For some, the highlight of a trip to Belgium is a visit to an ancient brewery or a demonstration of diamond cutting. When Australian Boyd Rayward travelled to Brussels in 1968 there was only one sight he wanted to see: a disused university anatomy theatre. Unusual? Perhaps, but Rayward was a graduate student in library science, and the cobwebby old theatre with leaking skylights housed something he had to see before it vanished forever. Inside the gloomy theatre, Rayward found piles of papers and archives that had remained untouched since 1944. These were the last remnants of the Mundaneum, a vast and visionary attempt at an immense proto-internet made from the most unlikely of materials: 3-by-5-inch index cards.
UNLIKELY as it sounds now, the hottest thing in information technology was once the index card. In the US, for instance, the War Department struggled with mountains of medical files until the newfangled method of card filing was adopted in 1887. Soon hundreds of clerks were transcribing personnel records dating back to the War of Independence. Housed in Ford’s Theatre in Washington DC – the scene of Abraham Lincoln’s assassination a generation earlier – the initiative succeeded a little too well. Six years into the project, the combined weight of 30 million index cards led to information overload: three floors of the theatre collapsed, crushing 22 clerks to death.
Belgian lawyer Paul Otlet was not deterred. His mission in life was to build an even bigger house of cards. Otlet had spent his youth in 1880s Brussels drifting through law school, hardly the background you might expect for a pioneer of IT. But a…
![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)


