2013年10月5日星期六

Business IEF2013: Silicon doctoring at Imec

Business IEF2013: Silicon doctoring at Imec

2013/10/04

imecPutting medical quality data in consumers’ hands is a key research area of Imec, Jo de Broeck, CTO of Imec, told the IEF 2013 meeting in Dublin.

As with most things chip-based, the technology scales. In 2001 it cost $1 billion to sequence a genome, said de Broeck, now it costs $100.

Imec is working with Pacific Biosciences to develop ICs for single molecule sequencing applications.

Sequencing is becoming a diagnostic tool for applications like early cancer diagnosis, therapy monitoring and surgery monitoring.

Sequencing requires massively parallel sequencing technology for ultra-deep sequencing which delivers answers in hours.

The prize for succeeding in this area is huge cost savings for governments. The USA spends 17.4% of GDP on healthcare, Europe spends 9.6 % and Japan spends 8.5%.

“Reducing diabetes and hypertension levels by 5 % would save $9 billion annually,” said de Broeck.

The worldwide cost of treating diabetes is $400 billion a year and the cost of treating heart disease is $1.6 trillion.

Imec is also developing neuroprobes for measuring neuro-degenerative disease. Here performance is doubling every seven years, said de Broeck.

The hunt at Imec is to understand Alzheimer’s, Parkinson’s, Depression, Schizophrenia, Epilepsy, Anorexia, Blindness, Deafness and Strokes.



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Business IEF2013: Plessey goes for $200bn a year market

Business IEF2013: Plessey goes for $200bn a year market

2013/10/04

MikeLeGoff100x140Michael Le Goff, CEO of Plessey, told Future Horizons’ IEF2013 in Dublin, about the huge challenges and huge opportunities of being in the LED business.

On the one hand, he’s competing with Osram, Bridgelux, Toshiba and Samsung. On the other hand LEDs are expected to be a $200 billion a year annual market in 2020.

“There are huge players in the market but we were first to market with GaN-on-silicon LEDs,” said Le Goff.

The best thing about the market is its immense potential. Between now snd 2020, it is expected that 182 billion LEDs will be required.

By 2020, LEDs are expected to represent 46% of the global lighting market saving 5 trillion kWh of electricity representing 489 billion in energy costs.

Plessey’s GaN-on-Si on six inch wafers in a gully depreciated fab is a cheaper alternative than the SiC on 2″ and 4″ wafers and the sapphire substrates used by competitors.

Asked if his technology could compete with the 8″ GaN-on-silicon production of Toshiba, Le Goff replied: “Certainly we see running on eight inch is better but it depends on which manufacturing assets you have available.” he added: “We have started experimentation on eight inch silicon substrates.”

Having entered the market this year, Plessey’s focus is now on product improvement and reduction in cost. Product improvement will come from making the die area more efficient. The cost aspiration is to get to $0.15 per 100 Lm by 2015. Currently it’s $0.25 per 100 Lm.

“Our challenge,” said Le Goff, ” is to make LED manufacture as high yielding as manufacturing a simple diode using existing, available semiconductor assets,”



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A better device to detect ultraviolet light

A better device to detect ultraviolet light

Although this radiation doesn't normally reach Earth's surface, it can leak through to just below the hole in the ozone layer. Monitoring this radiation is a way of tracking the hole in the ozone layer, and photodiodes that measure UVC are also used as flame sensors and for communication in space.

Now, Shinji Nakagomi and colleagues at Ishinomaki Senshu University in Japan have built a new kind of photodiode that can detect the whole range of UVC light while remaining insensitive to visible light from the sun -- two features that have eluded designers of current devices. By being "solar blind," photodiodes are more sensitive to the UVC range and are thus more useful.

Building a Better Photodiode

Some photo detectors consist of vacuum tubes on sale, but they have short lifetimes and are relatively large and unwieldy. Today, many photodiodes are instead based on a so-called p-n junction, in which a semiconductor that carries positive charge (the absence of electrons called holes) is put in contact with the same semiconductor that instead carries negative charge (electrons). When light with sufficient energy (short wavelength) strikes atoms near the interface between the two semiconductors -- called p-type and n-type, respectively -- it generates mobile electrons and holes, boosting electrical current across the p-n junction and signaling the presence of light.

