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Introduction

Prior to the Voyager missions and in the presence of only the photographs or the drawings by different authors, the observing results of 1973 mutual events have been much useful to define the physical parameters and the surface morphology of Jupiter and Saturn's satellites. As an example, the comparison between the albedo of eclipsed areas and the loss of light in different colors inferred the existence of bright polar caps, suggested by the drawings (Blanco and Catalano 1974).
Since the Voyager missions have provided accurate radii for all the satellites and described surface features and albedo variations, the observations of mutual events were best used for astrometric purposes. The relative separations in right ascension, cos, and declination, , of a satellite pair at midevent were estimated. The improvement of the integration time up to measures of the order of 0.1 sec, can supply relative positions with relevant residuals near 100 Km at Jupiter's mean distance and near 800 Km in longitude and about half in latitude at Saturn's distance (Aksnes et al. 1984). But after the 1980 campaign the observing conditions were completely changing by the coming of the receptors. Their resolution, of the order of arcsec per pixel, by the analysis of the lightcurve behavior during the event, also with small telescopes, makes it possible to obtain morphological details of the order of few kilometers. The use of several infrared wavelengths during Io's occultations by the other satellites, allows the detection of emitting hot spots associated to an intense volcanism on the first Galilean satellite of Jupiter (Arlot 1988).
The last part of the analysis is devoted to mutual events between Pluto and Charon, the only two bodies of the Solar System that have not been visited by a spacecraft yet. Together with the rare and sporadic stars occultations, mutual events represented the best opportunity to learn a great deal about this particular planetary system, especially to define the surface morphological characteristics of the two bodies. Useful suggestions of Pluto's redder color with respect to Charon's bluer (less red) color came from the different behavior of observed B and V lightcurves.




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