Symbiotic associations of the deepest recorded photosynthetic scleractinian coral (172 m depth)

The symbiosis between scleractinian corals and photosynthetic algae from the family Symbiodiniaceae underpins the health and productivity of tropical coral reef ecosystems. While this photosymbiotic association has been extensively studied in shallow waters (<30 m depth), we do not know how deeper corals, inhabiting large and vastly underexplored mesophotic coral ecosystems, modulate their symbiotic associations to grow in environments that receive less than 1% of surface irradiance. Here we report on the deepest photosymbiotic scleractinian corals collected to date (172 m depth), and use amplicon sequencing to identify the associated symbiotic communities. The corals, identified as Leptoseris hawaiiensis, were confirmed to host Symbiodiniaceae, predominantly of the genus Cladocopium, a single species of endolithic algae from the genus Ostreobium, and diverse communities of prokaryotes. Our results expand the reported depth range of photosynthetic scleractinian corals (0–172 m depth), and provide new insights on their symbiotic associations at the lower depth extremes of tropical coral reefs.Subject terms: Symbiosis, Microbial ecology

The ecological success of scleractinian corals, the engineers of one of the most productive and diverse ecosystems on Earth, relies on a myriad of symbiotic associations with microorganisms [1]. Among these symbioses, the association between the coral host and unicellular algae from the family Symbiodiniaceae is central to coral health and powers the metabolically expensive process of calcification [2]. The coral host provides limited inorganic nutrients, while Symbiodiniaceae share essential organic compounds derived from their photosynthetic activity [3]. This light-dependent association has mainly been studied in shallow waters (<30 m) because of technical limitations imposed by traditional scientific scuba diving. However, photosynthetic scleractinian corals have been observed in the mesophotic reef slope down to 150–165 m depth [4, 5].As depth increases, the waveband of solar radiation used by most algae for photosynthesis (from 400–700 nm) becomes attenuated in both intensity and width. Even in clear tropical waters, the irradiance levels below 120 m depth can be less than 1% of surface values, and the light spectrum is shifted toward the blue and blue–green wavelengths (~475 nm) (e.g. [4]). These light limitations pose a major constraint for the productivity of benthic organisms that rely on photosynthetic symbionts [6], including reef-building corals (scleractinians). While the scleractinian coral species Leptoseris hawaiiensis has been reported to occur as deep as 153 m in Hawaii and 165 m at Johnston atoll (reviewed in [4]), no live specimens were collected at these extreme depths. The fact that Symbiodiniaceae have been found at much greater depth in association with Antipatharians (396 m) [7], raises the possibility that they might also be present in scleractinian corals deeper than 165 m. Previous studies have genetically confirmed and identified endosymbiotic Symbiodiniaceae in Leptoseris down to 70 m on the Great Barrier Reef [8] and down to 125 m depth in Hawaii [9–11]. A specific host-Symbiodiniaceae association was reported between deep L. hawaiiensis and a Cladocopium from the ancestral C1 radiation [9–11], which represents a diverse group of Symbiodiniaceae commonly found in association with scleractinians on shallow coral reefs [8, 9, 12, 13]. To better understand how scleractinian corals can survive so far away from their presumed light optimum, it is critical to determine if these deep specimens (1) maintain their association with photosynthetic algae and/or (2) if their survival in the deepest mesophotic coral ecosystems requires a shift in their microbial communities, including Symbiodiniaceae and other microorganisms such as endolithic algae and bacteria.Here we report on the observation and collection of the deepest scleractinian corals in association with Symbiodiniaceae and other photosymbionts. Technical divers using closed-circuit rebreathers recovered three L. hawaiiensis colonies from the Gambier archipelago (French Polynesia, Fig. 1A) at 154, 168, and 172 m depth (n = 2 subsamples for each depth; Fig. 1B–D). Irradiance measured at 120 m depth was <2% of that recorded at 6 m depth and irradiance at 172 m was predicted to be <1% (Fig.​(Fig.1E1E and S1). ITS2 sequencing revealed Symbiodiniaceae presence in all three lower mesophotic colonies sampled, with nearly all of the retrieved amplicon sequence variants (ASVs; with most of these representing intragenomic sequence variants) classified as Cladocopium (Fig. 2). The most common ITS2 ASV representative sequence associated with these Leptoseris hosts (S-01, Fig. 2 and S2; 50–57% of total ASVs in each sample) was C1 (GeoSymbio and SymPortal databases; see supplementary methods). This represents one of the most common groups of Symbiodiniaceae, and it has previously been reported in Leptoseris [9, 10, 14], as well as other host species at depths ranging from the surface to 125 m [8, 10, 11, 13–15]. As a complementary approach, ITS2 profiles predicted by SymPortal were used as proxy for Symbiodiniaceae genotypes ([16]; see supplementary methods and data files S1–S4). These predicted ITS2 profiles were largely consistent among replicates but confirmed a different profile for the colony at 172 m depth compared to those at 154 and 168 m depth (Fig. S2). Nonetheless, the Symbiodiniaceae communities shared three ASVs that exactly matched C89 (S-02: 5% at 172 m vs. 17–19% at 154–168 m) and two different C variants (both S-05 and S-07: 7% at 172 m vs. ~2% at 154–168 m) in public databases (Fig. S3; GeoSymbio, SymPortal or Genbank). Of the 26 ASVs identified across all samples, one sequence originated from Durusdinium (S-24 D1 with GeoSymbio and SymPortal databases). This sequence is found in multiple heat-tolerant Durusdinium species including the enigmatic, cosmopolitan [17], host generalist D. trenchii [18]. However, whether or not the Symbiodiniaceae sampled here is D. trenchii or indeed thermally tolerant cannot be confirmed without further genetic and phenotypic data. Low abundance ASVs were observed at all three depths (172 m: 8 ASVs, 154 and 168 m: 10 ASVs, Fig. S3), including nine ASV sequences (Fig. 2) that have not been reported previously in the GeoSymbio [13] and SymPortal (access date: 2020-05-19_07-23-40) [16] databases (Fig. S3). Comparison of the overall Symbiodiniaceae SymPortal predicted ITS2 profiles (Fig. S2) did not confidently identify matches with previously encountered profiles (predominantly from shallow reef environments), indicating that they might be specific to this species and/or mesophotic environment. Given the extreme paucity of light at these depths, we hypothesize that lower mesophotic L. hawaiiensis may use different strategies to photoacclimate. Morphologically, the coral species were characterized by a thin flat skeleton (Fig. 1B–D), which is optimal for light harvesting and reducing skeletal carbonate deposition [19]. Leptoseris hawaiiensis has also been shown to display depth-associated physiological specialization and trophic plasticity (acquiring energy from different food sources) [9], and an unusual light-harvesting system, which enlarges the spectrum of wavelengths for photosynthesis by transforming the short, blue-shifted wavelength with their autofluorescent pigments [19].Open in a separate windowFig. 1Sampling location of the deepest photosymbiotic scleractinian coral recorded to date.A Map of the Gambier archipelago, French Polynesia. Pictures of Leptoseris hawaiiensis collected at 172 m depth in the Gambier archipelago (B) during the in situ sampling (screenshot of video © UTP III), (C) after reaching the surface and (D) after bleaching for taxonomic identification with the green color indicating the presence of endolithic algae. E Variation of the optical index of irradiance (in PAR) along the coral reef depth gradient from 6 to 120 m depth (predictions for 150 and 172 m depths) at Mangareva. For each depth, the three values represent a mean value for 3 days of measurements recorded every 5 min with a PAR logger (DEFI2-L Advantech) at three different time periods of the day (9 h30–10 h00, 12 h30–13 h00 and 15 h30–16 h00).Open in a separate windowFig. 2Microbial communities harbored by the three deep colonies.Composition of the microbial community in Leptoseris hawaiiensis collected at 172, 168, and 154 m. At each depth, two subsamples were analyzed for each colony. The ITS2 marker shows the relative proportion of different Symbiodiniaceae ASVs (with GeoSymbio and SymPortal v.2020-05-19_07-23-40 affiliations). The 16S rDNA marker shows the relative proportions of different ASVs for endolithic algae chloroplast composition and bacteria classes. Asterisk represents sequences with no exact match in the SymPortal database for Symbiodiniaceae.To identify other microorganisms associated with our lower mesophotic scleractinian colonies, we targeted the 16S rRNA gene (V4–V5 region; see supplementary methods). Sequencing data revealed the presence of green algal chloroplast sequences belonging to the genus Ostreobium (Fig. 2). This endolithic alga was abundant in the deep coral colonies as suggested by the marked green color observed below the living tissues (Fig. 1C) and within the skeleton after removing the soft tissues in bleach (Fig. 1D). We identified a single Ostreobium species (ASV ga-01), belonging to clade 2, that was dominant in all the colonies (Fig. 2 and S4), and has been previously reported across the depth gradient in scleractinian corals and octocorals worldwide [20, 21]. The nature of the interaction between corals and Ostreobium has been debated. Evidence supports a mutualistic association under extreme conditions such as coral stress (inducing bleaching) [22] or drastically reduced light exposure [23]. Under the low light conditions of the deep mesophotic fore reef slope, Ostreobium might complement Symbiodiniaceae’s function by providing photosynthates to the host. These endolithic algae are adapted to photosynthesize in near-darkness with increased numbers of light-harvesting xanthophyll pigments that can use shorter wavelengths compared to other green algae and optimize light capture (e.g. [24]).Bacteria associated with the lower mesophotic scleractinian colonies had an observed richness ranging from 106 to 211 ASVs per sample (Fig. S5). These bacteria mainly belonged to the classes Alpha- (19-49%) and Gamma-proteobacteria (8–17%), Bacteroidia (6–20%) and subgroup-6 of Acidobacteria (1–17%) (Fig. 2), which are known to associate with corals [25]. In total, we detected 843 different bacterial ASVs, among which 67–89% were unique to one colony or even unique to one subsample (Fig. S6 and Table S1). Our data suggest that the coral hosts displayed individual microbial signatures with some common ASVs shared between subsamples of the same colony (Fig. S6). However, this result might have been affected by the low-sequencing depth of the microbiome following the removal of the Ostreobium reads. Our results corroborate previous reports describing the high intra-specific variability of coral-associated bacterial communities at different spatial scales (e.g. [25, 26]), which might be driven by biological traits, such as the age [27] or diets of the colonies [28].This study reports a new depth record for scleractinian corals associated with symbiotic algae at 172 m. Similar to conspecifics previously sampled in mesophotic environments between 115 and 125 m depth [10], the deepest L. hawaiiensis reported here associated with symbiotic-microalgae belonging to the highly diverse C1 lineage. The deep colonies were also characterized by the presence and abundance of a single species of endolithic alga from the genus Ostreobium (clade 2). These filamentous green algae adapted to thrive in extreme low light conditions [24] might highly contribute to the survival of L. hawaiiensis at depth through photosynthates translocation [29]. In addition, bacterial communities were diverse, with intraspecific differences in community composition. Our findings provide new insights into the symbioses of scleractinian corals at depth, through the conservation of their associated photosymbiotic algae, raising important questions about the nature and mechanisms involved in the interactions between host and Symbiodiniaceae and/or Ostreobium (e.g. evolutionary theory of symbiosis [30]). Future studies should establish the contribution of photosynthetic symbionts to the energy budget of mesophotic corals. Understanding the biology of ecosystem engineers, such as tropical reef corals, living at the edge of their habitat range is important to determine the plasticity of these organisms and their ability to withstand environmental pressure.     