Other photodiodes made from materials like aluminum nitride and diamond are sensitive only to a limited range of UVC light. But recently, gallium oxide has shown promise because it's sensitive to the entire UVC range and is solar blind. The problem, however, is that it's difficult to make p-type gallium oxide.

Instead of a photodiode based on a conventional p-n junction, the researchers built one based on what's called a heterojunction, which is a p-n junction that incorporates two different semiconductors. The team used gallium oxide and silicon carbide, and found that their device responds quickly to UV light -- within milliseconds -- and has little dark current, which is the intrinsic electrical current that flows through the device even in the absence of light. Minimal dark current is important for a sensitive photodiode.

"The most important aspect about our device is that it is based on a heterojunction between gallium oxide and silicon carbide," said Nakagomi. "This gallium oxide and silicon carbide photodiode is promising for the detection of UV light."


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Scientists discover molecules that show promise for new anti-flu medicines

Scientists discover molecules that show promise for new anti-flu medicines

These novel compounds show promise for a new class of antiviral medicines to fight much-feared pandemic influenzas such as the looming "bird flu" threats caused by the H5N1 influenza A virus and the new H7N9 virus responsible for a 2013 outbreak in China.

Timely production of a vaccine is difficult when a pandemic flu strikes. A viable alternative is to treat with drugs.

"Right now there's really only one effective oral drug for treating influenza," said Eddy Arnold, Board of Governors Professor of chemistry and chemical biology in the School of Arts and Sciences at Rutgers and a member of the Center for Advanced Biotechnology and Medicine. And just as bacteria develop resistance to antibiotics, Arnold notes that some flu strains have developed resistance to Tamiflu, the sole orally available anti-flu drug.

Arnold and his collaborators have been working to create drugs beyond Tamiflu, especially ones that target different parts of the virus, using an approach that helped in the development of powerful anti-AIDS drugs. By synthesizing chemical compounds that bind to metal ions in a viral enzyme, the researchers found they could halt that enzyme's ability to activate a key step in the virus's replication process.

In Arnold's words, his team's compounds "really gum up" the targeted enzyme of influenza virus.

"We're at a key proof of principle stage right now," he said. "It's not trivial to go from this point to actually delivering a drug, but we're optimistic -- this class of inhibitors has all the right characteristics."

Rutgers' search for these binding compounds relies on technology that reveals the structure of this enzyme in extremely fine detail. Researchers Joseph Bauman and Kalyan Das first produced high-resolution images of an H1N1 flu enzyme, and Bauman and postdoctoral researcher Disha Patel screened 800 small molecule fragments for binding.

The researchers in Arnold's lab worked with Edmond LaVoie, professor and chair of medicinal chemistry in the Ernest Mario School of Pharmacy, to modify those compounds, making them more potent and selective in blocking the flu enzyme's activity. Working with virologist Luis Martinez-Sobrido at the University of Rochester, they were able to detect antiviral activity of the compounds in cells.

The enzyme that the scientists are attacking is especially crafty, Arnold noted, because it steals material from human cells to disguise the invading flu virus in a process called "cap-snatching." These "caps" are a small chemical structure that prime the process for reading genetic information."What we're doing by blocking or inhibiting this enzyme is to interefere with flu's ability to disguise itself," he said.

Arnold cited research by universities and pharmaceutical companies nearly two decades ago that took this approach, but initially the technology to obtain high-resolution images of the influenza protein wasn't available. One pharmaceutical company, Merck, later applied the approach of targeting metal-ion containing active sites in the HIV enzyme integrase and developed a highly successful anti-AIDS drug.

"It's truly remarkable what they did, and we're trying to pursue similar logic with influenza," said Arnold.

The researchers have recently published their findings in the American Chemical Society journal ACS Chemical Biology. Some of the work was funded by the National Institutes of Health. Two additional publications in the journals Bioorganic Medicinal Chemistry and ACS Medicinal Chemistry Letters have described LaVoie's synthetic medicinal chemistry used to make the new anti-flu agents and the observed structure-activity relationships.


