To simulate the solar system in Matlab, we can use Newton's law of gravitation to calculate the gravitational force between each pair of objects and use numerical methods to solve the resulting differential equations. Here is a basic example:
main.m1662 chars55 lines
This script defines the initial conditions of the Sun, Earth, and Moon system, sets up simulation parameters, and defines an Euler method to calculate the motion of the objects over time. The resulting trajectory of the system is plotted using the plot
command.
gistlibby LogSnag