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ORIGINAL ARTICLE
doi:10.1111/j.1558-5646.2011.01255.x
SPECIATION AND DISPERSAL ALONGCONTINENTAL COASTLINES AND ISLANDARCS IN THE INDO-WEST PACIFIC TURBINIDGASTROPOD GENUS LUNELLASuzanne Williams,1,2 Deepak Apte,3 Tomowo Ozawa,4 Fontje Kaligis,5 and Tomoyuki Nakano6
1Zoology Department, Natural History Museum, London SW7 5BD, United Kingdom2E-mail: [email protected]
3Bombay Natural History Society, Hornbill House, S. B. Singh Rd, Mumbai 400 001, India4Department of World Heritage, Cyber University, Nagoya Office, Ikegamicho-2-7-1-203, Chikusa-ku,
Nagoya 464-0029, Japan5Marine Science Study Program, Faculty of Fisheries and Marine Sciences, University of Sam Ratulangi,
Manado 95115 Indonesia6Department of Geology and Palaeontology, National Museum of Nature and Science, 3-23-1 Hyakunin-cho, Shinjuku-ku,
Tokyo 169-0073, Japan
Received August 12, 2010
Accepted February 1, 2011
Species trees were produced for the Indo-West Pacific (IWP) gastropod genus Lunella using MrBayes, BEAST, and ∗BEAST with
sequence data from four genes. Three fossil records were used to calibrate a molecular clock. Eight cryptic species were recognized
using statistical methods for species delimitation in combination with morphological differences. However, our results suggest
caution in interpreting ESUs defined solely by the general mixed Yule Coalescent model in genera like Lunella, with lower dispersal
abilities. Four almost entirely allopatric species groups were recovered that differ in ecology and distribution. Three groups occur
predominantly along continental coastlines and one occurs on island arrays. Sympatric species occur only in the torquata and
coronata groups along coastlines, whereas species in the cinerea group, distributed in two-dimensional island arrays, occur in
complete allopatry. Dispersal along island arcs has been important in the maintenance of species distributions and gene flow
among populations in the cinerea group. The emergence of new islands and their eventual subsidence over geological time has
had important consequences for the isolation of populations and the eventual rise of new species in Lunella.
KEY WORDS: Biogeography, Indo-West Pacific, speciation, species delimitation, tectonics.
Several interrelated exogeneous factors play pivotal roles in the
evolution of shallow-sea organisms. Four of the most impor-
tant factors are environment, geography, tectonics, and sea level.
These factors, in combination with biological differences, espe-
cially ecology and developmental mode, greatly affect patterns
of distribution and rates of speciation (Valentine and Jablonski
1982, 1983; Hellberg 1998; Collin 2003; Williams and Reid 2004;
Hoeksema 2007). In this study, we use a marine gastropod genus
to investigate the effects of these factors on species distributions
and patterns of speciation. In particular, we compare patterns
between species occurring in two different habitat types: one-
dimensional continental coastlines versus two-dimensional island
arrays.
The geography of a shallow-sea realm can be markedly af-
fected by tectonic events and changes to sea level. Continents
move laterally over time, coastlines change and islands subside
or emerge, resulting in the opening or closing passages and the
creation or loss of shallow-water habitat (Valentine and Jablonski
1 7 5 2C© 2011 The Author(s). Evolution C© 2011 The Society for the Study of Evolution.Evolution 65-6: 1752–1771
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SPECIATION ON COASTLINES AND ISLAND ARCS IN LUNELLA
1982; Wilson and Rosen 1998; Hall 2001; Paulay and Meyer
2002; Kuhnt et al. 2004; Hall 2009). These changes to geography
result in changes to climate and environment, including salinity
(affected by freshwater runoff), sea-water temperature and trophic
resources (Valentine 1971; Hall 2009). Combined, these in turn
alter ocean current velocities and direction of flow (Kuhnt et al.
2004; Hall 2009), affecting gene flow among populations (Paulay
and Meyer 2002). Organisms react to all these changes by ex-
panding or reducing their distribution or by evolving in response
to changing local selection pressures (Valentine and Jablonski
1982), profoundly affecting the biogeography of a region.
The vetigastropod genus Lunella (family Turbinidae) is a
model group to test how species distributions and patterns of spe-
ciation differ between species distributed along continental coast-
lines and island arcs and to identify key drivers. The genus is found
only in the IWP, occurring from the western Indian Ocean, along
the east coast of Africa and the Arabian Peninsula, across to the
more continental islands of the West Pacific (e.g., New Zealand,
Fiji and American Samoa). It does not occur in the East Pacific or
Hawaii or on the oceanic island archipelagos of the Pacific (e.g.,
Marianas, Tuvalu or Kiribati). Individual species occur on rocky
shores in the intertidal zone either along continental coastlines
or on island arrays. Fertilization is external in all species that
have been examined (e.g., L. torquata, Joll 1980; Ward and Davis
2002). In L. smaragdus the young hatch 24 h after fertilization and
settlement probably occurs within four days (Grange 1976). Stud-
ies of reproductive behavior have shown similar development for
other turbinid species (e.g., Megastraea undosa, Guzman del Proo
et al. 2003; Turbo marmoratus, Yamaguchi 1993; Dwiono et al.
2001), and some turbinid species produce benthic egg masses with
crawl-away larvae (e.g., Turbo radiatus, Eisawy and Sorial 1974;
T. stenogyrus; Kono and Yamakawa 1999). As such, dispersal in
Lunella is likely to be limited between populations separated by
hundreds of kilometers. The fossil record, as for many rocky-
shore taxa, is poor, but some fossils do exist that can be used to
calibrate a molecular clock.
In this study, we use a near-complete, species-level phy-
logeny of the genus Lunella to investigate species distributions
and patterns of speciation. In particular, we investigate how these
differ between species distributed along continental coastlines
and island arcs. We compare patterns of distribution with a robust
phylogeny dated with fossil calibrations to infer mechanisms of
speciation. As cryptic species have already been found in Lunella
(Williams 2007), we use sequence-based methods to delimit evo-
lutionary lineages.
Materials and MethodsSAMPLING AND IDENTIFICATION
A total of 229 specimens of Lunella were sequenced, with sample
sizes ranging from seven to 95 per species recognized prior to
this study. We include four of the five species recognized in Alf
and Kreipl (2003), plus the recently identified L. jungi and L.
ogasawarana. We also include both Australian (L. undulata and L.
torquata) and New Zealand endemics (L. smaragdus) that have at
times been referred to the genus Turbo because molecular studies
show that they belong to Lunella (Williams and Ozawa 2006;
Williams 2007; this study). We were unable to obtain samples
from only one species; L. viridicallus from the Red Sea. As in our
previous papers, we continue to use the name L. coreensis for the
(usually) imperforate species found in Japan and Korea and use L.
granulata for the (usually) umbilicate species found in China and
Vietnam. The name L. moniliformis (used in Alf and Kreipl 2003)
is a synonym of L. granulata (Cernohorsky 1974). All specimens
are listed in Table S1.
Each species was sampled as widely as possible; as a result,
samples in this study cover the entire geographic range of the
genus although some areas of possible endemism were not sam-
pled (e.g., Red Sea, Madagascar, western Indonesia). Sequence
was obtained for COI from all but two samples, and 28S, 16S, and
12S sequences were obtained for at least three specimens from
each deeply divergent, reciprocally monophyletic clade identi-
fied in preliminary neighbor joining analysis of COI (not shown).
Previously published Lunella sequences are from Williams and
Ozawa (2006), Williams (2007) and Nakano et al. (2007).
In MrBayes analyses only, Lunella sequences were analyzed
together with previously published sequences of outgroup species
from the subfamily Turbininae (12 species in total from five differ-
ent genera; sequences from Williams and Ozawa 2006; Williams
2007).
DNA EXTRACTION, AMPLIFICATION, AND
SEQUENCING
The DNA extraction and amplification protocols described by
Williams and Ozawa (2006) and Williams et al. (2010) were
used to amplify portions of four genes: the nuclear 28S rRNA
gene (28S: 1496 bp) and three mitochondrial genes: cytochrome
oxidase subunit I (COI: 709 bp), 16S rRNA (16S: ∼610 bp),
and 12S rRNA (12S: ∼685 bp). Sequence reactions were per-
formed directly on purified PCR products using a BigDye Termi-
nator version 1.1 Cycle Sequencing Kit (Applied Biosystems, Life
Technologies Corporation, Carlsbad, CA) and run on an Applied
Biosystems 3730 DNA Analyser automated capillary sequencer.
