Billions of snow crabs have vanished from Alaskan waters Danita Delimont / Alamy Stock Photo
So many snow crabs have disappeared from Alaskan waters that the Alaska Department of Fish and Game (ADF&G) has had to for the first time. It is not known exactly why the crabs are disappearing so quickly but warming waters could be to blame.
In 2018, there were around 8 billion 听(Chionoecetes opilio) scuttling along the floor of the Bering Sea. Last year, that number fell to just 1 billion 鈥 a population drop of more than 87 per cent.
The lack of crabs could be a result of particularly warm water in the Bering Sea in 2018 and 2019, says at ADF&G. The cold-water-loving crustaceans may have been limited to pockets of frigid water, which would reduce access to food and increase competition. That in turn could have made the crabs stressed and more susceptible to disease and predation, says Westphal.
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Since the early 1980s, snow crab populations have crept northward by around 30 kilometres, according to the US , probably because the animals were searching for colder temperatures.
Alaska has also paused the harvest of 听(Paralithodes camtschaticus) for the second year in a row, citing low numbers of mature female crabs. It isn’t yet clear how long the pause on snow crab harvests will last. Though it is an economic blow to the local fishing industry, officials say the move is necessary to protect the remaining crabs.
鈥淚t is likely that we will continue to see [snow crab] declines for the next 3 to 4 years,鈥 says Westphal, who notes that ADF&G saw large number of young crabs during its survey this summer. 鈥淲e are hopeful that if these small crab survive鈥 the population will eventually rebuild.鈥
![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)


