EP018
Earth 4D – a Deep Dive into the Habitability of the Blue Planet
Earth 4D – a Deep Dive into the Habitability of the Blue Planet
Session ID#: 81521
Session Description:
Leaving the thin surface veneer of the Blue Planet, investigations of the subsurface architecture of the marine and terrestrial subsurface are challenging our understanding of the distribution and age of water, fluxes of elements like carbon in and out of the subsurface, and the character and distribution of energy. Recent discoveries are transforming our understanding of habitability and the limits to life in the subsurface. How might our current understanding these systems be limited if our focus remains primarily on surficial, or high energy, or recent and readily accessible systems? What inferences can be draw from the Earth’s subsurface processes to inform the exploration of other planets and moons? This session will address how novel processes of energy production and transport in the crust, models of hydrogeologic connectivity (and/or isolation), and long-term transport and reaction timescales are providing new insight though the integration of biology, hydrogeology, geochemistry, and planetary science.
Co-Sponsor(s):
- GS: Geochemical Society -
Index Terms:
0456 Life in extreme environments [BIOGEOSCIENCES]
0495 Water/energy interactions [BIOGEOSCIENCES]
1829 Groundwater hydrology [HYDROLOGY]
5419 Hydrology and fluvial processes [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
Primary Convener: John F Mustard, Brown University, Department of Earth, Environmental and Planetary Sciences, Providence, RI, United States
Conveners: Barbara Sherwood Lollar, University of Toronto, Department of Earth Sciences, Toronto, ON, Canada and Magdalena R Osburn, Northwestern University, Earth and Planetary Sciences, Evanston, IL, United States
Primary Liaison: John F Mustard, Brown University, Department of Earth, Environmental and Planetary Sciences, Providence, RI, United States
See more of: Earth and Planetary Surface Processes
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