Corpses that could not be recognised by standard methods after an Air
Inter Airbus A-320 crash in January were eventually identified by DNA fingerprints.
This is the first time that genetic fingerprinting has been used during
a disaster and has raised the issue of whether DNA banks should be set up
for high-risk professions.
Within 10 days of the crash in woods near Strasbourg, a team of French
forensic scientists, dental surgeons and biologists had identified 68 of
the 87 corpses by conventional methods such as matching dental records and
blood tests.
‘We then decided to use genetic fingerprinting, both to identify the
remaining 19 and also on those already identified, which allowed us to assemble
all the remains of each individual,’ said Patrice Mangin, director of the
Institute of Forensic Medicine at the Louis Pasteur University in Strasbourg.
Sixteen of the remaining corpses were identified by comparing their
DNA profiles with those of nearest relatives; the other three could not
be identified. The technique relies on detecting familial traits within
DNA.
Advertisement
Whenever possible, both parents of the suspected victim had a blood
sample taken to give the best chance of a match. Where there was only one
parent, siblings and offspring provided further comparisons. Mangin also
used what he calls ‘reverse filiation’, in which a suspected victim’s children
supply DNA to identify the parent.
‘I don’t think DNA fingerprinting will take over from conventional methods
for the time being, said Mangin. The cost of fingerprinting after the Strasbourg
crash was 1.5 million francs ( £150 000).
‘Paradoxically,’ said Mangin, ‘it was very difficult to get information
for conventional identification on the crew. With a DNA bank it would be
fast and simple and would only cost £50 to take and stock a person’s
DNA for life.’ Identification of pilots after a fatal accident can be crucial.
Toxicology tests can reveal whether a pilot had taken alcohol or a medication
before the flight.
French airlines have shown no sign of wanting to use DNA banks. Air
Inter is creating identity files of all staff. These include dental X-rays
but not DNA profiles.
![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)


