Tuesday, March 31, 2020

Production of NASA's new X-59 supersonic jet continues amid coronavirus outbreak

By Chelsea Gohd,  Mon. March 30 2020
https://www.space.com/nasa-x-59-supersonic-jet-development-coronavirus.html

"Lockheed Martin is continuing with X-59 production operations."

The so-called quiet X-59 QueSST.
(Image: © NASA)

Production on NASA's new X-59 supersonic X-plane despite closures and delays in the space industry caused by the spread of COVID-19, the disease caused by the novel coronavirus SARS-CoV-2.

In a March 20 statement, NASA officials said that "in California, work continues by Lockheed Martin on X-59, NASA's first large-scale, piloted X-plane in more than 30 years, while NASA oversight and inspections will be conducted almost exclusively virtually."

"Lockheed Martin is continuing with X-59 production operations, and the only on-site NASA presence is a Quality Assurance representative when needed for the GMIPs (Government Mandatory Inspection Points)," said Craig Nickol, NASA's Low Boom Flight Demonstrator project manager, in a statement provided to Space.com.

Final assembly for the supersonic plane, which was officially named X-59 QueSST in 2018, was greenlit during a critical design review in 2019. The plane is designed to travel over land faster than the speed of sound. But, unlike earlier supersonic planes, its main draw is that it will supposedly create an ultra quiet sonic boom, making it much less of a disturbance to the general public.

As a Lockheed Martin representative told Space.com in February, "We're very confident. All kinds of modeling simulations and predictions align, so we believe, based on these models and simulations we've run, that it will achieve that low-boom sound once it reaches supersonic speeds."

The supersonic X-59 QueSST is not the only new X-plane NASA is continuing work on amid the coronavirus pandemic. The agency is also making advances on its new X-57 all-electric plane, NASA spokesperson Sasha Ellis of the Langley Research Center said via email.

The supersonic X-59 QueSST is not the only new X-plane NASA is continuing work on amid the coronavirus pandemic. The agency is also making advances on its new X-57 all-electric plane, NASA spokesperson Sasha Ellis of the Langley Research Center said via email.

Discussing further how work is progressing amid coronavirus, the spokesperson recently told Space.com that "work is also continuing on NASA's X-57, the agency's first all-electric X-plane."

"The team is maintaining communication and getting parts in place for functional tests, taxi tests, and eventually flight tests," Matt Kamlet, NASA's X-57 public affairs specialist at the Armstrong Flight Research Center in California, said in the statement.


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SPACE - S0 - 20200331 - Solar Wind, QuakeWatch, Survival, Galactic Sheet GCR

SPACE - S0 - 20200331 - Solar Wind, QuakeWatch, Survival, Galactic Sheet GCR

Good Morning, 0bservers!

   
    
We had two sharp upticks in solar wind speed, the first before midday with a jump from 350 KPS to 450 KPS, and the second about two hours later elevating further to the 500-525 KPS range with the current speed in the 450-500 KPS range (last reading at 485 KPS). There was a matching increase in density at the beginning of the speed bump, and the temperature also rose at same time and rate. The KP Index rose and, after midnight, popped into the KP-4 (minor storm) range. The electron flux rose as well, but stayed below the alert threshold. That new sunspot group in the North is quite active, very bright, and it'll be interesting to see the magnetic complexity level later when the imaging scans come through. At present the two distinct spots don't show much, but they're far enough apart to at least suggest beta-level complexity. Looks like Cycle 25 might actually have arrived. Only two ocean-bound quakes of note, a Mag 5.4 off the coast of Japan, and a 5.1 along the Mid-Indian Ridge. 
   
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Monday, March 30, 2020

Geopolymer concrete: Building moon bases with astronaut urine and regolith

MARCH 30, 2020, by Enrique Sacristán
Spanish Foundation for Science and Technology (FECYT)


Future moon bases could be built with 3D printers that mix materials such as moon regolith, water and astronauts' urine Credit: ESA, Foster and Partners

The modules that the major space agencies plan to erect on the moon could incorporate an element contributed by the human colonizers themselves: the urea in their pee. European researchers have found that it could be used as a plasticizer for concrete used to build structures.

NASA, the European Space Agency (ESA) and its Chinese counterpart plan to build moon bases in coming decades as part of a broader space exploration plan that will take humans to more distant destinations such as Mars.

However, the colonization of the moon poses problems such as high levels of radiation, extreme temperatures, meteorite bombardment and a logistical issue: getting construction materials there, although it may not be necessary.

