(Image: Simone Pika/Research Group “Comparative Gestural Signalling”/Max Planck Institute for Ornithology)
How do you capture a raven’s heart? Arrest its attention by showing it a twig or stone. Ravens use referential gestures – one of the foundations of human language – to initiate relationships.
From an early age we learn to use referential gestures such as pointing to direct another’s attention. “People think that this pointing forms the basis of language,” says Simone Pika at the Max Planck Institute for Ornithology in Seewiesen, Germany. “It has also been linked with mental-state attribution – the idea that you understand what I am pointing out.”
Apes raised in captivity can learn to use referential gestures to communicate with their human caregivers. Now Pika and Thomas Bugnyar at the University of Vienna, Austria, have recorded common ravens () using them for the first time.
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The researchers observed seven pairs of wild ravens showing and offering stones, twigs and moss to each other – by holding the object in their beaks – in an apparent attempt to grab the attention of another bird and initiate a relationship. Importantly, the ravens made these gestures only when another bird was watching, and the items they show and offer are not food. They usually gesture only to members of the opposite sex.
Like humans, ravens form monogamous pairs that will defend a territory and raise their young together. They even develop a repertoire of vocalisations that are exclusive to the couple.
This high degree of cooperation may be what prompted the evolution of referential gestures in both humans and ravens, Pika says. “If communication is governed by cooperation, then this could be what prompted the evolution of language.”
of the University of Cambridge says that the conclusions, although fascinating, should be viewed with caution. Although it might look like the birds are attempting to redirect the attention of another bird, the behaviour might simply be a mating or nesting ritual triggered by a peak in hormones, she says.
at the University of Oxford would like to know whether the ravens have as much flexibility as humans in their range of gestures and responses: “If both sender and receiver use a small, rigid set of targets, and fixed actions for responding, then the interactions could have more in common with classic avian communication systems than with human attention-sharing.”
Journal reference: , DOI: 10.1038/ncomms1567
![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)


