ORIGINAL RESEARCH article
Sec. Aquatic Microbiology
Volume 12 - 2021 | https://doi.org/10.3389/fmicb.2021.651567
Ultraviolet Radiation Stimulates Activity of CO2 Concentrating Mechanisms in a Bloom-Forming Diatom Under Reduced CO2 Availability
- 1State Key Laboratory of Marine Environmental Science and College of Ocean and Earth Sciences, Xiamen University, Xiamen, China
- 2Department of Technology and Resource Management, Guangdong Jiangmen Chinese White Dolphin Provincial Nature Reserve Management Bureau, Jiangmen, China
The diatom Skeletonema costatum is cosmopolitan and forms algal blooms in coastal waters, being exposed to varying levels of solar UV radiation (UVR) and reduced levels of carbon dioxide (CO2). While reduced CO2 availability is known to enhance CO2 concentrating mechanisms (CCMs) in this diatom and others, little is known on the effects of UV on microalgal CCMs, especially when CO2 levels fluctuate in coastal waters. Here, we show that S. costatum upregulated its CCMs in response to UVR (295–395 nm), especially to UVA (320–395 nm) in the presence and absence of photosynthetically active radiation (PAR). The intensity rise of UVA and/or UVR alone resulted in an increase of the activity of extracellular carbonic anhydrase (CAe); and the addition of UVA enhanced the activity of CCMs-related CAe by 23–27% when PAR levels were low. Such UV-stimulated CCMs activity was only significant at the reduced CO2 level (3.4 μmol L−1). In addition, UVA alone drove active HCO3− uptake although it was not as obvious as CAe activity, another evidence for its role in enhancing CCMs activity. In parallel, the addition of UVA enhanced photosynthetic carbon fixation only at the lower CO2 level compared to PAR alone. In the absence of PAR, carbon fixation increased linearly with increased intensities of UVA or UVR regardless of the CO2 levels. These findings imply that during S. costatum blooming period when CO2 and PAR availability becomes lower, solar UVR (mainly UVA) helps to upregulate its CCMs and thus carbon fixation, enabling its success of frequent algal blooms.
Anthropogenically released chemicals such as chlorofluorocarbons (CFCs) and other chlorine-containing volatile gases have resulted in the decline of ozone in the stratosphere since the 1970s, leading to increasing UV radiation (UVR) on the ground (Stolarski, 1988; Staehelin et al., 2001; Manney et al., 2011). Due to the effective implementation of the Montreal Protocol, stratospheric ozone depletion has been stalled and a recovery in the Antarctic ozone hole seems to occur (Newman and Mckenzie, 2011; Solomon et al., 2016). However, in 2020, record-low ozone levels stretched across much of the central Arctic, covering an area about three times the size of Greenland (Witze, 2020). This vast ozone hole is probably the biggest on record in the Northern Hemisphere, which was caused by very chilly temperatures that induced the formation of high-altitude clouds and the ozone-destroying reactions. Therefore, variations of solar UVR reaching the earth surface remains uncertain. Solar radiation is essential for photosynthesis of primary producers on Earth, but its UV component (100–400 nm) could do harms to living organisms. UVR is commonly divided into three wavelength bands: UVA (315–400 nm), UVB (280–315 nm), and UVC (100–280 nm). Most UVA and partial UVB can reach the surface of Earth with UVC completely filtered out by ozone in the Earth’s atmosphere (mainly stratosphere). UVB only accounts for about 0.2% of total solar irradiance that reaches the ground at noon and UVA accounts for about 5% in the areas without ozone holes (Koronakis et al., 2002; Dias and von Sperling, 2017). It has been intensively reported that UVB can induce free oxygen radicals, impair the structure and function of DNA and proteins (Boelen et al., 2000; Gao et al., 2009), inhibit photosynthetic activity (Sobrino et al., 2008; Yin and Ulm, 2017), and thus reduce algal growth and primary productivity (Gao et al., 2009; Li et al., 2011; Domingues et al., 2017). On the other hand, UVA at low to moderate levels was found to stimulate carbon fixation of algae. For instance, UVA could stimulate photosynthetic carbon fixation of phytoplankton in coastal waters of South China Sea in summer by up to 25% (Li et al., 2011). The growth rate of brown alga Fucus gardneri embryos was also enhanced by UVA radiation (Henry and Van Alstyne, 2004). Previous studies about the effects of UVR usually employed different radiation treatments in the presence of PAR with or without UVR. Since there are potential interaction between UVR and PAR (Liu et al., 2014), it would be more essential to expose cells to UVR alone when investigating the effects of UVR. However, this kind of studies is very few. Gao et al. (2007) found that photosynthetic carbon fixation of phytoplankton assemblages in a coastal area (23°29'N, 117°06'E) of the South China Sea increased linearly with UVA or UVR alone. In addition, it was reported that UVA alone could be utilized by the red alga Gracilaria lemaneiformis to drive O2 evolution and carbon fixation (Xu and Gao, 2010; Xu et al., 2018). However, the potential mechanisms of UVR driving carbon fixation of algae remain unclear.
