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In this paper we present a new simple method of construction of infinitenumber of solutions of Freidmann equations from the already known ones, whichallows for a startling conclusion of practical impossibility of correctpredictions on the universe's future dynamics which are based solely onastronomical observations on the value of a scale factor. In addition, wepresent particular examples of newly constructed solutions, such as the ones,describing the smooth dynamical (de)-phantomization, and the models lacking theevents horizons (both in classical and brane world cases). The generalizationof the method to the simplest anisotropic universes are presented as well.Comment: New version: 8 pages, RevTeX; the old title ''The dressing procedure  for the Friedmann equations and the indefinite future of the universe''; the  results about anisotropic cosmological models and references are adde

The dressing procedure for the cosmological equations and the indefinite future of the universe