Update 15 June: The decision to restrict the trade of red and pink corals has been reversed. The decision was initially passed on 13 June, but Algeria and Morocco pushed for discussions to be reopened during the last plenary session on 15 June. As a result of the plenary vote, trade in red and pink corals will not be restricted.
Original article:
Southern African countries have been permitted to sell off their stocks of ivory in return for a nine-year moratorium on further sales.
The deal was hailed as a boon for the continent’s beleaguered elephants, despite reports that such legal trade agreements make little difference to elephant survival.
The deal was hammered out by African environment ministers in a late-night bargaining session at a meeting of 169 member countries of the Convention on International Trade in Endangered Species (CITES) at The Hague, Netherlands.
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The meeting also agreed to protect other species, including restricting trade in red and pink corals, which are prized as jewellery.
CITES members voted to delay regulating export of corals for 18 months, partly because of worries by southern European producers that they would need time to adapt to new trade rules. Individuals will be able to carry a personal allowance of up to seven pieces of finished jewellery.
African divide
International trade in elephant ivory was banned in 1990, due to plummeting elephant stocks. But in 1997, CITES allowed South Africa, Botswana and Namibia – where elephant numbers were growing – to sell stocks of ivory taken from poachers or dead elephants. That sale took place in 1999.
Last week, the three countries asked for another sale and, with Zimbabwe, also asked for the resumption of regular, controlled exports.
In an unusual African split, they were opposed by other African countries, including Kenya and Mali, that consider elephants a valuable tourist attraction. They called for a 20-year ban on ivory sales, arguing, with conservationists, that trade encourages poaching and makes it harder to protect elephants.
A compromise was reached early on 14 June. The southern states will sell their stocks – thought to amount to 60 tonnes of ivory – to Japan. Then all sales must stop for nine years while a continent-wide elephant conservation plan is agreed.
“This is a clear win for elephants,” said Peter Pueschel of the International Fund for Animal Welfare, although the organisation fears the legal sale will encourage poaching.
However, the CITES ruling may have limited impact on the illegal ivory trade. A report by the Elephant Trade Information System (ETIS) found that the corruption index of the country concerned was the only factor linked to elephant killings.
![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)