Carbon dioxide (CO2) is the essential substrate for algal photosynthesis. Although there are abundant dissolved inorganic carbon (DIC, ~2 mM) in seawater, the predominant form is HCO3− with CO2 accounting for less than 1% (~13 μM). The key enzyme in photosynthetic carbon fixation, ribulose-1,5-bisphosphate carboxylase/oxygenase (Rubisco), that catalyzes the conversion of CO2 into organic carbon, has a relatively low affinity for CO2 and is commonly less than half saturated in most marine microalgae under current CO2 levels (Hopkinson et al., 2011; Goudet et al., 2020), limiting marine algal carbon fixation. Accordingly, most algae evolved CO2 concentrating mechanisms (CCMs), including enhanced carbonic anhydrase (CAe) activity, active uptake of HCO3−, acidified compartment, etc. (Giordano et al., 2005; Beardall and Raven, 2020), to deal with the CO2 limitation. Due mainly to human activities, CO2 level in seawater is predicted to increase in future (Pörtner et al., 2019) and, therefore, a large number of studies have been conducted to investigate the impacts of increased CO2 levels on algal CCMs and photosynthesis (Gao et al., 2017; Hennon et al., 2017; Raven et al., 2017; Porzio et al., 2018; Huang et al., 2019). On the other hand, CO2 level in coastal waters is very dynamic and could be lower than the current average value at noon when photosynthesis is intensive (Duarte et al., 2013; Raven et al., 2020). For instance, the pH at noon could reach 8.9 in seawater of toosh Island (48.32°N, 124.74°W) located in the Eastern Pacific, leading to a low CO2 condition (Wootton et al., 2008). During algal blooms, seawater pH could be extremely high with CO2 availability being very low. It was reported that pH level in the surface waters of Mariager Fjord, Denmark, achieved 9.75 during an algal bloom (Hansen, 2002). Algal tolerance to high pH and low CO2 varies among species, which may be related to the capacity of their CCMs (Björk et al., 2004; Gao et al., 2018a).
In terms of the combined effects of UVR and CO2 on diatoms, most studies used elevated CO2 levels compared to ambient levels (Sobrino et al., 2008; Domingues et al., 2014; Gao et al., 2018c) and little is known regarding the interaction of reduced CO2 levels and UVR. Skeletonema costatum, as a ubiquitous diatom species, can be found from equatorial to polar areas. It has optional applications in lipid diet and biofuels (Berge et al., 1995; Gao et al., 2019a). Meanwhile, it is an opportunist that can grow very rapidly and lead to algal blooms in many coastal waters when the conditions are suitable (Shikata et al., 2008; Gao et al., 2019b; Zeng et al., 2019). It has reported that both UVA and UVB reduced photosynthetic carbon fixation of S. costatum grown under incident solar radiation (Gao et al., 2009). On the other hand, the extracellular CA activity and photosynthetic carbon fixation of S. costatum (Greville) Cleve could be stimulated by moderate levels of UVA or UVR when treated with visible radiation (Wu and Gao, 2009), implying a possibility that UVR may modulate CCMs in this diatom, which are closely related to activity of its extracellular CAe (Chen and Gao, 2003). It seems likely that S. costatum have developed a strategy to cope with UVR and reduced CO2 availability during its blooming. Here, we hypothesized that S. costatum may utilize UVR to stimulate its CCMs to deal with lower CO2 condition and maintain its photosynthesis when the light intensity is low. In this study, we cultured cells of S. costatum at two levels of CO2 and exposed them to different levels of UVR to test this hypothesis by monitoring the change of carbon fixation, effective photochemical efficiency, CAe activity, HCO3− utilization, etc.