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Astronomers discover large 'hot' cocoon around a small baby star

Astronomers discover large 'hot' cocoon around a small baby star

Hot molecular clouds around new-born stars are called "Hot Cores" and have temperature of -- 160 degrees Celsius, 100 degrees hotter than normal molecular clouds. The large size of the hot core discovered by ALMA shows that much more energy is emitted from the central baby star than typical solar-mass young stars. This may be due to the higher mass infall rate, or multiplicity of the central baby star. This result indicates a large diversity in the star formation process.

The research findings are presented in the article "ALMA Observations of the IRDC Clump G34.43+00.24 MM3: Hot Core and Molecular Outflows," published in the Astrophysical Journal, Vol. 775, of September 20, 2013.

A large hot molecular cloud around a very young star was discovered by ALMA. This hot cloud is about ten times larger than those found around typical solar-mass baby stars, which indicates that the star formation process has more diversity than ever thought. This result was published in the Astrophysical Journal on September 20th, 2013.

Stars are formed in very cold (-260 degrees Celsius) gas and dust clouds. Infrared Dark Clouds (IRDC) are dense regions of such clouds, and thought that in which clusters of stars are formed. Since most of stars are born as members of star clusters, investigating IRDCs has a crucial role in comprehensive understanding the star formation process.

A baby star is surrounded by the natal gas and dust cloud, and the cloud is warmed up from its center. Temperature of the central part of some, but not all, of such clouds reaches as high as -160 degrees Celsius. Astronomers call those clouds as "hot core" -- it may not be hot on Earth, but is hot enough for a cosmic cloud. Inside hot cores, various molecules, originally trapped in the ice mantle around dust particles, are sublimated. Organic molecules such as methanol (CH3OH), ethyl cyanide (CH3CH2CN), and methyl formate (HCOOCH3) are abundant in hot cores.

International research team, led by Takeshi Sakai at the University of Electro-Communication, Japan, used ALMA to observe an IRDC named G34.43+00.24 MM3 (hereafter MM3) in the constellation Aquila (the Eagle). They discovered a young object from which the methanol molecular line is strongly emitted. A detailed investigation tells them that the temperature of the methanol gas is -140 degrees Celsius. This shows that MM3 harbors a baby star surrounded by a hot core. The size of the hot core is as large as 800 times 300 astronomical units (au, 1 au equals to the mean distance of the Sun and Earth; 150 million km). Typical size of hot cores around low-mass young stars is several tens to hundred of au, therefore the hot core in MM3 is exceptionally large. Sakai says "Thanks to the high sensitivity and spatial resolution, we need only a few hours to discover a previously unknown baby star. This is an important step to understand the star formation process in a cluster forming region."

The team also observed radio emission from carbon sulfide (CS) and silicon monoxide (SiO) to reveal the detailed structure of the molecular outflow from the baby star. The speed of the emanated gas is 28 km/s and the extent is 4,400 au. Based on these values, the team calculates the age of the outflow of only 740 years. Although molecular outflows are common features around protostars, the outflow as young as the one in MM3 is quite rare. In summary, ALMA finds that the protostar in MM3 is very young but has a giant hot core.

Why the hot core in MM3 is so large? In order to warm up the large volume of gas, the baby star should emit much more energy than typical ones. Protostars produce emission by converting the gravitational energy of infalling material to the thermal energy. The large size of the hot core in MM3 is possibly due to the high mass infalling rate than ever thought. The other possibility is that two or more protostars are embedded in the hot core. The research team has not reached the reason with this observation yet. "ALMA's spatial resolution improves much more in the near future," Sakai says, "Then much detail of the infalling material toward the protostar can be revealed, and it helps us answer to the mystery behind the diversity in star formation."


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Surprisingly simple scheme for self-assembling robots

Surprisingly simple scheme for self-assembling robots

Oct. 4, 2013 — Small cubes with no exterior moving parts can propel themselves forward, jump on top of each other, and snap together to form arbitrary shapes.


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In 2011, when an MIT senior named John Romanishin proposed a new design for modular robots to his robotics professor, Daniela Rus, she said, "That can't be done."

Two years later, Rus showed her colleague Hod Lipson, a robotics researcher at Cornell University, a video of prototype robots, based on Romanishin's design, in action. "That can't be done," Lipson said.

