Testing geological models of evolution of the Isthmus of Panama in a phylogenetic framework CHRISTINE D. BACON1*, ANDR?S MORA2, WARREN L. WAGNER3 and CARLOS A. JARAMILLO1 1Smithsonian Tropical Research Institute, Balboa, Anc?n, Republic of Panam? 2Instituto Colombiano del Petroleo, Ecopetrol, Piedecuesta, Colombia 3Department of Botany, Smithsonian Institution, MRC-166, PO Box 37012, Washington DC, 20013-7012, USA Received 9 February 2012; revised 28 May 2012; accepted for publication 31 May 2012 The emergence and closure of the Isthmus of Panama had regional and global impacts that were rivalled by few other Cenozoic geological events. The closure of the Central American Seaway and the rise of the Isthmus had dramatic affects on climate and air and oceanic currents worldwide. Formation of the Isthmus also drove terrestrial biotic interchange, ending the isolation of South America by permitting the mixing of its biota with that of North and Central America. A dated phylogenetic tree of a well-sampled clade of palms in the tribe Trachycarpeae (Copernicia, Pritchardia and Washingtonia) was used to conduct biogeographical analyses. Examination of the timing of lineage dispersal from North into South America was performed and two contrasting temporal hypotheses of the Isthmus formation were tested: occurrence in the Pliocene (c. 5 Mya to the present) or in the Miocene (prior to c. 5 Mya). Copernicia is inferred to have dispersed through the Isthmus of Panama region into South America and subsequently into the Caribbean, where it underwent a rapid radiation. Consistent with a geologically older age for the Isthmus than previously understood, our results support recent geological and palaeobiological data that suggest an early Oligocene to early Miocene model of evolution of the Isthmus of Panama. ? 2012 The Linnean Society of London, Botanical Journal of the Linnean Society, 2013, 171, 287?300. ADDITIONAL KEYWORDS: Arecaceae ? biogeography ? Caribbean ? Central American Seaway ? Cuba ? Hawaiian Islands ? Palmae ? phytogeography ? South America. INTRODUCTION The formation of the Isthmus of Panama is consid- ered by physical scientists as one of the most impor- tant geological events in Cenozoic history [last 60 million years (Mya); e.g. Graham, 2010]. The Isthmus is a narrow strip of land that separates the Caribbean Sea from the Pacific Ocean and links North and Central America with South America. The closure of the Central American Seaway (CAS) that separated North and South America stopped the westward pal- aeocurrent and all circulation between the Caribbean Sea and the Pacific Ocean (Collins, Budd & Coates, 1996; Newkirk & Martin, 2009), forcing Caribbean currents northeastward. The formation of the Isthmus had an enormous impact on global climate and, although controversial (Klocker, Prange & Schulz, 2005; Molnar, 2008), the northeastern shift in Caribbean currents has been hypothesized to have played a fundamental role in the onset of Plio- Pleistocene glaciations (Haug & Tiedemann, 1998; Haug et al., 2001; Bartoli et al., 2005). In addition to the climatic and oceanographic effects, the closure of the Isthmus of Panama is also considered to have been a defining event in the bio- geography of the Americas (e.g. Gentry, 1982). New land connections between North and South America ended the ?splendid isolation? of South America (Simpson, 1980) and facilitated the ?Great American Biotic Exchange? (Stehli & Webb, 1985). The fossil record of mammal fauna supports few migrations across the Isthmus before the Late Pliocene and the*Corresponding author. E-mail: christinedbacon@gmail.com bs_bs_banner Botanical Journal of the Linnean Society, 2013, 171, 287?300. With 3 figures ? 2012 The Linnean Society of London, Botanical Journal of the Linnean Society, 2013, 171, 287?300 287 Pleistocene (Simpson, 1980; Stehli & Webb, 1985; Graham, 1992; Burnham & Graham, 1999). For plants, a recent meta-analysis has shown older trans- CAS divergence times, implying a higher propensity for dispersal than animals throughout the geological period of Panamanian assembly (Cody et al., 2010) and/or the presence of a dispersal corridor (approxi- mating tectonic plates or stepping-stone islands between North and South America). The combined processes of plate disassembly and redistribution, together with phases of global warming and cooling, are thought to have afforded plants intermittent dis- persal opportunities that could have contributed to the direction of angiosperm diversification (Morley, 2003). In particular, long-distance dispersal has been demonstrated to be the likely cause of many plant distributions, including those in the Neotropics (e.g. Dick, Abdul-Salim & Bermingham, 2003; Lavin et al., 2004; S?rkinen et al., 2007). Previous studies based on isotopic, geochemical and fossil faunal data from sedimentary strata across the Isthmus of Panama were inferred to indicate a Pliocene emergence and closure of the Isthmus [c. 3 million years ago (Mya); Keigwin, 1978, 1982; Duque- Caro, 1990; Coates et al., 1992, 2004; Collins et