“…However, if the system is allowed to decelerate, the weight will follow a spiral trajectory that will become increasingly elongated in the vertical direction as the relative contribution of gravitational force grows." (Burrell,[2], p. 1) We focus on a particular deformation (to be specified later) of X = −ny 2n−1 ∂ ∂x +mx 2m−1 ∂ ∂y , with m, n ∈ N\{0} and m+n > 2, or Y = (y−x 2n ) ∂ ∂x with n ∈ N \ {0}. The vector field X has a center at (x, y) = (0, 0), with H(x, y) = x 2m + y 2n as a first integral, while Y has the curve of singularities C = {y = x 2n } and horizontal regular orbits (see Figure 1).…”