This paper presents a rigorous generalization of the classical Bäcklund transformation (BT) for space curves in Euclidean 3-space \(\mathbb {E}^{3}\) using the versatile quasi-frame (q-frame). The novelty lies in introducing the frame rotation angle, \(\theta (s)\) , as a continuous geometric control parameter for designing BTs that satisfy fundamental geometric constraints, notably the constant separation distance r. We derive a coupled system of first-order ordinary differential equations (ODEs) governing the evolution of both the frame rotation \(\theta (s)\) and the inclination angle \(\gamma (s)\) of the transformation. A key theoretical contribution is the demonstration that this class of BTs universally preserves the second quasi-curvature ( \(\tilde{\kappa }_{2}\) ) and the quasi-torsion ( \(\tilde{\tau }\) ) of the q-frame, implying that the geometric action is concentrated solely on the first quasi-curvature ( \(\kappa _1\) ). This invariance offers deep, intrinsic insight into the geometric nature of the transformation. Our formulation naturally encompasses the classical Frenet and Bishop frame BTs as special static cases. Numerical simulations starting from a circular helix illustrate the framework’s ability to generate complex, non-helical curves under specific dynamic geometric constraints, highlighting the utility of \(\theta (s)\) in geometric control theory.