Materials and Methods
Culture Conditions and Experimental Design
The experimental algal species, S. costatum (Greville) Cleve (strain 2042), was obtained from the Institute of Oceanography, Chinese Academy of Sciences. Before the experiment, cells were grown in sterilized seawater enriched with f/2 medium with the pH of 8.20 in an intelligent incubator (GXZ-300C, Jiangnan, Ningbo, China). The temperature was set at 20°C and intensity of PAR was 200 μmol photons m−2 s−1 (12:12 light:dark cycle). Cells at the exponential growth phase were harvested by centrifugation at 5,000 g for 10 min and transferred to two conditions. One was ambient CO2 (12.8 μmol L−1) and lower pH (8.2), and the other was lowered CO2 (3.4 μmol L−1) and higher pH (8.7) that simulates the situation when algal blooms occur (Brussaard et al., 1996). Before cultured at these two conditions, the harvested cells were washed twice with fresh media with the target CO2 levels. Cells were cultured in cylindrical quartz tubes (55 mm in diameter and 160 mm in length) and exposed to five radiation treatments (PAR, PAR + UVA, PAR + UVA + UVB, UVA, and UVA + UVB) for 1 h. The treatments of UVA and UVA + UVB were set to verify whether UVR alone could affect physiological performance of cells. Different radiance treatments were achieved by following operation: (1) PAR (395–700 nm), quartz tubes covered with Ultraphan film 395 (UV Opak; Digefra); (2) PAR + UVA (320–700 nm), quartz tubes covered with Folex 320 (Montagefolie no. 10155099; Folex, Dreieich, Germany); (3) PAR + UVA + UVB (295–700 nm), Ultraphan film 295 (UV Opak; Digefra, Munich, Germany); (4) UVA, a Folex 320 cutoff foil (Montagefolie, Nr. 10,155,099; Folex, Dreieich, Germany) was placed on the top of the PAR cutoff filter, UG11 (Schott, Mainz, Germany) to screen off UVB + UVC irradiance; and (5) UVA + UVB, a Ultraphan 295 foil (UV Opak; Digefra, Munich, Germany) was placed on the top of the UG11 filter (only UVR penetrable) to screen off UVC irradiance. Five levels of light intensity were set for five radiation treatments (Table 1), reflecting daily average light intensities of cloudy and sunny days in spring at Xiamen, China. Different radiance intensities were achieved by covering the tubes with different layers of neutral filtering screens. A solar simulator (Sol 1,200; Dr. Hönle GmbH, Martinsried, Germany) equipped with a 1,000-W xenon arc lamp was used for the experiment. The irradiances of PAR, UVA, and UVB were measured with a broadband filter radiometer (ELDONET, Real Time Computer, Möhrendorf, Germany). A cell concentration of 2 × 105 cells ml−1 representative of the biomass density during algal blooms (Gao et al., 2019b) was inoculated and the changes of pH levels were within 0.01 units. Cultures were carried out in triplicate.
Manipulation of Seawater Carbonate System
The two levels of pH (8.20 and 8.70) were obtained by adding NaHCO3 solution to sodium barbital buffered DIC-free seawater. DIC-free seawater was achieved by bubbling HCL acidified seawater (pH 2.0) with pure N2 for 1 h. The pHNBS was measured using a pH meter (Orion STAR A211, Thermo Scientific, United States) that was calibrated with standard National Bureau of Standards (NBS) buffers (pH = 4.01, 7.00, and 10.01 at 25.0°C; Thermo Fisher Scientific Inc., United States). The DIC was measured using a total organic carbon analyzer (TOC-5000A; Shimadzu, Kyoto, Japan). CO2 level in seawater was calculated via CO2SYS (Pierrot et al., 2006) based on measured pH and DIC and known levels of nutrients, using the equilibrium constants of K1 and K2 for carbonic acid dissociation (Roy et al., 1993) and the KSO4− dissociation constant from Dickson (1990).
Measurement of Carbon Fixation
Photosynthetic carbon fixation was measured using a 14C method (Gao et al., 2009). Briefly, cells grown under different treatments were transferred to cylindrical quarts tubes (15 ml, 17 mm in diameter and 69 mm in length) and injected with 50 μl-2.5 μCi (0.0925 MBq) NaH14CO3 solution (ICN Radiochemicals, United Kingdom). The incubation was conducted for 1 h under five radiation treatments (PAR, PAR + UVA, PAR + UVA + UVB, UVA, and UVA + UVB). Three quartz tubes were wrapped with aluminum foil as dark control. After the incubations, cells were filtered onto Whatman GF/F glass filters and then transferred into 20 ml scintillation vials. The filters were fumed with a high concentration of HCl (12 mol L−1) in a fuming cupboard for12 h to expel the non-fixed inorganic carbon and then dried in an oven for 6 h at 45°C (Gao et al., 2007). Three milliliter of scintillation cocktail (Wallac Optiphase HiSafe 3, United States) was added to the vials and incubated for 2 h at room temperature. The 14C incorporated via photosynthesis was counted with a liquid scintillation counter (LS 6500, Beckman Coulter, Fullerton, CA, United States), and the carbon fixation rate was calculated by the following equation: carbon fixation rate [mg C (mg Chl a)−1 h−1] = [(CPM(l)-CPM(d))/Ce] × If × DIC/A/T/CChl a, where CPM(l) and CPM(d) are the numbers of counts per minute in the “light” bottle and in the “dark” bottle, respectively, Ce is the counting efficiency of the counter, If is the isotope discrimination factor, DIC is the concentration of total dissolved inorganic carbon, A is the number of added μCi added multiplied 2.2 × 106, T is the incubation time, and C is the concentration of Chl a (Gao et al., 2007).
