Category Archives: Science

‘Stretching’ of the continents 56 million years drove global warming, study finds

Stretching of the continents 56 million years ago is likely to have caused one of the most extreme episodes of global warming in Earth’s history, new research suggests. 

During this time, the planet experienced an increase in temperature of 5-8°C (9-14°F), culminating in the Paleocene-Eocene Thermal Maximum (PETM), which lasted about 170,000 years.

It caused the extinction of many deep-sea organisms and reshaped the course of evolution of life on Earth. 

Scientists studied the effects of global tectonic forces and volcanic eruptions during the period of environmental change almost 60 million years ago. 

They believe that the extensive stretching of the continental plates in the northern hemisphere – rather like the pulling of a toffee bar that thins and eventually separates – massively reduced the pressures in the Earth’s deep interior.

This then drove intense, but short-lived melting in the mantle – a layer of sticky, molten rock just below the planet’s crust. 

The team, including experts from the universities of Southampton, Edinburgh and Leeds, suggests that the resulting volcanic activity coincided with, and likely caused, a massive burst of carbon release into the atmosphere linked to PETM warming. 

‘Stretching’ of the continents 56 million years ago is likely to have caused one of the most extreme episodes of global warming in Earth’s history, new research suggests. Pictured is a false colour satellite image of the Faroe Islands – one of the locations studied by scientists

The team studied volcanic ash layers and lavas in the laboratories of the Integrated Ocean Drilling Program’s (IODP) Bremen Core Repository, Germany

Scientists found that intense episodes of volcanism were likely responsible for rapid warming during the Paleocene-Eocene Thermal Maximum warming event. Pictured is a volcano in Montserrat, West Indies

WHAT WAS THE PALEOCENE-EOCENE THERMAL MAXIMUM?

The Paleocene-Eocene Thermal Maximum (PETM) was a global warming event that occurred about 56 million years ago.

During this time, scientists estimate about 3,000 to 7,000 gigatons of carbon accumulated over a period of 3,000 to 20,000 years.

This lead global temperatures to spike by 5 to 8 degrees Celsius (9 to 14 degrees Fahrenheit), bringing the average as high as 23 degrees Celsius (73 degrees Fahrenheit). 

It lead to dramatic changes in Earth’s climate, driving major organisms to extinction and forcing others to migrate.

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Dr Tom Gernon, an associate professor of Earth science at the University of Southampton and lead author of the study, said: ‘Despite the importance and wider relevance of the PETM to global change today, the underlying cause is highly debated.

‘It’s generally agreed that a sudden and massive release of the greenhouse gas, carbon, from the Earth’s interior must have driven this event, yet the scale and pace of warming is very hard to explain by conventional volcanic processes.’

The scientists found evidence from rock drilled from the seafloor for a widespread episode volcanic activity lasting 200,000 years, which coincided with the PETM.

Using archives of rock drilled beneath the seafloor near the edge of the Atlantic Ocean, the team found evidence of an abrupt and widespread episode of volcanic activity across the North Atlantic Ocean that lasted just over 200,000 years, strikingly similar to the duration of the PETM.

This finding prompted the researchers to investigate a broader expanse of the North Atlantic region, including Greenland and the Faroe Islands. 

Here, they found that kilometre-thick piles of lava that started to erupt just before the PETM show unusual compositions that point to a significant increase in the amount of melting of the uppermost solid part of Earth’s mantle beneath the continent.

Dr Gernon said this would have led to a rapid increase of carbon being released, which would have led to the global warming.

Fragments of lava from the Atlantic are pictured here under a microscope

The volcanism occurred as the North Atlantic region was in the final stages of rifting, or breaking apart, in some ways similar to the geological processes occurring today in the East African Rift Valley, pictured

The intense volcanic activity occurred just as the continental landmass that united Greenland and Europe was most intensely stretched by plate tectonic forces. 

Eventually, North America and Greenland finally separated from Europe, leading to the birth of the North Atlantic Ocean. 

Scientists believe it was this final phase of stretching that brought about substantial melting in the Earth’s mantle, leading to massive carbon release, and in-turn, global warming. 

Dr Thea Hincks, senior research fellow at the University of Southampton and co-author on the study, said: ‘Using physically realistic estimates of the key characteristics of these volcanic systems, we show that the amount of carbon needed to drive warming could have been attained by enhanced melting.’

Dr Gernon added: ‘Such rapid events cause a fundamental reorganisation of Earth’s surface environment, altering vast ecosystems.’

The study has been published in the journal Nature Geoscience.

WHEN WAS THE PALEOCENE AND HOW DID IT IMPACT BRITAIN’S CLIMATE?

