This is the study that, to date, has analyzed the highest number of samples for some mitochondrial genes in some Lyncodontini, such as G. vittata and L. patagonicus. Although the sample sizes are small, they are the largest used for both species to date. In this sense, this work aims to make known to the scientific community the large gaps that exist in the taxonomic, systematic, and evolutionary knowledge of the extant Neotropical Lyncodontini species and aims to stimulate other research groups to obtain many more samples of these species for molecular genetic studies. A limitation of this study has to do with the very small DNA sampling and the fact that this sampling is only of mtDNA, which may make a rather limited contribution to the knowledge of supraspecific relationships in the extant Lyncodontini. However, given a relatively large sampling of G. vittata individuals and the focus on mtDNA, this study’s results are important at the infraspecific level for this species.
4.1. Genetic Diversity and Historical Demographic Changes in G. vittata
Analyzing genetic diversity in G. vittata yielded moderately high estimates of its levels, which is positive from a conservation perspective. It was important to use gene fragments that showed strong variability in their evolutionary rates, as this is crucial for a comprehensive understanding of mitochondrial DNA evolutionary dynamics. The mt12S rRNA marker showed the lowest nucleotide diversity and, in turn, had the lowest rate of evolution per million years (0.42%). The mtNADH5 gene showed considerably higher nucleotide diversity (approximately 10 times higher than that of the previous gene), and its rate of evolution per million years (1.22%) was also three times higher. Finally, the mtD-loop marker showed very high nucleotide diversity (around 1.5 times higher than the nucleotide diversity found in the mtNADH5 gene and about 14 times higher than the nucleotide diversity recorded for the mt12S rRNA gene), also being the marker with the highest evolution rate per million years of the three mt genes employed (4%, more than three times that of the mtNADH5 gene and about 10 times that of the mt12S rRNA gene). Therefore, this study shows the importance of analyzing different mitochondrial genes (even if the fragments are small) with well-differentiated evolution rates to have a more accurate understanding of the overall evolution of mtDNA, as well as to be able to estimate with the greatest possible precision the evolution rates of these markers, which can potentially be used for other phylogenetically close organisms.
The average value for the three mt markers studied in
G. vittata was H
d = 0.67 ± 0.13 and π = 1.03 ± 0.24 in %. These values were considerably higher than those found by Filippini [
79] for
G. cuja in Argentina (H
d = 0.09 and π = 0.15%, 21 specimens sequenced at the mt
NADH5 gene) but lower for H
d compared to two studies with
G. cuja carried out in Brazil. Bornholdt [
16], using 50 concatenated sequences of the mt
NADH5 and mt
Dloop genes for
G. cuja from southeastern (n = 9) and southern Brazil (n = 34) and Argentina (n = 7), estimated 17 different haplotypes with H
d = 0.92 ± 0.02, while Bontempo et al. [
6], using the mt
Cyt-b gene for 28 specimens from east–central Brazil, obtained H
d = 0.90, even though the range considered for
G. vittata was notably larger in the present study (from Guatemala to Bolivia, passing through Colombia, Ecuador, Peru, and French Guiana). Nevertheless, the nucleotide diversity obtained in this study (π = 1.03%) for
G. vittata was like that found for the Brazilian populations in those two studies conducted in Brazil (π = 0.85 ± 0.1% [
16], π = 1.1% [
6], respectively). Considering the area studied in the present research compared to that of the two studies conducted in Brazil (excluding the Argentinian samples), the mt genetic diversity of
G. vittata may appear to be somewhat lower than that of
G. cuja.
Using the marker analyzed with the largest number of
G. vittata specimens, two procedures detected significant evidence of population expansion in female lineages. The mismatch distribution procedure detected the beginning of this population expansion between 370,000 and 635,000 ya. The BSP procedure fully coincided with these time estimates of population expansion for
G. vittata. It detected slow but steady population expansion over the last 0.6–0.5 mya. Around 250,000 ya, this expansion intensified considerably until about 80,000 ya. This period coincides with the last phase of the Bonaerense [
131], from 0.5 to 0.13 mya, and is characterized by a biozone of the giant sloth (†
Megatherium americanum) and a large increase in mammals with Holartic origin in South America (deer and Muridae rodents, for instance). This was a time of stable climate, with a warm and humid environment. This probably caused an expansion of the maternal haplotypes of
G. vittata. From that point, population decline began, becoming particularly pronounced from 40,000 ya onward, reaching its lowest point around 10,000 ya. During the cold period ca. 70,000 ya, large glaciers (Nevados) existed in Colombia and in northern South America [
132]. It was estimated that the temperature was 7 °C lower than today in the Savanah of Bogotá [
133]. From 70,000 to 35,000 ya [
133], there was a period of intense expansion of glaciers. During that period, for instance, approximately 17,108 km
2 of Colombia was covered by glaciers, and the ice reached down to 3000 ± 100 masl, with páramos at ca. 2500 masl. In fact, between 18,000 and 13,000 ya, the paramo that today is located between 3500 and 4500 masl was located at less than 2000 masl [
134]. With the arrival of the Holocene (around 12,000 ya), around that time, new population growth began until about 1000 years ago. In fact, from 14,000 to 11,000 ya, precipitation and temperature increased and glacial retreat occurred. This allowed the formation of a lake (Tauca Lake; 43,000 km
2) in the southern Bolivian Altiplano, which lasted until 11,000 ya [
135]. This extremely cold period (11,000–10,000 ya) was named “El Abra” in the northern Andes, Younger Dryas, or Dryas III, in Scandinavia and northern Europe (12,900–11,700 ya) [
136], or Tardi-glacial in central Europe [
137], being crucial in the extinction of some large mammals, such as Gomphoteriidae (proboscideans), giant sloths, large notoungulates, and the famous
Smilodon. Nonetheless, during a large part of the Holocene, there was an Optimum Climaticum [
138,
139], which occurred especially between 7000 and 3000 ya and was able to help, once again, population expansion of the female lineages of
G. vittata. For instance, in the Savanah of Bogotá, the lake levels have increased in the last 9500–7000 years, and the Andean forests have expanded. At ca. 5000–4500 YA, the level of the Titicaca Lake increased, and, around the 10th century BCE, the temperature increased [
135]. Although there were some periods of drought during the Holocene, these did not appear to negatively affect the size of
G. vittata populations. Finally, a certain decrease in recent centuries has been detected in
G. vittata. It is possible that this population reduction is the result of human hunting as well as climate change. The Little Ice Age (1400–1850 AC) is the most recent period of glacial advance. The ice sheets in Colombia descended on average to 4300 masl (currently, the ice front is ca. 5000 masl). Coinciding with the cooling of the environment, European colonizers arrived in the Andes. With their arrival came the introduction of domestic birds and mammals, as well as a considerable extension of maize and fruit crops in many Andean regions, in addition to habitat fragmentation and hunting the predators that could kill their domestic animals [
140].
