Fossil site is 'Rosetta Stone' for understanding early life

Leading edge technology has uncovered secrets about a world-renowned fossil hoard that could offer vital clues about early life on earth.

Researchers who analysed the 400 million-year-old-cache, found in rural north-east Scotland, say their findings reveal better preservation of the fossils at a molecular level than was previously anticipated.

Fresh scrutiny of the exquisitely preserved treasure trove from Aberdeenshire has enabled scientists to identify the chemical fingerprints of the various organisms within it.

Just as the Rosetta Stone helped Egyptologists translate hieroglyphics, the team hopes these chemical codes can help them decipher more about the identity of the life forms, that other more ambiguous fossils represent.

The spectacular fossil ecosystem near the Aberdeenshire village of Rhynie was discovered in 1912, mineralised and encased by chert -- hard rock composed of silica.Known as the Rhynie chert, it originates from the Early Devonian period -- about 407 million years ago -- and has a significant role to play in scientists understanding of life on earth.

Researchers combined the latest non-destructive imaging with data analysis and machine learning to analyse fossils from collections held by National Museums Scotland and the Universities of Aberdeen and Oxford.Scientists from the University of Edinburgh were able to probe deeper than has previously been possible, which they say could reveal new insights about less well-preserved samples.

Employing a technique known as FTIR spectroscopy -- in which infrared light is used to collect high-resolution data -- researchers found impressive preservation of molecular information within the cells, tissues and organisms in the rock.

Since they already knew which organisms most of the fossils represented, the team was able to discover molecular fingerprints that reliably discriminate between fungi, bacteria and other groups.

These fingerprints were then used to identify some of the more mysterious members of the Rhynie ecosystem, including two specimens of an enigmatic tubular "nematophyte."

These strange organisms, which are found in Devonian -- and later Silurian -- sediments have both algal and fungal characteristics and were previously hard to place in either category. The new findings indicate that they were unlikely to have been either lichens or fungi.

Dr Sean McMahon, Chancellor's Fellow from the University of Edinburgh's School of Physics and Astronomy and School of GeoSciences, said: "We have shown how a quick, non-invasive method can be used to discriminate between different lifeforms, and this opens a unique window on the diversity of early life on Earth."

The team fed their data into a machine learning algorithm that was able to classify the different organisms, providing the potential for sorting other datasets from other fossil-bearing rocks.

The study, published in Nature Communications, was funded by The Royal Society, Wallonia-Brussels International and the National Council of Science and Technology of Mexico.

Dr Corentin Loron, Royal Society Newton International Fellow from the University of Edinburgh's School of Physics and Astronomy said the study shows the value of bridging palaeontology with physics and chemistry to create new insights into early life.

"Our work highlights the unique scientific importance of some of Scotland's spectacular natural heritage and provides us with a tool for studying life in trickier, more ambiguous remnants," Dr Loron said.

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Genome research: Origin and evolution of vine

Cultivation and growth of grapevines have strongly influenced European civilizations, but where the grapevine comes from and how it has spread across the globe has been highly disputed so far. In an extensive genome project, researchers from the Chinese Yunnan Agricultural University have determined its origin and evolution from the wild vine to today's cultivar by analyzing thousands of vine genomes collected along the Silk Road from China to Western Europe. The collection of wild vines of Karlsruhe Institute of Technology (KIT) played an important role in the above project.

Grapevine is among the world's oldest crops. Wine was one of the oldest products traded all around the world. It pushed the exchange of cultures, ideas, and religions. At the end of the Ice Age, grapevine originated from the European wild vine, of which only a few relic populations have survived to date.

One of these populations can be found on the Ketsch peninsula on the Rhine river between Karlsruhe and Mannheim. So far, the traces of when and where exactly wild vines were domesticated, of whether grapes for wine production and table grapes have the same origin, and how thousands of vines developed have been hidden in the mist of the prehistoric era. Still, it is clear that grapevine survived partly drastic climate changes and gathered a number of genes from Asia as a result of early human migration movements. "For some years now, it has been known that today's Silk Road once was a wine road.

