| Literature DB >> 19478947 |
S Ivan Perez1, Valeria Bernal, Paula N Gonzalez, Marina Sardi, Gustavo G Politis.
Abstract
Currently, one of the major debates about the American peopling focuses on the number of populations that originated the biological diversity found in the continent during the Holocene. The studies of craniometric variation in American human remains dating from that period have shown morphological differences between the earliest settlers of the continent and some of the later Amerindian populations. This led some investigators to suggest that these groups--known as Paleomericans and Amerindians respectively--may have arisen from two biologically different populations. On the other hand, most DNA studies performed over extant and ancient populations suggest a single migration of a population from Northeast Asia. Comparing craniometric and mtDNA data of diachronic samples from East Central Argentina dated from 8,000 to 400 years BP, we show here that even when the oldest individuals display traits attributable to Paleoamerican crania, they present the same mtDNA haplogroups as later populations with Amerindian morphology. A possible explanation for these results could be that the craniofacial differentiation was a local phenomenon resulting from random (i.e. genetic drift) and non-random factors (e.g. selection and plasticity). Local processes of morphological differentiation in America are a probable scenario if we take into consideration the rapid peopling and the great ecological diversity of this continent; nevertheless we will discuss alternative explanations as well.Entities:
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Year: 2009 PMID: 19478947 PMCID: PMC2684646 DOI: 10.1371/journal.pone.0005746
Source DB: PubMed Journal: PLoS One ISSN: 1932-6203 Impact factor: 3.240
Figure 1Map showing geographic location of the crania samples analyzed.
Sample composition, abbreviations, age, gender distribution and sample sizes.
| Samples | Abbrev. | Region | Age | F | M | Total |
| Southeast Pampa | SEP-emH | Southeast Pampa | Early/Middle Holocene (ca. 7,800–6,300 years BP) | 3 | 3 | 6 |
| SEP-elH | Southeast Pampa | Earlier Late Holocene (ca. 2,500–1,500 years BP) | 2 | 7 | 9 | |
| SEP-llH | Southeast Pampa | Later Late Holocene (ca. 1,500–200 years BP) | 4 | 7 | 11 | |
| Isla Gama | IG-llH | Northeast Patagonia | Later Late Holocene (ca. 1,500–200 years BP) | 7 | 5 | 12 |
| San Blas | SB-llH | Northeast Patagonia | Later Late Holocene (ca. 1,500–200 years BP) | 15 | 18 | 33 |
| Laguna del Juncal | LJ-elH | Northeast Patagonia | Earlier Late Holocene (ca. 3,500–2,500 years BP) | 12 | 19 | 31 |
| Negro River Valley | RN-elH1 | Northeast Patagonia | Earlier Late Holocene (ca. 3,500–2,500 years BP) | 13 | 10 | 23 |
| RN-elH2 | Northeast Patagonia | Earlier Late Holocene (ca. 2,500–1,500 years BP) | 2 | 8 | 10 | |
| RN-llH | Northeast Patagonia | Later Late Holocene (ca. 1,500–200 years BP) | 9 | 12 | 21 | |
| San Antonio Este | SAE-llH | Centre Patagonia | Later Late Holocene (ca. 1,500–200 years BP) | 3 | 5 | 8 |
| Chubut River Valley | ChV-elH | Centre Patagonia | Earlier Late Holocene (ca. 2,500–1,500 years BP) | 6 | 10 | 16 |
| ChV-llH | Centre Patagonia | Later Late Holocene (ca. 1,500–200 years BP) | 18 | 20 | 38 | |
| Southwest Chubut | SWCh-llH | Centre Patagonia | Later Late Holocene (ca. 1,500–200 years BP) | 7 | 7 | 14 |
| South Mendoza | SM-elH | Northwest Patagonia | Earlier Late Holocene (ca. 2,500–1,500 years BP) | 8 | 15 | 23 |
| SM-llH | Northwest Patagonia | Later Late Holocene (ca. 1,500–200 years BP) | 6 | 9 | 15 | |
| Delta of Parana | Del-llH | Northeast Pampa | Later Late Holocene (ca. 1,500–200 years BP) | 5 | 8 | 13 |
| Total | 283 |
Approximate sample ages according to radiocarbon dating obtained from human bones and contextual information.
Samples characterized molecularly.
Figure 2Allocated geometric coordinates are displayed with different symbols.
Landmarks are represented as squares (▪), whereas semilandmarks are represented as circles (•) on face (A) and vault (B) views. The numbers correspond to the following landmarks: nasion (1); nasospinale (2); prosthion (3); alare (4); ectoconchion (5); frontotemporale (6); frontomalare temporale (7); ectomolare (8); post-mastoid (9).
Figure 3Relative Warp analysis of the face.
A) Ordination of the 16 East Central samples in the space of the first two relative warps, based on the partial warp and uniform component variables calculated for the face. The circles (•) represent the consensus individual or mean shape for each Later Late Holocene sample (llH), stars (★) represent the consensus individual for each Earlier Late Holocene sample (elH), and number sign (#) represents the consensus individual for the Early Holocene sample from Arroyo Seco 2 (eH). B and C) Facial shape changes implied by variation along the first relative warp axis is shown as deformation grids. Grids show shape changes for negative (B) and positive (C) deviations from the mean for RW1.
Figure 4Procrustes fit of geographic coordinates and temporal data (circle) onto the position of mean facial shape for each East Central Argentina sample on relative warps 1 and 2.
Figure 5Relative Warp analysis of the cranial vault.
A) Ordination of the individuals from East Central samples in the space of the first two relative warps, based on the partial warp and uniform component variables calculated for the vault. The circles (•) represent the individuals for Later Late Holocene sample (llH), stars (★) represent the individuals for each Earlier Late Holocene sample (elH), and number sign (#) represents the individual for the Early Holocene sample from Arroyo Seco 2 (eH). The ellipses are the 95% confidence intervals of Earlier and Later Late Holocene mean samples. B and C) Vault shape changes implied by variation along the first relative warp axis is shown as deformation grids. Grids show shape changes for negative (B) and positive (C) deviations from the mean for RW1.