With less than a year to go before the United Nations Conference on
Environment and Development takes place in Brazil – the so-called Earth
Summit – battle lines are being drawn up in earnest. Major skirmishes have
already occurred over moves to persuade all participants to agree on firm
targets for reducing emissions of carbon dioxide. But before too much blood
is spilt over the issue, we should ask whether the pursuit of consensus
over targets is, in fact, the best tactic for reaching a goal that all now
share: to reduce man-made global warming.
Certainly there are important lessons to be learnt from current experience
in Europe. In a fit of political zeal, the member states of the European
Community have committed themselves jointly to two goals: stabilising carbon
dioxide emissions by the end of the decade, and achieving a ‘substantial’
reduction thereafter.
So far, however, words speak louder than actions. As we report in this
issue, achieving such goals is technically feasible (See ‘Europe’s hot air
over carbon cuts’). But there will be political costs, since doing so will
require governments to take steps in conflict with other priorities: for
example, restricting rather than encouraging the growth of road transport.
To date, few governments have been willing to pay the necessary price.
Europe’s experience highlights the dilemma facing scientists, diplomats
and politicians around the world as they prepare for the Brazil meeting.
Even if consensus on targets is achieved – and, with the US still refusing
to make any type of commitment, that is still uncertain – will they be worth
any more than the paper they are written on?
Advertisement
The omens are not good. Take, for example, efforts to protect the ozone
layer. Last year in London, rich countries promised to spend $240 million
to buy poor countries ozone-safe technology. India alone estimates that
it will need $1.2 billion to comply with the ozone treaty. So far, however,
even the agreed pittance has been too much for rich countries to cough up:
the fund contains a paltry $9 million.
Those with longer memories will remember the ill-fated United Nations
Conference on Science and Technology for Development, held in Vienna in
1979. Here ‘consensus’ took the form of a commitment to a $250 million
fund to help the Third World. But less than a third of this sum materialised.
Surely we can do better. As long as they are wedded to public consensus,
those meeting in Brazil next year may well end up with words so banal that
everyone – even John Sununu, the White House chief of staff who doesn’t
believe climate change is a problem – can agree to them.
Perhaps the West should stop thinking of itself as a family that must
always agree. Perhaps those willing to set targets to cut greenhouse gases
should go forward with an international agreement and concentrate on achieving
their goals, without worrying whether everyone tags along.
Then it would be question, firstly, of devising strategies to persuade
recalcitrant nations to join the bandwagon, perhaps modelled on the safeguards
in the ozone treaty specifying no trade with non-joiners. And secondly,
of building a solid behind-the-scenes agreement that, whatever rhetoric
individual governments wish to use, there can no longer be ‘business as
usual’ on energy and resource policy.
There are, of course, dangers in this approach. Many will argue that
allowing major carbon dioxide producers – in particular the US, but also
some Third World countries too – to avoid a firm commitment to reduction
targets will let them off the hook. But this need not necessarily be the
case. And after all, the most important thing for any climate treaty agreed
in Brazil will not be whether it impresses voters back home, but whether
it works.



![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)