Identified taste bud cell proliferation in the perihatching chick [published erratum appears in Chem Senses 1998 Aug;23(4):459]

Developing taste buds in the anterior mandibular floor of perihatching chicks were studied by high voltage electron microscopic autoradiography in order to identify proliferating gemmal cell types. Montaged profiles of 29 taste buds in five cases euthanized between embryonic day 21 and posthatching day 2 were analyzed after a single [3H]thymidine injection administered on embryonic day 16, 17 or 18. Results showed that dark cells comprised 55% of identified (n = 900 cells) and 62% of labeled (n = 568 cells) gemmal cells as compared with light, intermediate, basal or perigemmal bud cells. Dark cells had both a greater (P < 0.05) number of labeled cells and a greater amount of label (grains/nucleus) than the other four bud cell types, irrespective of injection day. The nuclear area (micron 2) of dark cells was not significantly larger (P > 0.05) than that of the other gemmal cell types and therefore cannot account for the greater amount for label in the dark cells. Interestingly, only dark cells showed a positive correlation (P < 0.003) between amount of label and nuclear area. Results suggest that, during the perihatching period of robust cell proliferation, dividing dark cells may give rise primarily, but not exclusively, to dark cell progeny.      

X-ray diffraction and infrared circular dichroism of DNA-violamycin B1 complexes

X-ray diffraction and infrared linear dichroism of oriented samples of DNA-violamycin B1 complexes have been studied at different antibiotic/DNA phosphate ratios (r) as a function of relative humidity. Violamycin B1 binds to DNA according to the intercalation as well as to the outside binding model. At low r values, where the intercalation predominates the unwinding angle of DNA helix is between 6 degrees and 12 degrees per intercalation site as followed from the dependence of the pitch of helix versus r. At r greater than or equal to 0.17 the intercalation sites are saturated and the outside binding becomes prevalent; however the violamycin B1 chromophore is still oriented in the plane of DNA bases. Conformational mobility of DNA in the violamycin B1 complexes is largely inhibited compared with pure DNA, but it is higher than that of the daunomycin complexes. At least 30% of DNA in violamycin complexes has A conformation at the medium humidities as followed by IR linear dichroism. In the case of x-ray diffraction the A conformation was not detected. The distance between DNA molecules in the complex is found to be 23.2 A, that is 2 A less than in pure DNA at the same conditions and it does not depend upon r.     

Survival of adults and developmental stages ofSarcoptes scabiei var.canis when off the host

All life-stages ofSarcoptes scabiei var.canis survive in the hosts' environment for several days to several weeks depending on r.h. and temperature. Survival of larvae was comparable to males; survival of nymphs was comparable to females. Females and nymphs generally survived longer than larvae and males.Low temperature (10–15°) and high r.h. prolonged survival of all life stages. At 10–15°C, females and nymphs survived 1–3 weeks at 97% r.h., 1–2 weeks at 75% r.h. and 5–8 days at 45% r.h. At 20–25°C, survival was significantly reduced but all life-stages survived at least 2 days at 25% r.h. and 5–6 days at 75–100% r.h. Long survival off the host coupled with host-seeking behavior of these mites make it likely that environmental contamination is a source of scabies in domestic and wild mammals, and in humans.