What is wrong with my code, my equation is vdv/dy=-G*M/(y+R)^2 ?

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Laura
Laura el 4 de Abr. de 2023
Editada: Torsten el 4 de Abr. de 2023
cssCopy codefunction dydt = gravity(y, v, G, M, R)
% y: height above surface
% v: velocity at height y
% G: gravitational constant
% M: mass of the planet
% R: radius of the planet
dydt(1,1) = v; % v = dy/dt
dydt(2,1) = -G*M/(y+R)^2; % a = d^2y/dt^2 = dv/dt
end
scssCopy codeG = 6.67430e-11; % gravitational constant
M = 5.9722e24; % mass of Earth
R = 6.371e6; % radius of Earth
  7 comentarios
Dyuman Joshi
Dyuman Joshi el 4 de Abr. de 2023
Editada: Dyuman Joshi el 4 de Abr. de 2023
@Laura I am well aware that you are trying to solve the equation by MATLAB, that is not my point.
For what time range are you trying to solve the equation? What are the initial conditions to the differential equation?

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Respuestas (2)

Sam Chak
Sam Chak el 4 de Abr. de 2023
Editada: Sam Chak el 4 de Abr. de 2023
This is a simple example of using the solver's syntax that you can find in the ode45() documentation. If there are universal constants that they don't change, then place them inside the ode function, as suggested by @Dyuman Joshi. Otherwise, parameters that you would like to test with different value (i.e., mass), then you can pass the parameters to the ode function like @Cris LaPierre did.
What you need to do is to replace my free fall ODE with your description of Newton's law of universal gravitation.
Logically, when the object (point mass) hits the ground, then the simulation should stop. Anyhow, get familiar with the basic code. Click into the documentation for more examples.
% solving the ODE
tspan = [0 6]; % simulation time
y0 = [100 0]; % initial condition y(1) = 100 m; y(2) = 0 m/s
[t, y] = ode45(@freefall, tspan, y0);
% plotting the solution y(1)
plot(t, y(:,1), 'linewidth', 1.5),
xlabel('Time (sec)'), ylabel('Height (m)')
yline(0, '--', 'Ground level');
yregion(-80, 0)
% Describing the ODE
function dydt = freefall(t, y)
m = 1; % point mass
g = 9.8203; % gravity
dydt(1,1) = y(2); % dy/dt
dydt(2,1) = -g/m; % assume no air drag
end

Torsten
Torsten el 4 de Abr. de 2023
syms G M R y v(y)
Dv = diff(v,y);
eqn = diff(v,y,2) == -G*M/(y+R)^2;
cond = [v(0)==100,Dv(0)==0];
sol = dsolve(eqn,cond)
sol = 
Gnum = 6.67430e-11; % gravitational constant
Mnum = 5.9722e24; % mass of Earth
Rnum = 6.371e6; % radius of Earth
sol = vpa(subs(sol,[G M R],[Gnum,Mnum,Rnum]))
sol = 
fplot(sol,[0 6])
  2 comentarios
Dyuman Joshi
Dyuman Joshi el 4 de Abr. de 2023
@Torsten, the equation you wrote is incorrect.
It's
v*diff(v,y)
instead of
diff(v,y,2)
And it needs only 1 intial condition
Torsten
Torsten el 4 de Abr. de 2023
Editada: Torsten el 4 de Abr. de 2023
I also thought so first , but Laura's code (and all answers and comments thereafter) speak another language.
I think d^2v/dy^2 was misinterpreted as d(0.5*v^2)/dy.

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