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Genetic connectivity between land and sea: the case of the beachflea Orchestia montagui (Crustacea, Amphipoda, Talitridae) in the Mediterranean Sea
https://doi.org/10.1186/1742-9994-10-21
© Pavesi et al.; licensee BioMed Central Ltd. 2013
- Received: 21 November 2012
- Accepted: 3 April 2013
- Published: 25 April 2013
Abstract
Introduction
We examined patterns of genetic divergence in 26 Mediterranean populations of the semi-terrestrial beachflea Orchestia montagui using mitochondrial (cytochrome oxidase subunit I), microsatellite (eight loci) and allozymic data. The species typically forms large populations within heaps of dead seagrass leaves stranded on beaches at the waterfront. We adopted a hierarchical geographic sampling to unravel population structure in a species living at the sea-land transition and, hence, likely subjected to dramatically contrasting forces.
Results
Mitochondrial DNA showed historical phylogeographic breaks among Adriatic, Ionian and the remaining basins (Tyrrhenian, Western and Eastern Mediterranean Sea) likely caused by the geological and climatic changes of the Pleistocene. Microsatellites (and to a lesser extent allozymes) detected a further subdivision between and within the Western Mediterranean and the Tyrrhenian Sea due to present-day processes. A pattern of isolation by distance was not detected in any of the analyzed data set.
Conclusions
We conclude that the population structure of O. montagui is the result of the interplay of two contrasting forces that act on the species population genetic structure. On one hand, the species semi-terrestrial life style would tend to determine the onset of local differences. On the other hand, these differences are partially counter-balanced by passive movements of migrants via rafting on heaps of dead seagrass leaves across sites by sea surface currents. Approximate Bayesian Computations support dispersal at sea as prevalent over terrestrial regionalism.
Keywords
- Orchestia montagui
- Talitrids
- Mediterranean Sea
- Phylogeography
- Mitochondrial DNA
- Microsatellites
- Allozymes
- Approximate Bayesian Computation
Introduction
In many marine species genetic structure is often shallow as a consequence of large population sizes coupled with high potential for long distance dispersal. A high number of polymorphic markers, large sample sizes and ad-hoc designed sampling schemes are hence necessary to unveil population structure [1]. On the other hand, phylogeographic patterns with a clear geographic component are relatively common and easy to detect in terrestrial and/or freshwater species due to the intimately fragmented nature of their habitats [2]. Phylogeographic patterns in species living in the transition area between sea and land (supralittoral zone) have received relatively little attention compared to the wealth of work done on marine and terrestrial species [3–6]. However, a proper understanding of the evolutionary trajectories governing coastal communities is fundamental, especially in light of the increasing pressure that human beings have been exerting on them in the last decades [7].
Talitrid amphipods are often the dominant animal group in the supralittoral zone, where they are confined to a narrow area avoiding both the arid environment inland and submersion in seawater. Active dispersal is restricted to short, mostly nocturnal, foraging movements along the beach [8, 9]; maximal active distance recorded for talitrids in nature is 200 m [10]. Talitrids lack any planktonic larval stage and consequently they cannot rely on this stage for long-distance passive dispersal. They are, however, considered as facultative rafters [11, 12]. Generally speaking, rafting involves the traveling of organisms over the sea surface via floating material. Talitrids are often associated to wrack, wood or other floating material that could be washed away by waves and transported by sea surface waters from one beach to another. Rafters can be transported from short to medium-long distances and arrive in otherwise unreachable areas [12]. This process has a special impact on those species that are not able to actively disperse over long distances. In particular, it could potentially increase connectivity among populations, thus reducing the onset of local genetic divergence. Peracarid crustaceans are found in both high diversity and abundance on floating items, which seemingly play an important role in their life histories [12].
The semi-enclosed Mediterranean Sea is surrounded by thousands of kilometers of coasts. Previous genetic studies focused on multiple Mediterranean populations of seven different species of talitrids [8, 13–18] have revealed two main patterns of genetic structuring, corresponding to two groups of species with contrasting life histories. Those species (i.e. Orchestia montagui, O. mediterranea, Platorchestia platensis) that live within beached decaying seagrass, wrack or gravel, showed a shallow genetic structuring even on a wide geographical scale. Species (i.e. Talitrus saltator, O. stephenseni, Macarorchestia remyi) that are exclusively associated to sandy beaches or stranded rotting logs and have the tendency to burrow into the substrate were invariably highly structured genetically [17, 18]. De Matthaeis et al. [8, 15] interpreted these alternate patterns in terms of probabilities for talitrids to realize passive dispersal via rafting by being dragged away by waves. These probabilities would be high for the species belonging to the first ecological group because they colonize ephemeral habitats close to the waterline. On the other hand, they would be low for species of the second group bound to sand beaches or rotting logs; these species colonize the upper supralittoral zone and are not well suited to survive on rafts [19].
List of populations, genetic indices and different localities/samplings included in the study
Pop | Sampling location | Code | Basins | N (COI\msat\alz) | Hapl | H | Π | π n | HE | HO | AR | PA |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | Cala Lunga (Bonifacio, Corsica, France) | CCL | Tyrrhenian Sea | 9\9\- | 6 | 0.917 | 2.833 | 0.005 | 0.319 | 0.525 | 3.399 | |
2 | Sutta-Rocca (Bonifacio, Corsica, France) | CSR | Tyrrhenian Sea | 2\-\- | 2 | - | 2.000 | 0.003 | ||||
3 | Cala Reale (Asinara island, Sardinia, Italy) | SAR | West. Med. Sea | 14\29\27 | 4 | 0.67 | 0.813 | 0.001 | 0.306 | 0.555 | 3.539 | |
4 | Porto Pagliaccia (Asinara island, Sardinia, Italy) | SAP | West. Med. Sea | 15\30\17 | 5 | 0.562 | 4.742 | 0.008 | 0.322 | 0.614 | 3.931 | |
