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http://informahealthcare.com/ahbISSN: 0301-4460 (print), 1464-5033 (electronic)
Ann Hum Biol, 2014; 41(4): 312–322! 2014 Informa UK Ltd. DOI: 10.3109/03014460.2014.922616
REVIEW
Diagnosing Homo sapiens in the fossil record
Christopher Brian Stringer1 and Laura Tabitha Buck1,2
1Natural History Museum, Cromwell Road, London, UK and 2University of Roehampton, Whitelands College, Holybourne Avenue, London, UK
Abstract
Background: Diagnosing Homo sapiens is a critical question in the study of human evolution.Although what constitutes living members of our own species is straightforward, in the fossilrecord this is still a matter of much debate. The issue is complicated by questions of speciesdiagnoses and ideas about the mode by which a new species is born, by the argumentssurrounding the behavioural and cognitive separateness of the species, by the increasingappreciation of variation in the early African H. sapiens record and by new DNA evidence ofhybridization with extinct species.Methods and results: This study synthesizes thinking on the fossils, archaeology and underlyingevolutionary models of the last several decades with recent DNA results from both H. sapiensand fossil species.Conclusion: It is concluded that, although it may not be possible or even desirable to cleanlypartition out a homogenous morphological description of recent H. sapiens in the fossil record,there are key, distinguishing morphological traits in the cranium, dentition and pelvis that canbe usefully employed to diagnose the H. sapiens lineage. Increasing advances in retrieving andunderstanding relevant genetic data provide a complementary and perhaps potentially evenmore fruitful means of characterizing the differences between H. sapiens and its close relatives.
Keywords
Fossil record, hybridization, Neanderthal DNA,species definition
History
Received 30 April 2014Accepted 1 May 2014Published online 16 June 2014
Diagnosing Homo sapiens
It is self-evident that diagnosing Homo sapiens is a funda-
mental question in human origins. For most taxa, any
specimen in question can be compared to the type in order
to assess the case for its inclusion within that species. Yet, as
so often, our own species is seen as somewhat of a special
case. The type specimen for H. sapiens is Linneaus himself
(Notton & Stringer, 2010; Stearn, 1959); however, this is
more of a ceremonial honour than a useful taxonomic aid.
Being the only remaining representatives of our genus, all
living humans are similar enough, with demonstrable inter-
fertility, that there is no question as to which species they
belong. Diagnosing H. sapiens has only been regarded as an
issue of importance since other hominin species were found
and acknowledged, beginning with the discovery of the
skeleton from the Neander Valley in 1856, which was
subsequently named as the holotype of H. neanderthalensis
in 1864 (King, 1864). For many extinct hominins their species
definition is far from clear and, in diagnosing other species,
we must simultaneously diagnose our own. The delineation
of H. sapiens has varied widely since the discovery of fossil
human species and, although there are areas of agreement for
many, there is no overall consensus on what constitutes
H. sapiens. In recent years this question has been complicated
further by the genetic evidence, which shows that Pleistocene
species may have interbred with relative frequency, although
not necessarily with high levels of compatibility.
Underlying evolutionary model
Historically, different diagnoses of H. sapiens have been
influenced by their underlying evolutionary model. For many
years there has been disagreement about the mode by which
H. sapiens originated and came to populate the world and
about the explanation for the geographic differences in
phenotype seen in people from different regions today (see
for example Stringer (2014) for an overview of contrasting
models). Since the late 1980s, this disagreement has been
popularly distilled into the dichotomy between Recent
African Origin (RAO) and Multi-regionalism. Adherence to
these models leads to very different characterizations of the
species H. sapiens.
The idea of gradual, regional evolution of humans like
ourselves from local archaic populations is associated histor-
ically with Hrdlicka, Weidenreich, Coon and Brace (Stringer,
1994), but in its modern incarnation as Multi-regionalism,
it has largely been promulgated by Wolpoff and colleagues.
Multi-regionalists view all Homo from, and including,
H. erectus as one species (Wolpoff et al., 1994; Wolpoff &
Caspari, 1997a) and, if H. erectus and H. sapiens are
combined, the name H. sapiens has priority (Wolpoff &
Caspari, 1997b). Thus, the Multi-regionalist paradigm pro-
poses a single, polytypic H. sapiens species evolving regional
Correspondence: Laura Tabitha Buck, Natural History Museum,Cromwell Road, London SW7 5BD, UK. Tel: 020 7942 7004. E-mail:[email protected]
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variations from 41 Ma onwards, with significant gene
flow between regions preventing speciation. In this
view species can only be created by cladogenesis and the
cladogenetic event in this case was the origin of the genus
Homo, however much variation this might require the
resultant species to contain (Wolpoff et al., 1994;
Wolpoff & Caspari, 1997a).
During the last 25 years the model that has usually been
regarded as the antithesis of Multi-regionalism is the Recent
African Origin (RAO) model. As the name suggests, this
model posits that H. sapiens originated in Africa relatively
recently and subsequently spread out to inhabit the rest of the
world, replacing existing archaic populations in each region.
The date of origin of H. sapiens in this model has changed in
the face of new discoveries and dating work. Initially it was
placed at �100 ka, but dates for the appearance of ‘‘anatom-
ically modern humans’’ (that is to say fossils that are
demonstrably closer to living humans in morphology than to
any other species) in the fossil record now lie at �200 ka,
while the origin of the lineage of H. sapiens could be much
further back, at �400 ka (Stringer, 2012a). Although initially
vague in terms of the mode of speciation, at times there has
been an emphasis on punctuationalism, cladogenesis and the
importance of a late bottleneck by some advocates of RAO
(Stringer, 2002).