Measurement of PSII Activity
Activity of PSII, presented by the effective photochemical efficiency, was estimated by a portable pulse amplitude modulated fluorometer (PAMWATER-ED, Walz, Effeltrich, Germany). After exposed to different radiation treatments for 1 h, samples were transferred to the cuvette of the fluorimeter. The measuring light and saturating pulse were 0.01 and 4,000 μmol photons m−2 s−1 (0.8 s), respectively. The actinic light pulse was set to the corresponding intensity of PAR in the corresponding radiation treatments (zero for UV-alone treatments). The effective photochemical efficiency was determined as: F'v/F'm = (F'm − Ft)/F'm, where F'm is the instant maximal fluorescence and Ft is the steady-state fluorescence of light-adapted cells.
Estimate of Carbonic Anhydrase Activity
The activity of extracellular CAe of the intact cells was determined by an electrometric method based on Gao et al. (2009) with some modification. At the end of the exposure to different radiation treatments, the cells were immediately harvested by centrifugation (6,000 g, 4°C) for 10 min, washed and suspended in barbitone-buffered seawater (20 mM, pH 8.2). The cells were examined microscopically and no ruptured cells were found. One milliliter of cell suspension was added to 4 ml icy barbitone-buffered seawater and CO2-saturated icy distilled water (2 ml) was gently injected into the bottom of cell suspension (2 × 106 cells/ml). The time required for the pH to decrease from pH 8.2 to 7.2 was recorded. During the reaction, cell suspension was stirred and the temperature was controlled at 4°C. Activity of the enzyme was calculated as follows: EU = 10 × (T0/T − 1), where T0 and T represent the time required for the pH change in the absence or presence of the cells, respectively.
Test for pH Drift Under Different Radiation Treatments
To obtain the pH compensation point of S. costatum under different light conditions, cells grown at 200 μmol photons m−2 s−1 PAR were transferred to sealed quartz tubes (25 mm in diameter and 90 in length) and exposed to five radiation treatments at two levels of light intensity (Levels 3 and 5 in Table 1). The cell concentration for all treatments was 1.10 × 106 cells/ml and the temperature was kept at 20°C. The change of medium pH was monitored with a pH meter (Orion STAR A211, Thermo Scientific, United States) and the pH compensation point was obtained when there was no further increase in pH.
Results were presented as means of replicates ± SD and data were analyzed with the software SPSS v.23. The data from each treatment conformed to a normal distribution (Shapiro-Wilk, p > 0.05) and the variances could be considered equal (Levene’s test, p > 0.05). Three-way ANOVA was conducted to assess the effects of CO2, radiation spectrum and intensity on carbon fixation, effective photochemical efficiency, extracellular CAe activity, and pH compensation point. Least significant difference (LSD) was conducted for post hoc investigation. Repeated-measures ANOVA was conducted to assess the effect of incubation time on media pH in a closed system, with Bonferroni for post hoc investigation. The threshold value for determining statistical significance was p < 0.05.
Each factor (CO2, radiation spectrum, and intensity) affected CAe activity of S. costatum cells cultured in the presence of PAR and each two had an interactive effect (Supplementary Table S1). At ambient CO2 level (Figure 1A), CAe activity increased with radiation level until 51.84 W m−2 (238 μmol photons m2 s−1) PAR. There were no significant differences among radiation treatments. At lower CO2 level (Figure 1B), CAe activity increased first and then decreased with radiation level. Compared to PAR, PA stimulated CAe activity by 23 and 27% when PAR was 15.55 and 30.24 W m−2, respectively; PAB reduced it at all radiation levels. The lower CO2 level induced higher CAe activity at each treatment except for the highest PAB intensity.
Figure 1. Activity of extracellular carbonic anhydrase (CAe) of Skeletonema costatum cultured at ambient (A) and lower CO2 (B) levels when exposed to different radiation treatments. PAR, photosynthetically active radiation; PA, PAR + UVA, PAB, PAR + UVA + UVB. The error bars indicate the SDs (n = 3).
Similar to CAe activity in the presence of PAR, each factor (CO2, radiation spectrum, and intensity) affected CAe activity of S. costatum cells cultured in the absence of PAR, each two had an interactive effect except for radiation spectrum and intensity, and these three also interacted (Supplementary Table S1). When cells were transferred from the growth condition to UVA exposure (Figure 2A), cells grown under lowered CO2 condition had a big leap in CAe activity and the CAe activity increased with UVA intensity until 12.96 W m−2. On the other hand, CAe activity of cells grown under ambient CO2 condition did not change when transferred from growth condition to UVA intensities below 12.96 W m−2 and afterward it increased to 0.23 ± 0.02 EU at 12.96 W m−2 and did not vary until the highest intensity of 43.20 W m−2. When cells were exposed to UVR (Figure 2B), CAe activity in cells grown at lowered CO2 also increased with UVR intensity until 13.53 W m−2. For cells grown at ambient CO2, CAe activity did not change with light intensity but the highest intensity reduced it compared to the lowest intensity. For both UVA and UVR exposure, cells grown at lowered CO2 had much higher CAe activity than those at ambient CO2.
