Greenhouse gases widely blamed for causing global warming have climbed to record highs in the atmosphere, an Arctic researcher has revealed.
“Levels are at a new high,” said Kim Holmen, research director of the Norwegian Polar Institute, which oversees the Zeppelin measuring station on the Arctic archipelago of Svalbard, about 1200 kilometres (750 miles) from the North Pole.
He said that concentrations of carbon dioxide, the main greenhouse gas, emitted largely by burning fossil fuels in power plants, factories and cars, had risen to 390 parts per million from 388 ppm a year ago.
Levels have hit peaks almost every year in recent decades and are far above 270 ppm level seen before the Industrial Revolution of the 18th century.
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Holmen said the increase of 2 ppm from 2006 reflected an accelerating rise in recent years. “When I was young, scientists were talking about 1 ppm rises” every year, he said. “Since 2000, it has been a very rapid rate.”
Coal fired
Holmen suggests that the growth of Asian economies, led by China, may be responsible for this steeper rise. By some estimates, China is opening coal-fired power plants at the rate of almost one per week.
Carbon dioxide concentrations peak just before spring in the northern hemisphere, when plants start soaking up the gas as they grow. Southern hemisphere seasons have less effect as there are fewer land masses and plants south of the equator.
The Zeppelin station is run in cooperation with Stockholm University and is one of the main measuring points, along with a station in Hawaii. ¾«¶«´«Ã½s say the concentration of CO2 in the atmosphere is at its highest in at least 650,000 years.
90% chance
In a report published on 2 February, the world’s top climate scientists said they were more than 90% certain that human activities, led by burning fossil fuels, were to blame for global warming. That was up from 66% certainty in a previous report published in 2001.
The UN’s Intergovernmental Panel on Climate Change said that temperature rises were set to accelerate and could increase by between 1.1°C and 6.4°C 2100, bringing floods to some regions, droughts to others, and rising sea levels.
Apart from emissions caused by burning fossil fuels, scientists say other factors could affect CO2 levels in future. On one hand, plants may grow more in a warmer world, soaking up more CO2. But if the soil gets warmer, dead plants and leaves may rot more in winter, releasing more carbon.
Any heating of the oceans may mean less absorption of CO2, partly because the greater buoyancy of warmer water prevents it from mixing with deeper levels.
![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)


