Extended Y chromosome haplotypes resolve multiple and unique lineages of the Jewish priesthood
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- Hammer, M.F., Behar, D.M., Karafet, T.M. et al. Hum Genet (2009) 126: 707. doi:10.1007/s00439-009-0727-5
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It has been known for over a decade that a majority of men who self report as members of the Jewish priesthood (Cohanim) carry a characteristic Y chromosome haplotype termed the Cohen Modal Haplotype (CMH). The CMH has since been used to trace putative Jewish ancestral origins of various populations. However, the limited number of binary and STR Y chromosome markers used previously did not provide the phylogenetic resolution needed to infer the number of independent paternal lineages that are encompassed within the Cohanim or their coalescence times. Accordingly, we have genotyped 75 binary markers and 12 Y-STRs in a sample of 215 Cohanim from diverse Jewish communities, 1,575 Jewish men from across the range of the Jewish Diaspora, and 2,099 non-Jewish men from the Near East, Europe, Central Asia, and India. While Cohanim from diverse backgrounds carry a total of 21 Y chromosome haplogroups, 5 haplogroups account for 79.5% of Cohanim Y chromosomes. The most frequent Cohanim lineage (46.1%) is marked by the recently reported P58 T->C mutation, which is prevalent in the Near East. Based on genotypes at 12 Y-STRs, we identify an extended CMH on the J-P58* background that predominates in both Ashkenazi and non-Ashkenazi Cohanim and is remarkably absent in non-Jews. The estimated divergence time of this lineage based on 17 STRs is 3,190 ± 1,090 years. Notably, the second most frequent Cohanim lineage (J-M410*, 14.4%) contains an extended modal haplotype that is also limited to Ashkenazi and non-Ashkenazi Cohanim and is estimated to be 4.2 ± 1.3 ky old. These results support the hypothesis of a common origin of the CMH in the Near East well before the dispersion of the Jewish people into separate communities, and indicate that the majority of contemporary Jewish priests descend from a limited number of paternal lineages.
More than a decade ago a characteristic Y chromosome haplotype was found to be associated with the Jewish priesthood, a patrilineal dynasty thought to be founded by the first Jewish priest, the biblical Aaron (Skorecki et al. 1997). The sharing of this Y chromosome lineage between Ashkenazi and non-Ashkenazi Jews pointed to a common origin of the Cohanim before the separation of Jewish communities in the Diaspora. Subsequently, it was shown that ~50% of Cohanim carry a characteristic suite of alleles at six Y-linked STRs, which defined the Cohen Modal Haplotype (CMH). Dating based on variation associated with five of these six Y-STRs suggested that contemporary CMH chromosomes trace to a common ancestral chromosome 2,100–3,250 years ago (Thomas et al. 1998). This time roughly corresponds to the period between the biblical exodus and the destruction of the first temple. However, the small number of Y-STRs typed by Thomas et al. (1998) produced a “low resolution” CMH that was shared among many non-Jewish populations (Arredi et al. 2004; Behar et al. 2004; Bonne-Tamir et al. 2003; Cadenas et al. 2008; Cinnioglu et al. 2004; Nebel et al. 2001; Robino et al. 2008; Shen et al. 2004; Zalloua et al. 2008). Similarly, the few binary markers known at the time did not provide the phylogenetic resolution needed to infer the geographic origin of the CMH lineage. Also left unresolved is the paternal ancestry of Cohanim who do not carry Y chromosomes related to the CMH, leaving open the question of the number of founding lineages of the priesthood.
The recent publication of a revised Y chromosome haplogroup tree comprised of >600 binary markers (Karafet et al. 2008) and the availability of dozens of Y-STRs provides the opportunity to determine the origin(s) of Cohanim lineages with greater phylogenetic and geographic resolution than previously possible (Kayser et al. 2004; Lim et al. 2007; Redd et al. 2002). To further elucidate the paternal ancestry of Jewish priests, we genotype 75 binary markers and 22 Y-STRs in a sample of 122 Ashkenazi and 93 non-Ashkenazi Cohanim, and compare patterns of Y chromosome variation with similar data from 3,459 Jewish and non-Jewish men from the Near East, Europe, Central Asia, and India. We define a 12-locus “extended CMH” and then determine the phylogenetic position and geographic distribution of this lineage. To explore the origin of this and other Cohanim haplogroups, we estimate the ages of Y-STR diversity associated with several key lineages present at frequencies >5% in our sample of Cohanim. Finally, we discuss models for the origin and maintenance of multiple paternal lineages since the founding of the Jewish priesthood.
