‘Refining Bridge Editing: A Potential Improvement Over CRISPR for DNA Modification’

Bridge editing physically links two DNA strands

Visual Science

A powerful DNA-editing mechanism discovered in bacteria has the potential to enable much larger genome modifications than are currently possible with CRISPR-based techniques, but it is not yet clear whether it would work in human cells.

Patrick Shue Researchers at the Ark Institute in California call their new genome editing system the “bridge editing” system because it physically links, or bridges, two strands of DNA. “Using this system, we can modify large parts of the genome,” says Su. Su's team has figured out how bacterial “parasitic” DNA sequences naturally replicate using this system and how it can be applied to genome editing.

“We're excited about the possibility of making much broader genome modifications that go far beyond what we can do today with CRISPR,” he says, “and we see this as an important step toward a broader vision for genome design.”

CRISPR gene editing has revolutionized biology since it was introduced in 2012. It is used for a variety of purposes, and the first CRISPR-based therapeutic was approved last year. However, the basic form of CRISPR, which uses the Cas9 protein, is gene disruption rather than gene editing.

A standard CRISPR Cas9 protein has two parts: one part binds to a guide RNA molecule and looks for DNA that matches a specific section of the guide RNA. Custom guide RNAs are easy to create, so CRISPR Cas9 can be “programmed” to look for any part of the genome.

The second part of CRISPR Cas9 is a cutter that cuts the DNA when Cas9 binds to the target site. Once the cell has repaired the damage, Cas9 cuts it again. This action continues until an error is made during repair, resulting in the intended mutation of the target site.

While being able to mutate specific sites is useful, biologists want to make more precise changes, so they are modifying CRISPR proteins to edit DNA directly rather than relying on cellular repair mechanisms. For example, base editors can change one DNA letter to another without cutting the DNA, while prime editors can convert an extra section of guide RNA into DNA and add it to the target site.

These improved versions of CRISPR have the potential to treat a wide range of diseases, with several clinical trials already underway, but to address some diseases, more sophisticated genome modifications are needed. Many teams around the world are working on ways to achieve this. Some have realized that the mechanism by which genetic parasites cut and paste from one part of the genome to another, called IS110 elements, has potential because, like CRISPR, it is RNA-guided, but Hsu's team is the first to fully understand how it works.

The bridge-editing system consists of a so-called recombinase protein that binds to a guide RNA, such as the CRISPR Cas9 protein. What's unique about this system is that the guide RNA specifies two DNA sequences to seek out, not just one, Hsu's team found.

One sequence specifies the target site in the genome to modify, similar to CRISPR, and the other specifies the DNA to change. Using this system, DNA sequences of virtually any length can be added, deleted, or inverted.

There are already ways to do this, but they typically require multiple steps and leave behind a piece of extra DNA called a scar. “Bridge editing leaves virtually no scar,” Hsu says. “It offers an unprecedented level of control in engineering the genome.”

This means that it could be used for more than just replacing faulty genes, he says: It could also be useful for completely remaking the genomes of plants and animals. “What we want to do is go from inserting individual genes to doing chromosome-scale genome engineering,” Su says.

“The findings reported are certainly exciting and the underlying biology is truly surprising.” Steven Tang Bridge editing is being done at Columbia University in New York, but so far it has only been demonstrated to work in bacterial cells or in test tubes. Tang says it remains to be seen whether and to what extent bridge editing will work in complex cells like humans. But even if bridge editing doesn't work in initial tests in human cells, it may be possible to modify the system to work over time.

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Source: www.newscientist.com

Denmark Makes Historic Move by Implementing Carbon Tax on Gas-Emitting Cows and Pigs

Denmark is taking action to address methane emissions, a significant contributor to global warming. Starting in 2030, Denmark will be the first country to implement a tax on livestock farmers based on the greenhouse gas emissions produced by their cows, sheep, and pigs.

Tax Minister Jeppe Bruus aims to reduce Denmark’s greenhouse gas emissions by 70% by 2030 compared to 1990 levels.

From 2030, Danish livestock farmers will face a tax of 300 kroner ($43) per tonne of carbon dioxide equivalent, increasing to 750 kroner ($108) by 2035. However, with a 60% income tax credit, the effective cost per tonne will start at 120 kroner ($17.3) and gradually rise to 300 kroner by 2035.

While carbon dioxide is often the focus, methane is a potent greenhouse gas, trapping significantly more heat than carbon dioxide over a 20-year period, according to the National Oceanic and Atmospheric Administration.

Methane ConcentrationMethane emissions from various sources, including landfills, oil and gas systems, and livestock, have been on the rise. Livestock alone contributes to about 32% of man-made methane emissions, as reported by the United Nations Environment Programme.

Denmark’s move is a significant step towards achieving climate neutrality by 2045. The country is pioneering the implementation of a substantial carbon tax on agriculture, with hopes that other nations will also take similar actions.

In New Zealand, a similar law was passed but later revoked amid criticism from farmers. Denmark, on the other hand, reached an agreement with various stakeholders to implement the carbon tax.

The Danish Society for Nature Conservation hailed the tax agreement as a “historic compromise,” emphasizing the importance of restructuring the food industry beyond 2030.

Denmark’s decision comes after protests from farmers across Europe, who argue that climate policies are jeopardizing their livelihoods.

Despite Denmark’s status as a major dairy and pork exporter, the country plans to tax pigs alongside cows due to their significant emissions. The tax proposal is expected to receive broad support in the parliament.

Statistics Denmark reported a slight decrease in the number of cattle in the country as of June 30, 2022, with 1,484,377 cattle in total.

Source: www.nbcnews.com

Incredible Map Reveals Earth’s Place in the Expansive Universe

This story is part of our “Cosmic Perspective” series, which confronts the incredible vastness of the universe and our place in it. Read the rest of the series here.

This map shows the cosmic ring that surrounds us, stretching out to distances of up to 200 million light-years. At this scale, the universe is made up of galaxy clusters and voids, the latter being regions with relatively few galaxies. The Milky Way at the center is part of the Local Group, while the Virgo Cluster is our nearest neighbour.

The magnificent spiral

The Milky Way’s spiral structure is dominated by two major arms called Scutum-Centaurus and Perseus. It also features a dense region called the central bar. Our solar system sits on a more modest structure called the Orion Arm.

No matter how complex the questions about our metaphorical place in the universe, astronomy can help us understand Earth’s physical location.

Earth orbits at a distance of 150 million kilometers from the Sun, which in turn orbits the center of the Milky Way galaxy. Specifically, Earth is located in the Orion Arm, about 26,500 light years from the center.

The Milky Way Galaxy is part of the Local Group of galaxies. Its nearest neighbor, the Andromeda Galaxy, is about 2.5 million light-years away and is the largest galaxy in the Local Group. We are currently hurtling towards the Andromeda Galaxy at over 100 kilometers per second, and in about 4 billion years the two galaxies will collide.

Local Groups

It will shake up local groups, but it will barely be on the radar of the wider cosmic neighborhood.

Source: www.newscientist.com

How to Identify and Stay Safe from Human Waste in Your Local River

Have you ever experienced this feeling before? On a blazing hot day, the desire to plunge into a cool stream of water intensifies by the minute. The water appears pristine, clear, and incredibly refreshing. However, in reality, it could be extensively contaminated.

Even the purest rivers can harbor harmful bacteria, including fecal bacteria originating from livestock manure and human waste.

In a recent announcement, the Designated bathing area in the UK, a favored holiday spot, has been a subject of concern due to issues such as being submerged in sewage and incidents of rowers contracting E. coli infections. To address these concerns, we consulted with water and sanitation expert Professor David Werner to provide essential information for safely enjoying wild swimming this summer.


Werner’s research delves into treated sewage, stormwater (untreated sewage overflows following heavy rains), and occasionally illegal sewage disposal in dry weather. These factors impact both human health and ecosystem health. While human waste is discharged into oceans, rivers tend to exhibit higher concentrations of human waste and the accompanying harmful bacteria due to lower dilution levels compared to water bodies, increasing the risk of exposure to harmful substances.

(Notably, a microbiology professor, William Gays, mentioned in BBC Science Focus that rivers have only recently been subjected to the same microbial testing as coastal waters. Moreover, wastewater discharged into the ocean is often subjected to more stringent treatment standards than rivers, including ultraviolet disinfection.)

The following guidelines mainly focus on rivers but are also relevant for coastal swimming activities.

The key takeaway? Avoid swimming after rainfall.

How do diseases enter rivers, and what is the risk of swimming in them?

Fecal contamination doesn’t always mean significant. The majority of people’s stool contains beneficial bacteria essential for our health. However, the stool of an ill individual harbors bacteria responsible for the illness, potentially leading to disease transmission.

According to Warner, the risk of contracting a disease from a river is relatively low, but it escalates if you ingest river water (discouraged but not impossible).

This can result in unpleasant symptoms like infections and diarrhea. The worst-case scenario involves acquiring antibiotic-resistant bacteria, an eventuality deemed highly improbable by Warner.

So, should one abstain from wild swimming altogether? Ultimately, it boils down to whether you are willing to accept the (generally minimal) risk for the mental health benefits, as Warner highlights.

“There is no such thing as absolute safety or zero risk,” he states. “Each time we embark on a car journey, we weigh the trip’s advantages against the accident risks. Similarly, outdoor recreation offers significant mental health perks, particularly for urban dwellers.”

How to safeguard yourself from sewage while swimming

Warner and his team are currently devising a device capable of swiftly testing water for contaminants, akin to a lateral flow corona test, though substantial research is required to materialize this concept.

Until this technology is available, several straightforward methods can help identify sewage presence while swimming in rivers this summer. Here are Warner’s recommendations:

1. Choose your spot wisely

According to Werner, it is crucial to avoid swimming downstream from a sewage treatment plant under any circumstances. While untreated sewage overflows are a common concern, treating sewage does not completely eradicate the risks; it merely diminishes them.

“Treating wastewater significantly reduces the levels of harmful bacteria, possibly by a factor of 1,000, but it doesn’t eliminate them,” Werner explains.

“Hence, if a location is situated immediately downstream of a treatment plant discharge point, one can expect a consistent presence of fecal bacteria due to the continuous discharge.”

Individuals can consult the “Poop Map” and trace their local river upstream to identify any treatment facilities along the route.

2. Check the poop map

UK organizations such as Rivers Trust and Surfers Against Sewage have developed an interactive map showcasing regular treated sewage discharges and anticipated untreated sewage overflows across the UK in 2023.

To locate a wastewater treatment plant on The Rivers Trust map, click the yellow square corresponding to your area or tap the brown circle icon, peruse the cards to pinpoint locations. The phrase “Sewage Discharge – Final/Treated Effluent – Water Companies” typically indicates a wastewater treatment facility.

The Rivers Trust’s interactive wastewater map displaying treated and untreated sewage discharge locations into UK rivers in 2023. – Image credit: Rivers Trust

This year, the charity integrated near real-time data into its maps. “This marks a significant advancement for individuals seeking real-time updates,” remarks Warner. “We strongly recommend utilizing these online resources, offering current information.”

Presently, individuals can ascertain if sewage has been discharged within the last 24 hours, albeit inland data is exclusive to designated bathing locations and rivers within the Thames Basin (Northumbrian Water also provides a County-level map while coastal regions are included).

3. Monitor the weather

Despite the allure of swimming on a sunny day, verify there hasn’t been rainfall for a few days. Swimming post-rainfall significantly heightens the possibility of encountering contaminated water due to sewer overflows and increased water release during heavy downpours.

To compound matters, even as a dry spell seems to prevail and swimming appears safe, hidden risks could lurk upstream. Thunderstorms can unleash localized rainfall, implying that upstream areas may experience heavy showers despite sunshine at your location.

4. Steer clear of small rivers

In addition to potentially turbid waters, small rivers tend to exacerbate the situation as sewage, whether treated or untreated, is less diluted in these settings.

Warner adheres to a safety benchmark stipulating that raw sewage minimal dilution should be 1,000 times for paddling and over 10,000 times for swimming. While calculating these dilution levels is not advised, the underlying principle is straightforward: “A large river with vigorous flow signifies ample dilution,” Werner asserts.

Nonetheless, disparate river segments need not cause undue concern: while one side may seem stagnant relative to the center, the water mixes uniformly.

5. Keep tabs on the paper trail

Exhibit prudence: refrain from swimming if toilet paper is visible. Alarming indicators surpass toilet paper and include wet wipes and sanitary pads crafted from plastic materials that should not be flushed but often are.

According to Werner, unlike toilet paper and human excrement, these items do not disintegrate in swiftly moving waters.

6. Stay informed

“After frolicking in the river, diligently cleanse yourself. Embrace standard personal hygiene,” stresses Werner.