5 | Cala Barbarossa (Asinara island, Sardinia, Italy) | SAB | West. Med. Sea | 14\30\12 | 5 | 0.758 | 0.989 | 0.002 | 0.337 | 0.600 | 3.521 | |
6 | Molo Fornelli (Asinara island, Sardinia, Italy) | SAF | West. Med. Sea | 11\16\- | 8 | 0.927 | 8.09 | 0.014 | 0.313 | 0.522 | 3.517 | |
7 | Saline (Stintino, Sardinia, Italy) | SSS | West. Med. Sea | 15\30\- | 6 | 0.79 | 1.295 | 0.002 | 0.524 | 0.657 | 4.244 | |
8 | La Caletta (San Pietro island, Sardinia, Italy) | SPC | West. Med. Sea | 10\23\18 | 6 | 0.911 | 7.088 | 0.012 | 0.356 | 0.576 | 3.747 | |
9 | Cala Sapone (Sant’Antioco island, Sardinia, Italy) | SNS | West. Med. Sea | 15\30\- | 5 | 0.628 | 4.19 | 0.007 | 0.547 | 0.734 | 4.458 | 0.017(2) |
10 | Cala Lunga (Sant’Antioco island, Sardinia, Italy) | SNL | West. Med. Sea | 1\-\14 | 1 | - | 0 | 0 | ||||
11 | Spiaggia Grande (Sant’Antioco island, Sardinia, Italy) | SNG | West. Med. Sea | 15\29\- | 3 | 0.362 | 0.381 | 0.001 | 0.635 | 0.667 | 4.017 | 0.017(1) |
12 | Calasetta A (Sant’Antioco island, Sardinia, Italy) | SNA | West. Med. Sea | 15\30\12 | 7 | 0.828 | 3.79 | 0.001 | 0.372 | 0.565 | 3.565 | |
13 | Calasetta B (Sant’Antioco island, Sardinia, Italy) | SNB | West. Med. Sea | 3\-\- | 3 | - | 1.333 | 0.002 | ||||
14 | Cussorgia (Sant’Antioco island, Sardinia, Italy) | SNC | West. Med. Sea | 15\29\15 | 5 | 0.476 | 3.18 | 0.005 | 0.500 | 0.676 | 3.358 | 0.017(1) |
15 | Porticciolo (Cavoli island, Sardinia, Italy) | SCP | Tyrrhenian Sea | 7\7\25 | 2 | 0.476 | 0.952 | 0.002 | 0.357 | 0.552 | 3.250 | |
16 | Cala Ponente (Tavolara island, Sardinia, Italy) | STA | Tyrrhenian Sea | 15\29\2 | 11 | 0.905 | 3.828 | 0.007 | 0.328 | 0.578 | 3.743 | |
17 | Porto Massimo (Maddalena island, Sardinia, Italy) | SMM | Tyrrhenian Sea | 13\15\23 | 7 | 0.833 | 4.564 | 0.008 | 0.330 | 0.578 | 3.409 | 0.167(1) |
18 | Lo Spalmatore (Maddalena island, Sardinia, Italy) | SMS | Tyrrhenian Sea | 11\29\20 | 6 | 0.8 | 1.781 | 0.003 | 0.328 | 0.578 | 4.096 | |
19 | Baia Trinità (Maddalena island, Sardinia, Italy) | SMT | Tyrrhenian Sea | 15\30\21 | 5 | 0.771 | 1.657 | 0.003 | 0.449 | 0.607 | 4.037 | |
20 | Porto (Maddalena island, Sardinia, Italy) | SMP | Tyrrhenian Sea | -\-\19 | ||||||||
21 | Cala Portese (Caprera island, Sardinia, Italy) | SCA | Tyrrhenian Sea | -\-\18 | ||||||||
22 | Telamone (Grosseto, Tuscany, Italy) | TTA | Tyrrhenian Sea | 15\30\- | 12 | 0.971 | 6.314 | 0.011 | 0.326 | 0.537 | 3.763 | |
23 | S. Agostino (Civitavecchia, Latium, Italy) | LFM | Tyrrhenian Sea | 6\-\- | 5 | 0.933 | 5.133 | 0.009 | ||||
24 | La Frasca (Civitavecchia, Latium, Italy) | FRA | Tyrrhenian Sea | 14\30\105 | 9 | 0.835 | 8 | 0.014 | 0.371 | 0.504 | 3.676 | |
25 | Dahlet Qorrot (Gozo island, Maltese Archipelago) | GOZ | East. Med. Sea | 14\29\- | 6 | 0.604 | 1.714 | 0.003 | 0.408 | 0.681 | 3.719 | |
26 | Marina di Pulsano (Taranto, Apulia, Italy) | PMP | Ionian Sea | 15\30\- | 6 | 0.714 | 8.752 | 0.015 | 0.471 | 0.668 | 4.666 | 0.083(1) |
27 | Villaggio Nettuno (Lecce, Apulia, Italy) | PSF | Adriatic Sea | 15\30\- | 8 | 0.79 | 9.571 | 0.017 | 0.212 | 0.536 | 4.062 | |
28 | San Cataldo (Lecce, Apulia, Italy) | PSC | Adriatic Sea | 1\-\- | 1 | - | 0 | 0 | ||||
29 | Analipsi (Astipalea island, Greece) | GRE | Aegean Sea | -\-\15 |
Geographic distribution of sampling sites for the O. montagui populations included in the study. Details on each sampling site are given in Table 1. The names of the six sampled Mediterranean sub-basins are indicated along with the pattern of the main surface sea currents.
The aim of this study is thus to determine the genetic structure of the beachflea O. montagui in the central portion of the Mediterranean Sea. The species is tightly linked to stranded heaps of the seagrass P. oceanica and hence passive dispersal via rafting is a plausible hypothesis. Here we specifically ask whether such passive dispersal in O. montagui is a strong enough factor to promote genetic homogeneity over long distances. P. oceanica wrack may provide food and shelter; given the wide distribution of this seagrass in the Mediterranean Sea we suspect events of transports to be quite frequent. On the other hand, being strictly associated to a potential vector of dispersal does not necessarily imply that gene flow is realized. We indeed found a remarkably deep geographic partition in the population genetic structuring of the talitrid M. remyi, a species strictly associated to stranded rotting logs that should theoretically aid passive dispersal [18]. Here we used multiple genetic data sets (mtDNA, microsatellites and allozymes), which allowed testing the following two alternative scenarios (marine and terrestrial, respectively). Under the marine scenario if passive dispersal at sea were predominant, we would expect patterns of genetic structuring to be relatively shallow within basins and largely congruent with those of marine Mediterranean taxa with planktonic stages in the life cycle. Multiple authors recurrently placed a major breakpoint to gene flow in marine species at the Strait of Sicily (STS): this separates the Western from the Eastern Mediterranean basin (the so-called STS boundary; [24–27]). We also expect sea surface currents - the main carriers of floating wracks - to shape patterns of relationships among populations. Alternatively, if the bound to terrestrial environment prevailed over dispersal at sea, we would expect more pronounced genetic divergence also at the within-basin level with evidence of genetic regionalism. Support for both scenarios was evaluated with Approximate Bayesian Computation [28]. Finally, the study represents an opportunity to compare three marker systems characterized by different evolutionary properties regarding inheritance (maternal for mtDNA vs. bi-parental for microsatellites and allozymes) and pace of molecular evolution (from relatively slow for the protein-coding allozymic loci to very fast for the non-coding microsatellites).
Materials & methods
The study complies with the current laws of Italy and Germany regarding proper treatment of animals for research and was approved by the Ethical Committee of University of Rome "Sapienza", Italy.
Sampling
O. montagui specimens were collected by hand or using an aspirator on P. oceanica decaying leaves. A total of 26 populations were sampled for this study on rocky and sandy beaches along shores of the following Mediterranean basins: Tyrrhenian Sea (10 populations), Western Mediterranean basin (12 populations), Eastern Mediterranean basin (one population), Ionian Sea (one population), Adriatic Sea (two populations). All 26 populations were analyzed at the mtDNA level and 21 (out of 26) were genotyped for microsatellites.
