Maroua in northern Cameroon could soon be a mosquito-free zone. For
the past four weeks a 50-strong hit squad has been scouring the town in
search of cesspits and sewers where Culex quinque fasciatus lays its eggs.
Each potential pool of mosquito larvae has been sprayed with the team’s
secret weapon – a biological pesticide.
The WHO’s Tropical Disease Research programme backed this first large-scale
trial of the bacterium Bacillus sphaericus, whose spores contain a toxin
lethal to mosquito larvae.
The mobile anti-mosquito squad, led by French researchers, sprayed all
sources of stagnant water at the end of the dry season. They chose Maroua
because it is an ‘island’, separated from the nearest large town by more
than 200 kilometres of open country. Culex is essentially urban and cannot
survive in the savanna, so there is no pool of mosquitoes around the town.
‘By July, when people can be bitten over 300 times a night, we will
be able to assess the effectiveness of the pesticide,’ says the team’s leader,
Jean-Marc Hougard of ORSTOM, the French institute for scientific research
in development and cooperation. Already there are signs that the blitz may
be working. At one test site, where a typical sample yields around 90 mosquitoes,
the latest catch was a single elderly female.
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Hougard does not expect to eradicate the mosquito completely. But if
the pesticide proves efficient, it will provide a cheap method of control.
Although Culex is not much more than a nuisance in Maroua, on the other
side of the continent in East Africa it transmits the worms that cause filariasis,
a debilitating parasitic disease. ‘If it works, we can repeat the experiment
where there is filariasis, in Dar es Salaam or other East African cities,’
says Hougard.
Unfortunately, the bacterium cannot be used against the Anopheles mosquitoes
that carry malaria, because they lay their eggs in transient pools and puddles
rather than permanent wet spots such as sewers.
![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)


