Put . For , the solution of the linear secular forcing of a test particle equation is
The initial condition gives and . The proper eccentricity is the constant amplitude of the homogeneous response; its proper longitude of periapsis is . The forced eccentricity is the driven vector , not necessarily a constant magnitude.
On an Argand diagram, describes a circle of radius . Its center can itself move under the planetary modes, so need not trace one fixed circle in the inertial complex plane. At a secular resonance , that mode instead produces , and the undamped linear response grows until the approximation fails.
Figure 1. . Left: proper eccentricity around the forced vector. Middle: the annulus generated by a common semimajor axis and random proper phases. Right: a family of aligned orbits with constant forced eccentricity and a range of semimajor axes.