Tuesday, 25 March 2025

Chimpanzees act as 'engineers', choosing materials to make tools based on structural and mechanical properties

 

Date:
March 24, 2025
Source:
University of Oxford
Summary:
Researchers have discovered that chimpanzees living in Gombe Stream National Park in Tanzania employ a degree of engineering when making their tools, deliberately choosing plants that provide materials that produce more flexible tools for termite fishing.

A multidisciplinary team of researchers from the School of Anthropology and Museum Ethnography at the University of Oxford, the Max Planck Institute for Evolutionary Anthropology, the Jane Goodall Institute in Tanzania, the University of Algarve and the University of Porto in Portugal, and the University of Leipzig, have discovered that chimpanzees living in Gombe Stream National Park in Tanzania employ a degree of engineering when making their tools, deliberately choosing plants that provide materials that produce more flexible tools for termite fishing.



These findings, published in the journal iScience, have important implications for understanding the technical abilities associated with the making of perishable tools -- a topic which remains a highly unknown aspect of human technological evolution.

Termites are a good source of energy, fat, vitamins, minerals and protein for chimpanzees. To eat the insects, chimpanzees need to use relatively thin probes to fish the termites out of the mounds where they live. Given that the inside of the mounds is made up of winding tunnels, the scientists hypothesized that using flexible tools would be more effective for chimpanzees at fishing out the insects than using rigid sticks.

To test this, first author Alejandra Pascual-Garrido took a portable mechanical tester to Gombe and measured how much force it took to bend plant materials used by the apes compared to plant materials that were available but never used. Findings showed that plant species never used by chimpanzees were 175 percent more rigid than their preferred materials.

Furthermore, even among plants growing near termite mounds, those that showed obvious signs of regular use by the apes produced more flexible tools than nearby plants that showed no signs of use.

"This is the first comprehensive evidence that wild chimpanzees select tool materials for termite fishing based on specific mechanical properties," says Alejandra Pascual-Garrido, who has been studying the raw materials used in chimpanzee tools in Gombe for more than a decade.

Notably, certain plant species, such as Grewia spp., also constitute tool material for termite fishing chimpanzee communities living up to 5,000 kilometres away from Gombe, implying that the mechanics of these plant materials could be a foundation for such ubiquitous preferences, and that rudimentary engineering may be deeply rooted in chimpanzee tool-making culture.

Wild chimpanzees may therefore possess a kind of "folk physics" -- an intuitive comprehension of material properties that helps them choose the best tools for the job.

Their natural engineering ability is not just about using any stick or plant that is available; chimpanzees specifically select materials with mechanical properties that can make their foraging tools more effective.

Dr Alejandra Pascual-Garrido, Research Affiliate at the School of Anthropology and Museum Ethnography, University of Oxford, said: 'This novel approach, which combines biomechanics with animal behaviour, helps us better understand the cognitive processes behind chimpanzee tool construction and how they evaluate and select materials based on functional properties'.

The findings raise important questions about how this knowledge is learned, maintained and transmitted across generations, for example, by young chimpanzees observing and using their mothers' tools, and whether similar mechanical principles determine chimpanzees' selection of materials for making other foraging tools, such as those used for eating ants or harvesting honey.

'This finding has important implications for understanding how humans might have evolved their remarkable tool using abilities,' explains Adam van Casteren, Department of Human Origins, Max Planck Institute for Evolutionary Anthropology, a specialist in biomechanics and evolutionary biology. 'While perishable materials like wood rarely survive in the archaeological record, the mechanical principles behind effective tool construction and use remain constant across species and time'.

By studying how chimpanzees select materials based on specific structural and/or mechanical properties, we can better understand the physical constraints and requirements that would have applied to early human tool use. Using such a comparative functional framework provides new insights into aspects of early technology that are not preserved in the archaeological record.


Story Source:

Materials provided by University of Oxford.


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Monday, 24 March 2025

 

Saturday, 22 March 2025

Treasure trove of galaxies, glimpses of deep fields

 

Date:
March 19, 2025
Source:
European Space Agency
Summary:
On 19 March 2025, the European Space Agency's Euclid mission releases its first batch of survey data, including a preview of its deep fields. Here, hundreds of thousands of galaxies in different shapes and sizes take center stage and show a glimpse of their large-scale organization in the cosmic web.