al., 1996; Kameo & Sato, 2000; Beu, 2001; Newkirk & Martin, 2009]. However, some of the evidence sup- porting this Pliocene evolution model has alterna- tively been interpreted to show no causal relationship with Isthmus closure because these studies relied on indirect evidence (geochemical, biological records) assumed to be correlated with a Pliocene Isthmus closure (e.g. Molnar, 2008). Indeed, previous results are in contrast with a recently proposed model of Isthmus formation based on new mapping, petro- graphical, geochronological, palaeomagnetic and ther- mochronological data, which infer that the Isthmus of Panama region comprised primarily uplifted terres- trial landscapes above sea level with some shallow sea incursions from the late Eocene (c. 40?34 Mya; Montes et al., 2012a, b) until the early Miocene (c. 23?16 Mya; Farris et al., 2011). This Isthmus chain implies that the likelihood of dispersal between North and South America increased with the initiation of collision between the easternmost tip of the Central American Arc and northwestern South America, and that emergence and closure of the Isthmus are much older than previously recognized (CAS closure at 15 Mya; Montes et al., 2012a). This palaeogeographi- cal configuration also greatly restricted the width of the CAS during the late Oligocene to early Miocene (200-km-wide sea gap at 25 Mya; Farris et al., 2011; Montes et al., 2012a). The integration of phylogenetic, molecular dating and biogeographical methods can also be used to reconstruct the evolutionary history of the Isthmus of Panama, particularly when examining groups that are keystone components of Neotropical forests (e.g. Pennington, Richardson & Lavin, 2006). Palms (Arecaceae) are among the most important and char- acteristic components of tropical forests, particularly in terms of species diversity and abundance of indi- viduals (Kahn & de Granville, 1992; Phillips & Miller, 2002; Dransfield et al., 2008; Eiserhardt et al., 2011a). Over 90% of palm species diversity is restricted to tropical forests because of water- and energy-related variables (Bjorholm et al., 2005; Kreft, Sommer & Barthlott, 2006; Eiserhardt et al., 2011b) and because of fundamental anatomical constraints that inhibit palms from colonizing colder environments (Tomlin- son, 2006). The rich fossil history of Arecaceae dates back to the Cretaceous, and a recent family-wide analysis of divergence times inferred that palms have diversified in the tropical rainforest biome since its mid-Cretaceous origin at northern latitudes (Couvreur, Forest & Baker, 2011). Furthermore, palms are present in the first record of Neotropical forests (late Palaeocene Cerrej?n flora of Colombia; Gomez-Navarro et al., 2009; Wing et al., 2009). Taken together, palms are an excellent study system for understanding the evolutionary history of the Isthmus of Panama. Within the palms, a monophyletic group of three closely related genera of the palm tribe Trachy- carpeae, Copernicia Mart., Pritchardia Seem. & H.Wendl. and Washingtonia H.Wendl., are distributed on both sides of the Isthmus region in North and South America and comprise two explosive island radiations, one in the Caribbean (Cuba and Hispa- niola) and the other in the Pacific (Hawaiian Islands; Fig. 1; Bacon, Baker & Simmons, 2012a; Bacon et al., 2012b). A previous study has suggested that these genera originated from North America and that Copernicia lineages followed the Greater Antilles? Aves Ridge (GAARlandia) land bridge to disperse from the Caribbean to South America (Bacon et al., 2012a). GAARlandia putatively comprised large, closely spaced islands or possibly a continuous peninsula that linked South America to the Greater Antillean Islands in the Eocene?Oligocene transition (35?33 Mya; Iturralde-Vinent & MacPhee, 1999; but see Ali, 2012; Bayona et al., 2012). A GAARlandia dispersal route for Copernicia was proposed because the timing of dispersals predated a Pliocene Isthmus of Panama formation (Bacon et al., 2012a), but the recently proposed geologically older model of Isthmus evolution merits examination as an alternative dis- persal route. Copernicia, Pritchardia and Washingtonia species occur in dry, open savannas, deserts and areas prone to seasonal flooding or, on Pacific islands, in wet windward or dry leeward forests (Dransfield et al., 288 C. D. BACON ET AL. ? 