Morphology, Structure, and Origin of Island Paterae on Io

We are investigating both the small and large scale morphology of those paterae on Jupiter's moon Io which show central islands. At small scales a variety of features may be evidence of volatile transport processes. For example Loki Patera contains small bright spots colloquially known as sulfur bergs, which we suspect are fumarole deposits. They are near the limit of the best spatial resolution obtained in Voyager I images. Our preliminary results indicate their reflectance is consistent with sulfur (but not sulfur dioxide) as would be expected based on the temperatures seen in the infrared. At large scales we are beginning to model the stress patterns which could produce the overall morphology of island paterae. As discussed by Radebaugh (Ph.D. Dissertation, 2005) and Black (M.S. thesis, 2007), of 428 cataloged patera on Io, 35 contain bright islands. Most of these islands are irregularly shaped and may simply be regions not yet covered by lava. However several paterae, in particular Loki and Tupan, show more regular structure. Both patera have one straight edge, and in the case of Loki the most volcanically active part of the patera is located near that edge. As Turtle et al. (2001 JGR 106: 33175) and others have suggested, those straight edges may be faults which relieve the expected global compressive stresses and also act as magma conduits. Radebaugh (2005) has suggested that some of these large islands might be analogs of resurgent domes. We are investigating whether a hybrid stress model may be able to explain the overall morphology.