The Chinese symbol for alcohol is derived from Georgian wine jugs, so-called Qevri," explains Professor Peter Nick of KIT's Joseph-Gottlieb Kölreuter Institut for Plant Sciences (JKIP). Nick, who had already cooperated with Chinese researchers in a previous project to determine grapevine genomes, suggested to collect grapevines along the previous Silk Road and to analyze their genomes.

Most Detailed Model of the Evolution and Domestication of Grapevine So Far

Nick's idea gave rise to a network of researchers from 16 countries, who contributed not only wild vines and old species from their regions, but also knowledge on their origin and history. Under most difficult circumstances resulting from the global political situation, DNA samples of more than 3500 vines, including more than 1000 wild species, were sent to the State Key Laboratory for Conservation and Utilization of Bio-Resources of Yunnan Agricultural University. There, the genomes were decoded under the direction of Dr. Wei Chen and the most detailed model of the evolution and domestication of grapevines so far was generated. As a result, a number of new findings have been obtained. Now, the origin of winegrowing can be dated back to earlier than 11,000 B.C. in the South Caucasus. This means that wine is older than bread. Winegrowing technology very quickly spread across the Mediterranean to the west. Within shortest terms, cross-breeding with local wild vines produced a large variety of vines that were reproduced using cuttings. About 7000 years ago in the Middle East, large-berry species developed to table vines.

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Ultrafast beam-steering breakthrough

In a major breakthrough in the fields of nanophotonics and ultrafast optics, a Sandia National Laboratories research team has demonstrated the ability to dynamically steer light pulses from conventional, so-called incoherent light sources.

This ability to control light using a semiconductor device could allow low-power, relatively inexpensive sources like LEDs or flashlight bulbs to replace more powerful laser beams in new technologies such as holograms, remote sensing, self-driving cars and high-speed communication.

"What we've done is show that steering a beam of incoherent light can be done," said Prasad Iyer, Sandia scientist and lead author of the research, which was reported in the current issue of the journal Nature Photonics. The work was funded by the Department of Energy's Office of Science.

Incoherent light is emitted by many common sources, such as an old-fashioned incandescent light bulb or an LED bulb. This light is called incoherent since the photons are emitted with different wavelengths and in a random fashion. A beam of light from a laser, however, does not spread and diffuse because the photons have the same frequency and phase and is thus called coherent light.

In the team's research, they manipulated incoherent light by using artificially structured materials called metasurfaces, made from tiny building blocks of semiconductors called meta-atoms that can be designed to reflect light very efficiently. Although metasurfaces had previously shown promise for creating devices that could steer light rays to arbitrary angles, they also presented a challenge because they had only been designed for coherent light sources. Ideally, one would want a semiconductor device that can emit light like an LED, steer the light emission to a set angle by applying a control voltage and shift the steering angle at the fastest speed possible.

The researchers started with a semiconductor metasurface that had embedded tiny light sources called quantum dots. By using a control optical pulse, they were able to change, or reconfigure, the way the surface reflected light and steer the light waves emitted from the quantum dots in different directions over a 70-degree range for less than a trillionth-of-a-second, marking a significant success. Similar to laser-based steering, the steered beam restrained the tendency of incoherent light to spread over a wider viewing angle and instead produced bright light at a distance.

Taming light

A feat previously considered impossible, the team's proof-of-principle work paves the way for developments in the fields of nanophotonics and ultrafast optics. The ability to dynamically control incoherent light sources and manipulate their properties offers a wide range of applications.

One low-power use would be to brighten military helmet screens used to overlay maps or blueprints over ordinary vision. "In applications where space is valuable," Iyer said, "steering light emission with low-size-and-weight metasurface-LED displays could be made possible in the future with this technology. We can use the light emitted in a better way rather than just turning them off and on."

The technique could also provide a new kind of small display that can project holographic images onto eyeballs using low-power LEDs, a capability of particular interest for augmented and virtual reality devices. Other uses could be in self-driving cars where LIDAR is used to sense objects in the path of the car.