About our experts

David Warner serves as a Professor of Environmental Systems Modelling at Newcastle University. Previously, his research concentrated on sanitation and water quality in low-income countries by utilizing DNA sequencing and assessing microbial hazards in rivers. During travel restrictions amid the pandemic, he shifted his focus to the UK’s rivers. His research on post-rain fecal bacteria levels has been documented in various journals such as Water Science and Technology, Comprehensive Environmental Science, and Environmental Pollution.

William Gays, a Professor of Microbiology at the European Centre for Environment and Human Health within the University of Exeter’s Medical School, conducts research published in journals like International Journal of Antimicrobial Agents, Food and Environmental Virology, and Water Research.

Read more:

Source: www.sciencefocus.com

19 of the Most Incredible and Bizarre Insect Photos from Around the World in 2024

The winning work is Royal Entomological Society Photography Competition An exhibition has been announced showcasing amazing images of insects from around the world.

This tournament Insect Week It showcases the best insect photography by amateurs of all ages, shedding light on the miniature world of insects.

The overall winner of this year’s competition is Luke Chambers from the UK, whose piece “Sleeping Cuckoos” depicts two beautiful cuckoo bees resting on a blade of grass covered with morning dew (scroll down to see it).

The overall winner in the “18 and under” category was 17-year-old Gustaf Pallenmark from Sweden, whose work “Silence” shows a striped damselfly at rest.

The Royal Entomological Society exists to advance the science of insects through research and to increase public understanding and appreciation of insects and the vital role they play in the Earth’s ecosystems.

Here are this year’s fantastic contest winners and some other favourites.

Special Award for Under 18s – Purple Fire

Leaf-cutter wasp (Megachile lagopoda). This species is under threat due to intensive land use. Photo: Gustav Pallenmark

Portrait of Special Praise – Picasso Bug

The aptly named Picasso bug (Sphaerocoris annulus) was photographed in Louiru, Kenya. Photo by Robin Backhouse

Under 18 Runner-up – Robber Fly Breakfast

A spindly-legged centipede fly (Leptarththrus brevirostris) feeds on small insects. Photo by Jamie Smart

Special Award Portrait – Flowers of Evil

European mantis (Mantis religiosa) among cyclamen. Photo by Panagiotis Dalagiorgos

Honorable Mention Portrait – Brown Argus Roosting at Sunrise

A brown argus butterfly (Alicia agastis) warms itself on a stalk of grass as the sun rises, Martin Down, Dorset, UK. Photo by Richard Sheldrake

Particularly praised behavior – mating veins

Two mating Timandra comai moths. Timandra comai moths belong to the Geometridae family. They get their name from the distinctive reddish stripes that run from wing to wing. Photo by Heath McDonald

Specially praised environment – a pair of silverfish

These silverfish (family Bacillarioidea) appear to be stuck together in tiny clay nest structures. Some of their shiny silvery scales are frayed, which may indicate an imminent moult. Photographed in Western Australia. Photo by Frank Ashwood.

Under 18 Winner – Tranquility

A striped male Calopteryx splendens dragonfly photographed in Sweden. Photo by Gustav Pallenmark

Special Smartphone Award – Pollinator

A common Carder’s bumblebee (Bombus pascuorum) collecting pollen from a flower. Photo by Michael Wood

Particularly praised behavior – fatal attraction

A swarm of dead flying ants floats on the surface of a swimming pool. United States. Photo by Rosemary Haleem

Special Award for Under 18s – Camouflage Masters

An Indian praying mantis (Schizocephala bicornis) transforms into a leaf. The color of the mantis and the leaf are almost the same and it is impossible to spot the insect unless it is moving. The mantis’s body was following the veins of the leaf, making it difficult to identify. Photo by Kushaan A Ksheerasagar

Particularly praised behavior – Conopidae column

Male and female red-legged bees (Sicus ferrugineus) nestle after mating. The smaller male guards the female, making sure no other suitors ruin the night. Photo by Luke Chambers

Special Smartphone Award – Wasps join cream teas

A German hornet (Vespula germanica) joins a family enjoying a cream tea at a British cafe. Photo by Abi Batten

Special Smartphone Award – The Moth and the Mountain

A male wolf moth (Saturnia pavonia) rests on the heather on the slopes of Meal Buide. In the background you can see the summit of Stack an Lochaine in the Scottish Highlands. Photographed in Scotland, UK in May 2023. Photo by Marianne Cockburn.

Special Prize Portrait – Centipede

A brown heath robberies (Epitriptus cingulatus) resting on long grass in Droxford, Hampshire, UK. Photo by Stephen Mahy

Particularly rewarded behavior – Junk Bugs

Junk bugs (Chrysopidae) are voracious predators of the insect kingdom, so named because they wear vegetable matter and the exoskeletons of past victims on their backs as part of a complex camouflage to fool predators. Photo by Rosa Dunbar

Special Featured Portrait – The Third Eye

A photo of a velvet wasp (Ichneumonidae) in a moth trap in the UK. Photo by Ben James

2nd place overall – Caddisfly larvae

Spotted sedge caddisfly (Glyphotaelius pellucidus) larvae in a gelatinous egg sac. Taken on a leaf overhanging the water, this image shows newly hatched caddisfly larvae in a clear, gelatinous egg sac. The larvae fall into the water and live as aquatic insects through their larval and pupal stages. Photo by Tim Jonas

Overall Winner – Sleeping Cuckoo

A flying squirrel (Epeolus variegatus) sleeps on a leaf. Morning dew is visible on the surface of its eyes. Photo by Luke Chambers

read

Source: www.sciencefocus.com

Webb studies the intricate makeup of Jupiter’s ionosphere

Jupiter’s upper atmosphere consists of a neutral thermosphere and an electrically charged ionosphere. Astronomers using the NASA/ESA/CSA James Webb Space Telescope have discovered unexpected small-scale intensity features, including arcs, bands, and spots, in the low-latitude ionosphere in the region above Jupiter’s Great Red Spot.

This illustration shows the region observed by Webb, first with its location on the NIRCam image of the entire planet (left), and then the region itself as imaged by Webb’s Near-Infrared Spectrometer (NIRSpec) (right). Image credit: NASA / ESA / CSA / Webb / Jupiter ERS Team / J. Schmidt / H. Melin / M. Zamani, ESA and Webb.

Jupiter is one of the brightest objects in the night sky and can be easily seen on a clear night.

Apart from the bright Northern and Southern Lights at Jupiter’s poles, the glow from Jupiter’s upper atmosphere is weak, making details in this region difficult to discern with ground-based telescopes.

But Webb’s infrared sensitivity has allowed scientists to study the upper atmosphere of the infamous Great Red Spot in unprecedented detail.

The upper atmosphere of this gas giant is the interface between the planet’s magnetic field and the atmosphere below it.

Here you can see the bright and vibrant aurora borealis and southern lights, created by volcanic material erupting from Jupiter’s moon Io.

However, as one approaches the equator, the structure of the planet’s upper atmosphere is influenced by incoming sunlight.

Because Jupiter receives only 4% of the sunlight that Earth does, astronomers predicted that this region would be essentially homogeneous.

Astronomer Henrik Melin of the University of Leicester and his colleagues observed the Great Red Spot in July 2022 using an Integral Field Unit. Webb’s near-infrared spectrometer (NIR Spec).

Their early public science observations aimed to investigate whether this region was in fact dull, and the region above the iconic Great Red Spot was the subject of Webb’s observations.

They were surprised to find that the upper atmosphere contains a variety of complex structures, including dark arcs and bright spots across the entire field of view.

“We probably naively thought this area would be really boring. It’s actually just as interesting, if not more so, than the Northern Lights. Jupiter never fails to surprise us,” Dr Melin said.

The light emitted from this region is driven by sunlight, but the team suggests there must be another mechanism that changes the shape and structure of the upper atmosphere.

“One way this structure can be altered is by gravity waves, similar to how waves crashing on the shore create ripples in the sand,” Dr Melin said.

“These waves originate deep within the turbulent lower atmosphere around the Great Red Spot and can rise in altitude to alter the structure and emissions of the upper atmosphere.”

“These atmospheric waves are occasionally observed on Earth, but they are much weaker than those Webb observed on Jupiter.”

“In the future, we hope to carry out follow-up webbed observations of these complex wave patterns and investigate how they move within the planet’s upper atmosphere to improve our understanding of the energy budget of this region and how its features change over time.”

of Investigation result Published in a journal Natural Astronomy.

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H. Melin othersIrregularities in Jupiter’s ionosphere observed by JWST. Nat AstronPublished online June 21, 2024, doi: 10.1038/s41550-024-02305-9

Source: www.sci.news

CERN Scientists Aim to Produce Enigmatic Higgs Particle Duplicates

Physicists from the ATLAS Collaboration at the Large Hadron Collider (LHC) at CERN have announced the results of the most sensitive search to date for double Higgs production and self-coupling, achieved by combining five double Higgs studies from LHC Run 2 data.

Event display of a double Higgs candidate event, photographed in 2017. Image courtesy of ATLAS Collaboration / CERN.

Remember how hard it was to find one Higgs boson? Now try and find two of them in the same place at the same time.

This intriguing process, known as double Higgs production, can teach scientists about the Higgs particle's self-interaction.

By studying it, physicists can measure the strength of the Higgs particle's self-binding, a fundamental aspect of the Standard Model that links the Higgs mechanism to the stability of the universe.

Searching for the creation of double Higgs particles is a particularly challenging task.

This is an extremely rare process, about 1,000 times rarer than the creation of a single Higgs particle.

While LHC Run 2 produced 40 million collisions per second, ATLAS is expected to produce just a few thousand double Higgs events.

So how can physicists find these rare needles in a mountain of data?

One way to make it easier to find double Higgs production is to search in multiple locations.

By investigating the different ways in which the double Higgs decay (decay modes) and combining them, physicists can maximise their chances of discovering and studying the creation of the double Higgs.

The new results from the ATLAS collaboration are the most comprehensive search to date, covering more than half of all possible double Higgs events with ATLAS.

Each of the five individual studies in this combination focuses on a different mode of damping, each with its own strengths and weaknesses.

For example, the most likely double-Higgs decay mode is the decay into four bottom quarks.

However, the Standard Model QCD process likely also produces four bottom quarks, making it difficult to distinguish this background process from a double Higgs event.

The double-Higgs decay into two bottom quarks and two tau leptons involves moderate background contamination, but it occurs five times less frequently and there are neutrinos that escape undetected, complicating physicists' efforts to recreate the decay.

Decays into multiple leptons are not uncommon, but they have complex characteristics.

Other double Higgs decays are even rarer, such as the decay into two bottom quarks and two photons.

This final state accounts for only 0.3% of all double Higgs decays, but has a cleaner signature and much smaller background contamination.

Combining their findings for each of these decays, ATLAS physicists were able to find that the probability of producing two Higgs particles rules out more than 2.9 times the Standard Model prediction.

This result has a confidence level of 95% and an expected sensitivity of 2.4 (assuming this process does not exist in nature).

They were also able to provide constraints on the strength of the Higgs particle's self-coupling, achieving the highest sensitivity to date for this important observable.

They found that the magnitude of the Higgs self-coupling constant and the strength of the interaction between two Higgs particles and two vector particles are consistent with the Standard Model predictions.

“This overall result marks a milestone in the study of double Higgs particle production,” the researchers said.

their result will be published in journal Physics Review Letter.

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ATLAS Collaboration. 2024. Combined search for Higgs pair production in pp collisions at s√=13 TeV with the ATLAS detector. Physiotherapy Rev Lett,in press; arXiv:2406.09971

Source: www.sci.news

IXPE uncovers a new extremely luminous X-ray source in our galaxy

Cygnus X-3It is an X-ray binary system located about 7,400 parsecs (24,136 light years) away in the constellation Cygnus, and analysis of the data indicates that it is a type of extremely luminous X-ray source. NASA’s Imaging X-ray Polarimetry Probe (IXPE).



The halo around Cygnus X-3. Image courtesy of NASA.

“X-ray binaries are interesting systems that consist of two objects: a normal star and a compact object such as a black hole or neutron star that sucks material from the companion star,” explained astronomer Aleksandra Beredina from the University of Turku and her colleagues.

“To date, several hundred such sources have been identified in our Milky Way galaxy.”

“When it comes to the most powerful phenomena in the Universe, the release of gravitational energy in binary X-ray systems stands out as an extremely efficient process.”

“Among the first X-ray binary systems discovered in the Universe is the Cygnus X-3 system,” the researchers added.

“Since the early 1970s, this binary system has been noted for its ability to briefly appear as one of the most powerful radio sources, only to fade or disappear completely after a few days.”

“This unique feature prompted early efforts to coordinate astronomical observations around the world through telephone coordination.”

“The peculiar behaviour of this system during this short-lived, high-energy event contrasts with its normal nature and led to it being named ‘Astronomical Mystery Cygnus X-3’ by R.M. Helming in 1973.”

