The Isothermal Dendritic Growth Experiment constituted a series of three NASA-supported microgravity experiments (USMP-2, -3, and -4), which flew aboard the space shuttle Columbia. These space flight experiments grew and recorded dendrites in the absence of gravity-induced convective heat transfer. USMP-4, for the first time, allowed streaming of near-real-time video data. Using 30-fps video data, we studied both freezing and melting sequences for pivalic acid (PVA) at different supercoolings. We report on the melting process of a PVA dendritic mushy zone, observed for the first time under convection-free conditions. Conduction-limited melting processes are of importance in orbital melting of materials, meteoritic genesis, mushy-zone evolution, and in fusion weld pools where the length scales for thermal buoyancy are highly restricted. Microgravity video data show that PVA dendrites melt into fragments that shrink at accelerating rates to extinction. The melting paths of individual fragments follow a characteristic time dependence for the diminishing length scales within the mushy zone. The theoretical melting kinetics against which the experimental observations are compared is based on the conduction-limited quasi-static process of melting under shape-preserving conditions. Good agreement between theory and experiment was found for the melting of a selected needle-shaped prolate spheroidal PVA crystal fragment with an aspect ratio of C/A = 12.