Hydrated minerals on Europa's surface: An improved look from the Galileo NIMS investigation

To link to full-text access for this article, visit this link: http://dx.doi.org/10.1016/j.icarus.2010.05.026 Byline: Thomas B. McCord (a), Gary B. Hansen (b), Jean-Philippe Combe (a), Paul Hayne (a)(c) Keywords: Europa; Jupiter, Satellites; Satellites, Composition; Spectroscopy Abstract: The surface composition of Europa is of great importance for understanding both the internal evolution of Europa and its putative ocean. The Near Infrared Mapping Spectrometer (NIMS) investigation on Galileo observed Europa and the other Galilean satellites from 0.7 to 5.2[mu]m with spatial resolution down to a few kilometers during flybys by the spacecraft as it orbited Jupiter. These data have been analyzed and results published over the life of the Galileo mission and afterward. One result was the discovery of hydrated minerals at some locations on Europa and Ganymede. The data are noisy, especially for Europa, due to radiation affecting the NIMS electronics and detectors, and other artifacts are also present. The NIMS data are now being reprocessed using the accumulated knowledge gained over the entire missions to remove noise spikes and compensate for some other defects in the data. We are analyzing these reprocessed data in an attempt to defined better the nature of the hydrate spectral features and improve their interpretation. We report here on analyses of two NIMS reprocessed observations for the 0.7-3-[mu]m region. A revised hydrate spectrum is calculated and mapped in detail across two lineaments. The spectrum shows the expected distorted water features but little or no spectral structure in these features. A narrow, weak spectral feature appears at 1.344[mu]m, which is weakly correlated with lower albedo. Several other weak features may be present but are difficult to confirm in these limited data sets. The hydrate signature shows the greatest strength within and toward the center of the lineaments, confirming and strengthening the association of the hydrate with these endogenic features. This trend may indicate that the material in the lineaments is youngest toward the center and has more water frost coverage toward the edge. A small, visually dark, circular feature has a spectrum that shows both hydrate and crystalline water ice features and perhaps contains a hydrate different in spectral characteristics and perhaps composition than found in the lineament. Author Affiliation: (a) The Bear Fight Center, P.O. Box 667, 22 Fiddler's Road, Winthrop, WA 98862, United States (b) Dept. of Earth and Space Sci, University of Washington, Seattle, WA 98195, United States (c) Dept. of Earth and Space Sci, University of California, Los Angeles, CA 90095, United States Article History: Received 13 January 2009; Revised 23 May 2010; Accepted 31 May 2010