The Paleoscene (‘old recent’) is a geological period that stretched from 66 to 56 million years ago.  

During this period, the Earth’s climate was up to 15°C (27°F) warmer than it is today.

As a result, tropical and sub tropical forests extended further north and would have been widespread in the UK.

At the time there had not been an ice age for 100 million years.

The distance between Europe and Greenland was a tenth of what it is today.

There was massive volcanic activity between Baffin Island and northwest Europe that extended as far south as Bristol Channel. 

The shape of the continents were similar to those today except they were arranged differently due to tectonic plates. Britain, Ireland and Norway were all landlocked and the Arctic sea was almost completely surrounded by land

Britain, Ireland and Norway were all landlocked and the Arctic sea was almost completely surrounded by land.

The shape of the continents were similar to those today except they were arranged differently due to tectonic plates, according to a website dedicated to the Paleocene. 

Most of the world’s most famous geological features would not have been recognisable, including mountain ranges like the Alps and Himalayas which formed during the Tertiary period. 

Prior to the Paleocene-Eocene Thermal Maximum (PETM) – which occurred around 55 million years ago – non-avian dinosaurs had been extinct for around ten million years.

Early mammals, amphibians, reptiles, insects and flowering plants were the dominant forms of life.

Mammals were generally small, had short legs and five toes on each foot.

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25 Facts That Make You Feel Good

17.

“Cheetahs are very shy animals, so, some zoos give them support dogs like those for humans. It’s the cutest thing ever. The bigger reason for this is that a cheetah’s vision likes to hyper focus. In a crowd like the ones at the zoo, they would get anxious looking at each individual and would try to analyse each person, which can be very stressful for them. Dogs are VERY good at reading groups and crowds. They pair a dog with the cheetah to rely on emotionally. If the dog is calm, the cheetah will trust them that there’s nothing to worry about from those crowds.”

“How do zoos prevent the cheetah from killing the dog?

They’re typically introduced at a VERY young age and imprint on each other. Cheetahs are also not naturally driven to kill dogs as prey. A cheetah could kill a dog, but typically a cheetah would never hunt a dog in the wild. If it was in its territory, or if a dog appeared hurt and by itself, a cheetah might go for an opportunistic kill, but those are special circumstances. The most likely situation you’d see in the wild would be if they were hunting the same prey and they fought over a kill.”

— SnooWoofers455

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Giant sunspot doubled in size in 24 hours, and it’s pointing right at Earth

A gigantic sunspot has swelled to twice Earth’s size, doubling its diameter in 24 hours, and it’s pointed right at us. 

The sunspot, called AR3038, grew to 2.5 times Earth‘s size — making the sunspot roughly 19,800 miles, or 31,900 kilometers, in diameter — from Sunday (June 19) to Monday night (June 20), according to Spaceweather.com, a website that tracks news about solar flares, geomagnetic storms and other cosmic weather events. 

Sunspots are dark patches on the sun‘s surface where powerful magnetic fields, created by the flow of electric charges from the sun’s plasma, knot before suddenly snapping. The resulting release of energy launches bursts of radiation called solar flares and generates explosive jets of solar material called coronal mass ejections (CMEs). 

Related: Strange new type of solar wave defies physics

“Yesterday, sunspot AR3038 was big. Today, it’s enormous. The fast-growing sunspot has doubled in size in only 24 hours,” Spaceweather.com reported. “AR3038 has an unstable ‘beta-gamma’ magnetic field that harbors energy for M-class [medium-sized] solar flares, and it is directly facing Earth.”

When a solar flare hits Earth’s upper atmosphere, the flare’s X-rays and ultraviolet radiation ionize atoms, making it impossible to bounce high-frequency radio waves off them and creating a so-called radio blackout. Radio blackouts occur over the areas on Earth that are lit by the sun while a flare is underway; such blackouts are classified from R1 to R5 according to ascending severity. 

In April and May, two solar flares caused R3 blackouts over the Atlantic Ocean, Australia and Asia, Live Science previously reported. As solar flares travel at the speed of light, they take only 8 minutes to reach us, from an average distance of about 93 million miles (150 million kilometers). 

If an Earth-facing sunspot forms near the sun’s equator (where AR3038 is located), it typically takes just under two weeks for it to travel across the sun so that it is no longer facing Earth, according to SpaceWeatherLive. Currently, AR3038 lies slightly to the north of the sun’s equator and is just over halfway across, so Earth will remain in its crosshairs for a few more days. 

