| Literature DB >> 29624607 |
Elvira Mächler1,2, Maslin Osathanunkul1,3,4, Florian Altermatt1,2.
Abstract
The use of environmental DNA (eDNA) as a species detection tool is attracting attention from both scientific and applied fields, especially for detecting invasive or rare species. In order to use eDNA as an efficient and reliable tool, however, we need to understand its origin and state as well as factors affecting its degradation. Various biotic and abiotic environmental factors have been proposed to affect degradation of eDNA in aquatic environments and thus to influence detection rates of species. Here, we were interested in two of them, namely UV light, which can break down DNA, and the presence of filter feeders, which can remove DNA and DNA-bound particles. A few, mostly laboratory-based studies have found minor effects of UVB on the degradation of eDNA. Ultraviolet A radiation (UVA), however, has been neglected although it also causes DNA lesions and is 10- to 100-fold more prevalent than UVB when reaching the earth's surface. Filter feeders are common in aquatic ecosystem, but their effects on eDNA has hitherto been ignored. We conducted a full-factorial aquatic mesocosm experiment under near-natural outdoor conditions manipulating UV radiation as well as the presence of Dreissena polymorpha, a strong filter feeder capable of filtering cells or organelles containing DNA. Surprisingly, we found that neither UV radiation nor the presence of the filter feeder affected eDNA-based detection rates of macroinvertebrates, even though the experiment took place in summer when UV radiation intensity and filtration activity is high for the chosen experimental site and conditions. These results, in combination with studies from marine or laboratory settings finding no effect of sunlight and its UV components on the detectability of eDNA, suggest that eDNA based species assessments could be relatively robust with respect to our two factors studied.Entities:
Mesh:
Substances:
Year: 2018 PMID: 29624607 PMCID: PMC5889167 DOI: 10.1371/journal.pone.0195529
Source DB: PubMed Journal: PLoS One ISSN: 1932-6203 Impact factor: 3.240
Used primer pairs to detect species-specific eDNA.
| Aaq-L3 | 147 | Herein | ||
| Aaq-R3 | Herein | |||
| Gpu-L9 | 179 | Herein | ||
| Gpu-R11 | Herein | |||
| NZMSF | 89 | Goldberg | ||
| NZMSR | Goldberg |
a Amplicon size is including the primer pair length
List of species that were used to test the specificity of primers.
| No | no | ||
| No | yes | ||
| No | no | ||
| No | no | ||
| No | no | ||
| No | no | ||
| Yes | no | ||
| No | yes | ||
| No | no | ||
| Yes | no |
Fig 1Overview of the three different UV treatments and the specific cover material used.
In the control treatment, visible light (VIS) and all wavelengths of UV radiation can penetrate the cover. In the ‘No UVB’ treatment only VIS and UVA radiation can penetrate the cover, while UVB radiation will be reflected. Similar in the ‘No UVA and no UVB’ treatment: UVA and UVB radiation will be reflected and only VIS can reach the water in the mesocosms.
Fig 2Mean proportion of successful eDNA detection per UV treatment based on positive amplifications across five PCR replicates per mesocosm.
Error bars represent standard errors across all ten mesocosm replicates of the corresponding UV treatment. We did not process eDNA samples for day five for A. aquaticus and P. antipodarum due to logistic reasons.
GLMM results on the fixed effects of the UV and filter feeder treatments on the detection of each species.
| Intercept (UV: Control) | -0.7779 | 0.8429 | -0.92 | 0.36 |
| UV: No UVB | 0.3861 | 0.9113 | 0.42 | 0.67 |
| UV: No UVA and no UVB | -0.0991 | 0.9252 | -0.11 | 0.92 |
| Filter feeder: Present | 0.6748 | 0.7591 | 0.89 | 0.37 |
| Intercept (UV: Control) | -0.9799 | 0.7287 | -1.35 | 0.18 |
| UV: No UVB | -0.2661 | 0.6355 | -0.42 | 0.68 |
| UV: No UVA and no UVB | 0.5955 | 0.6065 | 0.98 | 0.33 |
| Filter feeder: Present | -0.0669 | 0.5154 | -0.13 | 0.90 |
| Intercept (UV: Control) | 0.2271 | 0.8808 | 0.26 | 0.80 |
| UV: No UVB | -0.3026 | 0.7214 | -0.42 | 0.68 |
| UV: No UVA and No UVB | -0.4077 | 0.7432 | -0.55 | 0.58 |
| Filter feeder: Present | -0.4594 | 0.5868 | -0.78 | 0.43 |
GLMM results of the random effects (mesocosm identity and day of experiment) on the detection of each species.
| Intercept (mesocosm) | 84.98 | 9.218 |
| Day | 32.79 | 5.726 |
| Intercept (mesocosm) | 25.314 | 5.031 |
| Day | 4.484 | 2.118 |
| Intercept (mesocosm) | 30.745 | 5.545 |
| Day | 9.905 | 3.147 |
Fig 3Mean proportion of successful eDNA detection per filter feeder treatment based on positive amplifications across five PCR replicates per mesocosm.
Error bars represent standard errors across all 15 mesocosm replicates of the corresponding filter feeder treatment. We did not process eDNA samples for day five for A. aquaticus and P. antipodarum due to logistic reasons.