Figure 2. Activity of CAe of S. costatum grown at ambient and lowered CO2 levels when exposed to UVA (A) or UV radiation (UVR; UVA + UVB; B). The blue points represent the CA activity of cells cultured at pH 8.20 before exposed to UVR. The error bars indicate the SDs (n = 3).
To test whether S. costatum can utilize HCO3− even when exposed to UVR alone, pH drift experiment was conducted (Figure 3). Incubation time interacted with light intensity and spectrum to affect the pH in the diatom culture (Supplementary Table S2). At the low light intensity (Figure 3A), media pH under different light treatments increased with time. After 9 h exposure, the media pH under PAB, PA, and P exceeded 9.20, being 9.22 ± 0.05, 9.26 ± 0.01, and 9.20 ± 0.03, respectively. After 13 h exposure, media pH under PAB, PA, and P reached 9.30 ± 0.04, 9.33 ± 0.05, and 9.27 ± 0.04, respectively. No significant differences among PAB, PA, and P were found for each time point. During 13 h exposure, the media pH at UVA or UVA + UVB did not reach 9.20 and was largely lower than that with PAR. The media pH at UVA + UVB was lower than that at UVA at 11 and 13 h exposure but did not have differences at other time points.
Figure 3. Changes of pH in a closed system driven by photosynthesis of S. costatum exposed to different light treatments. The initial pH was 8.20. The low (A) and high (B) density levels are 51.84 and 172.80 W m−2 for PAR, 12.96 and 43.20 W m−2 for UVA, and 13.53 and 45.09 W m−2 for UVR (UVA + UVB), respectively. The error bars indicate the SDs (n = 3). The dash line represents the pH compensation point above which indicates active HCO3− uptake.
At high light intensity (Figure 3B), media pH under different light treatments also increased with time. After 9 h exposure, only the media pH under PAR exceeded 9.20, being 9.22 ± 0.05, After 13 h exposure, the media pH under PAR and PA exceeded 9.20, being 9.31 ± 0.05 and 9.31 ± 0.03, respectively, while the media pH under PAB was still below 9.20, being 9.15 ± 0.02. The media pH under PAB was significantly lower than PAR since 5 h exposure. The media pH at UVR or UVA did not reach 9.20, being 8.40 ± 0.01 and 8.74 ± 0.09, respectively, after 13 h exposure. The media pH at UVR had been lower than that at UVA since 5 h exposure.
Although media pH at UVA or UVA + UVB did not reach 9.20 during 13 h exposure, they maintained a rising trend, indicating that the media pH may increase further if culture period is extended. Therefore, another pH drift experiment was conducted after setting the initial media pH 9.00 to verify whether S. costatum exposed to UVR only has the capacity of active uptake of HCO3− (Figure 4). Exposure time interacted with light intensity and spectrum to affect media pH over 11.4 h of incubation (Supplementary Table S2). Media pH exposed to HL-UVA increased with exposure time and reached 9.21 ± 0.03 and 9.23 ± 0.04, respectively, after 8.4 and 10.4 h culture. Media pH exposed to LL-UVA also rose with exposure time and reached 9.23 ± 0.04 after 10.4 h culture. On the other hand, media pH exposed to UVR did not show significant increase during 11.4 h of incubation.
Figure 4. Changes of pH in a closed system driven by photosynthesis of S. costatum when exposed to different UVR treatments. The initial pH was 9.00. The low (LL) and high (HL) light densities are 12.96 and 43.20 W m−2 for UVA, and 13.53 and 45.09 W m−2 for UVR (UVA + UVB), respectively. The error bars indicate the SDs (n = 3). The dash line represents the pH compensation point above which indicates active HCO3− uptake.
Carbon dioxide did not affect carbon fixation but both radiation spectrum and intensity affected it; each two factors had an interactive effect (Supplementary Table S3). At ambient CO2 (Figure 5A), presence of UVA (PAR + UVA) or UVR (PAR + UVA + UVB) did not affect carbon fixation at lower radiation levels (PAR ≤ 93.31 W m−2, 429 μmol photons m2 s−1) compared to PAR alone, though addition of UVA showed slightly higher values than that with UVR at PAR of 30.24 W m−2 (139 μmol photons m2 s−1). At higher radiation level [PAR = 172.80 W m−2 (795 μmol photons m2 s−1), UVA = 43.2 W m−2, and UVB = 1.89 W m−2], presence of UVA or UVR reduced carbon fixation by 20.35 and 28.66%, respectively. At lowered CO2 level (Figure 5B), the carbon fixation rate was higher with UVA compared to that under PAR alone at lower PAR levels (15.55 and 30.24 W m−2, corresponding to 72 and 139 μmol photons m2 s−1). However, UVA did not bring about such enhancement under higher PAR levels (PAR ≥ 51.84 W m−2, 238 μmol photons m2 s−1). Presence of UVR did not affect carbon fixation at lower radiation levels (PAR ≤ 93.31 W m−2, 429 μmol photons m2 s−1) but significantly reduced it at the highest radiation level (PAR = 172.80 W m−2, 795 μmol photons m2 s−1) by 46.18%.
