The satellites of the outer solar system show huge diversity in their chemical makeup, internal structures, surface geology, underpinning geophysics, and habitable potential. The habitability of these bodies is a property of their physical systems, and hence depends on a range of interacting geophysical, chemical, and celestial mechanical processes, including - but not limited to - climate, impacts and erosion, cryosphere,and ocean dynamics. Many of these different aspects are non-trivially coupled; understanding these worlds requires insight from multiple angles and subdisciplines, from Earth and Planetary scientists alike. This session aims to highlight the diversity of solar system moons, through a wide range of contributions covering atmospheres to the deep interior, instrumentation, laboratory work, and comparative planetology. We welcome contributions from all manner of studies focused on the scientific and technological advancements needed to further our understanding of icy and rocky outer solar system moons.
Please decide on your access
Please use the buttons below to download the display or to visit the external website where the presentation is linked. Regarding the external link, please note that Copernicus Meetings cannot accept any liability for the content and the website you will visit.
You are going to open an external link to the asset as indicated by the session. Copernicus Meetings cannot accept any liability for the content and the website you will visit.
The session PS2.6 is running on a video chat platform. Please find the button to access.
PS2.6 takes place on an external platform. When opening the external link, please be aware that Copernicus Meetings cannot accept any liability for the content and the website you will visit.