In terms of expressions of interest, the team has had several inquiries from commercial sources, said Sandia researcher Igal Brener, a paper author and lead scientist on the project. "A commercial product could be 5-10 years out, especially if we want to have all the functionality on-chip," Brener said. "You wouldn't use a control optical pulse to impart the changes in the metasurface needed to steer the light, but rather you would do this control electrically. We have ideas and plans, but it's still early. Imagine an LED light bulb that can emit light to follow you. Then you wouldn't waste all that illumination where there's nobody. This is one of the many applications that we dreamed about with DOE years ago for energy efficiency for office lighting, for example."

Similarly, tamed light may one day offer benefits in scenarios where focused illumination is only needed in a specific area of interest, such as surgery or in autonomous vehicles.

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Remains of a modern glacier found near Mars' equator implies water ice possibly present at low latitudes on Mars even today

In a groundbreaking announcement at the 54th Lunar and Planetary Science Conference held in The Woodlands, Texas, scientists revealed the discovery of a relict glacier near Mars' equator. Located in Eastern Noctis Labyrinthus at coordinates 7° 33' S, 93° 14' W, this finding is significant as it implies the presence of surface water ice on Mars in recent times, even near the equator. This discovery raises the possibility that ice may still exist at shallow depths in the area, which could have significant implications for future human exploration.

The surface feature identified as a "relict glacier" is one of many light-toned deposits (LTDs) found in the region. Typically, LTDs consist mainly of light-colored sulfate salts, but this deposit also shows many of the features of a glacier, including crevasse fields and moraine bands. The glacier is estimated to be 6 kilometers long and up to 4 kilometers wide, with a surface elevation ranging from +1.3 to +1.7 kilometers. This discovery suggests that Mars' recent history may have been more watery than previously thought, which could have implications for understanding the planet's habitability.

"What we've found is not ice, but a salt deposit with the detailed morphologic features of a glacier. What we think happened here is that salt formed on top of a glacier while preserving the shape of the ice below, down to details like crevasse fields and moraine bands," said Dr. Pascal Lee, a planetary scientist with the SETI Institute and the Mars Institute, and the lead author of the study.

The presence of volcanic materials blanketing the region hints of how the sulfate salts might have formed and preserved a glacier's imprint underneath. When freshly erupted pyroclastic materials (mixtures of volcanic ash, pumice, and hot lava blocks) come in contact with water ice, sulfate salts like the ones commonly making up Mars' light-toned deposits may form and build up into a hardened, crusty salt layer.

"This region of Mars has a history of volcanic activity. And where some of the volcanic materials came in contact with glacier ice, chemical reactions would have taken place at the boundary between the two to form a hardened layer of sulfate salts," explains Sourabh Shubham, a graduate student at the University of Maryland's Department of Geology, and a co-author of the study. "This is the most likely explanation for the hydrated and hydroxylated sulfates we observe in this light-toned deposit."

Over time, with erosion removing the blanketing volcanic materials, a crusty layer of sulfates mirroring the glacier ice underneath became exposed, which would explain how a salt deposit is now visible, presenting features unique to glaciers such as crevasses and moraine bands.

"Glaciers often present distinctive types of features, including marginal, splaying, and tic-tac-toe crevasse fields, and also thrust moraine bands and foliation. We are seeing analogous features in this light-toned deposit, in form, location, and scale. It's very intriguing," said John Schutt, a geologist at the Mars Institute, experienced icefield guide in the Arctic and Antarctica, and a co-author of this study.

The glacier's fine-scale features, its associated sulfate salts deposit, and the overlying volcanic materials are all very sparsely cratered by impacts and must be geologically young, likely Amazonian in age, the latest geologic period which includes modern Mars. "We've known about glacial activity on Mars at many locations, including near the equator in the more distant past. And we've known about recent glacial activity on Mars, but so far, only at higher latitudes. A relatively young relict glacier in this location tells us that Mars experienced surface ice in recent times, even near the equator, which is new," said Lee.

It remains to be seen whether water ice might still be preserved underneath the light-toned deposit or if it has disappeared entirely. "Water ice is, at present, not stable at the very surface of Mars near the equator at these elevations. So, it's not surprising that we're not detecting any water ice at the surface. It is possible that all the glacier's water ice has sublimated away by now. But there's also a chance that some of it might still be protected at shallow depth under the sulfate salts."

