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only need MATLAB code Use Euler integration to integrate the following equation for the motion of earth around the sun dt2d2r1=Gm2r1(t)r2(t)3r1(t)r2(t), gravitational constant, and m2=1.9891030kg
only need MATLAB code
Use Euler integration to integrate the following equation for the motion of earth around the sun dt2d2r1=Gm2r1(t)r2(t)3r1(t)r2(t), gravitational constant, and m2=1.9891030kg is the mass of the sun. You may assume r2(t)=0 at all times. Plot the trajectory of the earth for 2 years. Does the earth traverse the same path in the second year? if not, fix your time-step size until it does. What timestep size did you select? (hint: the equation above is a set of three uncoupled differential equations; use plot3 in MATLAB to plot the trajectory). Organize your code into sections before publishing it as a pdf. Append this pdf to the rest of the homework in a proper locationStep by Step Solution
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