Sequencing and PCR primers are listed in Table S2.
SEQUENCE ANALYSIS
Double stranded sequences were obtained for all gene fragments
and were edited using Sequencher (version 4.6 and version
4.8, Gene Codes Corporation, Ann Arbor, MI). All new se-
quences have been deposited in GenBank (accession numbers in
Table S1).
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SUZANNE WILLIAMS ET AL.
Alignments of both COI and 28S were unambiguous (both
including and excluding outgroups), requiring no insertions and
were done by eye in MacClade (version 4.08 OSX; Maddison
and Maddison 2003), checking amino acid translations in
COI. Alignment of mitochondrial ribosomal genes was more
complicated and these sequences were aligned using MAFFT
(Multiple Alignment using Fast Fourier Transform); a high speed
multiple sequence alignment program (version 6.0; Katoh et al.
2002; online http://align.bmr.kyushu-u.ac.jp/mafft/software/).
This programme has been shown to produce better alignments
than many more traditionally used programmes (e.g., Katoh et al.
2002). The Q-INS-i option was used, which is recommended
for a global alignment of highly diverged ncRNAs as secondary
structure of RNA is considered (Katoh and Toh 2008), and the
offset value was set at 0.1, as long gaps were not expected.
Poorly aligned sites in mitochondrial rRNA alignments were
identified using Gblocks Server (0.91b, Castresana 2000;
http://molevol.cmima.csic.es/castresana/Gblocks_server.html)
and removed from analyses. Parameters used in Gblocks allowed
for smaller final blocks and gap positions within the final blocks.
SPECIES DELIMITATION
Likely cryptic taxa were found in previous molecular studies
(Williams 2007) so we were concerned with delimiting species
correctly. We used sequence data to identify independently evolv-
ing lineages (or evolutionary significant units, ESUs; Moritz
1994) using the method of Pons et al. (2006), by estimating the
transition from coalescent to speciation branching patterns on an
ultrametric tree. This analysis exploits the predicted difference in
branching rates within and between species. Branching patterns
among species reflect the timing of speciation events (Yule 1924),
whereas branching rates within a species and among populations
reflect neutral coalescent processes (Kingman 1982; Monaghan
et al. 2009). This method identifies the point where a transition
between branching rates is most likely and the likelihood is com-
pared with a null model that all sequences are derived from a
single species (Pons et al. 2006; Monaghan et al. 2009).
We used the single-threshold, general mixed Yule-coalescent
(GMYC) model as implemented by SPLITS, code written by
T. Ezard, T. Fujisawa and T. Barraclough in R (version 2.10,
http://cran-project) to identify species from sequence variation in
COI, the “barcoding” gene. We then compared the validity of a
single gene approach with that of a multiple gene approach (based
on two loci) by comparing our results for COI with those based
on a tree produced by concatenation of all four genes.
Ultrametric trees for GMYC analyses were produced us-
ing BEAST (version 1.5.4.; Drummond and Rambaut 2007) us-
ing a relaxed lognormal clock, but without any fossil calibra-
tions and a fixed mean rate of substitutions set to one. We used
a constant coalescent prior, which is thought to be more con-
servative than a Yule prior for delimiting species (Monaghan
et al. 2009). Nucleotide substitution models used in prelimi-
nary analyses in BEAST were determined by MrModelTest us-
ing the hierarchical likelihood-ratio test (version 2.1, J. Nylan-
der, www.ebc.uu.se/systzoo/staff/nylander.html). Where multiple
models were suggested, the simplest was chosen. The best model
for each dataset was determined to be HKY + I + G for 16S and
COI, GTR + I + G for 12S and GTR + I for 28S. However, based
on preliminary analyses, nucleotide substitution models used in
GMYC/BEAST analyses were slightly different (HKY + I + G
for 16S and 12S, HKY + I for 28S and SDR06 for COI).
After preliminary runs, priors for various parameters were
changed, resulting in improved effective samples size (ESS) val-
ues. Each analysis ran for 50,000,000 generations with sample fre-
quency of 1000. The final trees were calculated based on 49,000
trees (after burnin of 1,001 generations) with maximum clade
credibility and median node heights. Length of burnin was deter-
mined by examination of traces in Tracer (version 1.5, avail-
able from http://beast.bio.ed.ac.uk/Tracer). Support for nodes
was determined using posterior probabilities (PP; calculated by
BEAST).
Average genetic distances for the “bar-coding” gene COI
were calculated using HKY + G + I (the model used in
phylogenetic analyses) and Kimura’s (1980) two-parameter
distances (K2P). The latter were calculated so that values
can be directly compared with other studies. Genetic dis-
tances and P ID (Liberal) among clades were calculated us-
ing a species delimitation plugin (B. Masters, V. Fan and H.
Ross; www.cebl.auckland.ac.nz/∼hros001/Software/SpDelim/)
for GeneiousPro (version 5.0.2; Drummond et al. 2009). P ID
(Liberal) is the mean probability of making a correct identifica-
tion of an unknown specimen of the focal species using BLAST
(best sequence alignment), DNA Barcoding (closest genetic dis-
tance) or placement on a tree, with the criterion that it falls sister
to or within a monophyletic species clade.
PHYLOGENY RECONSTRUCTION
A species-level phylogeny was produced using Bayesian infer-
ence as implemented in the programme BEAST. The analysis
was similar to that used for the GMYC analysis, but we used
a Yule prior, which is more appropriate for species-level phylo-
genies and assumes a constant speciation rate among lineages.
We used concatenated sequence from all four genes, and a single
individual to represent each species. Sequence variation was par-
titioned among genes and gene-specific nucleotide substitution
model parameters were used, with each gene allowed to evolve
at a different rate. We used similar nucleotide substitution mod-
els as were used in the 4gene BEAST/GMYC analysis (HKY +G + I for COI and 12S, HKY + I for 28S, HKY + G for 16S).
We used an uncorrelated relaxed, lognormal clock with three
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SPECIATION ON COASTLINES AND ISLAND ARCS IN LUNELLA
calibrations based on fossil evidence (see below). We ran the
analysis for 70,000,000 generations, sampling every 10,000 gen-
erations. The final species tree was a maximum clade credibility
tree with median node heights based on 6500 trees (after burnin
of 500 trees). In all analyses, sequences were assigned to species
based on results from species delimitation tests.
We also used the new Species Tree Ancestral Reconstruc-
tion (∗BEAST) method to confirm the topology obtained by the
BEAST analysis. It has been suggested that with some datasets
this method is superior to simple concatenation of multiple gene
partitions with respect to phylogenetic inference (Heled and
Drummond 2010). The ∗BEAST method coestimates gene trees
and a species tree and allows for the incorporation of multiple
exemplars of each species and the independent evolution of each
gene without fixing a single topology across genes (Heled and
Drummond 2010). Unlike “normal” BEAST analyses, it com-
bines priors for both speciation events and population genetics,
providing the opportunity to model for intraspecies polymorphism
and incomplete lineage sorting in phylogenetic estimation proce-
dures (Heled and Drummond 2010). In this analysis, all sequences
were included (as opposed to one per species in BEAST analyses),
with species defined a priori.
The ∗BEAST analysis ran for 900,000,000 generations with
a sample frequency of 10,000. The Yule tree prior was used for
species-level analyses and a constant coalescent model was used
for population-level analyses. Sequence variation was partitioned
among genes and gene-specific nucleotide substitution model pa-
rameters were used, with each gene allowed to evolve at a differ-
ent rate. We used the same nucleotide substitution models as were
used in the 4gene BEAST/GMYC analysis. Based on preliminary
analyses, we changed several of the priors, which resulted in im-
proved ESS values. A lognormal clock, but no fossil calibrations
were used in this analysis and mean rate was fixed to one. The
final ∗BEAST species tree was a maximum clade credibility tree
with median node heights based on 78,000 trees (after burnin of
12,000 trees). Length of burnin was determined by examination
of traces in Tracer. Support for nodes was determined using PP.
