I am working on a problem about navigation assuming a perfect sphere and hence ignore any spheroidal effects. I would like to be able to describe the shortest trajectory between two points and be able to do some kinematics.
I am aware that if I have two points on the globe, the shortest path between them is an arc of a great circle. I looked up online and by using spherical trigonometry, especifically, the spherical law of cosines, the lenght of this arc can be found to be
$$ \ell = R\Delta\sigma = R\arccos(\sin\phi_1\sin\phi_2 + \cos\phi_1\cos\phi_2\cos\Delta\lambda), $$
where $\Delta \sigma$ is the so-called central angle, $R$ the mean radius of the Earth and $(\phi_1,\lambda_1)$ and $(\phi_2,\lambda_2)$ are two points on the globe in terms of the latitute $\phi$ and longitude $\lambda$. Now, given a departure point $(\phi_1,\lambda_1)$, I can know how much distance until a later point in this trajectory and even calculate travel time assuming a constant cruising speed $\overline{v}$, since that's just $\Delta t= \ell/\overline{v}$.
Then comes the point where I am currently stucked. Assuming the aforementioned average cruising speed $\overline{v}$ and this great-circle trajectory with departure at $(\phi_1,\lambda_1)$ how can I calculate a later position given some elapsed time $\Delta t$?
Thank you in advance for any input!