Berlin
CERAMIC bearings can be used safely in industry now that German researchers
have developed a computer model to predict when they are close to cracking up.
The model has been developed by researchers at the Fraunhofer Institute for
Mechanics of Materials in Freiburg.
Bearings made from ceramic materials such as silicon nitride are much admired
because the material is harder and lighter than steel, so the bearings last
longer. Ceramic materials can also be immersed in corrosive liquids, unlike
steel, and they require less lubrication.
Although hybrid bearings made of ceramics and metal are becoming more common,
few companies have been willing to adopt bearings made completely from ceramics.
Industrial engineers “don’t trust them,” says Michael Rombach from the
Fraunhofer Institute. “They feel that the bearings cannot be safe.”
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Ceramic materials are more brittle than steel and can fail suddenly and
catastrophically. Engineers have limited experience with such materials and
cannot predict how they will behave.
But Rombach and his colleagues, working together with the company Cerobear,
based in Herzogenrath, near Aachen, have removed some of the guesswork. They
loaded bearings to their breaking point, and compared the laboratory results
with theoretical models. The result is a computer program that predicts the load
that can be carried by a ceramic bearing of any size or shape.
Rombach says all-ceramic bearings could have a bright future in the chemical
or food processing industries. Steel bearings used in industrial pumps, for
instance, need to be sealed off from food for reasons of hygiene, and from
corrosive liquids to protect the bearing. A ceramic bearing can be immersed in
such liquids with the liquids providing the lubrication.
William Coblenz, the Pentagon official responsible for research on ceramic
bearings, says that the US military is beginning to adopt hybrid bearings.
Coblenz says hybrid rollers eliminate the most common problem with metal
bearings—lubrication failure. When this occurs, the metal rollers become
welded to the surrounding metal surface. But at present, all-ceramic bearings
are not widely used. “The only place we’re looking at all-ceramic bearings is in
instruments like gyroscopes,” says Coblenz.
![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)


