Tully Rohrer, Lucie Knor, Fernando Pacheco, Daniel Fitzgerald with the CTD Rosette that collects Hawai‘i Ocean Time-series water samples.
view more
Credit: Carolina Funkey
Carbon dioxide in the atmosphere enters the ocean at the surface and has been increasing the acidity of Pacific waters since the beginning of the industrial revolution over 200 years ago. A new study, led by University of Hawai‘i at Mānoa oceanographers, revealed that the ocean is acidifying even more rapidly below the surface in the open waters of the North Pacific near Hawai‘i. Their discovery was published recently in the Journal of Geophysical Research: Oceans.
“Ocean acidification has far‐reaching consequences for ocean biology and the global climate,” said Lucie Knor, lead author of the study and postdoctoral researcher in the UH Mānoa School of Ocean and Earth Science and Technology (SOEST). “We expected some indicators of ocean acidification to be changing more rapidly below the surface, because that was what some global studies have previously discovered, but we were very surprised that this was true for every single ocean acidification indicator.”
Knor and co-authors analyzed a 35‐year record of ocean carbon measurements made by the Hawai’i Ocean Time-series program throughout the entire water column–from the surface to nearly three miles deep–at the open ocean field site 60 miles north of O‘ahu, Hawai‘i, Station ALOHA.
They found that in all layers, there are increases of carbon from natural decomposition of sinking organisms. In some layers, accelerated acidification is associated with fresher and colder waters.
“Deeper waters are already naturally quite acidic in the North Pacific, so quickly increasing acidity could negatively impact plankton species and other organisms that live below the surface,” said Knor. “In the long run, these changes in ocean chemistry also make it harder for the ocean to keep taking up more CO₂ from the atmosphere.”
In the past decade or so, there has been an onslaught of marine heat waves associated with unusual conditions in the ocean and atmosphere and strong, multi‐year El Niño events. Researchers, fisheries managers, and coral conservationists are concerned with the combined impacts of marine heat waves and ocean acidity events.
Subsurface waters at station ALOHA are formed farther north in the Pacific. Changes in seawater properties impacted by evolving environmental conditions in other areas of the North Pacific are then transported by ocean currents into the deeper layers of the ocean around Hawai‘i.
“We illustrate that regional-scale changes in source water chemistry and circulation are substantial drivers of the subsurface intensification of ocean acidification around Hawaii,” said Christopher Sabine, co-author of the article and Oceanography professor in SOEST.
Currently, the research team is investigating the carbon specifically from human-made sources in the water column at Station ALOHA and how that is changing over time in different layers.
Journal
Journal of Geophysical Research Oceans
Method of Research
Observational study
Subject of Research
Not applicable
Article Title
Drivers and Variability of Intensified Subsurface Ocean Acidification Trends at Station ALOHA
Article Publication Date
27-Jun-2025
COI Statement
The authors declare no conflicts of interest relevant to this study.
Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.
Simultaneous thermal analysis (STA) was employed to investigate the decomposition temperature and phase transformation of the synthesized ZnS. Figure 2-a demonstrates the thermal behavior of ZnS upon heating up to 1000 °C in an air atmosphere. Analysis of the thermogravimetric (TG) curve reveals approximately a 10% weight loss below 200 °C, which is associated with water elimination. This observation is supported by a gentle endothermic peak in the differential thermal analysis (DTA) curve32,33. Additionally, a weight change of about 16% is expected during the complete conversion of ZnS to ZnO, as shown in the TG curve in the temperature range of 550–700 °C34. The oxidation mechanism involves the release of sulfur species-typically in the form of SO₂-and the concurrent formation of ZnO as follows:
$$mathrm{ZnS+3/2 O_2rightarrow ZnO+SO_2}$$
(2)
Initially, oxygen molecules adsorb onto the surface of ZnS particles. At elevated temperatures, these O₂ molecules dissociate into reactive atomic oxygen species (O•), which can attack the Zn-S bonds. Mechanistically, intermediate species such as surface Zn-O-S or Zn-SOₓ compounds may form before complete desulfurization35. Consistent with this mechanism, the DTA curve reveals an exothermic peak around 640 °C, associated with the oxidation of ZnS. A subsequent decline between 640 and 680 °C indicates the complete conversion of ZnS to ZnO34,36. Beyond 700 °C, no significant weight loss is observed in the TG curve. The DTA peak observed around this temperature may be attributed to the release of residual sulfur species37. According to the thermal analysis result in Fig. 2-a, the oxidation temperature of ZnS is determined to be about 550 °C. Despite the fact that this oxidation is thermodynamically possible at lower temperatures, the kinetic barrier delays the reaction until higher temperatures are reached. Therefore, annealing treatments were performed at temperatures both below and above 550 °C, and the X-ray diffraction patterns of the obtained particles are presented in Fig. 2-b38. As illustrated in Fig. 2-b, the formation of ZnS and ZnO phases is confirmed by the characteristic diffraction peaks. Specifically, the (111), (220), and (311) crystal planes of cubic ZnS (JCPDS 36-1450) are observed at 28.59°, 47.62°, and 56.47°, respectively. Additionally, peaks at 31.83°, 34.48°, 36.32°, 47.62°, 56.76°, 62.93°, and 67.86° correspond to the (100), (002), (101), (102), (110), (103), and (112) planes of hexagonal wurtzite ZnO (JCPDS No. 36-1451)39,40,41,42.
