Recently I have been reading about Keplerian orbit and I came across the implicit relationship between $r$ and $\theta$ as: $\theta = \theta_{0} + L \int_{r_{0}}^{r} \frac{dr}{r^2} \frac{1}{\sqrt{2(E+1/r-L^2/2r^2)}}$
It's the equation of the path, that means by plotting this equation I should get an ellipse. If I have been provided with initial conditions on $r$, $\theta$, $\dot{r}$ and $\dot{\theta}$, then is it possible to derive all the parameters needed to integrate and plot an orbit numerically?