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Technical CommentsComment on "Whole-Genome Shotgun Sequencing of Mitochondria from Ancient Hair Shafts"
Gilbert et al. (Reports, 28 September 2007, p. 1927) reported that "hair shafts surpass comparably stored bone as an aDNA source [...] in regard to preservation and concentration of mtDNA." When experimental parameters are carefully controlled for, including adequate sampling, quantitative polymerase chain reaction analysis, and modeling the decay of DNA, the general importance of this claim is not supported.
McMaster Ancient DNA Centre, Department of Anthropology, McMaster University, 1280 Main Street West, Hamilton L8S 4L9, ON, Canada.
* To whom correspondence should be addressed. E-mail: debruyne{at}mcmaster.ca
Bone has long been the preferred matrix for DNA extraction from ancient samples, due to its prevalence in archaeological and paleontological contexts as well as its presumed preservation potential (1, 2). It has also been used in metagenomic approaches to whole genome reconstruction of both Neandertals and mammoths (3–5). However, Gilbert et al. (6) have recently confirmed earlier work (7) showing that ancient hair shafts are good sources of DNA that can also adequately be used in 454 sequencing. The purported novelty of their recent study lies in the comparative analysis of mitochondrial DNA (mtDNA) sequence data from both hair shafts and bone. They analyzed relative mtDNA concentrations and "assessed the state of DNA preservation through [...] untrimmed read length and [...] cytosine-to-thymine (C We commend their use of hair for ancient DNA studies but question the rigor of their general statements concerning preservation (fig. S1). First, Gilbert et al. compared 10 hair shafts and a single bone, from separate individuals, thereby precluding any within-sample comparisons and allowing only cross-comparisons between different preservational histories. Second, the 454 library from bone derived from a nebulized DNA extract, a step omitted for the preparation of all hair shaft libraries. The nebulization shears DNA down to short fragments (400 to 800 base pairs), involves a substantial loss of DNA, and may relatively enrich libraries in high-molecular-weight contaminants (4). Although the effects of nebulization on damaged ancient DNA, as well as the generation of additional forms of damage, have yet to be explored, the rate of C>T damage (qualitative criterion used by Gilbert et al.) calculated for their bone library (1.699%) could not be reproduced when clones of a non-nebulized DNA extract of the same bone from the same individual were sequenced. These yielded a rate of C>T as low as 0.483% (table S8), comparable to those from non-nebulized hair shaft samples [0.243 to 0.899%, (6)]. According to such a rate, the bone library no longer appears as an outlier in the thermal age comparisons (fig. S2). Third, hair shaft and bone libraries were sequenced on different genome sequencing (GS) systems. Whereas hair shaft libraries were sequenced using the Roche GS FLX [mean read length (MRL) expected: 240 base pairs (bp)], the bone library was sequenced using the Roche GS20 (MRL limited to 100 to 110 bp). MRL comparisons are thus artificial. Although Gilbert et al. (6) point out this limitation, they regard MRLs as their second qualitative criterion.
Last, the lack of experimental details in (6) precludes comparative analysis of some library specifics (supporting online text). To address these issues, we analyzed the mammoth mtDNA content of hair (shaft and root separately) and bone samples derived from the same individual: Lyakhov removed from the permafrost and preserved at room temperature since 1902 (9), as well as the Jarkov mammoth preserved frozen since its excavation in 1999 (10). In addition, bone samples from Fishhook (11) and the 2005/915 mammoth (5) were extracted for comparison. DNA extracts were generated following published protocols (12) and used in a series of 5 mt elephant-specific quantitative polymerase chain reaction (qPCR) assays that span 84 to 677 bp of the cytochrome b (5). All qPCR results were scaled to copies per milligram of sample (12). Copy numbers from the varying fragment lengths were used to derive a degradation curve according to Deagle et al.'s model (13): a linear regression of log-transformed copy numbers onto amplicon sizes allowing the derivation of the amount of DNA molecules (N), the frequency of damage ( Contrary to Gilbert et al., our results (Fig. 1 and table S1) depict varying DNA concentrations in bone and hair, depending on the level of degradation. The mammoth DNA from Lyakhov is highly fragmented and damaged (positive PCRs for the two shortest products only) and almost entirely preserved within bone (86%, versus 12% in hair root and only 2% in hair shafts). In contrast, the DNA from the frozen Jarkov shows 10 to 20 times as many mtDNA copies in the hair shaft than in bone for the two shortest fragments, a result consistent with Gilbert et al.'s data. However, this trend quickly reverses with the 677 bp piece only amplifiable from bone (Fig. 1).
This quantitative trend in Jarkov illustrates a differential qualitative pattern of DNA degradation (Fig. 2). The steeper slope from hair shafts suggests more damage than in the bone (
Paired tissue type comparisons thus confirm that ancient hair shafts may indeed contain large amounts of mtDNA, but they also reveal that the quantitative and qualitative superiority of hair shafts over bone does not appear to be a general feature. Our analysis supports that the chances of retrieval of endogenous DNA are not higher in hair than in bone. The field of ancient DNA has always been plagued by controversial conclusions leading some authors to establish a set of experimental criteria (2). Although those criteria need to be revisited with the advent of paleogenomic studies, proper experimental controls remain a necessity to ensure the applicability of generalized comments about DNA preservation.
Supporting Online Materialwww.sciencemag.org/cgi/content/full/322/5903/857a/DC1 Materials and Methods SOM Text Figs. S1 and S2 Tables S1 to S8 References
Received for publication 28 March 2008. Accepted for publication 10 October 2008.
The editors suggest the following Related Resources on Science sites:In Science Magazine
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Science. ISSN 0036-8075 (print), 1095-9203 (online)