Cyanobacteria and chloroflexi-dominated hypolithic colonization of quartz at the hyper-arid core of the Atacama Desert, Chile
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- Lacap, D.C., Warren-Rhodes, K.A., McKay, C.P. et al. Extremophiles (2011) 15: 31. doi:10.1007/s00792-010-0334-3
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Quartz stones are ubiquitous in deserts and are a substrate for hypoliths, microbial colonists of the underside of such stones. These hypoliths thrive where extreme temperature and moisture stress limit the occurrence of higher plant and animal life. Several studies have reported the occurrence of green hypolithic colonization dominated by cyanobacteria. Here, we describe a novel red hypolithic colonization from Yungay, at the hyper-arid core of the Atacama Desert in Chile. Comparative analysis of green and red hypoliths from this site revealed markedly different microbial community structure as revealed by 16S rRNA gene clone libraries. Green hypoliths were dominated by cyanobacteria (Chroococcidiopsis and Nostocales phylotypes), whilst the red hypolith was dominated by a taxonomically diverse group of chloroflexi. Heterotrophic phylotypes common to all hypoliths were affiliated largely to desiccation-tolerant taxa within the Actinobacteria and Deinococci. Alphaproteobacterial phylotypes that affiliated with nitrogen-fixing taxa were unique to green hypoliths, whilst Gemmatimonadetes phylotypes occurred only on red hypolithon. Other heterotrophic phyla recovered with very low frequency were assumed to represent functionally relatively unimportant taxa.
KeywordsAtacama Chloroflexi Chroococcidiopsis Desert Hyper-arid Hypolith
The Atacama Desert is an ancient coastal arid zone that extends across a large area of coastal Chile in South America (Thomas 1997). The desert is, like most arid regions on Earth, typified by a stony desert pavement terrain. This extends approximately 1,000 km along the Pacific coast of South America. At the hyper-arid core of the Atacama at Yungay (24°06′ S 70°01′ W with 1,051-m elevation), the mean annual rainfall (MAR) is around 2.4 mm making it the driest zone in the desert. Long-term climate data indicate that the hyperarid core of the Atacama Desert at Yungay is the driest non-polar desert location on Earth (Warren-Rhodes et al. 2006; Kuhlman et al. 2008).
Hyper-arid desert pavements are characterized by a lack of higher plants or animals (Thomas 1997), and microorganisms are often the only discernible life. This lends significance to microbial colonization as the predominant form of primary productivity and nitrogen input in such extreme desert regions. A ubiquitous feature of desert pavement microbial ecology has been the occurrence of hypolithic cyanobacterial colonization on quartz rocks both in hot (Schlesinger et al. 2003; Pointing et al. 2007; Warren-Rhodes et al. 2006; Warren-Rhodes et al. 2007) and in cold deserts (Broady 2005; Wood et al. 2008; Pointing et al. 2009; Cowan et al. 2010; Wong et al. 2010a, b). Whilst early studies identified cyanobacteria as the predominant colonist (Cameron and Black 1996; Friedmann and Galun 1974; Berner and Evenari 1978), several recent studies have used DNA fingerprinting techniques to inform community structure at a molecular level (Warren-Rhodes et al. 2006; Wood et al. 2008; Pointing et al. 2007). These have generally lacked a quantitative approach and so beta diversity remains uncharacterized, although such molecular studies indicated that hypolithic communities comprise significantly more complex diversity than previously appreciated. More recently, hypolith community structure has been elucidated using sequence data derived from clone libraries and this has yielded valuable data on beta diversity for cold desert hypoliths (Pointing et al. 2009; Wong et al. 2010a). Whilst clone libraries have well-documented limitations, they remain a widespread tool for inferring community structure but have, as yet, not been applied to Atacama hypoliths. Besides the value in more fully resolving microbial community assembly of ‘typical’ green hypoliths at the arid limit for life, the observation that red pigmentation of a quartz rock supported filamentous microbial colonization created a comparative motive for the current study between green and red hypoliths.
Materials and methods
Environmental data that included long-term mean annual temperature and precipitation were collected. Historical rainfall data were sourced from Dirección General de Aguas (http://www.dga.cl), Dirección Meteorológica de Chile (http://www.meteochile.com or http://docs.lib.noaa.gov/resecue/data_rescue_chile.html) and field measurements (McKay et al. 2003). Nanoclimate data for the hypolithic niche were collected in situ from October 2001–2005, including: (1) air and soil temperature and relative humidity at 1 m above the ground surface, at the ground surface and at ~2–5 mm, 2–5 cm, 10 cm, and 20 cm below the soil surface, using Onset Computer HOBO Pro® dataloggers; (2) presence of liquid water condensed on rock and soil surfaces from dew or fog, using a Campbell 237® leaf wetness moisture sensing grid and/or a Spectrum® moisture sensing grid; and (3) rainfall using an Onset Computer tipping bucket rain gauge. An Onset weather station was also installed, with additional sensors to measure solar flux, photosynthetically active radiation (PAR), barometric pressure, and wind speed and direction. The occurrence of liquid water in the soil sufficient to support photosynthesis was defined as a soil relative humidity of ≥95% (Schlesinger et al. 2003) and on soil or stone surfaces by the Campbell moisture sensing grid as a rise in voltage above the 0.005 V ‘dry’ baseline (or a drop in voltage from the 2.095 V ‘dry’ baseline for the Spectrum sensor). Measurements of photosynthetically active radiation (PAR), UV-A, and UV-B radiation were carried out at solar noon using a Li-Cor LI-I400 datalogger (Li-Cor Inc, Nebraska, USA) for PAR, and a UV UVX radiometer (UVP Inc, California, USA) for UV irradiance. For transmittance studies through rock substrates, the sensor was placed in situ under quartz rocks and edges sealed using plasticine.
