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Transcript
REVIEW
Understanding the Evolution of Human Pigmentation:
Recent Contributions from Population Genetics
Jonathan L. Rees1 and Rosalind M. Harding2
Variation in human skin and hair color is one of
the most striking aspects of human variability, and
explaining this diversity is one of the central questions of human biology. Only in the last decade or
so has it been realistically possible to address this
question experimentally using population genetic
approaches. On the basis of earlier studies in mice,
and on studies in humans with various Mendelian
disorders, many of the genes underpinning population variation in skin color have been identified. More
recently, genome-wide approaches have identified
other loci that appear to contribute to pigmentary
variation. The ability to study sequence diversity from
world populations has allowed examination of
whether the observed variability is due to random
genetic drift or is a result of natural selection. The
genetic evidence taken as a whole provides strong
evidence for natural selection, functioning so as to
increase pigment diversity across the world’s populations. Future larger studies are likely to provide more
details of this process and may provide evidence for
exactly which mechanistic pathways have mediated
selection.
Journal of Investigative Dermatology advance online publication, 24 November
2011; doi:10.1038/jid.2011.358
Defining the role of natural selection in explaining variation
in human skin and hair color is one of the classic problems of
human biology (Cavalli-Sforza, 2001; Barsh, 2003; Rees,
2003; Jablonski, 2004; Diamond, 2005; Robins, 2005, 2009;
Parra, 2007). Why exactly do humans vary in skin and hair
color, and what explains the longstanding correlations
between skin pigmentation and geographical and genetic
ancestry? Is this variation a reflection of physiological
1
Department of Dermatology, University of Edinburgh, Edinburgh, UK and
Department of Zoology, University of Oxford, Oxford, UK
2
Correspondence: Jonathan L. Rees, Department of Dermatology, University of
Edinburgh, Room 4.018, Lauriston Building, Lauriston Place, Edinburgh EH3 9HA,
UK. E-mail: [email protected] or Rosalind M. Harding, Department of
Zoology, University of Oxford, Tinbergen Building, South Parks Road, Oxford
OX1 3PS, UK. E-mail: [email protected]
Abbreviations: EHH, extended haplotype homozygosity;
MATP, membrane-associated transporter protein; MC1R, melanocortin 1
receptor; NS, nonsynonymous; OCA4, oculocutaneous albinism type 4;
S, synonymous; SNP, single-nucleotide polymorphism
Received 14 July 2011; revised 31 August 2011; accepted 21 September 2011
& 2011 The Society for Investigative Dermatology
necessity or merely a reflection of the play of chance in the
development and growth of our species? To put the question
provocatively, what exactly are red hair and freckles for?
In this article, we set out to review how recent work on
human population genetics affects our knowledge of human
evolution. Our target is the nonspecialist skin biologist and
dermatologist. Understanding human evolution is in part a
historical science, and answering many questions requires
contributions from many fields—genetics, physiology, animal
evolution, anthropology, human history and geography, and
medicine to name but a few. Our aim is to produce a
coherent overview of what we take to be some of the key
findings of recent work—but with the emphasis on how
modern population genetics has provided strong evidence for
natural selection contributing to human skin pigment
diversity. Even within this narrow field, we have had to
choose breadth over depth, although we have tried to provide
appropriate references for those wishing to peruse the topic
more deeply. There are three issues worth flagging up. First,
using genetic techniques to address evidence for, or against,
natural selection is a problem that requires a reasonable level
of statistical insight. This is unavoidable. Second, we do not
discuss in any depth the cell biology or physiology of
pigmentation, as there are several pertinent reviews available
(Nordlund et al., 2006; Costin and Hearing, 2007; Sturm,
2009). Furthermore, we would argue that one virtue of the
recent work in population genetics is to allow (and presage
further) experimental testing of the various competing hypotheses that physiologists and cell biologists have proposed.
Finally, we do not discuss the relationship between skin color
and society, or the role of sexual selection in explaining skin
color diversity (Aoki, 2002; Jablonski, 2004; Robins, 2005).
WHY NOW?
