The multitude of lenses that make up an insect’s eye is providing inspiration for a new generation of super-slim camera phone.
Conventional camera lenses cannot be shrunk below a few millimetres in thickness before reducing the field of view. But a compound lens, made from hundreds of tiny “micro lenses”, can be made around one-tenth of the width, while retaining the same field of view and quality of image.
A prototype compound eye, consisting of scores of polymer micro-lenses has now been developed by researchers at the Fraunhofer Institute for Applied Optics and Precision Engineering in Germany, Swiss company SUSS MicroOptics and the University of Neuchâtel in Switzerland.
The 2-millimetre-thick prototype has 21 light-channelling components, each of which contains three separate lenses. Each individual lens points in a slightly different direction and projects part of the image on to a photo sensor. “Each channel is, in effect, a pinhole camera,” says Andreas Bräuer at the Fraunhofer Institute.
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Different directions
Bräuer told New ¾«¶«´«Ã½ that in theory it should be possible to make compound lenses just a few hundred micrometres in thickness. This could make it possible to install a camera into a smart card that could then perform simple image recognition tasks, he says.
The image quality of such a small compound lens would be limited to about 250 by 250 pixels, or 0.06 of a megapixel. The lenses should be relatively cheap and simple to manufacture, as micro lenses can be made using existing lithographic techniques, Bräuer adds.
Jim Girkin, at the University of Strathclyde in Glasgow, UK, says micro lenses would be best suited to applications that require only low quality, because they are naturally prone to distortion. “If they can be made reliably and cheaply, then for certain applications they could prove very interesting,” he says.
Nick Jones, a mobile phone expert at analyst firm Gartner, UK, says size of a cell phone camera depends primarily on the mechanism used to focus and zoom. But he says a smaller lens could perhaps be integrated with an optical sensor to make a cheaper overall camera system.
Journal Reference: Optics Express (Vol 13, p 889)
![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)


