Using Neutron Tomography to study aqueous alteration processes on Mars

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Understanding the fluid pathways and timing(s) of fluid flow within Martian meteorites is critical to our understanding of the nature and origin of water at or near the red planet’s surface. Elucidating Mars’ aqueous past is critical to major questions on past or current habitable environments on Mars and the investigation of rocks and minerals formed through aqueous processes is a key driver for ESA and NASA robotic exploration missions. Neutron tomography’s sensitivity to hydrous...
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