Abstract:Silica-rich hydrothermal fluids that experience freezing temperatures precipitate cryogenic opal-A (COA) within ice-bound brine channels. We investigated cryogenic silicification as a novel preservation pathway for chemo-and photo-lithotrophic Bacteria and Archaea. We find that the copartitioning of microbial cells and silica into brine channels causes microorganisms to become fossilised in COA. Rod-and coccoidal-form Bacteria and Archaea produce numerous cell casts on COA particle surfaces, while Chloroflexus… Show more
“…After complete sublimation of ice this vein structure remains intact (Figures 1f and 1g). Ice‐free broken up cryogenic particles bear morphological features similar to those previously identified in terrestrial ice‐templated cryogenic opal‐A (COA), such as triple‐junctions, branched threads and sheets (Channing & Butler, 2007; Fox‐Powell et al., 2018; Figure ).…”
Section: Resultsmentioning
confidence: 55%
“…The resulting crystallization textures, expressed here at the 10 µm scale, are similar to eutectic solidification textures formed in igneous and metallic systems (Akamatsu & Plapp, 2016), thus we conclude they record the final solidification of the system at the eutectic. We also note that in pH 9 fluids, small filiform carbonates can morphologically resemble common terrestrial microorganisms (Figure 3d), with cautionary implications for interpreting potential microfossils in cryogenic particles (Fox-Powell et al, 2018).…”
Section: Direct Crystallization Versus Crystallization Upon Warmingmentioning
Saturn's ice‐covered moon Enceladus may contain the requisite conditions for life. Its potentially habitable subsurface ocean is vented into space as large cryovolcanic plumes that can be sampled by spacecraft, acting as a window to the ocean below. However, little is known about how Enceladus’ ocean fluids evolve as they freeze. Using cryo‐imaging techniques, we investigated solid phases produced by freezing simulated Enceladean ocean fluids at endmember cooling rates. Our results show that under flash‐freezing conditions (>10 K s−1), Enceladus‐relevant fluids undergo segregation, whereby the precipitation of ice templates the formation of brine vein networks. The high solute concentrations and confined nature of these brine veins means that salt crystallization is kinetically inhibited and glass formation (vitrification) can occur at lower cooling rates than typically required for vitrification of a bulk solution. Crystalline salts also form if flash‐frozen fluids are re‐warmed. The 10 µm‐scale distribution of salt phases produced by this mechanism differs markedly from that of gradually cooled (∼1 K min−1) fluids, showing that they inherit a textural signature of their formation conditions. The mineralogy of cryogenic carbonates can be used as a probe for cooling rate and parent fluid pH. Our findings reveal possible endmember routes for solid phase production from Enceladus’ ocean fluids and mechanisms for generating compositional heterogeneity within ice particles on a sub‐10 µm scale. This has implications for understanding how Enceladus' ocean constituents are incorporated into icy particles and delivered to space.