Bornholdt [
16], in studying nine specimens of
G. cuja from southeastern Brazil using mt
NADH5, observed a pattern in the MJ network suggesting recent population expansion in southeastern Brazil, with all haplotypes from this Brazilian region differing from each other by a single mutational step and smoothly resembling a star-shaped structure. Similarly, with the concatenated sequences of mt
NADH5 and mt
Dloop, the author found that the Fu’s F
s (= −2.55) and Tajima D (= −0.43) statistics were negative, which is consistent with population expansion, although only the former was statistically significant (
p = 0.04). Conversely, there was no evidence of population expansion for the
G. cuja population in southern Brazil (sample size of 34 specimens for the two previously mentioned mt markers). Furthermore, both statistical measures (Fu’s Fs and Tajima D) for that area of Brazil were positive (F
s = 4.82, and D = 1.9), which may be due to a bottleneck or the existence of several different gene pools in that area of Brazil. Nevertheless, Bornholdt [
16] did not estimate the period or how long ago this population expansion occurred in southeastern Brazil for
G. cuja.
Larger sample sets need to be analyzed to accurately determine how different Pleistocene events of a geological and climatological nature may have affected the population sizes of the three Lyncodontini species.
4.2. Molecular and Morphological Differentiation Between G. vittata and G. cuja and the Taxonomy of the Neotropical Lyncodontini Species
The molecular results obtained here showed that the three species of Lyncodontini (especially between
G. vittata and
G. cuja) can be perfectly differentiated, as previously determined by other authors [
5,
16], even with small fragments of mtDNA. For example, the genetic distances for the mt
NADH5 and
Dloop genes showed high values among these three species (16–19% for mt
NADH5, 6–11% for mt
Dloop), which represents a considerable magnitude of genetic differences that allows for their perfect discrimination. Bornholdt et al. [
5] had already detected considerable differences between the two
Galictis species, around 12.7%, with mt
NADH5. Conversely, the mt
12S rRNA gene detected considerably smaller genetic differences, around 1.8–2.4%, which could be genetic distances between distinct populations or subspecies of a single species. Nonetheless, it should be noted that this latter gene has a considerably lower rate of evolution per million years than the other two genes used in this study. This means that some of the morphological characteristics traditionally used to differentiate these taxa of grisons are truly useful, as we noted in the Introduction. The present molecular study, like those of Bornholdt et al. [
5,
16], shows that the morphological characteristic used by Thomas [
64] does have differential diagnostic value between both taxa.
Bornholdt et al. [
5] also analyzed the sequences of 12 nuclear genes. All of them showed the same situation as the mitochondrial genes, even when analyzed individually. In no case did common alleles appear between the geographic regions corresponding to
G. vittata and
G. cuja; there was reciprocal monophyly among the alleles of the 12 nuclear genes studied. Separate analysis of these 12 nuclear segments showed that both species were differentiated by one mutation (
JAK1 and
MACF1 loci), two mutations (
TRHDE,
AAMP2,
ADORA3,
PFKFB1, and
PTPN4 loci), three mutations (
GNAT1,
APOB, and
RHO1 loci), and up to six different mutations (
RAG1 and
WT1 loci). With the 12 segments of these genes concatenated, strong differentiation between
G. vittata and
G. cuja was also observed. Taking into consideration both mitochondrial and nuclear markers, the separation support for both species was greater than 90%.
It is important to have morphological variables with a phylogenetic signal confirmed by molecular differentiation, as the distribution ranges of G. vittata and G. cuja overlap certain regions of South America. It is also important to highlight that the Bolivian G. vittata specimen that we analyzed in the present study came from the department of Cochabamba, where G. cuja has traditionally been reported. Therefore, it is important to be able to distinguish specimens of both species in sympatric areas in the field.
Our molecular analysis using the mt
NADH5 gene on 13 specimens of
G. vittata (recall that this is the study with the most
G. vittata samples and the largest geographical area analyzed to date using molecular markers for this species) detected three distinct geographic groups. One group consisted of two specimens, one from Central America (Guatemala) and the other from the northern Caribbean region of Colombia (Sucre department). The other group comprised specimens sampled from the rest of South America (the rest of Colombia, Ecuador, Peru, Bolivia, and French Guiana). Within this latter group, the mt
NADH5 marker identified another geographically consistent subgroup. The three specimens sampled in French Guiana formed their own cluster (the mt
12S rRNA marker did not distinguish this last cluster). Therefore, there could be some correspondence between these three groupings and some of the subspecies of
G. vittata that have traditionally been proposed by different zoologists. The first grouping could correspond well with
G. v. canaster. Therefore, the morphological characteristics of this purported subspecies could have taxonomic value (dorsum is purer gray due to its light gray undercoat and guard hairs, with a light gray basal half, broad, black subterminal bands, and small white tips [
141]). Furthermore, this subspecies would reach northern South America (at least northern Colombia). The problem with the two groupings found in South America would be one of taxonomic nomenclature. Schreber [
142], with type locality in Suriname, defined the taxon that is now considered
G. v. vittata. Notwithstanding, Bell [
143], also using Suriname as the type locality, defined another grison species that would give rise to the so-called
G. allamandi, which some authors still considered valid until recently [
21,
22], although most do not take it into account. On the other hand, Jensen and Tarifa [
19] consider
G. allamandi to be a synonym of
G. v. brasiliensis, which is considered restricted to a significant portion of the Brazilian Atlantic coast. If
G. allamandi is indeed a synonym of
G. v. brasiliensis, then the form found in the geographic area of French Guiana could be
G. v. vittata, and those analyzed in Colombia (excluding the one from the Sucre department), Ecuador, Peru, and Bolivia could be related to
G. v. andina. Conversely, if
G. allamandi is not a synonym of
G. v. brasiliensis, then the French Guiana population could be called
G. v. allamandi. For the remaining specimens, the possibility of naming them either
G. v. vittata or
G. v. andina should be considered. If
G. v. vittata and/or
G. v. andina were groupings that could be demonstrated with further molecular analysis involving a larger number of samples and genes, the characteristics of
G. v. vittata, such as having dark brown or yellow-gray with white- or yellow-tipped hairs, or those of
G. v. andina, such as having a dull yellowish stripe on the head and tips of yellowish dorsal hairs, would be diagnostic of those subspecies. We cannot make any inferences about
G. v. brasiliensis because we have not analyzed any samples from the geographic range of that supposed subspecies of
G. v. vittata.
Regarding the taxonomy of
G. cuja, the research of Bornholdt [
16], Bornholdt et al. [
5], and Filippini [
79], as well as the present work, make some interesting contributions from a taxonomic point of view. The Argentine haplotypes could represent the subspecies
G. c. huronax, and the haplotypes from southern and southeastern Brazil could represent the subspecies
G. c. furax. If subsequent studies corroborate the observations of the aforementioned initial studies, the morphological characteristics that could differentiate both putative subspecies and present a real morphological diagnostic feature are a buffy or ochraceous buff in the diagonal stripe and tips of dorsal hairs but a dark central portion of guard hairs that is dark gray and relatively short in
G. c. furax, and very pale-buff or off-white haor in the diagonal stripe and tips of guard hairs and relatively more black in the central portion, giving the dorsum an even darker appearance in
