The two known exact solutions of Einstein's field equations describing rota
ting objects of physical significance - a black hole and a rigidly rotating
disk of dust - are discussed using a single mathematical framework related
to Jacobi's inversion problem. Both solutions can be represented in such a
form that they differ in the choice of a complex parameter and a real solu
tion of the axisymmetric Laplace equation only.
A recently found family of solutions describing differentially rotating dis
ks of dust fits into the same scheme.