THE waters around Antarctica may be teeming with a far greater diversity of
larvae than biologists realised. Researchers diving under the ice have
discovered 10 times as many different types of larvae as were previously known
to be there. They could provide a barometer to gauge the effects of climate
change, the scientists say.
Many bottom-dwelling marine animals, such as starfish, have larvae that drift
in the plankton. According to a rule proposed by the Danish marine biologist
Gunnar Thorson in 1950, the diversity of these drifting larvae should decline
from the tropics to the poles as waters get colder. Polar invertebrates are more
likely to produce larvae that stay on the bottom, as food supplies for drifting
larvae disappear in dark polar winters.
However, Damon Stanwell-Smith and his colleagues at the British Antarctic
Survey in Cambridge have found an unprecedented diversity of larval life
drifting in the chilly waters of the Weddell and Scotia Seas, where Thorson’s
rule predicts there should be only a few different species. Their two-year
survey around the South Orkney Islands netted 131 different types of planktonic
larvae in an area where just 12 were known before. “Nobody has sampled all year
round and nobody has looked at larvae in detail,” explains Lloyd Peck, who
supervised the study. “Biodiversity is as high as in temperate and maybe even
tropical latitudes.”
Stanwell-Smith collected the larvae while diving around Signy Island, towing
a plankton net by hand with the help of another diver. The team took samples
every two weeks, even during winter when the sea was covered by ice. They then
grouped the larvae into different types on the basis of their shapes.
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In a forthcoming issue of Philosophical Transactions of the Royal Society
B, the team will propose that ideas about the pattern of larval
biodiversity on our planet need to be revised. “All the work taught in
university courses is based on three or four surveys by Thorson in the 1930s and
1940s in the North Atlantic,” says Peck.
A clear picture of larval biodiversity will help biologists assess any
effects resulting from climate change. “If we’re going to see big losses in
species from climate change, the Antarctic is the place to look,” says Peck. “In
an environment where animals are adapted to low, very constant temperatures,
they will be vulnerable to small temperature changes.” Peck believes a slight
but sudden rise in temperature could have a catastrophic effect on the larvae,
as there is probably only a narrow range of temperatures in which they develop
normally.
“Our ideas about polar marine systems are changing very fast,”says David
Barnes, an Antarctic marine biologist at University College of Cork in Ireland.
“There’s a lot more going on in winter than people knew about, probably because
nobody really bothered to look.”
![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)


