IT COULD be the world’s smallest fence: a chain of five crude, squarish links is strung between posts just 40 micrometres apart. This microscopic barrier marks the threshold of a new world of fabrication.
The interlocking links of the chain would be impossible to make using conventional microfabrication techniques. Instead, they were conjured into existence by waving a magic wand – or rather, a laser beam. This method, called two-photon 3D microfabrication, is just starting to make its mark. Fast, cheap and flexible, it can create multilayered microchips, custom-designed crystals, pre-assembled propellers – tiny objects with fantastical curves, interlocking parts and 3D structures, all qualities difficult or impossible to achieve with traditional techniques. “It’s like making Frank Gehry-type buildings instead of flat warehouses,” says Malvin Teich, an engineer at Boston University.
The “flat warehouses” he means are the silicon computer chips made by photolithography, today’s standard in microfabrication. Photolithography etches the circuit onto the silicon by shining ultraviolet light through a flat mask perforated with the pattern of the chip circuitry. The technique can produce multilayer constructions, by depositing successive layers of silicon and using different masks to etch each layer, slowly building up a 3D structure. But you could never build a curvy Bilbao Guggenheim in this way.
Two-photon microfabrication is a different story. “You could do this on top of a desk, if you had the right lasers,” says John Fourkas, Teich’s collaborator at the University of Maryland in College Park. In fact, Fourkas is pretty much describing his lab, which is essentially just a big table with a laser hooked up to a computer and a few lenses. The laser scans through a drop of…
![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)


