In this study, the effect of rhenium (Re) addition on microstructural evolution of a new low-density Co-Ni-Al-Mo-Nb based superalloy is presented. Addition of Re significantly influences the g 0 precipitate morphology, the g/g 0 lattice misfit and the g/g 0 microstructural stability during long term aging. An addition of 2 at.% Re to a Co-30Ni-10Al-5Mo-2Nb (all in at.%) alloy, aged at 900 C for 50 h, reduces the g/ g 0 lattice misfit by~40% (from þ0.32% to þ0.19%, measured at room temperature) and hence alters the g 0 morphology from cuboidal to round-cornered cuboidal precipitates. The composition profiles across the g/g 0 interface by atom probe tomography (APT) reveal Re partitions to the g phase (K Re ¼ 0:34Þ and also results in the partitioning reversal of Mo to the g phase (K Mo ¼ 0:90) from the g 0 precipitate. An inhomogeneous distribution of Gibbsian interfacial excess for the solute Re (G Re , ranging from 0.8 to 9.6 atom.nm À2) has been observed at the g/g 0 interface. A coarsening study at 900 C (up to 1000 h) suggests that the coarsening of g 0 precipitates occurs solely by evaporationecondensation (EC) mechanism. This is contrary to that observed in the Co-30Ni-10Al-5Mo-2Nb alloy as well as in some of the Ni-Al based and high mass density CoAl -W based superalloys, where g 0 precipitates coarsen by coagulation/coalescence mechanism with an extensive alignment of g 0 along <100> directions as a sign of microstructural instability. The g 0 coarsening rate constant ðK r Þ and g/g 0 interfacial energy are estimated to be 1.13 Â 10 À27 m 3 /s and 8.4 mJ/m 2 , which are comparable and lower than CoAl -W based superalloys.