On 19 March 2025, the European Space Agency's Euclid mission releases its first batch of survey data, including a preview of its deep fields. Here, hundreds of thousands of galaxies in different shapes and sizes take centre stage and show a glimpse of their large-scale organisation in the cosmic web.



Covering a huge area of the sky in three mosaics, the data release also includes numerous galaxy clusters, active galactic nuclei and transient phenomena, as well as the first classification survey of more than 380,000 galaxies and 500 gravitational lens candidates compiled through combined artificial intelligence and citizen science efforts. All of this sets the scene for the broad range of topics that the dark Universe detective Euclid is set to address with its rich dataset.

"Euclid shows itself once again to be the ultimate discovery machine. It is surveying galaxies on the grandest scale, enabling us to explore our cosmic history and the invisible forces shaping our Universe," says ESA's Director of Science, Prof. Carole Mundell.

"With the release of the first data from Euclid's survey, we are unlocking a treasure trove of information for scientists to dive into and tackle some of the most intriguing questions in modern science. With this, ESA is delivering on its commitment to enable scientific progress for generations to come."


Tracing out the cosmic web in Euclid's deep fields

Euclid has scouted out the three areas in the sky where it will eventually provide the deepest observations of its mission. In just one week of observations, with one scan of each region so far, Euclid already spotted 26 million galaxies. The farthest of those are up to 10.5 billion light-years away. The fields also contain a small population of bright quasars that can be seen much farther away. In the coming years, Euclid will pass over these three regions tens of times, capturing many more faraway galaxies, making these fields truly 'deep' by the end of the nominal mission in 2030.

But the first glimpse of 63 square degrees of the sky, the equivalent area of more than 300 times the full Moon, already gives an impressive preview of the scale of Euclid's grand cosmic atlas when the mission is complete. This atlas will cover one-third of the entire sky -- 14,000 square degrees -- in this high-quality detail.

"It's impressive how one observation of the deep field areas has already given us a wealth of data that can be used for a variety of purposes in astronomy: from galaxy shapes, to strong lenses, clusters, and star formation, among others," says Valeria Pettorino, ESA's Euclid project scientist. "We will observe each deep field between 30 and 52 times over Euclid's six year mission, each time improving the resolution of how we see those areas, and the number of objects we manage to observe. Just think of the discoveries that await us."

To answer the mysteries it is designed for, Euclid measures the huge variety of shapes and the distribution of billions of galaxies very precisely with its high-resolution imaging visible instrument (VIS), while its near-infrared instrument (NISP) is essential for unravelling galaxy distances and masses. The new images already showcase this capability for hundreds of thousands of galaxies, and start to hint at the large-scale organisation of these galaxies in the cosmic web. These filaments of ordinary matter and dark matter weave through the cosmos, and from these, galaxies formed and evolved. This is an essential piece in the puzzle towards understanding the mysterious nature of dark matter and dark energy, which together appear to make up 95% of the Universe.

"The full potential of Euclid to learn more about dark matter and dark energy from the large-scale structure of the cosmic web will be reached only when it has completed its entire survey. Yet the volume of this first data release already offers us a unique first glance at the large-scale organisation of galaxies, which we can use to learn more about galaxy formation over time," says Clotilde Laigle, Euclid Consortium scientist and data processing expert based at the Institut d'Astrophysique de Paris, France.


Humans and AI classify more than 380,000 galaxies

Euclid is expected to capture images of more than 1.5 billion galaxies over six years, sending back around 100 GB of data every day. Such an impressively large dataset creates incredible discovery opportunities, but huge challenges when it comes to searching for, analysing and cataloguing galaxies. The advancement of artificial intelligence (AI) algorithms, in combination with thousands of human citizen science volunteers and experts, is playing a critical role.

"We're at a pivotal moment in terms of how we tackle large-scale surveys in astronomy. AI is a fundamental and necessary part of our process in order to fully exploit Euclid's vast dataset," says Mike Walmsley, Euclid Consortium scientist based at the University of Toronto, Canada, who has been heavily involved in astronomical deep learning algorithms for the last decade.

"We're building the tools as well as providing the measurements. In this way we can deliver cutting-edge science in a matter of weeks, compared with the years-long process of analysing big surveys like these in the past," he adds.