“Since then, there have been numerous efforts to understand its properties.”

Dr. Veredina and her co-authors used the Imaging X-ray Polarimetry Explorer to measure the X-ray polarization of Cygnus X-3.

“The X-ray polarization images provide insight into the composition of matter surrounding the compact object in Cygnus X-3,” the researchers said.

“We found that this compact object is surrounded by a dense, opaque membrane of material.”

“The light we see is a reflection from the inner walls of a funnel formed by the surrounding gas, similar to a cup with a mirror on the inside.”

“Cygnus X-3 is a type of Ultraluminous X-ray source (ULX), which consumes material at such a rate that a significant portion of the infalling material does not fall within the event horizon, but rather is ejected out of the system.”

“ULXs are usually observed as points of light in images of distant galaxies, and their radiation is amplified by the focusing effect of the funnel around the compact object, acting like a megaphone,” said Professor Juri Poutanen from the University of Turku.

“But these sources are so far away – thousands of times the extent of the Milky Way – that they appear relatively faint to X-ray telescopes.”

“This discovery reveals that luminous counterparts to these distant ULXs exist within our own Galaxy.”

“This important discovery marks a new chapter in our investigation into the source of this extraordinary universe, providing an opportunity to study its extreme matter consumption in detail.”

of result Published in the journal Natural Astronomy.

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A. Veredina othersIXPE discovered Cygnus X-3 as an ultra-luminous X-ray source in the galaxy. Nat AstronPublished online June 21, 2024, doi: 10.1038/s41550-024-02294-9

Source: www.sci.news

Astrobiologists pinpoint five key greenhouse gases found on terraformed exoplanets

The five man-made greenhouse gases identified by astrobiologist Edward Schwieterman of the University of California, Riverside, and his colleagues could be detected in relatively low concentrations in exoplanet atmospheres using the NASA/ESA/CSA James Webb Space Telescope and future space telescopes.

Diagram of the technological features of various planets, including artificial atmospheric gases. Image courtesy of Sohail Wasif / University of California, Riverside.

“For us, these gases are bad because we don’t want them to accelerate warming,” Dr Schwietermann said.

“But they could be useful to a civilization wanting to halt an impending ice age, or to terraform uninhabitable planets in its own system, as humanity has proposed for Mars.”

“These gases are not known to occur in large quantities in nature, so they have to be manufactured.”

“Finding them would therefore be evidence of the presence of intelligent, technological life forms. Such evidence is called a technosignature.”

The five gases proposed by the authors are used on Earth for industrial purposes, such as making computer chips.

These include fluorinated versions of methane, ethane and propane, as well as gases made of nitrogen and fluorine, or sulfur and fluorine.

One advantage is that it’s a very effective greenhouse gas — sulfur hexafluoride, for example, has a warming power 23,500 times that of carbon dioxide — and even a relatively small amount could heat a frozen planet to the point where liquid water could remain on the surface.

Another advantage of the proposed gas, at least from an alien perspective, is that it is extremely long-lived, surviving in an Earth-like atmosphere for up to 50,000 years.

“You won’t need to refill it very often to maintain a comfortable climate,” Dr. Schwieterman said.

Others suggest that refrigerant chemicals such as CFCs are technology signature gases because they are almost entirely man-made and visible in Earth’s atmosphere.

But unlike the chemically inert fully fluorinated gases discussed in the new paper, CFCs damage the ozone layer and may not be advantageous.

“If other civilizations had oxygen-rich atmospheres, they would have also had an ozone layer that they wanted to protect,” Dr Schwietermann said.

“CFCs will be broken down in the ozone layer while also catalyzing its destruction.”

“CFCs degrade easily and have a short lifespan, making them difficult to detect.”

Finally, for fluorinated gases to have an effect on climate, they need to absorb infrared radiation.

This absorption creates an infrared signature that can be detected by space telescopes.

Using current and planned technology, scientists may be able to detect these chemicals in nearby exoplanetary systems.

“In an Earth-like atmosphere, only one in a million molecules could be any of these gases and be detectable, and that concentration would be enough to even alter the climate,” Dr Schwietermann said.

To reach this calculation, the astrobiologists simulated a planet in the TRAPPIST-1 system, located about 40 light-years from Earth.

They chose this system because it contains at least seven rocky planets and is one of the best-studied planetary systems other than Earth.

Although it is not possible to quantify the likelihood of discovering man-made greenhouse gases in the near future, we are confident that, if they exist, they could be detected during missions currently planned to characterize the planet’s atmosphere.

“If telescopes are already characterizing planets for other reasons, there would be no need for extra effort to look for these technical features,” Dr Schwietermann said.

“And when you find them, it’s amazing.”

Team work Published in Astrophysical Journal.

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Edward W. Schwietermann others2024. Artificial greenhouse gases as a technological feature of exoplanets. ApJ 969, 20; doi: 10.3847/1538-4357/ad4ce8

Source: www.sci.news

Research shows active hydrothermal systems on small ocean planets have the potential to sustain life

Ocean worlds are planetary bodies with liquid oceans, often beneath an icy shell or within rocky interiors. In our solar system, several moons of Jupiter and Saturn are ocean worlds. Some ocean worlds are thought to have hydrothermal circulation, where water, rocks, and heat combine to pump and expel fluids to the ocean floor. Hydrothermal circulation influences the chemical composition of the water and rocks of ocean worlds and may help life develop deep beneath the icy surface. In a new study, planetary researchers used computer simulations of hydrothermal circulation based on well-understood systems on Earth to measure the effects of low gravity at values appropriate for ocean worlds smaller than our home planet. Simulations of ocean worlds with (lower) gravity result in fluid circulation that is roughly similar to that which occurs above and below the ocean floor on Earth, but with some key differences. Low gravity reduces buoyancy, so fluids do not become lighter as they heat up, which reduces their flow rate. This increases the temperature of the circulating fluids, which could lead to more extensive chemical reactions, possibly including those necessary to support life.

This diagram shows how Cassini scientists think rocks and water at the bottom of Enceladus’ ocean interact to produce hydrogen gas. Image courtesy of NASA/JPL-Caltech/Southwest Research Institute.

Rock-heat-fluid systems were discovered on the Earth’s ocean floor in the 1970s, where scientists observed releases of fluids carrying heat, particles, and chemicals.

Many of the vents were surrounded by a novel ecosystem, including specialized bacterial mats, red and white tube worms and heat-sensing shrimp.

For the new study, Professor Andrew Fisher from the University of California, Santa Cruz, and his colleagues used a complex computer model based on the hydrothermal cycle that occurs on Earth.

After varying variables such as gravity, heat, rock properties and depth of fluid circulation, the researchers found that hydrothermal vents could persist under a wide range of conditions.

If these flows occurred on an ocean world like Jupiter’s moon Europa, they could increase the chances of life surviving there as well.

“This study suggests that extraterrestrial ocean worlds may have supported low-temperature (but not hot enough for life) hydrothermal systems on timescales similar to those it took for life to become established on Earth,” Prof Fischer said.

The ocean circulation system on which the researchers based their computer model was discovered on the 3.5-million-year-old seafloor of the northwest Pacific Ocean, east of the Juan de Fuca Ridge.

There, cold undersea water flows through an extinct volcano (seamount), travels about 30 miles (48.3 km) underground, and then flows out into the ocean through another seamount.

“As water flows, it picks up heat, it’s warmer than when it entered, and its chemistry changes dramatically,” says Kristin Dickerson, a doctoral student at the University of California, Santa Cruz.

“The flow from seamount to seamount is driven by buoyancy – as water warms it becomes less dense and as it cools it becomes more dense,” Prof Fischer added.

“The difference in density creates a difference in fluid pressure within the rock, and the system is sustained by the flow itself. So as long as there is enough heat supplied and the rock properties allow for sufficient fluid circulation, the system will keep running. We call this a hydrothermal siphon.”

“Hot vent systems are primarily driven by sub-sea volcanism, while the Earth’s ocean floor experiences large amounts of fluid flowing in and out at much cooler conditions, driven primarily by Earth’s background cooling.”

“The flow of water through low-temperature vents is equivalent to all the rivers and streams on Earth in terms of the volume of water released, and accounts for about a quarter of the Earth’s heat loss.”

“About every 500,000 years, the entire volume of ocean water is pumped up and out of the ocean floor.”

Many previous studies of the hydrothermal circulation on Europa and Enceladus have considered hotter fluids.

“Cartoons and other illustrations often depict undersea systems that are similar to Earth’s black smokers, where cooler currents could occur just as much or even more than they do on Earth,” said Dr Donna Blackman from the University of California, Santa Cruz.

The results show that in very low gravity, such as on the ocean floor of Enceladus, the circulation can continue at low to moderate temperatures for millions or billions of years.

This could help explain why small ocean planets can have long-lived fluid circulation systems beneath their seafloors despite limited heating: the inefficiency of heat extraction could extend their lifetimes considerably, potentially for the entire lifetime of the solar system.

Scientists acknowledge that it is uncertain when active hydrothermal systems will be directly observed on the ocean planet’s seafloor.

The distance from Earth and physical characteristics pose significant technical challenges for spacecraft missions.

“It is therefore essential to make the most of the available data, much of which is remotely collected, and to leverage the understanding gained from decades of detailed study of the analog Earth system,” the authors concluded.

their paper Published in Journal of Geophysical Research: Planets.

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A.T. Fisher others2024. Gravitational maintenance of hydrothermal circulation in relation to the ocean world. Journal of Geophysical Research: Planets 129(6):e2023JE008202; doi:10.1029/2023JE008202

Source: www.sci.news

Extreme weather ushers in the start of summer, from scorching temperatures to devastating floods

summary

  • In the last week alone, extreme weather has wreaked havoc in many parts of the United States and around the world.
  • Climate change is increasing the likelihood of extreme temperatures and heavy rainfall such as those seen recently.
  • This year has been the warmest on record so far, with ocean temperatures breaking new records for more than 15 months.

Summer is quickly becoming a brutal season: Last week alone, record-breaking June heat forced schools to close across the Northeast and slowed some trains, flooding caused bridges to collapse in the Midwest and inundated towns across three states, and tropical storm-force winds prompted disaster declarations for 51 Texas counties.

The threat of climate change lurks behind many recent events.

“Last year, of course, was the warmest year on record by a pretty large margin, and this year, so far, has been the warmest on record for this time of June,” Daniel Swain, a climate scientist at the University of California, Los Angeles and the National Center for Atmospheric Research, said at a briefing on Monday.

While it will take time for climate scientists to understand and calculate the impact of global warming on individual weather events, the science is clear that as the planet warms, the likelihood of extreme temperatures increases, and the risk of heavy rains increases because a warmer atmosphere can hold and release more moisture.

As a result, the effects of climate change will be more noticeable in the summer, Swain said.

“It’s not surprising that we’re seeing another wave of record-breaking heat and record-breaking rainfall. It’s exhausting, but I think it’s really important that we don’t forget or let it slip away,” he said. “And this heat is especially pronounced in the summer, because, of course, the Northern Hemisphere summer is when most people on the planet experience the hottest weather.”

Extremely heavy rainfall over the weekend flooded communities in at least 80 counties in Iowa, South Dakota and Minnesota, temporarily isolating the town of Spencer, Iowa, of 11,000 people from the rest of the state. About 2,000 structures, including hundreds of homes, were damaged in Iowa alone.

Source: www.nbcnews.com

What If the Earth Was the Center of the Solar System?

Dead Planets Society is a podcast that takes some crazy ideas for how to tinker with the universe and tests their effects against the laws of physics, from snapping the moon in half to causing doomsday events with gravitational waves. apple, Spotify Or check out our podcast page.

By the end of the 16th century, pretty much everyone knew that the Earth revolved around the Sun, not the other way around. This was a huge blow to those who thought the Earth was the center of the universe, but the Dead Planets Society is here to ease their disappointment. Yes, we're trying to revive geocentrism.

Putting Earth at the center of the solar system requires more than just fudging the math: The Sun is much more massive than our puny planet, so forcing it to orbit the Sun would be nearly impossible, so hosts Chelsea White and Leah Crane would have to make some major changes to the solar system as we know it.

In this episode, Andy Rivkin Researchers at Johns Hopkins University in Maryland say the only way to make Earth an Earth-centered solar system would be to make it the most massive thing around – which would have some strange effects, assuming it doesn't collapse the planet into a black hole.

First, the Moon would have to speed up to maintain its orbit, orbiting the Earth in an hour or so before it would break apart. If the remaining planets didn't speed up too, they would all crash into the new giant Earth within a decade or two. The Earth's extra mass could also disrupt other nearby stars, causing them to start attracting it to Earth. A victorious Earth-centered solar system might not last long, but it would certainly come to a dramatic end.