Despite its alarmingly speedy growth, the giant sunspot is less scary than it may seem. The flares it will most likely produce are M-class solar flares, which “generally cause brief radio blackouts that affect Earth’s polar regions,” alongside minor radiation storms, the European Space Agency wrote in a blog post. M-class flares are the most common type of solar flare. Although the sun does occasionally release enormous X-class flares (the strongest category) with the potential to cause high-frequency blackouts on the side of Earth that’s exposed to the flare, these flares are observed much less often than smaller solar eruptions.

Sunspots can also belch solar material. On planets that have strong magnetic fields, like Earth, the barrage of solar debris from CMEs is absorbed by our magnetic field, triggering powerful geomagnetic storms. During these storms, Earth’s magnetic field gets compressed slightly by the waves of highly energetic particles, which trickle down magnetic-field lines near the poles and agitate molecules in the atmosphere, releasing energy in the form of light to create colorful auroras in the night sky.

The movements of these electrically charged particles can disrupt our planet’s magnetic field powerfully enough to send satellites tumbling to Earth, Live Science previously reported, and scientists have warned that extreme geomagnetic storms could even cripple the internet. Erupting debris from CMEs usually takes around 15 to 18 hours to reach Earth, according to the National Oceanic and Atmospheric Administration’s (NOAA) Space Weather Prediction Center.

Astronomers have known since 1775 that solar activity rises and falls according to a roughly 11-year cycle, but recently, the sun has been more active than expected, with nearly double the sunspot appearances predicted by NOAA. The sun’s activity is projected to steadily climb for the next few years, reaching an overall maximum in 2025 before decreasing again.

Scientists think the largest solar storm ever witnessed during contemporary history was the 1859 Carrington Event, which released roughly the same energy as 10 billion 1-megaton atomic bombs. After slamming into Earth, the powerful stream of solar particles fried telegraph systems all over the world and caused auroras brighter than the light of the full moon to appear as far south as the Caribbean. If a similar event were to happen today, scientists warn, it would cause trillions of dollars in damage and trigger widespread blackouts, much like the 1989 solar storm that released a billion-ton plume of gas and caused a blackout across the entire Canadian province of Quebec, NASA reported.

Originally published on Live Science.

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Five planets are lining up in the sky in June. Here’s how to see it.

Five planets are moving into a rare alignment, which will be visible from Earth this week. Mercury, Venus, Mars, Jupiter and Saturn are lining up — in that order — for the first time since December 2004. On Friday, June 24, the phenomenon will be the most visible to stargazers.

While it is common to see a conjunction of three planets close together, seeing five is rare, according to Sky & Telescope. The planets are lining up in their natural order from the Sun, which is also remarkable, says the science magazine published by American Astronomical Society.

The five so-called “naked-eye” planets were visible beginning on June 3 and 4, and the lineup could be seen with binoculars — but only for about half an hour, before Mercury was lost in the glare of the sun. 

Sky & Telescope says the best time to see the the planets line up on June 24 is 45 minutes before sunrise. It should be visible on the eastern horizon. 

Sky & Telescope


But on June 24, viewing will be optimal. Even if the distance between Mercury and Saturn increases, it’s getting easier to spot Mercury, so it is getting progressively easier to see all five planets, Diana Hannikainen, observing editor of Sky & Telescope, told CBS News via email. 

Hannikainen said the sky on the morning of the 24th “will present a delightful sight” because the waning crescent moon will also join the procession between Venus and Mars. 

The planets should be visible on the days leading up to this. Sky & Telescope says the best time to see the line up on June 24 is 45 minutes before sunrise. It should be visible on the eastern horizon. 

Four of the naked-eye planets have been lining up in the for the past few months, according to NASA. But over the next few months, Saturn, Mars, Jupiter and Venus will spread out. By September, Venus and Saturn will no longer be visible to most observers. 

Another astronomical phenomenon will be visible in June: the M13 globular star cluster, a tightly packed spherical collection of stars. The M13, also known as the Hercules Cluster, contains thousands of stars, which are thought to be around 12 billion years old — almost the age of the universe itself, NASA says.

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Five planets are lining up in the sky in June. Here’s how to see it.

Five planets are moving into a rare alignment, which will be visible from Earth this week. Mercury, Venus, Mars, Jupiter and Saturn are lining up — in that order — for the first time since December 2004. On Friday, June 24, the phenomenon will be the most visible to stargazers.

While it is common to see a conjunction of three planets close together, seeing five is rare, according to Sky & Telescope. The planets are lining up in their natural order from the Sun, which is also remarkable, says the science magazine published by American Astronomical Society.

