We report the discovery of a double ring structure in the waist of the nebu
la surrounding eta Carinae. The rings are detected in the mid-IR dust conti
nuum at wavelengths of 7.9, 11.9, 12.9 and 20 mum. The dust in the rings ha
s a temperature of about 300 K. The orientation of the rings is inclined wi
th respect to the axis of the homunculus by either 37 or 58 degrees. The ce
ntral star is not in the projected centre of the structure defined by the t
wo rings. This geometry is reminiscent of that seen in SN1987A and some pla
netary nebulae. We discuss several possible origins for this remarkable geo
metry and its orientation.