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Source: www.newscientist.com

Could space and time be an illusion of entanglement? Clues may be found in black holes

We tend to think of space-time as the underlying structure of the universe, but whether it’s truly fundamental, or whether it arises from something much deeper, is a question that keeps physicists up at night. “It’s not a philosophical question to debate over a beer,” physicists say. Marika Taylor “This is something that actually gets built into the calculations that people make,” say researchers from the University of Birmingham in the UK.

A great place to start is quantum mechanics, which describes the behavior of elementary particles. One of the core tenets of this notoriously counterintuitive theory is that connections between particles can transcend our usual concepts of space and time. This happens through a phenomenon called quantum entanglement, in which particles can affect each other’s properties even when they’re half a universe apart.

Cosmologists now generally accept that quantum entanglement is intimately connected to the emergence of space. If we know the degree of quantum entanglement between two quantum particles, we can derive the distance between them. When we do this for a network of many particles, a geometry begins to form from which we can call space emerge. In other words, space may emerge from quantum entanglement.

Entanglement and space-time

Furthermore, advances in string theory, a candidate theory of everything, suggest that what happens in the universe can be explained entirely by data held at the exterior, or boundary, of that space — a phenomenon known as holographic duality. Combine this with quantum entanglement and you can build a universe that boasts a spatial fabric of distance and geometry.

Spiridon Michalakismathematical…

Source: www.newscientist.com

The Ideal Location of Our Milky Way Galaxy for Discovering Extraterrestrial Life

CrackerClips Stock Media/Alamy

All life as we know it in the entire universe is tucked away on a tiny rock floating in a tiny branch of the Milky Way galaxy. There are billions of other planets that could potentially support life, but how does our location affect our chances of finding it?

So far, the search for life elsewhere has only scratched the surface. “The bubble of space we've been able to explore around the Sun is tiny compared to the size of our galaxy,” he said. Jesse Christiansen“But we've already discovered more than 5,000 planets, called exoplanets, that orbit other stars,” says John F. Kennedy, an astrophysicist at the California Institute of Technology. Some of these have been found throughout our galaxy and even in other galaxies, but most are within a few hundred light years of the sun, a stone's throw in the scheme of the universe.

Our Galactic Neighborhood

Astronomers are beginning to look at different types of stars in the galactic outskirts and how they affect the habitability of planets around them. We live in an arm of the Milky Way galaxy called Orion, inside the main plane of the galaxy called the thin disk. We are surrounded by stars in the Orion arm. Further outwards, we are surrounded by the dense bulge of the galaxy's dense core on one side, and the sparser outer parts of the other arms of the galaxy on the other side.

Thin, disk-shaped stars, like our Sun and other stars in the constellation Orion, generally…

Source: www.newscientist.com

Robotic grin crafted from living human skin cells

This robot's face can laugh

Takeuchi et al. (CC-BY-ND)

Researchers say smiles made from living human skin could one day be attached to humanoid robots, allowing the machines to emote and communicate in a more lifelike way – and the wrinkles could even be useful for the cosmetics industry.

The living tissue is a mixture of human skin cells grown on a collagen scaffold, then placed on a 3D-printed resin base. Unlike previous similar experiments, this skin also contains the equivalent of ligaments, which are embedded in the layers of tissue beneath the skin of humans and other animals and hold the skin in place, giving it incredible strength and flexibility.

Michio Kawai The Harvard researchers call their ligament equivalents “perforated anchors” because they were made by drilling holes in the robot's plastic base and filling the tiny V-shaped cavities with tissue, which helps the robot's skin stay in place.

The team attached the skin to a smiling robotic face a few centimeters wide, which could be moved by rods attached to a base, and to a similarly sized 3D shape in the shape of a human head (see below), which could not be moved.

“As the roles required of robots expand due to developments in AI technology and other factors, the functions required of robot skin are also starting to change,” Kawai said, adding that having human-like skin could make communication between robots and humans smoother.

3D head shape covered with living skin

Takeuchi et al. (CC-BY-ND)

The research could also have unexpected benefits for the cosmetics industry: In tests, the researchers made the tiny robot's face laugh for a month and found that they could replicate the formation of expression wrinkles on the skin, Kawai says.

“If we can reproduce wrinkle formation on a palm-sized research chip, it could also be used to test new cosmetics and skincare products aimed at preventing, delaying or improving wrinkle formation,” said Kawai, who conducted the research while at the University of Tokyo.

Of course, this skin still lacks some of the functionality and durability of real skin, Kawai says.

“They have no sensing capabilities and no blood vessels to provide them with nutrients and water, so they cannot survive long in air,” he says. “To address these issues, our current challenge is to incorporate neural mechanisms and perfusion pathways into the skin tissue.”

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Source: www.newscientist.com

The universe’s size and shape as revealed by space-time

NASA, ESA, CSA, STScI

In a sense, we are at the center of the universe. But that’s because we see the same distance in every direction, and the observable universe is perfectly spherical. Due to the limitations of the speed of light and the inexorable expansion of the universe, we can see about 46 billion light years away in every direction. What is beyond this horizon? That is a mystery that will never be solved.

But there are clues. The overall size of the universe is governed by two competing effects: gravity and dark energy. All matter has mass, which causes gravity, pulling everything to everything else. But to their surprise, early 20th-century cosmologists discovered that distant galaxies appear to be moving away from us at incredible speeds. The mysterious force that causes this strange expansion of space is called dark energy, and its nature remains a mystery to this day.

“Before we discovered dark energy and accelerating expansion, the universe was much simpler,” the cosmologist says. Wendy Friedman Researchers at the University of Chicago say that without dark energy, the universe would be much smaller, making its size easier to predict.

Even with dark energy, the universe may only be slightly larger than we can see. Jean-Luc LehnersHe then worked at the Max Planck Institute for Gravitational Physics in Germany. Jerome Quintin University of Waterloo, Canada The model was published It suggests that the period of rapid expansion just after the Big Bang, the so-called inflation, may have been even shorter than we thought, making the universe smaller…

Source: www.newscientist.com

The Chang’e-6 probe from China successfully returns with the first samples of rocks from the far side of the moon

The Chang’e-6 probe is recovered in Xiziwang Banner, Inner Mongolia, China.

Xinhua/Shutterstock

China’s Chang’e-6 spacecraft has returned to Earth, bringing back the first chunk of space rock from the far side of the moon.

The capsule separated from the orbital container at around 1:20 p.m. local time, 5,000 kilometers above the Atlantic Ocean, and landed in Xiziwang Banner, Inner Mongolia Autonomous Region, China on June 25.

The sample, which should contain about 2 kilograms of lunar material, descended the final 10 kilometres by parachute, landing at 2:07pm and being retrieved by scientists from the China National Space Administration.

Landing on the far side of the moon is difficult because it always faces away from Earth and there is no direct communication line, and this area’s surface remained unexplored until a Chinese spacecraft landed there earlier this month.

The landing and recovery operations relied heavily on autonomous processes and robotic tools, but Chinese engineers were able to send messages to the spacecraft through the Queqiao-2 relay satellite, which was launched in March this year and is still orbiting the moon.

The samples include surface and two meters of material scooped up by Chang’e-6 drilling into its landing site in Apollo Crater, which is within the larger South Pole-Aitken Basin. Scientists hope that this material will help explain how and when these basins formed, and may enable understanding of the origins of other similar lunar craters.

The rocks may indicate the amount of water ice in the region, which could be a key resource for a manned mission that China hopes to send to the moon by 2030.

Before embarking on its crewed mission, China plans to send two more spacecraft, Chang’e-7 and Chang’e-8, to the lunar south pole to gather information on a potential site for a base to be called the International Lunar Research Station. China is leading the mission in collaboration with Russian space agency Roscosmos.

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Source: www.newscientist.com

We are closer than ever to proving the existence of the multiverse.

Shutterstock/Dr. Norbert Lange

We think of this universe as containing everything that exists, has existed in the past, and will exist in the future, but that may not be the case – there are many ways in which other universes exist.

One is that we may be part of a branch of an infinite number of universes collectively known as the multiverse. These universes could have emerged shortly after the Big Bang, could be hiding in extra dimensions, or could suddenly appear whenever quantum properties shift from different states into a single reality.

The idea of a multiverse rose to scientific prominence in the 1980s with the invention of inflation, a period when the early universe suddenly expanded. Inflation explains why the universe is so flat and smooth, but it also predicts the creation of many independent bubble universes.

Cyclic Universe

But inflation is only one path to a multiverse, and critics say it has some merit. In recent years, many cosmologists have turned to alternative theories, such as cyclical universe theory, which claims that the universe is expanding and compressing endlessly. These theories still claim multiple universes, but at different times.

“What I don’t like about inflation is that there is very little true prediction. You never get back more than you put in.” Neil Tulloch Physicist at the University of Edinburgh in the UK. Model of a cyclical universe In my 2001 book Inflation Rivals, I argued that there must be a better explanation for inflation.

In a cyclical universe…

Source: www.newscientist.com

Is the universe structured like a giant brain and conscious?

An astrophysicist and a surgeon walk into a bar. No, this is not the start of a bad joke. A few years ago, an astrophysicist Franco Vazza I met my childhood friend Alberto FerrettiAnd then he became a neurosurgeon. Vazza was modeling the structure of the universe, while Ferretti was delving into the brain. The two men reminisced and talked about their work. And then an idea occurred to them: What if they compared?

Vazza, based at the University of Bologna in Italy, has done just that. He used statistical techniques to compare neurons in a region of the brain called the cortex to the cosmic web, the pattern of matter distribution throughout the universe. Vazza looked at the number of nodes in each network and how densely connected each node is. The results surprised him.“It's a really interesting level of similarity,” he says. Ignoring the difference in the structures' sizes, which are about 27 orders of magnitude, “the two patterns kind of overlap,” Vazza says.

Some physicists cannot ignore this similarity, suggesting that the universe may “think” – that is, be conscious in some sense – an idea that has roots in the philosophy of panpsychism.

Traditionally, researchers have explained consciousness in one of two ways. Materialists argue that there is only matter, and consciousness somehow arises from that. Dualists argue that there are fundamentally two kinds of matter: matter and consciousness. There has been much discussion about the shortcomings of both views. For example, how can consciousness arise from pure matter?

Panpsychism

For some,…

Source: www.newscientist.com

Hot water leaking beneath Antarctic ice sheet may quicken melting

Aerial photo of the Antarctic ice sheet

David Vaughn/BAS

Antarctica’s melting ice sheet could retreat faster as warmer ocean water invades underneath it, and rising ocean temperatures could trigger a “runaway” feedback effect that pushes warm water further inland, melting even more ice and accelerating sea-level rise.

As the climate warms, the future of Antarctica’s vast ice sheet remains uncertain, and predictions vary widely about how quickly it will melt and therefore how much it will contribute to sea-level rise. One dynamic that researchers have only recently begun to recognize as a key factor is the intrusion of warmer ocean water beneath the ice.

“The mechanisms of invasion are much more powerful than we previously understood.” Alexander Bradley At the British Antarctic Survey.

Such intrusions are driven by density differences between the freshwater flowing out from beneath the ice sheet and the warmer waters where the ice meets the sea floor, known as the grounding line. They are difficult to observe directly because they occur hundreds of meters beneath the ice, but simulations suggest that in some places the warm waters could extend several kilometers inland.

One model by Alexander Lovell Researchers from the Georgia Institute of Technology in Atlanta found that widespread ice-sheet intrusion could add heat from below, lubricating ice flow along bedrock and more than doubling ice loss from the ice sheet.

Bradley and his colleagues Ian Hewitt Using their model, Oxford researchers explained how the shape of cavities in the ice changes as the ice melts, altering how ocean water flows in.

The researchers found that once ocean water reaches a certain temperature threshold, ice from the ice sheet melts faster than it can be replaced by outflowing ice. If this cavity grows larger, more water could flow under the ice sheet and penetrate further inland, creating a so-called “runaway” positive feedback effect.

“Small changes in ocean temperature lead to dramatic changes in how far warm water can intrude,” Bradley said. The ocean warming needed to cause this effect is within the range expected this century, he said, but models cannot yet predict it for specific ice sheets, and not all ice sheets are equally susceptible to such intrusions.

“This positive feedback could lead to much more intrusion than we thought,” Lovell says. “Whether that’s a tipping point that leads to unrestrained intrusion of ocean water beneath the ice sheet is probably a stretch.”

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Source: www.newscientist.com

Why cats annoyingly always choose to disrupt your laptop usage

Do you own a precious and adorable cat? If so, your feline friend may be obstructing your view of this page and causing havoc once again, particularly if you are browsing on a laptop.

But why do cats have this tendency? What drives them to interfere with our computers?

Unfortunately, there have not been any extensive scientific studies to explore this question yet. However, cat behavior experts have a relevant theory that could shed light on why cats love to sit on keyboards.



Why does my cat sit on my laptop?