The study draws an analogy with the ancient ice islands on salt lakebeds, or salars, of the Altiplano in South America. There, old glacier ice has remained protected from melting, evaporation, and sublimation underneath blankets of bright salts. Lee and his co-authors hypothesize a similar situation to explain how sulfate salts on Mars might be able to offer protection to otherwise sublimation-vulnerable ice at low latitudes on the planet.

If there is still water ice preserved at shallow depths at a low latitude on Mars, there would be implications for science and human exploration. "The desire to land humans at a location where they might be able to extract water ice from the ground has been pushing mission planners to consider higher latitude sites. But the latter environments are typically colder and more challenging for humans and robots. If there were equatorial locations where ice might be found at shallow depth, then we'd have the best of both environments: warmer conditions for human exploration and still access to ice," said Lee.

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Stressed out: Mapping the human footprint on coastal areas globally

A global mapping project led by University of Queensland researchers has revealed the major stressors placed upon global coastlines by human activity.

The team quantified and mapped the presence and extent of major land-based and marine stressors, finding that 97 per cent of coastal areas globally had at least one major stressor present.

Professor Salit Kark from UQ's School of Biological Sciences said the research team were surprised at the sheer extent and far-reaching impact revealed by the footprint map created.

"There is hardly anywhere on the planet, outside of the polar and arctic regions, that does not show some form of human pressure on their coastline," Professor Kark said.

"In essence, we have influenced the majority of coastal areas globally.

"We therefore should aim to map and understand our impacts, and also leave some untouched coastlines."

UQ PhD candidate Hannah Allan said the research outlined the spatial extent and magnitude of 10 major land-based stressors and 10 major marine stressors that occur across coastlines globally.

"The threats human activity pose to coastal ecosystems and biodiversity come from both the land and sea, sometimes arriving far from human activity," Ms Allan said.

"Therefore, coastal conservation must incorporate land-sea connections.

"Human population size, tourism, and roads were some of the biggest contributors to the terrestrial component of Australia's coastal human footprint.

"As for marine stressors, increasing sea surface temperatures, nutrient pollution, and shipping were found to be major drivers of human pressure on Australian coastlines."

Professor Noam Levin said a map of this kind, which assembles both terrestrial and marine stressors and presents the coastal human footprint globally, has rarely been attempted.

"This research offers valuable insights that could help decision-makers and managers identify where to mitigate particular impacts," Prof. Levin said.

"For example, the database underlying the human footprint can show specific areas with high oil and gas operations, such as in Western Australia.

"This can help develop preparedness procedures for the very realistic chance of environmental disasters that impact coastal areas, such as oil spills.

"An added benefit of our new global map is that it helps prioritise these decisions based on how widespread the potential pressures of our human footprint in certain areas of the world might be.

"Coastal areas, where 90 per cent of Australians live, were not immune to these stressors.

"For Australia, the highest human footprint was found in the coastal cities, in the order of Melbourne, Sydney, Perth, Adelaide, and Brisbane.

"We also mapped 160 areas on the planet with the most pristine coastal areas, including several in Australia.

"Of those, nearly 40 per cent were totally unprotected -- opening an opportunity to identify coastal areas for further conservation actions.

"A key finding was that light pollution is increasing, with more white LEDs being used, placing great strain on areas of high importance for biodiversity, disrupting the natural patterns of wildlife."

Moving forward, researchers are looking to fine-tune the mapping process, looking more specifically at Australia's coastlines.

Read more at Science Daily

Cans or bottles: What's better for a fresh, stable beer?

The flavor of beer begins to change as soon as it's packaged, prompting a debate among afficionados: Does the beverage stay fresher in a bottle or a can? Now, researchers report in ACS Food Science & Technology that the answer is, well, complicated, and depends on the type of beer. An amber ale stayed fresher in bottles, whereas container choice made much less difference to the stability of an India Pale Ale (IPA).

