 Damped first-order resonant complex eccentricity

For an exterior $(p+1):p$ mean-motion resonance, use mean longitude in $\varphi =(p+1)\lambda -p{\lambda }_p-\varpi$, $z=e\exp (i\varphi )$, $x=(a-a_r)/a_r$ and $B=3p{n}_p/2$. Given $\dot{e}=-C\sin \varphi -Ae$ and $\dot{\varpi }=(C/e)\cos \varphi$, the leading Keplerian detuning gives $\dot{\varphi }=-Bx-(C/e)\cos \varphi$. Differentiating $z$ and using $e^{i\varphi }(\sin \varphi +i\cos \varphi )=i$ proves the displayed equation. It retains resonant forcing and eccentricity damping without the coordinate singularity at $e=0$. True longitude adds a fast orbital ripple and does not yield this autonomous averaged equation directly.