The five so-called “naked-eye” planets were visible beginning on June 3 and 4, and the lineup could be seen with binoculars — but only for about half an hour, before Mercury was lost in the glare of the sun. 

Sky & Telescope says the best time to see the the planets line up on June 24 is 45 minutes before sunrise. It should be visible on the eastern horizon. 

Sky & Telescope


But on June 24, viewing will be optimal. Even if the distance between Mercury and Saturn increases, it’s getting easier to spot Mercury, so it is getting progressively easier to see all five planets, Diana Hannikainen, observing editor of Sky & Telescope, told CBS News via email. 

Hannikainen said the sky on the morning of the 24th “will present a delightful sight” because the waning crescent moon will also join the procession between Venus and Mars. 

The planets should be visible on the days leading up to this. Sky & Telescope says the best time to see the line up on June 24 is 45 minutes before sunrise. It should be visible on the eastern horizon. 

Four of the naked-eye planets have been lining up in the for the past few months, according to NASA. But over the next few months, Saturn, Mars, Jupiter and Venus will spread out. By September, Venus and Saturn will no longer be visible to most observers. 

Another astronomical phenomenon will be visible in June: the M13 globular star cluster, a tightly packed spherical collection of stars. The M13, also known as the Hercules Cluster, contains thousands of stars, which are thought to be around 12 billion years old — almost the age of the universe itself, NASA says.

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Hubble Space Telescope catches dead star in cosmic cannibalism

The Hubble Space Telescope has spotted evidence of a white dwarf star devouring rocky and icy material from its own system, suggesting that water and other volatiles might be common in the outer reaches of planetary systems.

Astronomers used archival data from the Hubble Space Telescope and other observatories to analyze the spectral properties of the white dwarf star G238-44. The elements detected on the star’s surface show that the dead star is siphoning debris from its system’s inner and outer reaches.

“We have never seen both of these kinds of objects accreting onto a white dwarf at the same time,” Ted Johnson, the lead researcher and a recent graduate of the University of California, Los Angeles, said in a statement. “By studying these white dwarfs, we hope to gain a better understanding of planetary systems that are still intact.”

Related: A quarter of sunlike stars eat their own planets

Illustration shows a white dwarf star siphoning off debris from shattered objects in a planetary system. (Image credit: NASA, ESA, Joseph Olmsted (STScI))

The observation of this cosmic death dance provides a unique opportunity to see what planets were made of when they first formed around the star and to confirm ideas about the violent and chaotic end stages of similar systems.

G238-44 is a former sunlike star that has shed its outer layers and stopped burning fuel through nuclear fusion. The discovery that the stellar corpse is simultaneously capturing material from its asteroid belt and Kuiper Belt-like regions, including icy bodies, is significant because it suggests that a “water reservoir” might be a common feature in the outer reaches of planetary systems. 

Diagram of the planetary system G238-44 traces its destruction. (Image credit: NASA, ESA, Joseph Olmsted (STScI))

“Life as we know it requires a rocky planet covered with a variety of elements, like carbon, nitrogen and oxygen,” said Benjamin Zuckerman, professor emeritus in the UCLA Division of Astronomy and Astrophysics and co-author of the research. “The abundances of the elements we see on this white dwarf appear to require both a rocky and a volatile-rich parent body — the first example we’ve found among studies of hundreds of white dwarfs.”

The research group included astronomers at UCLA; the University of California, San Diego; and Kiel University in Germany. The team’s results were presented June 15 at an American Astronomical Society news conference.

Follow us on Twitter @Spacedotcom and on Facebook. 



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Unexpected solar weather is causing satellites to plummet from orbit

In late 2021, operators of the European Space Agency’s (ESA) Swarm constellation noticed something worrying: The satellites, which measure the magnetic field around Earth, started sinking toward the atmosphere at an unusually fast rate — up to 10 times faster than before. The change coincided with the onset of the new solar cycle, and experts think it might be the beginning of some difficult years for spacecraft orbiting our planet. 

“In the last five, six years, the satellites were sinking about two and a half kilometers [1.5 miles] a year,” Anja Stromme, ESA’s Swarm mission manager, told Space.com. “But since December last year, they have been virtually diving. The sink rate between December and April has been 20 kilometers [12 miles] per year.”

Satellites orbiting close to Earth always face the drag of the residual atmosphere, which gradually slows the spacecraft and eventually makes them fall back to the planet. (They usually don’t survive this so-called re-entry and burn up in the atmosphere.) This atmospheric drag forces the International Space Station‘s controllers to perform regular “reboost” maneuvers to maintain the station’s orbit of 250 miles (400 km) above Earth. 