2012 The Linnean Society of London, Botanical Journal of the Linnean Society, 2013, 171, 287?300 2008) and are dispersed by small mammals and birds (Henderson, 2002). Most wrens are insectivorous, but the largest species (Campylorhynchus griseus) nests and forages preferentially on Copernicia tectorum Mart. and, although it has been shown to disperse Copernicia seeds (Rabenold, 1990), dispersal does not occur over long distances because of their nonmigra- tory nature. Washingtonia spp. are also dispersed by nonmigratory birds (Bullock, 1980) and by coyotes (Cornett, 1985). In contrast, Pritchardia spp. disperse across long distances along avian migratory routes of various plovers (Pluvialis spp.) (e.g. Hodel, 2007). These differences in dispersal capabilities, together with the phylogenetic relationships among genera, can be used to test the temporal biogeographical history of the clade in the Neotropics. To inset Copernicia Pritchardia Washingtonia Extant outgroups Cenozoic fossil occurrences Niue Fiji Solomons Hawaii Cook Samoa Australia Pacific Ocean Tonga Distributions North America South America Caribbean Sea Pacific Ocean Isthmus of Panama Figure 1. Map of the palm genera examined. Copernicia is distributed in Argentina, Brazil, Colombia, Cuba, Dominican Republic, Haiti, Paraguay and Venezuela. Pritchardia is distributed in the Cook, Fiji, Hawaiian, Niue, Samoa, Solomon and Tonga Islands. Washingtonia is distributed in the USA and Mexico. The Cenozoic fossil outgroups are based on Sabalites fossil occurrences, which were derived from Read & Hickey (1972), Weber (1978), Harley (2006) and Dransfield et al. (2008). Although the nomenclatural use of Sabalites does not unequivocally associate fossils with any extant genus (e.g. Sabal), it is a good hypothesis of the palaeodistribution of the lineages examined. ISTHMUS OF PANAMA BIOGEOGRAPHY 289 ? 2012 The Linnean Society of London, Botanical Journal of the Linnean Society, 2013, 171, 287?300 In this study, we investigate the origin and diver- sification of Copernicia, Pritchardia and Washingto- nia palms in space and time by estimating speciation events under different biogeographical models. We explore the biogeographical history of Copernicia and the evolution of the Isthmus of Panama by testing whether the timing of lineage dispersal occurred in the Pliocene (5.25 Mya to the present; H1 sensu Keigwin, 1978) or whether it occurred in the Miocene (before 5.25 Mya; H2 sensu Montes et al., 2012a). Elucidation of the timing of formation of the Isthmus has major implications for the timing of biotic inter- change between North and South America, and hence for the elucidation of the diversification history of Copernicia, Pritchardia and Washingtonia. MATERIAL AND METHODS PHYLOGENETIC ANALYSES AND ESTIMATION OF DIVERGENCE TIMES Species of Copernicia, Pritchardia and Washingtonia and three outgroups representing other tribes of Coryphoideae [Fig. 1; Cryosophila stauracantha (Heynh.) R.J.Evans, Phoenix roebelenii O?Brian and Sabal palmetto (Walter) Lodd. ex Schult. & Schult.f.] were sequenced for three plastid and three nuclear genes (Bacon et al., 2012a, b). Eighty per cent of species were sampled, including 13 of the 22 species of Copernicia, one of the two Washingtonia species and all 26 currently recognized species of Pritchardia (Hodel, 2007; Bacon et al., 2012b). Forty-three termi- nals were included in the simultaneous analysis (Kluge, 1989; Nixon & Carpenter, 1996). Preliminary nucleotide alignments were obtained independently for each of the six loci using default parameters in MUSCLE v3.6 (Edgar, 2004) and manually adjusted in MacClade v4.03 (Maddison & Maddison, 2001) following Simmons (2004). Maximum parsimony (MP) tree searches were conducted using 1000 random addition tree bisection?reconnection (TBR) searches in PAUP* v4.0b10 (Swofford, 2001) with a maximum of ten trees held per replicate. Parsimony jackknife (JK) analyses (Farris et al., 1996) were conducted using PAUP* and 1000 replicates were performed with 100 random addition TBR searches per replicate. jModeltest v0.1.1 (Posada, 2008) was used to select the best-fit model of sequence evolution for each data matrix using the Akaike Information Criterion (Akaike, 1974) without considering invariant-site models, following Yang (2006). The data were parti- tioned by locus to allow for variation in substitution models and the analysis was run using the GTR + G model of nucleotide substitution with four rate cat- egories. Three iterations of Markov chain Monte Carlo (MCMC) analysis were conducted with 50 million generations sampled every 1000th generation to estimate the Bayesian topology in BEAST v1.6.2 (Drummond et al., 2006; Drummond & Rambaut, 2007). We estimated the divergence times using an uncorrelated log-normal molecular clock model and the Yule pure birth speciation model. We do not know of any unambiguously identified fossils in Copernicia, Pritchardia or Washingtonia, and we therefore used two secondary calibration points obtained from a family-level analysis based on four primary fossil calibrations (Couvreur et al., 2011). Normally distrib- uted priors have been shown to be most appropriate for modelling secondary calibrations because they reflect the uncertainty in age estimates (Ho, 2007; Ho & Phillips, 2009). Normal distributions for both the stem and crown nodes of Trachycarpeae were esti- mated and the bounds on the prior reflect the 95% credible interval of the constraints. The mean ages were 54 and 34 Mya, respectively, sensu Couvreur et al. (2011), and the standard deviations were set to 6 and 5 Mya, respectively, to capture the variation estimated around the mean (71?38 and 47?23 Mya, respectively, for the stem and crown nodes). The per- formance of the separate analyses (convergence of parameters, effective sample sizes) was assessed in AWTY (Wilgenbusch, Warren & Swofford, 2004; Nylander et al., 2008) and in Tracer v1.5 (Drummond & Rambaut, 2007). ANCESTRAL RANGE RECONSTRUCTION A presence?absence matrix was built representing the distribution of species (Fig. 1) in nine non- overlapping areas that reflect the distributions and endemism of genera, while at the same time minimizing the total number of areas (Sanmart?n & Ronquist, 2004): SU (southern USA: Arizona, California, Florida, Georgia, North and South Carolina); CM (Central America and Mexico); NW (northwestern South America: Colombia and Ven- ezuela); SC (south-central South America: Argentina and Brazil); HA (Hispaniola: Dominican Republic and Haiti); CU (Cuba); SP (south Pacific Islands: Cook, Fiji, Niue, Samoa, Solomon and Tonga); HI (Hawaiian Islands); and AS (Asia: China to Vietnam). Each species was assigned to one or more of the areas on the basis of its known current distribution (Henderson, Galeano & Bernal, 1995; Hodel, 2007). To reconstruct the historical biogeography of line- ages and, in particular, to examine whether Coperni- cia lineages followed a Central American (Isthmus of Panama) or Caribbean (GAARlandia) dispersal route into South America, we analysed an unconstrained matrix in which dispersal among all regions was equally probable using two methods: the Bayesian statistical dispersal?vicariance analysis, as imple- 290 C. D. BACON ET AL. ? 2012 The Linnean Society of London, Botanical Journal of the Linnean Society, 2013, 171, 287?300 mented in Reconstruct Ancestral State in Phylogenies (RASP in S-DIVA; Yu, Harris & He, 2010), and the dispersal?extinction?cladogenesis likelihood model (DEC), as implemented in Lagrange (build 20110117; Ree et al., 2005; Ree & Smith, 2008). To take into account the influence of phylogenetic uncertainty on biogeographical inference, unconstrained ancestral areas were optimized across a random sample of 1000 post-burn-in Bayesian trees from the dating analysis in RASP. Relative frequencies of ancestral areas for each node of the BEAST tree were computed by counting all trees with a certain area uniquely assigned to the node. Results that included the pro- portion of ambiguous reconstructions (< 6% relative probability) across the random sample were then translated into pie charts by importing the estimated relative frequencies from the RASP ?node view? into Excel. We also used the ultrametric tree generated by BEAST to infer ancestral distributions with DEC default parameters employing an unconstrained dis- persal matrix, and compared it with two constrained matrices, to test between alternative models on the formation of the Isthmus of Panama. The constrained matrices corresponded to Pliocene or Miocene palm dispersal and were based on the fact that dispersal probability increases as distance between areas decreases (isolation by distance; e.g. MacArthur & Wilson, 1967). Furthermore, the constraints restricted dispersal between North and South America and the Caribbean and Pacific basins, leaving the Asian and south-central South American biogeographical regions unconstrained. Constraints were defined by the mean of the age ranges of the two hypotheses: 5.25 Mya for the H1 Pliocene model (mean of 7.0 and 3.5 Mya) and 21.5 Mya for the Miocene H2 model [mean of 35 and 8 Mya; timing of the 200-km CAS gap sensu Farris et al. (2011) and Montes et al. (2012a)]. Differ- ences between models were assessed by direct com- parison of their respective log-likelihoods using the conventional cut-off value of two log-likelihood units following Ree et al. (2005). Palms do not require strict over-land dispersal or, in this case, completion of the Panamanian land bridge, but because of the dispersal capabilities of Copernicia, long-distance over-water events are unlikely. We therefore formed discrete hypotheses to allow for comparison and to emphasize two distinct temporal scenarios of isthmian evolution. Two iterations of hypothesis testing using biogeo- graphical constraints were performed. In the ?strict? analysis, the H1 matrix was constrained to only allow dispersal of palms from North America (SU and CM) across the Isthmus to South America (NW) from 7 to 0 Mya and through the CAS either to the Pacific (SP and HI) or Caribbean basins (CU and HA) from 20.00 to 5.25 Mya. We compared the likelihoods for H1 with H2, where the matrix was constrained to only allow dispersal across the Isthmus between 35 and 8 Mya and through the CAS from 50 to 21.5 Mya. In the ?relaxed? analysis, the H1 matrix allowed for low dispersal (0.25) into South America from 20.00 to 5.25 Mya and the H2 matrix allowed a medium rate of dispersal (0.5) into South America from 7 to 0 Mya. RESULTS PHYLOGENETIC RELATIONSHIPS Phylogenetic analyses of 6843 bp of nuclear and plastid data using parsimony and Bayesian methods were consistent with the maximum likelihood topol- ogy, but differed from the Bayesian topology, pre- sented in Bacon et al. (2012a; figs 2, 4 versus fig. 5) with respect to the placement of Washingtonia. Eleven