Transporting about 0.45 kg from the Earth to space costs about $10,000, which means that building a complete lunar module in this way would be very expensive. This is the reason that space agencies are thinking of using raw materials from the moon's surface—or even those that astronauts themselves can provide, such as their urine.

Scientists from Norway, Spain, the Netherlands and Italy, in cooperation with ESA, have conducted several experiments to verify the potential of urea as a plasticizer, an additive that can be incorporated into concrete to soften the initial mixture and make it more pliable before it hardens. Details are published in the Journal of Cleaner Production.

Device for printing 3D samples Credit: Shima Pilehvar et al./ Journal of Cleaner Production



"To make geopolymer concrete that will be used on the moon, the idea is to use what is already there: regolith (loose material from the moon's surface) and the water from the ice present in some areas," explains one of the authors, Ramón Pamies, a professor at the Polytechnic University of Cartagena (Murcia), where various analyses of the samples have been carried out using X-ray diffraction. "But moreover, with this study, we have seen that a waste product, such as the urine of the personnel who occupy the moon bases, could also be used. The two main components of urine are water and urea, a molecule that allows the hydrogen bonds to be broken and, therefore, reduces the viscosities of many aqueous mixtures."

Using a material similar to moon regolith developed by ESA, together with urea and various plasticizers, the researchers manufactured various concrete cylinders using a 3-D printer and compared the results.

The experiments, carried out at Østfold University College (Norway), revealed that the samples made with urea supported heavy weights and remained almost stable in shape. Their resistance was also tested at a temperature 80°C; it was found to increase even after eight freeze-thaw cycles like those on the moon.


Tests to see the ability to form layers of a mixture of material with 3% urea (sample U) and another with 3% naphthalene, a common plasticizer (sample N) Credit: Shima Pilehvar et al. / Journal of Cleaner Production


"We have not yet investigated how the urea would be extracted from the urine, as we are assessing whether this would really be necessary, because perhaps its other components could also be used to form the geopolymer concrete," says one of the researchers from the Norwegian university, Anna-Lena Kjøniksen, who adds: "The actual water in the urine could be used for the mixture, together with that obtained on the moon, or a combination of both."

The scientists stress the need for further testing to find the best building material for the moon bases, where it can be mass-produced using 3-D printers.


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SPACE - S0 - 20200330 - Sunspots Return, Ozone Extinctions, Primordial Magnetism

SPACE - S0 - 20200330 - Sunspots Return, Ozone Extinctions, Primordial Magnetism

Good Morning, 0bservers!

   
    
Solar wind speeds basically tanked from yesterday's spike at 450 KPS down to a current 350 KPS, despite a bit of Phi Angle instability just after midnight. The KP Index remains in the green zone, but without the expected KP-0 activity, mostly KP-1s and KP-2s. Some rather impressive bright spots crossed the lim overnight and they're showing some activity that suggests active cores and magnetic complexity. They're well North of the equator, but as they get closer to central heliographic longitude, they could pose a risk depending on whether they blow or decay. Have to wait and see (and we will). There's already been a slight rise in X-ray activity to match this new bright spot group. The majority of tectonic activity yesterday were deep blot echos (as per normal), with a notable Mag 5.6 blot echo in Ecuador, as well as a Mag 5.6 quake a little over 100 miles East of New Caledonia, a Mag 5.1 along the Northern Mid-Atlantic Ridge, and a Mag 5.0 180 miles South of Tonga.
   
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Sunday, March 29, 2020

New Paper Suggests Life Could Be Common Across The Universe, Just Not Near Us

EVAN GOUGH, UNIVERSE TODAY, 14 MARCH 2020
https://www.sciencealert.com/life-could-be-common-across-the-universe-just-not-in-our-neck-of-the-woods

Map of the observable universe. (Pablo Carlos Budassi/Wikimedia/CC BY 4.0)

The building blocks of life can, and did, spontaneously assemble under the right conditions. That's called spontaneous generation, or abiogenesis. Of course, many of the details remain hidden to us, and we just don't know exactly how it all happened.

Or how frequently it could happen.

The world's religions have different ideas of how life appeared, of course, and they invoke the magical hands of various supernatural deities to explain it all. But those explanations, while colorful tales, leave many of us unsatisfied.

'How did life arise' is one of life's most compelling questions, and one that science continually wrestles with.