G. c. huronax. Because we do not have genetic results for other possible subspecies of
G. cuja (
G. c. cuja and
G. c. luteola), we cannot make taxonomic inferences about them.
One comment regarding the phylogenetic trees concerns the BI and DT trees with the mt
Dloop marker. This is the only marker used to analyze two specimens of
L. patagonicus. In both analyses, the ancestor of the specimen from the Argentine province of La Pampa appears to have evolved earlier than the ancestor of the specimen from the Argentine province of Patagonia. The same is observed in the corresponding NJ network. This finding could suggest that the less southern form of
L. patagonicus (
L. p. thomasi) might be the original form and that the more southerly form might be a more derived one (
L. p. patagonicus). Moreover, this would coincide with Cabrera’s proposal [
63] of the existence of two subspecies or groups within
L. patagonicus. Nonetheless, molecular studies with many more samples of
L. patagonicus should be carried out to confirm this hypothesis.
In most of the analyses performed (ML and BI trees with the mtNADH5 gene, DT trees with the markers mtNADH5 and mtDloop, and in two out of three MJ networks with the mtNADH5 and Dloop markers), a closer phylogenetic relationship was observed between L. patagonicus and G. cuja than between this last and G. vittata. Other analyses showed the more traditional view of both Galictis species being more closely related to each other than either of them to Lyncodon (ML and BI trees with the mt12S rRNA and mtDloop markers, DT tree with mtD-loop, and the MJ network with mt12S rRNA). If we consider the first analyses mentioned, the taxonomy of G. cuja should show a closer relationship with Lyncodon than with G. vittata. Several alternative hypotheses could be presented. First, if more in-depth molecular studies incorporating a larger number of specimens, especially of Lyncodon, and a wide variety of different genes were to confirm this greater phylogenetic proximity between L. patagonicus and G. cuja, G. cuja would be renamed Lyncodon cuja (Lyncodon is older than Grisonella). Nevertheless, as a second possibility, because the genetic differentiation (at least with the mtNADH5 gene) is of a high magnitude among the three species of Neotropical Ictonychinae (16–18%), perhaps each of them deserves to belong to a different genus: Lyncodon patagonicus, Galictis vittata, and Grisonella (Thomas 1921) cuja. Conversely, if we consider the results of the 12S rRNA gene (1.8–2.4%), we could conclude that the current taxonomy that considers the existence of the two genera, Galictis and Lyncodon, is correct, or even that the three species could belong to a single genus (Galictis). Galictis (Bell 1826) would be chosen because this genus takes precedence over the genus Lyncodon (Gervais 1845). Therefore, a third species, Galictis patagonicus, would be added to the existing species of the genus Galictis, G. vittata, and G. cuja. Although this aspect discussed is speculative, only future research with a larger number of samples from the three species and with a wider variety of genetic markers will be able to more precisely elucidate the taxonomy of the Lyncodontini.
4.3. Tempo in Evolution of Neotropical Ictonychinae Species and in Other Genera of Mustelids
For the three mitochondrial markers studied (
NADH5,
12S rRNA, and
D-loop),
E. barbara was consistently recovered as the most basal lineage of the various mustelid genera studied, with divergence times around 9–13 mya, supporting its evolutionary distancing from the other Neotropical mustelids analyzed. The agreement in the phylogenetic position of this taxon and the proximity of the temporal divergence values of the branch that gave rise to this species among the three mitochondrial markers used reinforce the stability of this relationship, even though each gene showed different rates of evolution per million years. Even using very small fragments of several mitochondrial genes, this result fully agrees with Koepfli et al. [
8,
10], using a much more comprehensive set of genetic data. In the five most comprehensive studies on the molecular phylogeny of mustelids [
8,
10,
11,
12,
15], there are some discrepancies regarding the group to which
E. barbara belongs (Guloninae). Melinae and Guloninae were linked as sister groups in Koepfli et al. [
10], although with weak statistical support. On the other hand, Sato et al. [
12] found that Melinae was either a sister to Mellivorinae or constituted a distinct lineage. Nonetheless, Wolsan and Sato [
11] detected that
E. barbara was the outermost taxon of the Guloninae, which also coincided with Koepfli et al. [
8,
10]. Sato et al. [
12] and Hassanin et al. [
15] did not include any specimens of
E. barbara in their respective studies. Some of these internal branches of the mustelid phylogeny are short, which indicates that mustelids underwent rapid diversification, with six of the eight subfamily clades splitting from one another within a span of about four million years, during the Middle to Late Miocene [
10,
12,
144], as we also found in the present study.
The late Oligocene to early Miocene European
Plesictis is the oldest known stem mustelid, and its oldest known species is
Plesictis plesictis, with the oldest known occurrence of this species dating to 24.7–23.3 mya [
145,
146,
147]. Kollias and Fernández-Morán [
148] estimated the origin of Musteloidea to be approximately 32.4 to 30.9 mya in Asia. During the Miocene, fossils related to the subfamily containing
E. barbara began to appear, which is consistent with the diversification of the mustelid subfamilies during the Miocene, as we observed for the origin of the branch that gave rise to
E. barbara. During the period in which the Guloninae subfamily originated, there was a significant decrease in global temperatures. This cooling period coincides with the formation of a permanent Antarctic ice sheet in the Mid- to Late Miocene and an Arctic ice sheet in the Pliocene [
149]. In addition, several major sea-level low stands occurred during the Late Miocene and Pliocene, including the Serravallian sea-lowering event near the beginning of the Late Miocene, 11–10 mya [
150]. These changes in climate and sea level increased overall terrestrial aridity and seasonality, leading to the disappearance of tropical and subtropical forests and the emergence of a greater proportion of open vegetation habitats (woodlands and grasslands) [
151]. By the early Late Miocene, fossil evidence indicates that the Eurasian continent was a mosaic of vegetation types and generally more heterogeneous in vegetation structure than in earlier periods. These changes in vegetation had a concomitant impact on faunal communities and may have caused diversification within mustelids due to geographic isolation, divergent selection among different habitats, and/or ecological opportunity through the creation of new niches. Changes in habitat and extinction of earlier lineages of mustelids may have created ecological opportunities that enabled the adaptive radiation of modern mustelids. The Guloninae, the branch that directly gave rise to
E. Barbara, may have originated between 7.7 and 6.8 mya [
10]. In a previous study of
E. barbara [
152], it was determined that the temporal differentiation between the population of southern Central America and northern Colombia and the remaining South American population occurred between 6.4 and 4 mya, coinciding with the end of the Miocene and the beginning of the Pliocene. This may indicate that the ancestor of
E. barbara arrived in South America before the definitive closure of the Isthmus of Panama (3.5–2.8 mya), which shows that modern mustelids, like modern procyonids, arrived in South America much earlier than traditionally indicated from a paleontological perspective [
126].