According to Fig. 2-b, only ZnS peaks are observed up to 400 °C, confirming that no oxidation occurs at this stage-consistent with STA data. Although the conversion of ZnS to ZnO is thermodynamically feasible at lower temperatures, it is kinetically restricted. The increasing sharpness of ZnO peaks with increasing temperature indicates improved crystallinity37,43, with the most intense peak corresponding to the (101) plane, suggesting preferential growth along this orientation44. ZnO diffraction peaks gradually appear from 500 °C onward, while ZnS peak intensities diminish, indicating that oxidation begins at this point and completes around 650 °C. This observation also agrees with the STA data. At intermediate temperatures, the simultaneous presence of ZnS and ZnO diffraction patterns suggests the formation of ZnS-ZnO heterostructures.
Furthermore, The crystallite size of the synthesized specimens was calculated using the Debye-Scherrer equation41:
K is the shape factor, typically assumed to be 0.9.
λ denotes the wavelength of the Cu-Kα radiation, which is 1.54 Å.
β represents the full width at half maximum intensity.
θ is the Bragg angle.
The calculated crystallite sizes are presented in Table S1 (Supplementary Materials). As the annealing temperature increases, the crystallite size of ZnO and ZnS increases, which can impact the photocatalytic performance45,46,47.
Fig. 2
(a) STA curve of ZnS, and (b) XRD pattern of synthesized samples.
FESEM analysis was performed to investigate the morphology of the synthesized compounds. In Fig. 3-a, ZnS particles are observed to be clustered, exhibiting a lumpy appearance. The high surface-to-volume ratio of nanoparticles enhances their surface reactivity, contributing to this morphology48. The particles are predominantly spherical, with an average size of 13 nm, as indicated by the particle size distribution histogram. Figure 3-b shows the surface morphology of the ZnS-ZnO nanocomposite, where the particals are unevenly agglomerated with an average size of 43 nm. Finally, Fig. 3-c displays ZnO nanoparticles with a relatively smooth surface. These particles appear larger than those of ZnS, which is attributed to the reduction of sulfur and the complete conversion of ZnS into ZnO49. Additionally, each sample underwent energy dispersive X-ray spectroscopy (EDS) analysis to confirm their elemental composition, which are consistent with the corresponding XRD results. In Fig. 3-a, distinct peaks for zinc (Zn) and sulfur (S) confirm the presence of ZnS. In Fig. 3-b, the appearance of an oxygen (O) peak verifies the formation of ZnO in the nanocomposite. Furthermore, the decreasing intensity of sulfur in Fig. 3-c further supports the successful synthesis of ZnO.
Fig. 3
FESEM images, particle size dispensation diagram, and EDS analysis of (a) ZnS, (b) ZnS-ZnO, and (c) ZnO.
HRTEM results depicted in Fig. 4, provide further insight into the structure of ZnS-ZnO nanocomposite. The visible contrast between bright and dark regions at the interface signifies the formation of two distinct phases, thereby confirming the successful creation of a composite material50. ZnO nanoparticles are observed to be formed near the ZnS nanoparticles, with instances of structural aggregation in some regions. Analysis of the selected area electron diffraction pattern (SEDP) for ZnS-ZnO sample reveals a polycrystalline structure. The size of a single ZnS crystal is estimated to be approximately 6.5 nm, which is in good agreement with the crystallite size determined from XRD results. Each bright point and ring in the SEDP corresponds to the interplanar distances of ZnS and ZnO, indicating the crystalline structure of both materials. Notably, the lattice of ZnS and ZnO exhibits distinct characteristics, confirming their crystallization51. Moreover, Further analysis of the fast Fourier transform (FFT) diffraction pattern shows specific d-spacings values: 0.31 nm corresponding to the (111) plane of ZnS and 0.24 nm for the (101) plane of ZnO43. These observations confirm the successful formation of ZnS-ZnO heterojunctions.
Fig. 4
HRTEM image of (a) ZnS-ZnO structure and related SEDP pattern, (b) d-spacing of structure and related FFT pattern, and (c) ZnS crystallite.
FTIR spectra provide valuable insights into the chemical structure and any changes due to molecular interactions, particularly in composite materials52. In Fig. 5, the characteristic functional groups of ZnS, ZnO, and the ZnS-ZnO composite are identified. The peaks observed at 656 cm−1 and 1005 cm−1 in the spectra corresponds to sulfides and the Zn-S bond, respectively, which are characteristic of ZnS. In contrast, the peak at 621 cm−1 in the ZnO spectrum is linked to Zn-O stretching vibrations53,54. In the ZnS-ZnO composite spectrum, peaks appearing in the range of 550–900 cm−1 indicate the presence of both Zn-O and Zn-S bonds. Additionally, the bond associated with Zn-S in the 1050–1150 cm⁻¹ range confirms that ZnS remains in the composite55,56. Importantly, the absence of Zn-S peaks in the pure ZnO spectrum helps to the distinguish between ZnS and ZnO phases. A peak near 1122 cm−1, observed in both the ZnS and ZnO spectra, undergoes a shift in the ZnS-ZnO spectrum, suggesting changes in the bonding environment due to composite formation. This band is associated with C-O stretching vibrations57,58. A weak band near 1385 cm⁻¹ is attributed to N-O vibrations, likely arising from residual NaNO₃ by-products, indicating the persistence of trace secondary phases despite washing steps. Additionally, peaks at 2853 cm⁻¹ and 2922 cm⁻¹, corresponding to C-H stretching modes, are consistently present across all ZnS, ZnO, and ZnS-ZnO samples52,54. Moreover, ZnS, ZnO, and ZnS-ZnO spectra showed peak levels at 1618 cm−1, 1620 cm−1, and 1616 cm−1,respectively, are attributed to surface-adsorbed water (H₂O bending vibration). The reduction in intensity of these bands after heating confirms the partial removal of physically adsorbed water56,59. Finally, the broad absorption bands in the 3000–3600 cm−1 range correspond to O-H stretching vibrations. Strong peaks are observed at 3405 cm−¹ for ZnS, 3422 cm−¹ for ZnO, and 3417 cm−¹ for the ZnS-ZnO composite, further supporting the presence of hydroxyl groups in all samples51,60.
