  In this work we present an analytical proof of cosmic censorship in a
Kerr-like phantom wormhole (WH) which contains a singularity that is not
protected by an event horizon. We show that the naked singularity of this
space-time is causally disconnected from the universe. To do so, we consider a
slowly rotating limit and by means of the Hamilton-Jacobi theory separate the
Hamiltonian of the geodesics into two polynomials. During this process we find
a fourth conserved quantity. After examining the properties of these
polynomials we conclude that the ring singularity is untouchable by any
observer traveling in a geodesic of this space-time. We also derive the
conditions on the four constants of motion that are necessary for a traveler to
go back and forth both universes connected through the WH, and then compare its
structure to that of a negative mass Kerr black hole.