Natural selection functions on genetic variability such that,
depending on an individual’s genotype, an individual either
produces more or fewer offspring. That is, the level of fitness
varies between individuals. It is self-evident in humans—
unlike say in some model organisms—that we cannot
distinguish fitness differences easily: the contribution of
genetic inheritance may be small compared with the
importance of social, cultural, environmental, or chance
factors that influence reproductive success. Our task, then, is
to infer selection from the evidence detected in a range of
data. What has markedly changed the nature of this task is
our increased ability to produce and interpret genetic data
and sequence variation. There are two reasons for this change
with respect to human pigmentation. First, the combination
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JL Rees and RM Harding
Evolution of Human Pigmentation
Table 1. The full names or associated clinical
syndromes for some abbreviations used in the text
with selected OMIM (Online Mendelian Inheritance
in Man) numbers
Abbreviation
Full name or associated
clinical syndrome
OMIM
number
ASIP
Agouti signaling protein
600201
ATN
Attractin
603130
DTNBP1
Hermansky-Pudlak type 7
614076
HERC2
Noncoding downstream of OCA2.
Affects expression of OCA2
227220
KITLG
Kit ligand
184745
MC1R
Melanocortin-1-receptor
155555
MYO5A
Myosin V (Griscelli syndrome 1)
160777
OCA2
Oculocutaneous albinism 2
611409
RAB27A
Griscelli syndrome 1
607674
SILV
Melanocyte protein 17
155550
SLC24A5
Solute carrier family 24, member 5
609802
SLC45A2
Solute carrier family 45, member 2
606202
TYRP1
Tyrosinase related protein 1
203290
TRPM1
Melastatin
603576
of preexisting resources such as the mouse fancy (and more
recently zebrafish), coupled with both positional cloning in
humans and candidate gene approaches based on work in
mice, has allowed the identification of many genes involved
in human pigmentation (Sturm, 2009). This initially took the
form of finding the genes that caused the highly penetrant
Mendelian disorders such as the various types of albinism
(Sturm, 2009). Subsequently, variants of some of these genes
or single-nucleotide polymorphisms (SNPs) close to these
genes (see Table 1 for a list of relevant loci) were found to
contribute to normal variation in pigmentary phenotype
within a Mendelian framework (the distinction here is
between Mendelian traits and complex traits). For instance,
the melanocortin 1 receptor (MC1R) was found to not only
explain the quasi-Mendelian trait of red hair (Valverde et al.,
1995) but also contribute to skin color, sun sensitivity, and
other pigmentary traits such as freckling in the wider non-redheaded population (Flanagan et al., 2000; Healy et al., 2000).
Second, high-throughput sequencing has allowed rapid
examination of associations between pigmentary characteristics and multiple loci across whole genomes. In the span
of 20 years, we have gone from knowing little about any of
the genes involved in human pigmentation to a position
where quantitative models of the contribution of loci to
human pigmentation are available (Naysmith et al., 2004;
Oh et al., 2004; Lamason et al., 2005). This area of pigment
biology has been well reviewed (Sturm, 2009). Assessing
evidence of evolution and natural selection requires the
analysis of the basic unit of genetic change—sequence
2
Journal of Investigative Dermatology
diversity. The knowledge of many more genetic variants
associated with diversity in human pigmentation has opened
up new opportunities for assessing the role of selection in
their evolution.
HOW IS NATURAL SELECTION DETECTED BASED ON
ANALYSIS OF GENETIC SEQUENCE?
It may appear counterintuitive, but a large part, if not the
majority, of genetic change in human populations is not
thought to be due to natural selection but rather due to the
play of chance (genetic drift; Harris and Meyer, 2006; Li
et al., 2008; see Table 2 for a glossary of terms frequently
used in population genetics). Many opportunities for chance
can occur in the transmission of alleles from parents to
offspring, and evidently did occur as part of the demographic
process of dispersal out of Africa. Thus, finding differences in
the frequency of alleles at a particular locus between
populations is not an evidence of natural selection per se.
The default position is that of neutral theory, whereby chance
events account for most patterns of genetic diversity (Harris
and Meyer, 2006). Of course, deleterious mutations will be
selected against (purifying selection) and beneficial mutations
may increase in frequency to fixation, but overall these events
will contribute little to explaining the presence of most
polymorphisms. One advantage of this framework is that it
makes testable theoretical predictions about sequence
diversity. When sequence data are examined for evidence
of selection, we seek statistical evidence for departures from
what we would have expected under neutral theory. This will
be familiar to most experimentalists in the way that
classical–frequentist statistics test whether the evidence is
strong enough to allow the ‘‘null hypothesis’’ to be rejected.
In the case under discussion here, an expectation under
neutral theory is the null hypothesis. If the distribution of the
data is such that it would rarely occur under neutral theory,
then the data are taken as providing evidence for selection.
Note that finding evidence for selection does not in itself
determine what selective factors are operating. Harris and
Meyer (2006) provide a simple taxonomy of available
statistical procedures accessible to the nonexpert, but we
would highlight some of the key points below.