Additionally, we re-analyzed the dataset based on 21 allozymic loci of De Matthaeis et al. [8]. That study included 16 populations and 363 individuals. One population was from the Aegean Sea (an area that we could not cover with our new sampling) while 13 have been re-sampled for the present study. The different data sets combined hence include 29 populations: information about populations, sampling localities and markers used is listed in Table 1; all populations analyzed with mtDNA and microsatellites were collected anew for the study while De Matthaeis et al. [8] was the only source of the allozymic data. Figure 1 shows the geographic location of sampling sites.
Genetic analyses
Including the 153 samples analyzed in Pavesi et al. [23], we extracted total genomic DNA from 544 individuals using the “Qiagen DNeasy Blood & Tissue Kit” (Hilden, Germany) according to the manufacturer’s protocol.
Mitochondrial DNA
Folmer et al.’s [29] universal primers were used to amplify via Polymerase Chain Reaction (PCR) a 571 base pair long fragment of the mtDNA coding for the COI gene in 1 to 15 individuals per population for a total of 295 individuals (details are given in Table 1). COI double-stranded amplifications, purification of PCR products and sequencing reactions were carried out as described in [18, 23, 30]. Editing and alignment of sequences were performed using Sequencher 4.1 (Gene Codes, Ann Arbor, MI, USA) and checked by eye. We used Paup* v.4.0b10 [31] to calculate the number of parsimony-informative characters. We used Arlequin v.3.11 [32] to calculate genetic diversity (H), nucleotide diversity (π n ) and the mean number of pairwise differences between all pairs of haplotypes (π). The same software was used to assess the population genetic structure by hierarchical analysis of molecular variance (AMOVA; [33]). Populations were combined according to their geographic origin and to the results of phylogeographic analyses (see Results). AMOVA was initially run on populations combined in three groups. These pooled all Tyrrhenian samples (populations 1–2 and 15–24 in Table 1), North Western Sardinian + Ionian and Adriatic samples (populations 3–7 and 26–28) and South Western Sardinian + Gozo Is. populations (8–14 and 25). An additional AMOVA was run on five groups of populations. These included Corsican + South Eastern Sardinian + Tyrrhenian peninsular sites (populations 1–2; 15 and 23–24), North Western Sardinian localities + Gozo Is. (populations 3–7 and 25), South Western Sardinian localities (populations 8–14), North Eastern Sardinian localities (populations 16–21) and Adriatic + Ionian samples (populations 26–28). We also calculated pairwise FST values on all pairs of populations as a measure of their differentiation. Statistical significance of these values was assessed by 1,000 permutations after sequential Bonferroni correction for multiple tests [34]. We also performed a Mantel Test [35] with Arlequin, to test for the presence of Isolation-by-distance (IBD) in the dataset; variables were pairwise FST values and corresponding geographic coordinates distances Degrees-Minutes-Seconds (DMS). Geographic distances were measured as the shortest marine distances between each pair of populations, according to the circulation of surface currents [36, 37]. We used the spatial analysis of molecular variance (SAMOVA v.1.0) to detect genetic barriers among groups of populations that were geographically homogeneous and maximally differentiated from each other [38]. Arlequin was also used to assess the fit of demographic [39] and geographic [40] expansion models to O. montagui genetic variation (populations grouped according to the SAMOVA results). Mismatch distributions were used to fit the models of sudden demographic and geographic expansion and to estimate the τ parameter. In both models τ is a mutation-scaled measure of time since expansion (demographic or geographic) and can be used to estimate time in generations (T) since expansion, using T = τ/2 μ, where μ is the crustacean COI mutation rate per site per year of Knowlton et al. [41] already adopted in Pavesi et al. [23]. Goodness of fit was assessed by the sum of square deviations (SSD) between the observed and the expected mismatch, and its significance was determined by a parametric bootstrap with 10,000 replicates. Demographic equilibrium was also tested on each SAMOVA group by Tajima’s D[42] and Fu’s Fs[43] statistics in Arlequin. These parameters have been shown to be sensitive to signals of population expansion; their statistical significance was tested by simulating random samples (10,000 replicates). P-values were obtained as the proportion of simulated values smaller than or equal to the observed values (α = 0.05).
In order to estimate genealogical relationships among all haplotypes, we used Tcs v.1.13 [44] to carry out a statistical parsimony analysis with a 95% connection limit [45]. To better visualize the haplotype network layout, we used HapStar [46] combined with Inkscape, a free open-source Svg graphics editor [47]. HapStar directly combines the network connection output data generated from Arlequin with a force-directed algorithm to automatically lay out the network for easy visualization.
Microsatellites
We genotyped all 544 individuals (7 to 30 per population) at eight microsatellite loci (msats, Table 1). PCR amplifications were performed as described in [22, 23]. Fragment sizes were determined on an ABI 3100 automatic sequencer using the GeneMapper v.3.5 software and an internal size standard (GS500LIZ from Applied Biosystems). We used Microchecker v.2.2.3 [48] to identify genotyping errors (null alleles) and the scoring of stutter peaks in all microsatellites. Null alleles can cause deviations from Hardy–Weinberg proportions. In order to test for the impact of null alleles on our data set, we calculated global FST values with FreeNA software. These values were computed, as described in Chapuis and Estoup [49], with 10,000 bootstrap iterations, alternatively using and not using the Excluding Null Alleles (ENA) method. We used Arlequin v.3.11 [32] to calculate expected (HE) and observed (HO) heterozygosity, deviations from Hardy–Weinberg equilibrium and tests of linkage disequilibrium among loci. We corrected P-values using the sequential Bonferroni correction for multiple comparisons [34]. We used Fstat v.2.9.3 [50, 51] to calculate allelic richness (AR) for each population, and GenAlex v.6.3 [52] to determine the number of alleles per locus, the number of private alleles (PA) and their relative frequencies in each population. With Arlequin v.3.11 we calculated pairwise FST values and performed two AMOVA analyses (on three and five groups, respectively) and Mantel test as described for the mtDNA dataset in the previous paragraph. For the AMOVA we grouped populations based on the results of Structure v.2.3.2 [53] (three and five groups; see below).
We run Structure to evaluate genetic subdivision and to assign individuals to the most probable number of clusters (K). The software uses a Monte Carlo Markov Chain (MCMC) Bayesian clustering model that assumes that different loci are at Hardy-Weinberg and linkage equilibrium with one another within populations. We performed 10 independent runs for each value of K (K = 1–21) assuming an admixture model and using 100,000 replicates of the MCMC after a burn-in of 10,000 iterations. The number of clusters was calculated from the ΔK estimates using Evanno et al.’s method [54]. Assignments of individuals to the inferred clusters were estimated according to the highest Q-values (probability of membership).
We compared the results obtained from Structure with those from Tess v.2.3 [55]. The software is based on a hierarchical mixture model whose neighborhood system is obtained from the Voronoi tessellation [55]. We performed 10 runs (K = 2–21) with an admixture model with a total of 50,000 sweeps with a burn-in of 10,000. The number of clusters was calculated plotting the Deviance Information Criterion (DIC) against values of K and choosing the value of K that corresponded to a plateau of the curve [56].
