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We discuss Global Static Spherically Symmetric space-time models of mass with regular sources at the origin and asymptotically Minkowskian behavior at infinity; the interior model and the exterior one being matched at the radius of the source in the sense of Lichnerowicz. The global models depend in general on through a function of and . Although would be an spurious parameter if the exterior model was considered alone, it becomes intrinsic for the global model. The physical implication is that as well as determine, at some order of approximation, the dynamics of orbiting objects or viceversa that this dynamics puts conditions on the physical state of the source.

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