Molecular community characterization
Colonized rocks were collected from the hyperarid zone, Yungay area (24°06′ S 70°01′ W with 1,051-m elevation), of the Atacama Desert. The three rocks within the sampling zone at Yungay supporting hypolithic biomass (from the same sampling regime conducted by Warren-Rhodes et al. 2006) were used in the present study. Community DNA recovery was achieved following the protocol for environmental DNA recovery from lithic biofilms described in Warren-Rhodes et al. 2006. The entire colonized surface area of each rock was sampled. 16S rRNA genes were PCR amplified using bacteria-specific primers 8F (AGAGTTTGATCCTGGCTCAG) and 1391R (TGYACWCACCGCCCGTC) (Lane 1991). Archaeal-specific primers 8Fa (TCYSGTTGATCCTGCS) and 1492R (GGTTACCTTGTTACGACTT) (Costello and Schmidt 2006) and eukaryal-specific primers NS1 (GTAGTCATATGCTTGTCTC) and NS4 (CTTCCGTCAATTCCTTTAAG) (White et al. 1990) were also used, but did not give positive amplification. Purified PCR product was used to construct clone libraries for each rock sample (CloningPlus, Qiagen, Valencia, CA, USA). A minimum of 100 clones per library were screened by RFLP (MSP1 and CFO1, Amersham, Bucks, UK) and a total of 104 unique RFLP-defined phylotypes were sequenced (ABI 3730 Genetic Analyzer, Applied Biosystems, Foster City, CA, USA) to generate 70 unique 16S rRNA gene sequences (Operational Taxonomic Unit, OTU) of approximately 1,446 bp each. Phylogenetic OTU’s were determined using the computer program DOTUR described in Schloss and Handelsman (2005), with a 97% sequence similarity cutoff. The sufficiency of sampling from each library was estimated using non-parametric rarefaction and OTU Richness determined by Chao1 using Estimate S software (http://viceroy.eeb.uconn.edu/estimateS). Coverage estimates, Shannon’s Diversity Index (Llyod et al. 1968), and Pielou’s Evenness Index (Pielou 1966) were calculated using Primer v6 (Clarke 1993).
Chimera_Check software (Ribosome Database Project, http:/rdp.cme.msu.edu.html) was used to check possible chimeric structures among the sequence data. Approximate phylogenetic affiliations were then determined using BLAST searches of NCBI GenBank database. Multiple alignments were created using ClustalX v.1.81 (Thompson et al. 1997) with reference to sequences selected from the GenBank database. All phylogenetic analysis was performed using both GARLI (Genetic Algorithm for Rapid Likelihood Inference) 0.96 beta (Zwickl 2006) and PAUP* 4.0b10 (Swofford 2001). Maximum likelihood analysis was used to illustrate relationships of the 16S rRNA gene sequences to representative taxa. Bayesian posterior probabilities and bootstrap values of 1,000 replications were calculated and are shown for branch nodes supported by more than 50% of the trees. The phylogenetic differences among communities were quantified using the Fst statistic calculated using Arlequin v3.0 (Excoffier and Scheider 2005). Sequence data have been submitted to NCBI GenBank database with accession numbers FJ890991 to FJ891059.
Results and discussion
Summary of beta diversity for green and red hypoliths
Quartz rock sample
Green 1 (AY1)
Green 2 (AY5)
Red 1 (AY6)
Percentage of total phylotypes recovered
The extremely low colonization frequency of quartz rocks at the hyper-arid core of the Atacama Desert mean that locating hypolithic colonized rocks that can be analyzed is highly challenging (i.e. only 3 out of 3,723 stones were colonized at our site, across an area >2,000 m2) (Warren-Rhodes et al. 2006). The study reported here includes all three colonized rocks located within the survey area and therefore represents the total recoverable hypolithic diversity within this area. Despite equal effort in DNA recovery and cloning, the three rocks yielded significantly different rRNA gene-defined communities, and this heterogeneity was supported by microscopy that indicated major phylotypes recovered in each library were also the most commonly encountered morphotypes. The data revealed two major findings; that the two ‘green’ Chroococcidiopsis-dominated hypoliths supported a highly similar diversity although abundance levels varied; and that the ‘red’ hypolith supported chloroflexi rather than cyanobacteria as the dominant taxon plus a markedly different and more speciose heterotrophic component.