Figure 5. Photosynthetic carbon fixation rates of S. costatum grown at ambient (A) and lowered CO2 (B) levels when exposed to different radiation treatments. PAR, photosynthetically active radiation; PA, PAR + UVA, PAB, PAR + UVA + UVB. The error bars indicate the SDs (n = 3).
Changed CO2 levels did not affect UVR-driving carbon fixation; UVR spectrum and intensity affected it and they had an interactive effect (Supplementary Table S3). At ambient CO2 level (Figure 6A), carbon fixation of the cells grown under UVA or UVR alone increased linearly with radiation level (R2 = 0.957, p = 0.002 for UVA; R2 = 0.901, p = 0.009 for UVR), with the rate being higher under UVA than UVR at each radiation level, reflecting an inhibitory impacts of UVB. The gap between UVA and UVR became larger with increasing radiation levels. At the lowered CO2 level (Figure 6B), carbon fixation of cells grown under both UVA and UVR increased as well with increasing radiation levels (R2 = 0.985, p < 0.001 for UVA; R2 = 0.995, p < 0.001 for UVA + UVB), but the difference between UVA and UVR was not significantly different at any radiation level. For UVA, there was no significant difference between two CO2 levels at any radiation level. For UVR, ambient CO2 reduced carbon fixation although the decrease at 13.527 or 24.35 W m−2 was not statistically significant.
Figure 6. Carbon fixation rates of S. costatum grown at ambient (A) and lowered CO2 (B) levels when exposed to UVA or UVR (UVA + UVB). The error bars indicate the SDs (n = 3).
Each factor (CO2, radiation spectrum, and intensity) affected PAR-driving F'v/F'm, each two had an interactive effect and these three also interacted (Supplementary Table S4). At ambient CO2 level (Figure 7A), F'v/F'm decreased with radiation level. When PAR level was above 30.24 W m−2 (139 μmol m2 s−1), PA reduced F'v/F'm and PAB led to a larger decrease compared to PAR. At lowered CO2 level (Figure 7B), F'v/F'm also decreased with radiation level, but there were no differences among three radiation treatments (PAR, PA, and PAB). For each radiation treatment, cells had higher F'v/F'm at lower CO2 compared to ambient CO2 except for the highest PAB level.
Figure 7. Effective photochemical efficiency (F'v/F'm) of S. costatum cultured at ambient (A) and lower CO2 (B) levels exposed to different radiation treatments. PAR, photosynthetically active radiation; PA, PAR + UVA, PAB, PAR + UVA + UVB. The error bars indicate the SDs (n = 3).
Similar to PAR-driving F'v/F'm, each factor (CO2, radiation spectrum, and intensity) affected UVR-driving F'v/F'm, each two had an interactive effect and these three also interacted (Supplementary Table S4). When cells were exposed to UVA (Figure 8A), F'v/F'm did not change until UVA passed 12.96 W m−2 for both ambient and lowered CO2 conditions. Compared to the lowest intensity, the highest UVA intensity resulted in a decrease of 6.75% at lowered CO2 level while it was 20.97% for ambient CO2 level. When cells were exposed to UVR (Figure 8B), F'v/F'm did not change until UVR passed 13.53 W m−2 for lower CO2 level but it began to decrease when the light intensity was above 7.89 W m−2 for ambient CO2 level. Compared to the lowest light intensity, the highest UVR intensity resulted in a decrease of 6.31% at lower CO2 level while it was 30.49% for ambient CO2 level. F'v/F'm at lower CO2 was higher than that at ambient CO2 for each light intensity. For both ambient and lower CO2, cells had lower F'v/F'm under UVR compared to those under UVA at each radiation level.
Figure 8. Effective photochemical efficiency (F'v/F'm) of S. costatum cultured at ambient and lowered CO2 when exposed to UVA (A) or UVR (UVA + UVB; B). The error bars indicate the SDs (n = 3).
In the present work, we found that the diatom S. costatum up-regulated its CCMs due to synergistic effects of solar UVR and reduced CO2 availability, and showed that even UVR alone (without the presence of PAR) could stimulate the activity of CAe, induce active HCO3− uptake and thus promote photosynthetic carbon fixation. These results showed the first evidence that UVR alone can stimulate CCMs-mediated carbon acquisition.
