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The energy-momentum distributions of Einsteins simplest static geometrical model for an isotropic and homogeneous universe are evaluated. For this purpose, Einstein, Bergmann-Thomson, Landau-Lifshitz (LL), Mφller and Papapetrou energy-momentum complexes are used in general relativity. While Einstein and Bergmann-Thomson complexes give exactly the same results, LL and Papapetrou energy-momentum complexes do not provide the same energy densities. The Mφller energy-momentum density is found to be zero everywhere in Einsteins universe. Also, several spacetimes are the limiting cases considered here.