Tuesday, July 31, 2012

Nike's New Strobing Glasses Enhance Athletes' Visual Acuity and Sensory Skills


Nike SPARQ Vapor Strobe Eyewear Like glasses that help you see worse. NIKE
Nike has developed a means of increasing visual short-term memory retention and physical reaction time via a set of strobing goggles that rob athletes in training of some of their vision. The SPARQ Sensory Performance system evaluates an athlete for 10 visual performance skills and creates a training program specifically for him or her that involves wearing Nike’s SPARQ Vapor Strobe Eyewear, which basically fog over to block the wearer’s vision for short periods of time, forcing the athlete to anticipate what’s coming next.
The idea is to fine-tune an athlete’s sensory perception, visual acuity, and the brain’s ability to maintain a precise sense of timing absent a constant stream of visual input. The regimen is backed up by Duke University research that shows that the SPARQ system can indeed heighten visual skills and improve athletes’ reaction times. The system is apparently already in beta with some professional and collegiate sports programs, and will see a worldwide rollout soon.
It’s tough to say at this point how much that improvement translates to the playing field, but Nike isn’t the only entity out there looking for ways to groom the brain into a better tool for physical activity. DARPA and the DoD are constantly on the lookout for technological tools that will help soldiers stay more alert, improve physical reaction times, increase eye-hand coordination, and sharpen decision-making skills on the fly--so the implications for this technology beyond athletic training are certainly real.

Just A Week From Landing, Mars Rover Curiosity Makes Final Course Corrections


Mars Science Laboratory Aeroshell The Mars rover Curiosity is tucked inside this aeroshell, less than a week from landing on the Red Planet. NASA/JPL-Caltech
A week before its scheduled landing, the spacecraft carrying the Mars rover Curiosity is just about done arranging itself in space. There’s time for two more trajectory correction maneuvers, but the one the Mars Science Laboratory pulled off over the weekend should be the last nudge the spacecraft needs before entering the Martian atmosphere.
The spacecraft is designed to handle its own entry, descent and landing, so it can punch into Mars’ atmosphere a few miles away from its targeted landing site in Gale Crater. While its 15-foot heat shield protects the spacecraft and helps slow it down, it can automatically steer itself to correct for missing the target entry. But it would have been about 13 miles off, a little too far for comfort, which prompted NASA to make the trajectory change over the weekend. The adjustment changed MSL’s velocity by one centimeter per second, according to NASA.
Follow us on Twitter for the latest MSL updates, and stay tuned for live coverage of the landing from the Jet Propulsion Laboratory, just a few days from now.

Four-Ton Japanese Mega Bot Fires BBs At Smiling Humans

Kuratas via Plastic Pals
This boxy guy is called Kuratas, otherwise known as Vaudeville, and he stands 12 feet 5 inches tall. He weighs about 4.5 tons and is diesel-powered. Do not smile at him. He will shoot that grin right off your face.
Kuratas is a real-life mech from (where else?) Japan, and it's an art project designed by Suidobashi Heavy Industry. Iron worker/artist Kogoro Kurata, at right in the photo above, built his namesake robot and debuted it at something called Wonder Fest 2012, which took place over the weekend.
It has a ride-in cockpit, a master-slave joystick and a touchscreen interface, and its arms can be controlled via Kinect, so it could be trained as a champion boxer. Its twin BB Gatling guns can fire up to 6,000 BBs per minute, according to Plastic Pals. And it fires when a small camera inside the robot detects when you smile. This is just for fun, however — Kurata says he would never want his creation to harm anyone. But it could be used for robot competitions, he said.
You could pretend-order one of your own, via a slick website Kurata and his colleagues at Suidobashi designed. The mecha come in various color schemes and customizable weapons. But the base model starts at $1,353,500, so better start saving.

Billionaires: Russian Mogul Wants to Upload Your Brains Into Immortality


Avatar 2045 Goals 2045 Initiative
Earlier this year, a Russian media mogul named Dmitry Itskov formally announced his intention to disembody our conscious minds and upload them to a hologram--an avatar--by 2045. In other words he outlined a plan to achieve immortality, removing the human mind from the physical constraints presented by the biological human body. He was serious. And now, in a letter to the members of the Forbes World’s Billionaire’s List, he’s offering up that immortality to the world’s 1,266 richest people.
“Many of you who have accumulated great wealth by making success of your businesses are supporting science, the arts and charities. I urge you to take note of the vital importance of funding scientific development in the field of cybernetic immortality and the artificial body,” Itskov wrote in the letter. “Such research has the potential to free you, as well as the majority of all people on our planet, from disease, old age and even death.”
The 2045 Initiative claims to have hired 30 scientists to help it pursue its immortality goal. It is opening a San Francisco office this summer and launching a major social media effort to get scientists talking about cybernetic technologies. It’s hosting another Global Future Congress next year in New York City (the last one was in Moscow earlier this year). In other words, as crazy as this sounds Itskov is dead serious and the wheels are turning on this project.
The idea, as you can see above, is to incrementally move the human mind into more disembodied and--no better way to say it--futuristic vehicles: first a humanoid robot controlled entirely by a human brain via brain-machine interface, then a conscious human brain transplanted into a humanoid robot, then consciousness uploaded (sans biological gray matter) to a computer, and finally a hologram that contains a full conscious human mind.
Somehow. It seems far-fetched, but while that timeline seems ambitious we’re the last people that are going to say something is technologically impossible. If Itskov can rally the world’s richest to pay for the R&D, who knows what cool technology they might come up with--even the unintentional discoveries along the way could be mind blowing, even if offering immortality to the world’s richest people sounds something like the nefarious plot underpinning a comic book series. At least he’s asking them to invest in scientific achievement rather than investing in another billion.
“Currently you invest in business projects that will bring you yet another billion,” Itskov writes. “You also have the ability to finance the extension of your own life up to immortality. Our civilization has come very close to the creation of such technologies: it's not a science fiction fantasy. It is in your power to make sure that this goal will be achieved in your lifetime.”

How technology is going to make the 2020 Olympics better, safer, and more exciting

Summer Olympics: 2020 John MacNeill
The modern Olympics have been running for 116 years, but many events remain unsafe and difficult to score. We propose ideas that might help solve some of the toughest problems.

HOLOGRAPHIC OBSTACLES

About 100 riders are injured in eventing falls every year, and when a multimillion-dollar horse goes down, even a minor injury like a twisted ankle can end its career. Computerized bases on the ground could project holographic obstacles, such as four-foot fences and 15-foot-wide pools, in place of dangerous physical objects. Line-of-sight infrared beams could monitor the edges of the obstacles; if the horse breaks the beam, the system would instantly alert the judges—and the crowd—to the fault.

