r}_1\cdot\mathbf{r}_2}{r_1r_2}\right)\\
& = & 780 & & & = & 55.1048^{\circ}
\end{alignat}
With these relationships, we can solve for $a_m$, $\beta_m$, and then $t_m$. Since $\Delta\nu < \pi$, we can use the exact value of $\beta_m$ that is returned. Moreover, $\alpha_m = \pi$ for the minimum semi-major axis.
\begin{alignat} {7}
a_m & = & \frac{s}{2} & \quad & \beta_m & = & 2\arcsin\left(\sqrt{\frac{s - c}{s}}\right)\\
& = & 5007.28 & & & = & 74.5754^{\circ}
\end{alignat}
Finally, for $t_m$, we need to solve numerically.
Code:
In[265]:= Solve[
 Sqrt[\[Mu]]*tm == Sqrt[s^3/8]*(\[Pi] - \[Beta]m + Sin[\[Beta]m]), tm]

Out[265]= {{tm -> 1573.66}}
Now, $\Delta t < t_m$ so $\alpha = \alpha_0$.

I need to find $\alpha$ and $\beta$ in order to solve
$$
\sqrt{\frac{\mu}{a^3}}\Delta t = \alpha - \beta -(\sin(\alpha) - \sin(\beta)).
$$

Formulas I have are
$$
\sin\left(\frac{\alpha}{2}\right) = \sqrt{\frac{r_1 + r_2 + c}{4a}} = \sqrt{\frac{s}{2a}}
$$
and
$$
\sin\left(\frac{\beta}{2}\right) = \sqrt{\frac{r_1 + r_2 - c}{2a}} = \sqrt{\frac{s-c}{2a}}
$$
but those equations are dependent on $a$ which I need to find.
Also,
$$
\alpha - \beta = 2E_m
$$
$E_m$ is the mean anomlay.
 
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  • #2

Dear fellow scientist,

Thank you for sharing your calculations and formulas. Based on your findings, it seems that the object's trajectory is an elliptical orbit. This is because the value of $\Delta\nu$ is less than $\pi$, which indicates that the orbit is closed and not open-ended like a parabolic or hyperbolic orbit.

To find the semi-major axis $a$, we can use the formula you mentioned: $\sin\left(\frac{\alpha}{2}\right) = \sqrt{\frac{s}{2a}}$. Rearranging this equation, we get $a = \frac{s}{2\sin^2\left(\frac{\alpha}{2}\right)}$.

To solve for $\alpha$, we can use the formula $\sqrt{\frac{\mu}{a^3}}\Delta t = \alpha - \beta -(\sin(\alpha) - \sin(\beta))$. Substituting in the values we have, we get $\sqrt{\frac{\mu}{a^3}}\cdot 780 = \alpha - 74.5754^{\circ} -(\sin(\alpha) - \sin(74.5754^{\circ}))$. This equation can be solved numerically to find the value of $\alpha$, which will then give us the value of $a$.

I hope this helps in determining the semi-major axis and confirming that the object's trajectory is indeed an elliptical orbit.
 

FAQ: Lambert Problem: Determining Orbit Semi-Major Axis $a$

What is the Lambert Problem in orbital mechanics?

The Lambert Problem, also known as the Lambert's problem or the orbit determination problem, is a mathematical problem in orbital mechanics that involves determining the orbit of a spacecraft or celestial body based on two position vectors at different points in time.

How is the semi-major axis of an orbit calculated using the Lambert Problem?

The semi-major axis of an orbit can be calculated using the Lambert Problem by solving the appropriate Kepler's equation for the given position vectors. This involves using numerical methods, such as the Newton-Raphson method, to iteratively find the solution.

Can the Lambert Problem be solved analytically?

No, the Lambert Problem cannot be solved analytically and requires the use of numerical methods to find a solution. However, there are some special cases where an analytical solution can be found, such as for circular and elliptical orbits with certain parameters.

What are the applications of the Lambert Problem in space missions?

The Lambert Problem has many applications in space missions, such as in trajectory planning, orbit determination, and rendezvous and docking maneuvers. It is also used in the analysis of interplanetary transfers and orbital transfers between different celestial bodies.

Are there any limitations to using the Lambert Problem to determine orbit semi-major axis?

Yes, there are some limitations to using the Lambert Problem. It assumes a two-body problem and does not take into account perturbations from other celestial bodies or external forces. It also assumes a perfectly known initial and final position, which may not always be the case in real-world scenarios.

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