Another difference between the phylogenetic studies of Koepfli et al. [
8,
10], Wolsan and Sato [
11], Sato et al. [
12], and Hassanin et al. [
15] refers to the position of the Mustelinae. Mustelinae was recovered as the sister group to the Lutrinae in Koepfli et al. [
8,
10], while Wolsan and Sato [
11], Sato et al. [
12], and Hassanin et al. [
15] considered Ictonychinae and Lutrinae to be sister groups. This suggests that these clades diversified over a relatively short period of evolutionary time, and this can confound phylogenetic tree topologies because the phylogenetic signal from different DNA sequences is attenuated and often conflicts across such short branches. The results we present here agree perfectly with Koepfli et al. [
8,
10], as Mustelinae and Lutrinae were sister groups in all of the analyses we carried out. Our estimates of temporal genetic divergence between the ancestors of
Neogale and
Lontra ranged from 6 to 9 mya. These values were very similar to those of Koepfli et al. [
8,
10] obtained for the temporal divergence of Mustelinae and Lutrinae (8.7–9 mya) and somewhat lower than those obtained by Sato et al. [
12] (8.9–12.5 mya) although similar to the lower end of the range estimated by Sato et al. [
12] but much lower than the estimate made by Hassanin et al. [
15] between Lutrinae and Mustelinae (16–18.3 mya).
Another major proliferation of mustelid taxa occurred during the Pliocene (5.3–2.8 mya). Genetic studies have revealed this strong second proliferation of mustelid taxa, which generated as many as 20 different lineages representing modern mustelid genera and species originating within a period of less than four million years [
8,
10]. This rapid lineage splitting is one of the hallmarks of adaptive radiation. For mustelids, this diversification was driven by the cooling of global temperatures, the restructuring and redistribution of biomes, and major faunal turnovers across different continents.
This second cycle of global cooling and drying on Earth during the Pliocene coincided with the onset of high-latitude glacial cycles [
149], which resulted in a strong expansion of low-biomass vegetation, including grasslands and steppes at midlatitudes, and the development of taiga at high latitudes in Eurasia, North America, and probably South America [
151]. Associated with this was a significant diversification of muroid rodents and passerine birds that exploited these new habitats, which in turn provided new niches for predators [
153]. Many of the ancestors of modern
Martes and
Mustela species originated because of these processes, as they are specialists in hunting small rodents. King’s [
154] hypothesis suggests that the evolution of small body size in
Mustela (and, as we will argue later, also in the ancestor of
L. patagonicus) was driven by adaptation to exploit abundant resources presented by rodent diversification during the Pliocene, especially rodents that conquered the subsoil and, with them, the mustelid predators that followed to prey on them. Koepfli et al. [
8,
10] note that the diversification of four of the five species within
Martes, all closely associated with taiga forest habitat, coincides with the expansion of this habitat type across the Holarctic during the Plio-Pleistocene. This same phenomenon could have driven the beginning of the diversification of the Lyncodontini in South America, whose oldest extant genus may have been
Lyncodon. This same process of adaptive radiation and diversification in mustelids during the Pliocene has also been detected in Felidae [
155], and Cervidae [
156] at very similar dates.
Koepfli et al. [
8,
10] supported Eurasia as the origin of Ictonychinae, while Sato et al. [
12] favored either Asia (parsimony and ML trees) or Africa (BI tree). Where Ictonychini arose is also uncertain. Sato et al. [
12] favored Asia (parsimony tree) or Africa (BI tree) or that the ancestral range extended on to both continents (ML tree), while the results of Koepfli et al. [
10] are equivocal in this regard. The first occurrence of this clade was represented by the record of
Baranogale helbingi from Podlesice, Poland [
157,
158,
159,
160]. This fossil site is the reference locality of the European Neogene mammal chronological unit MN 14 and has been dated as a biostratigraphic zone that spans 4.9–4.2 mya [
161]. Recently, Marciszak et al. [
162] dated to 3.6–3.2 mya the abundant
B. helbingi material from one of the eight sites in Poland where this fossil species has been found. Like other European ichthyochini,
B. helbingi disappeared during the early Pleistocene. Among the Eurasian fossil taxa of this subfamily, the first to be described were
Enhydrictis and
Pannonictis [
163,
164]. The first genus was recovered from the late Pleistocene deposits of Monte S. Giovanni (Sardinia) and has been named
Enhydrictis galictoides. This form showed a strong affinity with the extant South American Lyncodontini
G. cuja and
G. vittata, even with the Neotropical Guloninae,
E. barbara [
163]. The second genus is well-characterized from the Plio-Pleistocene deposits of central and southern Europe. In fact, it is the best-known and most referenced genus in Eurasia [
165].
Jiangzuo et al. [
166] studied the rich Late Miocene assemblage of mustelids from northern and southern China. The authors differentiated different species,
Cernictis baskini,
Cernictis lufengensis,
Lutravus dianensis, and
Shansictis xinzhouensis.
Lutravus (originally from Asia and also found in North America) and
Shansictis (in a more basal position) were classified within Lyncodontini as the Neotropical
Galictis and
Lyncodon, whereas
Cernictis was found as a basal member of Ictonychini (of Asian origin, but also present in North America). The divergence of the two tribes was likely to have occurred in the Late Miocene of eastern Asia, with the subfamily undergoing rapid intercontinental Asian American dispersals after its initial diversification.
According to the paleontological record, the forms most closely related to the current Neotropical Lyncodontini are the following fossil forms, the earliest originating from North America.
Trigonictis arrived in the New World in the mid-Pliocene and was common in North American Blancan-age deposits [
167], which are dated between 4.9 mya and 1.8 mya.
Trigonictis differs little from the current
Galictis [
168], and two species have been distinguished by paleontologists: a larger
Trigonictis macrodon and a smaller
Trigonictis cookii. Another closely related genus and species of Ictonychinae is
Smithosinus bowleri, which has strong affinity to
Trigonictis and is possibly only a subgenus of the latter. In deposits located in Hagerman, Idaho, this representative of the North American Ictonychinae occurred in marshy habitats and for some paleontologists was possibly the ancestor of
G. cuja [
168,
169]. Some authors suggest that
T. cookii became larger and evolved into
T. macrodon as a chronospecies [
170]. Nevertheless, both
Trigonictis species coexisted in several local faunas [
168]. There has also been debate between the hypotheses that
Trigonictis is either ancestral to
Galictis [
167] or congeneric with
Galictis [
171]. Just as some authors have concluded that
S. bowleri may have been the ancestor of
G. cuja, others have concluded that
T. macrodon may have been the ancestor of
G. vittata, whereas
T. cookii was the ancestor of
G. cuja [
167]. Nonetheless, results using molecular genetic methods can offer a very different perspective on the evolution of Neotropical Lyncodontini. Additionally, the limb bones of
Trigonictis are not as robust as those of
Galictis, the M1 of
Trigonictis is more like that of
Eira, and
Trigonictis is almost equally like
Eira and
Galictis [
168].