K
K
Ratios of nonsynonymous (NS) to synonymous (S)
change. NS and S changes will affect function differently, with NS change much more likely to affect
function. Although high rates of NS/S provide evidence
of positive selection and low rates of NS/S provide
evidence of purifying selection, under strict neutrality
the predicted ratio would be close to unity. Where these
ratios differ for diversity within species in comparison
with divergence between species, changes in selective
pressures are implicated.
Levels of neutral polymorphism depend on mutation rate
and evolutionary population size. Alleles change frequency under genetic drift in random trajectories over
time spans predicted by the evolutionary population
size. Polymorphism at any particular site is a transient
state, but the time taken for a new variant to replace its
JL Rees and RM Harding
Evolution of Human Pigmentation
Table 2. Glossary of some of the terms and concepts used in population genetics
Extended haplotype homozygosity (EHH): A combined measure of the associated homozygosity plus the physical extent of a window of linkage
disequilibrium, judged against typical patterns of linkage disequilibrium produced by genetic drift. Comparisons made between those haplotypes carrying
the selected alleles versus those haplotypes carrying alternative variants provide useful statistics for evaluating partial selective sweeps.
Fitness: A measure of the relative rate of increase of a particular genotype. Relative fitness is represented in theoretical models using selection coefficients,
S. In a simple example, an S of 0.02 means that a genotype is only 98% as fit as the maximally fit genotype.
Fixation: The attainment by one allele of 100% frequency with the exclusion of all alleles previously present. This process may occur under either positive
selection or genetic drift. The fixation of alternative alleles in different subpopulations leads to FST=1.
Functional constraint: When the general effect of typical mutations of a gene (especially nonsynonymous mutations) is to generate new alleles that confer
lower fitness, that gene is said to be under functional constraint and subject to purifying selection.
Genetic drift: Change in allele frequencies in a population due to the play of chance in the transmission of an allele to successive generations.
Heterozygosity: Genetic variability due to the presence of (and degree of) pairing of different alleles at a genetic locus within (diploid) individuals in the
population. Contrast with homozygosity.
Linkage disequilibrium: A pattern recognized by correlations among allelic variants between loci in sets of DNA sequences that have been sampled from
a population. Windows of linkage disequilibrium show a lack of haplotype diversity. Interval length of these windows is delimited by the interplay of
recombination on the one hand, and genetic drift or selection on the other.
Natural selection: Organisms with genetic variants that better adapt them for survival and reproduction have a greater chance of contributing more offspring
to successive generations, and therefore the frequency of these particular genes (alleles) increases.
Neutral theory: Theory that accounts for the presence and turnover of most genetic variability (polymorphism) in a population as being due to random
frequency fluctuations of allelic variants (i.e., drift) originally produced by mutation.
Polymorphism: Genetic variability due to the presence of multiple alleles at a genetic locus in a population.
Population bottleneck: A rapid reduction in a population due to, for instance, disease or famine reduces the genetic variability in the population, and will
tend to increase inbreeding and the level of homozygosity.
Population structure: Arises when individuals do not mate randomly, with the consequence that alleles are not spread homogenously throughout a
population. In combination with the local effects of genetic drift and selection, genetic structure is produced, which can be measured by the fixation index
(FST). Values vary from 0 to 1, and those that are significantly different from 0 indicate structure.
Purifying (negative) selection: The loss of disadvantageous alleles, i.e., those that confer lower fitness, from the population. Contrast with positive selection of
advantageous alleles.
Selective sweep: An allele that attains fixation in the population under positive selection, thereby eventually replacing neighboring diversity with a singular
‘‘haplotype.’’ Diversity within such genomic regions is reduced compared with levels expected under neutrality. Alleles that attain fixation under selection
do so much faster than under genetic drift. The interval length of the associated window of linkage disequilibrium will be longer than for neutrally evolving
diversity because of the reduced opportunity for recombination over this shorter time span for fixation.
Synonymous and nonsynonymous variants: Point mutations in coding DNA that do not change the amino-acid sequence are synonymous (S, silent) and
those that do are known as nonsynonymous (NS).
K
K
ancestor (fixation) is typically long. Under positive
selection, a favored mutation has a rapid rise in
frequency, which will also lead to a reduction in overall
diversity close to the site, a change known as a selective
sweep. New mutations will eventually restore the
neighborhood heterozygosity; however, as this occurs
at the slower pace of neutral evolution, a detectable
footprint of selection remains for some time.
