Some early amphibians had legs strong enough to do press-ups, according
to American palaeontologists who have found the shoulder bone of an early
amphibian in Pennsylvania. The bone, which is 365 million years old, shows
markings where strong muscles were once attached.
Only one older amphibian is known: the 370-million-year-old Scat Craig
fossil found three years ago in Scotland. However, scientists were unable
to study the creature’s legs because the fossil was too fragmentary.
Amphibians evolved more than 370 million years ago from freshwater fish
that had bony lobe-shaped fins, similar to those in lungfish. The new amphibian,
named Hynerpeton, is described by Edward Daeschler of the Academy of Natural
Sciences of Philadelphia in Science (vol 265, p 639). When taken together
with other fossils, Daeschler says it points to the evolution of a range
of amphibians, instead of there being just a single evolutionary path.
So far, Daeschler has found only the shoulder and some skull fragments.
However, according to his colleague, Neil Shubin of the University of Pennsylvania,
the shoulder is the bone that reveals the most about early amphibians.
Marks on the bone show that the leg was strongly muscled, and could pivot
for walking. There is no sign of a ridge where gills attached in other amphibians,
indicating that Hynerpeton was adapted to breathing air.
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The creature was up to a metre long, and weighed about 10 kilograms.
It lived in a flat, marshy tropical area beside a stream. Early amphibians
may have evolved strong limbs to move in shallow water, and then moved toward
the land, which plants and insects had colonised. Some specialists think
amphibians came ashore to exploit food resources, but Daeschler suggests
the real advantage was escaping predators. ‘It was a fish-eat-fish world,’
he says.
![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)