In November, Romanishin -- now a research scientist in MIT's Computer Science and Artificial Intelligence Laboratory (CSAIL) -- Rus, and postdoc Kyle Gilpin will establish once and for all that it can be done, when they present a paper describing their new robots at the IEEE/RSJ International Conference on Intelligent Robots and Systems.

Known as M-Blocks, the robots are cubes with no external moving parts. Nonetheless, they're able to climb over and around one another, leap through the air, roll across the ground, and even move while suspended upside down from metallic surfaces.

Inside each M-Block is a flywheel that can reach speeds of 20,000 revolutions per minute; when the flywheel is braked, it imparts its angular momentum to the cube. On each edge of an M-Block, and on every face, are cleverly arranged permanent magnets that allow any two cubes to attach to each other.

"It's one of these things that the [modular-robotics] community has been trying to do for a long time," says Rus, a professor of electrical engineering and computer science and director of CSAIL. "We just needed a creative insight and somebody who was passionate enough to keep coming at it -- despite being discouraged."

Embodied abstraction

As Rus explains, researchers studying reconfigurable robots have long used an abstraction called the sliding-cube model. In this model, if two cubes are face to face, one of them can slide up the side of the other and, without changing orientation, slide across its top.

The sliding-cube model simplifies the development of self-assembly algorithms, but the robots that implement them tend to be much more complex devices. Rus' group, for instance, previously developed a modular robot called the Molecule, which consisted of two cubes connected by an angled bar and had 18 separate motors. "We were quite proud of it at the time," Rus says.

According to Gilpin, existing modular-robot systems are also "statically stable," meaning that "you can pause the motion at any point, and they'll stay where they are." What enabled the MIT researchers to drastically simplify their robots' design was giving up on the principle of static stability.

"There's a point in time when the cube is essentially flying through the air," Gilpin says. "And you are depending on the magnets to bring it into alignment when it lands. That's something that's totally unique to this system."

That's also what made Rus skeptical about Romanishin's initial proposal. "I asked him build a prototype," Rus says. "Then I said, 'OK, maybe I was wrong.'"

Sticking the landing

To compensate for its static instability, the researchers' robot relies on some ingenious engineering. On each edge of a cube are two cylindrical magnets, mounted like rolling pins. When two cubes approach each other, the magnets naturally rotate, so that north poles align with south, and vice versa. Any face of any cube can thus attach to any face of any other.

The cubes' edges are also beveled, so when two cubes are face to face, there's a slight gap between their magnets. When one cube begins to flip on top of another, the bevels, and thus the magnets, touch. The connection between the cubes becomes much stronger, anchoring the pivot. On each face of a cube are four more pairs of smaller magnets, arranged symmetrically, which help snap a moving cube into place when it lands on top of another.

As with any modular-robot system, the hope is that the modules can be miniaturized: the ultimate aim of most such research is hordes of swarming microbots that can self-assemble, like the "liquid steel" androids in the movie "Terminator II." And the simplicity of the cubes' design makes miniaturization promising.

But the researchers believe that a more refined version of their system could prove useful even at something like its current scale. Armies of mobile cubes could temporarily repair bridges or buildings during emergencies, or raise and reconfigure scaffolding for building projects. They could assemble into different types of furniture or heavy equipment as needed. And they could swarm into environments hostile or inaccessible to humans, diagnose problems, and reorganize themselves to provide solutions.

Strength in diversity

The researchers also imagine that among the mobile cubes could be special-purpose cubes, containing cameras, or lights, or battery packs, or other equipment, which the mobile cubes could transport. "In the vast majority of other modular systems, an individual module cannot move on its own," Gilpin says. "If you drop one of these along the way, or something goes wrong, it can rejoin the group, no problem."

"It's one of those things that you kick yourself for not thinking of," Cornell's Lipson says. "It's a low-tech solution to a problem that people have been trying to solve with extraordinarily high-tech approaches."

"What they did that was very interesting is they showed several modes of locomotion," Lipson adds. "Not just one cube flipping around, but multiple cubes working together, multiple cubes moving other cubes -- a lot of other modes of motion that really open the door to many, many applications, much beyond what people usually consider when they talk about self-assembly. They rarely think about parts dragging other parts -- this kind of cooperative group behavior."