Tomonori Totani is one scientist who finds that question compelling. Totani is a professor of Astronomy at the University of Tokyo. He's written a new paper titled Emergence of life in an inflationary universe. It's published in Nature Scientific Reports.

Totani's work leans heavily on a couple concepts. The first is the vast age and size of the Universe, how it's inflated over time, and how likely events are to occur. The second is RNA; specifically, how long a chain of nucleotides needs to be in order to "expect a self-replicating activity" as the paper says.

Totani's work, like almost all work on abiogenesis, looks at the basic components of life on Earth: RNA, or ribonucleic acid. DNA sets the rules for how individual life forms take shape, but DNA is much more complex than RNA.

RNA is still more complex, by orders of magnitude, than the raw chemicals and molecules found in space or on the surface of a planet or moon. But its simplicity compared to DNA makes it more likely to occur via abiogenesis.

There's also one theory in evolution saying that although DNA carries the instructions to build an organism, it's RNA that regulates the transcription of DNA sequences. It's called RNA-based evolution, and it says that RNA is subject to Darwinian natural selection, and is also heritable. That's some of the rationale behind looking at RNA vs DNA.




Double stranded RNA. (Supyyyy/Wikimedia/CC By 4.0)




RNA is a chain of chemicals known as nucleotides. Some research shows that a chain of nucleotides needs to be at least 40 to 100 nucleotides long before the self-replicating behaviour called life can exist.

Over time, enough nucleotides can form a chain to meet that length requirement. But the question is, has there been enough time in the life of the Universe? Well, we're here, so the answer must be yes, mustn't it?

But wait. According to a press release announcing this new paper, "… current estimates suggest that magic number of 40 to 100 nucleotides should not have been possible in the volume of space we consider the observable universe."

The key here is the term 'observable universe.'

"However, there is more to the universe than the observable," said Totani. "In contemporary cosmology, it is agreed the universe underwent a period of rapid inflation producing a vast region of expansion beyond the horizon of what we can directly observe. Factoring this greater volume into models of abiogenesis hugely increases the chances of life occurring."

Our Universe came into being during the Big Bang, a single inflation event. According to Totani's paper, our Universe "likely includes more than 10^100 Sun-like stars," whereas the observable Universe only contains about 10 sextillion (10^22) stars.

We know that life has occurred at least once, so it's not out of the question that abiogenesis occurred at least once more, even if the chances are infinitesimally tiny.

According to statistics, the amount of matter in the observable Universe should only be able to produce RNA that is 20 nucleotides long, well under the 40 to 100 number. But because of rapid inflation, much of the Universe is unobservable. It's simply too far away for light emitted since the Big Bang to reach us.

When cosmologists add up the number of stars in the observable Universe with the number of stars in the unobservable Universe, the resulting number is 10^100 Sun-like stars. That means there is much more matter in play, and the abiogenic creation of long enough chains of RNA is not only possible, but probable, or even inevitable.

In his paper, Professor Totani states the basic relationship under investigation. "Here, a quantitative relation is derived between the minimum RNA length/min required to be the first biological polymer, and the universe size necessary to expect the formation of such a long and active RNA by randomly adding monomers."

Is it getting confusing? Here's a hopefully more manageable summary.

The Universe is larger than its observable portion, and likely contains 10^100 Sun-like stars. For the probability of abiotic creation of RNA on an Earth-like planet to equal 1, or unity, then the minimum nucleotide length must be less than about 20 nucleotides, which is much smaller than the initially stated minimum of 40 nucleotides.

But scientists don't think that RNA only 20 nucleotides long can be self-replicating, at least not from our perspective as observers of terrestrial life. As Totani says in his paper, "Therefore, if extraterrestrial organisms of a different origin from those on Earth are discovered in the future, it would imply an unknown mechanism at work to polymerize nucleotides much faster than random statistical processes."

What would that process be?

Who knows, but this is likely an inflection point where people of faith can chime in and say, "Why God, of course."

Totani's work has by no means provided an answer. But like a lot of scientific work, it helps refine the question, and invites other to study it.

"Like many in this field of research, I am driven by curiosity and by big questions," said Totani.

"Combining my recent investigation into RNA chemistry with my long history of cosmology leads me to realize there is a plausible way the universe must have gone from an abiotic (lifeless) state to a biotic one. It's an exciting thought and I hope research can build on this to uncover the origins of life."


