Andrew N. Hock

Life in the Atacama: Searching for life with rovers (science overview)

[1] The Life in the Atacama project investigated the regional distribution of life and habitats in the Atacama Desert of Chile. We sought to create biogeologic maps through survey traverses across the desert using a rover carrying biologic and geologic instruments. Elements of our science approach were to: Perform ecological transects from the relatively wet coastal range to the arid core of the desert; use converging evidence from science instruments to reach conclusions about microbial abundance; and develop and test exploration strategies adapted to the search of scattered surface and shallow subsurface microbial oases. Understanding the ability of science teams to detect and characterize microbial life signatures remotely using a rover became central to the project. Traverses were accomplished using an autonomous rover in a method that is technologically relevant to Mars exploration. We present an overview of the results of the 2003, 2004, and 2005 field investigations. They include: The confirmed identification of microbial habitats in daylight by detecting fluorescence signals from chlorophyll and dye probes; the characterization of geology by imaging and spectral measurement; the mapping of life along transects; the characterization of environmental conditions; the development of mapping techniques including homogeneous biological scoring and predictive models of habitat location; the development of exploration strategies adapted to the search for life with an autonomous rover capable of up to 10 km of daily traverse; and the autonomous detection of life by the rover as it interprets observations on-the-fly and decides which targets to pursue with further analysis.

Robotic ecological mapping: Habitats and the search for life in the Atacama Desert

[1] As part of the three-year ‘Life in the Atacama’ (LITA) project, plant and microbial abundance were mapped within three sites in the Atacama Desert, Chile, using an automated robotic rover. On-board fluorescence imaging of six biological signatures (e.g., chlorophyll, DNA, proteins) was used to assess abundance, based on a percent positive sample rating system and standardized robotic ecological transects. The percent positive rating system scored each sample based on the measured signal strength (0 for no signal to 2 for strong signal) for each biological signature relative to the total rating possible. The 2005 field experiment results show that percent positive ratings varied significantly across Site D (coastal site with fog), with patchy zones of high abundance correlated with orbital and microscale habitat types (heaved surface crust and gravel bars); alluvial fan habitats generally had lower abundance. Non-random multi-scale biological patchiness also characterized interior desert Sites E and F, with relatively high abundance associated with (paleo)aqueous habitats such as playas. Localized variables, including topography, played an important, albeit complex, role in microbial spatial distribution. Site D biosignature trends correlated with culturable soil bacteria, with MPN ranging from 10-1000 CFU/g-soil, and chlorophyll ratings accurately mapped lichen/moss abundance (Site D) and higher plant (Site F) distributions. Climate also affected biological patchiness, with significant correlation shown between abundance and (rover) air relative humidity, while lichen patterns were linked to the presence of fog. Rover biological mapping results across sites parallel longitudinal W-E wet/dry/wet Atacama climate trends. Overall, the study highlights the success of targeting of aqueousassociated habitats identifiable from orbital geology and mineralogy. The LITA experience also suggests the terrestrial study of life and its distribution, particularly the fields of landscape ecology and ecohydrology, hold critical lessons for the search for life on other planets. Their applications to robotic sampling strategies on Mars should be further exploited.

Application of pulsed‐excitation fluorescence imager for daylight detection of sparse life in tests in the Atacama Desert

A daylight fluorescence imager was deployed on an autonomous rover, Zoe, to detect life on the surface and shallow subsurface in regions of the Atacama Desert in Chile during field tests between 2003 and 2005. In situ fluorescent measurements were acquired from naturally fluorescing biomolecules such as chlorophyll and from specific fluorescent probes sprayed on the samples, targeting each of the four biological macromolecule classes: DNA, protein, lipid, and carbohydrate. RGB context images were also acquired. Preparatory reagents were applied to enhance the dye probe penetration and fluorescence intensity of chlorophyll. Fluorescence imager data sets from 257 samples were returned to the Life in the Atacama science team. A variety of visible life forms, such as lichens, were detected, and several of the dye probes produced signals from nonphotosynthetic microorganisms.

