When a young researcher recently took a closer look at embryonic stem cells, he made an astonishing finding: according to his results, the vigorously growing cells he was looking at should have been dead or dying.
“I didn’t anticipate this,” says Thomas Zwaka, who works in the lab of James Thomson at the Wisconsin National Primate Research Center in Madison.
Zwaka had tested the embryonic stem cells (ESCs) for the presence of enzymes called caspases, proteins that chew up the cell from within. Their presence is usually considered a sure sign that cells are undergoing programmed suicide, or apoptosis – the body’s way of getting rid of damaged or redundant cells.
“That’s when I ran into the most confusing result,” he says. Although the cells had high levels of caspase activity, few of them were actually dying, he told a recent stem-cell meeting in Boston.
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To double-check his results, Zwaka looked for, and found, two other signs of cell suicide: the presence of a chewed-up protein called PARP-1, which is abundant in suicidal cells, and the shutting down of the power factories in cells, the mitochondria, indicated by the depolarisation of their membranes.
Zwaka speculates that the process of self-renewal may have evolved alongside cell death, and some of the processes may be the same.
The fact that signs thought to be characteristic of cell suicide appear in cells that are not dying might force a lot of researchers to re-examine their work, says stem-cell researcher Margaret Goodell from the Baylor College of Medicine in Houston, Texas. “I think it is potentially incredibly exciting.”
![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)