SMART LANDING PADS

Scoring the exact length of a long or triple jump can be imprecise and time-consuming. Athletes land in a sand pit, where they make several marks; officials must locate the mark closest to the takeoff line before they can measure. Researchers at Arizona State University have developed a 2,016-pressure-sensor array to map where an athlete hits the ground. Placed underneath the sand in the landing pit, a dozen or so of the mats could record the exact point of touchdown, and a computer could automatically calculate the length of the jump.

HEAD-UP GOGGLES

Swimmers are often unaware of their standing in a race until it’s over. Goggles with an integrated head-up display could broadcast a live view of the competition and help racers to better pace themselves. Waterproofed with an invisible layer of hydrophobic nanoparticles, a technique currently used on cellphones and other gadgets, a small computer tucked in the lower right-hand corner of the goggles would gather position information from other wired racers over Bluetooth and display it on a quarter-inch LCD.
Head-Up Goggles:  John MacNeill

AUTOMATIC GOAL KEEPER

In a low-scoring game like soccer, one bad goal call can do a lot of damage. A reversed call in a match against Germany, for example, cost the U.K. a potentially pivotal goal in the 2010 World Cup. To help refs, who may not always have a clear view of both the ball and net, German research institution Fraunhofer has developed an automated goal-tracking system. Actuators around the net generate a magnetic field across the face of the goal. When the ball passes through that field, a chip embedded in the ball sends a signal to the ref’s watch within one tenth of a second.

RETRACTABLE DIVING BOARD

On a good day, a diver’s head misses the board by a couple of inches. On a bad day, the two collide, as happened to American Chelsea Davis in the 2005 World Championships (she suffered a broken nose and needed several stitches) and, most famously, Greg Louganis in the 1988 Olympics. A hydraulic springboard could make diving safer. In the one second a typical diver is airborne above the plane of the board, it could retract as much as three feet. An accelerometer would sense each takeoff and initiate the movement.

Sunday, July 29, 2012

Own homemade satellite

"Making a satellite is no more difficult than making a cellphone," said Song Ho jun, 34, who said he built the $500 OpenSat to show people they could achieve their dreams.
"I believe that not just a satellite, but anything can be made with the help of the internet and social platforms. I chose a satellite to show that symbolically."
There's a long history of do-it-yourself satellites being launched by universities and scientific groups around the world, as well as amateur radio clubs, but Mr Song said his is the first truly personal satellite designed and financed by an individual.
An engineering student at university, Mr Song regularly incorporated technology into his art pieces. In a work called Apple he used light bulbs that would "ripen" – change colour from green to red when people take photos of it with flashes.
After working as an intern at a private satellite company, he came up with the idea for his "Open Satellite Initiative," which in turn led him to contact space professionals from Slovenia to Paris.
The bespectacled Mr Song spent nearly six years combing through academic papers, shopping online at sites that specialise in components that can be used for space projects, and rummaging through electronic stores hidden in the back alleys of Seoul.
He ran a small electronics business to support himself, but the bulk of his funds came from his parents.
(Reuters)
The cubical OpenSat weighs 1kg and measures 10 cubic centimetres. It will transmit information about the working status of its battery, the temperature and rotation speed of the satellite's solar panel.
Radio operators will be able to communicate with the satellite. If all goes well, it will repeat a message in Morse code using its LED lights at a set time and location.
The components cost only 500,000 won ($440). But the cost for launching it hit 120 million won after Song signed a contract with NovaNano, a French technology company, which acted as a broker to arrange the launch, including submitting paperwork and finding a rocket.
The satellite will be launched from the Baikonur Cosmodrome in Kazakhstan in December with another satellite.
Mr Song has been invited to talk at international universities and organisations including MIT Media Lab and CalArts, both in the United States, and the Royal College of Art in London.
"The reason why technology or science is talked about is not because it is an absolute truth, but rather because it generates interesting stories," he said. ($1 = 1146.9500 Korean won)

மருந்துக்கு கட்டுப்படாத எச்ஐவி தொற்று அதிகரிக்கிறது

மருந்துக்கு கட்டுப்படாத எச் ஐ வி தொற்று கிழக்கு ஆப்பிரிக்காவில் வேகமாக அதிகரித்துவருவதாக உலக சுகாதாரத்துறையின் ஆய்வு எச்சரித்திருக்கிறது.
உலக சுகாதார நிறுவனமும் லண்டன் பல்கலைக்கழக கல்லூரியும் இணைந்து செய்த ஆய்வின் படி கிழக்கு ஆப்ரிக்காவில் எச் ஐ வி வைரஸானது வேகமாக மருந்துக்கு கட்டுப்படாத தன்மையை அடைந்துவருவதாக தெரிய வந்திருக்கிறது.
உதாரணமாக அமெரிக்கா, பிரிட்டன் போன்ற பொருளாதார ரீதியில் வளர்ச்சியடைந்த நாடுகளில் எச் ஐ வி தொற்றுக்குள்ளானவர்களில் சுமார் 10 சதவீதத்திற்கும் குறைவானவர்களுக்கு மட்டுமே மருந்துக்கு கட்டுப்படாத தன்மை காணப்படும்.
அனால் கிழக்கு ஆப்ரிக்காவில் இப்படியானவர்களின் சதவீதம் 29 சதவீதமாக இருப்பதை கண்டுபிடித்த ஆய்வாளர்கள் இது ஆண்டுக்கு ஆண்டு வேகமாக அதிரித்துக்கொண்டிருப்பதாகவும் கண்டறிந்திருக்கிறார்கள்.
இந்த போக்கு இப்படியே போனால், கடந்த பத்து ஆண்டுகளாக எயிட்ஸ் மரணங்கள் தொடர்ந்து குறைந்துகொண்டே வரும் நிலைமை மாறி, மீண்டும் எயிட்ஸ் மரணங்கள் அதிகரிக்கும் ஆபத்து இருப்பதாகவும் இந்த ஆய்வை மேற்கொண்டவர்கள் எச்சரித்திருக்கிறார்கள்.
இவர்களின் எச்சரிக்கையில் உண்மை இருக்கிறது என்கிறார் தமிழ்நாடு எயிட்ஸ் கட்டுப்பாட்டு வாரியத்தின் எச் ஐ வி மருந்துகளை கையாளும் சிறப்பு நிபுணர் மருத்துவர் வளன். எயிட்ஸ் நோயை தோற்றுவிக்கும் எச்ஐவி வைரஸுக்கான முறையான மருந்துகளை, சரியான நேரத்தில் சாப்பிடாமலிருப்பது எச் ஐ வி வைரஸின் தீவிரத்தன்மையை அதிகப்படுத்திவருகிறது என்கிறார் அவர்.

