DEFINING AND CHARACTERIZING HABITABLE ENVIRONMENTS IN OCEAN WORLD SYSTEMS

• Published in: Oceanography (Washington, D.C.) Vol. 35; no. 1; pp. 30 - 38
• Main Authors: Glass, Jennifer B., Dierssen, Heidi M., Glein, Christopher R., Schmidt, Britney E., Winebrenner, Dale P.
• Format: Journal Article
• Language: English
• Published: 2230 Support Oceanography Society 01.06.2022; The Oceanography Society
• Subjects: Analogs; Earth; Instrumentation; Interfaces; Lunar And Planetary Science And Exploration; Ocean floor; Oceanic crust; Organic compounds; Polar environments; Polar regions; SPECIAL ISSUE ON OCEANS ACROSS THE SOLAR SYSTEM
• ISSN: 1042-8275; 2377-617X
• DOI: 10.5670/oceanog.2021.414

We explore the major characteristics of habitable environments on ocean worlds and how we can study them using Earth analogs and autonomous instrumentation. Earth analogs for habitable regions on ocean worlds include interfaces (e.g., ice-water and seafloor-water boundaries), hydrothermal systems, and inside of ice, snow, clathrates, and crustal rocks. These analogs are best known in Earth’s ocean, but they may also exist on Earth’s land, particularly in polar regions. Importantly, ocean habitability requires that parts of the planetary body interact dynamically with the ocean. Probing the habitability of currently inaccessible extraterrestrial ocean worlds will require establishing biogenicity and abiotic reference frames for organic compounds on ocean worlds and technological advances to explore subsurface liquid water environments beyond Earth. Next generation studies of ocean world habitability will also require integrated modeling tools and coordination between the Earth/ocean sciences and the planetary science communities.