To simulate the orbit of a satellite in the Earth-Moon system, we can use the following steps:
Define the parameters of the system, such as the masses of the Earth and the Moon, the distance between them, and the initial position and velocity of the satellite.
Use the gravitational force formula to calculate the acceleration of the satellite due to the gravitational attraction of the Earth and the Moon.
Update the position and velocity of the satellite using numerical integration techniques, such as Euler's method, Runge-Kutta method, or Verlet integration.
Repeat steps 2 and 3 for a certain number of time steps to simulate the orbit of the satellite.
Here's an example implementation of a simulation using Euler's method in Python:
main.py1165 chars45 lines
This code simulates the orbit of a satellite in the Earth-Moon system using Euler's method. It calculates the acceleration of the satellite due to the gravitational attraction of the Earth and the Moon, and updates its position and velocity using small time steps. The resulting trajectory of the satellite is plotted in a 3D graph using Matplotlib.
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