Fig. 5
FTIR spectra of ZnS, ZnS-ZnO, and ZnO.
Adsorption and desorption of N2 analyses were conducted to evaluate the porous nature and determine the specific surface area of the synthesized particles. The results are shown in Fig. 6 and were analyzed using the BET (Brunauer-Emmett-Teller) and BJH (Barrett-Joyner-Halenda) methods. The specific surface areas were determined to be 165 m² g−1, 35 m² g−1, and 10 m² g−1 for ZnS, ZnS-ZnO, and ZnO, respectively. Notably, ZnS exhibits the highest specific surface area, indicating the presence of mesoporous structures61. This significant surface area is particularly remarkable compared to typical hydrothermal synthesis conditions. Given that the molar volume of ZnS (24.48 cm³ mol−1) is greater than that of ZnO (14.5 cm³ mol−1), an increase in porosity was anticipated upon ZnS oxidation. However, ZnO particles are larger than ZnS particles, potentially contributing to the blocking or collapse of pores and the subsequent decrease in the specific surface area62. Furthermore, the conversion of micropores into mesopores also contributes to the decline in surface area. From Fig. 6-a, ZnS exhibits type IV isotherms with an H3 hysteresis loop, while ZnS-ZnO and ZnO display H1 hysteresis loops. These loop types provide insight into the dominant pore geometries: ZnS primarily features narrow parallel-plate pores, ZnS-ZnO presents cylindrical pores open at both ends, and ZnO demonstrates a mixture of non-parallel and cylindrical planar pores63,64. Furthermore, the BJH diagram (Fig. 6-b) indicates that the pore size distribution in ZnS-ZnO and ZnO is broader than that of ZnS. The average pore diameter for ZnS-ZnO is 23.5 nm, which is larger than those of ZnS (5.5 nm) and ZnO (13.6 nm). A broader hysteresis loop indicates an extensive range of pore sizes64. However, ZnS retains highest pore volume, indicating that oxidation leads to the development of larger pores while maintaining some of the smaller ones inherent to ZnS. Micropore volumes, as represented in the MP diagram and detailed in Table 1, support these observations. ZnS demonstrates a higher micropore volume compared to ZnS-ZnO and ZnO. In comparing the distribution of porosity, it is determined that ZnO predominantly contains mesopores, with a limited volume of micropores. This structural characteristic contributes to its relatively lower specific surface area when compared to ZnS. These findings emphasize the importance of both micro and mesoporous structures in controlling photocatalytic performance. The coexistence of mesopores (which improve molecular diffusion and light scattering) and micropores (which increase surface area and adsorption potential) enables more efficient interaction between dye molecules and active sites. Therefore, the observed degradation behavior is closely linked to the hierarchical porosity of the synthesized materials, rather than surface area alone15.
Fig. 6
(a) N2 adsorption/desorption isotherms, (b) BJH, and (c) MP-plot of ZnS, ZnS-ZnO, and ZnO.
The use of a non-solvent environment (ethanol) during the synthesis of ZnS contributes to its high specific surface area. However, the presence of the NaNO₃ by-product, which is insoluble in ethanol, requires washing with water to remove it. The removal of NaNO₃ is the main mechanism through which porosity is introduced into the samples. The XRD pattern of ZnS-NaNO₃ is provided in Figure S1 (Supplementary Materials). After washing, only ZnS peaks are observed, as shown in the XRD results of Fig. 2. The specific surface area of this sample is determined to be 9.26 m2 g−1 based on Figure S1-b (Supplementary Materials). The elimination of NaNO3 from the ZnS-NaNO3 induces porosity in the remained ZnS particles. A summary of all results obtained for the synthesized structures is presented in Table 1.
Table 1 Summary of BET analysis results.
According to the diffuse reflectance spectroscopy (DRS) analysis in Fig. 7, the samples exhibit strong absorption mainly in the ultraviolet (UV) range (200–400 nm) and relatively weak absorption in the visible region (400–700 nm). The absorption edge for ZnS appears around 370 nm, while ZnS-ZnO and ZnO both exhibit absorption edges around 450 nm. Notably, ZnS shows higher absorption in the UV region, whereas the opposite trend is observed in the visible light region.
To calculate the bandgap energies of the samples, Tauc’s theory was applied using the following equation:
$$:{upalpha:}h=A{({E}_{g}-h)}^{n}:$$
(4)
Here, α is the absorption coefficient, hν is the photon energy, Eg is the bandgap energy, A is a material-dependent constant, and n depends on the nature of the electronic transition. The Beer-Lambert law was used to determine the absorption coefficient65:
$$alpha = -frac{1}{t} InT$$
(5)
Where T is the value of the transmitted beam, and t is the thickness of the used sample. By extrapolating the plots of (αhυ)0.5-hυ, the bandgap energies of the ZnS, ZnS-ZnO, and ZnO were found to be 3.36 eV, 2.88 eV, and 2.96 eV, respectively.