Allozymes
We re-analyzed the dataset of De Matthaeis et al. [8] consisting of 21 allozymic loci, 16 populations and 363 individual (2 to 105 per population; see Table 1). We calculated pairwise FST values, AMOVA and IBD using Arlequin. We performed the AMOVA on three groups combining populations according to their geographical position and patterns of relationships as detailed in De Matthaeis et al. [8] (Tyrrhenian + Aegean Sea; North Western Sardinia; South Western Sardinia). We analyzed the genetic structure of populations by running Structure (K = 1–16) and Tess (K = 2–16) with the settings described in the microsatellite section.
Approximate Bayesian computation
We used Approximate Bayesian Computation in DIYABC 1.0.4.39 [57] to evaluate the two competing scenarios (marine vs. terrestrial) detailed in the Introduction. To reduce computation time, we selected nine populations (SCP, SNC, STA, SAR, CCL, FRA, GOZ, PMP, PSF) as representative of each sampled area. We chose populations with complete data sets for both mtDNA and microsatellites and with the lowest divergence from the other populations from the same area. The marine scenario was designed following the subdivision of the Mediterranean Sea in biogeographic sectors proposed by Bianchi & Morri [58]; these would group the West Mediterranean basin and the Tyrrhenian Sea together (hence SCP, SNC, STA, SAR, CCL, FRA were forced to merge into a common ancestor), the Maltese Archipelago (GOZ) would be a transition area between the former sector and the Ionian one (PMP) while the South Adriatic Sea (PSF) would form a separated biogeographic area. The terrestrial scenario was designed on the basis of the geographic origin of populations. We considered the following areas; North-Eastern (STA), North-Western (SAR), South-Western (SNC), South-Eastern Sardinia (SCP), Tyrrhenian Sea (CCL, FRA; one insular and one peninsular population), Maltese Archipelago (GOZ), Ionian (PMP) and Adriatic (PSF) Sea. Three data sets were considered in the analysis (mtDNA, microsatellites, both markers combined); for each scenario we simulated 2 × 106 data sets. For mtDNA we assumed the default settings in DIYABC for mitochondrial markers; for microsatellites the loci were assumed to follow a generalized stepwise mutation model. We calculated the posterior probabilities of the two competing scenarios for each data set by i) evaluating the relative proportions of each scenario found in the selected closest data sets (Direct estimate; 500 simulated data sets) and through ii) a polychotomous logistic regression on the 1% of the simulated data sets closest to the observed data sets (default settings in DIYABC). Before estimating the posterior probabilities of scenarios, we checked whether the combination of scenarios and prior distributions of their parameters have produced data sets that are similar enough to the observed ones by performing a Principal Component Analysis (PCA) of the first 100,000 simulated data sets to evaluate the position of the observed data compared to the simulated.
Results
Mitochondrial DNA
The 295 COI sequences identified a total of 82 unique haplotypes (25 from Pavesi et al. [23] plus 57 newly found in this study) and 71 variable and parsimony-informative sites (GenBank Accession N.: JQ390313-JQ390337, KC568143-KC568199).
Analyses of molecular variance (AMOVA) performed on COI, microsatellites and allozyme data for K = 3 and K = 5 groups
COI | Microsatellites | Allozymes | ||||
|---|---|---|---|---|---|---|
Source of variation | % of variation | Fixation index | % of variation | Fixation index | % of variation | Fixation index |
K = 3 | ||||||
Among groups | 1.27 | 0.012* | 5.71 | 0.057*** | 3.73 | 0.034* |
Among populations within groups | 28.08 | 0.284*** | 11.28 | 0.119*** | 9.27 | 0.096*** |
Within populations | 70.65 | 0.293*** | 83.01 | 0.169*** | 87.3 | 0.127*** |
K = 5 | ||||||
Among groups | 9.35 | 0.093** | 7.6 | 0.076*** | ||
Among populations within groups | 21.04 | 0.232*** | 9.25 | 0.100*** | ||
Within populations | 69.61 | 0.303*** | 83.15 | 0.168*** | ||
Pairwise F ST values for all comparisons among populations with mtDNA (upper diagonal), microsatellites (lower diagonal)
CCL | CSR | SAR | SAP | SAB | SAF | SSS | SPC | SNS | SNL | SNG | SNA | SNB | SNC | SCP | STA | SMM | SMS | SMT | TTA | LFM | FRA | GOZ | PMP | PSF | PSC | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
CCL | - | 0.061 | 0.217 | 0.280 | 0.168 | 0.078 | 0.289 | 0.152 | 0.086 | 0.242 | 0.083 | 0.053 | 0.330 | 0.399 | 0.090 | 0.127 | 0.144 | 0.162 | 0.131 | 0.054 | 0.076 | 0.127 | 0.254 | 0.194 | 0.152 | 0.083 |
CSR | - | - | 0.257 | 0.351 | 0.185 | 0.053 | 0.401 | 0.160 | 0.065 | 0.294 | 0.000 | 0.000 | 0.428 | 0.536 | 0.071 | 0.125 | 0.150 | 0.175 | 0.130 | 0.021 | 0.047 | 0.124 | 0.313 | 0.222 | 0.160 | 0.000 |
SAR | 0.242 | - | - | 0.385 | 0.286 | 0.207 | 0.408 | 0.269 | 0.217 | 0.351 | 0.330 | 0.228 | 0.429 | 0.487 | 0.211 | 0.249 | 0.268 | 0.278 | 0.250 | 0.178 | 0.221 | 0.247 | 0.363 | 0.307 | 0.269 | 0.330 |
SAP | 0.145 | - | 0.073 | - | 0.341 | 0.267 | 0.471 | 0.324 | 0.278 | 0.405 | 0.438 | 0.313 | 0.481 | 0.538 | 0.267 | 0.307 | 0.328 | 0.333 | 0.305 | 0.233 | 0.292 | 0.303 | 0.417 | 0.362 | 0.324 | 0.438 |
SAB | 0.161 | - | 0.057 | 0.040 | - | 0.160 | 0.357 | 0.225 | 0.170 | 0.308 | 0.242 | 0.164 | 0.385 | 0.444 | 0.168 | 0.205 | 0.222 | 0.235 | 0.206 | 0.134 | 0.168 | 0.203 | 0.319 | 0.264 | 0.225 | 0.242 |