nodes had relatively poor support values, but they corresponded to lineages within recent and rapid island radiations (Supporting Information, Fig. S1). Each genus was highly supported [posterior probabil- ity (PP) = 1; JK = 100%] as monophyletic, as were major clades within genera, such as South American Copernicia, south-central South American Copernicia, Hispaniolan Copernicia, Cuban Copernicia, south Pacific Pritchardia and Hawaiian Pritchardia. Many of the Pritchardia clades endemic to particular Hawaiian Islands were also resolved as highly sup- ported monophyletic biogeographical groups (PP = 1 for Kaua?i, Maui Nui and Hawaiian clades; Fig. 2). TEMPORAL RANGE EVOLUTION ACROSS THE ISTHMUS OF PANAMA Each of the three iterations of 50 million generations resulted in high effective sample sizes (ESSs) (> 500) and convergence of parameters (?Compare? function in AWTY), and 10% of the sampled trees were subse- quently treated as burn-in and removed. For all four data partitions (plastid, CISP4, CISP5, RPB2), the rate of covariance was centred on zero, which can be interpreted as a lack of evidence for rate autocorre- lation among lineages (Drummond & Rambaut, 2007). The estimated ages of the major clades are given in Table 1. The estimation of ancestral ranges was consistent between likelihood (DEC) and Bayesian (RASP) unconstrained inferences. Relative frequencies from the RASP analysis across the sample of posterior trees (Fig. 2) reconstructed the ancestral area of Copernicia, Pritchardia and Washingtonia as prima- rily distributed in the southern USA, but a few topolo- gies supported a Central America + Mexico ancestral area or a combination of the two regions. The ances- tral area of the Copernicia and Pritchardia clade was ISTHMUS OF PANAMA BIOGEOGRAPHY 291 ? 2012 The Linnean Society of London, Botanical Journal of the Linnean Society, 2013, 171, 287?300 inferred in the southern USA. The area reconstruc- tion suggests that Copernicia subsequently dispersed across the Isthmus of Panama region into northwest- ern South America, with lineages reaching the Car- ibbean only after the colonization of South America. Comparison of H1 and H2 across the two iterations of DEC constrained analyses resulted in four biogeo- graphical scenarios that were within two log- likelihood units of one another (Table 2). The best estimate from the comparison of log-likelihood values was that of a relaxed constraint on a Miocene (H2) colonization of South America across the Isthmus of Panama. This scenario was 0.35 log-likelihood units lower than the unconstrained and 0.22 units lower than the relaxed H1 results. Range evolution infer- ences under the relaxed H2 constraint exhibited less uncertainty in range reconstructions than did the strict or unconstrained models, showing that the relaxed model fit the data better. The likelihood-based and Bayesian biogeographical reconstructions are highly congruent and allow for a most likely hypothesis of lineage diversification and range evolution in Copernicia, Pritchardia and Wash- ingtonia (Fig. 3): the ancestral area of the three palm genera was located in the southern USA (SU) around 33.5 Mya with subsequent divergence of Copernicia and Pritchardia lineages also occurring in SU around 31 Mya. Copernicia dispersed into northwestern South America between 31 and 16.3 Mya, and then to the Caribbean islands between 16.3 and 5.5 Mya, whereas Pritchardia dispersed to the Pacific islands between 31 and 9.1 Mya (Table 1), with both genera Figure 2. Bayesian topology derived from three iterations of a 50-million-generation Markov chain Monte Carlo (MCMC) search. Branch support values for the nodes of interest were all resolved with a Bayesian posterior probability (PP) of 1.0. Nodes of interest that were resolved with less than 100% jackknife (JK) on the maximum parsimony (MP) strict consensus tree are beneath the respective branches, and * indicates relationships that were not present in the strict consensus. Pie charts of the relative frequencies of ancestral ranges at the nodes of interest are derived from 1000 posterior trees in Reconstruct Ancestral State in Phylogenies (RASP) and the grey stars indicate the two calibration points. 292 C. D. BACON ET AL. ? 2012 The Linnean Society of London, Botanical Journal of the Linnean Society, 2013, 171, 287?300 subsequently undergoing rapid radiations in Cuba (17 species at 4.45 Mya; Table 1) and the Hawaiian Islands (23 species at 4.17 Mya), respectively. DISCUSSION Robust molecular age estimates and biogeographical analysis of Copernicia, Pritchardia and Washingtonia were used to examine the likely dispersal route of Copernicia from North to South America and, subse- quently, to infer the timing of palm dispersal and diversification across the Panamanian Isthmus and to the Caribbean and Pacific oceanic basins. Divergence time estimations are consistent with a general pattern of angiosperm colonization of Hawaiian Islands occurring at approximately 5 Mya (~4 Mya in Pritchardia, Table 1; e.g. Baldwin & Sanderson, 1998; Frajman, Eggens & Oxelman, 2009; Bacon et al., 2012a), which has been attributed to the emergence of the extant volcanic islands, and also with the timing of the formation of the distinct components of Cuba into a single island terrain (Pliocene Cuban Coperni- cia radiation; Iturralde-Vinent & MacPhee, 1999; Graham, 2003; MacPhee, Iturralde-Vinent & Gaffney, 2003). Our results support a Copernicia dispersal event from North America via the Isthmus of Panama region into South America. Our results are also consistent with an early Oligocene to early Miocene formation of the Isthmus, which is older than tradi- tionally understood and is further supported by recent geological and palaeobiological data in the proposal of a revised tectonic model of evolution of the Isthmus of Panama. TESTING ALTERNATIVE HYPOTHESES ON THE FORMATION OF THE ISTHMUS OF PANAMA IN TRACHYCARPEAE PALMS After identifying a Copernicia dispersal route through the Isthmus of Panama region, we used a likelihood approach to test two alternative hypotheses. The first hypothesis (H1) was consistent with previous studies showing Pliocene dispersal across the Isthmus (here defined as a mean age of 5.25 Mya; but see Cody et al., 2010). The second hypothesis (H2) tested a revised tectonic model of Isthmus evolution proposed by Farris et al. (2011) and Montes et al. (2012a, b), where land emergence and subsequent formation of the Isthmus of Panama allowed for earlier biotic exchange (late Oligocene to early Miocene; here defined as a mean age of 21.5 Mya). The phylogenetic analysis suggests a biogeographi- cal disjunction between the Caribbean and Pacific basins. Sister groups that are disjunct between the Caribbean and Pacific are apparently rare and have been correlated with the formation of the Isthmus (Namoff et al., 2010), including the effects on global climate and air and oceanic currents. In angiosperms, this disjunction is exemplified in Darwiniothamnus Harling and Erigeron L. (Andrus et al., 2009), Jac- quemontia Choisy (Namoff et al., 2010), Fitchia Hook.f, Oparanthus Sherff, Narvalina Cass. and Selleophytum Urb. (Mort et al., 2008), Siemensia Urb. (Motley, Wurdack & Delprete, 2005), and as found here in Copernicia and Pritchardia. These genera of Trachycarpeae originated in North America between 41 and 25 Mya (Table 1) and lineages dispersed both across the Isthmus of Panama and to Pacific islands. Table 1. Crown and stem node mean and highest posterior density estimations in millions of years ago (Mya) for clades of interest based on two calibration points Clade Stem Crown Mean Upper Lower Mean Upper Lower Pritchardia 31.04 38.98 23.13 9.12 13.26 5.30 South Pacific Pritchardia 9.12 13.26 5.30 7.34 11.02 4.12 Hawaiian Islands Pritchardia 9.12 13.26 5.30 4.17 6.35 2.19 Kaua?i Pritchardia 2.84 4.28 1.55 2.28 3.62 1.09 Maui Nui Pritchardia * * * 1.57 2.63 0.66 Hawai?i Pritchardia * * * 1.43 2.44 0.55 Copernicia 31.04 38.98 23.13 16.34 22.11 10.65 Central-east South America Copernicia 9.66 14.17 5.53 4.99 8.02 2.36 Hispaniola Copernicia 5.55 8.26 3.07 2.33 4.23 0.73 Cuban Copernicia 5.55 8.26 3.07 4.45 6.68 2.49 Copernicia + Pritchardia 33.49 41.65 25.54 31.04 38.98 23.13 Copernicia + Pritchardia + Washingtonia 49.80 60.50 39.28 33.49 41.65 25.54 *Nodes supported by posterior probabilities lower than 0.50. ISTHMUS OF PANAMA BIOGEOGRAPHY 293 ? 2012 The Linnean Society of London, Botanical Journal of the Linnean Society, 2013, 171, 287?300 The biogeographical disjunction between Copernicia and Pritchardia evolved between 31 and 9.1 Mya and implies long-distance dispersal of Pritchardia by migratory birds from North America to the Hawaiian Islands and therefore may be unrelated to Isthmus formation, but this temporal framework corresponds to increased constriction of the CAS as inferred from geological and palaeobiological data (early Oligocene to early Miocene; Montes et al., 2012b). CAS closure not only rerouted air and west to east oceanic currents (Collins et al., 1996), but potentially avian migratory (and palm dispersal) routes by forming emergent terrestrial proto-isthmus breeding and feeding grounds that mitigated against further dispersal. Our results from divergence time and ancestral range reconstructions are consistent with an early Oligocene to early Miocene model of evolution for the Isthmus of Panama. In this model, dispersal between North and South America (Table 2) occurred between 31 and 16.3 Mya. Considering these scenarios in rela- tion to current species richness, it is striking that the North American ancestor lineage apparently did not diversify in a continental setting. Two Washingtonia spp. and three non-Caribbean Copernicia spp. gave rise to much more diverse island lineages: 19 Carib- bean island Copernicia spp. and 26 South Pacific island Pritchardia spp. The lack of continental diver- sification is interesting given that there was no dispersal barrier into newly available South American niches, as seen by Copernicia lineages that apparently failed to diversify after colonizing north- western South America by at least 16 Mya, unlike