Becoming Human by Ian Tattersall, Harcourt Brace, $27, ISBN
0151003408
IAN TATTERSALL has long made it his business to be a thorn in the side of the
body anthropological, prompting professionals and others to view the evolution
of humans as they would the evolution of any other animal. “Most people who
accept that mankind has an evolutionary history tend to think of our evolution
as a slow business of perfecting adaptation over the ages,” he says, “which, if
true, imparts in retrospect a certain inevitability to our having become human.”
This is dangerous for several reasons, not least because it encourages a gross
oversimplification of the story of human evolution.
It’s a story about which Tattersall has strong views. “There’s not a great
deal we can learn about ourselves by contemplating our evolutionary past that we
cannot learn by observing our often bizarre behaviour today,” reads the opening
to the final chapter of Becoming Human.
This might seem like an example of the above-mentioned bizarre behaviour,
because Tattersall heads the department of palaeoanthropology at the American
Museum of Natural History, New York. He is also a major intellectual presence in
the science of human evolution and has written a couple of highly acclaimed
popular books on human origins. Moreover, much of Becoming Human is
devoted to a wide-ranging—and highly readable—tour of the fossil
evidence of how, anatomically, we got to where we are today.
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Has Tattersall—as some of his adversaries have long
contended—flipped his lid? He acknowledges the tremendous “thirst to
explain our place in nature and to know where we come from”. Bumper sales of
magazines sporting concocted images of our ancestors on their covers attest to
that, Tattersall notes. The reason for the above, apparently contrary statement,
he explains, is that “the abilities of today’s Homo sapiens . . .
represent a huge leap away from those of our precursors”. In other words, modern
human behaviour is not a simple extrapolation of earlier trends, but something
entirely new. Evidence of this novel behaviour, such as the rate and degree of
technological innovation and the use of symbolism— implying modern levels
of language and consciousness—first appears in the archaeological record,
particularly of Europe, about 40 000 years ago.
These new behaviours are “more akin to an `emergent quality’,” says
Tattersall, “whereby for chance reasons, a new combination of features produces
totally unexpected results”. By their nature, emergent qualities cannot be
predicted on the basis of what preceded them.
Becoming Human, as we’ve come to expect of any work from Tattersall,
is wittily and cogently argued, and uncompromising. For instance, in his
discussion of the evolutionary origin of modern humans, there is no mention of
competing hypotheses. For Tattersall, the molecular and fossil evidence
overwhelmingly supports the notion that modern humans evolved in or near Africa
around 150 000 years ago. Period. It is this group that changed so radically 40
000 years ago.
He also neatly balances what some might consider conflicting positions, but
in reality are not. First, as mentioned, Tattersall describes modern human
behaviour as an “emergent quality” that, by its nature, can seem beyond
explanation and therefore special. Second, he berates some fellow
palaeoanthropologists for being less than scientific in their evolutionary
scenarios of human origins, and for invoking special processes to explain our
unquestionably special abilities. “We did not come by our special features as
the result of a special process,” he states emphatically. The (recent) origin of
fully modern language, perhaps as a result of one or a few small genetic
changes, is the key to the quantum shift in behaviour that is seen in the
archaeological record. “Almost all the unique cognitive attributes that so
strongly characterise modern humans . . . are tied up in some way with
language,” argues Tattersall. No mystery. Just something novel and powerful.
In a chapter titled “Evolution—for what?”, Tattersall traces the
genesis of the teleological view, including his discipline’s slow but eventually
enthusiastic acceptance of the “New Evolutionary Synthesis” in the 1940s and
1950s. The core of the synthesis—that all evolutionary change involves the
continuous, gradual accumulation of small changes —gave rise to the
linear, progressive perspective of evolution that dominated palaeoanthropology
for so long. For instance, the increase in the size of the brain over the past
five million years was assumed by many to have been a steady process, a gradual
increase in intelligence culminating in modern Homo sapiens.
Tattersall’s museum colleague Niles Eldredge helped to dispel this notion in
the 1970s and 1980s, when he and Stephen Jay Gould launched their then
controversial hypothesis of punctuated equilibrium. Much of evolution, including
human evolution, proceeds sporadically, with long periods of stasis and brief
bursts of change. Evolution by jerks, as one wit put it. The archaeological
record, which reveals widely spaced bursts of technological innovation (that is,
until the advent of modern humans), is a clear example in the behavioural
realm.
The 1990s have been a wildly busy time for palaeoanthropology, with the
discovery of several new species of hominid in the earliest part of the human
fossil record, the unearthing of two staggeringly rich fossil caches in
Atapuerca, northern Spain, one 300 000 and the other 800 000 years old, and of
eye-popping Ice Age art in recently found caves in southern France. Becoming
Human is therefore timely in its publication, and Tattersall has done a
fine job of including the new evidence, telling his version of how we came to be
what we are in a way that will delight anyone interested in this most compelling
of stories.
There is plenty of room for debate, of course. For instance, some
archaeologists argue that the advent of symbolic behaviour was not
revolutionary, but gradual, citing examples of putative symbolism as old as 300
000 years. But many of these examples are questionable. Tattersall also argues
that the number of hominid species currently recognised is far too low, in spite
of the richness of recent discoveries.
Becoming Human explores far more than has been covered here. A rich haul, it
includes the meaning of Ice Age art, what studies of chimpanzees tell us about
our common ancestor, the dynamics of stone tool technologies, and the place of
religion in our lives. Tattersall also challenges the popular notions spawned by
evolutionary psychology, which suggest that we are prisoners of our evolutionary
past. If, he argues, important human capacities are an emergent quality, not an
extrapolation of earlier behavioural trends, then this undermines “the notion
that our behaviours are programmed in any detail by our genetic heritage”.
![Astronomers have long known that understanding how star clusters come to be is key to unlocking other secrets of galactic evolution. Stars form in clusters, created when clouds of gas collapse under gravity. As more and more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet radiation and the supernova explosions of massive stars eventually disperse the cloud, and their light can bear down on other star-forming regions in the galaxy. This process is called stellar feedback, and it means that most of the gas in a galaxy never gets used for star formation. Researching how star clusters develop can answer questions about star formation at a galactic scale. Now, the state of the art has been further developed with both Hubble and Webb working together to provide a broad-spectrum view of thousands of young star clusters. An international team of astronomers has pored over images of four nearby galaxies from the FEAST observing programme (#1783), trying to solve this mystery. Their results show that it is the most massive star clusters that clear away their gaseous shroud the fastest, and begin lighting their galaxy the earliest. The team identified nearly 9000 star clusters in the four galaxies in different evolutionary stages: young clusters just starting to emerge from their natal clouds of gas, clusters that had partially dispersed the gas (both from Webb images), and fully unobstructed clusters visible in optical light (found in Hubble images). With Webb???s ability to peer inside the gas clouds, they were able to then estimate the mass and age of each cluster from its light spectrum. This image shows a section of one of the spiral arms of Messier 51 (M51), one of the four galaxies studied in this work, as seen by Webb???s Near-Infrared Camera (NIRCam). The thick clumps of star-forming gas are shown here in red and orange, representing infrared light emitted by ionised gas, dust grains, and complex molecules such as polycyclic aromatic hydrocarbons (PAHs). Within these gas complexes, each tens or hundreds of light years across, Webb reveals the dense, extremely bright clusters of massive stars that have just recently formed. The countless stars strewn across the arm of the galaxy, many of which would be invisible to our eyes behind layers of dust, are also laid bare in infrared light. [Image description: A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.]](https://images.newscientist.com/wp-content/uploads/2026/05/13114322/SEI_296271016.jpg)