A major milestone in this effort is the first detailed catalogue of more than 380,000 galaxies, which have been classified according to features such as spiral arms, central bars, and tidal tails that infer merging galaxies. The catalogue is created by the 'Zoobot' AI algorithm. During an intensive one-month campaign on Galaxy Zoo last year, 9976 human volunteers worked together to teach Zoobot to recognise galaxy features by classifying Euclid images.

This first catalogue released today represents just 0.4% of the total number of galaxies of similar resolution expected to be imaged over Euclid's lifetime. The final catalogue will present the detailed morphology of at least an order of magnitude more galaxies than ever measured before, helping scientists answer questions like how spiral arms form and how supermassive black holes grow.

"We're looking at galaxies from inside to out, from how their internal structures govern their evolution to how the external environment shapes their transformation over time," adds Clotilde.

"Euclid is a goldmine of data and its impact will be far-reaching, from galaxy evolution to the bigger-picture cosmology goals of the mission."


Gravitational lensing discovery engine

Light travelling towards us from distant galaxies is bent and distorted by normal and dark matter in the foreground. This effect is called gravitational lensing and it is one of the tools that Euclid uses to reveal how dark matter is distributed through the Universe.

When the distortions are very apparent, it is known as 'strong lensing', which can result in features such as Einstein rings, arcs, and multiple imaged lenses.

Using an initial sweep by AI models, followed by citizen science inspection, expert vetting and modelling, a first catalogue of 500 galaxy-galaxy strong lens candidates is released today, almost all of which were previously unknown. This type of lensing happens when a foreground galaxy and its halo of dark matter act as a lens, distorting the image of a background galaxy along the line of sight towards Euclid.

With the help of these models, Euclid will capture some 7000 candidates in the major cosmology data release planned for the end of 2026, and in the order of 100,000 galaxy-galaxy strong lenses by the end of the mission, around 100 times more than currently known.

Euclid will also be able to measure 'weak' lensing, when the distortions of background sources are much smaller. Such subtle distortions can only be detected by analysing large numbers of galaxies in a statistical way. In the coming years, Euclid will measure the distorted shapes of billions of galaxies over 10 billion years of cosmic history, thus providing a 3D view of the distribution of dark matter in our Universe.

"Euclid is very quickly covering larger and larger areas of the sky thanks to its unprecedented surveying capabilities," says Pierre Ferruit, ESA's Euclid mission manager, who is based at ESA's European Space Astronomy Centre (ESAC) in Spain, home of the Astronomy Science Archive where Euclid's data will be made available.

"This data release highlights the incredible potential we have by combining the strengths of Euclid, AI, citizen science and experts into a single discovery engine that will be essential in tackling the vast volume of data returned by Euclid."


Notes

As of 19 March 2025, Euclid has observed about 2000 square degrees, approximately 14% of the total survey area (14 000 square degrees). The three deep fields together comprise 63.1 square degrees.

Euclid 'quick' releases, such as the one of 19 March, are of selected areas, intended to demonstrate the data products to be expected in the major data releases that follow, and to allow scientists to sharpen their data analysis tools in preparation. The mission's first cosmology data will be released to the community in October 2026. Data accumulated over additional, multiple passes of the deep field locations will be included in the 2026 release.



About Euclid

Euclid was launched in July 2023 and started its routine science observations on 14 February 2024. In November 2023 and May 2024, the world got its first glimpses of the quality of Euclid's images, and in October 2024 the first piece of its great map of the Universe was released.

Euclid is a European mission, built and operated by ESA, with contributions from its Member States and NASA. The Euclid Consortium -- consisting of more than 2000 scientists from 300 institutes in 15 European countries, the USA, Canada and Japan -- is responsible for providing the scientific instruments and scientific data analysis. ESA selected Thales Alenia Space as prime contractor for the construction of the satellite and its service module, with Airbus Defence and Space chosen to develop the payload module, including the telescope. NASA provided the detectors of the Near-Infrared Spectrometer and Photometer, NISP. Euclid is a medium-class mission in ESA's Cosmic Vision Programme.


Story Source:

Materials provided by European Space Agency.