Although independent gene trees are obtained using∗BEAST, we did not use these trees as priors on population size
are such that there is a high likelihood of monophyly of species
as defined a priori (J. Heled, pers. comm. 2010). Therefore, in-
dividual gene trees were produced independently using Bayesian
inference as implemented in MrBayes (version 3.2, Huelsenbeck
and Ronquist 2001). Nucleotide substitution models used were
those suggested by MrModelTest, which were the same as those
for the ingroup alone, except for 16S (GTR + G + I). Analy-
ses were run for 7,500,000 generations with a sample frequency
of 1000. The first 2501 trees were discarded, so that 5000 trees
were accepted for each run after likelihood values had reached
a plateau. The datasets were analyzed in two independent runs,
and the final tree was computed from the combination of ac-
cepted trees from each run (a total of 10,000 trees). Conver-
gence between the two runs was tested by examining the poten-
tial scale reduction factors (PSRF) and standard deviation of split
frequencies.
FOSSIL CALIBRATIONS
Literature records state that the oldest fossil for Lunella is L.
miyarensis from the southern Ryukyu Islands, Japan, from the
Eocene Miyara group (MacNeil 1964). This group has been accu-
rately aged using foraminiferans and can be placed in the Priabo-
nian stage (37–34.2 Ma, Saito et al. 1984). The only specimen for
this species is the holotype, which is kept in the Smithsonian Insti-
tute (USNM 638646). Unfortunately, most of the fossil specimens
from this formation are poorly preserved, as the specimens occur
in consolidated hard limestone conglomerate and sandstone and it
is difficult to place this specimen accurately within the phylogeny.
We used it to constrain the cinerea and coronata groups, but not
species that were previously thought to belong in the genus Turbo.
The stem of the cinerea and coronata groups was constrained to
be at least 34.2 Ma (the youngest age of the fossil) (95% interval:
34.4–45 Ma; maximum age based on approximate mid-point of
Eocene, which allows both for the uncertainty of the fossil age,
and for the incompleteness of the fossil record) (mean in real
space: 2.5, log stdev: 1, offset 34.2).
We examined three specimens of L. kurodai (kindly donated
to the NHM by Susumu Tomida). This species is found in late
Early Miocene sediments of the Mizunami Group in central Japan
(approximately 16.5–17 Ma; S. Tomida, Chukyo Gakuin Univer-
sity, Nakatsugawa, Japan; pers. comm. 2010) and contemporane-
ous beds (Bihoku Group) in the Chugoku District, western Japan
(T. Ozawa, unpubl. data). Two of our specimens were collected
from the type locality (Kubohara sandstone of the Mizunami
Group in Kamigiri, Iwamura-cho, Ena City, Gifu Pref., Japan)
and one from Kujiri Bed, Mizunami Group in Inkyoyama, Kujiri,
Izumi-cho, Mizunami City, Gifu Prefecture, Japan (NHM PI TG
26505–07). Previous workers have suggested that L. kurodai is
most similar to L. coreensis (Itoigawa 1955). Comparisons of the
fossil specimens with our genetic samples suggest that shell shape
resembles that seen in several species within both the cinerea and
coronata groups. However, the pattern of spiral ribs made up of
small granules is found only in L. coreensis, L. granulata, L.
viridicallus and L. ogasawarana. Because these species represent
both subclades within the coronata group, we used L. kurodai to
date the age of the crown of the coronata clade. We used a log-
normal prior with 95% range from 16.5 Ma (the youngest age of
the fossil) to 34 Ma (which allows both for the uncertainty of the
fossil age, and for the incompleteness of the fossil record) (mean
in real space: 4.1, log stdev: 1, offset 16.15; 95% interval: 16.5 –
34 Ma).
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SUZANNE WILLIAMS ET AL.
Calibration of the cinerea clade was based on fossil spec-
imens of “Turbo versicolor” (=L. cinerea sensu latu) from
Junghun locations K (Cianjur, West Java) and R (Garut, Java) in
Indonesia (Leiden; RGM 11544). These locations have recently
been dated accurately by Willem Renema (Naturalis, Leiden, The
Netherlands), and his latest unpublished work suggests that both
correspond to the Middle Miocene. Of these two locations, loca-
tion R is older and likely to be approximately Langian (13–15 Ma)
(W. Renema pers. comm. 2010). A younger, complete specimen
from the oldest Pleistocene (also called “Turbo versiocolor”)
appears similar in size and shape to the central IWP form of
L. cinerea (Sonde, Central Java; Leiden; RGM 11545). However,
the Miocene samples are incomplete shells, showing some color
patterns, but lacking the columellar and lower part of the shell and
without the complete shell we are not confident to apply these fos-
sils to any particular lineage, although the species is definitely a
member of the cinerea group. We used the Miocene fossils to
calibrate the crown age of the cinerea group, with a lognormal
prior with 95% range from approximately 13 (the youngest age of
the oldest fossil) to 34 Ma (which allows both for the uncertainty
of the fossil age and incompleteness of the fossil record) (mean
in real space: 5, log stdev: 1, offset 12.6, 95% interval: 13 -34.1
Ma).
LOCATING CHANGES IN DIVERSIFICATION RATE
We used the relative cladogenesis statistic (RC) implemented in
END-EPI (version 1.0, Rambaut et al. 1997), to determine whether
there were any significant increases in diversification rates across
the phylogeny. The RC statistic uses a constant-rates birth–death
model and calculates the probability that a particular lineage exist-
ing at time t will have k extant tips. This probability is compared to
the total number of extant tips and the statistic identifies branches
with higher than expected rates of cladogenesis.
ResultsSEQUENCE ANALYSIS
For datasets used in the BEAST, ∗BEAST and GMYC/BEAST
analyses (which included only ingroup samples) the COI dataset
of 658 bp included 240 variable base pairs, of which 236 were
phylogenetically informative. For 28S, of 1452 bp, 40 were vari-
able, of which 36 were phylogenetically informative. Alignments
including outgroups (for MrBayes analyses) of COI and 28S in-
cluded (respectively) 258 and 60 variable base pairs, of which 249
and 49 bp were informative.
After removal of ambiguous blocks from mitochondrial ribo-
somal genes, 543 bp of sequence from 16S remained to be used in
phylogenetic analyses of ingroup taxa (86% of 626 bp) of which
207 bp were variable and 201 bp phylogenetically informative. A
total of 625 bp of sequence from 12S (90% of 690 bp) was used in
analyses, of which 288 bp were variable and 283 bp phylogenet-
ically informative. For datasets including outgroups, analysis of
16S was based on 499 bp of sequence excluding ambiguous sites
(77% of 645 bp), of which 200 bp were variable and 185 bp phy-
logenetically informative. Analysis of 12S was based on 566 bp
of sequence excluding ambiguous sites (79% of 708 bp), of which
282 bp were variable and 263 bp phylogenetically informative.
SPECIES DELIMITATION
Ultrametric trees were obtained for COI and concatenated se-
quences from all four genes with all ESS values greater than
200. In the GMYC/BEAST COI tree all ESUs were supported by
PP > 90% except I, J, L∗, and M that received very low support
(PP < 70%) and P and P′ which received only moderate support
(PP = 85%) (Fig. 1). In the GMYC/BEAST four-gene tree all
ESUs were well supported, with PP = 100% (Fig. 2).
The GMYC species delimitation test showed that the like-
lihood of the null model (that all specimens belong to a single
species) was significantly poorer than the maximum likelihood
of the GMYC model both for COI (2179 vs. 2191; ratio: 24.9,
P = 1.6 × 10−5) and for the four-gene tree (421 vs. 442; ratio:
41.8, P = 4.3 × 10−9). The threshold time (T) from the branch
tips at which the speciation-coalescent transition occurred ranged
from 0.007 in COI to 0.005 substitutions per site, resulting in 21
clusters being recognized in both the COI tree and in the four-
gene tree, although these did not completely correspond to the
same entities. Using the equivalent of a 95% confidence interval,
the total number of entities identified ranged from 19 to 26 in
the COI tree and 20 to 22 in the four-gene tree based on model
substitutions at two log-likelihood units from the maximum (C.I.;
Monaghan et al. 2009). If the lower C.I. is used to define species
in the COI tree, only 19 clusters are recognized with ESUs L∗and M combined, as are ESUs I and J. In the four-gene tree using
the lower C.I. limit ESUs P and P′ are combined.