There have, of course, been many intermediate viewpoints
between these two extremes, which have tended to be
simplified to highlight the contrasts between the models and
their protagonists. Brauer’s (African) Hybridization and
Replacement model, for example, combines RAO with a
degree of regional interbreeding between Africa-derived
H. sapiens and other hominin populations (e.g. Brauer,
1992, 2011), but he advocates a wider diagnosis of the
species, classifying both Middle Pleistocene Africans and
Neanderthals as ‘‘archaic H. sapiens’’. Multi-regionalism in
the strict or classic sense, as described above, has been
modified over the years in response to new data and today,
whilst its advocates would still argue for substantial and
widespread gene flow in the Pleistocene as the major impetus
behind the evolution of H. sapiens, many would admit that
Africa has been the principal source of genetic input.
A formalized version of this viewpoint is Smith and
Trinkaus’ Assimilation model (Smith, 1992; Trinkaus, 2005).
Improvements in dating over the last few decades have
enabled clarification of the chronology of recent human
evolution, showing there was a co-existence or alternation of
H. sapiens and Neanderthals in Israel, disproving the idea that
Neanderthals in Eurasia always preceded H. sapiens
(Grun et al., 2005). Genetic analyses also provided important
support for RAO, by showing that an African origin was the
most parsimonious explanation for the fact that non-African
genetic variation is largely a sub-set of that seen in Africa.
These advances led to a decline in the popularity of Multi-
regionalism and the pre-eminence of RAO models. For the
last two decades, the most popular view of H. sapiens has
been that of an African species that originated during the
Middle Pleistocene and which can be differentiated from
other Pleistocene species such as Neanderthals and H. erectus,
whom they are thought to have replaced on their dispersal out
of Africa.
Recently, however, new genetic data have shown that
extant H. sapiens did not derive purely from an African
origin, demonstrating multi-regional contributions to the
recent human gene pool. There is now evidence for inter-
breeding between both Neanderthals and H. sapiens and
between Denisovans and H. sapiens (see below). Thus, the
importance of a greater degree of genetic input from other
species has had to be accepted by those who favour RAO and
in some quarters there is renewed interest in Multi-regionalist
ideas (Finlayson, 2013; Hawks, 2010; Stringer, 2014).
Likewise, the greater numbers of fossils now available has
sometimes complicated issues of taxonomy rather than
simplified them (e.g. Hublin, 2014; Lordkipanidze et al.,
2013; Spoor, 2013) and we are still far from an agreement on
what constitutes H. sapiens in the past.
A definition of H. sapiens based on recent variation
One of us (CS) found from his doctoral research that certain
cranial angles and indices convincingly separated a group of
recent H. sapiens, Upper Palaeolithic H. sapiens and fossils
such as Skhul and Omo Kibish 1 from Neanderthals and other
‘‘archaic’’ groups (Stringer, 1974) and, thus, became inter-
ested in a morphological diagnosis of Homo sapiens. Using
measurements from Howells’ (1973) database, he formulated
the idea of using the range of recent H. sapiens variation to
diagnose H. sapiens in the fossil record. Fossils that fell
within the range of recent variation could be classed as
H. sapiens, while those that did not, by implication, would not
represent this species. Using Howells’ and his own data,
Stringer (1974, 1978) attempted to encapsulate key H. sapiens
traits such as a domed neurocranium, reduction in facial size
and projection, and increased basicranial flexion. Based on
these characteristics, Day & Stringer (1982) formulated what
they termed a ‘‘working definition’’ for H. sapiens
(Day & Stringer, 1982: 835). The purpose of this was to
test whether the Omo 1 fossil from Ethiopia should be
included in H. sapiens sensu stricto, as Stringer (1974, 1978)
had argued, or in a Neanderthal grade, as asserted by workers
such as Brose & Wolpoff (1971). Omo Kibish in Ethiopia is
key in diagnosing H. sapiens in the fossil record, as it is one of
the earliest known H. sapiens sites. It is also intriguing
because of the degree of morphological disparity between two
crania found there, Omo 1 and Omo 2. Omo 1 was found
partially in situ and in association with extinct fauna, whereas
Omo 2 was a surface find from �2.5 km away, thus
the relationship between the two specimens is unclear
(Day & Stringer 1982). Despite the lack of context for Omo
2, both specimens have been argued to date from �195 ka
(Shea et al., 2007), with this age for Omo 1 supported
by direct uranium series dating (Aubert et al., 2012).
However, there are many differences between the two crania
in features such as neurocranial globularity and occipital
morphology.
To see if Omo 1 could be included in H. sapiens sensu
stricto, Day and Stringer formulated a list of criteria for the
species based on the presence of putative shared H. sapiens
characteristics. The authors noted that the features used to
define H. sapiens sensu stricto would not be found in all
extant specimens, but suggested that the majority should be
DOI: 10.3109/03014460.2014.922616 Diagnosing Homo sapiens in the fossil record 313
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present. In addition, they acknowledged that some of the
features might also be found in non-H. sapiens fossils. They
suggested that a fossil should have over 50% of the diagnostic
features to be classed as H. sapiens. Based on this list it was
concluded that Omo 1 was H. sapiens sensu stricto, while
Omo 2 was not. In fact, in some aspects of morphology, the
latter fossil more closely resembled H. erectus than H.
neanderthalensis or H. sapiens (Day & Stringer, 1982). The
criteria chosen in the paper were deliberately strict in order to
be conservative regarding the inclusion of the fossil Omo
specimens in H. sapiens. They were never intended for the
diagnosis of large samples of recent H. sapiens based on
single traits, since it was recognized that not all recent
humans would display all of the characteristics.