To further investigate the electrochemical properties and energy band levels of the prepared semiconductors, the Mott-Schottky technique was used. The Mott-Schottky equation is as follows66:
where C is the depletion layer capacitance, εr is the dielectric constant of the semiconductor, ε0 is the vacuum permittivity, e is the initial electric charge, ND is the donor density, E is the applied potential, EFB is the flat band potential, k is Boltzmann’s constant, and T is the temperature.
The Mott-Schottky plots in Fig. 7(b-e) reveal n-type behavior for all three materials-ZnO, ZnS, and ZnS-ZnO-evidenced by the positive slopes in their respective plots. By extrapolating the linear portion of the curves, the flat band potentials were estimated and then converted to the normal hydrogen electrode (NHE) scale using the following equation:
$$:{E}_{NHE}={E}_{FB}+02$$
(7)
It is important to note that the conduction band (CB) level of an n-type semiconductor is typically 0.1 V more negative than the flat band potential66. Based on the conduction band energy and the previous calculated band gaps, the valance band (VB) energy levels were determined as shown in Table S2 (Supplementary Materials). Figure 7-e illustrates the energy levels of the semiconductors. Additionally, the charge carrier densities were calculated to be 9.21 × 1015 cm−3 for ZnS, 1.07 × 1016 cm−3 for ZnS-ZnO, and 2.58 × 1015 cm−3 for ZnO.
Photoluminescence (PL) analysis of the synthesized compounds provides valuable insights into charge generation and the behavior of electrons and holes. Figure 7(f) and (g) display the PL spectra of the three samples at excitation wavelengths of 300 nm and 350 nm, respectively. Emission in the 380–550 nm range is attributed to various defect states, including Zn2+ vacancies, S2− vacancies, dislocations, and interstitials. the intensity of emission associated with Zn2+ and S2− vacancies decreases upon oxidation, suggesting that charge carriers are trapped at defect sites41. An emission peak around 360 nm could be assigned to exciton recombination. The weak blue emission observed at approximately 450 nm may be due to zinc vacancies or surface states. For ZnS, the emission peak observed in the visible region (~ 480–520 nm) can be ascribed to sulfur vacancies and zinc interstitials67. In ZnO, a sharp emission at ~ 380 nm is due to the corresponding recombination, while a broad visible emission centered around ~ 500–550 nm is attributed to deep-level or trap-state emissions, commonly linked to intrinsic defects such as oxygen vacancies, zinc interstitials, and oxygen interstitials. Following oxidation, an increase in ultraviolet emission is observed, which may be due to ZnS-ZnO facilitating the tunneling or transportation of charge carriers from ZnS to ZnO. This process leads to a higher number of photogenerated electrons and holes being confined inside the ZnO68. Furthermore, The green emission observed at around 500 nm in ZnO is attributed to profound levels like oxygen vacancies or surface states69.
Fig. 7
(a) Bandgaps calculated from DRS data of ZnS, ZnS–ZnO and ZnO, mott-Schottky plots of (b) ZnS, (c) ZnS-ZnO, (d) ZnO, and (e) schematic of valence/conduction band’s energy level of ZnS and ZnO, PL spectra of ZnS, ZnS–ZnO, and ZnO at excitation wavelengths of (f) 300 nm and (g) 350 nm.
The photocatalytic potential was evaluated by monitoring the decomposition efficiency of methylene blue, an organic contaminant with a maximum absorption peak at 663 nm. As illustrated in Fig. 8(a-c), the absorption spectrum of methylene blue displays a distinct peak that decreases over time, indicating photocatalytic degradation. Figure 8-d displays the time-dependent changes in methylene blue concentration, reflecting the ability to absorb and the level of photocatalytic performance. To further quantify the degradation behavior, pseudo-first-order kinetic analysis was performed. The linear relationship of ln (C0/C) versus time provided rate constants (k) and correlation coefficients (R2) for each sample. Among the three photocatalysts, ZnS showed the highest rate constant (k = 0.005 min−1, R2 = 0.66), confirming its superior photocatalytic activity under visible light. ZnO and ZnS-ZnO also followed pseudo-first-order kinetics with a strong linear correlation. This kinetic evaluation supports the observed trends in dye removal efficiency. The decolorization efficiency (η) can be calculated using the following equation:
$$:{upeta:}=frac{{C}_{0}-C}{{C}_{0}}times:100$$
(8)
where C0 represents the initial concentration and C denotes the concentration following irradiation.
Figure 8-e illustrates the efficiency of color removal, with ZnS demonstrating the highest efficiency. ZnS-ZnO follows, achieving 55% decomposition, while ZnO exhibits the lowest efficiency, removing only 43% of the organic pollutants. Furthermore, Fig. 8-f presents the results of the absorption percentage of methylene blue in the dark. In dark status, ZnS shows higher absorption rate compared to the other samples within 30 min.
A collective interpretation of various analyses, including XRD, UV-Vis, FESEM, and. confirms the successful formation of crystalline, nanoscale semiconductors with a defined morphology and optical activity. While our synthesis does not involve phytochemical agents, the obtained structural and optical features are comparable to those reported in biogenic synthesis routes70,71.
Fig. 8
Methylene Blue absorbance spectra with (a) ZnS, (b) ZnS-ZnO, and (c) ZnO, (d) experimental results of degradation of methylene blue under LED lamp, (e) decolorization efficiency of methylene blue, and (f) bar chart of methylene blue adsorbed in darkness by ZnS, ZnS-ZnO, and ZnO catalysts.