It’s unlikely that your cat wants to mimic your typing or join in with your computer activities. Recent research suggests that cats are capable of imitating human actions, such as touching objects with specific body parts. However, typing is a behavior that cats struggle to replicate, as explained by Dr. David Sands, an Animal Psychology Expert with over 25 years of experience.

While laptops do emit heat which may attract cats, the main draw for felines is the smell of their owners on the keyboard. Cats have a strong sense of smell and enjoy leaving their scent on objects to show ownership. This behavior is more about claiming territory and marking their humans rather than seeking warmth or copying human actions.

“My Laptop, My Person” © Getty

In summary, it’s not harmful for your cat to sit on your laptop physically, but if the behavior becomes excessive or is accompanied by other signs of anxiety or attention-seeking, it may be worth monitoring.

About our Expert, Dr. David Sands

Dr. David Sands holds a PhD in Ethology (Animal Psychology) and boasts more than 25 years of experience in animal behavior clinics. He is affiliated with the Canine and Cat Behavioural Association (CFBA) and the Association for the Study of Animal Behaviour (ASAB) and has authored several books, including 500 Questions About Cats Answered.

Source: www.sciencefocus.com

Dark energy could be even more mysterious than previously believed

The choice to name a new project the Dark Energy Spectroscopic Instrument (DESI) may come across as presumptuous. Dark energy, you see, is completely unseen; it does not emit any detectable light for a spectrometer to analyze. In fact, dark energy has never been directly observed and has managed to evade capture despite efforts made using the most advanced telescopes and detectors available.

As far as we understand it, dark energy is invisible, uniformly spread throughout space, does not interact with matter or light, and serves the sole purpose of accelerating the universe’s expansion through a mechanism that remains a mystery to us.

So, with the recent announcement of DESI’s initial data release, are we witnessing a shift in our comprehension of dark energy, as promised?

In the search for elusive dark energy, our observations offer limited insights: dark energy merely stretches space-time. To investigate different theories about dark energy, we must examine how this stretching occurred over cosmic time.

One method is to observe the universe’s expansion history, while another involves examining how matter accumulated within galaxies and clusters at various junctures in the universe’s past.

Efforts to measure the expansion rate often involve constructing a precise 3D map of the universe’s matter. By studying the spectra of light, we can determine how much it has stretched due to the universe’s expansion. By combining this information with accurate physical distances, we gain valuable insights into the universe’s evolution.

DESI’s new model has stirred speculation by proposing that dark energy may have a more intricate history than previously believed. If these indications prove to be accurate, they could revolutionize our understanding of not just the universe’s past, but also its eventual fate.

The Concordance Model of Cosmology outlines the prevailing model of the universe and its components. In this model, dark energy is viewed as a cosmological constant, providing a minimal flexibility to every part of space.

DESI and other surveys commonly report their dark energy findings in terms of an “equation of state” parameter denoted as w. A value of w = -1 is expected if dark energy behaves as a cosmological constant. Any deviation from this value implies a different characteristic for dark energy.

The recent DESI findings present a puzzling scenario: while a constant w of -1 aligns well with the results, a scenario where w is variable suggests a different interpretation. When combined with data from other sources, these results hint at a changing w, implying a varying impact of dark energy on the universe over time.

While the implications of these findings remain uncertain, they raise intriguing possibilities about the future course of the universe and the role of dark energy within it. Though still preliminary, these results suggest that dark energy may continue to surprise us in unforeseen ways in the future.

Source: www.sciencefocus.com

Potential Lunar Conflict: The Moon World War looms on the horizon

The Moon, Earth’s steadfast companion that remains in orbit, has been a popular subject of discussion since the early days of space exploration. Missions have been planned, rovers have explored its surface, and even a flag has been planted there.

But why all the interest? The Moon is over 400,000 km away from Earth, a considerable distance to travel, and it poses many challenges as a potential habitat for humans, such as exposure to solar radiation.

However, the Moon offers other advantages. Being largely untouched, it presents opportunities for planetary research, scientific experiments, and notably, mining for valuable resources.

There is a growing interest in lunar exploration, raising the important question of lunar ownership. Philosopher and author AC Grayling addresses this topic in his new book, “Who owns the moon?”

SF: Why are we interested in going to the moon, and will it ever happen?

ACG: The Moon holds vast resources, making it a lucrative target for mining operations. Coupled with the rapid pace of technological advancements, the obstacles to lunar exploration are likely to be overcome. Significant investments are being made in this endeavor, indicating the potential benefits that could be derived.


While some argue that lunar exploration is not feasible, the lure of valuable resources like Helium-3 for clean nuclear fusion makes the Moon an attractive destination for mining activities.

SF: So who actually owns the moon?

The 1967 Outer Space Treaty, agreed upon by the United Nations, asserts that the Moon cannot be militarized or claimed for sovereignty or ownership. It is considered a shared resource belonging to all of humanity.

With various nations eyeing lunar exploration and exploitation, concerns about potential conflicts arise, highlighting the need for clearer regulations and agreements.

What are the next steps? Will the law be strengthened?

Efforts are being made to establish binding regulations, but the presence of multiple space agencies and rivalries between nations complicate the process. Initiatives like the Artemis Accords aim to set guidelines for responsible behavior in space.

However, the prospect of a new space race between major powers like the US, China, and Russia raises concerns about the potential for conflict and competition in space.

Can history give us any indication of what might happen?

The Antarctic Treaty serves as a model for international cooperation in preserving shared resources. However, challenges to extend the treaty’s scope and conflicting claims in Antarctica hint at the complexities of managing common territories.

Similar issues could arise in lunar exploration, especially with the potential for valuable mineral resources like Helium-3. The absence of clear regulations and the lack of a universal agreement on space governance present significant hurdles.

Is there an argument to leave the moon alone?

Given the Moon’s vast and barren nature, concerns about environmental impacts are minimal compared to Earth. Utilizing lunar resources for space exploration and sustainable practices could be more beneficial in the long run.

What’s the next step after the moon?

The Moon’s potential as a refueling station for Mars missions opens up new possibilities for further space exploration. As colonies on celestial bodies evolve, questions of independence and governance will arise, shaping the future of human presence in space.

In conclusion, the direction of space activities will determine whether they align with values upheld on Earth or devolve into profit-driven ventures. Clear regulations and international cooperation are essential to ensure a sustainable and equitable future in space.


About our expert, A.C. Grayling

AC Grayling is a philosopher and author of the book “Whose Moon is It?” He is also the founder of the New College of the Humanities and a respected figure in literary criticism and intellectual discourse.

Source: www.sciencefocus.com

Ancient Shipwreck Discovered in Mediterranean Sea with Canaanite Amphorae from 3,300 Years Ago

The ancient ship and its cargo are estimated to date to the 13th century BC, making it one of the oldest shipwrecks ever discovered.



Canaanite amphorae discovered in a 3,300-year-old shipwreck. Image courtesy of the Israel Antiquities Authority.

The 3,300-year-old shipwreck was discovered 90 kilometers (56 miles) off the coast of Israel, on the bottom of the Mediterranean Sea at a depth of 1.8 kilometers (1.1 miles).

“The ship appears to have sunk due to a storm or an attempted pirate attack,” said Dr Jacob Sharvit, head of the Israel Antiquities Authority’s maritime department.

“This is the first ship ever found in the deep waters of the eastern Mediterranean, 90 kilometres from the nearest coast, and also the oldest.”

“This is a history-changing discovery of global scale. It sheds light like never before on the navigational skills of ancient sailors who were able to cross the Mediterranean without ever seeing the coast. From this geographical point, all you can see is the horizon.”

“It seems likely that celestial objects were used to navigate by observing the positions and angles of the sun and stars.”

The discovery was made by a team from Energene, a London-based natural gas producer, during an environmental survey of the seabed.

“As part of our ongoing efforts to discover and extract natural gas from the deep sea, we are carrying out surveys to check various parameters using advanced submersible robots to explore the seabed,” said Dr Karnit Bahartan, head of Energean’s environmental staff.

“About a year ago, while surveying, we came across an unusual sight: a large pile of water jugs on the seabed.”

“We have been in constant contact with the Israel Antiquities Authority and when we sent them the images, it turned out to be a sensational find, far beyond our imagination.”



A 3,300-year-old shipwreck on the bottom of the Mediterranean Sea. Image courtesy of the Israel Antiquities Authority.

“Robotic investigation and mapping of the site revealed that the ship was a wreck approximately 12-14 metres (39-46 feet) long and was carrying hundreds of passengers. Late Bronze Age Canaanite storage vesselsOnly a small fraction of it is visible above the ocean floor,” Dr Sharbit said.

“There appears to be a second level of ship hidden in the muddy bottom, with the wooden beams of the ship also buried in the mud.”

“The type of vessel identified in the shipment was designed as the most efficient means of transporting relatively cheap, mass-produced products, such as oil, wine, and agricultural products such as fruit.”

“The discovery of such a large number of amphorae on a single ship attests to important commercial links between their country of origin and the ancient Near Eastern countries along the Mediterranean coast.”

“This is a truly stunning discovery. There are only two other known cargo-laden shipwrecks from the Late Bronze Age in the Mediterranean – the Cape Gelidnja ship and the Uluburun ship, both found off the coast of Turkey.”

“But both wrecks were found relatively close to shore and were accessible using standard diving equipment.”

“Based on these two discoveries, the previous academic hypothesis was that trade at that time was carried out by flying safely from port to port, keeping eye contact along the coastline.”

“The discovery of this ship completely changes our understanding of the capabilities of ancient seafarers. It is the first time that a ship has been found so far away that land is completely out of sight.”

“There is great potential for research here. Because the ship has been preserved at great depth, time has stopped since the moment of the disaster. The hull and the surrounding conditions have not been disturbed by human hands (divers, fishermen, etc.), nor have they been subject to the waves and currents that affect shipwrecks in shallow waters.”

“The significance of these discoveries has led to the decision to open the archaeological campus for ‘tasting’ tours this summer, to display these Canaanite ships excavated from the seabed and to tell the public their story,” said Dr. Eli Eskseed, Director General of the Israel Antiquities Authority.

“This visit will allow visitors to get a glimpse of this unique building, its mosaics and laboratories ahead of the official opening of the vast visitor centre, scheduled for two years from today.”

“We are extremely grateful to Energiaan for their swift response in identifying this ancient cargo and for committing resources to enable this initial understanding to be gained from this unusual shipwreck.”

Source: www.sci.news

New study sheds light on amino acid metabolism and transport in tea plants

High concentrations of free amino acids in tea leaves are important for tea’s flavor and health functions, but their biosynthesis, transport and turnover in the tea plant have remained unknown.

A practical model of nitrogen assimilation, amino acid synthesis, transport, and decomposition/recycling in tea plants. Image courtesy of Yu others., doi: 10.1093/hr/uhae060.

“Amino acids are essential for plant growth and have a significant impact on the flavor and health benefits of tea,” Professor Zhao Jian Hunan Agricultural University and colleagues.

“Especially the tea trees Camellia sinensis exhibits a unique amino acid profile that contributes to its distinctive taste and nutritional value.”

“Although the importance of amino acids such as theanine and glutamine (Gln) is known, the detailed dynamics of their synthesis, transport and degradation in tea plants remain unknown.”

“These challenges require intensive research to be carried out to understand the complex metabolic pathways and spatial distribution of amino acids within the tea plant.”

In the study, Professor Zhao and his co-authors analyzed the spatial dynamics of amino acid biosynthesis, transport and turnover in tea plants.

“This study provides a detailed analysis of the metabolic pathways and gene expression that control these processes,” the researchers said.

“By understanding these mechanisms, we hope to improve tea cultivation and enhance the quality of tea beverages.”

“This study revealed that nitrogen assimilation occurs mainly in the roots, where glutamate, theanine and arginine (Arg) are actively synthesized. These amino acids are then transported through the plant’s vascular system.”

“Transcriptome analysis revealed that genes involved in Arg synthesis are highly expressed in roots, whereas genes involved in Arg transport and degradation are expressed in stems and young leaves. This indicates that there is a sophisticated amino acid management system within the plant.”

“One of the key findings is the role of the CsGSIa gene, which is crucial for the synthesis, transport and recycling of amino acids.”

“Overexpression and knockdown experiments of CsGSIa in transgenic tea plants demonstrated significant effects on the levels of Gln and theanine.”

“The study also revealed that Arg, Gln, glutamic acid (Glu), and theanine are the major amino acids transported through xylem sap, facilitating long-distance nitrogen transport from roots to leaves.”

“Our findings provide a detailed map of amino acid metabolism in the tea plant, which is of vital importance for both basic science and applied agricultural practice,” Dr Zhao said.

“Understanding these metabolic pathways opens up new possibilities for breeding tea varieties with enhanced flavor and health benefits.”

The team’s findings have important implications for the tea industry.

