P038
The New Mars Underground 2.0: Towards a 3D Understanding of the Martian Crustal Subsurface
The New Mars Underground 2.0: Towards a 3D Understanding of the Martian Crustal Subsurface
Session ID#: 83347
Session Description:
The Martian crustal subsurface encompasses a wide range of environments at depths from ~centimeters to kilometers. These environments are relatively unexplored but are of enormous interest for planetary science. Recent results, e.g., methane fluctuations, radar data that are consistent with liquid subsurface water, and ongoing debates on RSL, all point to dynamic subsurface environments. We invite contributions that address the nature and diversity of Mars crustal subsurface environments (modeling, experiments, observations) or develop the tools/missions for exploring them (sounding, access, in situ analysis). We are particularly interested in contributions that advance our understanding of how the subsurface changes with geographic location and depth, in respect to: volatiles such as brines, ices, clathrates, salts, methane and oxidants, the potential for extant life and the preservation of signs of extinct life, the redox potential of past and present environments, and the technologies/mission concepts that enable such subsurface exploration.
Index Terms:
1829 Groundwater hydrology [HYDROLOGY]
5215 Origin of life [PLANETARY SCIENCES: ASTROBIOLOGY]
6225 Mars [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
6297 Instruments and techniques [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
Primary Convener: Vlada Stamenkovic, Jet Propulsion Laboratory, Pasadena, CA, United States
Conveners: Nina Lanza, Los Alamos National Laboratory, Los Alamos, NM, United States, Kris Zacny, Honeybee Robotics, Exploration Technology Group, Pasadena, CA, United States and John F Mustard, Brown University, Department of Earth, Environmental and Planetary Sciences, Providence, RI, United States
Primary Liaison: Vlada Stamenkovic, Jet Propulsion Laboratory, Pasadena, CA, United States
See more of: Planetary Sciences