Process mechanism
The degradation mechanism of methylene blue is schematically demonstrated in Fig. 9. As shown in Table 2, the superior photocatalytic activity of ZnS compared to ZnS-ZnO can be attributed to several factors, despite ZnS having a larger bandgap, fewer charge carriers, and a higher potential for electron-hole recombination. It is important to note that the photocatalytic tests were conducted under a cool-white LED light source (50 W, Brux, China), which emits primarily in the visible light range. One significant factor handling the present result is the high porosity of ZnS, which enhances light scattering and increases the degradation of pollutants. The presence of pores in ZnS particles provides additional active sites for adsorption and catalytic reactions, thereby enhancing overall methylene blue removal activity72. Additionally, porosity in ZnS can modulate its electronic properties by including its band structure and energy levels. These surface states can facilitate charge separation and reduce recombination, thus positively influencing photocatalytic activity.
The interconnected pores in the ZnS structure form continuous channels that facilitate the migration of photogenerated charge carriers (electrons and holes), reducing the diffusion length to active sites and increasing their lifetime. This structural feature enhances the probability of charge carriers reaching the catalytic interface before recombination, a phenomenon referred to as dynamic photocatalytic degradation. Moreover, ZnS exhibits a higher adsorption capacity under dark conditions compared to ZnS-ZnO and ZnO, due to its larger specific surface area (as shown in Fig. 8-b). When the lamp is turned on during the photocatalytic treatment, both the production of charge carriers and the adsorption of pollutants continue. This dual mechanism is schematically illustrated in Fig. 9 (a and b). In the initial stage (darkness), methylene blue is adsorbed onto the high surface area of ZnS particles, leading to a reduction in pollutant concentration. Subsequently, when the lamp is turned on, photons reach the ZnS surface, initiating the degradation (decomposition) of methylene blue most likely to CO2 and H2O73,74. This process refreshes the surface for the re-adsorption of pollutants, effectively enhancing the photocatalytic efficiency of ZnS.
Table 2 Summary of comparative results.
The inter-band energy levels in the ZnS structure can greatly influence its photocatalytic efficiency. In the ZnS lattice, the existence of defects can create sub-bands energy states located below the conduction band, thereby broadening the light absorption range and facilitating more effective photoexcitation. These additional energy states increase the number of excited electrons and holes available to participate in redox reactions, particularly in the oxidation of organic pollutants, thereby improving the overall photocatalytic activity. Defects within the ZnS lattice, such as S vacancies (VS), Zn vacancies (VZn), and interstitial atoms of Zn and S (IZn and IS), play a crucial role in this process. As illustrated in Fig. 9-c, the schematic energy level diagram shows how these four types of defects contribute to the electronic structure of ZnS. Sulfur vacancies and interstitial Zn atoms act as donor-like charge states, while Zinc vacancies and interstitial Sulfur atoms act as acceptor states.
Photoluminescence analysis supports this interpretation, with emission peaks in the blue (430–470 nm) and green (510–550 nm) regions. The blue emission is associated with sulfur vacancies, interstitial Zn atoms, and surface states, while the green emission originates from electron transitions between sulfur vacancy levels and intermediate sulfur states, followed by recombination. These defects not only modify the electronic properties of ZnS but also act as active sites that enhance the adsorption of reactant molecules and improve the separation of photogenerated electron-hole pairs. This suppression of charge carrier recombination extends their lifetimes and increases their participation in surface redox reactions, which is crucial for efficient photocatalysis. In particular, sulfur vacancies are known to reduce the energy barrier for interfacial charge transfer, thereby facilitating more efficient electron transport from the ZnS surface to adsorbed target molecules. These vacancies serve as electron “bridges,” effectively lowering the activation energy required for photocatalytic degradation reactions and enhancing overall efficiency69,75,76.
Finally, it is important to note that the light source-an LED lamp in the present study-also significantly influences the photodegradation performance of these three semiconductors. Selection of the light source the spectra of which can excite electrons from valence to conduction band, which means the energy of the photons are equal or greater than the band gap of the synthesized particles, results in substantial difference of their photodegradation performance77.
In addition to the surface- and defect-related mechanisms discussed earlier, it is worth mentioning the possible contribution of a dye-sensitization mechanism under visible light irradiation. ZnS, due to its wide band gap, does not intrinsically absorb visible light efficiently. However, methylene blue, which strongly absorbs in the visible region, may act as a photosensitizer. Upon excitation by visible light, methylene blue molecules can inject electrons into the conduction band of ZnS, initiating photocatalytic degradation via reactive oxygen species formation. This sensitization mechanism has been previously reported in similar systems where dye molecules extend the photoresponse of wide-band-gap semiconductors into the visible range through interfacial charge transfer78. While this effect was not the focus of this study, it may partially contribute to the unexpectedly high degradation efficiency observed for porous ZnS under visible LED illumination.
Fig. 9
The schematic of photocatalytic degradation of methylene blue (a) in darkness, and (b) after LED irradiation and (c) the schematic of ZnS inter-band energy levels.
In the ZnS-ZnO structure illustrated in Fig. 10, photoexcitation by incident photons promotes electrons from the valence band of ZnS to its conduction band, leaving behind holes. A similar excitation process occurs in ZnO. Due to the lower conduction band potential of ZnS relative to ZnO, electrons tend to migrate from ZnS to ZnO, establishing Fermi level equilibrium and generating an internal electric field across the heterojunction. This electric field facilitates the transfer of holes from the valence band of ZnS to that of ZnO, thereby enhancing charge separation, particularly on the ZnS side. However, the transfer of electrons from ZnS to ZnO is limited by energy barriers due to the differences in conduction and valence band energies between these two compounds. Thus, this heterojunction primarily facilitates the spatial separation of photogenerated charge carriers on the ZnS side, while contributing only modestly to charge separation in ZnO. Consequently, electron-hole pairs are not fully separated across both semiconductors, and recombination processes-particularly in ZnO-still occur.