The provisional 1982 criteria were subsequently modified
in recognition of their under-estimation of the amount of
variation in the species (Day & Stringer, 1991; Stringer et al.,
1984), but when the original criteria were tested by other
researchers on populations of recent H. sapiens, some of the
characteristics were found to be problematic (Lahr, 1996;
Lieberman et al., 2002; Wolpoff, 1986). Lahr (1996) found
that some recent populations fell outside the ‘‘modern’’ range,
as defined by Day & Stringer (1982) for some criteria, and
she concluded that this showed this diagnosis of H. sapiens
was insufficiently broad. In particular, she found the required
frontal angle for inclusion in H. sapiens was defined too
narrowly with, for example, her Fuegian/Patagonian sample
mean falling outside the range given by Day and Stringer
(Lahr, 1996). Wolpoff (1986) also found that several
Australian fossil crania did not meet the criteria, although
there was no question that they were H. sapiens. He wrongly
suggested that there was a Euro/African bias in the definition,
but this was refuted by Lahr (1996), who found the
problematic criteria were spread among different populations,
including Europeans.
A more comprehensive fossil record also began to show
glimpses of the much greater variation that had existed even
in the recent past. This included fossils such as Kow Swamp,
Willandra Lakes and Coobol Crossing from Australia and
Kennewick Man from North America. Only a sub-sample of
this variation continues in the present day, perhaps due to
population extinction events and homogenization within
Homo sapiens during the last 15 000 years. The need to
include earlier variation in any diagnosis of H. sapiens was
clear. Stringer’s subsequent phenetic analyses showed how it
was possible to look at differences between fossils as a whole,
rather than at individual characters and to see that, following
their divergence from the last common ancestor (LCA),
Neanderthals and H. sapiens had changed in different ways,
with globularization of the neurocranium and reduction in
face size predominating on the H. sapiens lineage and an
increase in neurocranial size and a change in facial shape
(with an increase in mid-facial prognathism) predominating
on that of the Neanderthals (Stringer, 1978, 1994).
Schemes such as that of Day & Stringer (1982) used all
the chosen criteria with equal weighting in their comparisons
of different taxa, but the expression of some traits may be
due to homoplasy or plasticity, and some are clearly
correlated with each other. Cladistics teaches us that only
synapomorphies (shared, derived characteristics), identified
with reference to one or more outgroups, should properly be
used to define relationships. An organism’s skeleton is able
to adapt to its environment during its lifetime due to
remodelling in response to strain and some regions are more
plastic than others, depending on levels of canalization
(Buck et al., 2010); thus some skeletal traits should be
treated with caution. The phylogenetic utility of a plastic
region should not be discounted out of hand, however. Von
Cramon-Taubadel (2009) has shown that masticatory regions
of the cranium are more plastic than non-masticatory
regions, as would be expected, but they are nonetheless no
less effective at reconstructing human population history.
It may also be profitable to consider the ontogeny of
different features. A mental eminence, or chin, is present (in
variable form) in Neanderthal and Paranthropus boisei
fossils (Schwartz & Tattersall, 2000; Wolpoff, 1986).
However, it is not seen in juveniles, whereas a chin is
always present in H. sapiens from an early age (Schwartz &
Tattersall, 2000). Not all traits are equally informative;
therefore, this is something that should be taken into account
in building species diagnoses.
Branches or tips?
Even if it is agreed, based on RAO, that H. sapiens is a recent
species, distinct from Neanderthals and from the probable
LCA, H. heidelbergensis, at what point do we define the cut-
off for H. sapiens? Should only the tips of the phylogenetic
tree be designated H. sapiens (or indeed H. neanderthalensis);
should the hypodigm contain only those individuals that
display all the traits diagnostic of that species or should there
be a looser definition (see Figure 1)?
One option would be to diagnose H. sapiens by compari-
son with H. neanderthalensis, i.e. to define as belonging to
H. sapiens anything on the H. sapiens lineage after the split
with the LCA of Neanderthals and H. sapiens (e.g. Stringer,
2002). The draw-back of this approach is that there is a great
deal of morphological variation in fossils that most would
agree lie on the H. sapiens lineage, after the split with
H. neanderthalensis. Not only do diagnostic H. sapiens
features not appear all at once, as a complete package, but,
where they appear, they appear in different combinations (see
below). This being the case, the question is what to do with
specimens that fall between the LCA and those specimens
that have the full suite of H. sapiens characteristics. The term
‘‘archaic H. sapiens’’ has been something of a conceptual
dustbin, often being used for specimens alternatively referred
to H. heidelbergensis or H. neanderthalensis, but one of us
(CS) has favoured using it to designate those members of the
H. sapiens lineage that lack a majority of the traits charac-
teristic of the living taxon. This term is then often juxtaposed
with the term ‘‘modern’’ H. sapiens. However, this is
potentially confusing due to the semantic baggage of the
word ‘‘modern’’, which may also imply behavioural/cognitive
criteria as well as morphological ones. Although this
difficulty may be avoided by the popular term ‘‘anatomically
modern’’ H. sapiens, this term can also carry its own baggage
with the implication that ‘‘modern’’ H. sapiens are somehow
an improvement on past populations and that evolution is
progressive.
314 C. B. Stringer & L. T. Buck Ann Hum Biol, 2014; 41(4): 312–322
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Another option which CS previously favoured (as dis-
cussed above) was to limit the use of H. sapiens to those
specimens that display the full suite of H. sapiens traits and
separate those ‘‘H. sapiens’’ that only show some of the
required traits as a separate species. The same usage could
also be applied to separate ‘‘classic Neanderthals’’ and those
fossils that show some, but not all H. neanderthalensis traits.
If this scheme is followed, the name with priority for the
species intermediate between H. heidelbergensis and
H. sapiens would probably be H. helmei (Stringer, 1996)
[this application of the species named from the Florisbad
cranium is distinct from the subsequent usage by Foley &
Lahr (1997)] and the equivalent designation for specimens
intermediate between H. heidelbergensis and H. neandertha-
lensis would probably be H. steinheimensis (see Figure 1[A]).
Yet to use these distinctions merely atomizes the problem
rather than solving it; unless there is truly punctuational
change, populations diverge by degrees and there will always
be intermediates between any two taxa. In this case it would
be very difficult to separate H. steinheimensis and
H. neanderthalensis based on morphology. Neanderthal
traits seem to appear relatively gradually in the fossil record
with specimens such as Swanscombe, Steinheim and Sima de
los Huesos exhibiting different mosaics of Neanderthal
characteristics (Stringer, 2002), much as early African
H. sapiens display variable H. sapiens characteristics
(see below). Differentiating them from the LCA and from
the terminal taxon therefore becomes rather arbitrary.
To call these indeterminate specimens ‘‘early H. sapiens’’
and ‘‘early H. neanderthalensis’’ is another option (see
Figure 1[B]), which, although it lacks taxonomic precision, is
perhaps most representative of the biological reality. The
conceit of species as a series of totally distinct, homogenous
entities may be helpful when considering fossil phylogeny,
but a series of over-lapping, interbreeding and slowly
diverging populations is closer to what we actually see in
living species (Ackermann, 2010; Jolly, 2001; Kelaita &
Cortes-Ortiz, 2013). The early parts of both the H. sapiens
and H. neanderthalensis lineages show some of the lost
diversity that once existed and both will contain groups not
ultimately ancestral to later members of either species.
If these terms are employed it logically follows to refer
to ‘‘recent’’ or ‘‘late H. sapiens’’ and perhaps also to ‘‘late
H. neanderthalensis’’.
A purely morphological diagnosis?
It has been argued that Homo species are different from other
animal species, that they are a special case because of their
great behavioural flexibility and unique reliance on culture
(e.g. Wolpoff & Caspari, 1997a). Can we only truly define our
species based on a combination of behavioural and morpho-
logical traits? This is a question that has engendered much
debate and which has, to a certain extent (excepting Wolpoff
and Caspari), been split along disciplinary lines, with
palaeoanthropologists and archaeologists both proclaiming
the primacy of their particular area of interest. It is also at the
crux of the previously discussed issue as to whether there is
a distinct difference between recent or ‘‘modern’’ H. sapiens
and the rest of our lineage post-dating the split from the LCA
with H. neanderthalensis.
What constitutes ‘‘H. sapiens behaviour’’ is at least as
nebulous a concept as what constitutes ‘‘H. sapiens anat-
omy’’. Traditional markers of recognizably ‘‘modern’’ H.
sapiens behaviour have been said to include:
Increasing artefact diversity; standardization of artefact
types; blade technology; worked bone and other organic
materials; personal ornaments and ‘art’ or images;
structured living spaces; ritual; economic intensification
reflected in the exploitation of aquatic or other resources
that require specialized technology; enlarged geographic
range; [and] expanded exchange networks (McBrearty &
Brooks, 2000: 491).
The arrival of this complex of behaviours has been termed a
Human Revolution (Mellars & Stringer, 1989) and its
description was initially focused on the beginning of the
European Upper Palaeolithic. In that context and at
that time, the term described the seemingly sudden appear-
ance of these complex behaviours about 35 ka (Mellars &
Stringer, 1989).
Figure 1. (A) H. sapiens andH. neanderthalensis as species representedonly at the tips of the phylogenetic tree, thoseindividuals with all the traits judged to bediagnostic. H. helmei and H. steinheimensisas intermediate species between eachterminal species and last commonancestor (LCA), here suggested to beH. heidelbergensis. (B) Looser definitions ofH. sapiens and H. neanderthalensis includingall populations after the split from the LCA.Both species encompass considerablemorphological variation along their lineagesand populations which go extinct withoutissue. The overall topography of the bothtrees and the estimated divergence and LCA‘‘dates’’ are derived from a study of wholemtDNA genomic data (Stringer 2012c).
DOI: 10.3109/03014460.2014.922616 Diagnosing Homo sapiens in the fossil record 315
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Despite the intuitive appeal of the Revolution idea, the
development of so-called modern behaviour, as with
‘‘modern’’ morphology, actually seems much more piece-
meal. It appears in the fossil record in fits and starts in
different places at different times, not as a package tied to
anatomical ‘‘modernity’’. As such it can be argued that
‘‘modern’’ human behaviour loses its utility as a diagnostic
criterion for the physical species. Indeed, there are strong
arguments against the conflation of behaviour and morph-
ology. At one extreme, for Klein (2000, 2008), the two were
completely decoupled so that ‘‘morphological modernity’’
appeared at least 100 ka before the punctuational appearance
of ‘‘behavioural modernity’’, said to be the result of novel
genetic mutations affecting the brain about 50 ka. Some
aspects of ‘‘modern’’ behaviour, however, certainly seem to
have been present in earlier H. sapiens populations at
�100 ka, for example the shell beads, ochre use and burial
behaviour from Skhul and Qafzeh (Bar-Yosef Mayer et al.,
2009; Salomon et al., 2012; Vanhaeren et al., 2006). In fact,
the early emphasis on Europe seems to have been more a
construct of the history of archaeology than a record of
exceptional behaviour in Europe (McBrearty & Brooks,
2000). As earlier and earlier examples of ‘‘modernity’’
emerged from Africa, this material was incorporated into the
Revolution theory, such that the birth of H. sapiens behaviour
might indeed have been more closely coeval with the birth of
anatomical H. sapiens in Africa at �200 ka (McBrearty &
Stringer, 2007).