Differences in the fixation index between populations
within a species. If a particular allele increases fitness in
one population but is either not present in another
population or was not selected for in this other
population, then the differentiation between the populations is increased. Outliers in the distribution of the
fixation index can be judged using predictions based on
neutrality.
Linkage disequilibrium. Over many meiotic stages,
regions within a chromosome are shuffled (recombined)
between homologs such that the farther they are from
each other the less likely they are to stay together. This
process breaks up any physical linkage between the
segregating sites of multiple polymorphisms. The older
any sequence variants are the more likely that they will
have been shuffled (and hence may attain ‘‘linkage
equilibrium with each other’’). However, if the time
taken to become shuffled is longer than the time taken
for variants to be lost by genetic drift, then linkage
equilibrium may not be attained, and the resulting
linkage disequilibrium establishes haplotypes. Different
human populations typically differ in haplotype composition through the interplay of mutation, recombination,
and genetic drift. If a mutation arises that improves
fitness, then a selective sweep occurs. The rapid increase
in frequency extends the typical haplotype length over
what we would have expected if there were no change
in fitness. As part of the same process, the local diversity
is reduced. These properties lend themselves to wholegenome SNP-based analyses that examine the extended
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JL Rees and RM Harding
Evolution of Human Pigmentation
haplotype homozygosity (EHH; Sabeti et al., 2002). A
selective sweep increases the favored haplotype to a
high frequency and extends the surrounding haplotype,
generating high EHH values, compared with patterns
seen elsewhere in the genome as a result of drift. Note
that such approaches allow scanning of the entire
genome and identification of areas that might be under
selection without prior knowledge of what functions
particular loci serve.
The above principles guide interpretation of sequence
data, but of course rely on certain assumptions. Population
expansion or bottlenecking will lead to violations of neutral
models that assume constant population size (Harris and
Meyer, 2006; Tang et al., 2007; Laval et al., 2010). One
major advantage of genomic scans is that they inform the
neutral ‘‘null’’ model and reveal evidence for selection. The
principle here is that demographic changes should affect all
neutral loci, whereas the focus of selection will be on
particular physiological pathways. Whole-genome scans also
allow empirical testing where literally tens of thousands of
SNPs are examined, and results that appear to be outliers in
terms of change are viewed as candidates for evidence of
having undergone selection (Voight et al., 2006; Tang et al.,
2007).
SELECTION AT THE MC1R
The MC1R was the first gene identified in humans that
determined normal variation in pigmentary characteristics
(Rees, 2000). It encodes a seven-pass transmembrane
receptor that signals via cAMP and alters (at least in hair if
not skin) the ratio of pheomelanin to eumelanin. The gene
was identified in mouse and underpinned the previously
described extension locus. The a-melanocyte-stimulating
hormone functions as an agonist at the mc1r; in the mouse,
at least there is clear evidence that agouti antagonizes this
effect (Robbins et al., 1993). For a recent review, see
Beaumont et al. (2011). The fact that the MC1R is under
1 kb and is devoid of introns facilitated analyses with the
sequencing technology available at that time (Rees, 2000).
Early studies showed that the MC1R was highly polymorphic in Northern European populations, with many lossof-function alleles or diminished-function alleles present at
high frequency (Smith et al., 1998). The majority of those
with red hair were compound heterozygotes for two of these
alleles, but there was also a clear effect of single alleles on
freckling, skin color, scalp hair color, and beard color
(Flanagan et al., 2000). Chemical analyses of hair melanins
showed this heterozygote effect (Naysmith et al., 2004).
However, the limited studies in human skin found that only
homozygotes with diminished-function alleles tended to have
lower amounts of both pheomelanin and eumelanin, rather
than a simple alteration in the ratio as with hair (Hennessy
et al., 2005; for the situation in mouse, see Van Raamsdonk
et al., 2009). Individuals harboring one of a range of variant
alleles are predisposed to both non-melanoma skin cancer
and melanoma skin cancer, as well as freckling (Valverde et al.,
1996; Smith et al., 1998). Subsequent functional studies and
4
Journal of Investigative Dermatology
population studies have further defined the functional status of
a range (but not all) of these alleles, which today number over
65 (Wong and Rees, 2005). Studies of Neanderthal DNA have
also shown changes in MC1R that would be predicted to lead
to a red-haired phenotype (the particular mutation seen has not
been found in modern-day humans).