Contrary to many previous studies that reported superior photocatalytic activity for ZnS-ZnO heterostructures compared to the individual components (Table 3), our experimental results show that pure porous ZnS outperforms the ZnS-ZnO composite in degrading methylene blue. While ZnS-ZnO structures are generally favored due to efficient heterojunction-mediated charge separation, our findings suggest that specific surface area is a more critical factor than previously assumed. In our study, electrons from the conduction bands of both ZnO and ZnS, as well as holes in the valence band of ZnO, contribute to the photocatalytic reaction. However, due to the lower specific surface area of ZnS-ZnO, fewer pores are exposed to methylene blue adsorption compared to ZnS, resulting in the decreased photocatalytic efficiency. This deviation between literature and our research can also be related to the interface mismatch between ZnS and ZnO, in addition to the specific surface area discussed above. This interface mismatch may hinder carrier movement and instead act as a site for electron-hole recombination, thereby reducing efficiency. Additionally, most charge recombination occurs in ZnO, further contributing to the lower removal efficiency compared to the other two compounds79,80,81.
Fig. 10
Energy-band diagrams of ZnS-ZnO (a) before irradiation, (b) during equilibration EF and (c) in the photocatalytic mechanism.
Table 3 Comparison of photocatalytic performance of ZnS-ZnO systems reported in recent literature with the present study.
As previewed earlier this year, Gemini in Google Docs will now let you “create audio versions of your documents.”
On the web, go to the Tools menu for a new “Audio” option in-between Voice typing and Gemini. Tapping “Listen to this tab” will open a pill-shaped player, with the duration noted. You can move this floating window anywhere on the screen.
Besides play/pause and a scrubber, available controls include playback speed and changing the “clear, natural-sounding voices.” Options include:
Narrator
Educator
Teacher
Persuader
Explainer
Coach
Motivator
Meanwhile, editors can add an audio button anywhere in the document for viewers of the document.
Advertisement – scroll for more content
Insert menu > Audio buttons > Listen to tab
@Listen to tab
Google Docs Audio is handy if you “want to hear your content out loud, absorb information better while reading, or help catch errors in your writing.”
This is currently just available in English and on the web, with the rollout starting today and continuing over the next few weeks. It’s available for Google AI Pro and Ultra subscribers, as well as:
Business Standard and Plus
Enterprise Standard and Plus
Customers with the Gemini Education or Gemini Education Premium add-on
Customers with the Gemini Business or Gemini Enterprise add-on*
Meanwhile, Google Docs on Android is rolling out the ability to generate images. This is also available for AI Pro/Ultra subscribers.
More on Google Docs:
FTC: We use income earning auto affiliate links. More.
People living in the most advantaged areas of Australia tend to drink more alcohol. But people who live in the least advantaged areas suffer the most alcohol-related harms, such as dying from alcohol-related disease or from alcohol-related injuries.
This puzzling phenomenon is known as the “alcohol harm paradox” And knowing what’s behind it has real-world implications.
It can help explain why educational campaigns to drink less alcohol, such as the “sober curious” movement, don’t always reach those most at risk of harm.
It can also help us design better policies to prevent alcohol-related harms – including some policies unrelated to alcohol.
So, rich people drink more?
In 2022, for example, about 31% of Australians living in the most advantaged neighborhoods exceeded national guidelines for risky drinking in the past year. That’s compared with about 22% in the least advantaged neighborhoods.
However, people living in more disadvantaged areas have more alcohol-related problems than people with living in more advantaged areas.
For instance, research from the United Kingdom shows those living in the most disadvantaged neighborhoods are about 2.2 times more likely to die from alcohol problems than those in the least disadvantaged neighborhoods.
Why is this happening?
Researchers have tried to explain why this is happening. Many have pointed to behavioral factors – choices that people make and actions they take.
For instance, researchers have questioned whether the type of alcohol, patterns of heavy drinking, or where people drink, might explain why people in disadvantaged areas suffer more from alcohol-related harms. But many studies show these factors do not explain it.
Could the combination of drinking with smoking and/or illicit drugs be a factor? Could it be linked to obesity, which we know is more common in lower socioeconomic groups? Research shows this is not the explanation either.
This focus on people’s behavior can have unintended consequences. Yes, it can lead to policies that try to get people to change their alcohol use or health behavior, which can work for some groups. But such policies can exclude those most at risk of harm.
Why educational campaigns don’t always work
One common policy to try to change people’s behavior is an educational campaign – the type we’d see on TV, online or on social media – to promote a healthy relationship with alcohol.
People living in more advantaged neighborhoods, or with higher incomes, have greater access to material and social resources. They can draw on these resources – including organizations or individuals that can support them – to avoid risks, reduce the consequences of health and social problems, and take treatment to improve their health and wellbeing.
But people in lower socioeconomic groups may not have equal access to public health messages (for instance, through less access to good quality health care), understand these messages in the same way, or have the same resources and capacities to change their behavior.
So educational campaigns can actually increase health inequalities.
Are you ‘sober curious’?
I was involved in an Australian study that looked at being “sober curious”, a social movement that emphasizes being curious about living life or attending events without drinking alcohol. We explored individuals of different socioeconomic status and whether they were prepared to engage with being sober curious.
