simulate the solar system in matlab

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.m
% Define initial conditions
G = 6.67430e-11; % gravitational constant
Ms = 1.989e30; % mass of the Sun
Me = 5.97e24; % mass of the Earth
Mm = 7.34e22; % mass of the Moon
rse = 147.09e9; % distance between Sun and Earth
rem = 384.4e6; % distance between Earth and Moon
vse = 30.29e3; % velocity of Earth
vem = 1.02e3; % velocity of Moon
x = [0 rse+rse*cosd(23.5) rem+rse+rse*cosd(23.5)]'; % initial x positions
y = [0 0 rse*sind(23.5)+rem+sind(23.5)*rse]'; % initial y positions
vx = [0 vse*cosd(23.5) vem+vse*cosd(23.5)]'; % initial x velocities
vy = [0 vse*sind(23.5) vse*sind(23.5)+vem]'; % initial y velocities
m = [Ms Me Mm]'; % masses

% Set up simulation parameters
dt = 100; % time step in seconds
tmax = 365*24*60*60; % total simulation time in seconds
t = 0:dt:tmax;
n = length(m);

% Initialize position and velocity matrices
r = [x y];
v = [vx vy];

% Simulate motion using the Euler method
for i = 1:length(t)-1
    % Calculate gravitational forces
    F = zeros(n,2);
    for j = 1:n
        for k = 1:n
            if j ~= k
                rjk = r(k,:) - r(j,:);
                F(j,:) = F(j,:) + G*m(j)*m(k)*rjk/norm(rjk)^3;
            end
        end
    end
    % Update positions and velocities
    r = r + v*dt + 0.5*dt^2*F./m;
    v = v + dt*F./m;
end

% Plot results
figure
hold on
plot(r(:,1),r(:,2),'linewidth',2) % plot trajectory of Sun-Earth-Moon system
plot(x(1),y(1),'r.','markersize',40) % plot Sun
plot(x(2),y(2),'b.','markersize',20) % plot Earth
plot(x(3),y(3),'k.','markersize',10) % plot Moon
axis equal
xlabel('x (m)')
ylabel('y (m)')
title('Solar System Simulation')
legend('Sun-Earth-Moon trajectory','Sun','Earth','Moon')
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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.

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