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Radar evidence of subglacial liquid water on Mars

Friday, November 09, 2018 - 12:00
Place: 
Donostia International Physics Center
Who: 
Federico Di Paolo
Source Name: 
DIPC

15), matching that of water-bearing materials. We interpret this feature as a stable body of liquid water trapped below the ice of the South Polar Layered Deposits of Mars."}" data-sheets-userformat="{"2":513,"3":[null,0],"12":0}" style="font-size: 10pt; font-family: Arial;">Between May 2012 and December 2015 the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS), a low-frequency radar onboard the Mars Express spacecraft of the European Space Agency (ESA) collected data above the Planum Australe region on Mars. Anomalously bright subsurface reflections in such area are evident within a well-defined, 20-kilometer-wide zone surrounded by much less reflective areas. Quantitative analysis of the radar signals shows that this bright feature has high relative dielectric permittivity (>15), matching that of water-bearing materials. We interpret this feature as a stable body of liquid water trapped below the ice of the South Polar Layered Deposits of Mars.

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