'எச் ஐ வியை முழுமையாக குணமாக்கும் சாத்தியம்'

எச் ஐ வி வைரஸை முழுமையாக குணப்படுத்தக்கூடிய சாத்தியப்பாட்டிற்கான முதல் படியை தாங்கள் எட்டியிருப்பதாக அமெரிக்க விஞ்ஞானிகள் அறிவித்திருக்கிறார்கள்.
எச் ஐ வி வைரஸானது மனித உடலுக்குள் புகுந்ததும் உடனடியாக தாக்குவதில்லை. மனித உடலில் சில செல்களுக்குள் புகுந்துகொண்டு செயற்படாமல் மறைந்து ஒளிந்துகொள்கிறது. இப்படியான நிலையில் இந்த எச் ஐ வி வைரஸானது பல ஆண்டுகள் மறைவாக இருக்க முடியும்.
இப்படி செல்களுக்குள் புகுந்துகொண்ட நிலையில் இருக்கும் எச் ஐ வி வைரஸை கண்டுபிடிக்கவே முடியாது. குறிப்பாக மனித உடலின் நோய் எதிர்ப்பு செல்களாலோ, எச் ஐ வி தொற்றுக்கு எதிரான ஆண்டி ரெட்ரோ வைரல் மருந்துகளாலோ இப்படியான வைரஸை கண்டுபிடித்து தாக்கமுடியாது. இதனால்தான் இன்றுவரை எச் ஐ வி தொற்றை முழுமையாக அழிக்கக்கூடிய மருந்துகளை கண்டுபிடிக்க முடியாத நிலை நிலவுகிறது.
இப்படி மறைந்திருக்கும் எச் ஐ வி வைரஸ்கள் திடீரென்று ஒருநாள் தான் ஒளிந்துகொண்டிருக்கும் செல்லிலிருந்து வெளியே வந்து மனிதனை தாக்கத்துவங்கும் நிலை இருப்பதால் தான் இன்றுவரை எச் ஐ வி தொற்றை முழுமையாக குணப்படுத்த முடியாத நிலை நிலவுகிறது. இந்த நிலைமையை மாற்ற முடியும் என்கிறார்கள் அமெரிக்க விஞ்ஞானிகள்.
மறைந்திருக்கும் எச் ஐ வி வைரஸை பலவந்தமாக வெளியே கொண்டுவந்து, அதை தாக்கி அழிக்கமுடியும் என்று இந்த ஆய்வை மேற்கொண்ட விஞ்ஞானிகள் நேச்சர் என்கிற விஞ்ஞான சஞ்சிகையில் தெரிவித்திருக்கிறார்கள்.
புற்றுநோய் மருந்து உதவும்
புற்றுநோய்க்கான மருந்தாக பயன்படுத்தப்படும் மருந்துகளில் ஒன்று ஒரினோஸ்டாட். இந்த மருந்தை எச் ஐ வி தொற்றுக்கு உள்ளானவர்களுக்கு கொடுப்பதன்மூலம், செல்களுக்குள் மறைந்திருக்கும் எச் ஐ வி வைரஸ் பலவந்தமாக அந்த செல்களில் இருந்து வெளியேற்றப்படுகிறது. இப்படி வெளியே வந்த செல்களை ஆண்டி ரெட்ரோ வைரல் மருந்துகள் தாக்கி அழித்துவிடுகின்றன.
இதற்கான முதற்கட்ட பரிசோதனைகள் எச் ஐ வி தொற்றுக்குள்ளான எட்டு பேரிடம் நடத்தப்பட்டன. இவர்களுக்கு ஒரே ஒருமுறை புற்றுநோய்க்கு எதிரான மருந்தான ஒரினோஸ்டாட் மருந்து அளிக்கப்பட்டதும், அவர்களின் உடலின் செல்களில் ஒளிந்திருந்த எச் ஐ வி வைரஸ்கள் எல்லாமே பலவந்தமாக வெளியே வந்தன. இந்த எதிர்வினை தங்களின் கண்டிபிடிப்பை உறுதி செய்திருப்பதாக கூறுகிறார் இந்த சோதனைகளை நடத்திய விஞ்ஞானிகள் குழுமத்தின் தலைமை விஞ்ஞானி டேவிட் மார்கோலிஸ்.
'ஆனால் நீண்ட காலம் பிடிக்கும்'
''மறைந்திருக்கும் எச் ஐ வி வைரஸை குறிவைத்து தாக்கவும், காலப்போக்கில் அழிக்கவும் கூடிய வழிகளை நாம் கண்டறியத் துவங்கியிருக்கிறோம். இப்படி ஒரு மனிதனின் உடலில் மறைந்திருக்கும் எச் ஐ வி வைரஸ்கள் அனைத்தையும் நாம் அழித்துவிட்டோமானால், நாம் அந்த நபரை எச் ஐ வி வைரஸ் தொற்றிலிருந்து முழுமையாக குணப்படுத்திவிட்டோம் என்று கூறமுடியும்'' என்கிறார் டேவிட் மார்கோலிஸ்.
உலகம் முழுவதும் எச் ஐ வி வைரஸால் பாதிக்கப்பட்ட லட்சக்கணக்கானவர்களுக்கு இது மிகப்பெரிய நம்பிக்கையளிக்கும் செய்தி. எச் ஐ வி தொற்றுக்குள்ளானவர்களுக்கு தற்போது அளிக்கப்படும் ஆண்டி ரெட்ரோவைரல் மருந்துகள் அவர்களின் தொற்றை கட்டுபடுத்தி அவர்களின் ஆயுளை நீட்டிக்க உதவுகின்றன. இதன் விளைவாக, எச் ஐ வி தொற்று ஏற்பட்டாலே உடனடி மரணம் என்கிற ஆரம்பகால ஆபத்து இப்போது இல்லை. இந்த பின்னணியில் இதை முழுமையாக குணப்படுத்த முடியும் என்கிற நம்பிக்கையை இந்த குறிப்பிட்ட ஆய்வின் முடிவுகள் முதல்முறையாக உண்டாக்குவதாகவும், இது ஒரு திருப்புமுனையாக இருக்கலாம் என்றும் கூறுகிறார் மருத்துவர் டேவிட் மார்கோலிஸ்.
ஆனால் இவரது இந்த எதிர்பார்ப்புகள் உண்மையாக நடைமுறைக்கு வருவதற்கு பல ஆண்டுகள் பிடிக்கலாம். எச் ஐ வி வைரஸை முழுமையாக அழித்து ஒழிக்கவல்ல நிலையை எட்டுவதற்கு மேலதிக ஆய்வுகள் தேவை. அதை மேற்கொள்வதற்கான ஊக்கத்தை இந்த ஆரம்பகட்ட முடிவுகள் அளித்திருக்கின்றன

