The application of coating materials to regulate nitrogen release is a crucial strategy for minimizing fertilizer loss and alleviating agricultural nitrogen pollution. However, it remains a significant challenge to develop ecofriendly coatings that are both biodegradable and effective in slow-release. In this study, Ca/Al layered double hydroxides (LDHs) were incorporated into a conventional polyvinyl alcohol/polyvinylpyrrolidone (PVA/ PVP) matrix to create PVA/PVP-LDHs composite films. The inclusion of LDHs (1.0 %, w/w) resulted in a 32 % enhancement in water resistance, a 10 % reduction in water vapor/ammonia permeability, and a 16 % improvement in mechanical properties. These enhanced performances by addition of LDHs were attributed to the combined effects of the tortuous diffusion pathways, and the formation of robust hydrogen bonding networks between the hydroxyl groups of LDHs and PVA/PVP at the organic-inorganic interface. These interactions could reduce free hydroxyl groups on the film surface, leading to hydrophobicity and structural integrity. The composite films exhibited significantly reduced nitrogen permeability under various pH conditions, indicating the improved stability in both acidic and alkaline soil environments. Degradation experiments revealed that the composite film lost 40 % of its mass over 120 days, with a half-life only 8.0 % longer than pure PVA/PVP. These results indicated that the incorporation of LDHs had minimal impact on biodegradability, maintaining the environmental compatibility of the films. These findings highlight the potential of PVA/PVP-LDHs composite films as sustainable, eco-friendly, and efficient slow-release fertilizer coatings, offering a practical solution for improving nitrogen use efficiency and reducing agricultural nitrogen pollution.

Environmentally persistent free radicals (EPFRs) are produced during biochar pyrolysis and, depending on biochar application, can be either detrimental or beneficial. High levels of EPFRs may interfere with cellular metabolism and be toxic, because EPFR-generated reactive oxygen species (e.g., hydroxyl radicals (center dot OH)) attack organic molecules. However, center dot OH can be useful in remediating recalcitrant organic contaminants in soils. Understanding the (system-specific) safe range of EPFRs produced by biochars requires knowing both the context of their use and their overall significance in the existing suite of environmental radicals, which has rarely been addressed. Here we place EPFRs in a broader environmental context, showing that biochar can have EPFR concentrations from 108-fold lower to 109-fold higher than EPFRs from other environmental sources, depending on feedstock, production conditions, and degree of environmental aging. We also demonstrate that center dot OH radical concentrations from biochar EPFRs can be from 104-fold lower to 1017-fold higher than other environmental sources, depending on EPFR type and concentration, reaction time, oxidant concentration, and extent of environmental EPFR persistence. For both EPFR and center dot OH concentrations, major uncertainties derive from the range of biochar properties and the range of data reporting practices. Controlling feedstock lignin content and pyrolysis conditions are the most immediate options for managing EPFRs. Co-application of compost to provide organics may serve as a postpyrolysis method to quench and reduce biochar EPFRs.

Disinfecting Aspergillus flavus represents a promising strategy to mitigate aflatoxin contamination in agricultural soils and crops. In this study, the efficient disinfection of Aspergillus flavus using a g-C3N4/alpha-Fe2O3 heterojunction under visible light irradiation, along with the roles and mechanisms of the main reactive oxygen species involved in the disinfection process were demonstrated. The g-C3N4/alpha-Fe2O3 exhibited a high photocatalytic disinfection efficiency of up to 91 %, with hydroxyl radicals (center dot OH) identified as the main active species. The production of chitin in the cell walls of Aspergillus flavus was mainly interfered with center dot OH, leading to the destruction of cellular components such as carbohydrates, proteins, and lipids during the disinfection process. The metabolic interference induced by center dot OH resulted in cell structural damage and the release of essential intracellular constituents, ultimately leading to the death of Aspergillus flavus. These findings provided valuable insights into Aspergillus flavus control that was beneficial for its future agricultural applications.

