Exo-Ocean Exploration with Deep-Sea Sensor and Platform Technologies J Aguzzi, M Flexas, S Flögel, C Lo Iacono, M Tangherlini, C Costa, S Marini, N Bahamon, S Martini, E Fanelli, et al. To cite this version: J Aguzzi, M Flexas, S Flögel, C Lo Iacono, M Tangherlini, et al.. Exo-Ocean Exploration with Deep- Sea Sensor and Platform Technologies. Astrobiology, Mary Ann Liebert, 2020, 20 (7), pp.897 - 915. 10.1089/ast.2019.2129. hal-03203246 HAL Id: hal-03203246 https://hal.archives-ouvertes.fr/hal-03203246 Submitted on 20 Apr 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. AST-2019-2129-ver9-Aguzzi_1P.3d 02/29/20 4:48am Page 1 AST-2019-2129-ver9-Aguzzi_1P Type: review-article ASTROBIOLOGY Volume 20, Number 7, 2020 Review Article ª Mary Ann Liebert, Inc. DOI: 10.1089/ast.2019.2129 Exo-Ocean Exploration with Deep-Sea Sensor and Platform Technologies J. Aguzzi,1,2 M.M. Flexas,3 S. Flo¨gel,4 C. Lo Iacono,1,5 M. Tangherlini,2 C. Costa,6 S. Marini,7 N. Bahamon,1 S. Martini,8 E. Fanelli,2,9 R. Danovaro,2,9 S. Stefanni,2 L. Thomsen,10 G. Riccobene,11 M. Hildebrandt,12 I. Masmitja,13 J. Del Rio,13 E.B. Clark,14 A. Branch,14 P. Weiss,15 A.T. Klesh,14 and M.P. Schodlok14 Abstract One of Saturn’s largest moons, Enceladus, possesses a vast extraterrestrial ocean (i.e., exo-ocean) that is increasingly becoming the hotspot of future research initiatives dedicated to the exploration of putative life. Here, a new bio-exploration concept design for Enceladus’ exo-ocean is proposed, focusing on the putative presence of organisms across a wide range of sizes (i.e., from uni- to multicellular and animal-like), according to state-of-the-art sensor and robotic platforms, technologies used in terrestrial deep-sea research. In particular, we focus on combined direct and indirect life-detection capabilities, based on optoacoustic imaging and passive acoustics, as well as molecular approaches. Such biologically oriented sampling can be accompanied by concomitant geochemical and oceanographic measurements to provide data relevant to exo-ocean exploration and understanding. Finally, we describe how this multidisciplinary monitoring approach is currently enabled in terrestrial oceans through cabled (fixed) observatories and their related mobile multiparametric platforms (i.e., Autonomous Underwater and Remotely Operated Vehicles, as well as crawlers, rovers, and biomimetic robots) and how their modified design can be used for exo-ocean exploration. Key Words: Exo-ocean—Enceladus— Deep-sea technology—Autonomous underwater vehicles—Crawlers—Cryobots. Astrobiology 20, xxx–xxx. 1. Introduction subsurface ocean, such as Saturn’s moon Dione, Neptune’s icy moon Triton, and the dwarf planet Pluto. Moreover, the iquid water is present in the form of vast extraterres- dwarf planet Ceres seems to have at least a subsurface sea Ltrial oceans (i.e., exo-oceans) on various icy moons of (Henin, 2018). our solar system (NASEM, 2018; Hendrix et al., 2019; Ka- The primary conditions under which we could expect to mata et al., 2019). Five icy moons have been confirmed as find extant life in exo-oceans (although this hypothesis is ocean worlds, namely, three satellites of Jupiter (Europa, still uncertain at this stage of scientific research) are the Ganymede, and Callisto) and two of Saturn (Enceladus and presence of energy sources that facilitate a non-equilibrium Titan, the latter with an exo-ocean below a thick hydrocarbon thermodynamic state of a marine-like medium containing layer; Iess et al., 2012). Another four are likely to host a abundant organic compounds (Schwieterman et al., 2018). 1Instituto de Ciencias del Mar (ICM-CSIC), Barcelona, Spain. 2Stazione Zoologica Anton Dohrn, Naples, Italy. 3California Institute of Technology, Pasadena, California, USA. 4GEOMAR Helmholtz Centre for Ocean Research Kiel, Kiel, Germany. 5National Oceanographic Center (NOC), University of Southampton, Southampton, United Kingdom. 6Consiglio per la ricerca in agricoltura e l’analisi dell’economia agraria (CREA)-Centro di ricerca Ingegneria e Trasformazioni agroalimentari - Monterotondo, Rome, Italy. 7National Research Council of Italy (CNR), Institute of Marine Sciences, La Spezia, Italy. 8Sorbonne Universite´, CNRS, Laboratoire d’Oce´anographie de Villefranche, Villefranche-sur-mer, France. 9Department of Life and Environmental Sciences, Polytechnic University of Marche, Ancona, Italy. 10Jacobs University, Bremen, Germany. 11Istituto Nazionale di Fisica Nucleare (INFN), Laboratori Nazionali del Sud, Catania, Italy. 12German Research Center for Artificial Intelligence (DFKI), Bremen, Germany. 13SARTI, Universitat Polite`cnica de Catalunya (UPC), Barcelona, Spain. 14Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA. 15COMEX, Marseille, France. 