Signatures of Habitats and Life in Earth’s High-Altitude Lakes: Clues to Noachian Aqueous Environments on Mars

14.1 IntroductionA series of astrobiological high-altitude expeditions to the South AmericanAndean Mountains were initiated in 2002 to explore the highest perenniallakes on Earth, including several volcanic crater lakes at or above 6000 min elevation. During the next five years, they will provide the first integratedlong-term astrobiological characterization and monitoring of lacustrineenvironments and their biology at such an altitude. These extreme lakesare natural laboratories that provide the field data, currently missingabove 4000 m, to complete our understanding of terrestrial lakes and biota.Research is being performed on the effects of UV in low-altitude lakesand models of UV flux over time have been developed (Cockell, 2000). Thelakes showing a high content of dissolved organic material (DOM) shieldorganisms from UV effects (McKenzie et al., 1999; Rae et al., 2000). DOMacts as a natural sunscreen by influencing water transparency, and thereforeis a determinant of photic zone depth (Reche et al., 2000). In sparselyvegetated alpine areas, lakes tend to be clearer and offer less protectionfrom UV to organisms living in the water. Transparent water, combinedwith high UV irradiance may maximize the penetration and effect of UVradiation as shown for organisms in alpine lakes (e.g., Vincent et al., 1984;Vinebrook and Leavitt, 1996). Shallow-water benthic communities in theselakes are particularly sensitive to UV radiation. Periphyton, which definescommunities of microorganisms in bodies of water, can live on varioussusbtrates. While on rocks, they include immobile species that cannot seeklow UV refuges unlike sediment-dwelling periphyton (Happey-Wood, 1988;Vincent et al., 1993) or alpine phytoflagellates (Rott, 1988) which bothundergo vertical migration. Inhibition of algal photosynthesis by UV radia-tion has been documented in the laboratory (Ha ¬der, 1993) and it has beenshown that phytoplankton production is reduced by formation of nucleic acidlesions (Karentz et al., 1991) or production of peroxides and free oxygenradicals (Cooper et al., 1989). Most of the experiments that have demon-strated in situ suppression of algal growth by UV radiation have eitherused artificially enhanced UV irradiance (Worrest et al., 1978) or shallowsystems (<1 cm) that lack significant natural attenuation of UV radiation(Bothwell et al., 1993, 1994). Our project is providing the field data thatare missing from natural laboratories above 4000 m and will complementthe postulation of the effects of UV on life and its adaptation modes(or lack thereof).The exploration of high-altitude lakes could shed light on early EarthOsbiological evolution as well. For two billion years, EarthOs atmosphere

Mitigation of environmental extremes as a possible indicator of extended habitat sustainability for lakes on early Mars

The impact of individual extremes on life, such as UV radiation (UVR), temperatures, and salinity is well documented. However, their combined effect in nature is not well-understood while it is a fundamental issue controlling the evolution of habitat sustainability within individual bodies of water. Environmental variables combine in the Bolivian Altiplano to produce some of the highest, least explored and most poorly understood lakes on Earth. Their physical environment of thin atmosphere, high ultraviolet radiation, high daily temperature amplitude, ice, sulfur-rich volcanism, and hydrothermal springs, combined with the changing climate in the Andes and the rapid loss of aqueous habitat provide parallels to ancient Martian lakes at the Noachian/Hesperian transition 3.7-3.5 Ga ago. Documenting this analogy is one of the focuses of the High-Lakes Project (HLP). The geophysical data we collected on three of them located up to 5,916 m elevation suggests that a combination of extreme factors does not necessarily translate into a harsher environment for life. Large and diverse ecosystems adapt to UVR reaching 200%-216% that of sea level in bodies of water sometimes no deeper than 50 cm, massive seasonal freeze-over, and unpredictable daily evolution of UVR and temperature. The HLP project has undertaken the first complete geophysical and biological characterization of these lakes and documents how habitability is sustained and prolonged in declining lakes despite a highly dynamical environment. The same process may have helped life transition through climate crises over time on both Earth and Mars.

Correction to ''The High-Lakes Project''

Nathalie A.Cabrol,EdmondA.Grin, GuillermoChong,EdwinMinkley,AndrewN. Hock,Youngseob Yu, Leslie Bebout, Erich Fleming, Donat P. Ha¨der, Cecilia Demergasso,John Gibson, Lorena Escudero, Cristina Dorador, Darlene Lim, Clayton Woosley,Robert L. Morris, Cristian Tambley, Victor Gaete, Matthieu E. Galvez,Eric Smith, Ingrid Ukstins Peate, Carlos Salazar, G. Dawidowicz, and J. Majerowicz