Measurements of the lunar surface have revealed a variable presence of hydration, which has contributions from both hydroxyl (OH) and molecular water (H2O). Recent observations of the lunar hydration suggest that a component of this signature is comprised of molecules that are readily mobile and actively migrate across the lunar surface over the course of a lunar day due to surface temperature variations. However, exospheric measurements of H2O suggest very low abundances above the dayside surface which previous work has argued is in conflict with the surface abundances and the putative occurance of ballistic migration. Here, we use a ballistic transport model to quantify the amounts of OH and H2O in the lunar exosphere and to characterize patterns in the transportation and retention of hydration across the lunar surface. We find that similar to 0.5% of a monolayer of hydration on the surface, with 99% OH and 1% H2O contribution to hydration signatures, matches observational upper limits for the presence of hydration in the exosphere. We conclude that there is no discrepancy between the low exospheric measurements and ballistic migration. However, the previously observed day-time recovery of the hydration signal cannot be explained by this ballistic migration, suggesting that OH/H2O production is also occurring on timescales less than a lunar day. Additionally, we find that ballistic transport results in the transportation of similar to 2% of the hydration sourced from surface desorption to the polar regions of the Moon.

The image of a bone-dry surface in the Moon's non-polar regions impinged by the Apollo missions was changed by the detection of widespread absorption near 3 mu m in 2009, interpreted as a signature of hydration. However, debates persist on the relative contribution of molecular water (H2O) and other hydroxyl (OH) compounds to this hydration feature, as well as the cause of the potential temperature-dependence of the OH/H2O abundance. Resolving these debates will help to estimate the inventory of water on the Moon, a crucial resource for future space explorations. In this study, we measured the abundance and isotope composition of hydrogen within the outermost micron of Chang'e-5 soil grains, collected from the lunar surface and from a depth of 1 m. These measurements, combined with our laboratory simulation experiments, demonstrate that solar-wind-induced OH can be thermally retained in lunar regolith, with an abundance of approximately 48-95 ppm H2O equivalent. This abundance exhibits small latitude dependence and no diurnal variation. By integrating our results with published remote sensing data, we propose that a high amount of molecular water (similar to 360 +/- 200 ppm H2O) exists in the subsurface layer of the Moon's non-polar regions. The migration of this H2O accounts for the observed latitude and diurnal variations in 3 mu m band intensity. The inventory of OH and H2O proposed in this study reconciles the seemingly conflicting observations from various instruments, including infrared/ultraviolet spectroscopies and the Neutral Mass Spectrometer (NMS). Our interpretation of the distribution and dynamics of lunar hydration offers new insights for future lunar research and space missions.

In-situ chemical oxidation is an important approach to remediate soils contaminated with persistent organic pollutants, e.g., polycyclic aromatic hydrocarbons (PAHs). However, massive oxidants are added into soils without an explicit model for predicting the redox potential (Eh) during soil remediation, and overdosed oxidants would pose secondary damage by disturbing soil organic matter and acidity. Here, a soil redox potential (Eh) model was first established to quantify the relationship among oxidation parameters, crucial soil properties, and pollutant elimination. The impacts of oxidant types and doses, soil pH, and soil organic carbon contents on soil Eh were systematically clarified in four commonly used oxidation systems (i.e., KMnO4, H2O2, fenton, and persulfate). The relative error of preliminary Eh model was increased from 48-62% to 4-16% after being modified with the soil texture and dissolved organic carbon, and this high accuracy was verified by 12 actual PAHs contaminated soils. Combining the discovered critical oxidation potential (COP) of PAHs, the moderate oxidation process could be regulated by the guidance of the soil Eh model in different soil conditions. Moreover, the product analysis revealed that the hydroxylation of PAHs occurred most frequently when the soil Eh reached their COP, providing a foundation for further microorganism remediation. These results provide a feasible strategy for selecting oxidants and controlling their doses toward moderate oxidation of contaminated soils, which will reduce the consumption of soil organic matter and protect the main structure and function of soil for future utilization. Environmental implications: This study provides a novel insight into the moderate chemical oxidation by the Eh model and largely reduces the secondary risks of excessive oxidation and oxidant residual in ISCO. The moderate oxidation of PAHs could be a first step to decrease their toxicity and increase their bioaccessibility, favoring the microbial degradation of PAHs. Controlling the soil Eh with the established model here could be a promising approach to couple moderate oxidation of organic contaminants with microbial degradation. Such an effective and green soil remediation will largely preserve the soil's functional structure and favor the subsequent utilization of remediated soil.