other angiosperms [e.g. Guatteria Ruiz & Pav. (Erkens Table 2. Constraints implemented in dispersal?extinction?cladogenesis likelihood model (DEC) analyses to test between the alternative models of Isthmus of Panama formation H1 H2 NW SP HI HA CU NW SP HI HA CU Strict 0?5.25 Mya SU 1 0 0 0 0 0 0 0 0 0 CM 1 0 0 0 0 0 0 0 0 0 5.25?21.5 Mya SU 0 1 1 1 1 1 0 0 0 0 CM 0 1 1 1 1 1 0 0 0 0 21.5?50 Mya SU 0 0 0 0 0 0 1 1 1 1 CM 0 0 0 0 0 0 1 1 1 1 ?ln L 42.76 42.47 Relaxed 0?5.25 Mya SU 1 0 0 0 0 0.5 0 0 0 0 CM 1 0 0 0 0 0.5 0 0 0 0 5.25?21.5 Mya SU 0.25 1 1 1 1 1 0.25 0.25 0.25 0.25 CM 0.25 1 1 1 1 1 0.25 0.25 0.25 0.25 21.5?50 Mya SU 0 0.5 0.5 0.5 0.5 0 1 1 1 1 CM 0 0.5 0.5 0.5 0.5 0 1 1 1 1 ?ln L 42.54 42.32 All other biogeographical regions not listed in the constraint matrix below were left unconstrained with a dispersal capability of ?1?. The strict analysis reduced dispersal to zero and prohibited movement between two areas during particular time periods, whereas the relaxed analysis reduced dispersal to 0.25 and 0.5 to allow for lower levels of dispersal. Constrained biogeographical areas are abbreviated as southern USA (SU), Central America and Mexico (CM), northwestern South America (NW), south Pacific Islands (SP), Hawaiian Islands (HI), Hispaniola (HA) and Cuba (CU). The three time periods constrained in Lagrange were 5.25 Mya (mean of 7?3.5 Mya sensu Keigwin, 1978), 21.5 Mya (mean of 35?8 Mya sensu Montes et al., 2012a) and 50 Mya (the stem node of the phylogeny estimated). Global maximum likelihood values at the root nodes (as measured by ?ln L) are used to test amongst the two constrained and unconstrained (?ln L of 42.67) likelihood analyses. 294 C. D. BACON ET AL. ? 2012 The Linnean Society of London, Botanical Journal of the Linnean Society, 2013, 171, 287?300 et al., 2007); Inga Mill. (Richardson et al., 2001)] or other groups [e.g. tanager birds (Weir, Bermingham & Schluter, 2009); North American mammals (Kirby, Jones & MacFadden, 2008)]. A REVISED MODEL OF EVOLUTION OF THE ISTHMUS OF PANAMA: ISSUES AND FUTURE PROSPECTS Despite the caveats involved in studies employing secondary calibration and a lack of biogeographical algorithms that take into account rate differences amongst regions in speciation, extinction or range evolution (Goldberg, Lancanster & Ree, 2011), our inferences from phylogenetic, divergence time and biogeographical analyses are consistent with an early Oligocene to early Miocene evolution of the Isthmus of Panama, as suggested previously by Farris et al. (2011). We did not find support for Eocene evolution as proposed by Montes et al. (2012a, b), in these palm lineages, perhaps because estimates based on fossil data can only provide minimum ages (e.g. Ho, 2007). Our data on Copernicia and Pritchardia support a divergence between the two clades showing east?west (31?9.1 Mya) and north?south (31?16 Mya) disjunc- tions, consistent with the idea of an earlier formation of the Isthmus of Panama. These results together with a geologically older formation of the Isthmus of Panama are consistent with other studies on Neotropical palms (Cuenca, Asmussen-Lange & Borchsenius, 2008; Roncal et al., Pacific O cean C aribbean S ea S A N C A 49.8 33.5 31.0 16.3 9.6 5.5 9.1 40.9 Biotic interchange between North and South America 20 Mya 10 Mya40 Mya SU SU SP SC NW SU SU SP NW NW HA 50 40 30 20 10 0 Mya EOCENE OLIGOCENE MIOCENE PLI PLE Figure 3. The most likely hypothesis of biogeographical events and diversification of Caribbean, Pacific, South American (SA) and North and Central American (NCA) lineages. Ancestral nodes are plotted against hypothetical palaeomaps of the Isthmus of Panama, where the shading darkens with the probability of biotic exchange between North and South America. Inferred dispersal events (arrows) and most likely ancestral areas are also indicated at the nodes of interest. HA, Hispaniola; NW, northwestern South America; PLE, Pleistocene; PLI, Pliocene; SC, south-central South America; SP, south Pacific; SU, southern USA. The grey gradient indicates the timing of palm dispersal across the Isthmus of Panama. ISTHMUS OF PANAMA BIOGEOGRAPHY 295 ? 2012 The Linnean Society of London, Botanical Journal of the Linnean Society, 2013, 171, 287?300 2010, 2011, 2012; Bacon et al., 2012a), where disper- sal events from North to South America predate a Pliocene model of Isthmus of Panama formation. Excluding studies that used the Isthmus as a calibra- tion point, which cannot test for the effects of closure, other phylogenetic studies are consistent with a model of Isthmus formation that is older than the Pliocene [e.g. other angiosperms (Cody et al., 2010), freshwater fish (Bermingham & Martin, 1998) and salt-water-intolerant frogs (Weight et al., 2005; Pinto- S?nchez et al., 2012)]. Support for an older early Oligocene to early Miocene model of Isthmus of Panama formation also derives from the palaeobiological record. Land mammal fossil occurrences have been shown to require a continuous land connection of Panama with North America by the early Miocene (Whitmore & Stewart, 1965; Kirby & MacFadden, 2005; Kirby et al., 2008). Fossil benthic foraminifera also indicate an effective biogeographical barrier between Carib- bean and Pacific surface water in the middle to late Miocene (Collins et al., 1996). Furthermore, regional palaeogeographical reconstructions account for a narrow gap, or the complete absence of a gap, between Central America and northwest South America in the Neogene (Wadge & Burke, 1983; Pindell & Kennan, 2009). Despite this evidence, other data remain to be explained, such as the dramatically low mitochondrial rate of mutation required to explain marine geminate sister species formed by a much older Isthmus of Panama vicariant event (e.g. Lessios, 2008). To this end, more dated phylogenetic analysis of Neotropical groups and refined meta- analyses examining biotic interchange in both marine and terrestrial organisms are needed (C. D. Bacon, C. Jaramillo & A. Antonelli, unpubl. data, but see Lessios, 2008; Weir et al., 2009; Cody et al., 2010; Smith & Klicka, 2010). The implications of a geologically older model of the emergence and formation of the Isthmus of Panama are wide ranging and include biological, climatic, oceanic and tectonic factors. Biologically, an early Oligocene to early Miocene (31?16.3 Mya) land con- nection between Central America and South America through the Isthmus of Panama implies that the lack of interchange in land mammals across the Isthmus until the late Pliocene?early Pleistocene may have been the result of a wet and hot climate in northern South America that stalled mammal dispersal until the formation of northern ice sheets and the evolution of savanna-like environments in Panama and north- ern South America (Molnar, 2008; Montes et al., 2012a). In contrast, if a phylogenetic niche conserva- tism hypothesis is asserted, the dispersal of dry- adapted Copernicia palms that are resistant to intermittent flooding may indicate the presence of savanna-type ecosystems at least in the Miocene, but further studies of biotic interchange among charac- teristic savanna species are needed to shed further light on the palaeoenvironment in the region. An early Oligocene to early Miocene Isthmus for- mation and land connection between Central and South America are also significant in the context of mountain building in the Andes. From the central (Oncken et al., 2006) to the northern (Mora et al., 2010) Andes, it has been suggested that deformation reached most of the present-day extension of the modern Andes in the late Oligocene to early Miocene. Farris et al. (2011) suggested the late Oligocene to early Miocene to be an important episode of deforma- tion in Panama. It appears likely that the faster westward South American drift, which is thought to be responsible for orogenesis in the Andes (Silver, Russo & Lithgow-Bertelloni, 1998; Oncken et al., 2006; Mora et al., 2010; Husson, Conrad & Faccenna, 2012), also influenced the late Oligocene to early Miocene closure of the CAS. Our data are robust to these suggestions because the age for Isthmus formation is coeval with important processes in the Andes. The refined inference of the formation of the Isthmus of Panama also has implications for the understanding of Andean biogeography. Previous studies of Andean lineages lacked unique and testable predictions that facilitated such investigations (e.g. Brumfield & Capparella, 1996) because events and processes causing Andean biogeographical and tem- poral patterns were thought to occur at overlapping time intervals (Pleistocene climatic shifts, uplift of the eastern cordillera of the northern Andes and the completion of the Isthmus of Panama; Pennington & Dick, 2010). Our results, together with the new tec- tonic model of evolution in the Isthmus of Panama proposed by Farris et al. (2011) and Montes et al. (2012a, b), allow for the disentanglement of the effects of the Isthmus closure and Pleistocene glacial cycles. ACKNOWLEDGEMENTS We acknowledge financial support from Ecopetrol (?Cronolog?a de la Deformaci?n en las Cuencas Subandinas? Project), the Montgomery Botanical Center, the National Tropical Botanical Garden and the Smithsonian Institution. We thank A. Antonelli for inviting us to submit a paper to this special issue on Neotropical Plant Evolution, T. L. P. Cou- vreur for comments on an early draft, F. Alda, E. Bermingham, D. A. Clague, H. A. Lessios, J. P. Price, J. G. R. Romero, J. Roncal and J. D. C. S?nchez for discussion, and the Associate Editor and two anony- mous reviewers for suggestions that improved the manuscript. 296 C. D. BACON ET AL. ? 2012 The Linnean Society of London, Botanical Journal of the Linnean Society, 2013, 171, 287?300 REFERENCES Akaike H. 1974. A new look at the statistical model identi- fication. IEEE Transactions on Automatic Control 19: 716? 723. Ali JR. 2012. Colonizing the Caribbean: is the GAARlandia land-bridge hypothesis gaining a foothold? Journal of Biogeography 39: 431?433. Andrus N, Tye A, Nesom G, Bogler D, Lewis C, Jaramillo P, Fransisco-Ortega J. 2009. 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