“By elucidating the pathway of amino acid metabolism, our study paves the way for the development of tea plants with higher contents of beneficial amino acids, enhancing both flavour and nutritional value,” the researchers said.

“These insights can be applied to breeding programs and cultivation practices to produce superior tea varieties.”

“Furthermore, understanding these metabolic processes can help us develop strategies to improve nitrogen use efficiency, contributing to more sustainable and productive tea farms.”

of study Published in the journal Horticultural Research.

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Shuwei Yu others2024. Analysis of spatial dynamics of biosynthesis, transport and metabolism of major amino acids in tea plants (Camellia sinensis). Horticultural Research 11(5):uhae060; doi:10.1093/hr/uhae060

Source: www.sci.news

A recently found bird species in Brazil

According to a multi-trait systematic study led by the Federal University of Pará, ornithologists Silver-cheeked anteater (Sacesphoroides cristatus) It actually represents not one but two species.

An illustration Sacesphoroides niedegidonaeImage courtesy of Eduardo Brettas.

A newly discovered species, the northern stingray (Sacesphoroides niedegidonae)teeth, CaatingaA natural area located in the interior of northeastern Brazil.

“Caatinga is the largest seasonally dry tropical forest in the Neotropics, located in northeastern Brazil, and is characterized by a predominantly deciduous forest and extreme seasonality of rainfall,” Dr. Pablo Cerqueira Emilio Goeldi from the Paraense Museum of the Federal University of Pará and his colleagues.

“Historically, this area has been treated as a biologically impoverished region, but recent studies have uncovered new diversification patterns and several new species of frogs, mammals, insects and fish.”

“The region's topography has played an important role in its biogeographical history, with altitudes ranging from sea level in the north to an average of 400-700 metres in the central states of Bahia and Minas Gerais, to over 1,000 metres on the slopes of the Sierra de Espinhaço mountain range.”

Sacesphoroides niedegidonae It is the second known species in the genus. SacesphoroidesThis also includes Sacesphoroides cristatus.

“Until recently, Sacesphoroides cristatus Classified into the genus SacesphorusHowever, new genetic and morphological data have revealed that the genus is non-monophyletic, prompting its transfer to a separate genus. Sacesphoroides” the researchers said.

In this study, a total of 1,079 Sacesphoroides cristatus Sample size (818 males, 261 females).

To investigate song variation, the researchers analyzed a total of 115 different audio recordings.

They also sequenced 58 tissue samples from across the country. Sacesphoroides cristatus The range is wide, with 39 of them belonging to the left bank of the San Francisco River and 19 on the right bank.

Of the 1,079 individuals analysed (skins and photographs), no diagnostic plumage differences could be identified among males, but two main plumage patterns were diagnosed in females, mainly across the river.

“Men Sacesphoroides niedegidonae The feathers are similar Sacesphoroides cristatus“The males are males, but the females have different colouring on the top of their heads, backs and tails than the males,” the scientists said.

Sacesphoroides niedegidonae It is generally lighter in color (amber) rather than chestnut brown. Sacesphoroides cristatus. “

The back is olive brown Sacesphoroides niedegidonae,on the other hand, Sacesphoroides cristatus It's cinnamon brown.”

“The overall color of the tail is Sacesphoroides niedegidonae Darker than Sacesphoroides cristatusThe most noticeable difference is the black and white stripes. Sacesphoroides cristatus It has a modest dull brown and reddish stripes, and no white stripes at all.”

“Sing out loud Sacesphoroides niedegidonae The general pattern is: Sacesphoroides cristatus“However, the shape of the first note is noticeably different,” they added.

“The new species is almost exclusively restricted to the left/north bank of the São Francisco River, with one population occurring on the right bank in the “Raço da Catarina” region of Bahia.”

“This population, discovered on the right/south bank of the San Francisco River, may have 'migrated' across the river due to changes in paleotopography, as detailed in the Discussion section below.”

Sacesphoroides niedegidonae It is a common species throughout most of its range and occurs in a variety of habitats in the Caatinga, including secondary growth vegetation.

“The range of the outbreak is estimated to be 630,000 km.2not approaching the threshold Vulnerable Status according to IUCN range criteria (<20,000 km2)2),” the authors state.

“Although population data is not available, the mature population is estimated at more than 10,000 individuals, and the species Least Concern. “

“But a new approach using niche modelling for future climate scenarios shows Sacesphoroides cristatus (include Sacesphoroides niedegidonae(same as treated prior to this study).

“When we apply the IUCN criteria to these estimated future range sizes, the threatened category is Near Threatened And more Vulnerable It depends on future global change scenarios.”

Discovery Sacesphoroides niedegidonae It has been reported paper In the journal Zoological scriptor.

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Pablo Cerqueira othersA new ant shrike (Aves: Shrikeidae) endemic to Caatinga and the role of climate variability and drainage change in shaping the potential diversity of a Neotropical seasonally dry forest. Zoological scriptorpublished online June 17, 2024. Source: 10.1111/zsc.12672

Source: www.sci.news

Millions at risk from ultrafine air pollution caused by airplanes

Jet engines emit large amounts of ultrafine particles

Aerovista Luchtfotografie/Shutterstock

The health of more than 50 million people living within 20 kilometres of Europe's busiest airport is being harmed by high levels of ultrafine particle pollution from jet engines, according to a report. the study It was commissioned by campaign group Transport & Environment (T&E).

Several Other studies It says ultrafine particles can increase the risk of respiratory diseases, cardiovascular diseases, neurological diseases, diabetes and pregnancy problems. Darn Fun Setters His team, working at the Dutch consultancy CE Delft, are using these studies to try to estimate the impact for Europe as a whole.

But ultrafine particle pollution is a less-studied aspect of air pollution and there is a lot of uncertainty: “There is little research in this area and the evidence is often inconclusive,” Van Seters said.

Most research on particulate air pollution has focused on particles smaller than 2.5 micrometers in diameter, so-called PM2.5. Ultrafine particles are particles smaller than 0.1 micrometers in diameter.

“They are very dangerous because they are so small and can get very deep into the human body.” Carlos Lopez de la Osa At T&E.

Jet engines emit more ultrafine particles than other types of engines, so people who live or work near airports are most likely to be exposed to this form of air pollution, but there are no effective limits on its levels.

Ultrafine particles are a type of PM2.5, but PM2.5 limits are set for the total mass of particles per cubic metre of air. Ultrafine particles are so small that even a huge number of particles per cubic metre would not exceed the PM2.5 limit.

In fact, there's very little monitoring of ultrafine particle levels, says Lopez de la Osa. “What we have are mostly regional studies around individual airports like Zurich, Amsterdam, Berlin, Los Angeles,” he says. “We don't have a comprehensive view, and that's one of the main reasons we decided to launch this study.”

To estimate the impact across Europe, van Seters and his colleagues first estimated ultrafine particle pollution levels around the continent's 32 busiest airports, based on figures from surveys of individual airports. The team assumed that ultrafine particle pollution increases linearly with the number of flights and did not take wind patterns into account.

Next, based on studies looking at health effects, the researchers estimated that ultrafine particle pollution near 32 airports was responsible for an additional 280,000 cases of hypertension, 330,000 cases of diabetes, and 18,000 cases of dementia over the years.

“This is a first-order estimate based on extrapolation, and we need to do epidemiological studies to get more precise estimates,” Van Seters said.

But he thinks that, if anything, is an underestimate because the study only looked at 32 airports and people living within 20 kilometres, and excluded people who work at the airports.

In terms of population at risk, Orly Airport near Paris tops the list, with more than six million people living within 20 kilometers of the airport, while London's Heathrow Airport comes in fourth, with more than three million people living within the airport's vicinity.

The research team's estimates of health effects rely heavily on a study carried out in 2022 at Schiphol Airport near Amsterdam. Nicole Jansen Contacted by CE Delft, Janssen and her colleagues at the National Institute for Public Health and the Environment in the Netherlands said they advised researchers not to try to quantify the impact in this way because of large uncertainties.

But they agree that more research is needed: “We would underscore our recommendation to further investigate the risk of ultrafine particles from aircraft around other international airports,” Janssen said.

There are ways to reduce ultrafine particle pollution levels, says Christina Toth of T&E. Jet fuel can be improved to reduce ultrafine particle emissions, for example by reducing its sulfur content. So-called “sustainable aviation fuels” (SAF) also reduce ultrafine particle pollution.

“Unfortunately, we know it will be a long time before SAF can be produced at scale and be effective,” Toth says.

Limiting airport expansion and flight frequencies and encouraging alternative modes of transport would help, and would also limit flying's impact on the climate.

topic:

Source: www.newscientist.com

Boeing spacecraft faces multiple delays in NASA astronauts’ return

The test flight of Starliner to the International Space Station is aimed at showcasing the spacecraft’s capability to safely transport astronauts to low Earth orbit and assess its various systems in space.

The launch of the capsule was delayed numerous times before finally taking off on June 5, several years behind schedule and significantly over budget.

According to NASA officials, the return date for the astronauts has not yet been determined, but they could potentially return after a spacewalk scheduled for July 2 from the International Space Station.

Officials mentioned that there is no urgency to depart as the space station has adequate supplies to accommodate the visitors. NASA will thoroughly investigate before approving the undocking of the capsule.

Wilmore and Williams are currently residing on the ISS alongside seven other crew members: NASA astronauts Michael Barratt, Matt Dominic, Tracy Dyson, and Janet Epps, as well as Russian cosmonauts Nikolai Chub, Alexander Grebenkhin, and Oleg Kononenko.

During their prolonged stay in space, Wilmore and Williams will assist in the operations of the space station and conduct various tests as part of the certification process for Starliner by NASA.

“Crew feedback has been extremely positive, and they recognize that all the insights gained during crew flight testing will enhance and refine the experience for future crew members,” stated Mark Nappi, vice president and program manager for Boeing’s Starliner program.

Ultimately, Boeing aims to provide scheduled flights to and from the space station for NASA, akin to the commercial services offered by SpaceX with its Crew Dragon spacecraft since 2020.

Source: www.nbcnews.com

Expedition to study human adaptation to extreme heat in the face of climate change

Walking on hot red sand is hard work, especially when the temperature exceeds 40°C (104°F). After about 40 minutes you are soaked, dehydrated and exhausted. It is hard to imagine doing this for 40 days with all your gear, including 40 liters of water for five days, on a two-wheeled trolley. But that is exactly what my traveling companions did.

I'm in the Nahud Desert, a vast expanse of sand and rocky wilderness in northern Saudi Arabia, to experience the almost unbearable heat and meet up with 20 other people who are part of an expedition. Deep ClimateHe is dedicated to understanding how humans respond to extreme situations. “The aim is to study how humans adapt to new kinds of environments,” he says. Christian Clotteleader of the expedition and director of the French Institute of Human Adaptation.

This problem becomes even more pressing as the climate gets warmer: even in the most optimistic scenarios, heatwaves exceeding 40°C, as observed in southern Europe and across the United States over the past few months, will become the norm in many parts of the world.

So the question of what happens to our brains and bodies, and how well the human physiology can handle extreme heat, is a question that matters to millions of people. “We're going to see large swaths of densely populated areas rise to unprecedented temperatures that nobody has seen in historical climates,” he said. Tim Renton He is a researcher at the University of Exeter in the UK and recently co-authored a research paper titled “…

Source: www.newscientist.com

How antibiotic resistance diminished the impact of the last pandemic

Shutterstock/Katerina Con

When Gene Marrazzo was announced as director of the National Institute of Allergy and Infectious Diseases (NIAID) last year, he became one of the world's leading public health policymakers, and the responsibilities are heavier than ever before for the institute's new director, who will succeed Anthony Fauci, who held the position during the coronavirus pandemic and became a household name.

After decades of working on HIV prevention and sexually transmitted diseases, as well as overseeing COVID-19 treatment interventions, Marrazzo is now responsible for NIAID's $6.6 billion annual budget and the future of infectious disease control in the United States.

This includes working with the institute's 21 laboratories across the country, leading the fight against Ebola and HIV, and spearheading the development of new vaccines, treatments, diagnostics and technologies.

Top of Marrazzo's to-do list is tackling antimicrobial resistance (AMR), or drug-resistant superbugs, which are predicted to cause 10 million deaths a year and cost the global economy $1 trillion annually by 2050. In May, Britain's former chief medical officer warned that the rise of these pathogens could make pandemics seem “small” and that the problem is more serious than climate change.

Global warming is one of the factors contributing to the increase in drug-resistant bacteria, and changes in the climate conditions on Earth Salmonella Causes cholera Biblio To survive, we'll need to avoid our current antibiotic arsenal altogether. Here, Marrazzo outlines what we should probably fear most, and some developments we can expect in the near future.

