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The Extraordinary Link Between Deep Neural Networks and the Nature of the Universe

Nobody understands why deep neural networks are so good at solving complex problems. Now physicists say the secret is buried in the laws of physics.

In the last couple of years, deep learning techniques have transformed the world of artificial intelligence. One by one, the abilities and techniques that humans once imagined were uniquely our own have begun to fall to the onslaught of ever more powerful machines. Deep neural networks are now better than humans at tasks such as face recognition and object recognition. They’ve mastered the ancient game of Go and thrashed the best human players.

But there is a problem. There is no mathematical reason why networks arranged in layers should be so good at these challenges. Mathematicians are flummoxed. Despite the huge success of deep neural networks, nobody is quite sure how they achieve their success.

Today that changes thanks to the work of Henry Lin at Harvard University and Max Tegmark at MIT. These guys say the reason why mathematicians have been so embarrassed is that the answer depends on the nature of the universe. In other words, the answer lies in the regime of physics rather than mathematics.

First, let’s set up the problem using the example of classifying a megabit grayscale image to determine whether it shows a cat or a dog.

Such an image consists of a million pixels that can each take one of 256 grayscale values. So in theory, there can be 2561000000 possible images, and for each one it is necessary to compute whether it shows a cat or dog. And yet neural networks, with merely thousands or millions of parameters, somehow manage this classification task with ease.

In the language of mathematics, neural networks work by approximating complex mathematical functions with simpler ones. When it comes to classifying images of cats and dogs, the neural network must implement a function that takes as an input a million grayscale pixels and outputs the probability distribution of what it might represent.

The problem is that there are orders of magnitude more mathematical functions than possible networks to approximate them. And yet deep neural networks somehow get the right answer.

Now Lin and Tegmark say they’ve worked out why. The answer is that the universe is governed by a tiny subset of all possible functions. In other words, when the laws of physics are written down mathematically, they can all be described by functions that have a remarkable set of simple properties.

So deep neural networks don’t have to approximate any possible mathematical function, only a tiny subset of them.

To put this in perspective, consider the order of a polynomial function, which is the size of its highest exponent. So a quadratic equation like y=x2 has order 2, the equation y=x24 has order 24, and so on.

Obviously, the number of orders is infinite and yet only a tiny subset of polynomials appear in the laws of physics. “For reasons that are still not fully understood, our universe can be accurately described by polynomial Hamiltonians of low order,” say Lin and Tegmark. Typically, the polynomials that describe laws of physics have orders ranging from 2 to 4.

The laws of physics have other important properties. For example, they are usually symmetrical when it comes to rotation and translation. Rotate a cat or dog through 360 degrees and it looks the same; translate it by 10 meters or 100 meters or a kilometer and it will look the same. That also simplifies the task of approximating the process of cat or dog recognition.

These properties mean that neural networks do not need to approximate an infinitude of possible mathematical functions but only a tiny subset of the simplest ones.

There is another property of the universe that neural networks exploit. This is the hierarchy of its structure. “Elementary particles form atoms which in turn form molecules, cells, organisms, planets, solar systems, galaxies, etc.,” say Lin and Tegmark. And complex structures are often formed through a sequence of simpler steps.

This is why the structure of neural networks is important too: the layers in these networks can approximate each step in the causal sequence.

Lin and Tegmark give the example of the cosmic microwave background radiation, the echo of the Big Bang that permeates the universe. In recent years, various spacecraft have mapped this radiation in ever higher resolution. And of course, physicists have puzzled over why these maps take the form they do.

Tegmark and Lin point out that whatever the reason, it is undoubtedly the result of a causal hierarchy. “A set of cosmological parameters (the density of dark matter, etc.) determines the power spectrum of density fluctuations in our universe, which in turn determines the pattern of cosmic microwave background radiation reaching us from our early universe, which gets combined with foreground radio noise from our galaxy to produce the frequency-dependent sky maps that are recorded by a satellite-based telescope,” they say.

Each of these causal layers contains progressively more data. There are only a handful of cosmological parameters but the maps and the noise they contain are made up of billions of numbers. The goal of physics is to analyze the big numbers in a way that reveals the smaller ones.

And when phenomena have this hierarchical structure, neural networks make the process of analyzing it significantly easier.

“We have shown that the success of deep and cheap learning depends not only on mathematics but also on physics, which favors certain classes of exceptionally simple probability distributions that deep learning is uniquely suited to model,” conclude Lin and Tegmark.