A comparison of ESUs defined by the two GMYC/BEAST
analyses revealed some differences. Two clades within L. coronata
were recognized as distinct ESUs in the COI tree (ESUs O and O′),but not in the four-gene tree. Likewise two different clades within
L. coronata were recognized as distinct in the four-gene tree, but
not in the COI tree (ESUs P and P′). The composition of two ESUs
(L and M) also differed slightly between the two analyses, with
samples from Vanuatu and one from New Caledonia occurring
along with samples from American Samoa in ESU L∗ in the COI
analysis but in ESU M (with the remainder of the New Caledonian
samples) in the four-gene analysis and the MrBayes analysis of
COI (Fig. 3).
Overall, we recognize 18 putative species in Lunella
(Tables 1, S1) of which 17 have been included in this study and
eight are new. ESUs that are conservatively treated as species
in this study are those that are recognized in both GMYC
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SPECIATION ON COASTLINES AND ISLAND ARCS IN LUNELLA
EVOLUTION JUNE 2011 1 7 5 7
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SUZANNE WILLIAMS ET AL.
analyses, when using the set of species suggested by their re-
spective lower confidence limits. A morphological examination
of specimens used in genetic analyses confirmed that these ESUs
can be distinguished from their sister species morphologically
either by shell characters and/or pattern of coloration on anten-
nae, head, and snout. A morphometric analysis of outline shape
also distinguishes some cryptic species (Williams et al. 2011).
Some clades occur in sympatry with sister taxa and/or have fixed
differences at 28S, both of which are consistent with clades be-
ing biological species (Table 1). In some cases, species shared
identical 28S genotypes (which is common in turbinids; e.g.,
Williams 2007) and morphological differences were small and
based on few individuals, so we consider our putative species
list as a working hypothesis, which will need to be confirmed by
more detailed studies. Estimated divergence times between sister
species were all greater than 1.8 Myr (Table 1). Genetic distances
between species/clades ranged from 5.4 to 46.6% (K2P = 4.5–
16.8; Table 1). P ID (liberal) for the 17 clades accepted as species
were all above 0.95 (0.96–1.00).
ESUs that are considered to represent either population struc-
ture or subspecies are L. cinerea from Japan and the central IWP
(ESUs I and J) and L. cinerea from Vanuatu, New Caledonia and
American Samoa (L and M). These clades were not supported
at the lower C.I. limits in the COI tree nor could they be dis-
tinguished on morphological grounds or by differences at 28S.
Four clades of L. coronata (O, O′, P and P′) were not combined
in any analysis, even at the lower C.I. cutoff (except P and P′),but the threshold time between the two pairs in the four-gene
GMYC tree is lower than that of some of the other pairs that we
combined. Therefore, we consider these four clades to represent
a single species despite some slight morphological differences of
the Gulf of Persia samples (ESU O′ tends to have a higher shell
spire) and a fixed (albeit polymorphic) difference at 28S between
the Indian and UAE clade (ESU O) and other L. coronata clades.
Average genetic distances for COI sequences among these clades
(considered to represent intraspecific variation) were also lower
than those observed among accepted species pairs, ranging from
2.7% to 4.8% (K2P = 2.3–4.0%; Table 1).
PHYLOGENETIC ANALYSES
Potential scale reduction factor in all MrBayes analyses were
1.00, showing that runs had converged (Gelman and Rubin
1992) and average standard deviation of split frequencies for
partitions with frequency >0.10 in at least one run approached
zero (28S: 0.000005, 12S: 0.001349, 16S: 0.000013, COI:
0.000117).
Ultrametric trees were obtained for BEAST analyses using
concatenated sequences from all four genes with all ESS values
greater than 200 (some more than an order of magnitude greater).
The total number of unique clades was 24 and the highest log
clade credibility was −0.37. It proved difficult to obtain ∗BEAST
analyses with acceptable ESS values even after very log run times,
so the analysis was run without calibrations (fixed mean rate).
An undated phylogeny was obtained with all ESS values greater
than 200 (some more than an order of magnitude greater). The
topology of the consensus species tree obtained from BEAST
and ∗BEAST analyses was identical, but support for nodes varied
slightly (Fig. 5)
All individual gene trees, except COI, recovered Lunella as
monophyletic (Figs. 3 and 4). The cinerea clade was recovered in
both BEAST and ∗BEAST trees and all three mitochondrial gene
trees and the coronata clade was recovered in both BEAST and∗BEAST trees and the 28S, 16S, and COI trees (Figs. 3 and 4). A
clade with L. torquata, L. undulata, and L. jungi was recovered in
all trees. The position of L smaragdus (endemic to New Zealand)
was unstable in the four independent gene trees, although in the
mitochondrial gene trees it always fell outside a clade containing
the cinerea and coronata groups. In both the BEAST tree and∗BEAST trees, it was sister to the cinerea and coronata clades.
The clades identified in the GMYC/BEAST analysis were also
recovered in individual gene trees, although some ESUs shared
the same 28S sequence. The phylogenetic relationships found in
this study are consistent with those in earlier studies with fewer
taxa (Williams 2007; Nakano et al. 2007).
LOCATING CHANGES IN DIVERSIFICATION RATE
No significant changes in rate were observed in the phylogeny
using the RC test so no further investigation was undertaken.
DiscussionSPECIES DELIMITATION
Overall, we recognize 18 putative species in Lunella, of which 17
are included in this study (listed in Table S1) and eight are new,
almost doubling the known diversity for this genus. Seven clades
Figure 1. Results of GMYC test on an ultrametric tree produced using BEAST for the cytochrome oxidase I sequences. (A) Tree with ESUs
and species names marked on the right-hand side. Specimen number and country of collection are given at nodes. ESUs considered to
represent a single species are bounded by gray boxes. The composition of ESU L∗ is similar, but not identical to ESU L in other trees.
Support for nodes are posterior probabilities, shown only for species-level relationships and PP > 50%. Branches in light gray indicate
population structure. The cinerea group is labeled with a solid circle, the torquata group with a star, and the smaragdus clade with a
triangle. (B). Lineage through time plot with gray line showing the threshold level suggested by GMYC. (C) Maximum likelihood plot
showing peak congruent with threshold limit in B.
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SPECIATION ON COASTLINES AND ISLAND ARCS IN LUNELLA
Figure 2. Results of GMYC test on an ultrametric tree produced using BEAST for concatenated sequences from all four genes. (A) Tree
with ESUs and species names marked on the right-hand side. Specimen number and country of collection are given at nodes. ESUs
considered to represent a single species are bounded by gray boxes. Support for nodes are posterior probabilities, shown only for species
level relationships and PP > 50%. Branches in light gray indicate population structure. The cinerea group is labeled with a solid circle, the
coronata group with a square, the torquata group with a star, and the smaragdus clade with a triangle. (B) Lineage through time plot
with gray line showing the threshold level suggested by GMYC. (C) Maximum likelihood plot showing peak congruent with threshold
limit in B.
EVOLUTION JUNE 2011 1 7 5 9
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SUZANNE WILLIAMS ET AL.
recognized by the GMYC/BEAST analyses correspond to cur-
rently recognized species (see Table 1), of which two have been
described only recently (L. jungi, in Lai 2006; L. ogasawarana,
in Nakano et al. 2007). However, two additional species, L.
cinerea and L. coronata, each correspond to a species complex.
The cinerea group contains nine clades, which we interpret here
as representing seven species. The West Indian Ocean coronata
group contains six clades (a maximum of five recognized in either
GMYC analysis), which we interpret here as representing three
species. The status of the only species not included in this study,
L. viridicallus, remains to be tested genetically. The newly recog-
nized species qualify as phylogenetic species, but in the cinerea
clade, where all sister species are allopatric it is not possible to
test whether they also qualify as biological species. Several names
exist in the literature that might be applied to these taxa, but a com-
prehensive revision of the genus is beyond the scope of this study
and will be published elsewhere (S. T. Williams, unpubl. data). It
is also possible that additional cryptic species may yet be found
in Lunella. Likely areas of endemism not investigated genetically
include the Red Sea (where L. viridicallus occurs; Alf and Kreipl
2003), Indonesia, and Madagascar.
