In the short span of a few hours, an accreting neutron star releases an X-ray Superburst with an energy equivalent to the energy output of our sun over a decade. The energy source driving this phenomenon with its spectacular energy release is presently unknown. It has been proposed that the Superburst is triggered by the fusion of in the neutron star’s outer crust. This scenario requires that fusion of neutron-rich light nuclei is enhanced relative to their β-stable counterparts. To investigate this hypothesis and better understand the fusion dynamics for such nuclei, we have launched an experimental effort to measure the total fusion cross-section for beams of low-intensity, neutron-rich nuclei (< 105 ions/s) such as 18O,19O, and 20O on light targets at energies near and below the Coulomb barrier. Evaporation residues, resulting from the fusion of oxygen and 12C nuclei, were identified by their energy and time-of-flight. Using this technique, the fusion excitation function was measured in the sub-barrier domain down to the ~800 µb level. Extension of our initial measurements of 18O + 12C using a radioactive beam of 19O will be described. Fusion of 19O ions on the 12C target is enhanced three-fold at near barrier energies as compared to 18O. This significant enhancement in the fusion cross-section is remarkable. The results of these initial measurements will be presented along with theoretical calculations and the prospect of extending these measurements to lower energies and other projectile-target combinations will be discussed.