Father Christmas has probably never gone “ho ho ho!” in his life. More likely, he just grunts, according to the largest ever study into the sound of laughter.
Photo: Marc Newton/PYMCA
This left the researchers with more than a thousand bursts of laughter to analyse. “One of the biggest surprises was the variety of sounds that constitute laughter,” she says.
Laughter can be “voiced” or song-like – such as giggles and chuckles – or unvoiced, like grunts and snorts. Most of the subjects produced a wide range of laughter types. But women produce voiced, song-like bursts of laughter more often than men, Bachorowski found, while men are more likely to grunt and snort.
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Laughter clichés
The researchers also noted the vowel sounds in the laughter. These can be central – with the mouth more open – as in “turn” or “car”, or non-central, as in “he” or “glow”.
The team heard very few examples of non-central vowels, scuppering the idea that people often go “tee hee” or “ho ho ho”. Other laughter clichés failed to hold up. “Stereotypes accounted for less than half of the laughter recorded,” she says.
The subjects were all Americans, but Bachorowski says the findings may apply to other cultures. “I suspect that culture shapes the circumstances in which we use laughter rather than its features.”
Journal reference: The Journal of the Acoustical Society of America (vol 110, p 1581)
![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)


