The amount of fat we eat is the most important factor controlling hunger
and appetite. This finding is linked to the observation that as countries
grow richer, the national consumption of fat eventually levels out at around
40 per cent of the nation’s total energy intake.
‘There seems to be an inherent tendency for free-choice diets to stabilise
at around 40 per cent energy from fat, so long as economic development allows,’
says Martin Wiseman, head of the Nutrition Unit in Britain’s Department
of ÎçÒ¹¸£Àû1000¼¯ºÏ. Speaking at a conference in Reading, Berkshire, on fat and the
diet, Wiseman presented data from seven countries that supported the view
that as nations become richer, fat consumption edges up towards the 40 per
cent mark.
Japan, for example, where fat intake has traditionally been very low,
is now speeding towards the plateau. A survey of 20 000 Japanese published
this month by the country’s ÎçÒ¹¸£Àû1000¼¯ºÏ and Welfare Ministry, showed that fat
forms 25.7 per cent of the diet. In 1955 this figure was only 8.7 per cent.
Wiseman speculates that the so-called ‘fat factor’ governing appetite
may have given humans some kind of evolutionary advantage in the past. People
with the most stored fat would be more likely to survive food shortages
than their leaner cousins. But, says Wiseman, such an adaptation may be
less healthy in today’s times of abundant food.
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The new evidence supporting the ‘fat factor’ theory comes from John
Blundell, a reader in biological psychology at the University of Leeds.
He carried out a study in which he monitored the diet of two dozen active
young men. As part of their diet, the men ate special breakfasts which included
scones that were high, medium or low in fat.
Blundell concealed the amounts of fat in the three kinds of breakfast
by substituting to differing degrees real fat with Olestra, a sucrose polyester
that mimics fat but is not digested and contains no calories.
He found that subjects on the low-fat diets developed hunger pangs sooner
than those eating fat-rich diets, and they eventually began to make up their
calories by eating more carbohydrate, particularly in their evening meals.
He concludes that the calories in fat do help to satiate and suppress
appetite, but that the effect is not immediate, ‘suggesting a post-absorptive
action’. In other words, eating fat does not immediately satisfy hunger,
but it will restrain your calorie intake in later meals.
Wiseman said that whether the fat factor theory proves correct or not,
Britons still eat far too much fat. Only one-third of Britons have been
able to limit their energy intake from fat to 35 per cent, as recommended
by the Department of ÎçÒ¹¸£Àû1000¼¯ºÏ’s Committee on Medical Aspects of Food Policy
(see ‘Britain’s deadly diet’, New Scientist, 11 May).



![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)