A Case for Using Ground-Based Thermal Inertia Measurements to Detect Martian Caves

Sunrise Thermal inertia Mars landing Sunset Spaceflight
DOI: 10.1089/ast.2013.1063 Publication Date: 2014-05-13T15:41:08Z
ABSTRACT
Martian caves are regarded as one of the most interesting locations in which to search for life on planet. Data obtained during MARS2013 expedition at Hamar Laghdad Ridge Tafilalt region Morocco indicate that even small cavities can display thermal behavior is characteristic caves. For example, temperature a cavity equaled 14°C±0.1°C before sunrise, was higher than ambient air (10°C±0.1°C) and proximate rocks (9°C±0.1°C) same time. Within 30 min after when surrounding corresponded 15°C, this relationship reversed. Measurements were conducted under simulated spaceflight conditions, including near-real-time interpretation data acquired complex flight planning environment. We conclude using ground-based contrast measurements, 7-14 μm band sunset, an effective method Mars astronauts identify caves, possibly superior usage space-based or ground-penetrating data.
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