That’s interesting and important work with significant implications. Artificial neural networks are famously based on biological ones. So not only do Lin and Tegmark’s ideas explain why deep learning machines work so well, they also explain why human brains can make sense of the universe. Evolution has somehow settled on a brain structure that is ideally suited to teasing apart the complexity of the universe.

This work opens the way for significant progress in artificial intelligence. Now that we finally understand why deep neural networks work so well, mathematicians can get to work exploring the specific mathematical properties that allow them to perform so well. “Strengthening the analytic understanding of deep learning may suggest ways of improving it,” say Lin and Tegmark.

Deep learning has taken giant strides in recent years. With this improved understanding, the rate of advancement is bound to accelerate.


Ref: arxiv.org/abs/1608.08225: Why Does Deep and Cheap Learning Work So Well


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Mars contamination fear could divert Curiosity rover

CM_edited.jpg (1024×690)

NASA

View from the Mars rover Curiosity at the foot of Aeolis Mons, before the rover starts to climb the mountain.

Four years into its travels across Mars, NASA’s Curiosity rover faces an un­expected challenge: wending its way safely among dozens of dark streaks that could indicate water seeping from the red planet’s hillsides.

Although scientists might love to investigate the streaks at close range, strict international rules prohibit Curiosity from touching any part of Mars that could host liquid water, to prevent contamination. But as the rover begins climbing the mountain Aeolis Mons next month, it will probably pass within a few kilometres of a dark streak that grew and shifted between February and July 2012 in ways suggestive of flowing water.

NASA officials are trying to determine whether Earth microbes aboard Curiosity could contaminate the Martian seeps from a distance. If the risk is too high, NASA could shift the rover’s course — but that would present a daunting geographical challenge. There is only one obvious path to the ancient geological formations that Curiosity scientists have been yearning to sample for years (see ‘All wet?’).

“We’re very excited to get up to these layers and find the 3-billion-year-old water,” says Ashwin Vasavada, Curiosity’s project scientist at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California. “Not the ten-day-old water.”

The streaks — dubbed recurring slope lineae (RSLs) because they appear, fade away and re­appear seasonally on steep slopes — were first reported1 on Mars five years ago in a handful of places. The total count is now up to 452 possible RSLs. More than half of those are in the enormous equatorial canyon of Valles Marineris, but they also appear at other latitudes and longitudes. “We’re just finding them all over the place,” says David Stillman, a planetary scientist at the Southwest Research Institute in Boulder, Colorado, who leads the cataloguing.

Dark marks

RSLs typically measure a few metres across and hundreds of metres long. One leading idea is that they form when the chilly Martian surface warms just enough to thaw an ice dam in the soil, allowingwater to begin seeping downhill. When temperatures drop, the water freezes and the hillside lightens again until next season. But the picture is complicated by factors such as potential salt in the water; brines may seep at lower temperatures than fresher water2.

Other possible explanations for the streaks include water condensing from the atmosphere, or the flow of bone-dry debris. “They have a lot of behaviours that resemble liquid water,” says Colin Dundas, a planetary geologist at the US Geological Survey in Flagstaff, Arizona. “But Mars is a strange place, and it’s worth considering the possibility there are dry processes that could surprise us.”

Source: Route: NASA; Terrain: ASU; RSLs: Ref. 4

A study published last month used orbital infrared data to suggest that typical RSLs contain no more than 3% water3. And other streaky-slope Martian features, known as gullies, were initially thought to be caused by liquid water but are now thought to be formed mostly by carbon dioxide frost.

Dundas and his colleagues have counted 58 possible RSLs near Curiosity’s landing site in Gale Crater4. Many of them appeared after a planet-wide dust storm in 2007 — possibly because the dust acted as a greenhouse and temporarily warmed the surface, Stillman says.

Since January, mission scientists have used the ChemCam instrument aboard the rover — which includes a small telescope — to photograph nearby streaks whenever possible.

So far, the rover has taken pictures of 8 of the 58 locations and seen no changes. The features are lines on slopes, but they have not yet recurred. “We’ve got two of the three letters in the acronym,” says Ryan Anderson, a geologist at the US Geological Survey who leads the imaging campaign.

Curiosity is currently about 5 kilometres away from the potential RSLs; on its current projected path, it would never get any closer than about 2 kilometres, Vasavada says. The rover could not physically drive up and touch the streaks if it wanted to, because it cannot navigate the slopes of 25 degrees or greater on which they appear.