This drag also helps clean up the near-Earth environment from space junk. Scientists know that the intensity of this drag depends on solar activity — the amount of solar wind spewed by the sun, which varies depending on the 11-year solar cycle. The last cycle, which officially ended in December 2019, was rather sleepy, with a below-average number of monthly sunspots and a prolonged minimum of barely any activity. But since last fall, the star has been waking up, spewing more and more solar wind and generating sunspots, solar flares and coronal mass ejections at a growing rate. And the Earth’s upper atmosphere has felt the effects.

Related: The biggest spacecraft ever to fall uncontrolled from space

“There is a lot of complex physics that we still don’t fully understand going on in the upper layers of the atmosphere where it interacts with the solar wind,” Stromme said. “We know that this interaction causes an upwelling of the atmosphere. That means that the denser air shifts upwards to higher altitudes.”

Denser air means higher drag for the satellites. Even though this density is still incredibly low 250 miles above Earth, the increase caused by the upwelling atmosphere is enough to virtually send some of the low-orbiting satellites plummeting. 

“It’s almost like running with the wind against you,” Stromme said. “It’s harder, it’s drag — so it slows the satellites down, and when they slow down, they sink.”

Knocked down by a solar storm  

The Swarm constellation, launched in 2013, consists of three satellites, two of which orbit Earth at an altitude of 270 miles (430 km), about 20 miles (30 km) above the International Space Station. The third Swarm satellite circles the planet somewhat higher — about 320 miles (515 km) above ground. The two lower-orbiting spacecraft were hit more by the sun’s acting out than the higher satellite was, Stromme said. 

The situation with the lower two got so precarious that by May, operators had to start raising the satellites’ altitude using onboard propulsion to save them. 

ESA’s Swarm satellites are not the only spacecraft struggling with worsening space weather. In February, SpaceX lost 40 brand-new Starlink satellites that were hit by a solar storm just after launch.

Related: Fiery death of SpaceX Starlink satellites captured on video after geomagnetic storm

The sun unleashed a major X1.1 class solar flare from an active sunspot cluster on its eastern limb on April 17, 2022. (Image credit: NASA/SDO and the AIA, EVE, and HMI science teams)

In such storms, satellites suddenly drop to lower altitudes. The lower the orbit of the satellites when the solar storm hits, the higher the risk of the spacecraft not being able to recover, leaving operators helplessly watching as the craft fall to their demise in the atmosphere.

Starlink satellites have operational orbits of 340 miles (550 km), which is above the most at risk region. However, after launch, Falcon 9 rockets deposit the satellite batches very low, only about 217 miles (350 km) above Earth. SpaceX then raises the satellites’ orbits using onboard propulsion units. The company says that approach has advantages, as any satellite that experiences technical problems after launch would quickly fall back to Earth and not turn into pesky space debris. However, the increasing and unpredictable behavior of the sun makes those satellites vulnerable to mishaps. 

New space and the unpredictable sun

All spacecraft around the 250-mile altitude are bound to have problems, Stromme said. That includes the International Space Station, which will have to perform more frequent reboost maneuvers to keep afloat, but also the hundreds of cubesats and small satellites that have populated low Earth orbit in the past decade. Those satellites — a product of the new space movement spearheaded by private entrepreneurs pioneering simple, cheap technologies — are particularly vulnerable.

“Many of these [new satellites] don’t have propulsion systems,” Stromme said. “They don’t have ways to get up. That basically means that they will have a shorter lifetime in orbit. They will reenter sooner than they would during the solar minimum.”

By coincidence (or beginner’s luck), the onset of the new space revolution came during that sleepy solar cycle. These new operators are now facing their first solar maximum. But not only that. The sun’s activity in the past year turned out to be much more intense than solar weather forecasters predicted, with more sunspots, more coronal mass ejections and more solar wind hitting our planet.

“The solar activity is a lot higher than the official forecast suggested,” Hugh Lewis, a professor of engineering and physical sciences at the University of Southampton in the U.K. who studies the behavior of satellites in low Earth orbit, told Space.com. “In fact, the current activity is already quite close to the peak level that was forecasted for this solar cycle, and we are still two to three years away from the solar maximum.”

Stromme confirmed those observations. “The solar cycle 25 that we are entering now is currently increasing very steeply,” she said. “We do not know if this means that it will be a very tough solar cycle. It could slow down, and it could become a very weak solar cycle. But right now, it’s increasing fast.”

Cleaning up orbits 

While the harsh solar activity is bad news for satellite operators, who will see the lifetimes of their missions shortened (even satellites with onboard propulsion will run out of fuel much faster because of the need for frequent altitude boosts), the situation will have some welcome purifying effects on the space around Earth. 

