Without liquid crystals there would be no life. Even the simplest single-celled
creature has an outer skin whose fabric is liquid crystalline. It is this
skin that forms the membrane separating the inner workings of the cell from
its surroundings. More complex life forms, such as human beings, use liquid
crystalline membranes for a vast variety of biological processes, for example,
transmitting nerve impulses and digesting fats.
You might be surprised to find out that cell membranes are liquid crystals.
In fact, the first recorded observations of the liquid crystalline phase
were of myelin, the material that coats nerve fibres. In 1855, a German
ophthalmologist called C. Mettenheimer was studying myelin under a polarising
microscope, and noted that, although it flowed like a liquid, it was brightly
coloured, or ‘birefringent’ like a crystal when viewed between crossed polarisers
(see ‘The fourth state of matter’, New Scientist, 4 May). It was not, however,
until much later that myelin was identified as a liquid crystalline material.
We now know that the liquid crystal structure of myelin consists of
regularly stacked layers of membranes, with each membrane consisting of
molecules that move around freely within it. In the direction of the stacked
membranes it behaves like a crystal, but in the plane of the membrane it
behaves like a liquid. Without exception, all biological membranes behave
simultaneously like a liquid and a solid, so liquid crystallinity must play
an important part in the function of cells. Over the past 20 years there
has been a surge of interest in biological liquid crystals. This has produced
new and exciting ideas about how liquid…





![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)

