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Thermal Diapirism and the Habitability of the Icy Shellof Europa
Authors:Javier Ruiz  Lilia Montoya  Valle López  Ricardo Amils
Institution:(1) Instituto de Astrofísica de Andalucía, CSIC, Camino Bajo de Huétor 50, 18008 Granada, Spain;(2) Centro de Biología Molecular, CSIC-Universidad Autónoma de Madrid, 28049, Cantoblanco, Madrid, Spain;(3) Seminario de Ciencias Planetarias, Facultad de Ciencias Geológicas, Universidad Complutense de Madrid, 28040 Madrid, Spain;(4) Centro de Astrobiología, INTA, 28855, Torrejón de Ardoz, Madrid, Spain
Abstract:Europa’s chaos and lenticulae features may have originated by thermal diapirs related to convective plumes. Warm ice plumes could be habitable, since their temperature is close to the ice melting temperature. Moreover, thermal plumes intruding into the lower stagnant lid warm several kilometers of country ice above 230 K for periods of 105 years, and hundreds of meters above 240 K for periods of 104 years. Diapir coalescence generating chaos areas should provide a large zone with temperature above ∼240 K for thousands of years. A temperature above ∼230 K is potentially interesting for astrobiology, since it corresponds to the lowest temperature at which microbial metabolic activity in Antarctic ice has been reported. So, the warming by thermal plumes could cause an aureole of biological activation/reactivation in the country ice. Adaptation of life to either high salinity or low temperature is similar: it requires the synthesis of compatible solutes, like trehalose or glycerol, which are efficient cryoprotectants. We therefore propose that the future astrobiological exploration of Europa should include the search for compatible solutes in chaos and lenticulae features.
Keywords:Astrobiology  Compatible solutes  Europa  Habitability  Thermal diapirism
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