Thursday, July 26, 2012

Researchers Produce First Complete Computer Model of an Organism

A team led by Markus Covert, assistant professor of bioengineering, used data from more than 900 scientific papers to account for every molecular interaction that takes place in the life cycle of Mycoplasma genitalium, the world's smallest free-living bacterium.
By encompassing the entirety of an organism in silico, the paper fulfills a longstanding goal for the field. Not only does the model allow researchers to address questions that aren't practical to examine otherwise, it represents a stepping-stone toward the use of computer-aided design in bioengineering and medicine.
"This achievement demonstrates a transforming approach to answering questions about fundamental biological processes," said James M. Anderson, director of the National Institutes of Health Division of Program Coordination, Planning and Strategic Initiatives. "Comprehensive computer models of entire cells have the potential to advance our understanding of cellular function and, ultimately, to inform new approaches for the diagnosis and treatment of disease."
The research was partially funded by an NIH Director's Pioneer Award from the National Institutes of Health Common Fund.
From information to understanding
Biology over the past two decades has been marked by the rise of high-throughput studies producing enormous troves of cellular information. A lack of experimental data is no longer the primary limiting factor for researchers. Instead, it's how to make sense of what they already know.
Most biological experiments, however, still take a reductionist approach to this vast array of data: knocking out a single gene and seeing what happens.
"Many of the issues we're interested in aren't single-gene problems," said Covert. "They're the complex result of hundreds or thousands of genes interacting."
This situation has resulted in a yawning gap between information and understanding that can only be addressed by "bringing all of that data into one place and seeing how it fits together," according to Stanford bioengineering graduate student and co-first author Jayodita Sanghvi.
Integrative computational models clarify data sets whose sheer size would otherwise place them outside human ken.
"You don't really understand how something works until you can reproduce it yourself," Sanghvi said.
Small is beautiful
Mycoplasma genitalium is a humble parasitic bacterium known mainly for showing up uninvited in human urogenital and respiratory tracts. But the pathogen also has the distinction of containing the smallest genome of any free-living organism -- only 525 genes, as opposed to the 4,288 of E. coli, a more traditional laboratory bacterium.
Despite the difficulty of working with this sexually transmitted parasite, the minimalism of its genome has made it the focus of several recent bioengineering efforts. Notably, these include the J. Craig Venter Institute's 2008 synthesis of the first artificial chromosome.
"The goal hasn't only been to understand M. genitalium better," said co-first author and Stanford biophysics graduate student Jonathan Karr. "It's to understand biology generally."
Even at this small scale, the quantity of data that the Stanford researchers incorporated into the virtual cell's code was enormous. The final model made use of more than 1,900 experimentally determined parameters.
To integrate these disparate data points into a unified machine, the researchers modeled individual biological processes as 28 separate "modules," each governed by its own algorithm. These modules then communicated to each other after every time step, making for a unified whole that closely matched M. genitalium's real-world behavior.
Probing the silicon cell
The purely computational cell opens up procedures that would be difficult to perform in an actual organism, as well as opportunities to reexamine experimental data.
In the paper, the model is used to demonstrate a number of these approaches, including detailed investigations of DNA-binding protein dynamics and the identification of new gene functions.
The program also allowed the researchers to address aspects of cell behavior that emerge from vast numbers of interacting factors.
The researchers had noticed, for instance, that the length of individual stages in the cell cycle varied from cell to cell, while the length of the overall cycle was much more consistent. Consulting the model, the researchers hypothesized that the overall cell cycle's lack of variation was the result of a built-in negative feedback mechanism.
Cells that took longer to begin DNA replication had time to amass a large pool of free nucleotides. The actual replication step, which uses these nucleotides to form new DNA strands, then passed relatively quickly. Cells that went through the initial step quicker, on the other hand, had no nucleotide surplus. Replication ended up slowing to the rate of nucleotide production.
These kinds of findings remain hypotheses until they're confirmed by real-world experiments, but they promise to accelerate the process of scientific inquiry.
"If you use a model to guide your experiments, you're going to discover things faster. We've shown that time and time again," said Covert.
Bio-CAD
Much of the model's future promise lies in more applied fields.
CAD -- computer-aided design -- has revolutionized fields from aeronautics to civil engineering by drastically reducing the trial-and-error involved in design. But our incomplete understanding of even the simplest biological systems has meant that CAD hasn't yet found a place in bioengineering.
Computational models like that of M. genitalium could bring rational design to biology -- allowing not only for computer-guided experimental regimes, but also for the wholesale creation of new microorganisms.
Once similar models have been devised for more experimentally tractable organisms, Karr envisions bacteria or yeast specifically designed to mass-produce pharmaceuticals.
Bio-CAD could also lead to enticing medical advances -- especially in the field of personalized medicine. But these applications are a long way off, the researchers said.
"This is potentially the new Human Genome Project," Karr said. "It's going to take a really large community effort to get close to a human model."
Stanford's Department of Bioengineering is jointly operated by the School of Engineering and the School of Medicine.

Sweat Glands Grown from Stem Cells

fundamentals have been known about the most common gland in the body, the sweat glands that are essential to controlling body temperature, allowing humans to live in the world’s diverse climates. Now, in a tour de force, researchers at The Rockefeller University and the Howard Hughes Medical Institute have identified, in mice, the stem cell from which sweat glands initially develop as well as stem cells that regenerate adult sweat glands.

In their study, published in Cell, the scientists devised a strategy to purify and molecularly characterize the different kinds of stem cell populations that make up the complex sweat duct and glands of the skin. With this information in hand, they studied how these different populations of stem cells respond to normal tissue homeostasis and to different types of skin injuries, and how the sweat glands differ from their close cousins, the mammary glands.



No sweat. Researchers in Elaine Fuchs's lab identified four different types of paw-skin progenitor cells that are responsible for homeostasis and wound repair. This image shows that the sweat ductal and epidermal progenitors (in red) proliferate and repair an epidermal scratch wound; the sweat gland progenitors (in blue and green) show no signs of proliferation to this type of wound, but instead respond to deep glandular wounds.

“Mammary gland stem cells respond to hormonal induction by greatly expanding glandular tissue to increase milk production,” explains Elaine Fuchs, Rebecca C. Lancefield Professor at Rockefeller and an investigator at the Howard Hughes Medical Institute. “In contrast, during a marathon race, sweat gland stem cells remain largely dormant, and glandular output rather than tissue expansion accounts for the 3 liters of sweat our body needs. These fascinating differences in stem cell activity and tissue production are likely at the root why breast cancers are so frequent, while sweat gland cancers are rare.” Their findings might also help in the future to improve treatments for burn patients and to develop topical treatments for people who sweat too much, or too little.