Subjects and methods
Blood or buccal samples were collected from a total of 3,674 individuals according to procedures approved by the Human Subjects Committees at the University of Arizona, Rambam Medical Center and the National Laboratory for the Genetics of Israeli Populations. Volunteers reported the birthplace of their father, grandfather, and in many cases, great grandfather. Jewish volunteers were also asked to report their affiliation to one of the three Jewish castes, Cohen, Levite, or Israelite. Those who did not know their caste status were classified as “unknown”. Table S1 lists the Jewish population samples genotyped, which were comprised of unrelated Jewish males representing the major Jewish communities across the Jewish Diaspora (n = 1,575), including 215 Cohanim, 738 Israelites, 154 Levites, and 468 of unknown caste status. Table S2 lists our surveyed samples of unrelated non-Jewish men from 30 populations representing Europe, India, the Near East, North Africa, and Central Asia (n = 2,099). We note that many additional markers were genotyped in samples that were previously reported, and that Cohanim samples reported here do not overlap with the original collection of Skorecki et al. (1997) and Thomas et al. (1998).
NRY marker analysis
For the microsatellite analysis, 12 short tandem repeats (Y-STRs): DYS19, DYS385a, DYS385b, DYS388, DYS389I, DYS389II, DYS390, DYS391, DYS392, DYS393, DYS426, and DYS439) were genotyped in 2 multiplex reactions following the protocol of Redd et al. (2002). To allow more accurate coalescence estimates and better comparison ability with published databases the Cohanim samples were genotyped by an additional set of the following ten STRs: DYS437, DYS438, DYS447, DYS448, DYS449, DYS454, DYS455, DYS458, DYS459a and DYS459b. For the duplicated microsatellites DYS385a,b and DYS459a,b, the short and long scores are reported according to allele size (i.e., without confirming that identical scores observed in two different samples represent the same locus). PCR products were electrophoresed on a 3730xl Genetic Analyzer (Applied Biosystems) and fragment lengths were converted to repeat number by the use of allelic ladders. Table S3 lists all 215 Cohanim surveyed here and their allele scores for 22 Y-STRs.
We follow the terminological conventions recommended by the Y Chromosome Consortium (Karafet et al. 2008) for naming NRY chromosomes. Capital letters A-T identify the 20 major NRY haplogroups and are followed by the names of the binary markers used to assign samples to their positions on the NRY phylogeny. When no further downstream markers in the Karafet et al. (2008) NRY phylogeny were typed, we considered the most derived marker to define a haplogroup (Fig. 1). Haplogroups not defined on the basis of a final derived character state represent interior nodes of the tree and are potentially paraphyletic. In these cases, all binary markers that were excluded by our genotyping strategy are noted within parentheses after an initial “x” symbol. We note that all Cohanim J-P58* chromosomes were found to have the ancestral state at the three downstream markers shown in Fig. 1 (i.e., M367, M368, and M369). Therefore, these chromosomes belong to paragroup J-P58(xM367, M368, M369) (or J1e*); however, we refer to this lineage as J-P58* for simplicity. The term haplotype is used to describe any combination of STRs for a given sample.
Compilation and organization of the data was performed using standard Excel files. Median Joining networks were created using the software NETWORK 220.127.116.11 using the following 12 STRs: DYS19, DYS385a, DYS385b, DYS388, DYS389I, DYS389II, DYS390, DYS391, DYS392, DYS393, DYS426, and DYS439. Networks were constructed by the median-joining method (Bandelt et al. 1995). We weighted the STR loci according to their observed variation in our collection of J-P58* Y chromosomes, giving less weight to STRs with higher variance in repeat numbers. To allow maximal resolution we included the duplicated microsatellite DYS385a,b in our network analyses (Niederstatter et al. 2005). While it is possible that identical scores in different samples represent different loci we assume that this potential error is less likely in the case of closely related Cohanim Y chromosomes. We applied the reduced-median algorithm followed by the median-joining algorithm as described at the Fluxus Engineering Web site.