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SPACE - S0 - 20200329 - Polar Wind & Magnetic Reversal, Tornado & Volcano

SPACE - S0 - 20200329 - Polar Wind & Magnetic Reversal, Tornado & Volcano

Good Morning, 0bservers!

   
    
Solar winds rose a bit in the afternoon and evening yesterday, and then took a small jump upward when there was a minor solar magnetic instability on the Phi Angle chart. However, that was only up to around 450 KPS, and we're currently back down to around 420 KPS, so it's nothing of concern. The KP Index has remained calm for the last three days, with KP-0s, 1s and a few 2s. The coronal hole at the South pole remains large, but it hasn't grown Northward again as it had earlier in the week. Expect the effects of that line in the next couple of days. No bright spots of note or concern on the solar face, but at the beginning of the video you'll see some beautiful activity at the Northeast lim. Two temblors of note yesterday - a Mag 5.8 off Indonesia, and a Mag 5.9 blot echo (about 60 miles deep) just off Vanuatu.
   
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Saturday, March 28, 2020

Space - Space Force launches first mission with virus precautions

Space Force launches first mission with virus precautions


By Associated Press,  March 27,  2020

A United Launch Alliance Atlas V rocket lifts off from launch complex 41 at the Cape Canaveral Air Force Station with a payload of a high frequency satellite. AP photo.

CAPE CANAVERAL, Fla. — The newly established US Space Force launched its first national security satellite Thursday with a leaner staff because of the coronavirus pandemic.
“Nothing stops the space launch mission!” the 45th Space Wing tweeted from Cape Canaveral.
The approximately $1 billion satellite is the sixth and final one in the US military’s Advanced Extremely High Frequency series. Upgraded from the older Milstar satellites, the constellation has provided secure communication from 22,000 miles up for nearly a decade.
A powerful Atlas V rocket hoisted the 13,600-pound satellite. The new Space Force seal adorned the United Launch Alliance rocket.
The Space Force officially became a new branch of the US military in December.
With the viewing area closed because of the coronavirus outbreak, fewer people than usual watched the liftoff from Cape Canaveral Air Force Station.
United Launch Alliance chief executive Tory Bruno said non-essential personnel were banned from the launch control room to reduce the size of the crowd.
“Can’t quite get 6 ft everywhere. Surfaces will be cleaned between people, etc.,” tweeted Bruno, who monitored the launch from company headquarters in Denver. He normally travels to the launch site.
Another pandemic effect: Cape Canaveral Air Force Station’s planned name change to Cape Canaveral Space Force Station is on hold.

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Defense - Nearly 4 years after commissioning, the US Navy is about to get a fully working stealth destroyer

Nearly 4 years after commissioning, the US Navy is about to get a fully working stealth destroyer


 , Defense News.   March 27,  2020

The destroyer Zumwalt was underway in Maine heading for builder trials. The U.S. Navy will finally get its ship fully operational in the coming days. (Robert F. Bukaty/AP)

WASHINGTON — The U.S. Navy’s first stealth destroyer, the Zumwalt, is on track to have its combat system installation completed and delivered within days, a source with knowledge of the program told Defense News.
It’s the end of a long journey for the ship that was commissioned in 2016 without a working combat system but is finally preparing to fully enter service. The ship was slated to have its installation completed in March, and the service is still on track to deliver on time, the source said.
In November 2016, BAE Systems was awarded a $192 million contract to deliver the combat system for Zumwalt and its sister ship the Michael Monsoor.

The Standard Missile-6 (SM-6) is an endo-atmospheric interceptor, which uses a blast-fragmentation warhead to engage cruise missiles, aircraft, and ballistic missiles in the terminal phase. 


The DDG-1000 program has been beleaguered by cost overruns and changes over the years. The ship’s original raison d'être, the Advanced Gun System, has been all but abandoned by the Navy as it has changed from a naval gunfire support platform for landing Marines to now a surface strike platform.
As the Navy truncated the buy of Zumwalt-class destroyers from 28 ships, to seven, and finally to three, the rounds for the guns became steadily more expensive, making the projectile — Long Range Land Attack Projectile — too valuable to fire. The Navy has yet to identify a replacement.
Instead, the ship has been predesignated a ship killer, with Maritime Strike Tomahawk and SM-6 integrated into its combat system.