Increasingly there is potential evidence for some of the
supposed hallmarks of behavioural ‘‘modernity’’ in other
species, particularly in Neanderthals. These include the use of
pigments (Zilhao et al., 2010); the possible symbolic use of
feathers (Finlayson et al., 2012; Peresani et al., 2011); dietary
breadth and diversification (Stringer et al., 2008); the
generally accepted evidence for intentional burial (e.g.
Rendu et al., 2013); and the much-disputed Chatelperronian
industry (e.g., Bailey et al., 2009; Bar-Yosef & Bordes, 2010;
Higham et al., 2010; Zilhao et al., 2006). Although not all
of these findings are universally accepted as evidence of
complex cognition, taken as a whole, they represent the slow
dissolution of a profound symbolic and technological demar-
cation between the behaviour and cognition of H. sapiens and
H. neanderthalensis (d’Errico & Stringer, 2011). Conversely,
where anatomically ‘‘modern’’ human remains are found,
they are not necessarily found in conjunction with evidence
for the whole ‘‘modern’’ human behavioural package. The
best example of this is in Australia, where as far as we know
only fully ‘‘modern’’ humans have ever lived, but where the
archaeological record apparently lacks consistent signals of
the supposed signature of behavioural ‘‘modernity’’ until well
into the Holocene (Brumm & Moore, 2005; but compare
O’Connell & Allen, 2007).
As Stringer (2002) has noted, using technology as a
taxonomic character is fundamentally ill-advised as it can be
passed between reproductively isolated populations or even
species. Based on the evidence now available, behaviourally
‘‘modern’’ H. sapiens seems too loose a concept to be of
much practical use. In the same way that morphological traits
indicative of H. sapiens are seen to appear (and at times
disappear) piecemeal in the fossil record, such is the case with
the behavioural evidence. Furthermore, some behaviours
argued to be definitively those of H. sapiens are both found
in other species and not found in some indisputably
H. sapiens populations. Although there is clearly a biological
component to behavioural capacity, behaviour in humans is
dominantly a learnt attribute and as such should not be used
to define hominin species. We know from ethnology (for
example, historical hunter-gather groups who lost their
previous abilities to make sea-going boats or fire) that
cognitive and behavioural capacities are not equivalent to
the practice of any given behaviour. Thus, even if there is such
a thing as a distinct human behavioural complex, we cannot
use the archaeological record to definitively prove its absence.
As discussed above, the lack of an absolutely distinct complex
of behavioural and morphological traits that characterizes
‘‘modern’’ H. sapiens makes this without doubt a problematic
concept, which may be made clearer by referring instead to
‘‘recent’’ H. sapiens.
Early H. sapiens in Africa
There is wide variation in fossil humans associated with
Middle Stone Age (MSA) archaeology in Africa, with
material from sites such as Singa (Sudan), Omo Kibish,
Herto (both Ethiopia), Ngaloba (Tanzania), Jebel Irhoud, Dar-
es-Soltane (both Morocco), Eliye Springs, Guomde (both
Kenya) and Florisbad (South Africa), all showing different
combinations of primitive and derived (recent H. sapiens-
like) traits. For some of the more complete specimens a
morphological progression can be suggested between Middle
Pleistocene fossils and recent H. sapiens—for example the
BOU-VP-16/1 cranium from Herto. Although this fossil is
primitive-looking in its occipital shape and the strong
supraorbital tori, it also has derived features not seen in
Mid-Pleistocene African hominins such as Broken Hill and
Bodo. These include a more globular neurocranium and
retracted face, which ally it to H. sapiens (Stringer, 2003;
White et al., 2003). White et al. (2003) concluded that Herto
is morphologically intermediate between more primitive
specimens such as Broken Hill, which they dated to
�500 ka, and more derived specimens from �100 ka, but
they also noted that the Herto material does not represent the
only possible intermediate between H. heidelbergensis and
recent H. sapiens.
A combination of the morphology exhibited by Omo 1 and
2 would provide a different model of H. sapiens evolution
from that suggested by Herto, as exemplified by the ER-3884
cranial material from Guomde, displaying another mix of
primitive and derived characteristics that might plausibly have
led to the morphology of recent H. sapiens. These potential
variations on the H. sapiens theme show that there is unlikely
to be a simple, linear relationship between H. heidelbergensis
morphology and H. sapiens morphology. Alternatively, the
variation between Omo 1 and 2 might reflect the co-existence
of two morphologically distinct populations at that time in
Ethiopia (Stringer, 2002, 2012b). It appears that evolution
progressed separately in different populations, morphological
structure at population level leading to a gradual coalescence
of the full suite of H. sapiens characteristics analogous to
that seen in the genetic data. This has been referred to as
316 C. B. Stringer & L. T. Buck Ann Hum Biol, 2014; 41(4): 312–322
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an African multi-regionalism, describing the evolution of
regional differences within the continent and between many
inter-fertile sub-divisions of one variable evolving species
(Stringer, 2003, 2012a). The same may have been the case for
Neanderthals in Eurasia too; the gradual but not always
precisely ordered accretion of Neanderthal synapomorphies
can be seen in fossils such as Swanscombe, Steinheim and the
Sima de los Huesos remains (Hublin, 2007).
As discussed above, study of MSA-associated human fossils
shows their great morphological variation, while the available
(if imperfect) chronological control provides only limited sup-
port for the idea of an ordered progression from ‘‘less H.
sapiens’’ to ‘‘more H. sapiens’’ through time. Instead we see
very varied fossils apparently juxtaposed in close temporal
proximity (Stringer, 2012b). Moreover, there is growing
evidence of the survival of early sapiens morphology into the
late Pleistocene at sites like Eyasi (e.g., Brauer, 2011) (see
below), while a key H. heidelbergensis specimen, Broken Hill
1, may well date to the late Middle Pleistocene, within the time
range of the MSA (Stringer, 2012b).