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Friday, 21 March 2025

Violent supernovae 'triggered at least two Earth extinctions'

 

Date:
March 13, 2025
Source:
Royal Astronomical Society
Summary:
At least two mass extinction events in Earth's history were likely caused by the 'devastating' effects of nearby supernova explosions, a new study suggests. Researchers say these super-powerful blasts -- caused by the death of a massive star -- may have previously stripped our planet's atmosphere of its ozone, sparked acid rain and exposed life to harmful ultraviolet radiation from the Sun. They believe a supernova explosion close to Earth could be to blame for both the late Devonian and Ordovician extinction events, which occurred 372 and 445 million years ago respectively

At least two mass extinction events in Earth's history were likely caused by the "devastating" effects of nearby supernova explosions, a new study suggests.



Researchers at Keele University say these super-powerful blasts -- caused by the death of a massive star -- may have previously stripped our planet's atmosphere of its ozone, sparked acid rain and exposed life to harmful ultraviolet radiation from the Sun.

They believe a supernova explosion close to Earth could be to blame for both the late Devonian and Ordovician extinction events, which occurred 372 and 445 million years ago respectively.

The Ordovician extinction killed 60 per cent of marine invertebrates at a time when life was largely confined to the sea, while the late Devonian wiped out around 70 per cent of all species and led to huge changes in the kind of fish that existed in our ancient seas and lakes.

Past research has failed to identify a clear cause for either event, although they are thought to have been linked to the depletion of Earth's ozone layer, which could have been triggered by a supernova.

The new study, published today in Monthly Notices of the Royal Astronomical Society, found that the rate supernovae occur near to our planet is consistent with the timings of both mass extinctions.

The authors say it is a "a great illustration for how massive stars can act as both creators and destructors of life."

That's because supernovae are also known to spread the heavy elements that help form and support life across the universe.

Supernovae occur when massive stars reach the end of their lives, run out of fuel, cool off, and then collapse under the pressure of gravity. The explosions are the biggest humans have ever seen.

Lead author Dr Alexis Quintana, formerly from Keele University and now at the University of Alicante, said: "Supernova explosions bring heavy chemical elements into the interstellar medium, which are then used to form new stars and planets.

"But if a planet, including the Earth, is located too close to this kind of event, this can have devastating effects."

Dr Nick Wright, from Keele University, added: "Supernova explosions are some of the most energetic explosions in the universe.

"If a massive star were to explode as a supernova close to the Earth, the results would be devastating for life on Earth. This research suggests that this may have already happened."

The researchers came to their conclusion after carrying out a "census" of massive stars within a kiloparsec (around 3,260 light-years) of the Sun.

They were studying the distribution of these massive stars, known as OB stars, to learn more about how star clusters and galaxies form by using the Milky Way itself as a benchmark, and the rate at which these stars form in our galaxy.

This census allowed the researchers to calculate the rate at which supernovae occur within the galaxy, which is important for observations of supernovae, and the production of supernova remnants and massive stellar remnants such as black holes and neutron stars throughout the universe.

The data will also be useful for future development of gravitational wave detectors, which are a useful tool for scientists studying the structure and origins of the universe.

As part of this the research team calculated the supernova rate within 20 parsecs of the Sun, or approximately 65 light-years, and compared this with the approximate rate of mass extinction events on Earth that have previously been attributed to nearby supernovae.

This excludes extinction events linked to other factors such as asteroid impacts or the ice ages.

Comparing these data sets, the experts found that their research supported the theory that a supernova explosion was responsible for both the late Devonian and Ordovician extinction events -- two of the five known mass extinctions in Earth's history.

"We calculated the supernova rate close to Earth and found it to be consistent with the rate of mass extinction events on our planet that have been linked to external forces such as supernovae," Dr Wright explained.

Astronomers believe about one or two supernovae -- or possibly at a rate even lower than that -- occur each century in galaxies like the Milky Way, but the good news is there are only two nearby stars which could go supernova within the next million years or so: Antares and Betelgeuse.

However, both of these are more than 500 light-years away from us and computer simulations have previously suggested a supernova at that distance from Earth likely wouldn't affect our planet.


Story Source:

Materials provided by Royal Astronomical Society


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Chimpanzees act as 'engineers', choosing materials to make tools based on structural and mechanical properties

  Date: March 24, 2025 Source: University of Oxford Summary: Researchers have discovered that chimpanzees living in Gombe Stream National Pa...