Mathematica How to Find Velocity at Final Location Using Mathematica?

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To find the velocity at a final location after solving a restricted three-body problem in Mathematica, numerical differentiation of position data can be performed. The position data was obtained using NDSolve, and the D[] function can be utilized for differentiation in Mathematica. The user exported position data to a CSV file for analysis. For further calculations in Excel, both time and position data are necessary to compute a numerical derivative. A trajectory plot was shared, indicating the positions of the Earth and the Moon relative to the L4 point.
Dustinsfl
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I used mathematica to solve a restricted 3 body problem and was able to export my position data at different time intervals. How can I find my velocity at that final location?
 
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What mechanism did you employ in Mathematica to get your position object? NDSolve? If so, you should be able to differentiate it numerically by using the usual D[] function.
 
Ackbach said:
What mechanism did you employ in Mathematica to get your position object? NDSolve? If so, you should be able to differentiate it numerically by using the usual D[] function.

I obtained my position data by
Code:
XYdata = Flatten[
   Table[Evaluate[{x1[t], x2[t], x3[t]} /. s], {t, 0, 122400, 3}], 1];
SetDirectory[NotebookDirectory[]];
Export["OrbitData.txt", XYdata, "CSV"];
Earth = {N[x1], 0};
L4 = {N[xL4], N[yL4]};
Export["Earth.txt", Earth, "CSV"];
 
So are you now looking at the data in Excel, or Mathematica? Because you should be able to do x1'[t]/.s to get the derivative in Mathematica. In Excel, you'd have to have the time data as well as the position data. Then you could compute a numerical derivative.
 
Here is the plot of my trajectory to L4.
The moon is the green dot in the bottom and Earth is blue.
 

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