The Moon is generally depleted in volatile elements and this depletion extends to the surface where the most abundant mineral, anorthite, features <6 ppm H2O. Presumably the other nominally anhydrous minerals that dominate the mineral composition of the global surface-olivine and pyroxene-are similarly depleted in water and other volatiles. Thus the Moon is tabula rasa for the study of volatiles introduced in the wake of its origin. Since the formation of the last major basin (Orientale), volatiles from the solar wind, from impactors of all sizes, and from volatiles expelled from the interior during volcanic eruptions have all interacted with the lunar surface, leaving a volatile record that can be used to understand the processes that enable processing, transport, sequestration, and loss of volatiles from the lunar system. Recent discoveries have shown the lunar system to be complex, featuring emerging recognition of chemistry unanticipated from the Apollo era, confounding issues regarding transport of volatiles to the lunar poles, the role of the lunar regolith as a sink for volatiles, and the potential for active volatile dynamics in the polar cold traps. While much has been learned since the overturn of the Moon is dry paradigm by innovative sample and spacecraft measurements, the data point to a more complex lunar volatile environment than is currently perceived.

Brown carbon (BrC) absorbs radiation in the near-UV and visible ranges, affecting atmospheric photochemistry andradiative forcing. Our understanding on the photochemicaltransformation of BrC is still limited, especially when mixed withthe abundant and photochemically labile inorganic salt, nitrate.Herein, we investigate the photochemical reactions of four BrCchromophores, including two methoxyphenols and two nitro-phenols. Experiments were conducted in the absence and presenceof different concentrations of H2O2and nitrate with lights of 254and 313 nm. The results show that the pseudo-first-order decayrate constants (k) of these four BrC compounds at 313 nmillumination were approximately 10 times lower than those at 254nm, demonstrating longer lifetimes of these BrC chromophoresunder tropospherically relevant irradiation. Photo-enhancement in the visible range was observed in most experiments, with thoseunder 313 nm illumination lasting longer, indicating the prolonged effects of nascent and transformed BrC chromophores onradiative forcing. Methoxyphenols had higher averagedkvalues than nitrophenols during direct photolysis with 254 or 313 nmlights, but thekvalues for nitrophenols under high-nitrate (or high-H2O2) conditions approached those of methoxyphenols. Thephoto-enhancement in the visible range for methoxyphenols in the presence of nitrate was substantially contributed by nitroproducts, while that for nitrophenols was mainly contributed by hydroxylated and/or dimerized products. Our results reveal thesimilarity and difference between the photolysis of methoxyphenols and nitrophenols, which may help better understand the aging ofdifferent types of BrC for better model representation of their effects on radiative forcing.

Brown carbon (BrC) absorbs radiation in the near-UV and visible ranges, affecting atmospheric photochemistry and radiative forcing. Our understanding on the photochemical transformation of BrC is still limited, especially when mixed with the abundant and photochemically labile inorganic salt, nitrate. Herein, we investigate the photochemical reactions of four BrC chromophores, including two methoxyphenols and two nitrophenols. Experiments were conducted in the absence and presence of different concentrations of H2O2 and nitrate with lights of 254 and 313 nm. The results show that the pseudo-first-order decay rate constants (k) of these four BrC compounds at 313 nm illumination were approximately 10 times lower than those at 254 nm, demonstrating longer lifetimes of these BrC chromophores under tropospherically relevant irradiation. Photo-enhancement in the visible range was observed in most experiments, with those under 313 nm illumination lasting longer, indicating the prolonged effects of nascent and transformed BrC chromophores on radiative forcing. Methoxyphenols had higher averaged k values than nitrophenols during direct photolysis with 254 or 313 nm lights, but the k values for nitrophenols under high-nitrate (or high-H2O2) conditions approached those of methoxyphenols. The photo-enhancement in the visible range for methoxyphenols in the presence of nitrate was substantially contributed by nitro products, while that for nitrophenols was mainly contributed by hydroxylated and/or dimerized products. Our results reveal the similarity and difference between the photolysis of methoxyphenols and nitrophenols, which may help better understand the aging of different types of BrC for better model representation of their effects on radiative forcing.

We investigate the interrelation between the hydration of the lunar regolith and the mineral composition of the surface of the Moon with respect to the concentrations of plagioclase, TiO2 (highly correlated with the oxide mineral ilmenite), and Mg-spinel. The spectral properties of lunar regions with a low concentration of plagioclase or a high concentration of TiO2 or Mg-spinel show a significant reduction in hydration at lunar midday compared to other compositions. This suggests that these oxide minerals contain less of the strongly bound OH component, which is not removed at lunar midday. The time-of-day-dependent variation of the 3 mu m band depth is greater in TiO2-rich areas compared to other mare regions. The TiO2-rich regions therefore appear to have a strong tendency to adsorb solar wind-induced hydrogen into binding states of low energy that can more readily desorb and readsorb OH/H2O on a daily basis.