In addition to water and ethanol, beer contains thousands of flavor compounds, which are metabolites produced by yeast, hops and other ingredients. During storage, chemical reactions break down some of those components while forming others. This reduces the content of some tasty flavors while generating unappetizing ones, contributing to the aging, or staling, of beer. To help brewers prolong shelf life, researchers have studied beer aging, but they've concentrated on light lagers and a limited group of chemicals. Jessica Prenni and colleagues wanted to extend that work to amber ale and IPA, as well as additional compounds. The team also wanted to conduct the first stability comparison of beer packaged in glass bottles versus aluminum cans.

Cans and brown bottles of amber ale and IPA were chilled for a month and then kept at room temperature for five months to mimic typical storage conditions. Every two weeks, the researchers analyzed the metabolites in newly opened containers. Throughout this time, the concentration of certain metabolites in amber ale -- including some amino acids and esters -- differed significantly depending on whether it was packaged in a bottle or can. IPA, however, was much less sensitive to packaging type, possibly because of its higher concentration of polyphenols from hops. These compounds not only prevent oxidation but also bind to amino acids, thus retaining them in the beer rather than allowing them to get stuck to the inside of a container.

The researchers also found that the metabolic profile of both amber ale and IPA changed over time, whether packaged in a can or bottle. However, amber ale in cans showed the greatest variation during aging. Once scientists find out how all of these changes affect flavor, brewers will be able to make more-informed decisions about the best type of packaging for their particular type of beer.

From Science Daily

First detection of neutrinos made at a particle collider

A team including physicists of the University of Bern has for the first time detected subatomic particles called neutrinos created by a particle collider, namely at CERN's Large Hadron Collider (LHC). The discovery promises to deepen scientists' understanding of the nature of neutrinos, which are among the most abundant particles in the universe and key to the solution of the question why there is more matter than antimatter.

Neutrinos are fundamental particles that played an important role in the early phase of the universe. They are key to learn more about the fundamental laws of nature, including how particles acquire mass and why there is more matter than antimatter. Despite being among the most abundant particles in the universe they are very difficult to detect because they pass through matter with almost no interaction. They are therefore often called "ghost particles."

Neutrinos have been known for several decades and were very important for establishing the standard model of particle physics. But most neutrinos studied by physicists so far have been low-energy neutrinos. Previously, no neutrino produced at a particle collider had ever been detected by an experiment. Now, an international team including researchers from the Laboratory for High Energy Physics (LHEP) of the University of Bern has succeeded in doing just that. Using the FASER particle detector at CERN in Geneva, the team was able to detect very high energy neutrinos produced by brand a new source: CERN's Large Hadron Collider (LHC). The international FASER collaboration announced this result on March 19 at the MORIOND EW conference in La Thuile, Italy.

FASER enables investigation of high energy neutrinos

The properties of neutrinos have been studied in numerous experiments since their discovery in 1956 by Clyde L. Cowan and Frederick Reines. One of the leading experiments to study neutrinos is the Deep Underground Neutrino Experiment (DUNE) being built in the USA. The University of Bern is a key contributor. Experiments like DUNE are general purpose and can study many properties of neutrinos from a variety of sources. One aspect that is not covered is very high energy neutrinos.

The highest energy accelerator available is the LHC at CERN, where new particles are produced by two beams of protons smashing together at extremely high energy. However, neutrinos have never been detected at any collider because they escape the existing detectors at the LHC.

The FASER experiment was proposed to fill this gap. "In this experiment we measure very high energy neutrinos produced by the LHC collider at CERN. The goal is to study how these neutrinos are produced, what their properties are and to look for signals of new particles," says Akitaka Ariga, leader of the FASER group at University of Bern's Laboratory for High Energy Physics (LHEP). The LHEP is part of the Physics Institute and of the Albert Einstein Center for Fundamental Physics (AEC). "The FASER experiment is a unique idea at the interface between the highest energy colliders and neutrino physics. Often new discoveries are made when taking such new approaches," says Michele Weber, director of the LHEP of the University of Bern.

Hidden physics in neutrinos?