1 AST-2019-2129-ver9-Aguzzi_1P.3d 02/29/20 4:48am Page 2 2 AGUZZI ET AL. Among the above-mentioned icy moons, Enceladus and primary producers, grazers, predators, scavengers, and re- Europa meet these conditions. Both host large water-based mineralizing organisms (e.g., Lelie`vre et al., 2018). oceans in which geothermal activity is present and where Unfortunately, exploration for life in Enceladus’ exo- life could be possible (Manga and Wang, 2007; Iess et al., ocean presents technological challenges of much higher 2014; Deamer and Damer, 2017; Rovira-Navarro et al., complexity than the exploration of any location in the deep 2019). In fact, relevant geothermal activity has been imaged sea on Earth. Instrument payloads will likely have a con- on both moons by the Cassini-Huygens probe as well as by straining effect on their use for the exploration of Enceladus the Galileo and Hubble Space Telescope space missions over the next decades, although the weight of their casing (Henin, 2018). Notwithstanding, the presence of organic can be greatly reduced compared to ocean instrumentation molecules as markers for more complex compounds (e.g., on Earth due to the reduced gravity on Enceladus. More- amino acids and nucleotides), dissolved into a salty marine over, the penetration of a potentially large ice shell requires medium, has been directly indicated by the Cassini-Huygens tools to carve or melt tunnels on the scale of kilometers, in probe of Enceladus’ plumes (McKay et al., 2014; Hsu et al., order to open the passage for any marine-like exploring 2015; Kimura and Kitadai, 2015; Mann, 2017; Postberg platforms (Weiss et al., 2008; Flo¨gel et al., 2018). Anyway, et al., 2018). This fact makes Enceladus the most promising those technological efforts are already in place. Different site for extraterrestrial life exploration (Postberg et al., projects such as the Enceladus Explorer (EnEx) and the 2018). Europa Explorer (EurEx) (Konstantinidis et al., 2013), as b AU1 Enceladus is 500 km in diameter with a gravity field of well as the Very-Deep Autonomous Laser-Powered only 1.2% that of Earth (Manga and Wang, 2007). Its vast Kilowatt-Class Yo-Yoing Robotic Ice Explorer (VALK- exo-ocean mechanically decouples the rocky core from the YRIE) are presently focusing on autonomous navigation and exterior ice shell (Thomas et al., 2016). The water body is control of robotic systems on, and especially under, exo- kept fluid by geothermal activity in combination with tidal ocean ice shells. warming through Saturn’s tidal pull forces and by ice shell thickness variations, all likely contributing to abrupt chan- 1.1. Objectives ges in water column pressure (Hussmann et al., 2006; Motivated by data indicating that Enceladus’ exo-ocean Manga and Wang, 2007; Jansen, 2016; Saxena et al., 2018; may host complex organic life and given the time span of its Hemingway and Mittal, 2019; Neveu and Rhoden, 2019). existence as a fluid body (Postberg et al., 2018), we provide Pressure changes result in active geysers, which eject water a perspective for implementing its environmental and life- plumes into space, creating the phenomenon of cryo- oriented exploration based on available deep-sea technologies. F1 c volcanism (Fig. 1). Strong geothermal gradients and high We first describe high-priority sensors that are currently in pressure produce large fluxes of hot water, transported use for marine sciences, when aiming at the characterization through the ice shell via cracks and crevasses (Choblet of pelagic and benthic seascapes, whose environmental et al., 2017). Due to decompression shocks, water suddenly conditions may affect life itself. Then we focus on those evaporates and freezes once it emerges into space, dropping sensors that allow the detection of multicellular life-forms back on the surface as snow (Beˇhounkova´ et al., 2017). (i.e., animal-like), which is, to date, primarily carried out by Exo-ocean salinity conditions on Enceladus seem to be imaging systems. At the same time, we also describe com- similar to those on Earth (Fifer et al., 2019), which would plementary molecular methods for indirect traceability of lead to a water density of approximately 1020 kg/m3,similar life (that would also allow the capability of detection of to that of terrestrial oceans (Hemingway and Mittal, 2019). unicellular life). Later, we illustrate the different marine mon- However, the average depth is much higher, being approxi- itoring platforms and their assemblage into high-tech networks mately between 30 and 50 km (Iess et al., 2014, Hemingway that could be used as test beds for exo-ocean life-detecting and Mittal, 2019). This would generate a total volume of technologies. Ultimately, we propose a forward-looking path- around 40% of the mass of the moon itself (Cˇ adek et al., way for environmental exploration of exo-oceans based on 2016).