Is it really not possible to obtain an analytical expression for when (if at all) a point $Q$ on a rotating stick will hit a point $P$?

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Say we have a stick on length $L$ that travels toward a point $P$ with linear velocity $v$ in the direction of $P$ and rotational velocity $\omega$. The point and the stick are initially $l$ apart. Will a point $Q$ on the stick, a distance $r$ from its center, hit $P$?

Let the starting position of the stick be such that it points along the $x$-axis and that the center of the stick is at the origin. Looking from the point of view of the stick, the point $P$ will have a velocity $-v$ towards the $x$-axis (and the stick). The initial position of $P$ is $(d,l)$.

The equations of motion are thus \begin{align} \overline{P}&=\begin{pmatrix} d \\ l-vt \end{pmatrix} \\ \overline{Q}&=r\begin{pmatrix}\cos(\omega t) \\ \sin(\omega t) \end{pmatrix} \end{align}

and the question becomes "when is there a $t$ such that the two are equal?"

Introducing $\gamma\equiv\arccos\frac{d}{r}$ (which clearly shows the constraint $r\geq \vert d\vert$), we have

$$\frac{l-\gamma \frac{v}{\omega}}{r}=\sin \gamma$$

However, this looks transcendental.

Is there really no way of analytically figuring out whether or not $Q$ hits $P$? Can we determine whether or not the stick hits at all (for any $Q$)?

Edit: Just an idea: Perhaps one can use the Intermediate value theorem to show that there must exist a solution given some initial conditions?

Edit: Perhaps the question should be "For which $r$s (or some other, single parameter) is $\frac{l-\gamma \frac{v}{\omega}}{r}=\sin \gamma$ true (given $d,\ell,v,\omega$)? Can we say anything sensible about this?

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$$ \frac{\ell - \gamma \frac{v}{\omega}}{r} = \sin\gamma. \tag{*} $$ Perhaps the problem is: Given $\ell,r,v,\omega$, solve for $\gamma$.

This is a transcendental equation. In fact, it is "Kepler's equation", and it is known that the solution (although unique) cannot be written in terms of "elementary functions".

LINK gives Kepler's equation as $$ M=E-e\sin E \tag{K}$$ where we should solve for $E$, given $M$ and $e$. We may substitute $$ E=\gamma \\ e=\frac{-r\omega}{v} \\ M=\frac{\ell \omega}{v} $$ to convert (K) into (*).

That link also discusses algorithms for numerical and series solution of (K).