In addition to becoming populated with hundreds of new satellites over the past decade, this region of space is  cluttered with a worrying amount of space debris (old satellites, spent rocket stages and collision fragments). Researchers like Lewis have long warned that the omnipresent junk hurtling around the planet threatens the safety of satellite services, forcing operators to conduct frequent avoidance maneuvers. Moreover, the debris might trigger an out-of-control situation known as Kessler syndrome, an unstoppable cascade of collisions as depicted in the 2013 Oscar-winning movie “Gravity.”

“Generally speaking, increasing solar activity — and its effect on the upper atmosphere — is good news from a space debris perspective, as it reduces orbital lifetimes of the debris and provides a useful ‘cleaning service,'” Lewis said. 

According to Jonathan McDowell, a space debris expert at the Harvard-Smithsonian Center for Astrophysics, the positive effect can already be observed, as fragments produced by the November 2021 Russian anti-satellite missile test are now coming down much faster than before. 

However, there is a downside to this cleansing process. 

“The increased rate of decay of debris objects can be perceived almost like rain,” Lewis said. “When solar activity is high, the ‘rain’ rate is higher, and missions at lower altitudes will potentially experience a greater flux of debris.”

A greater flux of debris means the need for even more frequent fuel-burning avoidance maneuvers and a temporarily increased risk of collisions, which could potentially generate more dangerous fragments. 

Stromme and her colleagues are currently raising the orbit of the two low-orbiting Swarm satellites by 28 miles (45 km). The satellites might require even more adjustments later this year, she added. The goal is to help the mission, which is currently in its ninth year and beyond its originally planned lifetime, to get through the solar cycle. Whether the team succeeds will largely depend on the behavior of the sun. 

“We still have fuel to get us hopefully through another solar cycle,” Stromme said. “If it grows like now, I will use up the fuel before the solar cycle is finished. If it slows down a little, I might save them through the solar cycle.”

Follow Tereza Pultarova on Twitter @TerezaPultarova. Follow us on Twitter @Spacedotcom and on Facebook



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Electronic Tattoo Offers Highly Accurate, Continuous Blood Pressure Monitoring

A new electronic tattoo that can be worn comfortably on the wrist for hours delivers continuous blood pressure measurements at an accuracy level exceeding nearly all available options on the market today. Credit: University of Texas at Austin

Blood pressure is one of the most important indicators of heart health, but it’s tough to frequently and reliably measure outside of a clinical setting. For decades, cuff-based devices that constrict around the arm to give a reading have been the gold standard. But now, researchers at The University of Texas at Austin and Texas A&M University have developed an electronic tattoo that can be worn comfortably on the wrist for hours and deliver continuous blood pressure measurements at an

High blood pressure can lead to serious heart conditions if left untreated. It can be hard to capture with a traditional blood pressure check because that only measures a moment in time, a single data point.

“Taking infrequent blood pressure measurements has many limitations, and it does not provide insight into exactly how our body is functioning,” said Roozbeh Jafari, a professor of biomedical engineering, computer science, and electrical engineering at Texas A&M and the other co-leader of the project.

E-tattoos are a good choice for mobile blood pressure monitoring because they reside in a sticky, stretchy material encasing the sensors that is comfortable to wear for long periods and does not slide around. Credit: University of Texas at Austin

The continuous monitoring of the e-tattoo allows for blood pressure measurements in all kinds of situations: at times of high stress, while sleeping, exercising, etc. It can deliver thousands of measurements more than any device thus far.

Mobile health monitoring has taken major leaps in recent years, primarily due to technology such as smartwatches. These devices use metallic sensors that get readings based on LED light sources shined through the skin.

However, leading smartwatches are not yet ready for blood pressure monitoring. That’s because the watches slide around on the wrist and might be far from arteries, making it hard to deliver accurate readings. And the light-based measurements can falter in people with darker skin tones and/or larger wrists.

Graphene is one of the strongest and thinnest materials in existence, and it is a key ingredient in the e-tattoo. It is similar to graphite found in pencils, but the atoms are precisely arranged into thin layers.

E-tattoos make sense as a vehicle for mobile blood pressure monitoring because they reside in a sticky, stretchy material encasing the sensors that is comfortable to wear for long periods and does not slide around.

“The sensor for the tattoo is weightless and unobtrusive. You place it there. You don’t even see it, and it doesn’t move,” Jafari said. “You need the sensor to stay in the same place because if you happen to move it around, the measurements are going to be different.”

