Video: Why a scared expression brings a survival advantage

You wrinkle your nose and squint when you see a dead rat in the road, but open your eyes, nose and mouth wide when you see a live one in your bedroom.
Why? Common facial expressions like disgust and fear, new research suggests, do more than just convey how you are feeling – they alter your sensory relationship to the world around you.
Charles Darwin, noticing that some facial expressions seem to hold across cultures and even species, proposed that they function to improve certain senses. Now and colleagues at the University of Toronto, Canada, have put that to the test.
Advertisement
The team wanted to know if fear, and its apparent sensory opposite, disgust, changed the way we use our senses. They hypothesised that the former, with its open eyes, raised eyebrows and gaping mouth, led to greater sensory acquisition, allowing greater vigilance, and disgust, with the face all scrunched up, led to less.
Face of fear
In one experiment, volunteers had to identify when a dot entered their visual field, while they maintained fearful, neutral or disgusted expressions.
In another, also with these expressions, they had to move their eyes as quickly as possible between two targets about 30 centimetres apart on a computer screen while their eyes were tracked.
The amount of air that could be breathed in while showing fear and disgust was also measured.
In each case, the researchers found, the expression of fear – or the “Home Alone face”, as Susskind nicknames it – let significantly more of the world in.
Speedy senses
The open eyes allowed quicker detection of objects on the periphery, as well as faster eye movements back and forth, while an open nose took in more air with each breath without any extra effort. An MRI scan confirmed the difference in the space in the nasal cavity.
“These changes are consistent with the idea that fear, for example, is a posture towards vigilance,” says Susskind, “and disgust a posture towards sensory rejection.”
Further experiments, he says, will explore to what extent the brain actually uses this extra information to enhance performance.
Cognitive neuroscientist at New York University, US, thinks the research could open up a whole new way of thinking about facial expressions. “What was nice was the number of different ways they got at this question,” she says.
Journal reference: (DOI: 10.1038/nn.2138)
![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)