But the rover’s sheer unexpected proximity to RSLs has NASA re-evaluating its planetary-protection protocols. Curiosity was only partly sterilized before going to Mars, and experts at JPL and NASA headquarters in Washington DC are calculating how long the remaining microbes could survive in Mars’s harsh atmosphere — as well as what weather conditions could transport them several kilometres away and possibly contaminate a water seep. “That hasn’t been well quantified for any mission,” says Vasavada.

The work is an early test for the NASA Mars rover slated to launch in 2020, which will look for life and collect and stash samples for possible return to Earth. RSLs exist at several of the rover’s eight possible landing sites.

For now, Curiosity is finishing exploring the Murray Buttes. These spectacular rock towers formed from sediment at the bottom of ancient lakes — the sort of potentially life-supporting environment the rover was sent to find. Curiosity’s second extended mission begins on 1 October.

Barring disaster, the rover’s lifespan will be set by its nuclear-power source, which will continue to dwindle in coming years through radioactive decay. Curiosity still has kilometres to scale on Aeolis Mons as it moves towards its final destination, a sulfate-rich group of rocks.

Nature
 
537,
 
145–146
 
()
 
doi:10.1038/537145a
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How DNA could store all the world’s data

 Natural Science-DNA

Modern archiving technology cannot keep up with the growing tsunami of bits. But nature may hold an answer to that problem already

For Nick Goldman, the idea of encoding data in DNA started out as a joke.

It was Wednesday 16 February 2011, and Goldman was at a hotel in Hamburg, Germany, talking with some of his fellow bioinformaticists about how they could afford to store the reams of genome sequences and other data the world was throwing at them. He remembers the scientists getting so frustrated by the expense and limitations of conventional computing technology that they started kidding about sci-fi alternatives. “We thought, 'What's to stop us using DNA to store information?'”

Then the laughter stopped. “It was a lightbulb moment,” says Goldman, a group leader at the European Bioinformatics Institute (EBI) in Hinxton, UK. True, DNA storage would be pathetically slow compared with the microsecond timescales for reading or writing bits in a silicon memory chip. It would take hours to encode data by synthesizing DNA strings with a specific pattern of bases, and still more hours to recover that information using a sequencing machine. But with DNA, a whole human genome fits into a cell that is invisible to the naked eye. For sheer density of information storage, DNA could be orders of magnitude beyond silicon — perfect for long-term archiving.

“We sat down in the bar with napkins and biros,” says Goldman, and started scribbling ideas: “What would you have to do to make that work?” The researchers' biggest worry was that DNA synthesis and sequencing made mistakes as often as 1 in every 100 nucleotides. This would render large-scale data storage hopelessly unreliable — unless they could find a workable error-correction scheme. Could they encode bits into base pairs in a way that would allow them to detect and undo the mistakes? “Within the course of an evening,” says Goldman, “we knew that you could.”

He and his EBI colleague Ewan Birney took the idea back to their labs, and two years later announced that they had successfully used DNA to encode five files, including Shakespeare's sonnets and a snippet of Martin Luther King's 'I have a dream' speech1. By then, biologist George Church and his team at Harvard University in Cambridge, Massachusetts, had unveiled an independent demonstration of DNA encoding2. But at 739 kilobytes (kB), the EBI files comprised the largest DNA archive ever produced — until July 2016, when researchers from Microsoft and the University of Washington claimed a leap to 200 megabytes (MB).

The latest experiment signals that interest in using DNA as a storage medium is surging far beyond genomics: the whole world is facing a data crunch. Counting everything from astronomical images and journal articles to YouTube videos, the global digital archive will hit an estimated 44 trillion gigabytes (GB) by 2020, a tenfold increase over 2013. By 2040, if everything were stored for instant access in, say, the flash memory chips used in memory sticks, the archive would consume 10–100 times the expected supply of microchip-grade silicon3.

That is one reason why permanent archives of rarely accessed data currently rely on old-fashioned magnetic tapes. This medium packs in information much more densely than silicon can, but is much slower to read. Yet even that approach is becoming unsustainable, says David Markowitz, a computational neuroscientist at the US Intelligence Advanced Research Projects Activity (IARPA) in Washington DC. It is possible to imagine a data centre holding an exabyte (one billion gigabytes) on tape drives, he says. But such a centre would require US$1 billion over 10 years to build and maintain, as well as hundreds of megawatts of power. “Molecular data storage has the potential to reduce all of those requirements by up to three orders of magnitude,” says Markowitz. If information could be packaged as densely as it is in the genes of the bacterium Escherichia coli, the world's storage needs could be met by about a kilogram of DNA (see 'Storage limits').

