New solutions are found for the non-relativistic hydrodynamical equations. These solutions describe expanding matter with a Gaussian density profile. In the simplest case, thermal equilibrium is maintained without any interaction, the energy is conserved, and the process is isentropic. More general solutions are also obtained that describe explosions driven by heat production, or contraction of the matter caused by energy loss.Introduction. The equations of hydrodynamics correspond to local conservation of some charges as well as energy and momentum. The equations are scale-invariant, hence can be applied to phenomenological description of physical phenomena from collisions of heavy nuclei to collisions of galaxies. Recently, a lot of experimental and theoretical effort went into the exploration of hydrodynamical behaviour of strongly interacting hadronic matter in non-relativistic as well as in relativistic heavy ion collisions, see for example refs.[1]- [7]. Due to the non-linear nature of the equations of hydrodynamics, exact solutions of these equations are rarely found. In ref.[2] an exact solution of hydrodynamics of expanding fireballs was found 20 years ago. The purpose of this Letter is to present and analyze a new, exact solution of the non-relativistic hydrodynamical equations, with a generalization to heat production or loss (e.g. due to radiation). We hope that the results presented herewith may be utilized to access analytically the time-evolution of the hydrodynamically behaving strongly interacting matter as probed by non-relativistic heavy ion collisions [4,5]. The results are, however, rather general in nature and they can be applied to any physical phenomena where the non-relativistic hydrodynamical description is valid.Adiabatic expansion. Consider a hydrodynamical system described by the continuity equation, the Euler equation and the local energy conservation: