The Last Ape: Chimpanzee Behaviour and Ecology by Takayoshi Kano, Stanford
University Press, pp 248, Dollar 45
In the primate world, the words ‘pygmy chimp’ have almost become synonymous
with promiscuity. Pygmy chimps occur only in Zaire and are smaller and slimmer
than common chimps. Like ourselves, they are far more sexually oriented
than chimpanzees. Females are nearly continuously receptive and will participate
in sexual activity as frequently with males as with each other. The so-called
G-G (genito-genital) rubbing between females often results in orgasm.
Takayoshi Kano believes that the female genitalia specifically evolved
for this purpose rather than for male-female mating. The increased level
of copulation, especially when food is present, suggests that sex plays
a social role in preventing aggression.
In general, pygmy chimps are more peaceful than their cousins: the cannibalism,
infanticide, group wars and domineering behaviour seen in common chimps
have yet to be witnessed. Despite their social dexterity however, no tool
use in the wild has been reported. Kano suggests that this is because food
resources are never in short supply.
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Because of the paucity of information on pygmy chimps – there are fewer
than 50 000 left – Kano’s book provides much needed data from the wild.
Although the information is still relevant, it has taken six years to reach
us from Japan. Meanwhile, the current political climate in Zaire has worsened
the chimp’s situation.
Sanjida O’Connell researches chimpanzee behaviour, and works as a BBC
producer
![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)