The degree of variation at MC1R was unexpected and
subsequent population studies by Harding et al. (2000) and
Rana et al. (1999) showed that this variation was largely
restricted to European populations when compared with
African or Asian samples (nucleotide diversity rates of 0.12%,
0.09%, and 0.07%, respectively). What was equally striking
was that the pattern of nucleotide change differed between
Northern European populations and the others examined. In
the European populations, NS changes predominated, whereas
the majority of changes see in African populations were
synonymous. Subsequent studies (John et al., 2003) have
detected some NS changes, although the African populations
sampled were from South Africa rather than the populations
from central and western Africa in the earlier studies.
This pattern of diversity is of course unusual in that for
most genetic loci diversity within African populations is
higher than the diversity in other world populations (CavalliSforza, 2001). Both Harding et al. (2000) and Rana et al.
(1999) analyzed the pattern of MC1R diversity, and agreed
that there was functional constraint on MC1R in African
populations. However, they proposed different interpretations of the reason for diversity in Northern European
populations. Harding et al. (2000) argued that NS mutations
of this gene diminished fitness and were therefore selected
against in Africa, but that relaxation of this constraint outside
of Africa was sufficient to explain the observed diversity
outside of Africa. Conversely, Rana et al. (1999) argued in
favor of diversifying selection. In other words, Harding et al.
(2000) argued that the diversity seen in Europe was not a
result of selection (for loss-of-function or diminished-function
alleles), but because there was little fitness difference
between any of these alleles. The observed data were not
sufficient to reject the neutral theory hypothesis. In contrast,
Rana et al. (1999) argued that the role of mutation at MC1R
was such as to have actively been selected for presumably on
the basis of a fitness advantage of a paler skin color. Harris
and Meyer (2006) provide a critical review of these two
papers. Large studies with greater population sampling might
resolve some of these differences in interpretation. As we will
see, the MC1R data are of interest in themselves because not
all pigment genes show the same evolutionary patterns, and
also because the pleitropy of MC1R cautions against
evidence based on one gene only.
SLC24A5
Differences in pigmentation are clearly not just due to
alterations in the ratio of eumelanin to pheomelanin
(‘‘pigment switch’’). Indeed, as previously mentioned,
although this switch is clearly evident in studies of mouse
or human hair, studies in human skin are less convincing.
Pigmentation in human skin reflects a complex series of
cellular processes, which at the least involve the production
JL Rees and RM Harding
Evolution of Human Pigmentation
of a myriad of different melanin polymers, the packaging of
these products into melanosomes, and the transfer of these
melanosomes into the surrounding keratinocytes. The pattern
adopted by these melanosomes after they have been taken up
by keratinocytes may also be important in photoprotection,
and it is well known that the size and shape of melanosomes differ between people with differences in skin color
(Nordlund et al., 2006).
Although, historically, mouse mutants have been the focus
of comparative pigment geneticists, the zebrafish have also in
recent years provided important insights. Zebrafish that are
homozygous for the golden mutation show hypopigmentation of the skin and retinal pigmented epithelium. The
pigment granules in these tissues are less dense and smaller.
Lamason et al. (2005), using linkage and morpholino knockdown experiments, cloned and identified the golden gene,
which in humans is known as SLC24A5. SLC24A5 based on
sequence is a member of the family of potassium-dependent
sodium–calcium exchangers. Lamason et al. (2005) noted a
polymorphism in the gene with the G and A alleles of the
SNP rs1426654 encoding alanine or threonine, respectively,
at amino acid 111 in the third exon. This SNP had previously
been shown to vary in frequency between populations with
different ancestries, ranging from over 98 to 100% for the
Thr111 variant in European populations, whereas in African or
East Asian populations the Ala111 allele had a frequency of
93–100%. These differences are striking, highly unusual for
the vast majority of SNPs, and of course compatible with
selection to almost fixation. To confirm the role of selection,
the authors noted that the pattern of heterozygosity around
SLC24A5 was less compatible with a selective sweep having
taken place under positive selection in European populations.
Physiological studies in admixed populations showed that the
allele has a direct effect on skin color, measured spectrophotometrically (Lamason et al., 2005). Differences in
SLC24A5 do not, however, account for differences in skin
color between Africans and East Asians because the ancestral
allele (Ala111) is found in both.
SLC45A2 (ALSO KNOWN AS THE MEMBRANEASSOCIATED TRANSPORTER PROTEIN (MATP))
Mutations of SLC45A2, another solute carrier similar to
SLC24A5, underlie oculocutaneous albinism type 4 (OCA4;
Newton et al., 2001). Other polymorphisms have also been
detected in this gene and are associated with pigmentary
phenotypes (Graf et al., 2005), as well as with ancestry.