“For now, the study represents a baby step towards these clinical goals, but a giant leap forward in our understanding of sweat glands,” says the study’s lead author, Catherine P. Lu, a postdoctoral researcher in Fuchs’s Laboratory of Mammalian Cell Biology and Development.


Each human has millions of sweat glands but they have rarely been extensively studied possibly due to the difficulty of gathering enough of the tiny organs to research in a lab, says Lu. The mouse is traditionally used as a model for human sweat gland studies, so in this project, Lu and colleagues laboriously extracted sweat glands from the tiny paw pads of mice, the only place they are found in these and most other mammals.


The research team sought to discover whether the different cells that make up the sweat gland and duct contained stem (progenitor) cells, which can help repair damaged adult glands. “We didn’t know if sweat stem cells exist at all, and if they do, where they are and how they behave,” she says. The last major studies on proliferative potential within sweat glands and sweat ducts were conducted in the early 1950s before modern biomedical techniques were used to understand fundamental bioscience.


Fuchs’ team determined that just before birth, the nascent sweat duct forms as a downgrowth from progenitor cells in the epidermis, the same master cells that at different body sites give rise to mammary glands, hair follicles and many other epithelial appendages. As each duct grows deeper into the skin, a sweat gland emerges from its base.


Lu then led the effort to look for stem cells in the adult sweat gland. The gland is made up of two layers -- an inner layer of luminal cells that produce the sweat and an outer layer of myoepithelial cells that squeeze the duct to discharge the sweat.


Lu devised a strategy to fluorescently tag and sort the different populations of ductal and glandular cells. The Fuchs team then injected each population of purified cells into different body areas of female host recipient mice to see what the cells would do.


Interestingly, when introduced into the mammary fat pads, the sweat gland myoepithelial cells generated fluorescent sweat gland-like structures. “Each fluorescent gland had the proper polarized distribution of myoepithelial and luminal cells, and they also produced sodium potassium channel proteins that are normally expressed in adult sweat glands but not mammary glands,” Lu says.


Intriguingly, when the host mice were put through pregnancy, some of the fluorescent sweat glands began to express milk, while still retaining some sweat gland features as well. Even more surprising was that sweat gland myoepithelial cells produced epidermis when engrafted to the back skin of the mice.


“Taken together, these findings tell us that adult glandular stem cells have certain intrinsic features that enable them to remember who they are in some environments, but adopt new identities in other environments,” Fuchs says. “To test the possible clinical implications of our findings, we would need to determine how long these foreign tissues made by the stem cells will last — unless it is long-term, a short-term “fix” might only be useful as a temporary bandage for regenerative medicine purposes,” Fuchs cautions.


Irrespective of whether the knowledge is yet prime-time for the clinics, the findings can now be used to explore the roots of some genetic disorders that affect sweat glands, as well as ways to potential ways to treat them. “We have just laid down some critical fundamentals of sweat gland and sweat duct biology,” Lu says. “Our study not only illustrates how sweat glands develop and how their cells respond to injury, but also identifies the stem cells within the sweat glands and sweat ducts and begins to explore their potential for making tissues for the first time.”


The study was supported by grants from the Stem Cell Research and Starr Foundation and from the National Institutes of Health. Researchers from the Université Libre de Bruxelles, in Belgium, and from St. Jude Children’s Research Hospital in Tennessee contributed to the study.

 

Solar Corona Revealed in Super-High-Definition

"Even though this mission was only a few minutes long, it marks a big breakthrough in coronal studies," said Smithsonian astronomer Leon Golub (Harvard-Smithsonian Center for Astrophysics), one of the lead investigators on the mission.
Understanding the Sun's activity and its effects on Earth's environment was the critical scientific objective of Hi-C, which provided unprecedented views of the dynamic activity and structure in the solar atmosphere.
The corona surrounds the visible surface of the Sun. It's filled with million-degree ionized gas, or plasma, so hot that the light it emits is mainly at X-ray and extreme-ultraviolet wavelengths. For decades, solar scientists have been trying to understand why the corona is so hot, and why it erupts in violent solar flares and related blasts known as "coronal mass ejections," which can produce harmful effects when they hit Earth. The Hi-C telescope was designed and built to see the extremely fine structures thought to be responsible for the Sun's dynamic behavior.
"The phrase 'think globally, act locally' applies to the Sun too. Things happening at a small, local scale can impact the entire Sun and result in an eruption," explained Golub.
Hi-C focused on an active region on the Sun near sunspot NOAA 1520. The target, which was finalized on launch day, was selected specifically for its large size and active nature. The resulting high-resolution snapshots, at a wavelength of 19.3 nanometers (25 times shorter than the wavelength of visible light), reveal tangled magnetic fields channeling the solar plasma into a range of complex structures.
"We have an exceptional instrument and launched at the right time," said Jonathan Cirtain, senior heliophysicist at NASA's Marshall Space Flight Center. "Because of the intense solar activity we're seeing right now, we were able to clearly focus on a sizeable, active sunspot and achieve our imaging goals."
Since Hi-C rode on a suborbital rocket, its flight lasted for just 10 minutes. Of that time, only about 330 seconds were spent taking data. Yet those images contain a wealth of information that astronomers will analyze for months to come.
"The Hi-C flight might be the most productive five minutes I've ever spent," Golub smiled.
The high-resolution images were made possible because of a set of innovations on Hi-C's telescope, which directs light to the camera detector. The telescope includes some of the finest mirrors ever made for a space mission. Initially developed at NASA's Marshall Space Flight Center in Huntsville, Ala., the mirrors were completed with inputs from partners at the Smithsonian Astrophysical Observatory (SAO) in Cambridge, Mass., and a new manufacturing technique developed in coordination with L-3Com/Tinsley Laboratories of Richmond, Calif. The mirrors were made to reflect extreme-ultraviolet light from the Sun by Reflective X-ray Optics LLC of New York, NY, and the telescope was assembled at the SAO labs in Cambridge, Mass.