Charlotte Lytton: In what ways…

Source: www.newscientist.com

Webb finds early universe protoglobular cluster

Astronomers using the NASA/ESA/CSA James Webb Space Telescope have discovered at least five young globular clusters within SPT 0615-JD1 (also known as the Cosmic Gems Arc), a strongly lensed galaxy that existed when the universe was 460 million years old.



These images show the galaxy cluster SPT-CL J0615-5746 (right) and part of this cluster (left), showing two clearly lensed galaxies. The Cosmic Gems arc is shown along with several galaxy clusters. Images courtesy of NASA / ESA / CSA / Webb / L. Bradley, STScI / A. Adamo, Stockholm University / Cosmic Spring Collaboration.

“These galaxies are thought to be the main source of intense radiation that reionized the early universe,” said Dr Angela Adamo, astronomer at Stockholm University and the Oskar Klein Centre.

“What’s special about the Cosmic Gems Ark is that thanks to gravitational lensing, we can actually resolve galaxies down to the parsec scale.”

SPT 0615-JD1 was originally discovered in Hubble Space Telescope images obtained by the RELICS (Reionizing Lensing Cluster Survey) program of the lensing galaxy cluster SPT-CL J0615-5746, located about 7.7 billion light-years away in the constellation of Scorpio.

The Webb telescope will enable Dr Adamo and his colleagues to see where stars are forming and how they are distributed, in a similar way that the Hubble telescope is used to study the local galaxy.

Webb’s observations provide a unique opportunity to study star formation and the internal structure of young galaxies at unprecedented distances.

“The combination of the Webb Telescope’s incredible sensitivity and angular resolution at near-infrared wavelengths, along with gravitational lensing by a large foreground galaxy cluster, made this discovery possible that would not have been possible with any other telescope,” said Dr. Larry Bradley, an astronomer at the Space Telescope Science Institute.

“The surprise and excitement I felt when I first opened the Webb images was overwhelming,” Dr. Adamo said.

“We saw a string of tiny bright dots projected from one side to the other. These cosmic gems are star clusters.”

“Without Webb, we would never have known we were observing star clusters in such a young galaxy.”

Astronomers say the discovery connects different scientific disciplines.

“These results provide direct evidence of the formation of protoglobular clusters in faint galaxies during periods of reionization and help us understand how these galaxies successfully reionized the Universe,” Dr Adamo said.

“This discovery also places important constraints on the formation of globular clusters and their early properties.”

“For example, the high stellar densities found in galaxy clusters provide the first indications of processes occurring within them and give new insights into the possible formation of very massive stars and black hole seeds that are important for the evolution of galaxies.”

In the future, the team hopes to construct a sample of galaxies that can achieve a similar resolution.

“I am convinced that there are more such systems in the early universe waiting to be discovered, which will improve our understanding of early galaxies even further,” said Dr Eros Vanzella, astronomer at the Bologna Observatory for Astrophysics and Space Sciences (INAF).

of Investigation result Published in today’s journal Nature.

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A. Adamo othersA bound star cluster observed in a lensed galaxy 460 million years after the Big Bang. NaturePublished online June 24, 2024, doi: 10.1038/s41586-024-07703-7

Source: www.sci.news

Small urban gardens are a haven for insects, even in the presence of invasive plants

Amsterdam’s tiny street gardens provide habitat for insects

Marijke Thyssen/Shutterstock

A study of small urban gardens in the Netherlands found that they can be havens for insects and other wildlife. The two most effective factors were having a lot of plants and a wide variety of plants, whether or not the plants were native.

“Even in a really small garden, just a few plants can make a big difference.” Joe Morpurgo At Leiden University in the Netherlands.

Morpurgo says there have been some studies on biodiversity in larger gardens, but virtually none on smaller ones, so in 2019 his team surveyed 65 urban gardens in Amsterdam and The Hague, all measuring less than 10 square metres.

The researchers measured factors such as the total number of insects, the number of different species, whether the plants were native, and the area covered by the plants. Plant cover was calculated by adding up the area covered by individual specimens, so the garden’s cover can be greater than the area of the land due to plant overlap.

The researchers found that insect abundance and species richness were strongly correlated with plant cover and plant richness, but surprisingly, neither garden size nor native plant cover made any difference.

In theory, native plants should be better: Pollinating insects often adapt to particular flower shapes, and some plant-eating insects will eat specific varieties.

There are several possible explanations for why the proportion of native plants had no effect, Morpurgo said. For example, insects that breed in cities could be omnivorous, or many of them could be invasive species (the study did not categorize insects as native or not).

A study on the large-scale gardens of Wisley, England produces almost the same results“The more plant matter there is, the more invertebrates there are.” Andrew Salisbury These studies were led by staff from the Royal Horticultural Society (RHS).

But one RHS study found that native plants could support slightly higher numbers of plant-eating species, such as caterpillars, Salisbury said.

Morpurgo said he would continue to encourage people to grow native plants, which he said have many more benefits, including cultural value as well as helping insects.

His main advice is to do nothing and just allow plants, even those we might call weeds, to grow and attract wildlife: “If you leave everything alone, nature will come into your garden,” says Morpurgo.

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Source: www.newscientist.com

Are You Brushing Your Teeth Incorrectly? Here’s How to Properly Brush Them

Maintaining good oral hygiene is crucial for overall health. It goes beyond just having clean and shiny teeth – it’s about preventing cavities, gum disease, and maintaining a healthy oral microbiome.

Everyone has their own oral care routine, but it’s important to know how to properly care for your teeth in between visits to the dentist. Dr. Kami Hoss, in his book If Your Mouth Could Speak, shares valuable insights on oral hygiene.


How should I brush my teeth?

Dr. Hoss recommends a specific order for your morning oral care routine. After breakfast, follow these steps:

  1. Use an alkaline mouthwash
  2. Floss
  3. Use a tongue cleaner
  4. Brush

Brushing your teeth should be the last step, as plaque builds up overnight and mouthwash helps loosen it. Flossing, using a tongue cleaner, and then brushing with a mild alkaline toothpaste complete the routine.

What kind of mouthwash should I use?

Dr. Hoss advises against using strong antiseptic mouthwashes, as they can disrupt the oral microbiome. Instead, opt for alkaline mouthwashes that restore pH balance in the mouth.

What causes tooth decay?

Tooth decay occurs when the pH in your mouth becomes acidic, leading to demineralization of tooth enamel. Avoiding sugary and acidic foods can help maintain a balanced pH level and prevent cavities.


About our Expert, Dr. Kami Hoss

Dr. Kami Hoss is a dentist with extensive education in dentistry and orthodontics. He is the co-founder of The Super Dentists and author of If Your Mouth Could Speak.

Read more about teeth:

This article was first published on May 12, 2022.

Source: www.sciencefocus.com

Is it possible for liquid water to exist on planets orbiting dwarf stars?

Denis Villeneuve's sci-fi masterpiece Dune: Part 2 The film hits theaters in the US in spring 2024. The movie follows the power struggles of the noble families of the desert planet Arrakis. But what if humanity had become an empire that spanned thousands of worlds in the distant future, as depicted in the film? Sand Dunes How common are desert planets or planets with no water at all in movies and novels?

In the search for these planets, a good place to start is with the most common stars: astronomers have observed what are called small, faint, cool, reddish stars. Red dwarf They make up most of the stars in the galaxy. Astronomers who study planets around stars other than the Sun estimate that every star has at least one planet. About half of the planets around red dwarfs are small, rocky planets with compositions similar to Earth. On the ground planet. Therefore, the most common type of terrestrial planet is thought to be around a red dwarf star.

For decades, astronomers have thought that red dwarfs are too cold for liquid water to exist on their surfaces. To reach the temperature range needed to support liquid water, planets around cooler stars need to orbit closer to their host stars than planets around hotter ones. But unlike stars like the Sun, which have a constant brightness, red dwarfs are born hotter and brighter than their final state for most of their lives.

The terrestrial planets formed with 15 to 70 times more water than Earth, most of it coming from drifting icy comets. But the heat of the young red dwarf star causes the water on these planets to evaporate, turning from liquid to gas in their atmospheres. In the planet's atmosphere, the intense starlight breaks down the water vapor into oxygen and hydrogen. Photolysis. The heavier oxygen stays on the planet while the lighter hydrogen drifts away, and astronomers estimate that as a result, planets around red dwarf stars lose tens of times as much water as Earth's oceans over their first billion years.

A team of Japanese scientists led by Hiroshi Kawamura challenged the paradigm that planets around red dwarfs should lose all their water in this way. They proposed that two factors could significantly reduce the initial water loss of planets orbiting dwarf stars. First, water is decomposed by the intense light in the planet's atmosphere, but some water is produced in the atmosphere when reactive free hydrogen mixes with hydrogen superoxide. Second, the decomposition of water in the atmosphere produces oxygen gas, which protects the water from further intense light.

Kawamura's team used software called the Photochemical and Radiation Transport Model to Proteus To test whether the planet would lose less water if these two factors were taken into account. The researchers calculated the water loss for an Earth-like planet with a water vapor-filled atmosphere and huge oceans. The planet orbits the dwarf star at a distance about 2% of the distance it orbits around the Sun, relative to TRAPPIST-1, shown in the featured image above. The researchers assumed that the only chemical reaction occurring in the planet's atmosphere is between hydrogen and oxygen. Kawamura and his team ran the model once to see if the results differed from previous studies and how they changed depending on the altitude of the planet's atmosphere.

The team found that the model planet's atmosphere turned out as expected: It had a very high layer of atmosphere, where starlight split water into free hydrogen and oxygen atoms, with the hydrogen escaping into space, and a layer of oxygen gas formed below, reducing the intensity of the starlight at lower altitudes, and the free hydrogen mixed with hydrogen superoxide in a chemical reaction to produce more water.

Ultimately, they calculated that the amount of water lost to space was only about seven times that of Earth's oceans. This means that even if a terrestrial planet started at the low end of the water content range, it could still have eight times as much water as Earth's oceans after its first billion years of existence. The researchers suggested that their findings imply that rather than a galaxy filled with planets with little water, like Earth, the universe could contain worlds with vast oceans orbiting dwarf stars. In other words, future humans are likely to discover Arrakis, but not Caladan. Still, they suggested that future researchers should test planetary water loss models with different atmospheric compositions, alternative cooling processes, and water trapped in the planet's rocks and magma.


Post View: 83

Source: sciworthy.com

Photographs of NGC 5253 by the Hubble Space Telescope

Astronomers have used the NASA/ESA Hubble Space Telescope to create two stunning images of NGC 5253, a dwarf starburst galaxy and a possible blue compact dwarf galaxy.



This Hubble Space Telescope image shows NGC 5253, a blue compact dwarf galaxy about 11 million light-years away in the constellation Centaurus. Image credit: NASA / ESA / Hubble / A. Zezas / D. Calzetti.

NGC 5253 It is located in the constellation Centaurus, about 11 million light years from Earth.

This galaxy, also known as ESO 445-4, IRAS 13370-3123, LEDA 48334, and UGCA 369, is discovered It was discovered on March 15, 1787 by German-born British astronomer William Herschel.

The galaxy is thought to be part of the Centaurus A/Messier 83 galaxy group, which also includes the well-known radio galaxy Centaurus A and the spiral galaxy Messier 83.

The first new images of NGC 5253 Hubble’s Advanced Camera for Surveys (ACS) wide-field channel, Wide-field Planetary Camera 2 (WFPC2).

The second image is High Resolution Channels (HRC) of ACS Instruments.



This Hubble image was taken with the High Resolution Channel (HRC) of Hubble’s Advanced Camera for Surveys (ACS) showing NGC 5253. Image courtesy of NASA / ESA / Hubble / WD Vacca.

“What was it about this galaxy that fascinated us so much that we studied it intensively for more than a decade using three of the Hubble Space Telescope’s instruments?” the Hubble astronomers said.

“It turns out that Hubble’s capabilities are the focus of several research areas that are essential.”

“Dwarf galaxies are thought to be important for understanding the evolution of stars and galaxies over time because they resemble ancient, distant galaxies.”

“NGC 5253 has been called both a starburst galaxy and a blue compact dwarf. These names refer to the fact that this galaxy is forming a population of bright, massive stars at an exceptional rate.”

“This Hubble Space Telescope image clearly shows the dense nebula that is being consumed to give birth to these stars, making NGC 5253 a laboratory for studying stellar composition, star formation and star clusters all at once.”

“Very high star formation rates are essential for the formation of star clusters, but NGC 5253 goes beyond that. Star formation is so active in a small region of the central core that the galaxy contains more than three superclusters.”

“Superclusters are extremely luminous, dense and massive open clusters that are thought to evolve into globular clusters,” the researchers said.

“Globular clusters themselves provide unique insights into how stars form and evolve, but their origins are poorly understood.”

“So we wanted to take advantage of the excellent resolution of HRC’s auxiliary instruments to zero in on these small, very dense clusters.”