The device takes its measurements by shooting an electrical current into the skin and then analyzing the body’s response, which is known as bioimpedance. There is a correlation between bioimpedance and changes in blood pressure that has to do with blood volume changes. However, the correlation is not particularly obvious, so the team had to create a machine learning model to analyze the connection to get accurate blood pressure readings.

In medicine, cuff-less blood pressure monitoring is the “holy grail,” Jafari said, but there isn’t a viable solution on the market yet. It’s part of a larger push in medicine to use technology to untether patients from machines while collecting more data wherever they are, allowing them to go from room to room, clinic to clinic, and still get personalized care.

“All this data can help create a digital twin to model the human body, to predict and show how it might react and respond to treatments over time,” Akinwande said.

Reference: “Continuous cuffless monitoring of arterial blood pressure via



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NASA’s InSight Mars Lander Gets a Few Extra Weeks of Science Operations

NASA’s InSight Mars lander uses a seismometer to study the inner layers of Mars. Seismic signals from quakes change as they pass through different kinds of materials; seismologists can “read” the squiggles of a seismogram to study the properties of the planet’s crust, mantle, and core. Credit: NASA/JPL-Caltech

The InSight mission’s team has chosen to operate its seismometer longer than previously planned, although the lander will run out of power sooner as a result.

As the power available to

NASA’s InSight Mars lander took this final selfie on April 24, 2022, the 1,211th Martian day, or sol, of the mission. The lander is covered with far more dust than it was in its first selfie, taken in December 2018, not long after landing – or in its second selfie, composed of images taken in March and April 2019. Credit: NASA/JPL-Caltech

Instead, the team now plans to program the lander so that the seismometer can operate longer, perhaps until the end of August or into early September. Doing so will discharge the lander’s batteries sooner and cause the spacecraft to run out of power at that time as well, but it might enable the seismometer to detect additional marsquakes.

“InSight hasn’t finished teaching us about Mars yet,” said Lori Glaze, director of NASA’s Planetary Science Division in Washington. “We’re going to get every last bit of science we can before the lander concludes operations.”


The InSight team will be available to answer your questions directly on June 28 at 3 p.m. EDT (noon PDT) during a livestream event on YouTube. Questions can be asked using the #AskNASA hashtag.


InSight (short for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) is in an extended mission after achieving its science goals. The lander has detected more than 1,300 marsquakes since touching down on Mars in 2018, providing information that has allowed scientists to measure the depth and composition of Mars’ crust, mantle, and core. With its other instruments, InSight has recorded invaluable weather data, investigated the soil beneath the lander, and studied remnants of Mars’ ancient magnetic field.

This is NASA InSight’s first full selfie on Mars. It displays the lander’s solar panels and deck. On top of the deck are its science instruments, weather sensor booms, and UHF antenna. The selfie was taken on December 6, 2018 (Sol 10). Credit: NASA/JPL-Caltech

All instruments but the seismometer have already been powered down. Like other Mars spacecraft, InSight has a fault protection system that automatically triggers “safe mode” in threatening situations and shuts down all but its most essential functions, allowing engineers to assess the situation. Low power and temperatures that drift outside predetermined limits can both trigger safe mode.

To enable the seismometer to continue to run for as long as possible, the mission team is turning off InSight’s fault protection system. While this will enable the instrument to operate longer, it leaves the lander unprotected from sudden, unexpected events that ground controllers wouldn’t have time to respond to.

This is NASA InSight’s second full selfie on Mars. Since taking its first selfie, the lander has removed its heat probe and seismometer from its deck, placing them on the Martian surface; a thin coating of dust now covers the spacecraft as well. This selfie is a mosaic made up of 14 images taken on March 15 and April 11 – the 106th and 133rd Martian days, or sols, of the mission – by InSight’s Instrument Deployment Camera, located on its robotic arm. Credit: NASA/JPL-Caltech

“The goal is to get scientific data all the way to the point where InSight can’t operate at all, rather than conserve energy and operate the lander with no science benefit,” said Chuck Scott, InSight’s project manager at NASA’s Jet Propulsion Laboratory in Southern California.

Regular updates on InSight’s power and observations from mission team members will appear on blogs.nasa.gov/insight.

The InSight team will also be available to answer your questions directly on June 28 at 3 p.m. EDT (noon PDT) during a livestream event on YouTube. Questions can be asked using the #AskNASA hashtag.