SAF | 0.231 | - | 0.177 | 0.126 | 0.162 | - | 0.274 | 0.144 | 0.081 | 0.231 | 0.073 | 0.047 | 0.314 | 0.378 | 0.084 | 0.121 | 0.136 | 0.154 | 0.124 | 0.050 | 0.070 | 0.120 | 0.242 | 0.185 | 0.144 | 0.073 |
SSS | 0.166 | - | 0.091 | 0.063 | 0.066 | 0.153 | - | 0.337 | 0.287 | 0.431 | 0.524 | 0.344 | 0.524 | 0.596 | 0.274 | 0.318 | 0.342 | 0.348 | 0.316 | 0.238 | 0.306 | 0.314 | 0.446 | 0.381 | 0.337 | 0.524 |
SPC | 0.149 | - | 0.151 | 0.114 | 0.117 | 0.211 | 0.134 | - | 0.153 | 0.290 | 0.210 | 0.141 | 0.367 | 0.424 | 0.152 | 0.189 | 0.205 | 0.219 | 0.190 | 0.119 | 0.150 | 0.187 | 0.301 | 0.248 | 0.210 | 0.210 |
SNS | 0.143 | - | 0.112 | 0.096 | 0.094 | 0.159 | 0.119 | 0.043 | - | 0.241 | 0.089 | 0.057 | 0.327 | 0.393 | 0.092 | 0.129 | 0.145 | 0.163 | 0.133 | 0.057 | 0.079 | 0.129 | 0.253 | 0.194 | 0.153 | 0.089 |
SNL | - | - | - | - | - | - | - | - | - | - | 0.371 | 0.261 | 0.448 | 0.505 | 0.233 | 0.272 | 0.291 | 0.300 | 0.271 | 0.200 | 0.249 | 0.270 | 0.383 | 0.329 | 0.290 | 0.371 |
SNG | 0.143 | - | 0.125 | 0.107 | 0.127 | 0.159 | 0.137 | 0.043 | 0.074 | - | - | 0.000 | 0.524 | 0.638 | 0.095 | 0.167 | 0.200 | 0.229 | 0.171 | 0.029 | 0.067 | 0.165 | 0.396 | 0.286 | 0.210 | 1.000 |
SNA | 0.188 | - | 0.122 | 0.093 | 0.113 | 0.148 | 0.131 | 0.060 | 0.055 | - | 0.020 | - | 0.383 | 0.481 | 0.063 | 0.110 | 0.132 | 0.155 | 0.115 | 0.018 | 0.040 | 0.110 | 0.278 | 0.196 | 0.141 | 0.000 |
SNB | - | - | - | - | - | - | - | - | - | - | - | - | - | 0.581 | 0.310 | 0.351 | 0.375 | 0.376 | 0.348 | 0.276 | 0.349 | 0.347 | 0.461 | 0.405 | 0.367 | 0.524 |
SNC | 0.218 | - | 0.181 | 0.165 | 0.187 | 0.181 | 0.195 | 0.151 | 0.132 | - | 0.018 | 0.049 | - | - | 0.367 | 0.411 | 0.438 | 0.433 | 0.405 | 0.333 | 0.427 | 0.406 | 0.519 | 0.462 | 0.424 | 0.638 |
SCP | 0.070 | - | 0.206 | 0.112 | 0.153 | 0.186 | 0.156 | 0.117 | 0.100 | - | 0.100 | 0.127 | . | 0.167 | - | 0.130 | 0.145 | 0.162 | 0.133 | 0.062 | 0.083 | 0.130 | 0.244 | 0.190 | 0.152 | 0.095 |
STA | 0.118 | - | 0.197 | 0.126 | 0.169 | 0.159 | 0.128 | 0.175 | 0.122 | - | 0.174 | 0.164 | - | 0.216 | 0.090 | - | 0.183 | 0.198 | 0.169 | 0.096 | 0.123 | 0.166 | 0.283 | 0.228 | 0.189 | 0.167 |
SMM | 0.196 | - | 0.210 | 0.125 | 0.166 | 0.155 | 0.165 | 0.131 | 0.129 | - | 0.129 | 0.165 | - | 0.227 | 0.163 | 0.139 | - | 0.215 | 0.185 | 0.111 | 0.141 | 0.182 | 0.303 | 0.245 | 0.205 | 0.200 |
SMS | 0.152 | - | 0.160 | 0.115 | 0.160 | 0.145 | 0.118 | 0.139 | 0.095 | - | 0.157 | 0.148 | - | 0.197 | 0.152 | 0.070 | 0.097 | - | 0.200 | 0.129 | 0.161 | 0.197 | 0.311 | 0.257 | 0.219 | 0.229 |
SMT | 0.098 | - | 0.185 | 0.091 | 0.108 | 0.170 | 0.139 | 0.079 | 0.092 | - | 0.140 | 0.131 | - | 0.196 | 0.132 | 0.134 | 0.074 | 0.096 | - | 0.100 | 0.127 | 0.168 | 0.282 | 0.229 | 0.190 | 0.171 |
TTA | 0.064 | - | 0.210 | 0.139 | 0.186 | 0.164 | 0.181 | 0.186 | 0.145 | - | 0.145 | 0.164 | - | 0.155 | 0.051 | 0.095 | 0.188 | 0.142 | 0.152 | - | 0.045 | 0.096 | 0.210 | 0.157 | 0.119 | 0.029 |
LFM | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | 0.123 | 0.263 | 0.196 | 0.150 | 0.067 |
FRA | 0.255 | - | 0.282 | 0.279 | 0.239 | 0.323 | 0.273 | 0.275 | 0.215 | - | 0.285 | 0.304 | - | 0.336 | 0.245 | 0.237 | 0.219 | 0.204 | 0.220 | 0.232 | - | - | 0.280 | 0.226 | 0.187 | 0.165 |
GOZ | 0.118 | - | 0.117 | 0.061 | 0.101 | 0.036 | 0.116 | 0.143 | 0.095 | - | 0.095 | 0.091 | - | 0.114 | 0.087 | 0.100 | 0.132 | 0.111 | 0.109 | 0.076 | 0.254 | - | 0.340 | 0.301 | 0.396 | |
PMP | 0.207 | - | 0.112 | 0.119 | 0.119 | 0.173 | 0.112 | 0.163 | 0.113 | - | 0.175 | 0.146 | - | 0.230 | 0.170 | 0.137 | 0.192 | 0.149 | 0.170 | 0.208 | - | 0.278 | 0.043 | - | 0.248 | 0.286 |
PSF | 0.293 | - | 0.141 | 0.175 | 0.160 | 0.221 | 0.183 | 0.222 | 0.158 | - | 0.210 | 0.185 | - | 0.258 | 0.248 | 0.207 | 0.253 | 0.222 | 0.245 | 0.261 | - | 0.340 | 0.178 | 0.138 | - | 0.210 |
PSC | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - |
SAMOVA suggested the existence of three groups (FCT = 0.45; P < 0.05), finding two barriers isolating the Adriatic from the Ionian populations and then these two basins from the rest. The analysis of mismatch distributions supported demographic expansion in the Adriatic group (PSSD = 0.283) only; geographic expansion was supported in all groups (PSSD ≥ 0.184). Tajima’s D and Fu’s Fs were not significant for the Ionic (D = −0.792, P D = 0.217; FS = 3.854, PF S = 0.95) and Adriatic (D = −1.468, P D = 0.06; FS = 0.932, PF S = 0.706) groups while they were negative and highly significant for the remaining populations lumped in a single group (D = −2.157, P D = 0.000; FS = −25.189, PF S = 0.000). In light of the relatively poor performance of mismatch distribution statistics in detecting population demographic expansion compared to D and FS statistics [59], we tend to favor the latter two, which support demographic expansion in the Western Mediterranean and Tyrrhenian populations. In the Adriatic group the timing of demographic expansion (τ = 34.63; T = 1.731 million years) preceded the spatial expansion (τ = 7.52; T = 376,000 years). In the Ionic basin the geographic expansion dates back to 500,000 years ago (τ = 10). In the Western Mediterranean and Tyrrhenian Sea the two expansions were more recent and coeval (τ = 1.01; T = 50,500 years), justifying the star-like shape of the haplotype network (see below). The relatively small τ values suggest that expansions always started from small effective population sizes.
