HIGH acidity may be the trigger that clears a path for immune cells to reach damaged tissue, according to researchers in Israel. The enzyme heparanase, which allows these cells to invade tissues, seems to be activated only in acidic environments such as those found in areas of inflammation.
T lymphocytes, immune cells which circulate in the blood, must migrate across the walls of blood vessels in order to reach inflamed tissue. Much is known about how these cells pass through vascular walls, but the controls that operate once they get to the other side are less well understood.
When T cells encounter specific antigens, molecules which provoke an immune response, they start to produce large amounts of heparanase. This enzyme breaks down heparan sulphate, a major component of the dense complex substance known as the “extracellular matrix” that binds and stabilises tissues and blood vessels. This allows the T cells to penetrate the matrix and reach sites of inflammation.
Now it appears that the action of the enzyme is “switched” on and off depending on the pH of tissues. Dalia Gilat at the Weizmann Institute of Science in Rehovot, working with colleagues there and at Hadassah-Hebrew University Hospital in Jerusalem, found that heparanase functions as an enzyme only at low pH levels (Journal of Experimental Medicine, vol 181, p 1929). Acidic conditions are found in inflamed tissue and in growing tumours that are beginning to spread to other sites in the body. The pH in these tissues is around 6.8 because oxygen levels are low, causing carbon dioxide and lactic acid to accumulate.
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At the higher pH of normal tissues (around 7.2), however, heparanase was found to function in an entirely different way. It binds to heparan sulphate without degrading it, and also binds to proteins on the surfaces of T cells. This anchors T cells in the extracellular matrix, stopping them invading normal tissue.
![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)


