Experimental Approaches for Testing the Hypothesis of the Emergence of Life at Submarine Alkaline Vents

Since the pioneering experimental work performed by Urey and Miller around 70 years ago, several experimental works have been developed for approaching the question of the origin of life based on very few well-constructed hypotheses. In recent years, attention has been drawn to the so-called alkaline hydrothermal vents model (AHV model) for the emergence of life. Since the first works, perspectives from complexity sciences, bioenergetics and thermodynamics have been incorporated into the model. Consequently, a high number of experimental works from the model using several tools have been developed. In this review, we present the key concepts that provide a background for the AHV model and then analyze the experimental approaches that were motivated by it. Experimental tools based on hydrothermal reactors, microfluidics and chemical gardens were used for simulating the environments of early AHVs on the Hadean Earth (~4.0 Ga). In addition, it is noteworthy that several works used techniques from electrochemistry to investigate phenomena in the vent–ocean interface for early AHVs. Their results provided important parameters and details that are used for the evaluation of the plausibility of the AHV model, and for the enhancement of it.

A seawater throttle on H2production in Precambrian serpentinizing systems

Since the initial discovery of low-temperature alkaline hydrothermal vents off the Mid-Atlantic Ridge axis nearly 20 y ago, the observation that serpentinizing systems produce abundant H2has strongly influenced models of atmospheric evolution and geological scenarios for the origin of life. Nevertheless, the principal mechanisms that generate H2in these systems, and how secular changes in seawater composition may have modified serpentinization-driven H2fluxes, remain poorly constrained. Here, we demonstrate that the dominant mechanism for H2production during low-temperature serpentinization is directly related to a Si deficiency in the serpentine structure, which itself is caused by low SiO2(aq) concentrations in serpentinizing fluids derived from modern seawater. Geochemical calculations explicitly incorporating this mechanism illustrate that H2production is directly proportional to both the SiO2(aq) concentration and temperature of serpentinization. These results imply that, before the emergence of silica-secreting organisms, elevated SiO2(aq) concentrations in Precambrian seawater would have generated serpentinites that produced up to two orders of magnitude less H2than their modern counterparts, consistent with Fe-oxidation states measured on ancient igneous rocks. A mechanistic link between the marine Si cycle and off-axis H2production requires a reevaluation of the processes that supplied H2to prebiotic and early microbial systems, as well as those that balanced ocean–atmosphere redox through time.

A hydrogen dependent geochemical analogue of primordial carbon and energy metabolism

Hydrogen gas, H2, is generated in alkaline hydrothermal vents from reactions of iron containing minerals with water during a geological process called serpentinization. It has been a source of electrons and energy since there was liquid water on the early Earth, and it fuelled early anaerobic ecosystems in the Earth’s crust1–3. H2is the electron donor for the most ancient route of biological CO2fixation, the acetyl-CoA (or Wood-Ljungdahl) pathway, which unlike any other autotrophic pathway simultaneously supplies three key requirements for life: reduced carbon in the form of acetyl groups, electrons in the form of reduced ferredoxin, and ion gradients for energy conservation in the form of ATP4,5. The pathway is linear, not cyclic, it releases energy rather than requiring energy input, its enzymes are replete with primordial metal cofactors6,7, it traces to the last universal common ancestor8and abiotic, geochemical organic syntheses resembling segments of the pathway occur in hydrothermal vents today9,10. Laboratory simulations of the acetyl-CoA pathway’s reactions include the nonenzymatic synthesis of thioesters from CO and methylsulfide11, the synthesis of acetate12and pyruvate13from CO2using native iron or external electrochemical potentials14as the electron source. However, a full abiotic analogue of the acetyl-CoA pathway from H2and CO2as it occurs in life has not been reported to date. Here we show that three hydrothermal minerals — awaruite (Ni3Fe), magnetite (Fe3O4) and greigite (Fe3S4) — catalyse the fixation of CO2with H2at 100 °C under alkaline aqueous conditions. The product spectrum includes formate (100 mM), acetate (100 μM), pyruvate (10 μM), methanol (100 μM), and methane. With these simple catalysts, the overall exergonic reaction of the acetyl-CoA pathway is facile, shedding light on both the geochemical origin of microbial metabolism and on the nature of abiotic formate and methane synthesis in modern hydrothermal vents.

Synchronized chaotic targeting and acceleration of surface chemistry in prebiotic hydrothermal microenvironments

Porous mineral formations near subsea alkaline hydrothermal vents embed microenvironments that make them potential hot spots for prebiotic biochemistry. But, synthesis of long-chain macromolecules needed to support higher-order functions in living systems (e.g., polypeptides, proteins, and nucleic acids) cannot occur without enrichment of chemical precursors before initiating polymerization, and identifying a suitable mechanism has become a key unanswered question in the origin of life. Here, we apply simulations and in situ experiments to show how 3D chaotic thermal convection—flows that naturally permeate hydrothermal pore networks—supplies a robust mechanism for focused accumulation at discrete targeted surface sites. This interfacial enrichment is synchronized with bulk homogenization of chemical species, yielding two distinct processes that are seemingly opposed yet synergistically combine to accelerate surface reaction kinetics by several orders of magnitude. Our results suggest that chaotic thermal convection may play a previously unappreciated role in mediating surface-catalyzed synthesis in the prebiotic milieu.

Nature's electrochemical flow reactors?: Alkaline hydrothermal vents and the origins of life

Understanding the evolution and beginnings of biochemistry is a fundamental problem which needs to be addressed in origins of life research. The development of highly complex chemical systems from simple inorganic beginnings is difficult to comprehend and has resulted in much heated scientific debate. The debate is further fuelled by the fact we know very little about conditions present on the early Earth at the time life began. Owing to the highly dynamic nature of the Earth, the geological record for the earliest period of Earth's history when life began is practically non-existent. Without geochemical indicators, we have no idea about the composition of the atmosphere or oceans, when or how much water was present on the Earth's surface or the chemical inventory present before the emergence of life. There has been much speculation and argument around all of these points about what could be acceptably deemed ‘prebiotically plausible’ environmental conditions. We do know that life started somewhere, but the where, when and how may only be solved by a process of elimination by experimentation.