The coalescence times of closely related clusters of haplotypes were estimated using several approaches. First, the age of the Cohanim lineages were calculated as previously reported by Zhivotovsky et al. (2004). The age of STR-variation was computed by averaging across loci the single-locus variances in repeat scores (i.e., with respect to median value at each locus), and then dividing by an average mutation rate of 0.00069 per 25 years. Standard errors were computed across loci as described by Zhivotovsky et al. (2004). The duplicated loci, DYS385ab and DYS459ab, were omitted from the analysis. In addition DYS449 was excluded as it was previously shown to be characterized by multi-repeat variation that substantially differs from all other genotyped STRs (Kayser et al. 2004). We also performed calculations based on a subset of the 17 Y-STRs used in the above analysis. To control for the use of different STRs in our study and that of Zhivotovsky et al. (2004), we calculated divergence times using the same nine Y-STRs in Zhivotovsky et al. (2004): DYS19, DYS388, DYS389I, DYS389II, DYS390, DYS391, DYS392, DYS393, and DYS439. In addition, we used the same five Y-STRs as in the original CMH paper by Thomas et al. (1998): DYS19, DYS390, DYS391, DYS392, and DYS393.
We also estimated coalescence times for key Cohanim lineages by employing the Bayesian Analysis of Trees With Internal Node Generation (BATWING) program of Wilson et al. (2003). To do this within a population genetics framework, we constructed an Ashkenazi population by including our sample of Ashkenazi Israelites and a sub-sample of our Ashkenazi Cohanim to equal 5% of the total population. We used both Y-STR and SNP data to constrain the coalescence of lineages and estimate the TMRCA of individual haplogroups. To estimate the age of a particular Cohanim haplogroup, we excluded non-Cohanim samples carrying this haplogroup (i.e., so that only Cohanim samples carried the particular haplogroup under study). For example, in the case of J-P58*, we included all 317 Ashkenazi Israelite samples that did not carry J-P58*, and a random sample of 17 Cohanim (i.e., which could carry any Y chromosome lineage including J-P58*). We repeated this analysis four times with a different random sample of Cohanim. A phylogenetic tree of binary markers (UEPs) was considered (under option 2) using SNPs that were variable in the Ashkenazi population: M96, M123, P14, M201, M69, P123, M304, M67, P58, M172, M410, M12, M9, M45, M207, M173, M269, M17, and M70. The priors used were: gamma(1.46, 2124) for STR mutation rate, corresponding to a mean of 0.00069 and standard error of 0.00057 as in Zhivotovsky et al. (2004); gamma(1.2, 0.00016) for N, corresponding to a mean ancestral population size of 7,500 and a standard deviation of 6,847; gamma(1.5, 75) for alpha, corresponding to a mean exponential growth rate of 0.02 and a standard deviation of 0.016; and gamma(1.2, 4) for beta, the time of start of expansion (in units of N generations). These priors returned posteriors of the mutation rate that were similar to the prior for mutation rate. A total of 5 × 104 samples of the program’s output were taken after discarding the first 2 × 104 samples as “burn-in”. Convergence was confirmed by finding that results of longer runs (i.e., 105 MCMC cycles) were similar to those of the shorter runs.
Simulations of the decay of paternal lineages
Simulations of the decay of paternal lineages were performed in Matlab using code written for this purpose. The standard constant population size Wright-Fisher model without mutation was used, since only the loss of lineages due to drift was of interest. Each simulation began by assigning the N individuals a number indicating haplogroup membership. In the first set of simulations, each individual was given a unique number representing N distinct founding lineages, while in the second, each individual was randomly assigned to a haplogroup (with the number of haplogroups varying from 2 to 10) (see Supplementary Material). For all initial conditions 10,000 simulations were performed and the results were averaged. Simulations were run for 160 generations corresponding to between 4 and 5,000 years. We note that a bottleneck or founder event would reduce the number of haplogroups faster on average than we see in a population with constant size, whereas the decay of lineages would be slower on average in an expanding population.