A rendering of Lockheed Martin's Long-Range Anti-Ship Missile. (Courtesy of Lockheed Martin)

The Navy has stood up the Surface Development Squadron to help it integrate new technologies into the fleet, such as unmanned surface vessels and the DDG-1000.
An image of the Long-Range Anti-Ship Missile. (Courtesy of Lockheed Martin)


The Michael Monsoor should have its combat system activation done by the second quarter of 2020, according to a Naval Sea Systems Command program brief from January. The third and final ship of the class, the Lyndon B. Johnson, is still under construction at Bath Iron Works in Maine and should be delivered by December 2020.
The ship will then transit to San Diego, California, and have its combat system installed like its sister ships.

The destroyer USS Michael Monsoor successfully completed acceptance trials in February 2018. (Navy via Bath Iron Works)


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Bubbles go with the flow: Simulating behavior of fluids moving through pipes

MARCH 27, 2020, by University of Tokyo
https://phys.org/news/2020-03-simulating-behavior-fluids-pipes.html

The University of Tokyo researchers develop a new physical model incorporating the density dependence of viscosity to understand the interactions of flowing viscous fluids with pipe walls, with promise to improve efficiency of industrial processes such as oil transportation. 
Credit: Institute of Industrial Science, The University of Tokyo

Researchers at the Institute of Industrial Science, The University of Tokyo, used a sophisticated physical model to simulate the behavior of fluids moving through pipes. By including the possibility of shear-induced bubble formation, they find that, contrary to the assumptions of many previous works, fluids can experience significant slippage when in contact with fixed boundaries. This research may help reduce energy losses when pumping fluids, which is a significant concern in many industrial applications, such as gas and oil suppliers.

Fluid dynamics is one of the most challenging areas of physics. Even with powerful computers and the use of simplifying assumptions, accurate simulations of fluid flow can be notoriously difficult to obtain. Researchers often need to predict the behavior of fluids in real-world applications, such as oil flowing through a pipeline. To make the problem easier, it has been common practice to assume that at the interface between the fluid and the solid boundary—in this case, the pipe wall—the fluid flows without slipping. However, the evidence to support this shortcut has been lacking. More recent research has shown the slippage can occur under certain circumstances, but the physical mechanism has remained mysterious.

Now, to understand more rigorously the origin of flow slippage, researchers at the University of Tokyo created an advanced mathematical model that includes the possibility of dissolved gas turning into bubbles on the pipe's inner surface.

"The no-slip boundary condition of liquid flow is one of the most fundamental assumptions in fluid dynamics," explains first author Yuji Kurotani. "However, there is no rigorous physical foundation for this condition, which ignores the effects of gas bubbles."

To do this, the researchers combined the Navier-Stokes equations, which are the basic laws that govern fluid flow, with Ginzburg-Landau theory, which describe phase transitions such as the change from a liquid to a gas. The simulations revealed that flow slippage can be caused by tiny microbubbles that form on the pipe wall. The bubbles, which are created by the shear forces in the fluid, often escape detection in real life because they remain very small.

"We found that the density changes that accompany viscosity variation can destabilize the system toward bubble formation. Shear-induced gas-phase formation provides a natural physical explanation for flow slipping," says senior author Hajime Tanaka.

Says Kurotani, "The results of our project can help design new pipes that transport viscous fluids, like fuel and lubricants, with much smaller energy losses."

The work is published in Science Advances as "A novel physical mechanism of liquid flow slippage on a solid surface."

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Science - Dyson developed and is producing ventilators to help treat COVID-19 patients

Dyson developed and is producing ventilators to help treat COVID-19 patients






The company plans to produce 15,000 ventilators

SPACE - S0 - 20200328 - What Will Happen to Trees, Galactic Halos, Flooding

SPACE - S0 - 20200328 - What Will Happen to Trees, Galactic Halos, Flooding

Good Morning, 0bservers!

   
    
We had a bit of wind variability in the last few hours when, after a drop down to around 360 KPS, there was a sudden jump due to some Phi Angle instability up to nearly 400 KPS, but has settled back into the 360-370 KPS range. Mostly KP-1s and KP-2s yesterday, but before and after midnight when the speed was dropping it went to KP-0 for two readings and it's back to KP-1s. X-ray flux is on the floor, and Electron flux is back under the threshold from Thursday's slight rise. The coronal hole system in the South passed the midpoint yesterday, and I'm not seeing any new hole formation in the offing. Indonesia had a quake about 80 miles NNW at Mag 5.6 and a Mag 5.0 100 miles NNW of Papua New Guinea was the only lithospheric activity of note yesterday, with a small scattering of blot echos to round out the picture.
   