For the current observation of neutrinos, the experiment took data at the LHC in 2022. The team detected 153 events that are neutrino interactions with extremely high certainty. The neutrinos detected by FASER are of the highest energy ever produced in a lab and are similar to the neutrinos coming from deep-space that trigger dramatic particle showers in our atmosphere or the earth. They are therefore also an important tool to researchers for better understanding observations in particle astrophysics.

"This achievement is a historical milestone for obtaining a new neutrino source with unexplored features," says Akitaka Ariga. The presented result is just the very beginning of a series of explorations. The experiment will continue to take data till the end of 2025. "There might be hidden physics in neutrinos at high energy scale," says Akitaka Ariga.

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Mix-and-match kit could enable astronauts to build a menagerie of lunar exploration bots

When astronauts begin to build a permanent base on the moon, as NASA plans to do in the coming years, they'll need help. Robots could potentially do the heavy lifting by laying cables, deploying solar panels, erecting communications towers, and building habitats. But if each robot is designed for a specific action or task, a moon base could become overrun by a zoo of machines, each with its own unique parts and protocols.

To avoid a bottleneck of bots, a team of MIT engineers is designing a kit of universal robotic parts that an astronaut could easily mix and match to rapidly configure different robot "species" to fit various missions on the moon. Once a mission is completed, a robot can be disassembled and its parts used to configure a new robot to meet a different task.

The team calls the system WORMS, for the Walking Oligomeric Robotic Mobility System. The system's parts include worm-inspired robotic limbs that an astronaut can easily snap onto a base, and that work together as a walking robot. Depending on the mission, parts can be configured to build, for instance, large "pack" bots capable of carrying heavy solar panels up a hill. The same parts could be reconfigured into six-legged spider bots that can be lowered into a lava tube to drill for frozen water.

"You could imagine a shed on the moon with shelves of worms," says team leader George Lordos, a PhD candidate and graduate instructor in MIT's Department of Aeronautics and Astronautics (AeroAstro), in reference to the independent, articulated robots that carry their own motors, sensors, computer, and battery. "Astronauts could go into the shed, pick the worms they need, along with the right shoes, body, sensors and tools, and they could snap everything together, then disassemble it to make a new one. The design is flexible, sustainable, and cost-effective."

Lordos' team has built and demonstrated a six-legged WORMS robot. Last week, they presented their results at IEEE's Aerospace Conference, where they also received the conference's Best Paper Award.

MIT team members include Michael J. Brown, Kir Latyshev, Aileen Liao, Sharmi Shah, Cesar Meza, Brooke Bensche, Cynthia Cao, Yang Chen, Alex S. Miller, Aditya Mehrotra, Jacob Rodriguez, Anna Mokkapati, Tomas Cantu, Katherina Sapozhnikov, Jessica Rutledge, David Trumper, Sangbae Kim, Olivier de Weck, Jeffrey Hoffman, along with Aleks Siemenn, Cormac O'Neill, Diego Rivero, Fiona Lin, Hanfei Cui, Isabella Golemme, John Zhang, Jolie Bercow, Prajwal Mahesh, Stephanie Howe, and Zeyad Al Awwad, as well as Chiara Rissola of Carnegie Mellon University and Wendell Chun of the University of Denver.

Animal instincts

WORMS was conceived in 2022 as an answer to NASA's Breakthrough, Innovative and Game-changing (BIG) Idea Challenge -- an annual competition for university students to design, develop, and demonstrate a game-changing idea. In 2022, NASA challenged students to develop robotic systems that can move across extreme terrain, without the use of wheels.

A team from MIT's Space Resources Workshop took up the challenge, aiming specifically for a lunar robot design that could navigate the extreme terrain of the moon's South Pole -- a landscape that is marked by thick, fluffy dust; steep, rocky slopes; and deep lava tubes. The environment also hosts "permanently shadowed" regions that could contain frozen water, which, if accessible, would be essential for sustaining astronauts.

As they mulled over ways to navigate the moon's polar terrain, the students took inspiration from animals. In their initial brainstorming, they noted certain animals could conceptually be suited to certain missions: A spider could drop down and explore a lava tube, a line of elephants could carry heavy equipment while supporting each other down a steep slope, and a goat, tethered to an ox, could help lead the larger animal up the side of a hill as it transports an array of solar panels.