Wednesday, July 25, 2012

Highly Transparent Solar Cells for Windows That Generate Electricity

The UCLA team describes a new kind of polymer solar cell (PSC) that produces energy by absorbing mainly infrared light, not visible light, making the cells nearly 70% transparent to the human eye. They made the device from a photoactive plastic that converts infrared light into an electrical current.
"These results open the potential for visibly transparent polymer solar cells as add-on components of portable electronics, smart windows and building-integrated photovoltaics and in other applications," said study leader Yang Yang, a UCLA professor of materials science and engineering, who also is director of the Nano Renewable Energy Center at California NanoSystems Institute (CNSI).
Yang added that there has been intense world-wide interest in so-called polymer solar cells. "Our new PSCs are made from plastic-like materials and are lightweight and flexible," he said. "More importantly, they can be produced in high volume at low cost."
Polymer solar cells have attracted great attention due to their advantages over competing solar cell technologies. Scientists have also been intensely investigating PSCs for their potential in making unique advances for broader applications. Several such applications would be enabled by high-performance visibly transparent photovoltaic (PV) devices, including building-integrated photovoltaics and integrated PV chargers for portable electronics.
Previously, many attempts have been made toward demonstrating visibly transparent or semitransparent PSCs. However, these demonstrations often result in low visible light transparency and/or low device efficiency because suitable polymeric PV materials and efficient transparent conductors were not well deployed in device design and fabrication.
A team of UCLA researchers from the California NanoSystems Institute, the UCLA Henry Samueli School of Engineering and Applied Science and UCLA's Department of Chemistry and Biochemistry have demonstrated high-performance, solution-processed, visibly transparent polymer solar cells through the incorporation of near-infrared light-sensitive polymer and using silver nanowire composite films as the top transparent electrode. The near-infrared photoactive polymer absorbs more near-infrared light but is less sensitive to visible light, balancing solar cell performance and transparency in the visible wavelength region.
Another breakthrough is the transparent conductor made of a mixture of silver nanowire and titanium dioxide nanoparticles, which was able to replace the opaque metal electrode used in the past. This composite electrode also allows the solar cells to be fabricated economically by solution processing. With this combination, 4% power-conversion efficiency for solution-processed and visibly transparent polymer solar cells has been achieved.
"We are excited by this new invention on transparent solar cells, which applied our recent advances in transparent conducting windows (also published in ACS Nano) to fabricate these devices," said Paul S.Weiss, CNSI director and Fred Kavli Chair in NanoSystems Sciences.
Study authors also include Weiss; materials science and engineering postdoctoral researcher Rui Zhu; Ph.D. candidates Chun-Chao Chen, Letian Dou, Choong-Heui Chung, Tze-Bin Song and Steve Hawks; Gang Li, who is former vice president of engineering for Solarmer Energy, Inc., a startup from UCLA; and CNSI postdoctoral researcher Yue Bing Zheng.

River Networks On Saturn's Largest Moon, Titan, Point to a Puzzling Geologic History

In 2004, the Cassini-Huygens spacecraft -- a probe that flies by Titan as it orbits Saturn -- penetrated Titan's haze, providing scientists with their first detailed images of the surface. Radar images revealed an icy terrain carved out over millions of years by rivers of liquid methane, similar to how rivers of water have etched into Earth's rocky continents.
While images of Titan have revealed its present landscape, very little is known about its geologic past. Now researchers at MIT and the University of Tennessee at Knoxville have analyzed images of Titan's river networks and determined that in some regions, rivers have created surprisingly little erosion. The researchers say there are two possible explanations: either erosion on Titan is extremely slow, or some other recent phenomena may have wiped out older riverbeds and landforms.
"It's a surface that should have eroded much more than what we're seeing, if the river networks have been active for a long time," says Taylor Perron, the Cecil and Ida Green Assistant Professor of Geology at MIT. "It raises some very interesting questions about what has been happening on Titan in the last billion years."
A paper detailing the group's findings will appear in the Journal of Geophysical Research-Planets.
What accounts for a low crater count?
Compared to most moons in our solar system, Titan is relatively smooth, with few craters pockmarking its facade. Titan is around four billion years old, about the same age as the rest of the solar system. But judging by the number of craters, one might estimate that its surface is much younger, between 100 million and one billion years old.
What might explain this moon's low crater count? Perron says the answer may be similar to what happens on Earth.
"We don't have many impact craters on Earth," Perron says. "People flock to them because they're so few, and one explanation is that Earth's continents are always eroding or being covered with sediment. That may be the case on Titan, too."
For example, plate tectonics, erupting volcanoes, advancing glaciers and river networks have all reshaped Earth's surface over billions of years. On Titan, similar processes -- tectonic upheaval, icy lava eruptions, erosion and sedimentation by rivers -- may be at work.
But identifying which of these geological phenomena may have modified Titan's surface is a significant challenge. Images generated by the Cassini spacecraft, similar to aerial photos but with much coarser resolution, are flat, depicting terrain from a bird's-eye perspective, with no information about a landform's elevation or depth.
"It's an interesting challenge," Perron says. "It's almost like we were thrown back a few centuries, before there were many topographic maps, and we only had maps showing where the rivers are."
Charting a river's evolution
Perron and MIT graduate student Benjamin Black set out to determine the extent to which river networks may have renewed Titan's surface. The team analyzed images taken from Cassini-Huygens, and mapped 52 prominent river networks from four regions on Titan. The researchers compared the images with a model of river network evolution developed by Perron. This model depicts the evolution of a river over time, given variables such as the strength of the underlying material and the rate of flow through the river channels. As a river erodes slowly through the ice, it transforms from a long, spindly thread into a dense, treelike network of tributaries.
Black compared his measurements of Titan's river networks with the model, and found the moon's rivers most resembled the early stages of a typical terrestrial river's evolution. The observations indicate that rivers in some regions have caused very little erosion, and hence very little modification of Titan's surface.
"They're more on the long and spindly side," Black says. "You do see some full and branching networks, and that's tantalizing, because if we get more data, it will be interesting to know whether there really are regional differences."
Going a step further, Black compared Titan's images with recently renewed landscapes on Earth, including volcanic terrain on the island of Kauai and recently glaciated landscapes in North America. The river networks in those locations are similar in form to those on Titan, suggesting that geologic processes may have reshaped the moon's icy surface in the recent past.
"It's a weirdly Earth-like place, even with this exotic combination of materials and temperatures," Perron says. "And so you can still say something definitive about the erosion. It's the same physics."
This research was supported by NASA's Cassini Data Analysis Program.

