Berlin
A HYDROGEN-powered aeroplane could take to the air by the end of the century.
The plane, which is being developed by engineers at Daimler-Benz Aerospace
Airbus (DASA), will eliminate carbon dioxide emissions and produce less
pollution from nitrogen oxides than conventional aircraft.
Aircraft manufacturers have experimented with hydrogen, which is lighter than
conventional fuel, in the past. In 1956, the US military successfully flew a
Canberra bomber on hydrogen, although the plane needed conventional fuel to take
off. And in the 1980s, Russian researchers converted a Tupolev 155 to run on
natural gas or hydrogen.
The German project, however, is the first to redesign the combustion chamber
of the engine in order to reduce emissions of nitrogen oxides. Engineers at the
University of Aachen created a “micro-mixing” system to replace the standard
fuel nozzles. Hydrogen enters the combustion chamber through tiny pores,
creating thousands of “flamelets”, says Friedemann Suttrop, a professor of
aeronautics at Aachen. Suttrop says the system achieves a more complete mixing
of air and fuel, resulting in lower combustion temperatures and lower emissions
of nitrogen oxides.
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Suttrop and his colleagues have installed the new combustion chambers in a
small turbine engine, the auxiliary power unit from an Airbus 320. In tests
carried out over the past few months, emissions of nitrogen oxides were cut by
up to 70 per cent compared with conventional fuel.
The next step, says Suttrop, will be to convert the engines of a Dornier 328
aircraft. This is planned as a joint project with Tupolev, Pratt & Whitney
and Dornier, and is supposed to fly by the year 2000. DASA has already carried
out wind tunnel tests with a model, but the project is awaiting funding from the
German government.
Ian Poll, head of Britain’s College of Aeronautics at Cranfield University
near Milton Keynes, says the German project still does not solve the two biggest
problems of hydrogen use. “The volume of hydrogen is ridiculously large, and it
presents horrendous safety problems,” he says.
Liquid hydrogen fuel requires four times as much storage space as
conventional fuel. If the Dornier 328 is converted to hydrogen, additional fuel
tanks will have to be hung from its wings. These must be insulated with vacuum
chambers to keep the fuel cool. But DASA engineers say that hydrogen weighs less
than conventional fuel, allowing converted aircraft to carry up to 25 per cent
more payload.
![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)