Participants of higher socioeconomic status found notions of being sober curious resonant, useful and fitted their lifestyles. But participants of lower socioeconomic status found it “for someone else” and didn’t identify with the concept.
In other words, the group most at risk of alcohol-related harms would have been least likely to take part.
Other interventions that may worsen alcohol-related inequalities also focus on an individual changing their behavior. These include national guidelines on how much alcohol is safe to drink, and bans on drinking in public spaces that marginalize disadvantaged communities. These are policies that many Australians and policy makers think useful or necessary.
So to reduce alcohol-related inequality we need to fundamentally rethink the types of policies to reduce its harms.
So how can we design better policies?
We need to shift the focus from individual behavioral factors to see how broader social and structural conditions affect people’s health, and design policies to address these.
We need national policies that reduce drinking across the population. These include policies to reduce the availability of alcohol, especially avoiding clustering alcohol outlets in disadvantaged areas.
Another proven effective policy measure involves increasing the price of alcohol so that it cannot be sold under a certain “floor price”. This reduces the availability of very cheap alcohol.
However, policies that address the alcohol harm paradox most successfully may not be relevant to alcohol, but those that focus on reducing health inequality more broadly. These might include more equitable access to housing and better workplace policies as well as more equitable access to health care.
Amy Pennay is Senior Research Fellow and Deputy Director, Centre for Alcohol Policy Research, La Trobe University.
The Conversation is an independent and nonprofit source of news, analysis and commentary from academic experts.
Roughly 12,800 years ago, as Earth was emerging from its last great ice age, temperatures in the Northern Hemisphere suddenly plummeted back to near-glacial conditions. The cause of this abrupt shift—known as the Younger Dryas cool period—remains a mystery to this day, but new evidence may give credence to its most controversial explanation.
Researchers analyzed sediment cores extracted from the seafloor of Baffin Bay near Greenland, finding indicators of a cosmic impact event inside the layer that correlates to the Younger Dryas. The findings, published August 6 in the journal PLOS One, suggest that a comet—or its remnants—exploded in Earth’s atmosphere at around the same time that this 1,200-year-long cold snap began.
A controversial hypothesis
The study offers new support for the Younger Dryas Impact Hypothesis. In 2007, researchers proposed that fragments of a disintegrating comet or asteroid struck Earth around 12,800 years ago, triggering wildfires across North America. Such a calamity would have produced enough soot and ash to blot out the Sun and plunge the Northern Hemisphere back into a colder state.
It’s an elegant explanation, but a highly contested one. Researchers haven’t found an impact crater that would prove this event took place, so proponents largely rely on geochemical evidence found in sediment layers that date back to just before the Younger Dryas began.
Amid a lack of definitive evidence for the Younger Dryas Impact Hypothesis, most experts instead subscribe to the Meltwater Pulse Hypothesis, which suggests that a deluge of freshwater from the melting ice sheet that covered most of North America during the Pleistocene temporarily interfered with Earth’s heat-transporting ocean currents. Previous geochemical evidence from ocean sediment cores supports this idea, but scientists have yet to determine the exact route taken by this apparent flood.
Searching for impact clues
The authors of this latest study, led by University of South Carolina archaeologist Christopher R. Moore, suggest that both hypotheses may be true. “The [Younger Dryas Impact Hypothesis] is often cited as an alternative to the Meltwater Pulse Hypothesis,” Moore said in an interview with PLOS One. “What many don’t understand is that the YDIH proposes the impact event (potentially involving many thousands of impacts and airbursts globally) would destabilize the glacial ice sheet in the Northern Hemisphere, leading to the collapse of massive glacial meltwater lakes and subsequently shutting down the ocean’s conveyor belt.”
Previous studies of terrestrial sediment cores have found geochemical clues of a comet impact around the onset of the Younger Dryas, but Moore and his colleagues wanted to see whether ocean cores would contain the same clues. If so, this would dispel arguments that land-based evidence of a Younger Dryas impact event resulted from ancient human activities, according to Moore. His team uncovered multiple impact proxies that date back to the appropriate time period inside the ocean cores, including metal particles with compositions that suggest cometary origin and iron- and silica-rich microspherules.
Skepticism remains
Still, not everyone is convinced. “I do not see anything in this new paper that overcomes the chronic and ongoing problems with their previous papers,” Mark Boslough, an applied physicist and research professor at the University of New Mexico, told Gizmodo in an email. As an outspoken critic of the Younger Dryas Impact Hypothesis, he believes there are much simpler explanations that are more consistent with our current understanding of impact and airburst physics, earth science, and astronomy.
“On the surface, they report materials that sound exotic and impressive, but these are not expected results of extraterrestrial events, and I don’t think the authors seriously considered more ordinary explanations,” Boslough said.
Research led by investigators at Mass General Brigham suggests that the health benefits of more aggressive blood pressure control outweigh concerns about overtreating people with high blood pressure readings. Results of the simulation study are published in Annals of Internal Medicine.
The study used data from the Systolic Blood Pressure Intervention Trial (SPRINT) trial, the National Health and Nutrition Examination Survey (NHANES), and other published literature to simulate lifetime health outcomes—including heart attack, stroke, and heart failure—for patients whose systolic blood pressure targets were set at <120 mm Hg, <130 mm Hg, and <140 mm Hg. Recognizing that blood pressure medication comes with side effects, the researchers also simulated and compared the risk of serious events resulting from the treatment.
The simulation model also accounted for common errors in patients’ blood pressure readings based on what has been observed in routine clinical practice.