Achieving that potential won't be easy. Before DNA can become a viable competitor to conventional storage technologies, researchers will have to surmount a host of challenges, from reliably encoding information in DNA and retrieving only the information a user needs, to making nucleotide strings cheaply and quickly enough.

But efforts to meet those challenges are picking up. The Semiconductor Research Corporation (SRC), a foundation in Durham, North Carolina, that is supported by a consortium of chip-making firms, is backing DNA storage work. Goldman and Birney have UK government funding to experiment with next-generation approaches to DNA storage and are planning to set up a company to build on their research. And in April, IARPA and the SRC hosted a workshop for academics and industry researchers, including from companies such as IBM, to direct research in the field.

“For ten years we've been looking beyond silicon” for data archiving, says SRC director and chief scientist Victor Zhirnov. “It is very difficult to replace,” he says. But DNA, one of the strongest candidates yet, “looks like it may happen.”

Long-term memory

The first person to map the ones and zeroes of digital data onto the four base pairs of DNA was artist Joe Davis, in a 1988 collaboration with researchers from Harvard. The DNA sequence, which they inserted into E. coli, encoded just 35 bits. When organized into a 5 × 7 matrix, with ones corresponding to dark pixels and zeroes corresponding to light pixels, they formed a picture of an ancient Germanic rune representing life and the female Earth.

Today, Davis is affiliated with Church's lab, which began to explore DNA data storage in 2011. The Harvard team hoped the application might help to reduce the high cost of synthesizing DNA, much as genomics had reduced the cost of sequencing. Church carried out the proof-of-concept experiments in November 2011 along with Sri Kosuri, now at the University of California, Los Angeles, and genomics expert Yuan Gao at Johns Hopkins University in Baltimore, Maryland. The team used many short DNA strings to encode a 659-kB version of a book Church had co-authored. Part of each string was an address that specified how the pieces should be ordered after sequencing, with the remainder containing the data. A binary zero could be encoded by the bases adenine or cytosine, and a binary one could be represented by guanine or thymine. That flexibility helped the group to design sequences that avoided reading problems, which can occur with regions containing lots of guanine and cytosine, repeated sections, or stretches that bind to one another and make the strings fold up. They didn't have error correction in the strict sense, instead relying on the redundancy provided by having many copies of each individual string. Consequently, after sequencing the strings, Kosuri, Church and Gao found 22 errors — far too many for reliable data storage.

At the EBI, meanwhile, Goldman, Birney and their colleagues were also using many strings of DNA to encode their 739-kB data store, which included an image, ASCII text, audio files and a PDF version of Watson and Crick's iconic paper on DNA's double-helix structure. To avoid repeating bases and other sources of error, the EBI-led team used a more complex scheme (see 'Making memories'). One aspect involved encoding the data not as binary ones and zeroes, but in base three — the equivalent of zero, one and two. They then continuously rotated which DNA base represented each number, so as to avoid sequences that might cause problems during reading. By using overlapping, 100-base-long strings that progressively shifted by 25 bases, the EBI scientists also ensured that there would be four versions of each 25-base segment for error-checking and comparison against each other.

Sources: Making memories, ref. [1]; Storage limits, ref. [3]

They still lost 2 of the 25-base sequences — ironically, part of the Watson and Crick file. Nevertheless, these results convinced Goldman that DNA had potential as a cheap, long-term data repository that would require little energy to store. As a measure of just how long-term, he points to the 2013 announcement of a horse genome decoded from a bone trapped in permafrost for 700,000 years4. “In data centres, no one trusts a hard disk after three years,” he says. “No one trusts a tape after at most ten years. Where you want a copy safe for more than that, once we can get those written on DNA, you can stick it in a cave and forget about it until you want to read it.”

A burgeoning field

That possibility has captured the imaginations of computer scientists Luis Ceze, from the University of Washington, and Karin Strauss, from Microsoft Research in Redmond, Washington, ever since they heard Goldman discuss the EBI work when they visited the United Kingdom in 2013. “DNA's density, stability and maturity have made us excited about it,” says Strauss.

