Berlin
UP TO a quarter of young Germans have damaged their hearing by listening
to loud music, according to a study of military recruits. And one in ten of the
country’s 18-year-olds may have suffered damage severe enough to handicap them
in normal conversation, a separate study has found. The results have prompted
German officials to propose Europe-wide limits on the volume of personal
stereos.
Researchers at the Institute for Occupational Medicine at the Heinrich Heine
University in Düsseldorf examined 1800 men between the ages of 16 and 24 at
several military recruiting offices around the country. They found some hearing
loss in around a quarter of them. They also discovered that the recruits with
poor hearing were more likely to have spent time listening to loud music.
In a second study, supported by the government’s Federal Environment Office
(FEO), researchers examined the listening habits and hearing of 270 students in
Berlin. According to Hartmut Ising, a specialist on noise pollution at the FEO,
nearly 10 per cent of students aged between 16 and 18 had lost so much of their
hearing that they had difficulty understanding some normal conversation.
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The researchers also found that students who listened to music on headphones
for more than two hours a day and visited discos at least once a week suffered,
on average, a 10-decibel reduction in their hearing sensitivity. Most of this
loss was in the frequency range between 3 kilohertz and 6 kilohertz, which might
prevent a person distinguishing between the sounds of the letters “s” and “f”.
Adrian Davis, who works at the Medical Research Council’s Institute of
Hearing Research in Nottingham, says he is “a little sceptical” about the German
results. His own studies have failed to find a similar pattern of hearing damage
among British youngsters who listen to loud music. Similar studies in Sweden
have also failed to establish such a pattern.
The German government, however, is now calling for the European Union to
limit the noise levels of personal stereos. It has proposed a maximum output of
90 decibels, a significant reduction from the 120 decibels produced by some
personal stereos. The proposal is under consideration by CENELEC, a body within
the European Commission that sets standards for electronic equipment. Other
countries have been asked to submit their views on the German proposal by 15
July.
The German move follows unilateral action by France, which last year passed a
law capping the output of personal stereos at 100 decibels
(“Falling on deaf ears”,
New ¾«¶«´«Ã½, 29 June 1996, p 12).
Manufacturers claim that there is no widely accepted method for measuring the
sound emitted by personal stereos. Sound levels measured by a microphone on the
earphones of a music system are not equivalent to what is actually heard by the
ear, they say.
![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)