Even when including this error rate, the simulation model found the <120 mm Hg target prevented more cardiovascular events, such as heart attacks, strokes, and heart failure than the <130 mm Hg target. However, the lower target led to additional adverse events related to treatment, such as falls, kidney injury, hypotension, and bradycardia. The lower target also increased overall healthcare spending due to increased antihypertensive use and more frequent visits with clinicians.
Comparing the cost-effectiveness of the three blood pressure targets with typical levels of measurement error, the researchers found the <120 mm Hg target was cost-effective, associated with a cost of $42,000 per quality-adjusted life-year gained.
“This study should give patients at high cardiovascular risk and their clinicians more confidence in pursuing an intensive blood pressure goal,” said lead author Karen Smith, PhD, an investigator at the Department of Orthopedic Surgery at Brigham and Women’s Hospital, a founding member of the Mass General Brigham healthcare system. “Our findings suggest the intensive <120 mm Hg target prevents more cardiovascular events and provides good value, and this holds true even when measurements aren’t perfect.”
Smith also cautioned, “Our results examine the cost-effectiveness of intensive treatment at the population level. However, given the additional risk of adverse events related to antihypertensives, intensive treatment will not be optimal for all patients. Patients and clinicians should work together to determine the appropriate medication intensity based on patient preferences.”
Compact, reflective, easy to manufacture mirrors are a critical component for advancing astronomical technology in space. Mirrors are a key component in most telescopes, though they are notoriously hard to manufacture with the necessary precision, especially at large scales. A new paper from researchers in the UK uses additive manufacturing to make a thin, flexible, and lightweight mirror out of aluminum and analyzes its properties to see if it will be useful in applications such as CubeSats.
Before the researchers could make the actual mirror, they had to make several decisions about its design. In choosing a lattice, they decided to use a “split-p internal lattice”, which basically looks like a honeycomb. In finite element analysis (FEA) modeling, it was shown to be the most robust. The team also designed a mounting structure that utilized four printed circuit boards (PCBs) as mounting rods, which was part of the overall CubeSat bus design the system was going for.
In running further FEA models, the researchers found they could reduce the weight of the mirror by about 56%, close to the 60% it was originally designed for. They then went about actually manufacturing five prototypes, which was designed in an annular shape with the outer ring approximately 84mm an an inner one at 32mm. The printing was completed using a standard laser-bed powder fusion process commonly used to 3D print metals. In this case, the metal was AlSi10Mg, a typical alloy of aluminum used in the 3D printing.
Fraser discusses the disadvantages/disadvantages of CubeSats vs large missions.
But since this was intended for use as a mirror, the print underwent further processing once it was initially laid down. Two underwent Hot Isostatic Pressing, which heats the print and then applies pressure to it in an effort to reduce its porosity and increase its surface uniformity. Chasing a smooth surface, the researchers subjecting four samples to single-point diamond turning, a post-processing technique that removes the top layer of material using a precise diamond-coated lathe.
After post-processing the samples were analyzed both internally and externally. To scan a samples internals the researchers used X-ray Computed Tomography, and found that there were small pores throughout the structure, and they seemed to track along the path of the laser used in the fusion process. There was a higher density of them around the perimeter, where the laser turns around.
Surface roughness is a key metric of mirrors used in telescopes, and all of the samples had less than 8nm of surface roughness, though those subjected to HIP were slightly rougher than the ones milled off with a diamond. The tradeoff was that the HIP process did in fact reduce porosity, making the material stronger internally. HIP processed mirrors also had a higher Total Integrated Scatter value, probably because of their higher surface roughness. Which also means they were bad for use in a telescope.
Details on CubeSat Optics from the 2021 CubeSat Developers Workshop. Credit – CubeSat YouTube Channel
There were also scratches scattered throughout the surface, seemingly caused by an alloy of titanium and vanadium. That would imply the feedstock aluminum alloy might have been inadvertently mixed with another metal powder.
Despite these setbacks, the process described in the paper represents a step forward for the development of CubeSat suitable, lightweight flexible mirrors. In the future, the researchers plan to add a chromium optical coating to the surface to try to improve the surface quality of the samples. They’ll also test the thermal flexibility of the system, testing what it would be like in an actual space environment. As the mirrors continue their path up the technology readiness levels, there will be an increasing demand from an increasing number of CubeSat manufacturers who will need inexpensive, robust, lightweight mirrors.
Learn More:
I. Aziz et al – Additive manufacturing in aluminium of a primary mirror for a CubeSat application: manufacture, testing and evaluation.
UT – Lightweight Telescopes In CubeSats Using Carbon Nanotube Mirrors
UT – Teeny Tiny CubeSats Could Have Deployable Mirrors Like James Webb
UT – A CubeSat Design for Monitoring the Whole Sky In UV
In a world where prices on everything seem to be skyrocketing, it’s only natural that everyone is searching for cheaper alternatives to their go-to products —and that includes beauty.
While you might love that $60 serum or foundation, your bank account is secretly hoping that you’ll buy a budget-friendly option instead.
If you think nothing can compete with your favorite luxury makeup and skincare, think again. Drugstore beauty brands like e.l.f., Milani, and Maybelline are delivering high-performing products at unbelievably low prices.
Even more, these drugstore finds are dupes for fan-favorite products from Charlotte Tilbury, Milk Makeup, Dr. Dennis Gross, and more.
Basically, you don’t have to skimp on quality if you want to save, because the drugstore has alternatives that work as well (or even better) than their high-end counterparts.
Why spend when you can save? Keep reading to shop the best drugstore alternatives to luxury brands.