  Given an integer $\kappa\geq2$, we introduce a class of nearly integrable
systems on $\mathbb{A}^3$, of the form $$ H_n(\theta,r)=\frac12 \Vert r\Vert
^2+\tfrac{1}{n} U(\theta_2,\theta_3)+f_n(\theta,r) $$ where $U\in
C^\kappa(\mathbb{T}^2)$ is a generic potential function and $f_n$ a
$C^{\kappa-1}$ additional perturbation such that $\Vert
f_n\Vert_{C^{\kappa-1}(\mathbb{A}^3)}\leq \tfrac{1}{n}$, so that $H_n$ is a
perturbation of the completely integrable system $h(r)=\frac12\Vert r\Vert ^2$.
  Let $\Pi:\mathbb{A}^3\to\mathbb{R}^3$ be the canonical projection. We prove
that for each $\delta>0$, there exists $n_0$ such that for $n\geq n_0$, the
system $H_n$ admits an orbit $\Gamma_n$ at energy $\frac12$ whose projection
$\Pi(\Gamma_n)$ is $\delta$-dense in $\Pi(H_n^{-1}(\tfrac{1}{2}))$, in the
sense that the $\delta$-neighborhood of $\Pi(\Gamma_n)$ in $\mathbb{R}^3$
covers $\Pi(H_n^{-1}(\frac{1}{2}))$.