As has often been the case in studies to date there were more
GMYC clades than have been previously recognized as species by
traditional taxonomy (e.g., Papadopoulou et al. 2008; Monaghan
et al. 2009; Claremont et al. 2011). However, even with the benefit
of hindsight, we have not yet found strong evidence to support the
recognition of some clades as separate species and in this study,
we treat them as evidence of population structure. To delimit
species, we combined ESUs that were not supported in either tree
at the lower confidence limit and for which we could find no ad-
ditional evidence of specific status, and ESUs with splits younger
than those collapsed for other reasons. Detailed analysis of a gas-
tropod genus with higher dispersal abilities and therefore less
population structure (Stramonita, Claremont et al. 2011) suggests
that although the GMYC model identifies more ESUs than recog-
nized by traditional taxonomy, these ESUs nonetheless directly
correspond to biological species. However, our results suggest
that it may be necessary to use lower confidence limits to
distinguish between population structure and species in lower
Figure 3. Molecular phylogeny for Lunella with outgroups from
Turbininae based on Bayesian analysis of the single gene COI pro-
duced with MrBayes. Specimen number and country of collection
are given at nodes. ESUs are labeled on the right-hand side, fol-
lowing Figs. 1 and 2. Support values are posterior probabilities
(PP); branches with PP < 50% were collapsed. Not all PP values are
given for the sake of clarity. The cinerea group is labeled with a
solid circle, the coronata group with a square, the torquata group
with a star, and the smaragdus clade with a triangle. See Table S1
for details.
1 7 6 0 EVOLUTION JUNE 2011
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SPECIATION ON COASTLINES AND ISLAND ARCS IN LUNELLA
Ta
ble
1.
Sum
mar
yo
fES
Us
iden
tifi
edb
yG
MY
Can
alys
is(F
igs.
1an
d2)
and
dis
cuss
edin
the
text
;in
clu
din
gth
en
um
ber
of
spec
imen
sse
qu
ence
d(n
);ap
pro
xim
ate
geo
gra
ph
ical
ran
ge
(in
som
eca
ses
bas
edo
ng
enet
icse
qu
ence
so
nly
and
inth
eca
seo
fES
Us
Lan
dM
,b
ased
on
clad
esin
Fig
s.2–
4);
sist
ercl
ades
/sp
ecie
s(b
ased
on
rela
tio
nsh
ips
inth
eB
EAST
tree
inFi
g.
5);
div
erg
ence
tim
eb
etw
een
sist
ercl
ades
(Myr
;b
ased
on
Fig
.5)
;th
ep
rese
nce
of
mo
rph
olo
gic
ald
iffe
ren
ces
(eit
her
shel
lo
rso
ftti
ssu
e;Y-
yes,
N-
no
)b
etw
een
sist
er
clad
es/s
pec
ies
(bas
edp
rim
arily
on
seq
uen
ced
spec
imen
s);
wh
eth
ersi
ster
clad
es/s
pec
ies
occ
ur
insy
mp
atry
;th
eo
ccu
rren
ceo
ffi
xed
dif
fere
nce
sb
etw
een
sist
ercl
ades
/sp
ecie
sfo
r
seq
uen
cefr
om
28S
(P=
po
lym
orp
hic
fixe
dd
iffe
ren
cee.
g.,
Yvs
.T);
reci
pro
calm
on
op
hyl
yo
fcl
ades
/sp
ecie
sin
MrB
ayes
gen
etr
ees
(Fig
s.3
and
4);a
vera
ge
K2P
dis
tan
ceb
ased
on
CO
I
seq
uen
ced
ata
wit
hin
each
ESU
,an
db
etw
een
the
ESU
liste
dan
dth
ecl
ade
(lis
ted
inth
en
ext
colu
mn
)se
par
ated
by
the
smal
lest
gen
etic
dis
tan
ceu
sin
gC
OIs
equ
ence
on
ly;a
vera
ge
HK
Y+I
+Gd
ista
nce
bas
edo
nC
OIs
equ
ence
dat
ab
etw
een
ESU
and
the
clad
elis
ted
inth
en
ext
colu
mn
;an
dp
relim
inar
yco
ncl
usi
on
sab
ou
tES
Ust
atu
s—O
ne
spec
ies
=cl
ade
incl
ud
es
all
seq
uen
ces
ob
tain
edfo
ra
sin
gle
,d
iscr
ete
spec
ies;
—Po
pu
lati
on
stru
ctu
re=
clad
ein
clu
des
som
e,b
ut
no
tal
lse
qu
ence
so
bta
ined
for
asi
ng
lesp
ecie
s.N
od
ata
are
pro
vid
edfo
r
com
par
iso
nb
etw
een
ESU
sP
and
P′ o
rO
and
O′ b
ecau
seth
ese
clad
esw
ere
each
iden
tifi
edin
on
lyo
ne
of
the
GM
YC
/BEA
STtr
ees.
Bet
wee
nsi
ster
spec
ies/
clad
esR
ecip
roca
lmon
ophy
ly(M
rBay
es)
ESU
Spec
ies
nG
eogr
aphi
cal
rang
eSi
ster
clad
eD
ivtim
eM
yr
Mor
phdi
ffs
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patr
icFi
xed
diff
s28
S
CO
I12
S16
S%
K2P
intr
aC
OI
%K
2Pin
ter
CO
I
% HK
Y+
I+G
inte
rC
OI
Clo
sest
spec
ies
(CO
Ige
netic
dist
ance
)K
2P/H
KY
+I+
G
Prel
imin
ary
conc
lusi
ons
AL
.jun
gi7
Taiw
anB
+C19
YN
YY
YY
0.1
14.0
31.2
L.u
ndul
ata
One
spec
ies
BL
.tor
quat
a10
Sout
hern
Aus
tral
iaC
8.2
YY
YY
YY
0.4
12.4
21.5
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ndul
ata
One
spec
ies
CL
.und
ulat
a10
Sout
hern
Aus
tral
iaB
8.2
YY
YY
YY
0.7
12.4
21.5
L.t
orqu
ata
One
spec
ies
DL
.sm
arag
dus
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eala
ndE
-T35
.1Y
NY
YY
Y0.
117
.546
.6L
.cin
erea
NW
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tral
ia/L
.ci
nere
aFi
ji
One
spec
ies
EL
.cin
erea
NW
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tral
ia9
Nor
thW
este
rnA
ustr
alia
F+G
3.2
YN
NY
YY
0.3
6.7
8.7
L.c
iner
eaSu
law
esi
One
spec
ies
FL
.cin
erea
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wes
i4
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wes
i,In
done
sia
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3Y
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YY
Y0.
55.
67.
1L
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erea
NE
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tral
iaO
nesp
ecie
s
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erea
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tral
ia10
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thE
aste
rnA
ustr
alia
F2.
3Y
NP
YY
Y0.
35.
67.
1L
.cin
erea
Sula
wes
iO
nesp
ecie
s
HL
.cin
erea
Indi
anO
cean
18N
orth
-eas
tern
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anO
cean
E−G
6Y
NN
YY
Y0.
411
.317
.7L
.cin
erea
NW
Aus
tral
iaO
nesp
ecie
s
Ian
dJ
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iner
eacI
WP
24C
entr
alIn
do-W
est
Paci
fic
E−H
7.8
YN
NY
YY
1.3
12.6
24.8
L.c
iner
eaN
WA
ustr
alia
One
spec
ies
-I
–L
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erea
cIW
PA
7Ja
pan
J–
NN
NY
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Popu
latio
nst
ruct
ure
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erea
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entr
alIn
do-W
est
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fic
I–
NN
NY
NN
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eacI
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latio
nst
ruct
ure
Co
nti
nu
ed
EVOLUTION JUNE 2011 1 7 6 1
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SUZANNE WILLIAMS ET AL.
Ta
ble
1.
Co
nti
nu
ed
Bet
wee
nsi
ster
spec
ies/
clad
esR
ecip
roca
lmon
ophy
ly(M
rBay
es)
ESU
Spec
ies
nG
eogr
aphi
cal
rang
eSi
ster
clad
eD
ivtim
eM
yr
Mor
phdi
ffs
Sym
patr
icFi
xed
diff
s28
S
CO
I12
S16
S%
K2P
intr
aC
OI
%K
2Pin
ter
CO
I
% HK
Y+
I+G
inte
rC
OI
Clo
sest
spec
ies
(CO
Ige
netic
dist
ance
)K
2P/H
KY
+I+
G
Prel
imin
ary
conc
lusi
ons
KL
.cin
erea
Fiji
10Fi
jiL
M7.
6Y
NY
YY
Y0.