Soejima et al. (2006) studied the pattern of diversity in this
gene within the coding and exon-flanking regions. They
found lower diversity than expected under neutrality only in
those of European descent; they also found that one
haplotype was overrepresented in European populations, in
keeping with a positive selective sweep (for lightening of skin
color; Soejima et al., 2006). As for MC1R, SLC45A2 was
under constraint in African populations.
WHOLE-GENOME STUDIES AND RELATED METHODS
The studies described above have focused on single genes.
The MC1R is small and easily sequenced, and coding region
variants are very frequent in European populations. SLC24A5
and SLC45A2 were identified on the basis of work in model
systems and human studies that examined candidate SNPs in
terms of effect on phenotype, ancestral distribution, and
subsequently whether there was evidence for selection.
The development of high-throughput sequencing methods
over the past 10 years has, however, allowed new
approaches to the study of genes involved in human
pigmentation. Genome-wide scans have both confirmed a
role for a number of candidate genes in human pigmentation—previously identified on the basis of work in the mouse
or other model systems—and identified new loci, which with
further work are likely to be found to be causal in explaining
human pigmentary differences (Sulem et al., 2007, 2008;
Han et al., 2008). These include, as well as the ones
discussed above, TYR, TYRP1, OCA2, ASIP, KITLG, and loci
that were previously not suspected to harbor a role in
pigmentation, including SLC24A4, IRF4, HERC2, and TPCN2
(for a review of relevant cell biology, see Sturm, 2009).
Knowledge of the loci implicated in determining pigmentary characteristics coupled with the statistical methods
described earlier has allowed several groups to seek evidence
for natural selection at a number of different candidate loci.
Examples include Lao et al. (2007), who used EHH evidence
for inferring positive selection in European populations at a
number of pigmentary loci including at OCA2, TYRP1, and
KITLG, as well as in Asians (OCA2, DCT, KITLG, EGFR, and
DRD2); Izagirre et al. (2006), who have conducted similar
candidate-based studies, although their results differ from
some others in the literature (see Lao et al. 2007 for a
critique); and Norton et al. (2007), who analyzed FST for
known pigmentation genes to suggest that ASIP and OCA2
may be involved globally in explaining skin color adaptations, whereas other loci, such as SLC24A5, MATP, and TYR,
may have contributed to adaptation in European populations
but not in East Asian populations.
However, the most powerful approaches have scanned the
whole genome, looking for evidence of loci that, on the basis
of EHH statistics, look as though they have been subjected to
selective sweeps (Sabeti et al., 2002, 2007). One advantage
of this approach is that it allows the distribution of values
across the genome for EHH to be calculated and then interest
focused on those loci that show extreme values, the
assumption being that if EHH values are unusually high then
selection is likely. The resulting areas can then be summarized and interpreted on the basis of likely physiological
functions. Thus, if a screen finds that many of the genes with
high EHH values are involved in pigmentation, or immunity,
or absorption of dietary products, then it is possible to paint a
picture of how our environment has shaped our recent
biological history.
Voight et al. (2006) used data from the International
HapMap Project to create a first-generation map of selection
across the human genome. Their chief test statistics were
derived from the EHH principle. They showed, as expected,
that genes involved in fertility and reproduction are subject to
rapid adaptive evolution, but that some of the strongest
signals of recent selection were for genes involved in
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JL Rees and RM Harding
Evolution of Human Pigmentation
pigmentation in Europeans, including OCA2, MYO5A,
DTNBP1, and TYRP1. The technique they used has limited
power where alleles have achieved fixation or are close to
fixation, but signals for SCL24A5 were also strong. These
signals of selection for pigmentation postdated the divergence
of the three main population groups around the world (Africa,
Europe, and Asia). Other statistical analyses—but still based
on EHH—have also confirmed some of these same pigmentation loci (MYO5A and SCL24A5) as being under selection
using data sets from both the HapMap Project and Perlegen
Sciences (Tang et al., 2007), and SCL24A5 and SCL45A2 as
being under positive selection in Europe (Sabeti et al., 2007;
Barreiro et al., 2008). Loci identified as being related to
pigmentation and showing evidence of selection in one or
more studies include OCA2, TYRP1, DNTPB1, SLC24A5,
MYO5A, SCL45A2, ABCC11, KITLG, MATP, HERC2, SILV,
TRPM1, RAB27A, and ATRN. The HapMap and Perlegen
data sets have limited sampling with only one or two
populations from within the main regions (Africa, Europe,
and East Asia). Pickrell et al. (2009) therefore looked at just
under 1000 individuals from 53 world populations using the
Human Genome Diversity-CEPH Panel. They used EHH and
related statistics, as well as looked at FST. For some
population comparisons (e.g., Europe vs. Africa), differences
in allele frequencies were much greater for various,
previously identified, pigmentation genes than those typically
found for other loci, and haplotype analyses again showed
evidence for selection of SLC24A5 and KITLG. They also
found evidence for selection of genes such as MLPH and
RGS19, which are known to have a role in pigmentation in
other mammals, but not to date in humans. Finally, echoing
some of the work of Norton et al. (2007), they note that
different genes may cause skin lightening in different parts of
the world (i.e., the causes of lightening in European
populations may differ genetically from lightening in East
Asians).