And on their return to Washington state, says Strauss, she and Ceze started investigations with their University of Washington collaborator Georg Seelig. One of their chief concerns has been another major drawback that goes well beyond DNA's vulnerability to errors. Using standard sequencing methods, there was no way to retrieve any one piece of data without retrieving all the data: every DNA string had to be read. That would be vastly more cumbersome than conventional computer memory, which allows for random access: the ability to read just the data that a user needs.

The team outlined its solution in early April at a conference in Atlanta, Georgia. The researchers start by withdrawing tiny samples from their DNA archive. They then use the polymerase chain reaction (PCR) to pinpoint and make more copies of the strings encoding the data they want to extract5. The proliferation of copies makes the sequencing faster, cheaper and more accurate than previous approaches. The team has also devised an alternative error-correction scheme that the group says allows for data encoding twice as dense as the EBI's, but just as reliable.

As a demonstration, the Microsoft–University of Washington researchers stored 151 kB of images, some encoded using the EBI method and some using their new approach, in a single pool of strings. They extracted three — a cat, the Sydney opera house and a cartoon monkey — using the EBI-like method, getting one read error that they had to correct manually. They also read the Sydney Opera House image using their new method, without any mistakes.

Economics versus chemistry

At the University of Illinois at Urbana–Champaign, computer scientist Olgica Milenkovic and her colleagues have developed a random-access approach that also enables them to rewrite the encoded data6. Their method stores data as long strings of DNA that have address sequences at both ends. The researchers then use these addresses to select, amplify and rewrite the strings using either PCR or the gene-editing technique CRISPR–Cas9.

The addresses have to avoid sequences that would hamper reading while also being different enough from each other to stop them being mixed up in the presence of errors. Doing this — and avoiding problems such as molecules folding up because their sequences contain stretches that recognize and bind to each other — took intense calculations. “At the beginning, we used computer search because it was really difficult to come up with something that had all these properties,” Milenkovic says. Her team has now replaced this labour-intensive process with mathematical formulae that allow them to devise an encoding scheme much more quickly.

“Once we can get those written on DNA, you can stick it in a cave and forget about it.”

Other challenges for DNA data storage are scale and speed of synthesizing the molecules, says Kosuri, who admits that he has not been very bullish about the idea for that reason. During the early experiments at Harvard, he recalls, “we had 700 kB. Even a 1,000-fold increase on that is 700 MB, which is a CD”. Truly making a difference to the worldwide data archiving problem would mean storing information by the petabyte at least. “It's not impossible,” says Kosuri, “but people have to realize the scale is on the order of million-fold improvements.”

That will not be easy, agrees Markowitz. “The dominant production method is an almost 30-year-old chemical process that takes upwards of 400 seconds to add each base,” he says. If this were to remain the approach used, he adds, billions of different strings would have to be made in parallel for writing to be fast enough. The current maximum for simultaneous production is tens of thousands of strings.

A closely related factor is the cost of synthesizing DNA. It accounted for 98% of the expense of the $12,660 EBI experiment. Sequencing accounted for only 2%, thanks to a two-millionfold cost reduction since the completion of the Human Genome Project in 2003. Despite this precedent, Kosuri isn't convinced that economics can drive the same kind of progress in DNA synthesis. “You can easily imagine markets to sequence 7 billion people, but there's no case for building 7 billion people's genomes,” he says. He concedes that some improvement in costs might result from Human Genome Project-Write (HGP-write), a project proposed in June by Church and others. If funded, the programme would aim to synthesize an entire human genome: 23 chromosome pairs containing 3.2 billion nucleotides. But even if HGP-write succeeds, says Kosuri, a human genome contains just 0.75 GB of information and would be dwarfed by the challenge of synthesizing practical data stores.

Zhirnov, however, is optimistic that the cost of synthesis can be orders of magnitude below today's levels. “There are no fundamental reasons why it's high,” he says.

In April, Microsoft Research made an early move that may help create the necessary demand, ordering 10 million strings from Twist Bioscience, a DNA synthesis start-up company in San Francisco, California. Strauss and her colleagues say they have been using the strings to push their random-access storage approach to 0.2 GB. The details remain unpublished, but the archive reportedly includes the Universal Declaration of Human Rights in more than 100 languages, the top 100 books of Project Guttenberg and a seed database. Although this is much less of a synthesis challenge than the HGP-write faces, Strauss stresses the significance of the 250-fold jump in storage capacity.

“It was time to exercise our muscle handling larger volumes of DNA to push it to a larger scale and see where the process breaks,” she says. “It actually breaks in multiple places — and we're learning a great deal out of it.”