Statistical parsimony haplotype network of COI (mtDNA) haplotypes. The size of each circle is proportional to the haplotypes frequency; numbers beside circles refer to the number of individuals carrying that haplotype (N = 1 when no number is indicated). Black dots represent missing haplotypes; haplotypes are one mutational step away from one another if not indicated otherwise. Different colors identify the geographic origin: green – Tyrrhenian Sea; red – Northern-Sardinia (Western Mediterranean Sea); blue – Southern Sardinian (Western Mediterranean Sea); black – Eastern Mediterranean Sea; orange – Ionian Sea; yellow– Adriatic Sea.
Microsatellites
Global F ST values at eight microsatellite loci calculated using FreeNA software and employing 10000 bootstrap iterations
Locus | Global FSTnot using ENA | Global FSTusing ENA |
|---|---|---|
1 | 0.301606 | 0.280849 |
2 | 0.065796 | 0.080518 |
3 | 0.119156 | 0.118377 |
4 | 0.159405 | 0.141352 |
5 | 0.114114 | 0.101403 |
6 | 0.146024 | 0.125829 |
7 | 0.124407 | 0.118899 |
8 | 0.099773 | 0.082684 |
AMOVA indicated a significant genetic structure and most of the genetic variability, when populations were grouped either in three (83.01%) or five groups (83.15%), was apportioned within populations (Table 2). Population differentiation (pairwise FST, Table 3) was significant for all pairwise comparisons except two comparisons (TTA-SCP and CCL-SCP). The Mantel test did not detect a pattern of IBD (R = 0.0001; P = 0.465).
Patterns of genetic divergence at the eight microsatellite loci as revealed by Structure (above) and Tess (below) for K = 3 and K = 5. Each vertical line represents one individual. The length of each line reflects the percentage probability of each individual’s membership to each cluster. For K = 3 clusters are shown in green, blue and red. For K = 5 clusters are indicated in light green, red, blue, orange and dark green. Codes for populations are as in Table 1.
With K = 5 Tess identified the following five geographic clusters: 1) Northern Sardinian populations (Western Mediterranean basin); 2) Southern Sardinian populations (Western Mediterranean basin), 3) Tyrrhenian basin, 4) GOZ (Maltese Archipelago; Eastern Mediterranean basin), 5) Ionian plus Adriatic basins. When Structure was forced to use K = 5, the software also split the Western Mediterranean populations in two groups (corresponding to Northern and Southern Sardinian locations). Additional groups were formed by the Ionian and the Adriatic populations together and by two Tyrrhenian clusters. The Tyrrhenian groups corresponded to North Eastern Sardinian islets (populations STA, SMM, SMS and SMT) and Italian peninsular sampling sites (TTA, FRA and SCP).
Intriguingly, individuals carrying the four deeply divergent COI haplotypes (Figure 2) do not possess a similarly deviant microsatellite genotype. Membership of the Tyrrhenian/Ionian, S-W Sardinian, and Adriatic individuals to the respective clusters ranges between 0.84 and 0.98 (Structure and Tess). Tess assigned the N-W Sardinian individual to the Northern Sardinian group with a membership of 0.75 while Structure suggested for this individual a membership shared between cluster 1 and 2 (0.36, 0.43).
Allozymes
Pairwise F ST values for all comparisons among populations with allozymes
SAR | SAP | SAB | SPC | SNL | SNA | SNC | SCP | STA | SMM | SMS | SMT | SMP | SCA | FRA | GRE | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
SAR | - | |||||||||||||||
SAP | 0.055 | - | ||||||||||||||
SAB | 0.034 | 0.022 | - | |||||||||||||
SPC | 0.032 | 0.011 | −0.007 | - | ||||||||||||
SNL | 0.066 | 0.102 | 0.112 | 0.076 | - | |||||||||||
SNA | 0.101 | 0.169 | 0.165 | 0.132 | −0.016 | - | ||||||||||
SNC | 0.060 | 0.096 | 0.102 | 0.080 | −0.018 | −0.006 | - | |||||||||
SCP | 0.068 | 0.109 | 0.096 | 0.062 | −0.015 | −0.012 | −0.007 | - | ||||||||
STA | 0.257 | 0.492 | 0.418 | 0.413 | 0.438 | 0.472 | 0.406 | 0.433 | - | |||||||
SMM | 0.054 | 0.015 | 0.031 | 0.014 | 0.043 | 0.084 | 0.040 | 0.038 | 0.429 | - | ||||||
SMS | 0.105 | 0.164 | 0.164 | 0.128 | −0.005 | −0.015 | 0.008 | −0.003 | 0.449 | 0.083 | - | |||||
SMT | 0.049 | 0.027 | 0.022 | 0.000 | 0.059 | 0.111 | 0.059 | 0.050 | 0.418 | 0.003 | 0.098 | - | ||||
SMP | 0.062 | 0.058 | 0.101 | 0.062 | −0.003 | 0.050 | 0.017 | 0.035 | 0.469 | 0.043 | 0.055 | 0.045 | - | |||
SCA | 0.056 | −0.008 | 0.053 | 0.025 | 0.051 | 0.121 | 0.063 | 0.080 | 0.491 | 0.026 | 0.121 | 0.028 | 0.002 | - | ||
FRA | 0.122 | 0.191 | 0.173 | 0.155 | 0.054 | 0.033 | 0.027 | 0.028 | 0.388 | 0.111 | 0.029 | 0.130 | 0.131 | 0.180 | - | |
GRE | 0.012 | 0.152 | 0.063 | 0.023 | 0.093 | 0.194 | 0.071 | 0.104 | 0.387 | 0.034 | 0.154 | −0.032 | 0.025 | 0.044 | 0.164 | - |
Patterns of genetic divergence at twenty-one allozymic loci. a,b Allozymes results for Structure (a) and Tess (b) (K = 3). Histograms show the average membership to one of the three clusters of each population (see Table 1 for details). Clusters are indicated by light green, blue and dark green and correspond to Tyrrhenian Sea and Northern Sardinia (Western Mediterranean Sea) (light green), Southern Sardinia (Western Mediterranean Sea) (blue) and Aegean Sea (dark green) (see text for details).
Approximate Bayesian Computations
Results of the Approximate Computation Analyses. a,b,c ABC results for mtDNA (a), microsatellites (b) and both marker systems combined (c). On the left are shown the posterior probabilities based on direct estimates, on the right posterior probabilities are obtained through a logistic regression. In all circumstances the marine scenario is better supported than the terrestrial one.
Discussion
In the last two decades we have been accumulating genetic data on Mediterranean talitrids with the aim to comparatively describe the genetic structure of different species at the scale of the whole Mediterranean Basin (see [60] and references therein for a review on the issue). So far, the present contribution is the largest one both in terms of individuals screened and number of markers used focused on a single talitrid species.
