ANCIENT they may be, but the Icelandic sagas could provide new insights
into the genetic causes of many common diseases. A company called deCode
Genetics, based in Reykjavik, has been set up to take advantage of Iceland’s
unique combination of fastidious record keeping—which has its origins in
the medieval sagas—and the population’s extremely low genetic variability.
These two factors make Iceland an ideal place to search for disease
genes.
The 270 000 Icelanders alive today are almost all descended from a small
group of Norwegian pioneers who colonised the island in the 9th century. To
identify genes connected with particular diseases, geneticists study families
with a history of the condition. They compare DNA sequences of affected family
members with those from healthy relatives, looking for unusual sequences in
affected people that might turn out to be the defective genes. Identifying the
disease genes is much easier if the population as a whole shares very similar
DNA.
Medical and family records in Iceland are among the best in the world, and
extend back for centuries. For instance, deCode Genetics has shown that 107 of
Iceland’s 1200 asthmatics can trace their ancestry to a single individual who
lived 11 generations ago.
Already, the company’s 55 researchers believe they are close to discovering a
gene linked to multiple sclerosis. They are also hot on the trail of genes for
inflammatory bowel disease, insulin-dependent diabetes and psoriasis, says
Kári Stefansson, deCode’s president.
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Stefansson hopes that his company, which has been financed by venture capital
from the US and Europe, will boost the country’s economy. “Iceland traditionally
lives by fish alone, so there’s a tremendous need to diversify into new
industries,” he says.
Although many companies around the world possess automated DNA sequencing
machines, the technology is often not the limiting factor. “The scarce resource
is not technology or gene sequences, it’s access to the right populations,” says
Stefansson.
John Todd, a specialist in the genetics of diabetes at the University of
Oxford, says that geneticists worldwide have been trying to get their hands on
Icelandic DNA samples. “The Icelanders have repelled all these invaders and
decided to do it themselves,” he says.
DeCode is now negotiating with some of the world’s largest pharmaceuticals
companies, which hope to use deCode’s genetic insights to design new drugs.
Stefansson would like these deals to reward Icelanders for the genetic
information they are providing. “I think it’s very likely that partners will be
asked to donate drugs or offer services at lower prices than usual to the
population,” says Stefansson.
![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)