512
.423
.1L
.cin
erea
SWPa
cifi
cO
nesp
ecie
s
Lan
dM
L.c
iner
eaSW
Paci
fic
21So
uth-
Wes
tPac
ific
K7.
6Y
NY
YY
Y1.
812
.423
.1L
.cin
erea
Fiji
One
spec
ies
-L
–L
.cin
erea
SWPa
cifi
cA
5A
mer
ican
Sam
oaM
–N
NN
YY
N0.
24.
04.
8L
.cin
erea
SWPa
cifi
cB
–Po
pula
tion
stru
ctur
e
-M
–L
.cin
erea
SWPa
cifi
cB
16N
ewC
aled
onia
and
Van
uatu
L–
NN
NY
YN
0.4
4.0
4.8
L.c
iner
eaSW
Paci
fic
A–
Popu
latio
nst
ruct
ure
NL
.cor
onat
aop
hiol
item
orph
10U
nite
dA
rab
Em
irat
esO
−Q11
.5Y
YY
YY
Y<
0.1
16.8
43.8
L.c
oron
ata
coro
nate
One
spec
ies
Oan
dO
′
and
Pan
dP
′
L.c
oron
ata
coro
nate
mor
ph37
Wes
tInd
ian
Oce
anQ
5.2
YY
NY
YY
1.8
9.7
15.6
L.c
oron
ata
Om
anO
nesp
ecie
s
-O
and
O′
–L
.cor
onat
aco
rona
teA
and
B
24U
nite
dA
rab
Em
irat
esan
dIn
dia
Pan
dP
′–
NY
NN
NN
0.8
2.4
3.4
L.c
oron
ata
coro
nate
C–
Popu
latio
nst
ruct
ure
-P
and
P′
–L
.cor
onat
aco
rona
teC
13W
estI
ndia
nO
cean
Oan
dO
′–
NY
NN
NN
0.9
2.4
3.4
L.c
oron
ata
coro
nate
Aan
dB
–Po
pula
tion
stru
ctur
e
QL
.cor
onat
aO
man
6O
man
O−P
5.2
YY
NY
YY
0.4
9.3
15.6
L.c
oron
ata
coro
nate
One
spec
ies
RL
.cor
eens
is10
Sout
hE
astA
sia
S+T
4.6
YY
YY
YY
0.3
8.3
11.5
L.o
gasa
war
ana
One
spec
ies
SL
.oga
saw
aran
a10
Oga
saw
aran
aIs
land
s,Ja
pan
T1.
8Y
NY
YY
Y0.
14.
55.
4L
.gra
nula
taO
nesp
ecie
s
TL
.gra
nula
ta21
Sout
hE
astA
sia
S1.
8Y
NY
YY
Y0.
44.
55.
4L
.oga
saw
aran
aO
nesp
ecie
s
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SPECIATION ON COASTLINES AND ISLAND ARCS IN LUNELLA
Fig
ure
4.
Mo
lecu
lar
ph
ylo
gen
yfo
rLu
nel
law
ith
ou
tgro
up
sfr
om
Turb
inin
aeb
ased
on
Bay
esia
nan
alys
iso
fin
dep
end
ent
gen
es28
SrR
NA
,12S
rRN
A,a
nd
16S
rRN
Ap
rod
uce
dw
ith
MrB
ayes
.Su
pp
ort
valu
esar
ep
ost
erio
rp
rob
abili
ties
(PP)
;bra
nch
esw
ith
PP<
50%
wer
eco
llap
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SUZANNE WILLIAMS ET AL.
Figure 5. Chronogram for Lunella based on Bayesian analysis of concatenated sequence from 28S rRNA, COI, 12S rRNA, and 16S rRNA
genes incorporating an uncorrelated relaxed, lognormal clock produced with BEAST. Branch lengths are proportional to time and scale in
millions of years (Myr) is given below. Tree is a maximum clade credibility tree with median node heights based on 6500 trees. Horizontal
gray bars correspond to 95% highest posterior density (HPD) interval for node heights (ages). The 95% HPD is shortest interval that
contains 95% of the sampled values. Support values are posterior probabilities (PP) from BEAST/∗BEAST. Species names and ESUs are
labeled on the right-hand side. The cinerea group is labeled with a solid circle, the coronata group with a square, the torquata group
with a star, and the smaragdus clade with a triangle.
dispersal groups like Lunella. In fact, three cinerea clades (ESUs
E, F, and G) show similar biogeographic distributions to divergent
clades in another rocky-shore gastropod Echinolittorina vidua
(Reid et al. 2006). Reid et al. (2006) decided that the E. vidua
clades belonged to a single, highly structured species but K2P
distances for COI sequences between the three cinerea clades
(5.6–6.7%) are higher than those observed among the correspond-
ing E. vidua clades (2.15–3.77%) supporting our decision to retain
these ESUs as species pending further studies.
Differences in the analysis of sequences from COI alone ver-
sus four genes suggest that some clades are identified for spurious
reasons. First, the GMYC analysis presupposes a well-resolved
tree, but in fact, several nodes in the COI tree defining clades
were not well supported (with PP < 50%). This is particularly
important when it affects branching order because in an ultramet-
ric sister branches have the same height, switching branches may
make populations appear to be more distinct than they really are
(compare relationships within the West Indian Ocean coronata
group in Figs. 1, 2 and 3). Second, GMYC analysis of sequences
from four genes (although only two loci) resulted in the loss of one
clade and changed the composition of another; suggesting that it
may always be useful to compare results from several datasets and
raises (again) the question of accuracy when barcoding a single
gene. Additional, independent nuclear loci may also be helpful, if
they evolve at a sufficiently fast rate to identify recent divergences.
Finally, the importance of sampling has been raised as a potential
problem with GMYC analyses (Lohse 2009, although see also
Papadopoulou et al. 2009), and we believe that the separation of
ESUs P and P′ in the four-gene study may have been the result
of more limited sampling in that tree. Despite these limitations
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SPECIATION ON COASTLINES AND ISLAND ARCS IN LUNELLA
and used conservatively this method provides a nonsubjective
preliminary hypothesis for species delimitation, which can then
be used as a framework for further testing (Papadopoulou et al.
2009), helping to identify groups in need of greater taxonomic
work.
ENVIRONMENT
Various authors have noted that shallow-water marine species
show preferences for habitats that range from “continental,” along
continental coastlines or on high islands to “oceanic,” on low,
oceanic atolls (e.g., Reid 1986; Taylor 1997). Habitats along this
range differ in local nutrients, salinity, turbidity, and chlorophyll
among a vast range of other factors. It is not known exactly which
factors are important in determining distribution patterns, but it
may have to do with nutrients (Taylor 1997) and selection acting
on larvae (Williams and Reid 2004). Lunella occur on rocky-
shores along continental land margins or on high, continental
islands. Some species seem to prefer clearer water, but even these
species occur on high islands, not oceanic atolls (following defini-
tions in Springer 1982). For example, Lunella occurs in the Bonin
Islands, where the habitat is more continental and reefs are poorly
developed (Fukuda 1994), but not in the more oceanic Mariana
Islands.
Because all Lunella species share similar habitats and are
continental by preference, it seems unlikely that this habitat pref-
erence has had much impact on speciation in Lunella. However,
it may have been important in the evolution of deeper nodes. The
coronata clade is more common on continental coastlines whereas
its sister, the cinerea group, is more common on islands, suggest-
ing that ecology may have been important in the evolution of
these clades. Equally, distribution with respect to the littoral zone
may also have been important. Most of the cinerea and coronata
group occur in the high or mid intertidal zone, whereas L. smarag-
dus occurs in the mid to sub-littoral zone (Walsby 1977) as do L.
torquata and L. undulata (G. Vermeij, pers. comm. 2010). Similar
results have been found for other gastropods living in comparable
habitats (e.g., Nerita, Frey 2010, Echinolittorina, Williams and
Reid 2004; Reid et al. 2006; compare with Littoraria, Reid et al.
2010). Future studies involving ecological niche modeling may
be informative.