Present genetic data suggest that the beachflea O. montagui has a complex phylogeographic structure. By using ABC, we found that a scenario with marine forces assumed as predominant in shaping the species genetic structure is clearly better supported than a scenario of regionalism based on the geographic origin of populations (terrestrial scenario). The marine scenario is favored regardless the marker system analyzed (mtDNA and microsatellites; either separately or combined). It is worth noting that, in spite of this robust evidence, patterns of relationships yielded by mtDNA and microsatellites (and also allozymes but to a lesser extent) are not mirroring one another but major differences emerged that can be explained considering the intrinsically different evolutionary properties of these markers.
Populations east and west of the theoretical STS boundary are significantly differentiated at the mtDNA level (SAMOVA results) while microsatellites are ambivalent on the issue (compare the most likely groupings identified by Structure and Tess; three and five respectively). The population sampled on Gozo Is. (Maltese Archipelago; Eastern Mediterranean basin) shares both mtDNA haplotypes and microsatellite alleles with Western Mediterranean, Tyrrhenian, Ionian and Adriatic populations. The lack of isolation by distance in the mtDNA and both nuclear datasets excludes geographic distance as the main determinant of genetic divergence. On the other hand, the vast majority of pairwise FST values and the AMOVA results are statistically significant regardless of the marker considered. This evidence points to an overall scenario of complex genetic fragmentation that needs to be carefully evaluated to correctly resolve population structure in the species.
As pointed out by Thiel and Haye [61], population connectivity of rafters depends on a variety of factors (distances between habitats, sea current patterns, dispersal capability and colonization potential of organisms) and unraveling the relative importance of each one is a hard task that would require coupling genetic and field data. O. montagui is a small enough organism to hypothesize that it could cling, find shelter and feed on P. oceanica wrack while at sea for as long as the wrack would persist and/or strand in a new location. The reproductive biology of amphipods may enhance dispersal and recruitment; by incubating the embryos and developing juveniles in the brood pouch females provide extended parental care [62]. Migrating gravid females would favor persistence of rafters over generations. The four deeply divergent COI haplotypes that we found in our dataset (Figure 2) could indeed represent immigrants from geographical areas that we did not cover with our sampling. The mtDNA legacy of these alleged immigrants has persisted in five locations due to the mtDNA maternal inheritance while their ancestry has vanished at the microsatellite level due to the bi-parental inheritance of these markers. The sporadic occurrence of haplotypes profoundly divergent from an otherwise locally homogeneous set of lineages has been already reported in the talitrid T. saltator[17].
In spite of this convincing evidence, we suggest caution in interpreting the previous and following findings in light of our incomplete sampling coverage in the Eastern Mediterranean Sea and the small sample size for one Adriatic population.
Divergence among and within basins: historical vs. contemporary processes
The SAMOVA analysis conducted on mtDNA data detected barriers to gene flow between Adriatic and Ionian populations and between these two and the remaining basins. Patterns of mtDNA relationships within each of the above groups are not similar. Adriatic and Ionian haplotypes are scattered in the network of Figure 2 and many intervening missing haplotypes need to be postulated to connect them. Conversely, the vast majority of haplotypes from the Tyrrhenian, Western and Eastern Mediterranean basins clusters around the two most frequent mtDNA variants and differs from them by one single mutational step. This indicates that haplotypes coalesce earlier into their last common ancestor in the Tyrrhenian, Western and Eastern Mediterranean basins than they do in the Adriatic and Ionian ones. A variety of reasons either intrinsic to the species ecology (different rates of population crashes) or basin-specific (differences in rates of formation of favorable conditions, i.e. heaps of stranded seagrasses, intermittent rafting routes, marine genetic barriers) could be responsible. Field studies aimed to gain a detailed understanding of the factors regulating the species’ niche are needed to properly understand the causes of these alternate mtDNA patterns.
Western Mediterranean/Tyrrhenian, Ionian and Adriatic mtDNA clusters (i.e. the three groups recognized by SAMOVA but see also ABC results) perfectly overlap with the corresponding biogeographic provinces identified within the Mediterranean Sea [58]; this evidence suggests historical factors to be responsible for the mtDNA pattern. Barriers to mtDNA gene flow can be traced back to the Pleistocene [23], when the sea level repeatedly dropped at each ice age peak and the different Mediterranean basins shrunk and became largely isolated from one another ([58] and references therein). The demographic and geographic expansions detected in our mtDNA data sets are indeed recurrently placed after major drops in sea level [63].
Microsatellites (and to a lesser extent allozymes) cluster individuals preferentially concordant to their geographic origin, while many mtDNA haplotypes from geographically far away locations are recurrently gathered together in the haplotype network and differ by one or few substitutions. The geographically close Ionian and Adriatic populations have quite similar microsatellite profiles (Figure 3) whereas divergence emerges between Northern and Southern Western Sardinian populations. Divergence was detected also among the Tyrrhenian, Western and Eastern Mediterranean basins. A closer look at the haplotype network of Figure 2 reveals that Northern and Southern Western Mediterranean populations have inverted frequencies of the two most common haplotypes, giving partial support (yet not detected by SAMOVA) to the microsatellite evidence. Altogether, patterns of relationships at the mtDNA level have relatively less geographical structure than those yielded by microsatellites. How could we then reconcile these discrepancies in light of the inherently different evolutionary properties of mtDNA and microsatellites [64]? The finer degree of microsatellite structuring would argue in favor of a female-biased gene flow. In our recent study on O. montagui based on a subset of six populations, we invoked male-biased dispersal to explain why the mtDNA fragmentation was not apparent at the microsatellite level [23]. In the current study, which relies on a better coverage of the species geographic distribution, the pattern is reversed. In light of this, we tend here to favor the female-biased gene flow hypothesis. This would also be in agreement with field studies showing that populations of Mediterranean talitrids, including O. montagui, generally have a strongly female-biased sex ratio ([65] and references therein).
O. montagui is able to disperse actively only over short distances; individuals could nonetheless be dragged away by waves within floating banks of P. oceanica and – theoretically –carried over ample ranges. The pattern of genetic structuring yielded by microsatellites is, in our opinion, reflecting these present-day processes and is influenced by the surface circulation of water masses, which are the principal carriers of floating material at sea. Genetic connectivity mirrors quite remarkably patterns of Mediterranean surface currents. Water masses flow in a south–north direction along the Tyrrhenian coast of the Italian peninsula and bifurcate along the Tuscan coasts into two branches (see Figure 1 modified from [37]). The first branch flows northward along the eastern coast of Corsica while a second one moves southward following the Sardinian eastern coasts. This pattern would explain why microsatellites consistently cluster Tyrrhenian populations together. Along the Sardinian western coasts water masses flow in a northward direction and a major gyre exists in the area, which is likely the cause of the microsatellite divergence found between South- and North-Western Sardinian populations (Western Mediterranean basin). The currents flowing in and out of the Adriatic Sea would promote gene flow between the Adriatic and Ionian populations. Finally, the highly admixed genetic profile of the sole Eastern Mediterranean population included in the study (GOZ) might be due to the position of the Maltese Archipelago at the crossroads between the main current flowing from the Atlantic Ocean to the Aegean Sea and that descending along the Ionian and South-eastern Sicilian coasts. The former would carry immigrants of Western Mediterranean and Tyrrhenian origin while the latter would be the source of Ionian and Adriatic alleles.
