The Protean Self by R. J. Lifton, Basic Books, pp 262, $25
Robert Jay Lifton has written some fine books that have examined trauma
and the evil people can inflict on each other. The Protean Self is learned,
personal, packed with references to poetry, painting and politics, but somehow
rather disappointing.
Lifton argues that our sense of self is changing in response to social
and technological changes, and named his book after the Greek sea god Proteus,
who was able to alter his shape at will. We, too, are in flux and in fragments,
aware in the post-Freudian world of the many bits of ourselves that go to
make up the whole, or not so whole.
One difficulty with the book is that Lifton sometimes seems to suggest
that a key difference between our advanced civilisation and that of Rene
Descartes, David Hume and others is that they wrestled with the problems
of philosophy in a fax-free, modem-free world. There were many problems
of which they were unaware – the trilocation of time, for example. Descartes
knew what time it was. He was not obsessed by the fact that when he was
having lunch in Paris, it was dinner time in Tokyo – a major mind, and appetite,
warp for your intercontinental pundit, who also remembers that the last
time he had dinner in Tokyo he was remembering a power breakfast he once
had in Los Angeles.
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I am being frivolous, but that is what Lifton’s slightly smug tone elicits.
He argues that Sigmund Freud broke us down into ego, id and superego, but
did little to encourage change or integration. Freud was resigned, reckoning,
more or less, that all was for the worst in the worst of all possible worlds.
Hardly a bizarre conclusion, given the state of Germany in the 1930s.
Lifton does offer some interesting chapters. There are potted case histories
of high achievers, and an account of discussions with Chinese men and women
who lived through Mao Tse-tung’s various revolutions and explained to Lifton
how they had to change to survive. But he seems too optimistic about his
main thesis.
Travel and communications have been revolutionised. We are the first
people who can go from London to New York and back in 24 hours. But does
that alter our psychology that much? Especially when airports look the
same all over the world? Does the speed of travel make it easier for us
to adapt to profound social changes? In many ways, the developed world is
becoming much the same, from Athens to Santiago. The self may travel more
miles these days but perhaps it crosses fewer canyons.
The area the book explores is fascinating, but Lifton is too ready to
pat us on the back for being so fluid, so self-aware, so good at coping
with our many selves and so damned modern in our global village. Many chapters
talk of achievers and those with ‘high goals’. The self for many people
may be more stubborn, rooted and primitively clinging. We can see more of
the world than ever, but there is plenty of evidence (anecdotal, as is Lifton’s)
that suggests it is awareness of other cultures that makes people resist
change.
David Cohen founded Psychology News and is a film maker.
![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)