Galictis fossils appeared in South America during the Marplatan land mammal age, Vorohuean subage (formerly Uquian land mammal age; 2.5 mya) [
172,
173,
174]. Three taxa of the subgenus
Galictis are known as fossils.
Galictis sorgentinii occurred in the early Pleistocene of Argentina [
172],
Galictis sanandresensis from the San Andres Formation, Argentina, near where
G. sorgentinii was found, and
G. vittata is also known as a fossil [
174]. Other fossil remains, such as
Galictis intermedius (Pleistocene deposits in Minas Gerais, Brazil) and
Galictis allamandi (=
vittata)
fossilis (Brazil), appear to be indistinguishable from the extant
G. vittata [
175]. With reference to
G. cuja, fossils related to this extant species have also been found. This is the case for
Galictis hennigi (subgenus
Grisonella, from Argentina) [
174], the extant
G. cuja [
20], and an unidentified
Galictis mandible (Bolivia) [
176]. Other forms, such as
Galictis major and
Galictis robusta, appear indistinguishable from
G. cuja [
174]. In fact, the aforementioned
G. hennigi from Argentina [
174] is known from a single specimen, and some authors consider it indistinguishable from
G. cuja. The oldest fossil known of
Lyncodon is a skull of
L. bosei [
177] from a site in the Ensenada Formation, Argentina [
178]. This site is dated within a range of 1.07–0.99 mya [
179]. Nevertheless, the oldest taxon of
Galictis obtained in the South American fossil record is the aforementioned
G. sorgentinii [
180]. This fossil is referred to as the Vorohuean subage, and it was dated about 3.0–2.4 mya [
180]. Nevertheless, it should not be forgotten that some authors have not been able to differentiate
G. sorgentinii from
G. cuja.
The study by Koepfli et al. [
10] estimated the origin of Ictonychinae at 7.9–8.2 mya, while these figures were somewhat higher in the study by Sato et al. [
12], reaching 9–9.5 mya. Our work could not provide estimates in this regard, as we did not study Ictonychinae from Asia or Africa. Notwithstanding, comparing our estimates of temporal divergence among Neotropical Lyncodontini taxa with those obtained by the two aforementioned studies do provide interesting insights into the evolution of this group of mustelids in Central and South America. The extreme values found for the divergence of the ancestors of
Lyncodon and
Galictis in [
12] were between 2.4 and 3.8 mya ([
10] did not include
Lyncodon in its analysis). Our average time estimate was 4.8 mya, with extreme values between 2.7 and 6.9 mya, considerably higher than the previously discussed estimate [
12]. That is, our estimates identified the divergence of
Lyncodon and
Galictis primarily during the early Pliocene. Nonetheless, 5 mya ago, the Isthmus of Panama had not yet definitively closed (2.8–3.5 mya, [
181,
182]), which creates a dilemma that we will attempt to resolve in the next section. The presumed time split between
G. vittata and
G. cuja ranges from 2.8–3.0 mya [
10] to 1.2–2.9 mya [
12]. Bornholdt et al. [
5] estimated that the differentiation based on the nuclear genes they analyzed was consistent with the estimate of divergence time between
G. cuja and
G. vittata, around 2 to 3 mya. Our average estimate of the temporal split between
G. vittata and
G. cuja was 3.4 mya, with extreme values between 1.4 and 6.9 mya, slightly higher than previous temporal estimates but with considerable overlap. Therefore, there appears to be agreement between the temporal divergence estimates between
G. vittata and
G. cuja obtained in previous studies and the estimates presented here. The split between the two species would have occurred in the late Pliocene or early Pleistocene.
4.4. Mode of Evolution of Neotropical Ictonychinae Species
The traditional view of when and how the ancestors of present-day grisons arrived in South America is as follows [
5,
79]. The fossil record indicates that Lyncodontini probably originated in North America, descending from a common ancestor, the Pliocene genus
Trigonictis [
170]. Representatives of the genus
Galictis then colonized South America during the Great American Biotic Interchange (GABI) [
183] (the time of divergence among grisons was around 2.5–2.8 mya, during the second and largest wave of mustelid diversification in the Pliocene), through the complete emergence of the Isthmus of Panama [
12,
172], which provided a land bridge for the exchange of fauna between North and South America. The first fossil record of
Galictis in South America appeared in Argentina in the Vorohuean subage of the late Pliocene [
171,
183,
184], dated at 3.0–2.5 mya. Therefore, several North American ancestors of
Galictis (paleontological view) or a single
Galictis ancestor (molecular view) invaded South America via the Panamanian isthmus early during the GABI [
183,
184], soon afterwards giving rise to the two extant species, as well as additional extinct members of the genus [
171]. The traditional interpretation that current mustelid taxa in South America are largely descended from North American species that arrived as part of the GABI following the rise of the Panamanian isthmus is repeated time and again [
10,
12]. Undoubtedly, there are cases that fit this interpretation well. For example, this relationship is clearly indicated for the clade of New World otters, in which
L. canadensis is a sister to
L. felina and
L. longicaudis, with the latter two species found in the Neotropics. Their corresponding split is estimated to have occurred 2.8–3.4 mya (95% HPD: 1.6–5.2 mya), which overlaps well with the timing of the formation of the Panamanian land bridge [
10]. Nevertheless, the case of the Neotropical Lyncodontini may have been very different.
Our new results could allow us to hypothesize a different colonization route by the ancestors of present-day Neotropical Lyncodontini. All of the phylogenetic trees obtained, but especially the three haplotype networks (MJ networks), showed that, assuming the haplotypes of the ancestor of E. barbara were the first to diverge among the mustelids studied, the haplotypes of L. patagonicus were the first to appear, followed by those of G. cuja, and finally by those of G. vittata (in fact, in several analyses, the haplotypes of G. cuja are closer to those of L. patagonicus than those of G. vittata, with the taxonomic implications discussed above). Similarly, the DT trees showed, for the three mt markers, that the branches for L. patagonicus (first) and for G. cuja are denser and deeper than those for G. vittata, which would appear to be a more recent species. This would imply that the evolution and speciation of modern Neotropical Lyncodontini originated in southern South America (the Argentine Pampas and Patagonia, L. patagonicus), passing through north–central Argentina, southern and southeastern–central Brazil, Bolivia, and southern Peru (G. cuja), and more recently giving rise to G. vittata in what is now north–central Peru, Ecuador, Colombia, and Central America (with the populations in the latter area being the most recent). Furthermore, this process would have begun in South America at the end of the Miocene and the beginning of the Pliocene, well before the definitive closure of the Isthmus of Panama (2.8–3.5 mya). This hypothesis would significantly alter the traditional paleontological and molecular view on the matter. This hypothesis is based on the following points.