Comparisons to other Mediterranean species
We could not detect a decrease in genetic variability from the Western to the Eastern Mediterranean Sea, as previously shown by Viñas et al. [66] in swordfish. Multi-taxa evidence supports a marked decrease in variability between the Mediterranean and the Black Sea but not necessarily in a west–east direction within the Mediterranean Sea [67].
When we compare our data within those available on a similar geographic scale for other Mediterranean species an interesting result emerges. Several marine species are genetically more homogeneous in the Western Mediterranean basin than they are in the Eastern Mediterranean, Ionic or Adriatic Sea. This was recurrently observed in fishes (i.e. gobids; with Adriatic, Aegean and Tunisian groups, [25]; anchovies, with a clear distinction between Adriatic, Aegean and the rest of Mediterranean Sea, [68]). O. montagui partially follows this scheme; the uniqueness of the Adriatic and Ionic populations is evident at the mtDNA level only. Likewise, Western and Tyrrhenian basins are shallowly fragmented at the mtDNA level while microsatellites revealed within-groups patchiness. Interestingly enough, allozymes detected a fixed alternative allele between the Aegean population (GRE) and all the others analyzed in [8]. Unfortunately, since we did not have access to any samples from the Aegean Sea for mtDNA or microsatellites, we cannot be conclusive on the issue.
Previous studies on Mediterranean talitrid amphipods coarsely found that species with a profound population genetic structure are generally confined to sandy beaches where they burrow into sand (i.e. T. saltator, D. deshayesii) or dig into rotting logs (M. remyi) [8, 15, 18, 60]. Various species of Orchestia, including O. montagui, associated with heaps of decaying wrack were thought to be genetically homogeneous, even across vast geographical ranges [8–15]. The spatial scale at which genetic divergence would become apparent was found to vary considerably in talitrids, from few kilometers with no sharing of mtDNA haplotypes in M. remyi[18] to hundreds of kilometers in O. montagui ([8]; allozyme data). In T. saltator, allozymes clearly distinguished reciprocally isolated Tyrrhenian, Adriatic and Aegean groups [8].
The intrinsic active mobility of organisms is only one determinant of the amount of the realized dispersal [69]. Active dispersal is always limited in talitrids, independently from the single species’ ecology. Hence, differences in their degree of genetic structuring must have arisen because of differences in the amount of passive dispersal the various species are able to achieve. M. remyi lives in strong association with rotting logs stranded on sandy beaches; T. saltator burrows deeply into the sand to escape dehydration. In both circumstances, the chances for individuals to be dragged away by waves are far lower than those of O. montagui, which colonizes a temporally ephemeral habitat close to the water line. This would explain why our focus species was thought to be genetically poorly structured [8–15]. On the other hand, we believe that the conclusions to which previous studies on Mediterranean talitrids have arrived should be critically evaluated, especially for those species identified as able to sustain high levels of gene flow at the scale of the whole Mediterranean Sea. We have here shown that O. montagui can no longer be considered a species with a shallow genetic structure, as De Matthaeis et al. [8–15] concluded on allozyme basis. We have demonstrated that long distance dispersal through surface currents might happen in this species but these episodes are not frequent enough to ensure high levels of gene flow that would counteract the onset of appreciable local differences. A possible limiting factor could be identified in the relatively short persistence in time of the vector of passive dispersal (the P. oceanica wrack) at sea surface due to its negative buoyancy [61].
By comparing patterns yielded by microsatellites and allozymes for the same set of populations, we obtained an identical number of clusters (3) but membership of individuals was consistently higher in the microsatellite analyses, pointing – as expected – to a much better resolving power of these markers. The molecular footprint of high gene flow under low-resolution molecular assays that O. montagui was believed to bear has in fact converted to an appearance of intermediate gene flow under more stringent assays.
Conclusions
We were able to unveil the genetic structuring of O. montagui within the Mediterranean Sea at a fine geographical scale. By combining molecular markers with different evolutionary properties we distinguished historical processes from present-day forces. Pleistocene climatic changes caused the isolation and divergence of mtDNA lineages. Current dynamics – namely surface marine currents jointly with rafting via seagrass wrack – produced new and different patterns of structuring, which were revealed by microsatellites. ABC gave strong support to a scenario of genetic fragmentation molded predominantly by marine forces.
The lack of a statistically significant pattern of IBD at both classes of markers under a scenario of genetic fragmentation (see FST and AMOVA results) suggests that the species has not yet approached equilibrium between gene flow and drift [70], probably because expansions (both demographic and geographic) started from small effective population sizes and are relatively young, as revealed by the mismatch analyses. On the other hand, this conclusion should be considered with caution in light of the fact that we could cover only a small fraction of the eastern part of the species’ ranges.
Our results also pinpoint the difficulties in describing the population genetic structure in an ecotonal species, because of its simultaneous exposure to forces typical of two ecosystems (land and sea). The semi-terrestrial life style acquired by O. montagui prevents the species from realizing long-distance dispersal at sea at a rate comparable to that of truly marine organisms, especially those with a planktonic stage in their life cycle. The sea, on the other hand, functions as a means for passive dispersal by carrying individuals of O. montagui with floating materials across sites. The species’ genetic structure can indeed be largely explained in light of the pattern of circulation of surface sea currents. This passive process, being intrinsically unpredictable and variable, cannot counteract the onset of local genetic differences. Passive dispersal via floating material is extremely difficult to observe in nature and no information exists either on the rate of survival of these amphipods during the process or on their chances to settle on new sites following dispersal. Future avenues of research should foresee the development of ecological experiments capable of tracking single biological particles (talitrids in this case) in floating wracks to ultimately link genetic and oceanographic data in a unified framework [71].
Declarations
Acknowledgments
We wish to thank F. Pavesi for preparing Figure 1 and B.R. MacKenzie for critically reading a first draft of the manuscript. We wish to thank the followings for the authorizations to sample in the National Park and respective Marine Protected Areas: “Ente Parco Nazionale dell’Arcipelago di La Maddalena” (SMM, SMS, SMT samples), “Ente Parco dell’Area Marina Protetta Isola dell’Asinara” (samples SAP, SAB, SAR, SAF), “Area Marina Protetta Capo Carbonara” (SCP sample), “Area Marina Protetta di Tavolara” (STA sample). We wish to thank Dr. G. Fanelli (CNR Taranto-Istituto per l’Ambiente Marino Costiero, Italy) and Prof. S. Piraino (University of Lecce, Italy) for suggestions about the sampling localities along the Apulian coasts. The associate editor Nora J Besansky and three anonymous reviewers provided useful comments that improved the quality of the manuscript.
Authors’ Affiliations
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