Thinking Alien Abysses: How High-Pressure Experimental Thermodynamics of Aqueous Systems Help Us Constrain the Structure and Habitability of Deep Planetary Hydrospheres
When: April 11, 2017 3PM PDT
The possible presence of deep aqueous salty oceans in icy moons (Europa, Ganymede, Titan, etc.), and potentially in water-rich exoplanets, has generated a lot of enthusiasm in the astrobiology community and is one of the focus of future NASA and ESA missions (Europa Clipper and JUICE, respectively). However, as the pressure, temperature and chemistry expected to characterize these oceans lie beyond those encountered in Earth’s natural environments, our understanding of these alien places remains hindered by a historical lack of experimental and theoretical constraints of aqueous systems at these specific conditions. Pressure, temperature and chemistry induce important changes to the physical properties of fluids and ices (e.g. density, crystallographic structure), to the extent that structural models of icy worlds can not rely solely on extrapolated properties of pure water. We will present current experiments and models from our team at the ESS-UW and highlight potential effects of these altered properties on the structure and habitability of large icy worlds.
To join using a videoconferencing system:
Please RSVP to Mike Toillion (email@example.com) if you will be joining by Polycom.
To view the slides, connect to http://connect.arc.nasa.gov/uwseminar/
To join using a web browser:
The slides and audio/video for this meeting will be presented using Adobe Connect. To join the meeting, connect to:
If you are having problems connecting, you can try joining http://connect.arc.nasa.gov/uwseminar/?launcher=false, or rebooting your computer, or try joining from another network.