In ongoing work, the MIT researchers are building an army of 100 cubes, each of which can move in any direction, and designing algorithms to guide them. "We want hundreds of cubes, scattered randomly across the floor, to be able to identify each other, coalesce, and autonomously transform into a chair, or a ladder, or a desk, on demand," Romanishin says.

Video: http://www.youtube.com/watch?v=6aZbJS6LZbs



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Well-connected hemispheres of Einstein's brain may have sparked his brilliance

Well-connected hemispheres of Einstein's brain may have sparked his brilliance

"This study, more than any other to date, really gets at the 'inside' of Einstein's brain," Falk said. "It provides new information that helps make sense of what is known about the surface of Einstein's brain."

The study, "The Corpus Callosum of Albert Einstein's Brain: Another Clue to His High Intelligence," was published in the journal Brain. Lead author Weiwei Men of East China Normal University's Department of Physics developed a new technique to conduct the study, which is the first to detail Einstein's corpus callosum, the brain's largest bundle of fibers that connects the two cerebral hemispheres and facilitates interhemispheric communication.

"This technique should be of interest to other researchers who study the brain's all-important internal connectivity," Falk said.

Men's technique measures and color-codes the varying thicknesses of subdivisions of the corpus callosum along its length, where nerves cross from one side of the brain to the other. These thicknesses indicate the number of nerves that cross and therefore how "connected" the two sides of the brain are in particular regions, which facilitate different functions depending on where the fibers cross along the length. For example, movement of the hands is represented toward the front and mental arithmetic along the back.

In particular, this new technique permitted registration and comparison of Einstein's measurements with those of two samples -- one of 15 elderly men and one of 52 men Einstein's age in 1905. During his so-called "miracle year" at 26 years old, Einstein published four articles that contributed substantially to the foundation of modern physics and changed the world's views about space, time, mass and energy.

The research team's findings show that Einstein had more extensive connections between certain parts of his cerebral hemispheres compared to both younger and older control groups.

The research of Einstein's corpus callosum was initiated by Men, who requested the high-resolution photographs that Falk and other researchers published in 2012 of the inside surfaces of the two halves of Einstein's brain. In addition to Men, the current research team included Falk, who served as second author; Tao Sun of the Washington University School of Medicine; and, from East China Normal University's Department of Physics, Weibo Chen, Jianqi Li, Dazhi Yin, Lili Zang and Mingxia Fan.


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2013年10月4日星期五

Business Plessey goes for $200bn a year market

Business Plessey goes for $200bn a year market

2013/10/04

Michael Le Goff, CEO of Plessey, told Future Horizons’ IEF2013 in Dublin, about the huge challenges and huge opportunities of being in the LED business.

On the one hand, he’s competing with Osram, Bridgelux, Toshiba and Samsung. On the other hand LEDs are expected to be a $200 billion a year annual market in 2020.

“There are huge players in the market but we were first to market with GaN-on-silicon LEDs,” said Le Goff.

The best thing about the market is its immense potential. Between now snd 2020, it is expected that 182 billion LEDs will be required.

By 2020, LEDs are expected to represent 46% of the global lighting market sabing 5 trillion kWh of electricity representing 489 billion in energy costs.

Plessey’s GaN-on-Si on s ix inch wafers in a gully depreciated fab is a cheaper alternative than the SiC on 2″ and 4″ wafers and the sapphire substrates used by competitors.

Asked if his technology could compete with the 8″ GaN-on-silicon production of Toshia, Le Goff replied: “Certainly we see running on eight inch is better but it depends on which manufacturing assets you have available.” he added: “We have started experimentation on eight inch silicon substrates.”

Having entered the market this year, Plessey’s focus is now on product improvement and reduction in cost. Product improvement will come from making the die area more efficient. The cost asprstion is to get to $0.15 per 100 Lm by 2015. Currently it’s $0.25 per 100 Lm.

“Our challenge,” said Le Goff, ” is to make LED manufacture as high yielding as manufacturing a simple diode using existing, available semiconductor assets,”



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Business Foundries have 53% capex-to-sales ratio

Business Foundries have 53% capex-to-sales ratio

2013/10/03

The total capital outlays by the Big 4 pure-play foundries are forecast to be $16.6 billion in 2013, which would represent 53% of their combined sales, says IC Insights, which far exceeds the industry average of 18% capital-spending-to-sales ratio.  

tsmcThe Big 4’s capital spending as a percent of “final sales” is forecast to be 24% in 2013, still well above industry average.