Summary of diversity data for clone libraries generated from green and red hypoliths
No. of positive transformants selected
No. of RFLP-defined phylotypes
No. of OTU (<97% sequence similarity)
Coverage (C) (%)
Chao1 richness ± SD
Shannon’s diversity index (H)
Pielou’s evenness (J)
Green 1 (AY1)
20.8 ± 5.2
Green 2 (AY5)
17.3 ± 5.2
Red 1 (AY6)
32.4 ± 9.7
The red hypolith represented an opportunity to describe a novel hypolithic colonization, often previously assumed to represent an abiotic red/brown patina on rocks. Our study revealed surprisingly different community structure between red and green hypoliths (Table 1). The most striking feature was the dominance by a collection of phylogenetically relatively diverse chloroflexi (Fig. 2). The chloroflexi have traditionally been associated with hot spring environments (Jing et al. 2005; Lau et al. 2006, 2008, 2009; Lacap et al. 2007), but recently have emerged as colonists of hot (Pointing et al. 2007) and cold (Wong et al. 2010a) desert hypoliths, in addition to cold tundra soils (Costello and Schmidt 2006) and endoliths (Wong et al. 2010b). As a phylum they may therefore display a general adaptation to arid environments. The phylotypes affiliated with the genera Roseiflexus, Anaerolinea and also formed a deep-branching cluster of uncharacterized Chlofoflexi (Fig. 2), possibly indicating a novel group of green non-sulfur bacteria. The cyanobacterial genus Chroococcidiopsis was the second most abundant group, whilst the Nostocales comprised only 10% of the community. Interestingly, no other putative nitrogen fixing taxa were indicated from the phylogenies, and this may reflect a higher degree of nitrogen sufficiency within this micro-niche, or generally more abundant nutrients since the chloroflexi are heterotrophically capable and may have out-competed the cyanobacteria under such conditions. The difference is unlikely a function of moisture availability since the sampled area experiences very similar water input and residence times (Warren-Rhodes et al. 2006).
We measured light transmittance (PAR, UVA, and UVB) through all rocks from the point of soil surface to the depth of colonization, with no marked differences between green and red colonized rocks. We therefore discount a selective effect from light transmittance. Whilst low abundances of commonly encountered arid soil heterotrophic bacteria (Yeager et al. 2004; Garcia-Pichel et al. 2001; Walker 1993) from the phyla Actinobacteria and Bacteriodetes were shared between green and red hypoliths, the red hypolith also supported additional unique heterotrophic phylotypes (Table 2; Fig 2). The actinobacterial phylotypes affiliated with the genus Rubrobacter, a noted radiation tolerant desert bacterium (Ferreira et al. 1999). This included the Deinococci, which affiliated with those recovered from arid soils in other hot deserts (Rainey et al. 2005; Chanal et al. 2006; Pointing et al. 2007). The Deinococci are noted for their desiccation and radiation tolerance (De Groot et al. 2005)) although they appear to be a feature of hot rather than cold desert hypoliths. The remaining red hypolith phylotypes affiliated with the Gemmatimonadetes, which are emerging as a common taxon in hypoliths from hot (Pointing et al. 2007) and cold (Pointing et al. 2009) deserts, plus unidentified beta proteobacteria and other unidentified phyla. The greater diversity and abundance of heterotrophic phylotypes may indicate that the chloroflexi-dominated hypolith represents a community structured under more nutrient sufficient conditions.
Statistical analyses of the phylogenetic data (Table 2) indicated that whilst the red hypolith community was most biodiverse, all three hypoliths displayed significantly different diversity and evenness indices (Table 2). The phylogenetically informed community structure was demonstrated as significantly different between all three communities (Table 2). This is interesting, since given the high coverage of our libraries (due to the relatively low diversity of hypoliths); this indicates that hypolith communities can be highly heterogenous within a given climatic biome. This is likely due to unmeasured differences in the microclimate beneath each quartz rock.
The Atacama Desert supports several distinct microbial oases, including quartz hypoliths, halite endoliths, and microbial mats in hypersaline waters (Weirzchos et al. 2009). It is noteworthy that similar cyanobacterial taxa occur in all of these niches and so they may act as local reservoirs for ‘extreme’ colonists in a variety of challenging niches. It will be interesting to establish in future work the extent to which common cyanobacterial taxa are involved in community assembly within each niche, and whether non-cyanobacterial taxa, such as the chloroflexi are also widespread in these niches.
The authors acknowledge support extended by NASA’s Astrobiology Science and Technology for Exploring Planets (ASTEP) program, and the Hong Kong Research Grants Council (Grant number HKU7733/08M HKU7763/10).
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