UVR Enhancing CCMs Activity at Reduced CO2 Level
Carbonic anhydrase, which catalyzes the interconversion between CO2 and water and the dissociated ions of carbonic acid, is deemed as an important component of algal CCMs (Giordano et al., 2005; Beardall and Raven, 2020). Therefore, changes in CA activity have been considered as a signal of regulation of CCMs. Lowered CO2 availability usually induces CA activity to different extents under different levels of nutrients (Gao et al., 2018a,b). While it is known that decreased CO2 concentration and increased levels of light can trigger higher CA activity in S. costatum (Chen and Gao, 2003; Giordano et al., 2005), only limited knowledge has been documented on effects of UVR on it (Wu and Gao, 2009). In this work, the addition of UVA to PAR enhanced CAe activity, while UVB appeared to be inhibitive when combined with UVA. On the other hand, the CAe activity of cells grown at higher CO2 was not induced by UVA or UVR (Figure 1). This might be caused the downregulation of CCMs by the higher CO2 level, consequently dampening the UV-mediated effects on CCMs activity. Furthermore, we provided the first evidence that UVR alone drove CAe activity (Figure 2). This may be related to the change of the redox activity in the plasma membrane induced by UVA (Wu and Gao, 2009) and additionally the energy of UVA may also be utilized for the synthesis of CA through photosynthetic electron transport.
Active uptake of HCO3− is another pathway of algal CCMs (Giordano et al., 2005). A pH compensation point over 9.2 has been deemed as a sign of active HCO3− uptake for algae because there is hardly any CO2 available in water with a pH above 9.2 (Axelsson and Uusitalo, 1988; Gao et al., 2018a). In the present study, the addition of UVA to PAR promoted active uptake and utilization of HCO3−, so that pH increased to higher extent (Figure 3A). On the other hand, active uptake of HCO3− did not occur when PAR + UVR increased to a higher level. Sobrino et al. (2005) speculated that UVR may damage one or more of the processes involved with HCO3− transport in Nannochloropsis gaditana. Our pH drift tests showed that damage of UVR on algal HCO3− transport was due to UVB rather than UVA, since the cells exposed to PAR + UVA maintained a high pH compensation point over 9.2 while addition of UVB led to lower value (Figure 3B), reducing the pH compensation point to the value below 9.2. In addition, UVA alone drove HCO3− transport and utilization in S. costatum while UVR did not make it (Figure 4), indicating the damaging effect of UVB again. To the best of our knowledge, this is the first report on the UVR-driving active uptake of HCO3− in algae. As shown in this study, UVR can drive electron transport in PSII and the generated ATP may be utilized for active uptake of HCO3−. This can help to explain why UVA alone can drive photosynthetic carbon fixation at low CO2 levels.
UVR Driving Carbon Fixation Under Changing CO2 Levels
In this study, exposures to moderate levels of UVA or UVR in the presence of PAR did not affect carbon fixation of S. costatum, and high levels of UVR (UVA of 43.2 W m−2 or UVR of 45.1 W m−2) significantly reduced its carbon fixation under ambient CO2 level (Figure 5A). On the other hand, when CO2 level decreased to 2.8 μmol L−1, the addition of UVA to PAR increased carbon fixation of S. costatum grown at lower irradiance levels and did not reduce it even at the highest irradiance level (Figure 5B). The stimulating effect of UVA on carbon fixation was also found in phytoplankton assemblages in coastal waters of the South China Sea (Gao et al., 2007; Li et al., 2011). Such stimulation is most likely due to compounded effects of the UV-mediated CCMs activity and photosynthetic capture of UVA as a supply of energy. Since the CCMs activity was only induced with reduced availability of CO2 in S. costatum (Chen and Gao, 2003), our data indicate that UVR, especially, UVA only functions positively during the period when CCMs regulation is modulated, and there is a threshold beyond which UVR turns to damage CCMs-related proteins and inhibit carbon fixation.
UVA or UVR alone drove carbon fixation of S. costatum with lesser extent in the presence of UVB, indicating its inhibitory effect (Figure 6), which is the first time evidenced in this diatom. While diatom-dominated phytoplankton assemblages in the coastal waters were shown to be capable of photosynthesizing, and presence of UVB exhibited inhibitory effects (Gao et al., 2007), our results support this by providing species-level evidence. In the present work, presence of UVB reduced carbon fixation at ambient CO2 level but did not significantly affect it at lower CO2 level, suggesting that low to moderate levels of UVB may be utilized under lower CO2 level. Such a utilization of UVB has also been reported in a freshwater cyanobacterium Nostoc sphaeroides, in which photosynthesis and biomass production were even enhanced by low-dose UVB via enhancing the primary quinone-type acceptor (QA) re-oxidation, plastoquinone (PQ) pool re-oxidation, photosystem I (PSI) content, and cyclic electron transfer around PSI (Chen et al., 2020). Subsequently, both UVA and UVB may play roles in signaling for additional processes in addition to photosynthetic carbon fixation and CCMs.
