While writing my former post Pluto Transiting Sagittarius Ascendant: More Thoughts something strange but fabulous happened.

@article{8480, author = {Saur, J. and Politano, H. and Pouquet, A. and Matthaeus, W.H.}, format = {print}, journal = {Astron. Astrophys.}, keywords = {Jupiter, Magnetohydrodynamics, Magnetohydrodynamic turbulence, Turbulence}, month = {May}, pages = {699--708}, refdb_id = {http://solarphysics.livingreviews.org/refdb/record/8480}, title = {Evidence for weak MHD turbulence in the middle magnetosphere of Jupiter}, volume = {386}, year = {2002} }

@article{8478, author = {Saur, J. and Pouquet, A. and Matthaeus, W.H.}, format = {print}, journal = {Geophys. Res. Lett.}, keywords = {Auroral phenomena, Jupiter, Magnetosphere}, month = {July}, pages = {19--22}, refdb_id = {http://solarphysics.livingreviews.org/refdb/record/8478}, title = {Correction to ``An acceleration mechanism for the generation of the main auroral oval on Jupiter''}, volume = {30}, year = {2003} }

@article{8566, author = {Smith, C.W. and Goldstein, M.L. and Matthaeus, W.H.}, format = {print}, journal = {J. Geophys. Res.}, keywords = {Bow waves, Energetic particles, Jupiter, Magnetohydrodynamic waves, Planetary magnetic fields, Plasma turbulence, Power spectra, Shock waves, Solar planetary interactions, Solar wind, Space plasmas, Voyager}, month = {July}, number = {17}, pages = {5581--5593}, refdb_id = {http://solarphysics.livingreviews.org/refdb/record/8566}, title = {Turbulence analysis of the Jovian upstream wave phenomenon}, volume = {88}, year = {1983} }

A striking similarity between the moons of Jupiter, Saturn and Uranus could be explained by a new model of how they formed.