THERE are six in the line-up. But not one of them is human. Instead, on a laboratory bench stand six dental casts and a large photograph of an ugly-looking bite. Examining them is a forensic odontologist who must decide which, if any, of the sets of teeth made that mark.
Such dental identity parades are more common than you might think. American serial killer Ted Bundy was convicted largely because of a bite he left on one of his victims. In Britain last January, a perfect match between bite marks and a set of disfigured teeth belonging to Edwin Hopkins, a 20-year-old apprentice paint sprayer, helped to convict him of the brutal murder of schoolgirl Naomi Smith.
Nor do the experts only have to deal with bite marks left on a victim’s skin. “People leave bites in food and inanimate objects such as pencils and bottle tops,” says Bernard Sims, an odontologist attached to the department of morbid anatomy at the Royal London Hospital, and one of two consultants to Britain’s Home Office. Sims once identified the driver of a getaway car from the tooth marks left in the plastic end of a car key-and a murderer in Essex from a half-eaten pear left at the scene of his crime.
In the US, Gerald Vale, chief forensic dental consultant for Los Angeles County, was called in to give evidence in the case of the “AIDS bandit”, a robber who threatened his victims with a syringe of blood, allegedly infected with HIV. “At one crime scene he left behind a Styrofoam cup with amazingly detailed bite marks that could be matched…
![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)


