CORDIS - EU research results
CORDIS

Searching and Characterizing Extraterrestrial Subsurface Oceans

Project description

Searching for sub-surface liquid water in the moons of the solar system

The occurrence of liquid water is one of the few essential prerequisites for life – at least as we know it on Earth. Vast bodies of water can lie beneath the icy crust of moons in our solar system. Combining computer simulations and new telescope observations, the EU-funded Exo-Oceans project plans to search for oceans on Saturn's moons (Titan and Enceladus) and also outside our solar system. The research work will allow detailed analyses of the oceans on Jupiter's moons (Europa and Ganymede). Although it is already known that there is water on the two moons, previous approaches failed to characterise these hidden oceans. The project's results will serve as a fundamental basis for the study of extraterrestrial oceans and extraterrestrial life.

Objective

The existence of liquid water is one of the few preconditions for life as we know it. Therefore, the search and characterization of liquid water outside of Earth plays an essential role in the search for extraterrestrial life. Prominent candidates to host liquid water are moons in the outer solar system, which can maintain oceans under their icy surfaces. The currently most effective way to identify such subsurface oceans is through effects of their salinity and thus electrical conductivity. The conductivity modifies the magnetic field around these moons through a process referred to as electromagnetic induction. Spacecraft measurements of associated magnetic field perturbations provided evidence for oceans within Jupiter’s moon Europa and Ganymede. Current analysis tools however reached an impasse. No scientific techniques are available, which provide quantitative estimates and uncertainties of key ocean properties when the effects of the dense magnetized plasmas around the moons are included. Here we propose entirely new approaches, which overcome these issues. Our novel techniques will include a simultaneous treatment of the physics in all internal and external conductive layers and will for the first time use all available observations including auroral emission to go beyond considering magnetic fields only. EXO-OCEANS will systematically characterize the ocean properties on Europa and Ganymede including the ocean candidate Callisto. Characterizing the oceans on Ganymede, Europa and Callisto are at the heart of ESA’s Juice and NASA’s Europa Clipper missions. For Saturn’s moons Titan and Enceladus where currently existing techniques do not work, we will invent a new detection technique. In parallel we will use the Hubble Space Telescope to search and characterize aurora in extrasolar planetary systems to pave the way for ocean detections beyond the solar system.

Host institution

UNIVERSITAT ZU KOLN
Net EU contribution
€ 2 116 582,00
Address
ALBERTUS MAGNUS PLATZ
50931 Koln
Germany

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Region
Nordrhein-Westfalen Köln Köln, Kreisfreie Stadt
Activity type
Higher or Secondary Education Establishments
Links
Total cost
€ 2 116 582,50

Beneficiaries (1)