A few years ago, TSMC stated that it planned to keep its capital spending at about 20% of its sales, but that was before GlobalFoundries and Samsung brought competitive pressure to the market and started chipping away at TSMC’s business.

TSMC spent $5.9 billion in capital spending in 2010 (a budget that was increased twice in the first half of the year), an all-time record amount of capital spending for the company at that time. TSMC spent $8.3 billion in capital expenditures in 2012 and plans to further increase its capex spending to $10.0 billion in 2013.

It appears that TSMC will be aggressive in its marketshare fight with GlobalFoundries and Samsung and is likely to greatly exceed its 20% of sales goal for capital spending outlays over the next few years.

The question with regard to the expected combined 2011-2013 IC foundry spending by the Big 4 pure-play suppliers ($46.3 billion) is whether it is too much.

The “final sales” capital-spending-to-sales ratio of the major foundries was a relatively low 14-15% in 2005-2007 before falling to only 9% in 2008 and 12% in 2009.  In 2010, this figure rose to 23%, a level not seen since the boom year of 2004.  Spurred by the surge in capital spending by TSMC and GlobalFoundries, this figure rose to 30% in 2011.

For 2012, the capital spending as a percent of sales figure for the Big 4 foundries dropped back to a more “reasonable” 24%, with the same percentage expected for 2013.  Given the major foundries high capacity utilization levels for leading-edge device production, it appears that current spending levels are warranted and should not lead to significant overcapacity issues.

With demand for IC foundry services from fabless and fab-lite IDM companies expected to be high over the next five years, there is little doubt that demand for IC foundry production will remain strong.

Overall, IC Insights believes that the pure-play foundry market will further divide into the leading-edge IC foundries like TSMC, GlobalFoundries, UMC, and Samsung, and the specialty foundries like TowerJazz, X-Fab, etc.

Thus, the vast majority of future foundry capital spending can still be expected to come from the small group of major foundries targeting leading-edge IC production.



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SUV System Ltd is Electronic Components Distributor Supplies,Find Quality Electronic Components Supplies Products IC(Integrated Circuits),Connectors,Capacitor,Resistors,Diodes,Transistors,LED at Suvsystem.com. Sourcing Other Energy, Environment, Excess Inventory Products from Manufacturers and Suppliers at Suvsystem.com

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Bright nearby double star Fomalhaut is actually a triple

Bright nearby double star Fomalhaut is actually a triple

Oct. 3, 2013 — The nearby star system Fomalhaut -- of special interest for its unusual exoplanet and dusty debris disk -- has been discovered to be not just a double star, as astronomers had thought, but one of the widest triple stars known.


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In a paper recently accepted for publication in the Astronomical Journal, researchers show that a previously known smaller star in its vicinity is also part of the Fomalhaut system.

Eric Mamajek, associate professor of physics and astronomy at the University of Rochester, and his collaborators found the triple nature of the star system through a bit of detective work. "I noticed this third star a couple of years ago when I was plotting the motions of stars in the vicinity of Fomalhaut for another study," Mamajek said. "However I needed to collect more data and gather a team of co-authors with different observations to test whether the star's properties are consistent with being a third member of the Fomalhaut system."

Serendipity also played a part. A chance meeting in Chile between Mamajek and Todd Henry, from Georgia State University and director of the Research Consortium On Nearby Stars (RECONS) team, revealed a clue that helped solve the mystery: the distance to the star. Henry recalls sitting in the kitchen of a motel in La Serena, Chile, with Mamajek, discussing nearby stars. "Eric was playing detective on this third star and I just happened to be sitting there with an observing list that contained the unpublished parallax," Henry said. Parallax is a type of measurement astronomers use to determine distances. "A student at the time, Jennifer Bartlett at the University of Virginia, was working with us on a sample of potentially nearby stars for her Ph.D. thesis, and LP876-10 was on it. Eric and I got to talking, and here we are with a cool discovery."

By carefully analyzing astrometric (precise movements) and spectroscopic measurements (that allow the temperature and radial velocity to be determined), the researchers were able to measure the distance and speed of the third star. They concluded that the star, until recently known as LP 876-10, is part of the Fomalhaut system, making it Fomalhaut C.