(1) The traditional viewpoint has been that the GABI occurred throughout the development of an overland corridor across the Panamanian region and that this ended around 3.0 mya. Nonetheless, it was already known by paleontologists that there was limited exchange of taxa in both directions prior to this time and prior to the development of a well-defined “land bridge,” with the precursors being designated as “New Island Hoppers” [
185] or “heralds” [
171,
186]. Geological and tectonic reconstructions [
187] have shown that the Panamanian region contained a series of islands around 6 mya, with the Central American Seaway largely interrupted by an evolving volcanic arc about 12 mya as the southwestern margin of the Caribbean Plate collided with the South American continent. Apparently, this fostered the entry of the first sloths into North America around 9 mya [
188] and the arrival of the first Holartic mammals into South America (Argentina) approximately 7.3 mya during the Huayquerian (Late Miocene, 9–6.8 mya). They were procyonids of the genera
Cyonasua and
Chapalmalania [
189,
190]. In fact, four taxa of North American origin (proboscideans, tapirids, peccaries, and dromomerycins such as
Suramerix), dating in 9.5 mya to the Amazon Basin from beds putatively older than those reported for both procyonids, have been found. The next immigrants were endemic genera of sigmodontine rodents and a procyonid genus
Parahyaenodon from the Montehermosan Age (6.8–4 mya, Late Miocene–Early Pliocene; [
191,
192]). Many of these taxa were linked to forest environments, and they were not well-adapted for colonizing islands. Therefore, a terrestrial bridge was necessary for these colonization events. All of these events could be related to the development of the Baudo Bridge around 10 mya, which connected northwestern South America to the central area of Panama throughout the cordilleras of San Blas and Baudo [
193]. They could also be linked to the closure of the Central American Sea Channel, which happened around 10 mya [
194,
195]. Recently, Wolsan and Sato [
62] proposed a very interesting hypothesis. These authors showed that previously examined carnivoran species that include tetrapods in their diets possess functional
TAS1R1–
TAS1R3 genes due to the presence of substances such as purine 5′-monophosphate ribonucleotides, which are the main agonists of
TAS1R1–TAS1R3 genes in carnivorans. Nonfunctional
TAS1R1–TAS1R3 genes have previously been found only in carnivoran species specialized in feeding on fish, aquatic mollusks, and aquatic invertebrates. This is expected, as purine 5′-monophosphate ribonucleotides are relatively scarce in tissues of living or recently dead fish and aquatic invertebrates. Wolsan and Sato [
62] demonstrated that
L. patagonicus and
G. cuja are exceptional among carnivorans in that they possess a nonfunctional
TAS1R1–TAS1R3 genes despite their diets high in umami-taste-eliciting compounds, including purine 5′-monophosphate ribonucleotides. The results of the study indicated that the lack of
TAS1R1–TAS1R3 gene function in these Lyncodontini is a remnant of their common ancestor that lived within a time interval of around 3 to 9.5 mya as part of the Lyncodontini’s stem lineage. Because loss of taste receptor function is achieved through a stochastic process that continues over evolutionary time, Wolsan and Sato’s [
62] hypothesis claimed a prolonged semi-aquatic episode in the evolutionary history of the Lyncodontini’s stem lineage. In fact,
Lutravus (7.5 mya) [
166] exhibits otter-like dentition suggestive of otter-like feeding habits and habitat (which would support the phylogenies of Wolsan and Sato [
11], Sato et al. [
12], and Hassanin et al. [
15] versus the phylogeny of Koepfli et al. [
8,
10] in reference to the relationship between Ictonychinae and Lutrinae). If some of the ancestors of modern Lyncodontini maintained their aquatic habits, this would have greatly favored the colonization of South America by this group long before the definitive closure of the Isthmus of Panama. Therefore, either as “New Island Hoppers” or via the land bridges that existed during the late Miocene, the ancestors of present-day Neotropical Lyncodontini were able to reach South America before the definitive closure of the Isthmus of Panama (2.8–3.5 mya). This latter fact has greatly influenced the interpretation, even with molecular data, of when the ancestors of present-day Lyncodontini arrived in South America [
5,
12]. Just as with procyonids, such as
Nasua and
Procyon, which were thought to have entered South America during GABI 4 (0.125 mya [
183]) and in recent years have been molecularly demonstrated to have developed in situ in northwestern South America well before the definitive closure of the Isthmus of Panama (10–13 mya) [
158,
196], something similar appears to have occurred with mustelids, and at least the evolution of Lyncodontini seems to have taken place in situ in South America from the late Miocene and early Pliocene. It had also been shown that the ancestors of the modern
E. barbara may have arrived in South America between 6.4 and 4 mya [
152]. Therefore, the arrival of the ancestors of present-day Neotropical Lyncodontini around 5–6 mya should not be viewed with surprise.
(2) The oldest surviving branch of the Neotropical Lyncodontini is that of
L. patagonicus. This means that the earliest forms related to the current
L. patagonicus, which is highly adapted to the semi-desert climate of what is now Patagonia, and with an increasing number of small, subterranean prey (especially rodents), adapted their morphology to the ecology of these rodents. Recall that many genera of sigmodontine rodents appear in the South American fossil record at that time (6.8–4 mya, Late Miocene–Early Pliocene; [
192]). Just as in the Northern Hemisphere, with the formation of steppes (taiga, tundra) due to the cold, dry climate that caused much of the water on Earth to be frozen, allowing for the rapid and prolific adaptive radiation of
Martes and
Mustela (the latter with very small bodies for capturing prey underground) due to the proliferation of small mammals and birds [
10], South America also underwent these events. For example, the first camelids in South America (represented by the endemic genus
Lama) were recorded around 4.2–4.0 mya (Pliocene) [
197]. If camelids well-adapted to the savanna environment already existed in South America at that time, it is because savannas already existed because of cooling and desertification of much of South America due to the planetary cooling that occurred at the end of the Miocene and during much of the Pliocene.
Our hypothesis is strongly supported by several morphological studies conducted by various authors. Law [
198] showed that the expansion of grasslands and diversification of rodents and lagomorphs during the Middle to Late Miocene led to increased clade carrying capacity within extant mustelids, particularly Mustelinae, Lutrinae, and Ictonychinae. To reach these conclusions, Law [
198] analyzed an important morphological dataset that incorporates cranial shape, body size, and body shape to understand phenotypic evolution in a clade of extant small-sized predators, finding that within extant mustelid sub-clades (particularly Ictonychinae, Mustelinae, and Lutrinae), evolutionary shifts towards more robust crania, small body sizes, and elongated bodies all occurred during the Mid-Miocene Climate Transition, around 15.97–11.61 mya, a period of time characterized by arid climates, open habitat expansions, and rodent and lagomorph diversification, as we previously explained. Shortening the rostrum and broadening the mastoid and zygomatic arch breadth are often associated with increases in relative bite forces. Therefore, an evolutionary shift towards these broader cranial shapes favoring larger jaw muscle attachment areas may counteract the weaker bite forces associated with smaller body sizes. Concurrent shifts towards smaller, more elongated body plans would enable these mustelids to actively chase prey down into burrows or crevices, as is the case with the extant
L. patagonicus, and their relatively large bite forces for their smaller sizes would facilitate the successful dispatch of prey that can be up to 10 times larger than many mustelids.
