PART of the Mir space station may be abandoned forever after a failed attempt
by astronauts last weekend to find a hole left when a cargo vessel collided with
the station’s Spektr module in June.
Despite a six-hour space walk to search for the tear in Spektr’s outer skin
that left it crippled and airless, the astronauts could find nothing. Now some
space officials in the US and Europe are predicting privately that the module,
which housed scientific experiments, will remain unoccupied even if the hole is
eventually fixed. They are worried that the tear might reopen.
Russian and American specialists are experimenting with materials with which
to plug the hole, should it be found. They are looking for resins that will bond
to the metal of Spektr’s outer skin and create a strong seal. But Greg Harbaugh,
a NASA official responsible for the agency’s work on Mir, says: “How do you
satisfy yourself, once you’ve done the repair, that it’s OK to send human beings
back in there?”
The original hole was small and the air escaped slowly, giving astronauts
several minutes to seal off the damaged module. But according to German
astronaut Reinhold Ewald, who was on board Mir earlier this year, the rupture of
a resin patch might create a much larger hole in the station.
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NASA officials say that they can continue their scientific experiments
without the Spektr module. But they will carry on helping with the repair effort
because it is providing training for maintenance work on the future
International Space Station.
Russian specialists suspect that the hole in Spektr is beneath the base of a
solar panel damaged in the collision. When a space shuttle visits Mir in late
September it will deliver a metal plate that could be used to patch any leak.
![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)


