RUSSIAN cosmonauts who ventured into the damaged module of the Mir space
station last week put their trust in a series of simulations that promised they
would not encounter shards of glass or toxic chemicals. According to John Uri,
NASA’s mission scientist for Mir, tests on a refrigerator and a laptop computer
similar to equipment left in the Spektr module showed no ill effects from
depressurisation. In the tests, the equipment “pretty much just sat there”, says
Uri.
The simulations proved accurate. When Pavel Vinogradov opened the hatch to
Spektr, all he saw were some white flakes floating in the vacuum. He speculated
that they were residues from Michael Foale’s shampoo bottle, which could have
exploded.
Vinogradov and his partner Anatoly Soloveyov quickly succeeded in their main
task, reconnecting some cables that will deliver critical power from solar
panels mounted on the Spektr module. Russian officials hope the repairs will
provide an additional 8 kilowatts, boosting Mir’s power-generating capacity by
50 per cent.
The cosmonauts reported two strange phenomena inside Spektr that mystified
flight controllers. Vinogradov insisted that there was condensation on some of
the equipment, although Russian experts say that in a complete vacuum, water
vapour should have long since disappeared.
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The cosmonauts also reported hearing fans and other equipment coming back to
life inside Spektr as they connected the electrical cables. This seemed
impossible because sound cannot travel in a vacuum, and the cables the
cosmonauts were connecting are not linked directly to any equipment in the
module.
NASA officials offered an explanation a few hours later. When Mir emerged
from the shadow of Earth into direct sunlight, some current flowed from the
solar panels directly to batteries and equipment in the Spektr module, causing
some fans to spin.
Researchers on the ground cheered news that the cosmonauts had retrieved a
laptop computer and a stack of computer discs. These may contain data from
several experiments that were interrupted on 25 June, when a supply ship crashed
into Spektr, forcing the crew to abandon the module. Most of the experiments
were devoted to studying the effects of long-term spaceflight on the human body.
Although some data might now be recovered, blood and urine stored in a
refrigerator were ruined.
A team of German and Italian researchers were not so happy. They are
investigating how well muscles can perform sudden, strenuous tasks, such as
jumping, after long periods of weightlessness. But when they arrived in Moscow
they learnt that Vasili Tsibliev, who was at Mir’s controls when the supply ship
rammed Spektr, would no longer take part in their tests. He has been said to
suffer from an irregular heartbeat, but he is also bitter at accusations that he
is partly to blame for Mir’s problems.
Tsibliev and his flight engineer, Alexander Lazutkin, were supposed to fill
out a weekly questionnaire while in orbit, reporting on how they felt about life
on board. The stress and strain of recent months may make for some interesting
results, says Nick Kanas, the psychologist who designed the study for NASA. “I
just hope they filled out their questionnaires and that they did it honestly.”
![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)