GEOGRAPHY: COASTLINES VERSUS ISLAND ARRAYS
Sympatric sister species occur only along coastlines in Lunella
in the coronata and torquata groups. In the torquata group, L.
torquata and L. undulata are sympatric across a large proportion
of their ranges along southern temperate Australia, although only
L. undulata is found in Tasmania and L. torquata occurs further
up the west coast of Australia. In the coronata group two cryptic
species apparently arose independently on the Arabian Peninsula
(ESUs N and Q). Both occur in sympatry over at least part of their
range with L. coronata coronate morph (ESUs O, O′, P and P′)although apparently not with each other. One is endemic to Oman
(L. coronata Oman ESU Q) and the other to the Gulf of Oman
coast of the United Arab Emirates and the Musandam Peninsula,
an exclave of Oman (G. Feulner, pers. comm. 2011) (L. coronata
ophiolite morph ESU N). Both of these localities harbor high lev-
els of endemicity with many other small range endemic species
(e.g., gastropods Trochita dhofarensis and Haliotis mariae, kelp
Ecklonia, Taylor and Smythe 1985; Turbo jonathani, Dekker et al.
1992; parrotfish, Randall and Hoover 1995; Eoacmaea omanen-
sis [as Patelloida], Kirkendale and Meyer 2004; cuttlefish Sepia
pharaonis, Anderson et al. 2010). The Oman endemics occur in a
region of upwelling and may have evolved as a result of the colder
thermal regime (Taylor and Smythe 1985; Randall and Hoover
1995; Kemp 1998; Kirkendale and Meyer 2004) or increased nu-
trients. Alternately, ocean currents may act as a physical barrier
to larval dispersal.
Species tend to range long distances along linear coastlines,
even if their dispersal ability is poor (Valentine and Jablonski
1982, 1983). Range end-points are not randomly distributed, as
might be expected if they were affected by dispersal ability, but
rather cluster at biogeographic boundaries, often corresponding
to a shift in thermal regime or the confluence of water masses
(Valentine and Jablonski 1983). As predicted, the most widely
distributed species is L. coronata coronate morph, which occurs
along the coast of east Africa and the Arabian Peninsula into
India. Other coronata and torquata species also range long dis-
tances with species boundaries most likely set by temperature.
Range limits along the coasts of east Africa, southern Australia,
and southeast Asia also mirror those seen in many other taxa.
The range end point of L. coronata coronate morph in India cor-
responds with an area of low salinity and high turbidity due to
freshwater run-off from river deltas. Species in these groups with
small ranges are L. jungi and L. ogasawarana, which occur only
on islands, and the two Arabian endemics.
Populations within L. coronata coronate morph are not pan-
mictic. Genetic structure within this species suggests that there
are semi-permeable boundaries to gene flow along the Arabian
Peninsula, although not along the east coast of Africa. Population
samples of the L. coronata coronate morph from the Persian Gulf
(ESU O′) have higher spired shells than the African clade (ESU
P and P′) and there is a fixed, albeit polymorphic, difference in
a nuclear gene in Indian and Gulf of Oman populations (ESU
O). All three distinct populations (ESUS, O, O′, and P and P′)co-occur in UAE (in the Gulf of Oman). Likely partial barriers
to gene flow for L. coronata coronate morph are the Persian Gulf
and long stretches of unsuitable habitat between the UAE and
India where long sandy beaches occur, and few rocky headlands.
However, similar patterns have also been observed in other
organisms that do not share the same habitat preferences. For
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SUZANNE WILLIAMS ET AL.
example, the cuttlefish Sepia pharonis species complex includes
several divergent clades, with clades from the Persian Gulf and
Gulf of Oman highly divergent from both central (India and Thai-
land) and western Indian Ocean clades (Red Sea and Gulf of
Aden) (Anderson et al. 2010).
Population structure is also observed in L. torquata, which
was thought by early malacologists to be two species: one found in
western Australia and the other in east Australia. These two forms
are distinct, but intermediates occur in central south Australia.
There are two clades in the COI tree; one corresponding to samples
from western Australia and the other with samples from both
New South Wales (southeast Australia) plus western Australia.
A break has been observed in genetic studies of many temperate
marine taxa between east and west Australia, with the boundary
at the southeast corner of Australia (e.g., Waters et al. 2005; Ayre
et al. 2009; Colgan and Schreiter 2011). This break is thought
to be due in part to a historical barrier to dispersal in the form
of a land bridge between mainland Australia and Tasmania in
the Pleistocene (Dawson 2005). Modern day dispersal may also
be limited by the confluence of two ocean currents and a stretch
of habitat unsuitable for many rocky-shore taxa (Billingham and
Ayre 1996; Ayre et al. 2009). In some species, there are two clear
clades (e.g., Nerita “atramentosa”; Waters et al. 2005), but in L.
torquata there appears to have been gene flow from NSW into
west Australia subsequent to a period of isolation (see also Waters
et al. 2007). Conversely there is no evidence at all of a break across
the same region in L. undulata (see also Ayre et al. 2009 for other
similar examples).
Unlike the torquata and coronata groups, which are dis-
tributed along one-dimensional coastlines, the cinerea group is
distributed on two-dimensional array of islands and continental
shelf segments. Species ranges in this habitat are predicted to
depend upon dispersal ability and habitat preference. In keeping
with this prediction, all species in the cinerea group have small
ranges, consistent with their likely low dispersal ability. Within
the group, the two species found along the coast of Australia have
longer ranges and L. cinerea SW Pacific is likely to have a range
including Solomon Islands (no genetic data), New Caledonia,
Vanuatu, and American Samoa.
Although exact ranges are not known for the species making
up the cinerea group that occur in the central IWP and southwest
Pacific, to date none have been found in sympatry. In fact, all
seven species are allopatric, which is consistent with allopatric
speciation. In island arrays, particularly archipelagos of oceanic
island atolls, allopatric speciation may be common in species
with lower dispersal abilities where dispersal between archipela-
gos may occur stochastically and infrequently (e.g., Paulay and
Meyer 2002; Meyer 2003; Kirkendale and Meyer 2004; Williams
and Reid 2004; Meyer et al. 2005). Species on the periphery with
smaller ranges may also be subject to a higher rate of specia-
tion and extinction (Jablonski and Roy 2002; Jablonski and Hunt
2006).
Broad continental shelf segments (included in two-
dimensional habitats) may also have played an important role in
maintaining regional diversity. During the Quaternary, sea-level
fluctuations were frequent and of great amplitude, with sea level
dropping possibly by as much as 135 m (Peltier 2002; Kuhnt
et al. 2004). The effect of lowered sea level was profound in the
central IWP, where it exposed large expanses of shallow conti-
nental shelf and markedly changed the geography of the region. It
has been suggested that many marine organisms went locally ex-
tinct on the Sunda Shelf (Hoeksema 2007; Bellwood et al. 2011),
northwest Australia (Kuhnt et al. 2004) and from islands in the
west Pacific as a result of habitat loss during periods of lowered
sea level (Paulay 1990). However, the existence of species that
predate Pleistocene glaciations and that are (currently) endemic
to nearshore northwest and central northern Australia (e.g., L.
cinerea NW Australia) suggests that not all species were extir-
pated. Either species survived in pockets of refugia or only partic-
ular habitats were affected. Indeed Paulay (1990) showed that on
island atolls qualitative, not quantitative loss of habitat resulted in
extinction.
TECTONIC PROCESSES
Oceanic–oceanic plate convergence results in subduction of one
plate under the other and in the process a deep trench may be
formed along the plate margin and volcanic arcs are created,
often forming emergent island chains (Hall 2001). These arcs
provide stepping-stones for dispersal (Springer 1982; Hall 2001;
Paulay and Meyer 2002). Dispersal via island arcs is likely to be
of greatest importance in regions that are tectonically active like
Southeast Asia, which has been active throughout the Cenozoic
(Hall 2001, 2002, 2009). Island arcs are likely to appear more
often and be more transient in regions that are tectonically active,
affecting gene flow among populations, as they become either
better connected or more isolated. Because tectonic features can
disappear over very short periods of time (Hall 2001), the loss of
stepping-stones will result in fragmented populations that may fol-
low independent evolutionary trajectories leading to genetically
structured populations and eventually speciation. Alternatively,
emergence of new island chains may reconnect fractured popu-
lations before they have had a chance to speciate or allow the
dispersal of new species back into ancestral habitats.
One possible example of speciation as a result of the loss
of stepping-stones is found in Japan. Lunella granulata, which
occurs on mainland Asia, Taiwan, and in the Okinawa Prefecture
of Japan is sister to L. ogasawarana, an endemic of the Bonin
Islands (known in Japan as the Ogasawara Group; Fig. 6B) some
1000 km south of Tokyo. This sister relationship between the
Bonin Islands and Okinawa is similar to that observed for other
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SPECIATION ON COASTLINES AND ISLAND ARCS IN LUNELLA
Figure 6. Distribution maps for (A) cinerea group and (B) coronata group showing distributions of cryptic taxa based on genetic samples.