We conducted an extended literature search for Cohanim haplotypes identified here, by comparing allelic scores at as many Y-STRs as possible (i.e., that were typed in our study and the published literature). Allele scores at the 12 STRs that we use to define the extended CMH (DYS19, DYS385a, DYS385b, DYS388, DYS389I, DYS389II, DYS390, DYS391, DYS392, DYS393, DYS426, and DYS439) are 14-13-15-16-13-30-23-10-11-12-11-12, respectively (Table S4). The addition of the four STRs DYS437, DYS438, DYS459a, and DYS455 showed no further variation while the addition of DYS459b and DYS454 demonstrated two additional haplotypes that were each comprised of two samples one mutation step away from the extended CMH. The four remaining STRs DYS447, DYS448, DYS449 and DYS458 contained most of the observed variation with 26, 21, 26, and 17.2, respectively, being the most frequent scores observed for these sites. A similar pattern was found for with two relatively frequent haplotypes that are closely related to the extended CMH at 12 Y-STRs (see “Results and Discussion”). A total of 14 out of the possible 17 STRs were compared with the YHRD database: DYS19, DYS385a, DYS385b, DYS389I, DYS389II, DYS390, DYS391, DYS392, DYS393, DYS437, DYS438, DYS439, DYS448 and DYS458. The search yielded zero out of 10,243 matching haplotypes in 66 populations for the extended CMH and its two closely related haplotypes. The same STRs demonstrated no matches when compared to Cadenas et al. (2008). No matches were found when the following 12 STRs were used to the dataset reported by Arredi et al. (2004): DYS19, DYS388, DYS389I, DYS389II, DYS390, DYS391, DYS392, DYS393, DYS426, DYS437, DYS438 and DYS439. Similarly, no matches were found when the following 14 STRs were used to compare with Robino et al. (2008) dataset: DYS19, DYS385, DYS389I, DYS389II, DYS390, DYS391, DYS392, DYS393, DYS437, DYS438, DYS439, DYS448, DYS458. Two matches were found when the following nine STRs were screened in Cinnioglu et al. (2004): DYS19, DYS388, DYS389I, DYS389II, DYS390, DYS391, DYS392, DYS393 and DYS439; one of which was J1-M369 and the second was J1-M267(xM369). Three Lebanese samples from Zalloua et al. (2008), defined as J-M304(xM172) matched the extended CMH or its two closely related haplotypes when the following 11 STRs were compared: DYS19, DYS388, DYS389I, DYS389II, DYS390, DYS391, DYS392, DYS393, DYS437, DYS438, DYS439. In a recent survey of Hg J-M267, only five of the 282 J-M267 samples studied fell within J-P58; all of these were M367 positive and did not fit within the J-P58* lineage found among our Cohanim sample (Tofanelli et al. 2009). We compared the following 15 STRs overlapping between our paper and Tofanelli et al. (2009) and found no matches: DYS19, DYS389I, DYS389II, DYS390, DYS391, DYS392, DYS393, DYS385a, DYS385b, DYS388, DYS437, DYS438, DYS439, DYS448 and DYS458. Available datasets that did not allow comparison of more than seven STRs were not included in our comparative database because they did not allow a sufficiently high level of resolution.
Results and discussion
The availability of a greater number of binary markers enables examination of the distribution of the original and extended CMH across the branches of a highly resolved Y chromosome haplogroup tree. In our dataset, the original CMH is observed in a total of 215 chromosomes, all of which belong to haplogroup J. Notably, most of these chromosomes are partitioned between the J1 and J2 subclades of the J haplogroup, specifically on the J-P58* and J-M67 lineages. A small number of original CMH chromosomes (n = 9) are found within other subclades of Hg J. In contrast, the extended CMH and its two closely related haplotypes shown in Fig. 3 are almost entirely limited to P58 chromosomes within the J1 clade: the extended CMH appears outside of J-P58* only once (i.e., within J-M319), while one of its two closely related haplotypes appears within haplogroup J-M67.
A survey of our database confirms that chromosomes carrying the original CMH are not specific to either Cohanim or Jewish populations. The original CMH is present at moderate frequencies (5–8%) in the other Jewish castes (i.e., Levites and Israelites), among non-Jewish Yemenites (13%) and Jordanians (~7%), and as singletons in a number of other non-Jewish populations (Druze, Egyptians, Palestinians, Syrians, Turks, Iranians, Italians, Romanians, and Uzbeks). In contrast, the extended CMH and its two related haplotypes are observed only among Cohanim (29.8%) and Israelites (1.5%) (i.e., it is completely absent from the Levites and non-Jews surveyed here). We also performed a search of the current literature (Arredi et al. 2004; Cadenas et al. 2008; Cinnioglu et al. 2004; Robino et al. 2008; Zalloua et al. 2008) and found a similar pattern: the original CMH is present in several Near Eastern populations, while the extended CMH is extremely rare outside of Jewish populations.