Synthesizing these various developments suggests that the
mechanism for the evolution of H. sapiens traits in different
places at different times could have been repeated population
fluctuations resulting from glacial/inter-glacial and shorter cli-
matic cycles. Such oscillations could have led to the creation/
removal of biogeographical barriers such as the expansion and
contraction of tropical rainforests, or of the Sahara Desert
(Stringer, 2012b). The greening or re-desertification of the
Sahara is likely to have been important for contact between
populations in northern and tropical Africa, facilitating or
preventing expansions. Fluctuations in rainfall would have
similarly created or removed green pathways connecting
populations in tropical and southern Africa (Blome et al.,
2012; Coulthard et al., 2013), whilst also forming barriers of
dense tropical rainforest at times, which were probably
impenetrable to early humans. This would have had direct
demographic effects on human populations, leading to periods
of isolation and even regional extinctions, followed by periods
of dispersal into new habitats or re-occupation of old ones.
The use of refugia into which populations could retreat to
survive the worse of climatic down-turns has been suggested
as a key catalyst of adaptive behavioural changes (Stewart &
Stringer, 2012), but equally it can be argued that climatic
ameliorations were important in fuelling denser, networked
populations, thus facilitating genetic and cultural change
(Stringer, 2012b; Ziegler et al., 2013). The result of these
processes culminated in the composite we call recent
H. sapiens, genetically, morphologically and behaviourally,
but there was never a single centre of origin.
Hybridization in Africa?
It is not only in MSA Africa that the H. sapiens fossil record
is highly variable, complicating interpretations of relation-
ships and species definitions. As mentioned above, there are
also a number of relatively recent African sites with fossils
that exhibit combinations of recent H. sapiens and more
primitive traits, allying them to much older specimens.
Stringer found the Iwo Eleru fossil from Nigeria to be
idiosyncratic in his doctoral research, where it showed
affinities with Ngandong, Saccopastore and Omo 2 (which
are disparate in time, space and inferred taxonomic position),
as well as with recent H. sapiens. This result highlighted the
unusual combination of traits seen in the fossil (Stringer,
1974). It was recently confirmed as dating to the very end of
the Pleistocene (�11.7–16.3 ka) (Harvati et al., 2011);
however, it is morphologically unlike recent African crania
(Harvati et al., 2011, 2013; Stringer, 1974). Despite its late
date, in geometric morphometric comparisons with a wide
range of extant crania, Iwo Eleru falls outside the range of
recent African variation and groups instead with the much
older Elandsfontein and Ngaloba fossils from Africa and with
Skhul and Qafzeh from Israel (Harvati et al., 2011, 2013). The
Ishango fossils from the Democratic Republic of Congo are
slightly older than Iwo Eleru (�20 ka), but, interestingly,
morphometric characteristics and dental size also place them
at the edge of extant African diversity and their inner ear
morphology appears more like that of Middle Palaeolithic
hominins than those of H. sapiens of comparable age
(Crevecoeur et al., 2010). These specimens from Central
and West Africa emphasize how little we know about the
fossil record of large swathes of the continent. They have also
been suggested as evidence of population sub-structure and
the late retention of great morphological diversity in
our species, possibly as a result of hybridization between
H. sapiens and an archaic hominin species, perhaps
H. heidelbergensis (Hammer et al., 2011; Harvati et al.,
2011; Stringer, 2012a,b,c).
Hammer and colleagues’ work on recent African nuclear
DNA shows traces of recent (550 ka) archaic introgression in
Africa from a population that split from the ancestors of
recent H. sapiens at �700 ka (Hammer et al., 2011). They
suggest at least one introgression event could have taken place
in Central Africa [see also Lachance et al. (2012)]. Ishango
notwithstanding, there is virtually no fossil record from this
region, so it is difficult to even speculate about the source of
this introgression. There is also new evidence of an ancient Y
chromosome lineage in West Africa, increasing the estimated
coalescence date for the Y chromosome in H. sapiens to 237–
581 ka (Mendez et al., 2013). As this matches or exceeds the
age of the oldest known H. sapiens fossils, it has been
suggested that the early date could also reflect introgression
from a now extinct species (Mendez et al., 2013).
Hybridization in Eurasia
In the years since the first publication of a relatively high
quality Neanderthal nuclear genome in 2010, it has become
accepted that most extant H. sapiens populations from outside
sub-Saharan African have �2% Neanderthal-derived DNA
(Green et al., 2010). The amount of introgression varies
between populations, with a greater extent observed in Chinese
and Japanese populations (Wall et al., 2013), but this disparity
now appears to be smaller than previously indicated and could
be due to the differential effect of drift acting on separate
populations across Eurasia (Prufer et al., 2014) or to multiple
hybridization events (Vernot & Akey, 2014). Traces of
Neanderthal-derived DNA have even been observed in East
African Maasai and elsewhere in sub-Saharan Africa, but since
there is no evidence that Neanderthals ever lived in Africa, it is
DOI: 10.3109/03014460.2014.922616 Diagnosing Homo sapiens in the fossil record 317
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most parsimonious to suppose that this introgression derives
from back-migrations from Eurasia (Meyer et al., 2012;
Pickrell et al., 2014; Wall et al., 2013).
In 2010 it was also shown that some populations in south
east Asia and Oceania have an additional component of
introgression, from the Denisovans. This group has so far only
been identified from its DNA, which showed it to be
neither Neanderthal nor H. sapiens (Krause et al., 2010).
