Orbit of satellite 2nd order ODE using Matlab

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The discussion revolves around solving a set of second-order differential equations for a geosynchronous satellite orbit using Euler's method in MATLAB. The equations describe the motion with respect to the circular orbit, where the velocity vector is perpendicular to the radius vector. The user has correctly reformulated the equations into a system of first-order ODEs but is unsure about the initial conditions for the variables. It is clarified that any initial position on the circular orbit can be used, with the velocity calculated as the orbit's circumference divided by one sidereal day. The conversation emphasizes the importance of understanding initial conditions in the context of orbital mechanics.
olski1
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Hi,

I am completely stuck on this problem that has been given to us.

I must solve a set of 2nd order differential equations using Euler's method. It is for a geosychronous orbit of a satellite, meaning the orbit is circular and the velocity vector is perpendicular to the radius vector (r.V=0). The equations are:

d2x/dt2=-k2x/r3

and

d2y/dt2=-k2y/r3

k^2,r and V are all given.

My first step was to set up sets of ode's to solve.

for the first equation we have,

let y1=x and y2=dy1/dt

hence, dy2/dt= -k2y1/r3

and for the second,

let y3=y and y4=dy3/dt

hence, dy4/dt= -k2y3/r3

which I think is correct.

Now I have to pass this into a MATLAB function which uses eulers method. But I have no idea how to implement it. my main problem at the moment is that I do not know what to use as my initial y1,2,3,4 values in the function vector.

Can anyone help?
 
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I am not sure why anyone would want to solve and ODE for motion which is completely known, but still.

You can take any initial position as long as it is on the orbit (circle). The velocity, as you say, is perpendicular to it and must be equal to the length of the orbit divided by one sidereal day.
 
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