"Fomalhaut C looks quite far apart from the big, bright star that is Fomalhaut A when you look up at the sky from Earth," added Mamajek. There are roughly 5.5 degrees between the two stars, which is as if they were separated by roughly 11 full moons for an observer on Earth. Mamajek explained that they look this far apart, in part, because Fomalhaut is relatively close to Earth as stars go -- approximately 25 light years. If these stars were far away from Earth, they would appear much closer together in the sky. That they appear so far apart could explain why the connection between LP 876-10 and Fomalhaut had been previously missed. Being able to obtain high quality astrometric and velocity data were the other keys.

The researchers also had to show that it would be feasible for these two stars to be bound, rather than moving independently. "Fomalhaut A is such a massive star, about twice the mass of our Sun, that it can exert sufficient gravitational pull to keep this tiny star bound to it -- despite the star being 158,000 times farther away from Fomalhaut than the Earth is from the Sun," Mamajek said.

Mamajek worked with a large team of collaborators to piece together the story of this interesting tiny star. "Henry and the RECONS team have been doing an exhaustive survey of the "Solar Neighborhood," characterizing the stellar systems that are closest to our solar system and discovering new nearby stars," said Mamajek. "His team had already gathered several years of observations on this particular star -- using the SMARTS 0.9-meter telescope at Cerro Tololo in Chile." The researchers also needed to know the radial velocity of the star, which Andreas Seifahrt from the University of Chicago measured, and which they pinpoint in the paper to be within about one kilometer per second of that of Fomalhaut A.

There are another 11 star systems closer to our Sun than Fomalhaut that consist of three or more stars, including the closest star system, Alpha Centauri. The new measurements in the paper also show that the Fomalhaut system is the most massive and widest among these nearby multiple systems.

Fomalhaut A is also the 18th brightest star visible in our night sky and one of the few stars with both a directly imaged exoplanet and a dusty debris disk. The famous star has been featured in science fiction novels by writers Isaac Asimov, Stanislaw Lem, Philip K. Dick, and Frank Herbert. Despite being a well-studied system, it was only recently confirmed that Fomalhaut was a binary star -- two stars that orbit each other -- although it had been first suggested in the 1890s.

One of Mamajek's colleagues at Rochester, Professor of Physics and Astronomy Alice C. Quillen, has worked for years to understand the way planets shape stellar dust disks like the one surrounding Fomalhaut. In 2006, she predicted the existence of a planet around Fomalhaut, as well as the shape of its orbit, by trying to understand why the debris ring was off-center and why it had a surprisingly sharp edge. The following year a new planet around Fomalhaut was imaged.

Many questions about Fomalhaut A's exoplanet and debris disk still remain unanswered. For example, astronomers are puzzled by why the exoplanet known as Fomalhaut "b" is on such an eccentric orbit and why the debris disk does not appear to be centered on the star Fomalhaut A. It is possible that Fomalhaut's wide companions B and C have gravitationally perturbed the Fomalhaut "b" exoplanet and debris belt orbiting Fomalhaut A, however the orbits of Fomalhaut's companion stars are not well-constrained. The orbits of Fomalhaut B and C around Fomalhaut A are predicted to take millions of years, so pinning down their orbits will be a challenge for future astronomers.

While Fomalhaut C is a red dwarf star -- the most common type of star in the universe -- Fomalhaut B is an orange dwarf star about three-fourths the mass of our Sun. From the vantage point of a hypothetical planet orbiting Fomalhaut C, Fomalhaut A would appear to be a brilliant white star nine times brighter than Sirius (the brightest star in our night sky) appears from Earth, similar to the typical brightness of the planet Venus. Fomalhaut B would appear to be an otherwise unremarkable bright orangish star similar in brightness to Polaris. The age of the trio is about 440 million years -- roughly a 10th of the age of our solar system.

Other collaborators who worked on this paper include Jennifer Bartlett, now at the U.S. Naval Observatory who published a preliminary distance to the star in her Ph.D. thesis, and Matt Kenworthy, from the Leiden Observatory, who measured the rotation period showing Fomalhaut C is a very fast rotator.



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