A 10-tonne rocket broke into three high above its launch pad in Lapland
last week. Maxus 1, a rocket built jointly by Sweden and Germany, was designed
to compete with the space shuttle as a vehicle for experiments in microgravity.
Fifteen of the rockets are planned.
The cause of the disintegration is not yet known. ‘For the first 37
seconds everything was in order,’ said Jan Englund, of S-Range, the Swedish
space centre. ‘Then the rocket encountered a disturbance. But the guidance
system on the rocket was able to correct the problem.’ A few seconds later,
another ‘disturbance’ sent the rocket spinning out of control. It broke
into pieces 30 kilometres above its launch site.
‘We know it was a problem with the motor,’ said Englund. ‘We don’t know
exactly what caused the motor failure.’
The rocket, fuelled by a solid propellant, was made by Thiokol, the
American-based company that builds boosters for NASA’s space shuttle. The
rocket was designed to ascend to 1000 kilometres and spend 14 minutes in
microgravity, just long enough to complete the experiments on board. When
the rocket broke up, the payload compartment was saved by a parachute and
the experiments were recovered 60 kilometres from the launch pad.
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Most of the experiments belonged to the European Space Agency, which
has lined up numerous experiments for the Maxus rockets. ‘We don’t think
we will lose ESA as a contractor,’ said Englund. ‘This was a problem that
can be fixed.’ Englund anticipates another liftoff within a year. ‘There
is a very big demand for microgravity payloads. The lead time for a microgravity
experiment on this rocket is only about a year, but on the shuttle it is
almost 10 years.’
![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)