During the Late Pleistocene and the Holocene,
L. patagonicus occurred in eastern portions of Buenos Aires province, where it is now absent [
56]. This geographic occurrence was related to the existence of more arid climates in these areas compared to present times [
56,
199]. In the Late Holocene, the species was also present on the Chilean side of Isla Grande de Tierra del Fuego [
200] and is the only known mustelid that reached this island. Nonetheless, as aridity decreased and the climate became more humid, the geographic range of
Lyncodon diminished, which suggests that during the cold, dry, and arid periods of South America during the Miocene and Pliocene, the ancestors of this genus were able to thrive.
Considering that a good part of the analyses carried out (genetic distances for the mt
NADH5 and
Dloop markers, DT trees, and the three MJ networks) show a tendency towards a greater relationship between the sequences of
L. patagonicus with
G. cuja than of the latter with
G. vittata, our hypothesis maintains that the next ancestor to appear after that of
L. patagonicus was that of
G. cuja. As the climate became more humid and semi-desert and steppe zones receded, an ancestor of the branch that gave rise to
L. patagonicus began to colonize more northerly zones, dry and partially humid forests, and steppes at varying altitudes. This coincided with an increase in prey variety, leading to a corresponding increase in size and resulting in the somewhat larger body of present-day
G. cuja. This species occurs in multiple habitats from sea level to 4200 masl. It may be abundant in open habitats [
23,
35]. Therefore, this grison colonized more diverse environments (with a greater variety of prey) than the direct ancestor of
L. patagonicus, resulting in a selective process that favored increased body size due to the availability of more diverse and larger prey. Some authors have postulated that different climatic conditions affect the body and cranial size of different populations of
G. cuja living in different environments [
7]. In fact, Miglioni et al. [
7] indicated the significant association between skull size and latitude, following the predictions of Bergmann’s rule [
201]. This rule establishes that within endothermic species, specimens from colder climates or higher latitudes are generally larger than those from warmer regions or lower latitudes. Notwithstanding, we do not believe that Bermann’s rule, nor directly the climatological conditions, are what directed the evolution of body size in Neotropical Lyncodontini from southern South America to northern South America, as we will discuss below.
Finally, during its northward colonization, this lineage penetrated humid forests where the variety, quantity, and size of prey increased, as did the number of competing predators. Consequently, its size increased, giving rise to the present-day
G. vittata. This view aligns with the assertion by Koepfli et al. [
10] that mustelids display such substantial ecomorphological diversity within one family that they provide a striking example of the rapid diversification of species into different ecological niches from a common ancestor (adaptive radiation). In the case of
G. vittata, it is a species often found near rivers, streams, and wetlands, from sea level to 1500 masl, but mostly below 500 masl [
26]. In some countries,
G. vittata and
G. cuja coincide, but they do so in different biomes or ecoregions [
202]. For example,
G. vittata in Peru seems to occur in the broad region of the Peruvian Amazon but not in the Peruvian Andes or the drier region of the Pacific coast. In contrast,
G. cuja inhabits the southern Peruvian Andes in the montane grassland and scrublands (Puna grasslands) region. In Bolivia, the only record of
G. vittata originates from the Tropical and Subtropical Dry Broadleaf Forest (Chiquitano), whereas those for
G. cuja include this same biome as well as other Bolivian Andean regions. In Paraguay, both species seem to co-exist in the Tropical and Subtropical Moist Broadleaf Forests (Atlantic Forest) in the southern region of the country, although
G. cuja also occurs in the Savanna (Chaco). Within Brazil, there seems to exist a clear biogeographical division between the species, with
G. vittata exclusively present in the Amazon basin and
G. cuja occurring in other biomes, including the drier Cerrado (savanna) and Caatinga (deserts and xeric shrublands) of the northeast, as well as the Atlantic Forest throughout the eastern seaboard and the pampas grasslands towards southern Brazil. Therefore,
G. vittata is much more actively linked to humid forest environments than the other two Neotropical Ictonychinae species. Bonrnholdt et al. [
5] examined a total of 67 specimens of
G. vittata, whose identification was confirmed based on morphological characteristics, and they did not find evidence corroborating the occurrence of
G. vittata in northeastern, southeastern, or southern Brazil. Likewise, these authors observed that the northernmost limit of
G. vittata is the Mexican provinces of San Luis Potosi and Veracruz. This region is the boundary between humid and semi-humid forests in southern Mexico to drier and more open regions in northern Mexico (where
G. vittata seems not to be found). This is an interesting distributional pattern because it is very similar to that observed in the southernmost limits of the species.
When two morphologically and/or ecologically similar species geographically overlap, a change in size or morphology is expected to minimize competition. Both species may have competed for resources at the boundary of their ranges, which would inhibit pervasive geographical overlap [
203]. This could have occurred when the lineage that gave rise to
C. cuja began to diverge into the lineage that would expand further north, becoming
G. vittata. It is possible that the earlier geographical distribution of both species overlapped more than it does today. The fossil records of both species already occurred in Lagoa Santa in the Brazilian Cerrado biome [
204]. Likewise, there are fossil remains of
G. cuja in Pleistocene deposits in the northern Cerrado, at Aurora, in the state of Tocantins, bordering the Amazon. These data show that the extant southern South American distribution of
G. cuja and the northern South American distribution of
G. vittata may have been more sympatric than they are today and that their contact area may have varied more recently due to climate change [
204].
Another hypothesis that could be key to understanding the body size variation from south to north in the Neotropics is that proposed by McNab [
205], known as the “resource rule.” This rule states that spatial variation in mammal body size can be explained by the availability and characteristics of the resources consumed. Mustelids have higher energy needs than expected for their body mass, which may require a larger prey size to satisfy their energetic requirements [
205]. For example,
G. cuja feeds on rabbits in Argentina and is significantly larger than specimens from southern Brazil, which feed exclusively on small rodents, despite the high abundance of
Lepus europaeus in the region [
206], where there is no evidence of its consumption. The number and size of species are greater in the tropical areas inhabited by
G. vittata than in the regions inhabited by
G. cuja, which could have selected for a larger body size, as could the presence of the metaconid in the lower carnassial, which might help in chewing larger pieces of prey. Notwithstanding, this hypothesis can be combined with another, according to which the size difference among the three extant Neotropical Lyncodontini species is mostly influenced by trophic competition with other living or extinct mustelids and not directly among themselves. Among the extinct taxa that might have driven such size evolution are other species of the genus
Galictis, whose presence is well-known in the South American fossil record [
171,
189]. The concurrent existence of these congeneric species throughout the late Pliocene and Pleistocene may support the hypothesis that they played a competitive role in shaping the size of the extant Neotropical Lyncodontini species, just as other competing carnivores such as other Mustelidae (
E. barbara, for instance), Felidae, and Canidae may have done [
207]. Additionally,
G. cuja occupies savannas, steppes, rocky areas, and forests, and its adaptation to different habitats might have led to its observed variation in coat color, which is greater than that found in
G. vittata. Furthermore, this species often reaches high altitudes and latitudes, which may have historically led to selective pressures for denser fur. The situation of
G. vittata is different, as it exhibits a more homogeneous coloration. The mixture of black and white fur, producing a pale gray coat, might be favored in dense vegetation and darker landscapes, such as tropical forests, where
G. vittata lives. This would allow it to remain less conspicuous to its prey and avoid larger and more competitive predators. Additionally, the shorter and sparser fur in this species is likely an adaptation to the warm temperatures prevalent throughout its geographical range [
5]. Therefore, our knowledge of the biogeographical distribution and morphological evolution of Neotropical Lyncodontini can be reconciled with the molecular results obtained to propose the hypothesis of a southern-to-northern South American evolution of present-day Neotropical Lyncodontini species.