"As we were thinking of these animal inspirations, we realized that one of the simplest animals, the worm, makes similar movements as an arm, or a leg, or a backbone, or a tail," says deputy team leader and AeroAstro graduate student Michael Brown. "And then the lightbulb went off: We could build all these animal-inspired robots using worm-like appendages.'"

Snap on, snap off

Lordos, who is of Greek descent, helped coin WORMS, and chose the letter "O" to stand for "oligomeric," which in Greek signifies "a few parts."

"Our idea was that, with just a few parts, combined in different ways, you could mix and match and get all these different robots," says AeroAstro undergraduate Brooke Bensche.

The system's main parts include the appendage, or worm, which can be attached to a body, or chassis, via a "universal interface block" that snaps the two parts together through a twist-and-lock mechanism. The parts can be disconnected with a small tool that releases the block's spring-loaded pins.

Appendages and bodies can also snap into accessories such as a "shoe," which the team engineered in the shape of a wok, and a LiDAR system that can map the surroundings to help a robot navigate.

"In future iterations we hope to add more snap-on sensors and tools, such as winches, balance sensors, and drills," says AeroAstro undergraduate Jacob Rodriguez.

The team developed software that can be tailored to coordinate multiple appendages. As a proof of concept, the team built a six-legged robot about the size of a go-cart. In the lab, they showed that once assembled, the robot's independent limbs worked to walk over level ground. The team also showed that they could quickly assemble and disassemble the robot in the field, on a desert site in California.

In its first generation, each WORMS appendage measures about 1 meter long and weighs about 20 pounds. In the moon's gravity, which is about one-sixth that of Earth's, each limb would weigh about 3 pounds, which an astronaut could easily handle to build or disassemble a robot in the field. The team has planned out the specs for a larger generation with longer and slightly heavier appendages. These bigger parts could be snapped together to build "pack" bots, capable of transporting heavy payloads.

"There are many buzz words that are used to describe effective systems for future space exploration: modular, reconfigurable, adaptable, flexible, cross-cutting, et cetera," says Kevin Kempton, an engineer at NASA's Langley Research Center, who served as a judge for the 2022 BIG Idea Challenge. "The MIT WORMS concept incorporates all these qualities and more."

Read more at Science Daily

Lasers and chemistry reveal how ancient pottery was made -- and how an empire functioned

Peru’s first great empire, the Wari, stretched for more than a thousand miles over the Andes Mountains and along the coast from 600-1000 CE. The pottery they left behind gives archaeologists clues as to how the empire functioned. In a new study in the Journal of Archaeological Science: Reports, researchers showed that rather than using “official” Wari pottery imported from the capital, potters across the empire were creating their own ceramics, decorated to emulate the traditional Wari style. To figure it out, the scientists analyzed the pottery’s chemical make-up, with help from laser beams.

“In this study, we looked at the idea of cosmopolitanism, of incorporating different cultures and practices into a society,” says M. Elizabeth Grávalos, a postdoctoral researcher at the Field Museum in Chicago and the study’s lead author. “We’re trying to show that potters were influenced by the Wari, but this influence was blended with their own local cultural practices.”

Grávalos says this model of cosmopolitanism is a little like trying to replicate a recipe from another culture, but with a local spin. “If you live in the US and you’re making pad thai at home, you might not have access to all the ingredients that someone living in Thailand would have, so you substitute some things,” she says. “Wari ceramics are a little like that — people throughout the empire were interested in Wari material culture, but they weren’t necessarily getting it directly from the Wari heartland. More often than not, we see local people trying to make their own version of Wari pottery.”

Grávalos and her colleagues led archaeological digs throughout Peru, working with local communities to excavate the thousand-year-old remains of households, tombs, and administrative centers, in search of Wari lifeways. The researchers were then granted permission from Peru’s Ministry of Culture to bring samples of ceramics from their excavations to Chicago for analysis.

