On the convergence of the three body disturbing function

In summary, to check the convergence of the three-body-disturbing function expanded in multipolar orders, one can calculate the residuals of the expansion and check if they decrease as the order of the multipole increases. This method was used by Laskar in his paper "Explicit expansion of the three-body disturbing function for arbitrary eccentricities and inclinations" by calculating the maximum absolute residual for each order and checking if it decreases below a certain threshold. If the threshold is not reached for a certain set of parameters, then the series is not converging.
  • #1
Maher
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For the three-body-disturbing function expanded in multipolar orders with respect to the ratio of the semi major axes, the function converges for small ratios, how to check the convergence for a certain set of parameters? I'm using the work of the Laskar in his paper "Explicit expansion of the three-body disturbing function for arbitrary eccentricities and inclinations".
 
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  • #2
The convergence of the three-body disturbing function expanded in multipolar orders can be determined by calculating the residuals of the sum of the terms in the expansion. The residuals should decrease as the order of the multipole increases, until they reach a small enough value that indicates that the series is converging. In the paper by Laskar, the convergence is tested by calculating the maximum absolute residual for each order and checking if it decreases below a certain threshold with increasing order. If this threshold is not reached for a certain set of parameters, then the series is not converging.
 

1. What is the three body disturbing function?

The three body disturbing function is a mathematical function used in celestial mechanics to describe the gravitational interactions between three celestial bodies. It takes into account the masses, positions, and velocities of the three bodies to calculate the effects of their gravitational forces on each other.

2. Why is the convergence of the three body disturbing function important?

The convergence of the three body disturbing function is important because it determines the stability of a three-body system. If the function converges, it means that the system will remain stable over time. However, if the function does not converge, it indicates that the system is chaotic and unpredictable.

3. How is the convergence of the three body disturbing function calculated?

The convergence of the three body disturbing function is calculated using numerical methods, such as the Runge-Kutta method, which involves breaking the function down into smaller steps and iteratively solving for the values at each step. The convergence is determined by comparing the results of these calculations to a predetermined threshold.

4. What factors can affect the convergence of the three body disturbing function?

Several factors can affect the convergence of the three body disturbing function, including the masses, positions, and velocities of the three bodies, as well as the distance between them. Other factors, such as external forces or perturbations, can also have an impact on the convergence of the function.

5. How does the convergence of the three body disturbing function relate to the stability of the solar system?

The convergence of the three body disturbing function is directly related to the stability of the solar system. The fact that the solar system has remained stable for billions of years indicates that the function must converge, meaning that the three-body interactions between the sun, planets, and other celestial bodies are in a state of equilibrium. Any significant changes in the convergence of the function could potentially have a major impact on the stability of the entire solar system.

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