Divergence time (based on method of Zhivotovsky et al. (2004)) (ky) (mean ± SE) of Cohanim lineages based on Y-STR loci
Cohanim sample (N)
3.2 ± 1.1
3.0 ± 1.5
2.4 ± 0.8
2.8 ± 1.2
5.9 ± 2.0
4.9 ± 1.9
4.2 ± 1.3
3.8 ± 1.4
3.8 ± 1.2
4.2 ± 1.8
12.1 ± 4.4
5.5 ± 1.9
3.4 ± 1.2
4.0 ± 1.8
6.7 ± 2.5
4.3 ± 2.0
3.0 ± 1.3
4.3 ± 2.0
1.3 ± 0.5
1.9 ± 0.8
11.5 ± 2.8
14.1 ± 4.1
In sum, the high frequency of a closely related set of J-P58* chromosomes among Ashkenazi and non-Ashkenazi Cohanim that share a common modal haplotype, and that are estimated to have diverged from a common ancestor >2,000 years ago, is consistent with the hypothesis that the J-P58* lineage traces the Cohanim dynasty to a time before the Jewish diaspora. While the frequency of the J-P58* lineage is higher among Ashkenazi Jews (Fig. 2a), Y-STR variation associated with this haplogroup is older in the non-Ashkenazi community (e.g., we obtained divergence time estimates of 4.6 ± 1.8 and 3.5 ± 2.1 kyears for the 17- and 9-locus datasets, respectively). In this regard, it is also worth noting that the J-P58* network topology suggests population expansion, especially within the Ashkenazim. This may be attributable to the strong founder effect previously suggested for the Ashkenazi population (Behar et al. 2004, 2006).
Our results also document a set of non-J-P58* lineages that are carried collectively by more than 50% of Cohanim. Some of these lineages are members of the J2 subclade, while others are more distantly related (i.e., within haplogroups R and E) (Figs. 1, 2). To further explore the origin of these Cohanim lineages, we estimate the ages of Y-STR diversity associated with the J-M410*, J-M318, J-M12, and R-M269 lineages (Table 1), all of which are found at frequencies >5% in the Cohanim sample groups examined here (Fig. 2b). J-M410*, which is carried by both Ashkenazi (18.9%) and non-Ashkenazi (8.6%) Cohanim, is also found in ~5% of non-Cohanim Jews, as well as in many non-Jewish populations from the Near East (data not shown). Moreover, there is a modal Cohanim haplotype that is shared between Ashkenazi and non-Ashkenazi (North African and Sephardi) communities (Figure S1), and absent from non-Jewish populations. Divergence time estimates of Cohanim J-M410* chromosomes based on 17 and 9 Y-STRs range between 5.9 ± 2.0 and 4.9 ± 1.9 kyears, respectively. However, median-joining networks constructed from our Cohanim and non-Jewish data indicate that two Cohanim individuals carry divergent haplotypes that do not appear to descend from a common (modal) cluster of Cohanim J-M410* chromosomes (Figure S2). When we exclude these two divergent haplotypes from the analysis, we obtain divergence time estimates of 4.2 ± 1.3 and 3.8 ± 1.4 kyears for 17 and 9 Y-STRs, respectively. Our BATWING analysis returns coalescence time estimates of 3.2 kyears (95% CI, 0.7–16.7 kyears) (Table S5), similar to the divergence time estimates for Ashkenazi Cohanim in Table 1. These results support the hypothesis that J-M410* represents a second major founding lineage of the Cohanim, coalescing to a point within the early history of the ancient Hebrews of the Near East.
Similar results are obtained for the less frequent J-M12 lineage, which is carried by 16 Cohanim in our survey (14 of which are of Ashkenazi descent). As in the case of J-M410*, a median-joining network suggests that 2 of 16 individuals (1 Ashkenazi and 1 non-Ashkenazi Cohen) carry divergent haplotypes that may have entered the Cohanim population recently (Figure S3). Divergence time estimates made after removing these individuals are comparable to those for the Cohanim J-P58* and J-M410* lineages (3.4 ± 1.2 and 4.0 ± 1.8 kyears for the 17- and 9-locus datasets, respectively) (Table 1). In contrast, our network and divergence time analyses suggest that R-M269 chromosomes entered the Cohanim population via several “migration” events, and do not represent a single Cohanim founding lineage. For example, divergence time estimates are much older for Cohanim R-M269 chromosomes (>10 kyears) than for the three Cohanim lineages in haplogroup J discussed above, and median-joining networks of Cohanim R-M269 chromosomes lack a modal haplotype and show many unrelated singleton haplotypes that are interspersed among Cohanim and non-Jewish samples (Figure S4).