Goldman is confident that this is just a taste of things to come. “Our estimate is that we need 100,000-fold improvements to make the technology sing, and we think that's very credible,” he says. “While past performance is no guarantee, there are new reading technologies coming onstream every year or two. Six orders of magnitude is no big deal in genomics. You just wait a bit.”

Nature
 
537,
 
22–24
 
()
 
doi:10.1038/537022a
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PHILAE FOUND-Rosetta Probe

Rosetta Probe-ESA

Less than a month before the end of the mission, Rosetta’s high-resolution camera has revealed the Philae lander wedged into a dark crack on Comet 67P/Churyumov–Gerasimenko.

ESA_Rosetta_PhilaeFound

The images were taken on 2 September by the OSIRIS narrow-angle camera as the orbiter came within 2.7 km of the surface and clearly show the main body of the lander, along with two of its three legs.

The images also provide proof of Philae’s orientation, making it clear why establishing communications was so difficult following its landing on 12 November 2014.

Close-up of the Philae lander, imaged by Rosetta’s OSIRIS narrow-angle camera on 2 September 2016 from a distance of 2.7 km. The image scale is about 5 cm/pixel. Philae’s 1 m-wide body and two of its three legs can be seen extended from the body. The images also provide proof of Philae’s orientation. The image is a zoom from a wider-scene, and has been interpolated. Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

Close-up of the Philae lander, imaged by Rosetta’s OSIRIS narrow-angle camera on 2 September 2016 from a distance of 2.7 km. The image scale is about 5 cm/pixel. Philae’s 1 m-wide body and two of its three legs can be seen extended from the body. The images also provide proof of Philae’s orientation.
The image is a zoom from a wider-scene, and has been interpolated.
Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

“With only a month left of the Rosetta mission, we are so happy to have finally imaged Philae, and to see it in such amazing detail,” says Cecilia Tubiana of the OSIRIS camera team, the first person to see the images when they were downlinked from Rosetta yesterday.

“After months of work, with the focus and the evidence pointing more and more to this lander candidate, I’m very excited and thrilled that we finally have this all-important picture of Philae sitting in Abydos,” says ESA’s Laurence O’Rourke, who has been coordinating the search efforts over the last months at ESA, with the OSIRIS and SONC/CNES teams.

Philae was last seen when it first touched down at Agilkia, bounced and then flew for another two hours before ending up at a location later named Abydos, on the comet’s smaller lobe.

After three days, Philae's primary battery was exhausted and the lander went into hibernation, only to wake up again and communicate briefly with Rosetta in June and July 2015 as the comet came closer to the Sun and more power was available.

An OSIRIS narrow-angle camera image taken on 2 September 2016 from a distance of 2.7 km in which Philae was definitively identified. The image has been processed to adjust the dynamic range in order to see Philae while maintaining the details of the comet’s surface. Philae is located at the far right of the image, just above centre. The image scale is about 5 cm/pixel. Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

An OSIRIS narrow-angle camera image taken on 2 September 2016 from a distance of 2.7 km in which Philae was definitively identified. The image has been processed to adjust the dynamic range in order to see Philae while maintaining the details of the comet’s surface. Philae is located at the far right of the image, just above centre. The image scale is about 5 cm/pixel. Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

However, until today, the precise location was not known. Radio ranging data tied its location down to an area spanning a few tens of metres, but a number of potential candidate objects identified in relatively low-resolution images taken from larger distances could not be analysed in detail until recently.

While most candidates could be discarded from analysis of the imagery and other techniques, evidence continued to build towards one particular target, which is now confirmed in images taken unprecedentedly close to the surface of the comet.

At 2.7 km, the resolution of the OSIRIS narrow-angle camera is about 5 cm/pixel, sufficient to reveal characteristic features of Philae’s 1 m-sized body and its legs, as seen in these definitive pictures.

“This remarkable discovery comes at the end of a long, painstaking search,” says Patrick Martin, ESA’s Rosetta Mission Manager. “We were beginning to think that Philae would remain lost forever. It is incredible we have captured this at the final hour.”

“This wonderful news means that we now have the missing ‘ground-truth’ information needed to put Philae’s three days of science into proper context, now that we know where that ground actually is!” says Matt Taylor, ESA’s Rosetta project scientist.

