Berlin
IT IS now possible to hear plants scream. Physicists at the University of
Bonn have developed a device that listens to the stress responses of household
plants. They hope it will reveal what makes so many geranium seedlings die after
the long trip to Germany from their nurseries in the Mediterranean.
When plants are under stress, because of drought or exposure to salt, ozone
and cold, they emit ethylene gas. The experimental device, built by researchers
at Bonn’s Institute of Applied Physics, excites ethylene molecules with an
infrared laser. The laser beam is “chopped” or interrupted 2000 times per
second. Each time the beam excites the ethylene molecules, they release their
energy in the form of a tiny shock wave in the surrounding atmosphere.
These 2000-hertz vibrations are amplified with a resonance tube, similar to a
small organ pipe, then detected with a sensitive microphone. Higher levels of
ethylene produce a louder sound.
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The basic technique was developed by scientists at the Catholic University of
Nijmegen in the Netherlands. But the new German device is more sensitive, and
allows scientists for the first time to study living plants for long periods
while subjecting them to stress-producing conditions.
Frank Kühnemann, one of the researchers, says that the Bonn team has so
far have measured stress levels in tobacco plants deprived of water and exposed
to high levels of ozone. Kühnemann hopes that horticulturalists will now
use the device to identify which conditions—such as vibration and
temperature—kill fragile geranium seedlings in transit.
![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)