We note that divergence times for the J-P58*, J-M410, and J-M12 lineages are not statistically significantly different from one another as a result of the large standard deviations in Table 1. Moreover, we cautiously interpret dating of lineages that are not defined by the derived state at a terminal SNP (i.e., are internal nodes on the Y chromosome tree) and those that we have not typed all known downstream SNPs (J-M410*/J-P58* and J-M12, respectively) because subsets of chromosomes within these lineages may be marked by undiscovered SNPs. Our estimate of the age of J-M318 may be more reliable because this SNP represents a terminal mutation within the M410 sub-clade of the J2 branch (Fig. 1). Originally discovered in a single Libyan Jew (Shen et al. 2004), we find the derived allele at M318 to be present in 16 individuals in this survey—13 of which are Cohanim from Tunisia/Libya or the island of Jerba (the remaining 3 samples come from Tunisian or Libyan Jews who did not have information on their Cohen, Levite, or Israelite status). The much younger estimated divergence time for the J-M318 haplogroup (1.3 ± 0.5 and 1.9 ± 0.8 kyears for the 17- and 9-locus datasets, respectively) (Table 1) suggests that either the M318 mutation (a) arose within the Cohanim population of North Africa, (b) expanded within this community following migration of a founding J-M318 Cohen from another geographic location, or (c) became incorporated into the Cohanim patriline via conversion, adoption or non-paternity. The first of these possibilities (a) is supported by the fact that the M318 mutation occurred on the M410 background (Fig. 1), and median-joining network analysis links the cluster of Cohanim J-M318 chromosomes to that of the Cohanim J-M410* chromosomes (i.e., rather than to other J-M410* chromosomes from North Africa and the Near East) (Figure S5). The high frequency (~60%) of the otherwise rare J-M318 haplogroup in our sample from the island of Jerba may be the result of an ancient founder effect in this Jewish isolate, which is thought to be descended from one of the earliest Diaspora communities that left the Middle East before the destruction of the second Temple in 70 A.D. (Tessler and Hawkins 1980).
Here, we discuss alternative explanations for presence of several founding lineages within the Cohanim. One possibility is that multiple males were designated as Cohanim early in the establishment of the priesthood. We performed exploratory simulations to assess the likelihood of survival of multiple paternal lineages in the history of the Ashkenazi Cohanim. The probability of survival of more than a single haplogroup depends mainly on the population size and to a lesser extent, on the number of haplogroups that are assumed to have founded the initial Cohanim group. For example, if we begin with an initial population of 50 Cohanim carrying a total of 10 haplogroups, we find that there is a very low probability of survival of more than a single haplogroup after 120 generations. We obtain a similar result if we begin the simulation with 50 males each carrying a unique haplogroup (Figure S6). However, if we begin with 100 males carrying 10 haplogroups the mean number of haplogroups surviving for 120 generations is >1 (Figure S7). Thus, there would be a reasonably high probability that more than a single Cohen haplogroup could have survived in the Ashkenazi population since the initial founding of the priesthood ~3,000 years ago (Thomas et al. 1998) if we would be willing to accept an initial founding population size of >50 priests. However, our simulation results also suggest that it is highly unlikely that as many haplogroups as we actually observe (e.g. Fig. 2) would persist under this simple model. Another model that deserves consideration is a metapopulation (Wakeley 2004) in which semi-isolated communities maintain multiple Cohen lineages, each with a certain probability of extinction and replacement. In this model, multiple Cohanim lineages would then persist in the entire population, and new lineages would be expected to accrue among Cohanim over time. The presence of several founding lineages among the Cohanim of this survey—both shared between or specific to the Ashkenazi and non-Ashkenazi communities, as well as highly variable frequencies of these lineages among sub-populations within Ashkenazi and non-Ashkenazi communities (data not shown), may lend support to a metapopulation model. Mutation alone does not provide an explanation for the multiplicity of Cohanim haplogroups, because the ages of most of these haplogroups predate the foundation of the Jewish people (Cruciani et al. 2006; Karafet et al. 2008; Semino et al. 2004). Indeed, our divergence time estimates for the J-P58*, J-M410*, J-M12 lineages based on variation at the set of 9 STRs in our Israelite population sample are 19.0 ± 5.6, 22.6 ± 2.9, and 15.1 ± 3.1 kyears, respectively (data not shown).
We thank the individuals who provided samples for this study, including the National Laboratory for the Genetics of Israeli Populations. We also thank Connie Bormans for technical assistance. S.R. is partially supported by EU grant MIRG-CT-2007-208019 and L.Z. is supported by the RFBR- Russian Foundation for Basic Research.
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