Martian Superoxide and Peroxide O2 Release (OR) Assay: A New Technology for Terrestrial and Planetary Applications

Fast Degradation of Hydrogen Peroxide by Immobilized Catalase to Enable the Use of Biosensors in Extraterrestrial Bodies

Hydrogen peroxide has been postulated to be present on the surface of Europa and Enceladus. While it could represent a potential source of energy for possible life-forms, H₂O₂ may also interfere with a number of current detection technologies, including biosensors. To take advantage of the selectivity and portability of these devices, simple and reliable routes to degrade the potential H₂O₂ present should be developed and implemented to prepare for this possibility. Unfortunately, most of the current approaches for removing H₂O₂ are slow, may affect the sample, or could interfere with the performance of biosensors. To address these limitations, catalase was immobilized onto silica particles and used as a means to selectively decompose H₂O₂ prior to the analysis of common biomarkers with a biosensor. For these experiments, glucose, l-leucine, and lactic acid were used as representative examples of biomolecules such as carbohydrates, amino acids, and organic acids, respectively, which could be used as biomarkers on extraterrestrial bodies. While the decomposition reaction between catalase and H₂O₂ is well known, to our knowledge this is the first instance where catalase has been used in combination with a microfluidic paper-based analytical device (μPAD) to implement selective sample pretreatment.

The Oxygen Release Instrument: Space Mission Reactive Oxygen Species Measurements for Habitability Characterization, Biosignature Preservation Potential Assessment, and Evaluation of Human Health Hazards

We describe the design of an instrument, the OxR (for Oxygen Release), for the enzymatically specific and non-enzymatic detection and quantification of the reactive oxidant species (ROS), superoxide radicals (O2•-), and peroxides (O22-, e.g., H2O2) on the surface of Mars and Moon. The OxR instrument is designed to characterize planetary habitability, evaluate human health hazards, and identify sites with high biosignature preservation potential. The instrument can also be used for missions to the icy satellites of Saturn's Titan and Enceladus, and Jupiter's Europa. The principle of the OxR instrument is based on the conversion of (i) O2•- to O2 via its enzymatic dismutation (which also releases H2O2), and of (ii) H2O2 (free or released by the hydrolysis of peroxides and by the dismutation of O2•-) to O2 via enzymatic decomposition. At stages i and ii, released O2 is quantitatively detected by an O2 sensor and stoichiometrically converted to moles of O2•- and H2O2. A non-enzymatic alternative approach is also designed. These methods serve as the design basis for the construction of a new small-footprint instrument for specific oxidant detection. The minimum detection limit of the OxR instrument for O2•- and O22- in Mars, Lunar, and Titan regolith, and in Europa and Enceladus ice is projected to be 10 ppb. The methodology of the OxR instrument can be rapidly advanced to flight readiness by leveraging the Phoenix Wet Chemical Laboratory, or microfluidic sample processing technologies.

Polysulfides and products of H2S/S-nitrosoglutathione in comparison to H2S, glutathione and antioxidant Trolox are potent scavengers of superoxide anion radical and produce hydroxyl radical by decomposition of H2O2

Exogenous and endogenously produced sulfide derivatives, such as H₂S/HS^-/S^2-, polysulfides and products of the H₂S/S-nitrosoglutathione interaction (S/GSNO), affect numerous biological processes in which superoxide anion (O₂^-) and hydroxyl (OH) radicals play an important role. Their cytoprotective-antioxidant and contrasting pro-oxidant-toxic effects have been reported. Therefore, the aim of our work was to contribute to resolving this apparent inconsistency by studying sulfide derivatives/free radical interactions and their consequent biological effects compared to the antioxidants glutathione (GSH) and Trolox. Using the electron paramagnetic resonance (EPR) spin trapping technique and O₂^-, we found that a polysulfide (Na₂S₄) and S/GSNO were potent scavengers of O₂^- and cPTIO radicals compared to H₂S (Na₂S), GSH and Trolox, and S/GSNO scavenged the DEPMPO-OH radical. As detected by the EPR spectra of DEPMPO-OH, the formation of OH in physiological solution by S/GSNO was suggested. All the studied sulfide derivatives, but not Trolox or GSH, had a bell-shaped potency to decompose H₂O₂ and produced OH in the following order: S/GSNO > Na₂S₄ ≥ Na₂S > GSH = Trolox = 0, but they scavenged OH at higher concentrations. In studies of the biological consequences of these sulfide derivatives/H₂O₂ properties, we found the following: (i) S/GSNO alone and all sulfide derivatives in the presence of H₂O₂ cleaved plasmid DNA; (ii) S/GSNO interfered with viral replication and consequently decreased the infectivity of viruses; (iii) the sulfide derivatives induced apoptosis in A2780 cells but inhibited apoptosis induced by H₂O₂; and (iv) Na₂S₄ modulated intracellular calcium in A87MG cells, which depended on the order of Na₂S₄/H₂O₂ application. We suggest that the apparent inconsistency of the cytoprotective-antioxidant and contrasting pro-oxidant-toxic biological effects of sulfide derivatives results from their time- and concentration-dependent radical production/scavenging properties and their interactions with O₂^-, OH and H₂O₂. The results imply a direct involvement of sulfide derivatives in O₂^- and H₂O₂/OH free radical pathways modulating antioxidant/toxic biological processes.

Radiation-Driven Formation of Reactive Oxygen Species in Oxychlorine-Containing Mars Surface Analogues

The present study demonstrates that γ-radiolyzed perchlorate-containing Mars soil salt analogues (in a CO₂ atmosphere) generate upon H₂O wetting the reactive oxygen species (ROS) superoxide radical (O₂^•-), hydrogen peroxide (H₂O₂), and hydroxyl radicals (^•OH). This study also validates that analogue radiolysis forms oxychlorine species that, in turn, can UV-photolyze to ^•OH upon UV photolysis. This investigation was made possible by the development of a new assay for inorganic-origin O₂^•- and H₂O₂ determination and by the modification of a previous assay for soil ^•OH. Results show that radiolyzed Mg(ClO₄)₂ generates H₂O₂ and ^•OH; and when included as part of a mixture analogous to the salt composition of samples analyzed at the Mars Phoenix site, the analogue generated O₂^•-, H₂O₂, and ^•OH, with ^•OH levels 150-fold higher than in the radiolyzed Mg(ClO₄)₂ samples. Radiolyzed Mars Phoenix site salt analogue that did not contain Mg(ClO₄)₂ generated only ^•OH also at 150-fold higher concentration than Mg(ClO₄)₂ alone. Additionally, UV photolysis of the perchlorate γ radiolysis product chlorite (ClO₂^-) generated the oxychlorine products trihalide (Cl₃^-), chlorine dioxide (ClO₂^•), and hypochlorite (ClO^-), with the formation of ^•OH by UV photolysis of ClO^-. While the generation of ROS may have contributed in part to ¹⁴CO₂ production in the Viking Labeled Release (LR) experiment and O₂ (g) release in the Viking Gas Exchange (GEx) experiment, our results indicate that they are not likely to be the major contributor to the LR and GEx results. However, due to their highly reactive nature, they are expected to play a significant role in the alteration of organics on Mars. Additionally, experiments with hypochlorite show that the thermal stability of NaClO is in the range of the thermal stability observed for thermally liable oxidant responsible for the Viking LR results. Key Words: Mars-Oxygen-Salts-Radiation-Habitability. Astrobiology 17, 319-336.