'Seeds' of Massive Black Holes Found at the Center of the Milky Way Galaxy

Many galaxies contain enormous amounts of molecular gas in small areas near their nuclei. Highly condensed molecular gas is a birthplace of lots of stars. Moreover, it is considered to closely relate to activities of galactic nuclei. Therefore, it is important to investigate the physical state and chemical properties of molecular gas at galaxy centers through observation. To obtain detailed observation data, it is best to survey the center of the Milky Way Galaxy in which our solar system exists.
                         The research team observed emission lines at wavelengths of 0.87 mm, emitted from carbon monoxide molecules in an area of several degrees that includes the center of the Milky Way Galaxy. The ASTE 10 m telescope in the Atacama Desert (4,800 meters above sea level) of Chile was used for observation. More than 250 hours in total were spent on the prolonged observation from 2005 to 2010.
The research team compared this observation data with data of emission lines at wavelengths of 2.6 mm, emitted from carbon monoxide molecules in the same area, which were obtained using the NRO 45m Telescope (Note: 1). When intensity values of emission lines at different wavelengths, emitted from carbon monoxide molecules, are compared, it is possible to estimate temperature and density of molecular gas. In this way, the research team succeeded in drawing detailed distribution maps of "warm, dense" molecular gas of more than 50 degrees Kelvin and more than 10,000 hydrogen molecules per cubic centimeter at the center of the Milky Way Galaxy for the first time ever.
Oka, the research team leader, said, "The results are astonishing." The "warm, dense" molecular gas in that area is concentrated in four clumps (Sgr A, L=+1.3°, L=-0.4°, L=-1.2°). Moreover, it turns out that these four gas clumps are all moving at a very fast speed of more than 100 km/s. Sgr A, one of the four gas clumps, contains "Sagittarius A*," the nucleus of the Milky Way Galaxy. Oka added, "The remaining three gas clumps are objects we discovered for the very first time. It is thought that 'Sagittarius A*' is the location of a supermassive black hole that is approximately 4 million times the mass of the sun. It can be inferred that the gas clump 'Sgr A' has a disk-shaped structure with radius of 25 light-years and revolves around the supermassive black hole at a very fast speed."
On the other hand, the team found signs of expansion other than rotation in the remaining three gas clumps. This means that the gas clumps, L=+1.3°, L=-0.4°and L=-1.2°, have structures that were formed by supernova explosions that occurred within the gas clumps. The gas clump "L=+1.3°" has the largest amount of expansion energy. Its expanding energy is equivalent to 200 supernova explosions. The age of the gas masses is estimated as approximately 60,000 years old. Therefore, given that the energy source is the supernova explosions, the supernova explosions have continued to occur every 300 years.
The research team used the NRO 45m Telescope again to further examine the molecular gas's distribution, motion and composition to determine whether supernova explosions caused the expansion. "Observation clearly showed that the energy source of L=+1.3° is multiple supernova explosions. We detected multiple expansion structures and molecules attributed to shock waves," Oka said about the excitement when observing it. "Based on the observation of L=+1.3°, it is also natural to think that the expanding gas clumps L=-0.4° and L=-1.2° derived energy from multiple supernova explosions," Oka added.
A supernova explosion is a huge explosion that occurs when a star with more massive than eight to ten times the mass of the sun ends its life. Such a high occurrence of supernova explosions (once per 300 years) indicates that many young, massive stars are concentrated in the gas clumps. In other words, this means that there is a massive "star cluster" in each gas clump. Based on the frequency of the supernova explosions, the team estimated the mass of the star cluster buried in L=+1.3°as more than 100,000 times the mass of the sun, which is equivalent to that of the largest star cluster found in the Milky Way Galaxy.
As just described, the star cluster is huge, but it had not been discovered until now. "The solar system is located at the edge of the Milky Way Galaxy's disk, and is about 30,000 light-years away from the center of the Milky Way Galaxy. The huge amount of gas and dust lying between the solar system and the center of the Milky Way Galaxy prevent not only visible light, but also infrared light, from reaching the Earth. Moreover, innumerable stars in the bulge and disc of the Milky Way Galaxy lie in the line of sight. Therefore, no matter how large the star cluster is, it is very difficult to directly see the star cluster at the center of the Milky Way Galaxy," Oka explained.
"Huge star clusters at the center of the Milky Way Galaxy have an important role related to formation and growth of the Milky Way Galaxy's nucleus," said Oka. According to theoretical calculations, when the density of stars at the center of star clusters increases, the stars are merged together, one after another. Then, it is expected that IMBHs with several hundred times the mass of the sun are formed. Eventually, these IMBHs and star clusters sink into the nucleus of the Milky Way Galaxy. It can be thought that the IMBHs and star clusters are then merged further, and form a massive black hole at the Milky Way Galaxy's nucleus. Alternatively, the IMBHs and star clusters could help expand an existing massive black hole.
It can be thought that the supermassive black hole at "Sagittarius A*," the nucleus of the Milky Way Galaxy, has also been grown up through these processes. In summary, the new discovery is the finding of "cradles" of IMBHs that become "seeds" of the supermassive black hole at the nucleus.
"We would like to observe IMBHs in the star cluster. Actually, our observation data has already indicated traces of IMBHs," Oka said. One of the newly discovered gas masses, "L=-0.4°," contains two small gas clumps moving at a very fast speeds. If it is confirmed that these small gas clumps are rotating, it can be inferred that there are "invisible huge masses" at the center of the gas clumps. These "invisible huge masses" are likely to be IMBHs hidden in the center of the star cluster. Professor Oka expects developments in future research, saying, "In order to confirm the existence of IMBHs, we are planning to conduct further observations. The new discovery is an important step toward unraveling the formation and growth mechanism of the supermassive black hole at the Milky Way Galaxy's nucleus, which is a top-priority issue in galactic physics."

