Spectral Units on the Icy Galilean Satellites from Voyager Imagery

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We are performing new analyses of the visible Voyager imagery in order to more accurately define spectral units on the icy Galilean satellites in an attempt to provide the best context for the Galileo mission results. The Galileo imaging system and the NIMS, with a resolution of up to 1 km, are returning superior spectral imagery to Voyager but only for selected regions of the satellites. Therefore, the Voyager data remains an important source of information. We use revised Voyager spectral images, formatted in an image cube calculated by Granahan et al. [1] to produce improved mosaics of the icy satellites in a format similar to those of Nelson et al. [2]. However, these data are superior to those used in these and other earlier analyses [2,3] due to a better calibration and improved software which enable a more accurate smoothing of the boundaries between image frames reducing the chance of misconstruing irregularities in the photometric function correction for compositional differences. We are presenting displays of spectral units for Ganymede and Callisto with the color assignments indicative of the spectral nature of the unit. These satellites show consistent evidence of surface emplacement of materials of exogenic and endogenic origin. [1] Granahan, J.C., K.S. Polk, F.P. Fanale, and T.B. McCord (1996) Lunar Planet. Sci. XXVII (abstract), 443-444. [2] Nelson, M.L., T.B. McCord, R.N. Clark, T.V. Johnson, D.L. Matson, J.A. Mosher, and L.A. Soderblom (1986). Icarus 65, 129-151. [3] Johnson, R.E., M.L. Nelson, T.B. McCord, and J.C. Gradie (1988). Icarus 75, 423-436. Johnson, T.V., L.A. Soderblom, J.A. Mosher, G.E. Danielson, A. F. Cook, and P. Kupferman (1983).J. Geophys. Res. 88, 5789-5805. McEwen, A.S. (1986). J. Geophys. Res. 91, 8077-8097.

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