(3) Although there are few genetic population studies with Neotropical Lyncodontini, they can provide some data favorable to the hypothesis presented here. When we compare the genetic diversity values (no data exist for
L. patagonicus) between
G. cuja and
G. vittata, we observe that the H
d values for
G. cuja in different areas of Brazil are higher [H
d = 0.92 in southern (Rio Grande do Sul, Santa Catarina, and Paraná states) and southeastern (Federal District and Brazilian states of São Paulo and Minas Gerais) areas of Brazil [
5] and H
d = 0.90 in the states of Paraíba, Minas Gerais, and Rio de Janeiro [
6]] than those found in the present study for
G. vittata, including Guatemala, Colombia, Ecuador, Peru, Bolivia, and French Guiana (H
d = 0.66). The π values were similar in the three studies (around 1%), but the geographic area considered for
G. vittata was significantly larger, including more biomes, so the π value can be considered proportionally lower in
G. vittata than in
G. cuja. This difference in genetic diversity could be explained by the central–marginal hypothesis [
208,
209]: the central distribution range of a species tends to exhibit higher levels of genetic diversity than the populations located at the periphery of the distribution range. This could indicate that
G. cuja acts more like a central population and
G. vittata more like a peripheral population derived from the former. Similarly, nucleotide and haplotype diversity within these populations from Brazil are different [
5]. Southern Brazil has high values of H
d (0.87 ± 0.03) and moderate values of π (0.99 ± 0.49 in %), while southeastern Brazil has higher H
d (0.92 ± 0.09) but lower π (0.28 ± 0.18 in %). Similarly, the southern Brazilian population historically showed a stable population, while the southeastern Brazilian population showed signs of population expansion [
5]. Although no solid genetic structure exists, the split between the two major
G. cuja groups in Brazil (considering the concatenated data of mt
NADH5 and mt
Dloop) implies at least 15 mutational steps, which is considerably deep, especially considering that it is not geographically localized [
16]. This suggests that the
G. cuja population in southern Brazil is more original and older than that of southeastern Brazil or more northerly areas in central and coastal Brazil, which shows signs of more recent expansion. This aligns well with a south-to-north colonization pattern like the one we propose in this work. Similarly, Bontempo et al. [
6] found that genetic diversity based on the mt
Cyt-b gene identified high haplotypic diversity, although with low nucleotide diversity, suggesting that this population underwent population expansion and confirming the presence of gene flow. Filippini [
79] obtained the same results for the Argentinian and Brazilian data taken together.
G. vittata also showed signs of population expansion, at least for the marker in which the most samples were studied (mt
NADH5), which could be related to its more recent existence. In turn, the mt
NADH5 gene haplotypes of
G. cuja from Argentina (even further south) that we studied appear to have given rise to the haplotypes of southern Brazil (south–north colonization, again). On the other hand, the Argentinian specimens studied, even though they had more original haplotypes, were basically genetically impoverished, exhibiting genetic diversities close to 0 [
16,
79]. Even though the Argentinian population is more ancestral than the Brazilian ones, it may have more recently experienced a bottleneck or may have become extinct, reconstituting itself from very recently acquired populations in southern Brazil that possessed original haplotypes. Another very interesting genetic data point that reinforces our hypothesis of south–north colonization and speciation for Neotropical Lyncodontini is that presented by Bornholdt et al. [
5]. These authors showed a haplotype network with the nuclear
RAG1 gene, where the position of the root was based on two outgroup species (
Poecilogale albinucha and
Ictonyx striatus). The
G. vittata haplotype was derived from a central haplotype of
G. cuja, another genetic indication of south–north colonization and speciation in the Neotropical Lyncodontini.
Of all of the genetic data obtained, only one could introduce doubt regarding the hypothesis we present. The two specimens from Guatemala and northern Colombia (putatively
G. v. canaster) showed in different phylogenetic trees (especially DT trees of the mt
NADH5 and mt
12S rRNA genes and in some MJ networks) that they originated earlier than the remaining South American haplotypes for
G. vittata. This could be consistent with north–south colonization for this species. An alternative hypothesis is that the
L. patagonicus and
G. cuja lineage (but this would require admitting that the genus
Galictis is paraphyletic) arrived in South America first, taking advantage of the early development of prominent Northern Hemisphere glaciations [
183]. This supports the hypothesis of Webb [
210], who proposed that proto-GABI dispersals were aided by the development of Northern Hemisphere glaciations. These promoted the development of savanna-like ecologies in Central America, in contrast to their generally tropical character, and thereby permitted savanna-adapted mammals to cross between North and South America. Already in South America, the ancestor of
L. patagonicus would have given rise to the ancestor of
G. cuja. Meanwhile, in the tropical and forested part of Central America, the ancestor of
G. vittata would have arisen, which more recently penetrated the tropical part of north–central South America. The problem with this alternative hypothesis lies in two points. The first is that not all molecular analyses show the paraphyly of the genus
Galictis, and the second is that all of these processes would have had to occur in the last approximately 2.8 mya, and all our estimates of temporal divergence, in general, exceed those dates. It would be very important to be able to determine the nonsense and frameshift mutations in
TAS1R1 and
TAS1R3 genes in
G. vittata. Depending on the results obtained, it would be possible to support the colonization of Lyncodintini from north to south or from south to north of South America (or the possibility that
L. patagonicus and
G. cuja are more strongly associated with each other, while
G. vittata forms another distinct lineage, and the taxonomic and systematic implications this could have).
The proposed hypotheses can only be considered if much larger genetic datasets can be generated. Here, we have presented a first outline with a very limited number of specimens and genetic markers, intended merely as a small seed for a possible reinterpretation of the colonization and speciation of important South American mammal species. This requires studying a much larger number of specimens for the three Neotropical Lyncodintini species, especially L. patagonicus and G. vittata. Furthermore, the analysis of complete mitogenomes and, if possible, whole metagenomes that effectively represent these three species is necessary.