The surprising strategy employed by weaver ants has left scientists stunned, as their unique approach to teamwork could potentially transform the field of robotics. A recent study published in Current Biology reveals that individual weaver ants actually increase their contribution to tasks when working in larger groups, defying the long-standing problem of declining performance with team size.

This phenomenon was first observed by French engineer Max Ringelmann in 1913, who found that human teams’ total force increased as more people joined in, but each individual’s contribution decreased. In contrast, weaver ants (Oecophylla smaragdina) have evolved to form super-efficient teams where individuals actually get better at working together as the group gets bigger.

Lead author Madelyne Stewardson from Macquarie University explains that each individual ant almost doubles their pulling force as team size increases. The researchers set up experiments enticing weaver ant colonies to form pulling chains to move an artificial leaf connected to a force meter. They found that the ants split their work into two jobs: some actively pull while others act like anchors to store the pulling force.

The key to this mechanism lies in the “force ratchet” theory developed by co-lead author Dr Daniele Carlesso from the University of Konstanz. Ants at the back of chains stretch out their bodies to resist and store the pulling force, while ants at the front keep actively pulling. This method allows longer chains of ants to have more grip on the ground, better resisting the force of the leaf pulling back.

The discovery has significant implications for robotics, as current robots only output the same force when working in teams as when alone. Dr Chris Reid from Macquarie’s School of Natural Sciences says that programming robots to adopt ant-inspired cooperative strategies could allow teams of autonomous robots to work together more efficiently.

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As scientists continue to explore the vast expanse of our solar system, a new study has shed light on a long-held assumption about the conditions necessary for life to thrive. Researchers at NYU Abu Dhabi have made a groundbreaking discovery that challenges the traditional view that life can only exist near sunlight or volcanic heat. Their findings suggest that high-energy particles from space, known as cosmic rays, could create the energy needed to support microscopic life underground on planets and moons in our solar system.

The research, led by Principal Investigator Dimitra Atri, focused on what happens when cosmic rays hit water or ice underground. The impact breaks water molecules apart and releases tiny particles called electrons. Some bacteria on Earth can use these electrons for energy, similar to how plants use sunlight. This process is called radiolysis, and it can power life even in dark, cold environments with no sunlight.

Using computer simulations, the researchers studied how much energy this process could produce on Mars and on the icy moons of Jupiter and Saturn. These moons, which are covered in thick layers of ice, are believed to have water hidden below their surfaces. The study found that Saturn’s icy moon Enceladus had the most potential to support life in this way, followed by Mars, and then Jupiter’s moon Europa.

“This discovery changes the way we think about where life might exist,” said Atri. “Instead of looking only for warm planets with sunlight, we can now consider places that are cold and dark, as long as they have some water beneath the surface and are exposed to cosmic rays. Life might be able to survive in more places than we ever imagined.”

The study introduces a new idea called the Radiolytic Habitable Zone. Unlike the traditional “Goldilocks Zone” — the area around a star where a planet could have liquid water on its surface — this new zone focuses on places where water exists underground and can be energized by cosmic radiation. Since cosmic rays are found throughout space, this could mean there are many more places in the universe where life could exist.

The findings provide new guidance for future space missions. Instead of only looking for signs of life on the surface, scientists might also explore underground environments on Mars and the icy moons, using tools that can detect chemical energy created by cosmic radiation.

This research opens up exciting new possibilities in the search for life beyond Earth and suggests that even the darkest, coldest places in the solar system could have the right conditions for life to survive. As we continue to explore the mysteries of our universe, it’s clear that there’s still much to learn, and this discovery is a thrilling reminder of the incredible potential that lies just beneath the surface.

The iconic monitor lizards of Australia, commonly known as goannas, have long been a symbol of the country’s unique wildlife. However, beneath their scaly skin lies an unexpected secret: a hidden layer of bony skin structures known as osteoderms. These structures, which were previously thought to be rare in lizards, are found in nearly half of all lizard species worldwide and may hold the key to understanding how these ancient reptiles not only survived but thrived in one of the world’s harshest environments.

A recent study published in the prestigious Zoological Journal of the Linnean Society has shed new light on the widespread presence of osteoderms in lizards. The research, which was conducted by an international team of scientists from Australia, Europe, and the United States, used cutting-edge micro-CT scanning to examine nearly 2,000 reptile specimens from major museum collections.

“We were astonished to find osteoderms in 29 Australo-Papuan monitor lizard species that had never been documented before,” said Roy Ebel, lead author and researcher at Museums Victoria Research Institute and the Australian National University. “It’s a fivefold increase in known cases among goannas.”

Osteoderms are most commonly associated with crocodiles, armadillos, and even some dinosaurs like Stegosaurus. However, their function has remained something of an evolutionary mystery. While they may provide protection, scientists now suspect that osteoderms may also support heat regulation, mobility, and calcium storage during reproduction.

This new research reveals that osteoderms are far more widespread in lizards than previously thought, occurring in nearly half of all lizard species worldwide – an 85% increase on earlier estimates. The findings have significant implications for our understanding of reptile evolution and the adaptation of these ancient creatures to harsh environments.

At the heart of this discovery lies the power of museum collections. Scientific institutions like Museums Victoria Research Institute play a critical role in preserving biodiversity through time, enabling researchers to study species long after they were collected. Many of the specimens used in this study were decades, and in some cases over 120 years old, but advances in imaging technology enabled scientists to uncover new insights without harming the original material.

“What’s so exciting about this finding is that it reshapes what we thought we knew about reptile evolution,” said Dr Jane Melville, Museums Victoria Research Institute Senior Curator of Terrestrial Vertebrates. “It suggests that these skin bones may have evolved in response to environmental pressures as lizards adapted to Australia’s challenging landscapes.”

The discovery of osteoderms in monitor lizards opens up new questions about how these lizards adapted, survived, and diversified across the continent. This landmark study not only tells a new chapter in the story of Australia’s goannas but provides a powerful new dataset for exploring how skin, structure, and survival have intertwined across millions of years of evolution.