Clay from different regions has a different chemical makeup, so studying the ceramics’ chemical makeup could tell the researchers if the pots were produced in different places or if they were all imported from the Wari capital.

“We’d take a tiny piece of a pot and used a laser to cut an even tinier piece, basically extracting a piece of the ceramic’s clay paste,” says Grávalos. “Then helium gas carried it to the mass spectrometer, which measures the elements present in the  clay paste.” (The lab set-up didn’t have open laser beams and floating shards of pottery cutting across the room, though — the whole process takes place on a microscopic scale inside a big boxy machine.)

The analysis showed that the pots excavated from distinct regions of Peru have different chemical signatures, and were therefore made with distinct clays. That helps show how the Wari culture spread.

Some empires, like the ancient Romans, took a “top-down” approach to spreading their aesthetic, shipping pottery across the Mediterranean so that people throughout the empire were using the official Roman style. Local potters emulating the traditional Wari style in their own work seems to hint at a more “bottom-up” approach.

“Of course, local people in all empires have some degree of agency and creative control — the only empire that’s truly top-down is the Borg from Star Trek,” says Patrick Ryan Williams, Curator of Archaeological Science and Director of the Elemental Analysis Facility  at the Field Museum and the study’s senior author. “Even the Romans had local people doing things their own way. But what we’re finding in this study is the agency of local peoples and the importance of local economies. In some regions, we find that Wari colonists had their own production centers and were recreating Wari lifeways locally. In other areas, we see that local communities made Wari pottery in their own way. I think that’s what’s really important about this study.”

The researchers say that the patterns revealed by this pottery could help explain why the Wari empire was able to thrive for so long. “Local production, even in a cosmopolitan society with lots of far-flung connections, makes a society more resilient,” says Williams. “If you’re entirely dependent on someone far away sending you things you need, you’re extremely vulnerable.”

Read more at Science Daily

New approach to harvesting aerial humidity with organic crystals

Researchers of the Smart Materials Lab (SML) and the Center for Smart Engineering Materials (CSEM) at NYU Abu Dhabi (NYUAD) have reported a novel method of harvesting water from naturally occurring sources such as fog and dew.

In the study, Research Scientist Patrick Commins and Post-doctoral Associate Marieh B. Al-Handawi observed for the first time the process of water spontaneously condensing from its vapor to liquid form and moving across the surface of a slowly subliming organic crystal. This was found to be caused by changes in the width of small channels that appear on the surface of the crystal over time, which guide the condensed water across the crystal's surface.

In the paper titled Autonomous and Directional Flow of Water and Transport of Particles across a Subliming Dynamic Crystal Surface published in the journal Nature Chemistry, researchers describe the process of condensation and movement of water that carries particles on the surface of crystals of hexachlorobenzene, a compound that is often used as a fungicide. Due to sublimation, the surface of this material has a rigid topography with defined parallel channels. Small solid particles such as dust or even metallic nanoparticles were observed to move autonomously along the channels. The motion of these particles was found to be caused by the condensed aerial water, which migrates through the channels due to the change in the cross-section and width of the channels over time.

Autonomous water flow has previously been achieved utilizing either surface chemical modifications or precisely fabricated microchannels, or on the surface of natural systems such as some plants or insects. The findings from this new study hold the potential to guide the creation of new technologies to utilize naturally occurring sources of water such as dew and fog, which are currently only used by some desert plants and animals for survival. The new research builds on the understanding of water collection mechanisms of such biological structures, while it presents a fundamentally different mechanism for water transportation.

"The motion of water on solid surfaces is one of the most fundamental phenomena found in nature," said Panče Naumov, a leader of the Smart Materials Lab and Director of the Center for Smart Engineering Materials, and the corresponding author of the study. "Through millennia-long evolutionary processes, surfaces of natural organisms have been optimized for efficient transport of water for a variety of life-supporting functions. Plants have been seen to do this by moving water against gravity. Our team has discovered a new way to move water across a dynamic solid surface, a fundamentally new underlying principle of water collection. This can provide an inspiration for emerging technologies that could potentially maximize the efficiency of experimental systems used for the collection of aerial humidity."

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