Gray shading indicates approximate range of each species complex. Open circles show the location of museum samples examined. Museum
records have not been identified to species. Colored icons indicate ESUs (according to keys in figures). Note that cladograms indicate
BEAST/∗BEAST tree topology, but branch length has no meaning.
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SUZANNE WILLIAMS ET AL.
endemic species (Fukuda 1994, 1995). In a study of a low-
dispersal patellogastropod, Nakano et al. (2009) explained a simi-
lar pattern by suggesting that an ancestral limpet species dispersed
to the Bonin Islands from mainland Japan on the Kuroshio Cur-
rent, possibly with the help of stepping-stones in the form of
islands between Izu and Bonin Islands. They suggested that these
islands became emergent as a result of falling sea levels during
periods of glaciation and/or by tectonic activity, because there
are several sea mounts along the Shitito-Iwojima oceanic ridge.
The loss of these “stepping-stone” islands by further tectonic pro-
cesses or rising sea levels would have resulted in the isolation
and subsequent divergence of the populations on the Ogasawara
Islands (Nakano et al. 2009). Paleogeographic reconstructions
confirm that the Izu-Bonin-Mariana arc was likely to have been
locally and intermittently emergent at sites of volcanic activity
(Hall 2001).
The estimated age of the divergence between L. granulata
and L. ogasawarana is approximately 1.8 Ma (95% HPD: 1.0–
2.7 Ma; Fig. 5). The Bonin Islands formed during the Palaeo-
gene, but emerged above sea level in the Pleistocene (Kaizuka
1977; Imaizumi and Tamura 1984). Molecular clock estimates
for endemic plants (Ito and Ono 1990) and other shallow marine
gastropods (limpets, Nakano et al. 2009) are also consistent with
Plio–Pleistocene origins.
One of the most important tectonic events in the IWP during
the Oligo-Miocene was the collision of the Australia and New
Guinea plate with the southeast extremity of the Eurasian plate
and the Philippines-Halmahera-New Guinea arc system approxi-
mately 25 Ma (Hall 1998). Molecular and fossil evidence suggests
that this was followed by a period of rapid diversification of zoox-
anthellate corals and associated shallow-water faunas between 20
Ma and 25 Ma (Kohn 1990; Wilson and Rosen 1998; Barber and
Bellwood 2005; Read et al. 2006; Alfaro et al. 2007; Alfaro et al.
2007, 2009; Williams 2007; Williams and Duda 2008; Renema
et al. 2008; Frey and Vermeij 2008; Bellwood et al. 2011). How-
ever, although clades of this age were identified in Lunella (e.g.,
cinerea + coronata groups, 25 Ma; 95% HPD: 20.2–29.7 Ma), no
statistical evidence of increased cladogenesis was observed in this
group, or in a previous study of mangrove snails (Littoraria, Reid
et al. 2010). Moreover, although the rocky-shore genus Echinolit-
torina showed a substantial increase in the rate of cladogenesis,
the increase was statistically nonsignificant (P = 0.07; Williams
and Duda 2008). This suggests that fauna living high in the in-
tertidal zone on rocky shores or mangroves benefited less from
the increase in habitat and the increase in diversity of niches and
trophic resources than reef-associated organisms.
ACKNOWLEDGMENTSWe are grateful to D. Reid, A. Kohn, G. Vermeij, G. Paulay, G. Feulner, M.Hellberg, J. Taylor, B. Marshall, and R. Hall for reading the manuscript
and for thoughtful comments. We also thank G. Feulner, H. Dekker,K. Kreipl, A. Alf, C. Meyer, B. Marshall, P. Lozouet, F. Wesselingh, andG. Paulay for discussions about turbinids; D. Reid, C. Meyer, G. Paulay,F. Naggs, and A. Kohn for interesting discussions about biogeographyof southeast Asia; T. Fujisawa, J. Heled, P. Foster, M. Claremont, and C.Drummond for discussion about analyses; and P. Marko, A. Kohn, andD. Eernisse for an invitation to speak at an AMS symposium that helpedto shape this article. We thank S. Tomida for donating fossil specimensand are grateful to W. Renema for allowing us to use unpublished fossildates. We also thank G. Shimpi and Y. Shouche of National Center ofCell Studies and N. Thakur for sequencing samples from India and J.Llewellyn-Hughes and C. Griffin for operating automated sequencers atthe NHM. We are grateful to the following people for providing samples,access to loan material (of both recent and fossil material) or help withfieldwork: T. Al Abdessalaam (Environment Agency, Abu Dhabi), M.Bemis (UF, Gainesville), P. Bouchet (MNHN, Paris), F. Boneka (USR,Manado), B. Buge (MNHN, Paris), J.-J. Cassan (Department of EconomicDevelopment and Environment, Noumea), B. Chan (AS, Taiwan), M.-H.Chen (KMU, Taiwan), A. Fields (JCU, Townsville), G. Feulner (Dubai,UAE), M. Florence (SI, Washington DC), M. Frey (UC, Davis), J. George(NHM, London), G. Giribet (MCZ, Harvard), E. Glover (NHM, London),T. Haga (University of Tokyo), G. Harasewych (SI, Washington DC), D.Herbert (Natal Museum, Natal), V. Heros (MNHN, Paris), R. Hornby(Nautica Environmental Associates, Abu Dhabi), P. Kendrick (CALM,Dampier), K. Kreipl (Meeresmuseum Oehringen, Germany), J. Liddelow(CALM, Dampier), I. Loch (AM, Sydney), L. Kirkendale (UVic, GreaterVictoria), H. Kinyo (Japan), P. Kuklinski (PAS, Sopot), K. Lam (UHK,Hong Kong), P. Maestrati (MNHN, Paris), M. Malaquias (NHM,London), B. Marshall (Te Papa Tongarewa, Wellington), R. Marwoto(LIPI, Indonesia), C. Meyer (SI, Washington DC), A. Miller (AM, Syd-ney), R. Moolenbeek (ZMA, Amsterdam), C. Muller (CALM, Dampier),T. Nangammbi (Natal Museum, Natal), B. Olivera (University of Utah),M. Pandolfi (Service de l’environnement marin, Noumea), G. Paulay(UF, Gainesville), N. Pilcher (Marine Research Foundation, Sabah), R.Pouwer (Naturalis, Leiden), R. Przeslawski (GA, Canberra), N. Puil-landre (MNHN, Paris), D. Reid (NHM, London), B. Richer de Forges(IRD, Noumea), M. Ruf (Marine Research Foundation, Sabah), A. SaadAl-Cibahy (Environment Agency, Abu Dhabi), N. Saguil (Philippines),T. Shimira (Japan), S. Slack-Smith (WAM, Perth), J. Slapcinsky (UF,Gainesville) T. Tajima (Japan), J. Taylor (NHM, London), K. Tilbrook(AUT, Auckland), J. Todd (NHM, London), G. Walker (NHM, London),M. Wallace (South Africa), T. Waller (SI, Washington DC), F. Wells (Dept.Fish., Perth), F. Wesseling (Naturalis, Leiden), C. Whisson (WAM, Perth),R. Willan (Museum and Art Gallery of the Northern Territory, Darwin), G.Williams (UHK, Hong Kong), P. Williams (Perth, Australia), I. Zagorskis(AIMS, Townsville). This study was supported in part by a grant fromthe Natural Environment Research Council to STW (NE/C507453/1),JSPS to TN (207024). Fieldwork by STW was partially funded by theSystematics Research Fund of the Linnean Society of London and theSystematics Association.
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Associate Editor: M. Hellberg
Supporting InformationThe following supporting information is available for this article:
Table S1. List of taxa used in study. Lunella species in order of clades named in Figure 5, followed by outgroups.
Table S2. Forward (F) and reverse (R) PCR primers (also used in sequencing), and forward (FS) and reverse (RS) internal
sequencing primers.
Supporting Information may be found in the online version of this article.
Please note: Wiley-Blackwell is not responsible for the content or functionality of any supporting information supplied by the
authors. Any queries (other than missing material) should be directed to the corresponding author for the article.
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