“…After complete sublimation of ice this vein structure remains intact (Figures 1f and 1g). Ice‐free broken up cryogenic particles bear morphological features similar to those previously identified in terrestrial ice‐templated cryogenic opal‐A (COA), such as triple‐junctions, branched threads and sheets (Channing & Butler, 2007; Fox‐Powell et al., 2018; Figure ).…”
Section: Resultsmentioning
confidence: 55%
“…The resulting crystallization textures, expressed here at the 10 µm scale, are similar to eutectic solidification textures formed in igneous and metallic systems (Akamatsu & Plapp, 2016), thus we conclude they record the final solidification of the system at the eutectic. We also note that in pH 9 fluids, small filiform carbonates can morphologically resemble common terrestrial microorganisms (Figure 3d), with cautionary implications for interpreting potential microfossils in cryogenic particles (Fox-Powell et al, 2018).…”
Section: Direct Crystallization Versus Crystallization Upon Warmingmentioning
Saturn's ice‐covered moon Enceladus may contain the requisite conditions for life. Its potentially habitable subsurface ocean is vented into space as large cryovolcanic plumes that can be sampled by spacecraft, acting as a window to the ocean below. However, little is known about how Enceladus’ ocean fluids evolve as they freeze. Using cryo‐imaging techniques, we investigated solid phases produced by freezing simulated Enceladean ocean fluids at endmember cooling rates. Our results show that under flash‐freezing conditions (>10 K s−1), Enceladus‐relevant fluids undergo segregation, whereby the precipitation of ice templates the formation of brine vein networks. The high solute concentrations and confined nature of these brine veins means that salt crystallization is kinetically inhibited and glass formation (vitrification) can occur at lower cooling rates than typically required for vitrification of a bulk solution. Crystalline salts also form if flash‐frozen fluids are re‐warmed. The 10 µm‐scale distribution of salt phases produced by this mechanism differs markedly from that of gradually cooled (∼1 K min−1) fluids, showing that they inherit a textural signature of their formation conditions. The mineralogy of cryogenic carbonates can be used as a probe for cooling rate and parent fluid pH. Our findings reveal possible endmember routes for solid phase production from Enceladus’ ocean fluids and mechanisms for generating compositional heterogeneity within ice particles on a sub‐10 µm scale. This has implications for understanding how Enceladus' ocean constituents are incorporated into icy particles and delivered to space.
“…Hydrothermal activity in cold surface conditions can enhance fossil preservation (Fox-Powell, 2018). “Cryogenic opal-A” (COA) precipitates within ice-bound brine channels in Icelandic hot springs.…”
Section: Taphonomic Processesmentioning
confidence: 99%
“…The surfaces of COA particles were populated with bacterial and archaeal rods and coccoids, and particle interiors retained Chloroflexus filaments. Fox-Powell et al (2018) also detected biomolecules and inorganic microbial metabolic products in COA. The authors concluded that fossil preservation in COA is highly relevant to the exploration of extraterrestrial environments where hydrothermal activity has occurred under freezing conditions, for example on Mars and Enceladus.…”
This report reviews how terrestrial hot spring systems can sustain diverse and abundant microbial communities and preserve their fossil records. Hot springs are dependable water sources, even in arid environments. They deliver reduced chemical species and other solutes to more oxidized surface environments, thereby providing redox energy and nutrients. Spring waters have diverse chemical compositions, and their outflows create thermal gradients and chemical precipitates that sustain diverse microbial communities and entomb their remnants. These environments probably were important habitats for ancient benthic microbial ecosystems, and it has even been postulated that life arose in hydrothermal systems. Thermal spring communities are fossilized in deposits of travertine, siliceous sinter, and iron minerals (among others) that are found throughout the geological record back to the oldest known well-preserved rocks at 3.48 Ga. Very few are known before the Cenozoic, but it is likely that there are many more to be found. They preserve fossils ranging from microbes to trees and macroscopic animals. Features on Mars whose morphological and spectroscopic attributes resemble spring deposits on Earth have been detected in regions where geologic context is consistent with the presence of thermal springs. Such features represent targets in the search for evidence of past life on that planet.
“…Geyserites and silica sinters could thus experience variable temperature of formation that could influence their NIR signatures. Also, some opals can form under cryogenic conditions in contact with ice grains and/or snow, like in Iceland or within the Yellowstone Park, during the winter (Channing and Butler, 2007;Jones and Renaut, 2010;Fox-powell et al, 2018). We hypothesize that some geyserites and silica sinters may exhibit CRC values consistent with continental weathering or low-temperature hydrothermal processes (below 50°C) even if formed in hydrothermal setting.…”
Section: Hydrothermal Vs Weathering Martian Hydrated Silicamentioning
et al., Toward the geological significance of hydrated silica detected by near infrared spectroscopy on Mars based on terrestrial reference samples, Icarus(2020),
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