Robotic Astrobiology
Evidence suggests that the interior of the Chilean Atacama Desert, the most arid region on Earth, contains no living organisms. Yet,
where the desert meets the Pacific Coastal Range, desiccation-tolerant microorganisms are known to exist. The gradient of
biodiversity and habitats of life in the Atacama’s subregions remain unexplored.
Robotic field investigation will bring new scientific understanding of the Atacama as a habitat for life with distinct
analogies to Mars. Our goal is to make genuine discoveries about the limits of life on Earth and to generate knowledge about
life in extreme environments that can be applied to future planetary missions. In order to conduct this investigation, we will develop
Robotic Astrobiology.
Field investigation over three years will use a rover to make transects of the Atacama with instruments to detect
microorganisms and chlorophyll-based life forms and to characterize habitats. The rover will integrate panoramic imagers,
microscopic imagers, spectrometers, as well as mechanisms for shallow subsurface access.
Robotic considerations in addition to instrument integration include platform configuration, planetary-relevant
localization, complex obstacle negotiation, over-the-horizon navigation, and power-cognizant activity planning.
An architecture that coordinates these capabilities, provides health monitoring and fault recovery, and allows for variability
in the degree of autonomy is vital to long-duration operations.
The measurement and exploration technique produced by this investigation combines long traverses, sampling measurements
on a regional scale and detailed measurements of individual targets. When compared to the state of the art in robotic
planetary exploration our approach will result in dramatic increase in the number of measurements made and data collected
by rover instruments per command cycle. This result will translate into substantial productivity increases for future
planetary exploration missions.
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