The Denisovans seemed at first to be a sister group to
H. sapiens/Neanderthals based on mtDNA (Krause et al.,
2010), but when nuclear DNA was sequenced they were
shown to be more closely related to Neanderthals (Reich
et al., 2010). Although Denisovan remains are so far only
known from Siberia, levels of diversity between the known
mitochondrial genomes suggest that their population size may
have been historically greater than that of the Neanderthals
and, by inference, they were probably once widespread
through south east Asia (Cooper & Stringer, 2013). This fits
with the finding that Denisovan-like DNA is largely found
in extant H. sapiens across the Wallace Line, with the highest
percentage in New Guinean and Australian aborigines, at
�4% (Cooper & Stringer, 2013). Furthermore, recent research
shows that the source of this introgressed DNA was a distinct
sub-population of Denisovans from the one known from
Siberia (Prufer et al., 2014).
Prufer et al. (2014) have now shown that interbreeding also
occurred between Neanderthals and Denisovans and possibly
between the Denisovan lineage and an unknown archaic
hominin. The more we find out, the more it seems that inter-
breeding between taxa was common, albeit at relatively low
levels. The amount of Neanderthal (and Denisovan) DNA in
extant H. sapiens populations is small, which could reflect
relatively few matings, but recent evidence instead suggests
that there was only limited reproductive compatibility
between the two species, despite their evolutionary closeness
(Sankararaman et al. 2014), a scenario which is also
compatible with the lack of mtDNA introgression (Currat &
Excoffier, 2011). This incompatibility seems to have been
particularly related to reduced male fertility and our genes
still show the signs of selection to remove Neanderthal
genetic components responsible for this reduction
(Sankararaman et al., 2014). Of course other barriers to
cross-species breeding, such as low population densities,
geographic and cultural boundaries may also have contributed
to the low component of Neanderthal DNA seen in H. sapiens
today (Currat & Excoffier, 2011). The relatively low levels of
Denisovan DNA on the X chromosome of those H. sapiens
populations where it is present may tell a similar story of
limited inter-fertility (Meyer et al., 2012). Despite the on-
going complications involved in a morphological diagnosis,
it is evident that genetic characterization of our species vs
others is increasingly feasible.
The effect of inter-breeding on phenotype
What effect would inter-breeding with an extinct species have
on phenotype? Based on the evidence so far, the amount of
introgressed DNA originating from Neanderthals and
Denisovans is small and may not be expressed in any of the
gross morphological features of H. sapiens. Some functional
genes are known to be included in Neanderthal-derived DNA,
but so far nothing has been reported that relates to significant
changes in skeletal anatomy. Regions of the H. sapiens
genome that show high levels of selection to retain
Neanderthal genetic input are engaged in such activities as
the building of keratin and sugar metabolism (Sankararaman
et al., 2014). It has been suggested that Neanderthal DNA in
these regions could have been advantageous in helping
H. sapiens to adapt to non-African environments
(Sankararaman et al., 2014; Vernot & Akey, 2014), but
it has also been shown that several alleles associated with
disease risk in H. sapiens seem to be correlated with
the presence of Neanderthal DNA (The Type 2 Diabetes
Consortium, 2013; Sankararaman et al., 2014; Vernot &
Akey, 2014).
It seems unlikely that much of the claimed skeletal
evidence of hybridization that has regularly been cited (e.g.
Trinkaus, 2005, 2011) is really a reflection of introgressed
DNA, not least because several examples date from long after
the time of hypothesized inter-breeding, when levels of
introgressed DNA had probably already fallen away. This
assertion is supported by Fu et al.’s (2013) finding that
Tianyuan (dated to �40 ka) apparently has no more
Neanderthal DNA than extant Chinese people, despite its
supposedly archaic features. In any case, the evidence from
other primate species is that the effects of hybridization are
complex, difficult to interpret and may even be cryptic,
particularly if the specimen in question is not a first
generation hybrid (Ackermann, 2010; Kelaita & Cortes-
Ortiz, 2013).
Conclusion
Based on current research, there are evidently genetic traces
of inter-breeding with at least three extinct human groups. We
can truly be said to be a genetic ‘‘patchwork’’ (Stringer,
2012a), but what does this say about the definition of
H. sapiens? Does some degree of inter-fertility necessarily
falsify a specific difference? Of course the answer to this
question depends on the species definition and, using a strict
biological species concept, the answer would be yes.
However, the utility of this concept for fossil species is
questionable, since in most cases it is impossible to test and
its strict use would negate many currently accepted extant
species divisions as well. Within the primate order there are
many hybridizations in the wild and in zoos between long-
accepted species (Ackermann, 2010; Jolly, 2001; Kelaita &
Cortes-Ortiz, 2013, also reviewed by Winder & Winder, this
volume); indeed Jolly (2001) estimates that inter-fertility
could exist between species up to 4 Ma after their divergence.
Clear and impermeable species divisions may be a useful way
of thinking about the fossil record, but this does not
correspond to biological reality. As Jolly (2001: 129) stated
in comparing the taxonomy of recent papionins and of fossil
hominins,
The message . . . is to concentrate on biology, avoid
semantic traps and realize that any species-level taxonomy
based on fossil material is going to be only an approximate
reflection of real-world complexities.
318 C. B. Stringer & L. T. Buck Ann Hum Biol, 2014; 41(4): 312–322
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Morphometric comparisons of differences in cranial shape
show Neanderthals and H. sapiens (both recent and Upper
Palaeolithic) to be more different than Pan troglodytes and
Pan paniscus (Harvati, 2003) and comparable to differences
found between many other primate species (Harvati et al.,
2004; Lordkipanidze et al., 2013; Stringer, 2012a,b).