Source: www.sci.news

New GLP-1 medications offer potential for weight loss and improved health

Exciting developments are on the horizon in the world of obesity medications.

Pharmaceutical companies are racing to create new drugs, building on the success of existing medications like Novo Nordisk’s Ozempic and Wegovi, as well as Eli Lilly’s Maunjaro and Zepbound.

In addition to targeting diabetes and weight loss, some experimental drugs show promise in improving liver and heart function while reducing common side effects such as muscle loss seen with current treatments. Data on 27 GLP-1 drugs in development will be presented at the 2024 American Diabetes Association meeting in Orlando, Florida.

According to Marlon Pragnell, PhD, the ADA’s vice president of research and science, the pipeline now includes a variety of drug candidates in different stages of development, creating an exciting landscape of innovation.

While most of the data currently available comes from animal studies or early human trials, some drugs may be available in the United States over the counter within a few years, with FDA approval likely further down the line.

As the field of GLP-1 drugs continues to expand, there is hope for more affordable medications with fewer side effects to become available, offering new possibilities for patients.

Exploring Different Hormones for Weight Loss

GLP-1 drugs function by slowing down the digestive process and promoting a sense of fullness. In addition to GLP-1, emerging weight-loss drugs are examining the impact of another hormone called glucagon, which can mimic the effects of exercise.

One such drug, Pemvidutide from Maryland-based Altimmune, combines glucagon with GLP-1 to potentially enhance weight loss effects.

Results from a Phase 2 trial involving obese or overweight adults showed promising weight loss outcomes, paving the way for further research into the drug’s potential benefits.

Altimmune’s Chief Medical Officer, Dr. Scott Harris, highlighted the drug’s ability not only to aid in weight loss but also to provide additional health benefits for liver and heart function while preserving lean body mass.

Altimmune plans to move forward with Phase 3 trials and aims to introduce the drug in the U.S. by 2028.

Competition and Cost Considerations

Having a variety of weight-loss drugs available can help address shortages and potentially drive down costs over time. The high prices of current medications like Wegobee and Zepbound in the U.S. can pose financial challenges for many patients.

Different patients may respond differently to various treatments, as highlighted by Dr. Fatima Cody Stanford of Harvard Medical School. Having a range of options is crucial to tailor treatments to individual needs.

Stay Informed with the Latest News on Weight Loss Drugs

New developments in the pharmaceutical world present opportunities for improved treatment outcomes and potentially life-changing solutions for patients struggling with obesity.

For individuals like Danielle Griffin, who have not seen the desired results from current medications, the prospect of innovative drugs offers hope and excitement for the future.

Advancements in Metabolic Health

Companies like Eli Lilly are exploring new combinations of hormones to enhance the efficacy of weight-loss drugs. Retatortide, a new injectable medication from Lilly, shows promising results in weight loss and blood sugar control.

Additional studies on drugs like Mazduchid highlight the potential for improved metabolic status and weight loss outcomes, paving the way for new treatment options in the near future.

These ongoing developments underscore the dynamic landscape of obesity treatment, offering hope for a new generation of medications that could revolutionize the field and improve outcomes for patients.

The Future of Obesity Treatment

As research and development in the field of obesity medications continue to advance, there is optimism for more effective, affordable, and patient-friendly treatments to become available in the coming years.

With the potential for improved metabolic health, weight loss outcomes, and reduced side effects, the next wave of obesity treatments holds great promise for individuals struggling with obesity-related health issues.

The ongoing innovation in this field signifies a new era of possibilities in obesity treatment, offering hope for a healthier future for many individuals.

Source: www.nbcnews.com

Impending Lunar Battle: Tensions rise as a possible moon war looms on the horizon

The Moon, Earth’s loyal companion that remains steadfast in its orbit around our planet, has been a topic of fascination and exploration ever since the early days of space travel. Missions have been planned, rovers have traversed its surface, and even a flag has been planted on its barren landscape.

But what is the appeal of the Moon? Situated about 400,000 km away from Earth, it poses numerous challenges for human habitation, such as high levels of solar radiation. However, the Moon offers a unique opportunity for planetary research, scientific experiments, and potentially lucrative mining ventures due to its untapped resources.

With the allure of untapped resources comes a race to be the first to claim ownership of the Moon. This begs the question: Who does the Moon truly belong to? Philosopher and author AC Grayling explores this complex issue in his latest book, Who owns the moon?

SF: Why the interest in the Moon, and will we ever reach it?

ACG: The Moon holds vast potential for mining operations as it is rich in resources, presenting a more feasible option compared to Earth. Despite logistical challenges, rapid technological advancements and substantial investments indicate that lunar exploration is imminent.

Some argue that a robotic base alone may not suffice for the extraction of valuable resources like Helium-3, crucial for clean nuclear fusion. The lure of economic gains raises concerns about potential conflicts over lunar territory.

SF: So, who lays claim to the Moon?

The 1967 Outer Space Treaty, ratified by the United Nations, prohibits militarization and territorial ownership of the Moon, declaring it a common heritage of mankind. This ambiguity has spurred competition among nations to pioneer lunar technologies.

Efforts to establish guidelines were made in 1979, yet the absence of binding agreements leaves room for potential disputes over lunar resources, particularly valuable elements like Helium-3. The lack of a regulatory framework raises concerns about future conflicts, extending beyond Earth.

Credit: Gremlin

What’s next, and will legal frameworks evolve?

The need for stringent regulations is apparent, given the burgeoning interest in lunar exploration by various space agencies. Proposals for lunar space stations and the Artemis Accords, a collaborative effort among nations for responsible space conduct, hint at evolving norms to govern lunar activities.

Historically, the 1961 Antarctic Treaty provides a model for international cooperation in preserving a common resource. However, challenges arise as countries like China and Russia seek to assert territorial claims in Antarctica, signaling potential conflicts over resource exploitation.

The Moon’s status as a shared resource prompts calls for inclusive lunar laws and international treaties to ensure equitable benefits. Efforts to establish regulatory frameworks face obstacles, mirroring past struggles in maritime law and resource management.

Is there a case for leaving the Moon untouched?

The Moon’s vast expanse and desolate nature diminish concerns over environmental impact, distinguishing it from Earth. Despite existing space debris, the Moon’s remote location offers ample space for exploration and development.

What lies beyond the Moon?

Envisioning a future where lunar infrastructure facilitates Mars exploration through water extraction for fuel production, heralds a new era of space colonization. Echoing historical precedents, colonies in space may strive for autonomy, shaping interplanetary relations akin to terrestrial geopolitics.

As humanity embarks on extraterrestrial endeavors, adherence to ethical principles and equitable resource-sharing remains pivotal for a sustainable cosmic future.

This conversation has been edited for length and clarity.

About our expert, A.C. Grayling

AC Grayling, a distinguished philosopher and author, sheds light on lunar ownership in his book “Whose Moon is It?” He is also the founder of the New College of the Humanities, recognized for his contributions to literary criticism and philosophical discourse.

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Source: www.sciencefocus.com

Why your cat insists on sitting on your laptop (not as charming as you think)

Are you the owner of a lovely and precious cat? Then your cat might be blocking the display of this page and ruining everything again, especially if you are reading this page on a laptop.

But what is the reason behind this behavior? Why are cats so obsessed with our computers?

Unfortunately, no large-scale (and probably highly impractical) scientific experiments have yet been conducted to delve into this question, but experts in cat behavior do have an important theory that might explain keyboard cats.



Why does my cat sit on my laptop?

Unfortunately, it’s probably not a case of imitation behavior — your cat just sees you typing and doesn’t want to join in.

Indeed, recent research suggests that felines can mimic human behavior. Cats can map their bodies onto humans to repeat actions(For example, touching the box with the head or a specific limb).

but, Dr. David Sands – Animal Psychology Expert with over 25 years of clinical experience – Cats cannot easily imitate the behavior of typing, so your cat probably won’t be interested if you tempt him with a decoy old laptop.

Read more about cats:

It’s also unlikely that cats are attracted solely to the heat emitted by laptops: “Yes, laptops do generate heat, and cats do like warm places, but you need to ask why a cat wouldn’t sit next to a radiator, for example,” Sands says.

What really makes your laptop attractive to cats is its smell — or, more specifically, the smell you keep on it.

“You can’t smell it, but your cat can smell you all over the keyboard,” Sands says.

“Cats are olfactory machines, from the tip of their tail to the tip of their nose. Their world revolves around smells. Their eyesight is developed for nocturnal hunting, and their sense of smell is Really Other times it matters.”

But while it’s possible that your cat is sitting on your computer because it enjoys the smell, Sands says another explanation is far more likely.

“Your cat is most likely trying to steal your scent by leaving his own scent on you. It’s a matter of ownership. By doing this, your cat is essentially saying, ‘You’re mine!'”

“People often think that when a cat rubs itself against you or the objects you touch it’s an affectionate sign, but in reality cats are very possessive creatures. The more they rub against you and leave your scent behind, the better!”

“My Laptop, My Person” © Getty

In case you’re wondering whether cats are desperately trying to become the dominant force in the home, Sands adds: “Dogs have been bred to be companions to humans, but cats have also become quite feral. Cats have been bred primarily for pest control, so they are selfish creatures rather than sociable animals.”

“Remember, cats are evil geniuses. They James Bond There’s a reason to watch movies.”

Is it unhealthy for my cat to sit on my laptop?

From making you close important documents without saving to sending your boss another “s,ll,;;;;;l;mk” message, a cat snuggling on your laptop can take a huge toll on you. If your cat is getting in the way of your work, Sands recommends cleaning your laptop regularly.

But your cat is unlikely to be harmed by lounging on your computer: “Physically, it’s not harmful, and cognitively, it’s only something to be concerned about if this behavior occurs with other cats,” he says.

“If your cat meows a lot and follows you around the house, it could be a sign of anxiety or attention-seeking.”

But what if your cat isn’t showing these signs? There’s no reason why your cat can’t lie on your keyboard – it owns it, and everything else in your home.

About our Expert, Dr. David Sands

Sands has a PhD in Ethology (Animal Psychology) from the University of Liverpool and has over 25 years of experience in animal behaviour clinics. He is a member of the Canine and Cat Behavioural Association (CFBA) and the Association for the Study of Animal Behaviour (ASAB). Sands is also the author of several books. 500 Questions About Cats AnsweredHamlin, 4 pounds).

Read more about cat science

Source: www.sciencefocus.com

There is a possibility that dark energy is even more mysterious than previously believed.

Naming a new project the Dark Energy Spectroscopic Instrument (DESI) may come across as overly confident. This is because dark energy is undetectable and cannot be examined or analyzed through traditional methods like spectroscopy. Despite numerous attempts, dark energy has never been directly observed and remains a mystery in the realm of astrophysics.

Dark energy is believed to be a uniform force throughout the universe that does not interact with matter or light in any discernible way. Its primary function is to expand space at an accelerating rate, a process that baffles scientists due to its unknown underlying mechanism.

The recent release of data from DESI has sparked interest and debate in the scientific community. This project aims to shed light on the behavior of dark energy by mapping the expansion history of the universe. By studying the motion of galaxies and measuring the stretching of light emitted from distant objects, researchers can gain insights into the evolution of the cosmos.

The current prevailing model of cosmology suggests that dark energy exists as a static cosmological constant, affecting the fabric of space uniformly. However, DESI’s findings hint at a more complex history for dark energy, challenging conventional theories about its nature and implications for the future of the universe.

As researchers delve deeper into the mysteries of dark energy, they may uncover new discoveries that challenge existing paradigms and push the boundaries of our understanding of the cosmos. The DESI project represents an important step towards unraveling the enigma of dark energy and its profound impact on the universe.

Source: www.sciencefocus.com

Science has proven the most effective method for cutting a sandwich

It is commonly believed that cutting a sandwich diagonally to create two triangles is the best way, but there is limited scientific evidence to support this claim.

One theory suggests that the triangular shape allows for the first two bites to be taken from a 45-degree corner, which has crust on only one side, making it easier to access the center of the sandwich where the filling is most concentrated.

After eating the corner, take 1-3 bites diagonally, missing the crust. Depending on the size of the sandwich, you may be left with an additional small triangle.


Ultimately, each triangle will become a single 90-degree chunk of crust. However, cutting the sandwich into rectangles would result in two crust corners on each half.

Another reason for cutting sandwiches into triangles is that they are easier to eat. Starting at one of the corners leads to a cleaner bite, and the 45-degree angle of the triangle maximizes the engagement depth.

If taken to the extreme, cutting the sandwich into four triangles allows for a neat eating experience in three bites.

This cutting strategy is often used at children’s parties, though kids might not always start with the 45-degree corner. In such cases, simply cutting off the crust altogether may be the best option.

This article provides insight into the scientifically best way to cut a sandwich, as inquired by Jeremy Fry of Felixstowe.

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Source: www.sciencefocus.com