A number of Philae’s features can be made out in this image taken by Rosetta’s OSIRIS narrow-angle camera image on 2 September 2016. Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

A number of Philae’s features can be made out in this image taken by Rosetta’s OSIRIS narrow-angle camera image on 2 September 2016, including one of the CIVA panoramic imaging cameras, the SD2 drill and SESAME-DIM (Surface Electric Sounding and Acoustic Monitoring Experiment Dust Impact Monitor). Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

"Now that the lander search is finished we feel ready for Rosetta's landing, and look forward to capturing even closer images of Rosetta's touchdown site,” adds Holger Sierks, principal investigator of the OSIRIS camera.

The discovery comes less than a month before Rosetta descends to the comet’s surface. On 30 September, the orbiter will be sent on a final one-way mission to investigate the comet from close up, including the open pits in the Ma’at region, where it is hoped that critical observations will help to reveal secrets of the body’s interior structure.

Further information on the search that led to the discovery of Philae, along with additional images, will be made available soon.

 

For contact information, please see the story on the main ESA web portal.

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Jupiter’s north pole


Jupiter's north pole
NASA's Juno spacecraft captured this view as it closed in on Jupiter's north pole, about two hours before closest approach on Aug. 27, 2016.
Credits: NASA/JPL-Caltech/SwRI/MSSS

Jupiter's polar cloud tops
Juno was about 48,000 miles (78,000 kilometers) above Jupiter's polar cloud tops when it captured this view, showing storms and weather unlike anywhere else in the solar system.
Credits: NASA/JPL-Caltech/SwRI/MSSS

Infrared image of Jupiter's southern aurora
This infrared image from Juno provides an unprecedented view of Jupiter's southern aurora. Such views are not possible from Earth.
Credits: NASA/JPL-Caltech/SwRI/MSSS

NASA’s Juno spacecraft has sent back the first-ever images of Jupiter’s north pole, taken during the spacecraft’s first flyby of the planet with its instruments switched on. The images show storm systems and weather activity unlike anything previously seen on any of our solar system’s gas-giant planets.

Juno successfully executed the first of 36 orbital flybys on Aug. 27 when the spacecraft came about 2,500 miles (4,200 kilometers) above Jupiter’s swirling clouds. The download of six megabytes of data collected during the six-hour transit, from above Jupiter’s north pole to below its south pole, took one-and-a-half days. While analysis of this first data collection is ongoing, some unique discoveries have already made themselves visible.

“First glimpse of Jupiter’s north pole, and it looks like nothing we have seen or imagined before,” said Scott Bolton, principal investigator of Juno from the Southwest Research Institute in San Antonio. “It’s bluer in color up there than other parts of the planet, and there are a lot of storms. There is no sign of the latitudinal bands or zone and belts that we are used to -- this image is hardly recognizable as Jupiter. We’re seeing signs that the clouds have shadows, possibly indicating that the clouds are at a higher altitude than other features.”

One of the most notable findings of these first-ever pictures of Jupiter’s north and south poles is something that the JunoCam imager did not see.

“Saturn has a hexagon at the north pole,” said Bolton. “There is nothing on Jupiter that anywhere near resembles that. The largest planet in our solar system is truly unique. We have 36 more flybys to study just how unique it really is.”

Along with JunoCam snapping pictures during the flyby, all eight of Juno’s science instruments were energized and collecting data. The Jovian Infrared Auroral Mapper (JIRAM), supplied by the Italian Space Agency, acquired some remarkable images of Jupiter at its north and south polar regions in infrared wavelengths.

“JIRAM is getting under Jupiter’s skin, giving us our first infrared close-ups of the planet,” said Alberto Adriani, JIRAM co-investigator from Istituto di Astrofisica e Planetologia Spaziali, Rome. “These first infrared views of Jupiter’s north and south poles are revealing warm and hot spots that have never been seen before. And while we knew that the first-ever infrared views of Jupiter's south pole could reveal the planet's southern aurora, we were amazed to see it for the first time. No other instruments, both from Earth or space, have been able to see the southern aurora. Now, with JIRAM, we see that it appears to be very bright and well-structured. The high level of detail in the images will tell us more about the aurora’s morphology and dynamics.”

Among the more unique data sets collected by Juno during its first scientific sweep by Jupiter was that acquired by the mission’s Radio/Plasma Wave Experiment (Waves), which recorded ghostly-sounding transmissions emanating from above the planet. These radio emissions from Jupiter have been known about since the 1950s but had never been analyzed from such a close vantage point.