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Friday, March 27, 2020

SPACE - S0 - 20200327 - Climate Controls, The Loss of Stability, The Sun

SPACE - S0 - 20200327 - Climate Controls, The Loss of Stability, The Sun

Good Morning, 0bservers!

   
    
Solar winds stayed mostly stable from yesterday, staying in the 380-410 KPS range throughout the period. The Phi-Angle is still jumping around quite a bit, but it's not being reflected in either wind speed or magnetic instability, as the KP Index stays well within the safe zone. The Electron Flux again bumped above the 10² threshold yesterday mid-morning, but dropped well below that with some rather "squiggly" readings between 10² and 10¹ after midnight. The main Southern coronal hole passed the midpoint just a couple hours ago, but no new holes seem to be developing behind them. Also no bright spot activity of note. A more active lithosphere (comparatively) yesterday, with a Mag 6.1 blot echo near the Philippines, a Mag 5.0 a bit west of Mentone Texas, a Mag 5.8 just over 100 miles WSW of Indonesia, and a Mag 5.3 about 70 miles SSE of Kuh Sefid, Iran.
   
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Thursday, March 26, 2020

A wearable, freestanding electrochemical sensing system

MARCH 26, 2020 FEATURE, by Thamarasee Jeewandara , Phys.org
https://phys.org/news/2020-03-wearable-freestanding-electrochemical.html

FESS design rationale, implementation, and application. (A) Schematic of the biomarker information delivery pathway enabled by the FESS, illustrating sampling, sensing, and routing of epidermally retrieved biomarker information to readout electronics through a single entity. (B) Design rationale of the FESS. (C) Representative implementation of the FESS, demonstrating flexibility and no in-plane interconnection. (D) Representative family of FESS devices, containing 1 × 2, 3 × 3, and 6 × 6 electrode arrays. (E) Custom-developed and FESS-enabled smartwatch for biomarker monitoring. (F and G) Deployment of the FESS-enabled smartwatch in stationary (F) and high-intensity exercise (G) settings.
 (Photo credit: Peterson Nguyen, Kaili Chiu, Yichao Zhao, University of California, Los Angeles.) 
Credit: Science Advances, doi: 10.1126/sciadv.aaz0007

In a new study published on Science Advances, Yichao Zhao and a research team in integrated bioelectronics and materials and engineering in the U.S. engineered a disposable, free-standing electrochemical sensing system (FESS). The FESS allowed them to realize a system-level design strategy to address the challenges of wearable biosensors in the presence of motion and allow seamless integration with consumer electronics. The team developed a FESS-enabled smartwatch, featuring sweat sampling, electrochemical sensing and data display or transmission, within a self-contained wearable platform. The team used the FESS-smartwatch to monitor the profiles of sweat metabolites among individuals in sedentary and high-intensive exercise settings.

The internet-of-things (IOT) infrastructure can be used in wearable consumer electronics to transform personalized and precision medicine by harvesting physiologically relevant data with minimal user intervention. Scientists have typically used physical sensors in commercial wearable platforms to track a user's physical activity and vital signs. However, to gain insight into the body's dynamic chemistry, researchers require electrochemical sensing surfaces to target the biomarker molecules within non-invasively retrieved body fluids such as sweat. To accomplish this, it is critical to precisely engineer the information delivery pathway from the skin to a readout unit. For electrochemical sensing, the information delivery pathway must sample and deliver the biomarker-rich biofluid to the sensor surface in a microfluidic structure, followed by signal transduction through interconnected elements to the readout electronics. The signal must be maintained along this pathway in the presence of motion-induced strain.



Bio-inspired in situ sensing and signal interconnection. (A) Conceptual illustration of the physiological information exchange between intracellular/extracellular matrices facilitated by cell adhesive molecules (integrin) via sensing, out-of-plane signal interconnection, and double-sided adhesion. (B) In-situ sensing, out-of-plane signal interconnection, and double-sided adhesion enabled by FESS, as a single entity, placed between skin and electronics. Credit: Science Advances, doi: 10.1126/sciadv.aaz0007


In this work, Zhao et al. developed the freestanding electrochemical sensing system (FESS) and simultaneously adhered it to the skin and to electronics using double-sided adhesion forces without rigid connectors. The FESS sampled and directed epidermally retrieved biofluids for electrochemical sensing, followed by routing to readout electronics through a strain-isolated pathway. They integrated the FESS inside a custom-built smartwatch for sweat induction, sampling, .....


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