LINKING GENES WITH THE PHYSICAL ENVIRONMENT
Another powerful use of whole-genome SNP analysis has
been an attempt to link markers of selection with measures
of climatic change directly. It has been long known that
climatic factors are important determinants of species
distribution and are likely key determinants of phenotypic
variation. Examples would include change in body shape
and mass with temperature, and of course skin pigmentation. Hancock et al. (2011) have correlated allele frequencies
at a range of SNPs and climate variables such as solar
radiation, humidity, precipitation, and so on. They report a
striking enrichment of genic and nonsynonymous SNPs
relative to nongenic SNPs among those that are correlated with climate variables. Changes in SCL24A2 and
OCA2 were particularly noteworthy, but also of relevance
was a SNP in keratin 77 (KRT77), a gene that is expressed in
sweat glands, and genes involved in UVR-related DNA
repair. As they state, a common theme of their analyses and
other similar analyses is that genes involved in pigmentation
and UV radiation are among those with the strongest signals
of selection.
6
Journal of Investigative Dermatology
WHAT DRIVES NATURAL SELECTION?
Just over 10 years ago, the world literature on genetic
evidence for natural selection on human pigmentation
comprised only two papers, both dealing with sequence
diversity in the only gene then known to have a role in
normal (rather than pathological) pigmentation variation, the
MC1R (Rana et al., 1999; Harding et al., 2000). Subsequent
candidate-based approaches show evidence for SLC24A5
(Lamason et al., 2005) and SLC45A2 (Soejima et al., 2006).
Unbiased scans using a range of techniques to detect
selection have now involved a range of loci including
OCA2, TYRP1, DNTPB1, SLC24A%, MYO5A, SCL45A2,
ABCC11, KITLG, MATP, HERC2, SILV, TRPM1, RAB27A, and
ATRN (Hancock and Rienzo, 2008).
The breadth of this evidence is important (Pritchard et al.,
2010). The pattern of selection is not the same in all
populations studied, with different alleles being selected for
skin lightness in some European and Asian populations, and
evidence of sweeps for many but not for MC1R. For technical
reasons relating to the diversity and representation present in
many genome-wide studies, there may be a bias toward
genes important in European populations rather than African
populations (Pritchard et al., 2010; Casto and Feldman,
2011). African populations remain under strong selective
forces, and although the majority of pigment diversity is
between continents, there remains substantial pigmentary
variation within Africa (Relethford, 2002), which is as yet
largely unexplained in genetic terms.
Ascribing single functions to some genes may on occasions also be premature. Perhaps the clearest example is
again the MC1R. The MC1R was identified on the basis of its
coat color phenotype in the mouse. Human studies reasonably focused on association studies between allelic variants
and the pigmentary phenotype, and particularly, given the
thrust of this essay, the relationship between its evolution and
ambient UVR exposure. The fact that MC1R has a role in
photoprotection is compelling, but should we necessarily
attribute MC1R diversity to the inverse of the same selective
pressures? Consider the unexpected findings in 2005 of pain
researchers who found that in the mouse, mc1r had
pronounced effects on responses to some types of pain
stimuli (Mogil et al., 2003). Subsequent studies have
extended this work into humans, and although the effect on
phenotype appears complex and confined to the females, the
effect appears real, although the mechanism is unknown
(Mogil et al., 2003; Delaney et al., 2010). This inevitably
emphasizes the importance of studying groups of genes
sharing some commonality or overlap of function over
evidence from just a single locus, where unexpected
phenotypes could undermine what appear to be clearcut
conclusions. Similarly, the study by Hancock et al. (2011)
relating selection to measures of ambient UVR allows not
only the study of pigmentation phenotypes but also of genes
that have a role in UVR-induced DNA repair. Furthermore,
thinking in terms of physiological pathways seems appropriate. However, another caveat here is required; although
sequence changes over a range of genes that affect
pigmentation may strengthen the overall case for selection
JL Rees and RM Harding
Evolution of Human Pigmentation
on pigmentation, one can also ask—as for MC1R and pain—
whether other factors could be driving changes in some genes
independently of affects on skin color and photoprotection.
