MERCURY, which is known to damage the nervous system and disrupt mental
development, can also cause infertility in men at levels well below those the
WHO says are safe.
Mike Dickman, a biologist at the University of Hong Kong, and Clement Leung
of the In Vitro Fertilisation Centre in Hong Kong measured mercury levels in men
with fertility problems. They found that the hair of men with slow, deformed or
sparse sperm contained on average 40 per cent more mercury than that of men with
normal sperm. At any given age, men with 3.7 parts per million or more of
mercury in their hair were twice as likely to be subfertile as men with 2 ppm or
less. The WHO’s safety limit is 10 ppm.
Acute mercury poisoning is known to harm sperm formation in mice and monkeys.
But this is the first clear association between reduced fertility in men and
environmental exposure to mercury. The results will be published in The
Science of the Total Environment in June.
The men got their mercury from seafood, says Dickman. Volcanoes and
coal-fired power stations release the metal into the environment. It is
converted to methyl mercury by marine bacteria and taken up by fish. “Men in
Hong Kong who eat four or more seafood meals per week have significantly more
mercury than those who eat less,” he says.
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The authors say the WHO’s recommended safe level for mercury in food of 0.5
ppm is too high for places such as Hong Kong where people eat lots of seafood.
Last year, the US Environmental Protection Agency estimated that at least 170
000 people in the US receive higher doses than the WHO recommends.
![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)


