Solution to the Two-Body Problem: Cross-Product and Dot-Product Integration

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SUMMARY

The discussion focuses on solving the two-body problem using vector calculus, specifically through the integration of cross-products and dot-products. The initial equation presented is $$\ddot{\textbf{r}}+\frac{GM}{r^2}\frac{\textbf{r}}{r}=0$$, leading to the momentum vector $$\textbf{h}=\textbf{r}\times\dot{\textbf{r}}$$. The solution is derived by taking the cross-product with the constant momentum vector and integrating, resulting in $$r=\frac{h^2/(GM)}{1+ecos\theta}$$. Participants express confusion regarding the integration process and the treatment of variables, particularly the distinction between constant and time-dependent variables.

PREREQUISITES
  • Understanding of vector calculus, specifically cross-products and dot-products.
  • Familiarity with the two-body problem in classical mechanics.
  • Knowledge of gravitational mechanics, particularly Newton's law of gravitation.
  • Ability to perform integrations involving time-dependent variables.
NEXT STEPS
  • Study the derivation of the two-body problem solutions in classical mechanics.
  • Learn about the application of cross-products in physics, particularly in momentum calculations.
  • Explore the integration techniques for time-dependent variables in vector equations.
  • Review Landau and Lifshitz's "Mechanics" for comprehensive insights into the two-body problem.
USEFUL FOR

Students and professionals in physics, particularly those studying classical mechanics, as well as educators looking to clarify the two-body problem and its solutions through vector calculus.

TimeRip496
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Homework Statement


Two-body problem given as
$$\ddot{\textbf{r}}+\frac{GM}{r^2}\frac{\textbf{r}}{r}=0$$
$$\textbf{h}=\textbf{r}\times\dot{\textbf{r}}$$
where the moment of the momentum vector mh

Homework Equations


The vector solution to the above equation may be obtained by first taking the cross-product with the constant h and integrating once with respect to time. This yields
$$\dot{\textbf{r}}\times\textbf{h}=GM(\frac{\textbf{r}}{r}+\textbf{e})$$

The final solution to the equation is then obtained by taking the dot product of above equation with r, is
$$r=\frac{h^2/(GM)}{1+ecos\theta}$$

The Attempt at a Solution


I have no idea what the author is doing. How does cross product with the momentum and then dot product with r solve the equation?

I try following his step but I get a different integration result
$$\dot{\textbf{r}}\times\textbf{h}=GM(\frac{\textbf{r}}{r^3}t\times\textbf{h}+\textbf{e})$$
I have no idea how his integration w.r.t. time for the GM/r2 reduces it to GM/r and how to cross product GM/r2 with h since they are unknown variables?
 
Last edited:
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What's the objective here? To find ##r(t)## and ##\theta(t)##? If so, the solution is well-known...Landau / Lifshitz "Mechanics" has a good summary if you've never seen it.
 
TimeRip496 said:
I try following his step but I get a different integration result
$$\dot{\textbf{r}}\times\textbf{h}=GM(\frac{\textbf{r}}{r^3}t\times\textbf{h}+\textbf{e})$$
How did you get the first term on the right: ##GM(\frac{\textbf{r}}{r^3}t\times\textbf{h}) \,##?

Keep in mind that ##\mathbf r## and ##r## are functions of time. You cannot treat them as constants when integrating with respect to time.
 

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