UVR Driving Light Reaction Under Changing CO2 Levels
The addition of UVA or UVR to PAR significantly reduced the effective photochemical efficiency (F'v/F'm) of S. costatum grown at ambient CO2 (Figure 7A). Similar results were also found in the diatoms Cylindrotheca closterium f. minutissima (Wu et al., 2012) and Thalassiosira weissflogii (Gao et al., 2018c). It has been documented that UVR could inhibit PSII activity by impairing photosynthetic apparatus, such as PSII subunits PsbA (D1), and PsbD (D2) proteins (Six et al., 2007; Gao et al., 2018c). In contrast, the addition of UVA or UVR to PAR did not affect F'v/F'm under lowered CO2 condition even at the highest irradiance levels (Figure 7B). The energy of UV should be consumed during low CO2-induced upregulation of CCMs and hence the PSII was protected. Compared to lower CO2 (13.3 μmol L−1), higher CO2 (33.7 μmol L−1) exacerbated the stress of UVR on photosystem II function in the diatom T. weissflogii through reducing PsbD removal rate and the ratio of RbcL to PsbA during UVR exposure (Gao et al., 2018c). In the present study, compared to the cells grown at 2.8 μmol L−1 CO2, those grown at 10 μmol L−1 CO2 were more vulnerable to UVR in terms of photochemical performance, combined with the study by Gao et al. (2018c) study, indicating that the sensitivity of diatom to UVR may increase with the increase of CO2 level; therefore, inducing higher NPQ was in induced as reported in another work (Li et al., 2012). Under reduced CO2 availability, light energy could be transported and converted quickly and thus UVR did not reduce activity of PSII, which could be due to the upregulation of CCMs (Gao et al., 2012). Under lower CO2 conditions, intracellular CO2 is not enough to saturate carbon fixation. CCMs are usually activated or upregulated to increase intracellular DIC pools but the operation of CCMs is energy-consuming (Mishra et al., 2018). Since UVR can be used to stimulate CCMs in S. constatum, it could be quickly drained to fuel the energy demand associated with CCMs, avoiding the harm to PSII. Furthermore, UVA or UVR alone could drive electron transport in PSII (Figure 8). This indicates that the carbon fixation driven by UVA or UVR was through the electron transport and operation of PSII that supplies ATP and NADPH, following the same pathway as PAR.
The findings in the present study verifies the hypothesis proposed in the introduction that S. costatum could utilize UVR particularly UVA to drive carbon fixation at the lower CO2 condition by stimulating CCMs. The only deviated result is that presence of UVB, when combined with UVA, did not stimulate the activity of CCMs, carbon fixation, or photochemical quantum yield. Therefore, it is shorter wavebands of UVB that may have played an inhibitory role. The photons of UVA can be absorbed and transported through PSII and transformed into chemical energy ATP, which can be used to upregulate CCMs via enhancing CA activity and HCO3− utilization. Such UV-utilizing capability is particularly important for S. costatum to maintain survival and growth when PAR is low. With increased biomass density during the diatom blooms, both CO2, light, and UV levels are usually reduced due to self-shading. Therefore, harmful impacts of high levels of UVR can hardly be expected; instead, the low levels of UVR can promote CCMs and thus carbon fixation, so that successful and frequent occurrence of diatom blooms becomes possible. More studies in future should be conducted to investigate whether other diatoms or algae could also utilize UVR to upregulate CCMs when CO2 and PAR are in low levels.
Data Availability Statement
The raw data supporting the conclusions of this article will be made available by the authors, without undue reservation.
GG: conceptualization, investigation, methodology, formal analysis, visualization, writing – original draft preparation, writing – reviewing and editing, and funding acquisition. WL: writing – reviewing and editing, investigation, and methodology. XZ: methodology, investigation, and writing – reviewing and editing. KG: conceptualization, methodology, writing – original draft preparation, writing – reviewing and editing, supervision, and funding acquisition. All authors contributed to the article and approved the submitted version.
This work was supported by the National Natural Science Foundation of China (41890803 and 42076154), the Fundamental Research Funds for the Central Universities (20720200111), and the MEL Internal Research Program (MELRI2004).
Conflict of Interest
The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
The handling editor declared a past co-authorship with one of the authors [KG].
We thank Lin Gao and Shuyu Xie for their assistance with the pH drift experiment.
The Supplementary Material for this article can be found online at: https://www.frontiersin.org/articles/10.3389/fmicb.2021.651567/full#supplementary-material
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Keywords: bicarbonate uptake, carbonic anhydrase, microalgae, photochemical efficiency, photosynthesis, Skeletonema costatum
Citation: Gao G, Liu W, Zhao X and Gao K (2021) Ultraviolet Radiation Stimulates Activity of CO2 Concentrating Mechanisms in a Bloom-Forming Diatom Under Reduced CO2 Availability. Front. Microbiol. 12:651567. doi: 10.3389/fmicb.2021.651567
Edited by:Feixue Fu, University of Southern California, Los Angeles, United States
Reviewed by:Gang Li, Chinese Academy of Sciences, China
Kathleen Scott, University of South Florida, United States
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*Correspondence: Kunshan Gao, firstname.lastname@example.org