Murder detectives finally have a reliable way to determine how long a victim has been dead from their bones, as well as glean valuable information about where the person lived.
Stuart Black, an environmental geochemist at the University of Reading, is pioneering a technique similar to carbon dating, but that uses isotopes of other elements. He has just finished his first case.
From the charred remains of a man who was repeatedly stabbed and then set on fire, he determined that the victim was probably from the former Soviet Union and had been dead about a week.
“While that doesn’t give us a name and address, it helps immensely,” says Detective Superintendent David Hankins of the Cambridgeshire police. “Dr Black has given us an incredible amount of information.” Police are so impressed, Black’s lab is already working on two other murder cases, and three more are awaiting analysis.
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Decay rate
To date remains, forensic scientists normally rely on studies of how bodies decay in different climates (New ¾«¶«´«Ã½ print edition, 6 January 2001). But the temperature and moisture conditions where the corpse was left are often unknown, making these methods imprecise.
“The error is unquantifiable. It relies on pathologists saying ‘oh, I’ve seen a bone like that before, and it was about this old’,” says Black.
Instead, Black looks at the decay of radioactive isotopes. Carbon dating has long been used by archaeologists looking at bones that are centuries old, but is little use for younger bones. To date more recent remains, Black is using isotopes with shorter half-lives than carbon-14. He has found that the most useful are lead-210 and polonium-210, with half-lives of 22 years and 134 days respectively.
These and other elements entering our bones are primarily from food, so Black can also use his measurements to sketch the victim’s diet. A depletion of certain elements will reveal if the person was a vegetarian, for example.
Regional diet
Black has also refined a way of using various stable isotopes of lead to indicate where the victim lived in the last decade of their life. This lead is breathed in with air, and the amount depends on factors such as local geology and the kind of petrol used by cars in the area.
Knowing where the victim lived is useful for police, but also means Black can take regional differences in diet into account, to pin down the age of the bones even more accurately. In Britain, he consults the Food Standards Agency’s database to check how much radioactive lead and polonium is in different foods.
Black originally tested the technique on a sample of bones from 25 elderly women from a small Portuguese town. He found he could pin down the date of death to within two years for women who had been dead 50 years. That precision probably reflects the fact that they had very similar diets, says Black. To work out how accurate the technique is in other cases, he says we need to find out how variable these radioactive elements are within other populations.
But even with a big margin of error, the method could still sort out the surprisingly common confusion about whether bones are years or centuries old, according to forensic scientist Kenneth Pye, who heads a consultancy in London. “You get heaps of remains found in London building sites. These are treated as crime scenes, but they often turn out to be medieval.”
![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)