To speculate beyond the remit of this essay, do changes in
MC1R reflect some form of sexual selection for red hair and
porcelain skin? It is beyond the nature of the evidence
available to us to make a reply.
The available studies do not tell us why pigmentation has
been the subject of natural selection, why dark skin has been
selected for in sub-Saharan populations, or why lighter skin
has been selected in European populations and in some of
the Asian populations (Relethford, 2002). The conventional
explanation is of course that this variation is related to
ambient UVR, and indeed studies such as those of Hancock
et al. (2011) are quite compatible with this. Of course,
compatible does not mean that they are correct. Nevertheless, most opinion converges on the idea that human
interfollicular pigmentation evolved to compensate the loss
of body hair in our ancestors, driven by the need for effective
sweating, an activity that is severely limited by a dense
coat or sunburn. The evidence presented strongly argues that
the skin color of ancestral modern humans was dark, and
this pigmentation provided a defense against UVR damage.
As our ancestors migrated out of Africa, the need for such
effective protection diminished and indeed as we have
learned, paler skin—skin that receives more damage from
UVR—was favored. The time course of these latter changes
are not known with any confidence (ranging from 6,000 years
to over 50,000 years), nor is there tight agreement on the time
course of our recent demographic history (Laval et al., 2010).
The principal theories relating to variation in pigmentation
and UVR relate to vitamin D biosynthesis, folate depletion,
sunburn, skin cancer dysfunction (reviewed by Robins, 2005;
Juzeniene et al., 2009), or barrier dysfunction (Elias et al.,
2009). The presence of dark skin protects against sunburn and
possibly folate deficiency, whereas in areas with less ambient
UVR, lightening of the skin is necessary to allow sufficient
vitamin D biosynthesis, and the problem of sunburn or skin
cancer or folate deficiency is relatively less (Robins, 2005). It
is difficult, however, to conjure up experiments to meaningfully test these various hypotheses. For instance, skin
cancer is often judged to be irrelevant because it affects
individuals usually of a post-reproductive age. However, we
know that extreme syndromes such as xeroderma pigmentosum and albinism (Robins, 2005; Parra, 2007) show markedly
impaired fitness, and quantitative data on how those with
pale skin would manage in equatorial regions without the
benefits of modern life are not available (Diamond, 2005).
The case for sunburn and any resulting secondary infection
leading to impaired fitness seems easier to make than the
adverse risks from skin cancer in older individuals.
The role of vitamin D in our physiology over our
evolutionary past is hard to definitively judge. It is clear that
our cereal-based diet in historically recent times coupled
with life at Northern latitudes provides a vitamin D-poor diet.
However, problems remain as to whether this is the
explanation for skin lightening in earlier periods. Whereas
we have a good idea of what levels of vitamin D are required
for bone health early in life, we are uncertain about what
levels are needed for a number of other putative biological
functions, including resistance to infectious diseases. Our
knowledge of how these various factors affected over the past
5–50,000 years is scant, as is direct evidence of our vitamin D
status over all but recent historical times. There are similar
gaps in our knowledge about whether variation in pigmentation can be accounted for in terms of selection against UVR
degradation of folate.
Given the historical nature of the subject matter, it may
seem easy to be pessimistic that we will obtain answers to
these questions. However, just over 10 years ago it was hard
to imagine the results we have now: that merely by relating
patterns of DNA variation to population and to measures
of environmental stress (and there is no good reason to
imagine there have been significant global changes in UVR
over the last millions of years), clusters of genes involved
not only in pigmentation but also in cellular responses to
UVR DNA damage would be flagged up by tests for selection.
It seems possible at least that as we learn to burrow
down further into our shared DNA that other footprints of
physiological stress—vitamin D deficiency or folate deficiency—might have caused patterns of diversity that function as tracers for those forces that have shaped us. Finally,
our knowledge of the genes underpinning pigmentation,
and the technical ability to identify DNA from Neanderthals
and other hominins (Laleuza-Fox et al., 2011), means that
there may still be a lot to learn about why we look the way
we do. As is often repeated, evolution is the greatest story
ever told, and there will surely be more episodes, if not
surprises, to follow.
CONFLICT OF INTEREST
The authors state no conflict of interest.
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