THE urge to explore strange new worlds leads some scientists deep into the
oceans or the weightlessness of space. Reinhard Hüttl’s final frontier was
easier to reach. He needed only to move east across Germany, from the Black
Forest town of Freiburg to the region known as Lausitz, near the Polish border.
Here Hüttl encountered a landscape as eerie and fascinating as another
planet’s: lakes as acid as vinegar but teeming with microorganisms, more than a
thousand square kilometres of sandy soil that threatens to collapse underfoot at
any moment, and rivers swollen with extraordinary quantities of water pumped
from deep underground.
This bizarre terrain is a legacy of decades of intensive coal mining. “We
have conditions here that are unique in the world,” says Hüttl, with a hint
of pride. He now occupies a newly established chair for Land Preservation and
Recultivation at the University of Cottbus, in the heart of the region.
For environmentalists, the coal mines are a disaster. But for Hüttl and
hundreds of researchers like him, they offer a remarkable research opportunity.
The German government is spending billions of marks to restore these areas to
productive uses, and has called on an army of geochemists, hydrologists and
microbiologists for advice on how to go about it. There are even those who see a
different sort of value in the region, and want to preserve it as a unique
natural habitat harbouring rare native species.
What makes Germany’s mining regions extraordinary, says Hüttl, is their
colossal scale. During the 1970s and 1980s, tiny East Germany was second only to
China in…
![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)