More About the Mission



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Theoretical calculations predicted now-confirmed tetraneutron, an exotic state of matter

Andrey Shirokov, left, of Moscow State University in Russia, who has been a visiting scientist at Iowa State, and James Vary of Iowa State are part of an international team of nuclear physicists who theorized, predicted and announced a four-neutron structure in 2014 and 2016. Credit: Christopher Gannon / Iowa State University College of Liberal Arts and Sciences

James Vary has been waiting for nuclear physics experiments to confirm the reality of a “tetraneutron” that he and his colleagues theorized, predicted and first announced during a presentation in the summer of 2014, followed by a research paper in the fall of 2016.

“Whenever we present a theory, we always have to say we’re waiting for experimental confirmation,” said Vary, an Iowa State University professor of physics and astronomy.

In the case of four neutrons (very, very) briefly bound together in a temporary quantum state or resonance, that day for Vary and an international team of theorists is now here.

The just-announced experimental discovery of a tetraneutron by an international group led by researchers from Germany’s Technical University of Darmstadt opens doors for new research and could lead to a better understanding of how the universe is put together. This new and exotic state of matter could also have properties that are useful in existing or emerging technologies.

Neutrons, you probably remember from science class, are subatomic particles with no charge that combine with positively charged protons to make up the nucleus of an atom. Individual neutrons aren’t stable and after a few minutes convert into protons. Combinations of double and triple neutrons also don’t form what physicists call a resonance, a state of matter that is temporarily stable before it decays.

Enter the tetraneutron. Using the supercomputing power at the Lawrence Berkeley National Laboratory in California, the theorists calculated that four neutrons could form a resonant state with a lifetime of just 3×10-22 seconds, less than a billionth of a billionth of a second. It’s hard to believe, but that’s long enough for physicists to study.

The theorists’ calculations say the tetraneutron should have an energy of about 0.8 million electron volts (a unit of measurement common in high-energy and nuclear physics—visible light has energies of about 2 to 3 electron volts.) The calculations also said the width of the plotted energy spike showing a tetraneutron would be about 1.4 million electron volts. The theorists published subsequent studies that indicated the energy would likely lie between 0.7 and 1.0 million electron volts while the width would be between 1.1 and 1.7 million electron volts. This sensitivity arose from adopting different available candidates for the interaction between the neutrons.

A just-published paper in the journal Nature reports that experiments at the Radioactive Isotope Beam Factory at the RIKEN research institute in Wako, Japan, found tetraneutron energy and width to be around 2.4 and 1.8 million electron volts respectively. These are both larger than the theory results but Vary said uncertainties in the current theoretical and experimental results could cover these differences.

“A tetraneutron has such a short life it’s a pretty big shock to the nuclear physics world that its properties can be measured before it breaks up,” Vary said. “It’s a very exotic system.”

It is, in fact, “a whole new state of matter,” he said. “It’s short-lived, but points to possibilities. What happens if you put two or three of these together? Could you get more stability?”

Experiments trying to find a tetraneutron started in 2002 when the structure was proposed in certain reactions involving one of the elements, a metal called beryllium. A team at RIKEN found hints of a tetraneutron in experimental results published in 2016.

“The tetraneutron will join the neutron as only the second chargeless element of the nuclear chart,” Vary wrote in a project summary. That “provides a valuable new platform for theories of the strong interactions between neutrons.”

Meytal Duer of the Institute for Nuclear Physics at the Technical University of Darmstadt is the corresponding author of the Nature paper, titled “Observation of a correlated free four-neutron system” and announcing the experimental confirmation of a tetraneutron. The experiment’s results are considered a five-sigma statistical signal, denoting a definitive discovery with a one in 3.5 million chance the finding is a statistical anomaly.

The theoretical prediction was published October 28, 2016, in Physical Review Letters, titled “Prediction for a Four-Neutron Resonance.” Andrey Shirokov of the Skobeltsyn Institute of Nuclear Physics at Moscow State University in Russia, who has been a visiting scientist at Iowa State, is the first author. Vary is one of the corresponding authors.

“Can we create a small neutron star on Earth?” Vary titled a summary of the tetraneutron project. A neutron star is what’s left when a massive star runs out of fuel and collapses into a super-dense neutron structure. The tetraneutron is also a neutron structure, one Vary quips is a “short-lived, very-light neutron star.”

Vary’s personal reaction? “I had pretty much given up on the experiments,” he said. “I had heard nothing about this during the pandemic. This came as a big shock. Oh my God, here we are, we may actually have something new.”


Physicists demonstrate existence of new subatomic structure


More information:
M. Duer et al, Observation of a correlated free four-neutron system, Nature (2022). DOI: 10.1038/s41586-022-04827-6
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Theoretical calculations predicted now-confirmed tetraneutron, an exotic state of matter (2022, June 22)
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