The expansive behavior of alumina-magnesia refractory castable, attributed to the in-situ spinel formation, is affected by the magnesia source and its grain size. In the present work, increasing MgO grain size induced cracking, and, consequently, reduced the mechanical properties as a result of a large expansion. Scanning electron microscopy evaluations after firing at 1500 ºC showed distinct microstructures for castables containing different grain sizes (< 45 µm and < 100 µm). For the composition with finer magnesia, phases commonly detected in the literature were observed: spinel and CA6. Nevertheless, besides those two phases, the castable with the coarse magnesia also presented forsterite and monticellite around the magnesia remaining grains. Hence, the objective of this work is to analyze how the refractory castable properties could be considerably affected even by changing a single parameter: the magnesia grain size.
MgO grain size; microstructure; in-situ spinel formation
