A novel way of cleaning the standard kilogram is to be tested next month. Metrologists at the (BIPM) in Sèvres, France, will try using ozone and ultraviolet light to remove grime from one of the weights and compare this with the traditional method using alchohol and steam jets.
Some 100 national standard kilograms are dotted around the world and are verified against the international prototype every 50 years or so. But, no matter how well these platinum-iridium alloy cylinders are stored, they typically gather about five micrograms of dirt each year.
Cleaning the weights is problematic. Currently they are rubbed with chamois leather impregnated with alcohol, then washed with a steam jet, a method known as nettoyage-lavage. The process is so tricky that just one person does it: Richard Davis, head of mass at BIPM, who learned the technique from his predecessor. After cleaning it can take up to a year for a kilogram to become stable again.
Ozone chamber
Now Stuart Davidson of the (NPL), UK, has adapted a process for cleaning semiconductor wafers as a non-contact method for scrubbing the kilogram.
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A platinum-iridium weight is placed in a chamber containing an ozone-enriched atmosphere and then illuminated with UV light. This breaks the ozone down into atomic oxygen and O2. Dirt on the surface of the weight – mostly long-chain hydrocarbon molecules – reacts with the oxygen to produce carbon dioxide and water molecules that are readily taken up by the atmosphere, leaving the weight clean.
“The main benefit is that the method is repeatable and not user-dependent like the nettoyage-lavage process,” says Davidson. “Potentially any of the national standard laboratories can return their kilograms to the same clean state using this technique.”
Experiments at BIPM will begin in March 2008 when NPL and BIPM scientists will compare the two cleaning techniques for the first time.
![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)