Uniting H. sapiens and H. neanderthalensis would also
lack any morphological coherence, since a species
combining Neanderthals and H. sapiens would be diagnosed
simultaneously by a long, low neurocranium and a
high globular neurocranium; by large, continuous supraorbital
tori; and by no continuous supraorbital tori, etc. (Stringer,
2014). This certainly appears unworkable as a species
diagnosis.
Nevertheless, fossil and genetic evidence compiled over
the last few decades show H. sapiens to be a morphologically
variable species and it may, thus, seem that there are not
sufficient features in common to form a cohesive whole.
However, it is important to distinguish between shared species
level traits, which can be seen (in various combinations) in the
fossil record going back hundreds of thousands of years
(derived from a recent African origin) and regional or
‘‘racial’’ traits (added subsequently). The latter category is
largely due to the combined effects of natural selection, drift,
founder effect and sexual selection operating over only the
last 60 ka. H. sapiens share specific traits including a high,
round neurocranium, small face, true chin, small supraorbital
tori and gracile skeleton, but recent H. sapiens from different
regions may also vary further in body shape, skin and hair
colour and the form of the hair, nose, eyes and lips. These
regional traits could potentially be affected by some degree
of archaic introgression, but the evidence so far is that the
phenotypic effects of this are small.
While it certainly seems problematic to cleanly delineate
morphologically recent H. sapiens, anatomical characteriza-
tion of the Homo sapiens lineage should still be possible from
features such as cranial globularity, basicranial flexion, dental
microstructure, inner ear morphology and pelvic shape. The
shape of the parietal region in H. sapiens seems particularly
distinctive (Bruner, 2010; Stringer, 1974, 1978, 2002) and
makes a significant contribution to cranial globularity in both
lateral and occipital views. Basicranial flexion is a complex
feature, but H. sapiens certainly appears distinctive in various
measurements of this (Bastir et al., 2010; Lieberman et al.,
2002). Dental microstructure, especially with the advent of
micro-CT and synchrotron technology, is also revealing clear
differences between early and recent H. sapiens and other
hominin species, in features such as enamel thickness and the
shape of the enamel dentine junction (Crevecoeur et al., 2014;
Smith et al., 2012). Inner ear morphology has long been
recognized as distinguishing between H. sapiens and
H. neanderthalensis, but recent research is increasing reso-
lution, which should also allow discrimination between
H. sapiens and species such as H. heidelbergensis and
H. erectus (Spoor, 2013). Pelvic morphology clearly differ-
entiates an anatomically recent H. sapiens pattern that was
present by at least 100 ka at Skhul and Qafzeh (Rak, 1990),
but the problem here is that the lack of African post-cranial
fossils from the Middle Pleistocene prevents any determin-
ation of when this pattern first appeared.
The discovery of a large sample of Middle Pleistocene
humans in the Sima de los Huesos, Atapuerca (Arsuaga
et al., 1990, 1993; Martinon-Torres et al., 2012) and of
several penecontemporaneous, but distinctive crania from
Dmanisi in Georgia (Gabunia & Vekua, 1995;
Lordkipanidze et al., 2013; Vekua et al., 2002) shows
how little of intra-population variation is typically sampled
in the fossil record. In the case of the Sima sample this has
led to much discussion about its classification (e.g. Gracia-
Tellez et al., 2013; Stringer, 2012c) and, in the case of
Dmanisi, there had been debate over whether the specimens
could all belong to the same species. It has recently been
argued that their level of variation does not exceed that
found in recent H. sapiens or chimpanzees and that it,
therefore, is justifiable to place them in a single species
(Lordkipanidze et al., 2013). Based on the level of variation
described at Dmanisi, the authors went even further in
suggesting that there was insufficient variation in the
African record of early Homo to designate multiple species.
They therefore suggested the sinking of species such as
H. rudolfensis and H. habilis into a polytypic H. erectus
(Lordkipanidze et al., 2013). This conclusion has been
criticized on the grounds that the authors made no attempt
to distinguish between primitive and derived characters, did
not consider the post-cranial evidence (Spoor, 2013) or the
dental evidence and included elderly (edentulous) and
juvenile crania (Hublin, 2014). In addition there was use
of an overly general landmark set for geometric morpho-
metric analyses, which fails to fully distinguish between
some extant non-human primate species (Hublin, 2014). It
has also been asserted that Dmanisi has derived H. erectus
traits not seen in H. habilis or H. rudolfensis and, thus, is
most parsimoniously an early example of H. erectus as
more strictly defined (Spoor, 2013). Finally, even the recent
affirmation that the Dmanisi sample does represent one
variable population has already been challenged on the
basis of its great range in mandibular morphology
(Bermudez de Castro et al., 2014).
We look forward to further increases in the size of fossil
samples for vanished hominin populations in order to assay
their variation more realistically and to improved technology
to scrutinize their morphology in ever-greater detail. The
most significant advances in diagnosing our species, however,
are likely to come from the burgeoning studies of both extant
and extinct genomes. With further research on the function-
ality of DNA differences and of epigenetic controls on the
expression of that DNA (Gokhman et al., 2014), we will
eventually be in a much stronger position to combine our
studies of the genome and phenome in both ancient and living
humans and ultimately determine much more firmly the
boundaries of H. sapiens as a morphologically and genetically
distinct species.
Acknowledgements
CS would like to thank Sarah Elton and Kevin Kuykendall for invitinghim to participate in the SSHB conference in Durham. Both authorswould like to thank Ros Fleming, Jon Buck and two anonymousreviewers for their helpful comments and the Human Origins ResearchFund of the Natural History Museum, London and The CallevaFoundation for funding.
DOI: 10.3109/03014460.2014.922616 Diagnosing Homo sapiens in the fossil record 319
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Declaration of interest
The authors report no conflicts of interest. The authors alone areresponsible for the content and writing of this article.
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