Hundreds of Random Mutations in Leukemia Linked to Aging, Not Cancer

Scientists at Washington University School of Medicine in St. Louis have found that even in healthy people, stem cells in the blood routinely accumulate new mutations over the course of a person's lifetime. And their research shows that in many cases only two or three additional genetic changes are required to transform a normal blood cell already dotted with mutations into acute myeloid leukemia (AML).
The research is published July 20 in the journal Cell.
"Now we have a very accurate picture of how acute leukemia develops," says senior author Richard K. Wilson, PhD, director of The Genome Institute at Washington University. "It's not hundreds of mutations that are important but only a few in each patient that push a normal cell to become a cancer cell. Finding these mutations will be important for identifying targeted therapies that can knock down a patient's cancer."
The study is the first to investigate how often mutations typically develop in healthy stem cells in the blood. These immature cells in the bone marrow give rise to all the blood cells in the body.
AML is a blood cancer that develops when too many immature blood cells crowd out the healthy cells. In recent years, Washington University researchers at the Siteman Cancer Center at Barnes-Jewish Hospital and Washington University School of Medicine have sequenced the genomes of 200 patients with AML to try to understand the mutations at the root of the disease.
Without fail, each patient's leukemia cells held hundreds of mutations, posing a conundrum for scientists, who have long believed that all the mutations in a cancer cell are likely to be important for the disease to progress.
"But we knew all of these mutations couldn't be important," says co-first author Daniel Link, MD, professor of medicine. "It didn't make any sense to us that so many mutations were present in all the cells in the tumor."
To investigate the origin of these mutations, the researchers isolated blood stem cells from healthy people of different ages. The youngest were newborns, and the oldest was in his 70s.
Every person has about 10,000 blood stem cells in their bone marrow, and the researchers found that each stem cell acquires about 10 mutations over the course of a year. By age 50, a person has accumulated nearly 500 mutations in every blood stem cell.
"Mutations are known to develop in cells as we age, but no one had any idea how many mutations occur in blood stem cells and how frequently they develop," Link says. "These random, background mutations occur during cell division and are unrelated to cancer. Our DNA can tolerate a huge number of these hits without any negative consequences. But if a cancer-initiating event occurs in one of these stem cells, it captures the genetic history of that cell, including the earlier mutations, and drives leukemia to develop."
As part of the study, the researchers sequenced the genomes of 24 patients with AML and compared the mutations in their leukemia cells to those that occurred in the blood stem cells of the healthy individuals. The scientists were surprised to see that the total number of mutations varied by age, not by whether a patient had leukemia. Thus, a healthy person in his 40s had just about the same number of mutations in his blood stem cells as a leukemia patient of the same age had in his cancer cells.
The study's results help to explain why leukemia occurs more frequently as people age.
"AML is relatively uncommon until about age 60," says co-first author John Welch, MD, PhD, assistant professor of medicine. "It is the persistent, random accumulation of mutations in blood stem cells that contributes to the risk of the disease."
By sequencing the genomes of the AML patients, the researchers also were able to identify 13 novel "driver" mutations that are likely to be important for leukemia to develop in other patients. They also identified a number of additional cooperating mutations that work together with the driver mutations to give blood stem cells a growth advantage over other cells. In many patients, it appeared that in addition to an initiating driver mutation, only a one or two additional cooperating mutations were important for cancer to occur.
While the findings are important to leukemia, they may also hold true for other cancers.
"Our study does not provide proof that this model applies to other cancers," says corresponding author Timothy Ley, MD, professor of medicine and of genetics. "But this research suggests that scientists should look. This model could explain the large numbers of mutations we and other researchers are finding in breast, lung and other cancers. The idea that the vast majority of mutations occur in a cell before it becomes cancer is completely novel and should be explored further."
The research is supported by the National Human Genome Research Institute (NHGRI U54 HG003079), the National Cancer Institute (P01 CA101937 and K99 HL103975) and the Barnes-Jewish Hospital Foundation.

Tuesday, July 24, 2012

You May Never Need to Clean Your Car Again, Thanks to New Coating Technology

Researchers at Eindhoven University of Technology (TU/e) have developed a coating with a surface that repairs itself after damage. This new coating has numerous potential applications -- for example mobile phones that will remain clean from fingerprints, cars that never need to be washed, and aircraft that need less frequent repainting.
The results were published in the 17 July edition of the influential scientific journal Advanced Materials.
Functional coatings, for example with highly water-resistant or antibacterial properties, have at their surface nano-sized molecular groups that provide these specific properties. But up to now, these molecular groups are easily and irreversibly damaged by minor contact with their surface (such as by scratching), quickly causing their properties to be lost. This has been a big limitation to the possible applications of these coatings. Researcher Catarina Esteves of the department of Chemical Engineering and Chemistry at TU/e and her colleagues have now found a solution to this problem. They have done this by developing surfaces with special 'stalks' carrying the functional chemical groups at their ends, and mixing these through the coating. If the outer surface layer is removed by scratching, the 'stalks' in the underlying layer re-orient to the new surface, thereby restoring the function.
This development can be of great importance for many applications. For example it will be possible to make a self-cleaning car, with a highly water-resistant coating that keeps this self-cleaning property for long periods. The superficial scratches will be self-repaired and the water droplets simply roll off the car, taking dirt with them. An occasional rain shower is all that's needed to keep the car clean. In the same way, products like mobile phones, solar panels or even aircraft will remain clean for a longer time. For aircraft a cleaner surface means less air resistance, which in turn reduces fuel consumption. Other applications are contact lenses that self-repair their scratches, and coatings that resist the formation of algae, which is an advantage for ships. A limitation of the new technology is that it only works with superficial scratches that do not completely penetrate the coating.
Researcher Esteves and her team now intend to further develop this finding together with other universities and with industrial partners. She expects the first coatings to be ready for production within six to eight years, at prices comparable to those of today's coatings.

Scientists Connect Seawater Chemistry With Ancient Climate Change and Evolution

"Seawater chemistry is characterized by long phases of stability, which are interrupted by short intervals of rapid change," says Professor Ulrich Wortmann in the Department of Earth Sciences at the University of Toronto, lead author of a study to be published in Science this week. "We've established a new framework that helps us better interpret evolutionary trends and climate change over long periods of time. The study focuses on the past 130 million years, but similar interactions have likely occurred through the past 500 million years."
Wortmann and co-author Adina Paytan of the Institute of Marine Sciences at the University of California Santa Cruz point to the collision between India and Eurasia approximately 50 million years ago as one example of an interval of rapid change. This collision enhanced dissolution of the most extensive belt of water-soluble gypsum on Earth, stretching from Oman to Pakistan, and well into Western India -- remnants of which are well exposed in the Zagros mountains.
The authors suggest that the dissolution or creation of such massive gyspum deposits will change the sulfate content of the ocean, and that this will affect the amount of sulfate aerosols in the atmosphere and thus climate. "We propose that times of high sulfate concentrations in ocean water correlate with global cooling, just as times of low concentration correspond with greenhouse periods," says Paytan.
"When India and Eurasia collided, it caused dissolution of ancient salt deposits which resulted in drastic changes in seawater chemistry," Paytan continues. "This may have led to the demise of the Eocene epoch -- the warmest period of the modern-day Cenozoic era -- and the transition from a greenhouse to icehouse climate, culminating in the beginning of the rapid expansion of the Antarctic ice sheet."
The researchers combined data of past seawater sulfur composition, assembled by Paytan in 2004, with Wortmann's recent discovery of the strong link between marine sulfate concentrations and carbon and phosphorus cycling. They were able to explain the seawater sulfate isotope record as a result of massive changes to the accumulation and weathering of gyspum -- the mineral form of hydrated calcium sulfate.
"While it has been known for a long time that gyspum deposits can be formed and destroyed rapidly, the effect of these processes on seawater chemistry has been overlooked," says Wortmann. "The idea represents a paradigm shift in our understanding of how ocean chemistry changes over time and how these changes are linked to climate."