The magnetic interaction of a line current source and a superconducting sphere in the Meissner state is studied theoretically. An analytic solution for the magnetostatic scalar potential Φ yielding the image system due to the induced current line positioned at x = d and y = 0 in front of a sphere of radius a is obtained by mimicking an approach utilized earlier in hydrodynamics. The method resulted in an image system consisting of edge and surface currents all located in a circle inside the superconducting sphere. The magnetic field components B x , B y , B z , B r are generated from our exact solution, revealing certain symmetries with respect to the coordinates. It is demonstrated that various non-dimensional parameters including radius-distance ratio, which can be expressed as \(\frac {a}{d}\) or \(\frac {d}{a}\), influence the magnetic field significantly. The contour plots of the radial component portray contrasting patterns along the three coordinate planes confirming the true nature of three-dimensionality. Radial and axial components are found to have extreme values indicating strong interaction between the line current and the sphere. The levitation force on the superconducting sphere is extracted directly from the analytic solution and is expressed as a quadrature. The expression for the interaction force has a logarithmic contribution and further depends on the z coordinate. It is found that when the line current is very close to the superconductor (\(\frac {a}{d} \sim 1\)), the force is singular in the limit \(\frac {z}{d} \rightarrow 0\). The singular behavior and z dependence property of the force are new and do not occur in source-sphere and dipole-sphere superconducting systems. The computed levitation force is maximum when the line current is positioned closer to the sphere and minimum when it is farther from the sphere. It is shown numerically that the order of magnitude of the increase of the force going from large to small separations is 104. The simple nature of our theoretical results can be directly applied to models for magnetic levitation and magnetic microscopy.