“Jupiter is talking to us in a way only gas-giant worlds can,” said Bill Kurth, co-investigator for the Waves instrument from the University of Iowa, Iowa City. “Waves detected the signature emissions of the energetic particles that generate the massive auroras which encircle Jupiter’s north pole. These emissions are the strongest in the solar system. Now we are going to try to figure out where the electrons come from that are generating them.”

The Juno spacecraft launched on Aug. 5, 2011, from Cape Canaveral, Florida and arrived at Jupiter on July 4, 2016. JPL manages the Juno mission for the principal investigator, Scott Bolton, of Southwest Research Institute in San Antonio. Juno is part of NASA's New Frontiers Program, which is managed at NASA's Marshall Space Flight Center in Huntsville, Alabama, for NASA's Science Mission Directorate. Lockheed Martin Space Systems, Denver, built the spacecraft. Caltech in Pasadena, California, manages JPL for NASA.

More information on the Juno mission is available at these sites:

http://www.nasa.gov/juno

http://missionjuno/org

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Brain Engineering Research Center


Ph.D Research Opportunities
 

Job description: Brain engineering research center is providing an excellent opportunity for PhD students who are interested in systems/cognitive neuroscience for performing his/her research dissertations at IPM. The lab is broadly interested in vision and neural engineering with a specific focus on electrophysiological studies on primate vision, computational neuroscience, and visual prosthesis. The candidates should be a PhD student in electronic and computer engineering or basic science such as mathematics and neuroscience. 


Benefits: The ideal applicants will be supervised by Dr. Reza Lashgari, Prof. Jose Manuel Alonso, and Prof. Jacqueline Gottlieb. The candidate students will be supported financially for three years academic research program. We also provide an opportunity for candidates to attend to the partner labs abroad for 6 months. 


General requirements 

  • Good scientific communication and ability to work in team
  • Fluent in spoken and written English
  • Full time available in the lab
  • Interest in neuroscience

Special skill requirements 

  • For computer engineering PhD students strong programming skills, familiarity with software methodology, and a background in pattern recognition, machine learning, or image processing is needed.
  • For electrical engineering PhD students strong background in electronics, good knowledge about VLSI and MEMSs and skills in digital signal processing is needed.
  • For neuroscience PhD students strong background in physiology or biology, general knowledge in electrophysiology, and familiarity with signal processing and Matlab is needed.
  • For mathematics PhD students strong programming skills and familiarity with general biological modeling techniques (e.g. probability, statistics, dynamical system, graph theory, topology) is needed.

Contact: If interested, please send a CV, brief statement of previous research work and current research interest, and two letters of recommendation to Dr. Reza Lashgari (rezalashgari@ipm.ir). 


http://braineng.ipm.ac.ir


گذراندن پایان نامه دانشجوی دکتری در مرکز مهندسی عصبی پژوهشگاه دانش های بنیادی 


شرح فرصت: آزمایشگاههای تخصصی الکتروفیزیولوژی نخستیان (پریمات) و واسطه های عصبی مهندسی عصبی واقع در پژوهشگاه دانشهای بنیادی از بین افراد واجد شرایط در مقطع دکتری مهندسی برق، کامپیوتر ، ریاضی، فیزیک و نوروساینس به منظور پژوهش و انجام رساله دکتری خود دانشجو می پذیرد. در آزمایشگاه های مذکور، با استفاده از ثبت نورونی از قشر اولیه بینایی میمونهای هوشیار و بیهوش به مطالعه مدارهای نورونی دخیل در سیستم بینایی پرداخته خواهد شد. بطوریکه با ثبت الکتروفیزیولوژی از سیگنالهای نورونی و ارایه مدلهای محاسباتی به نگاشت دقیق از عملکرد نورونهای کورتکس اولیه بینایی پرداخته تا با نگرش مهندسی طراحی و ساخت پروتز های مغزی نقش بسزایی را در درمان اختلالات بینایی و شناختی فراهم سازیم. در آزمایشگاه واسطه های عصبی نیز با استفاده از طراحی آرایه های چندگانه الکترودی و کنترل جابجایی الکترودها به روش بیسیم به مطالعات سیستمیک مدارهای شناختی نورونی قشر مغز و هسته های نورونی زیر قشر مغز پرداخته خواهد شد. 


مزایا: دانشجویان دکتری برای مدت سه سال از حمایت مالی حق التحقیق به منظور فعالیت پژوهشی برخوردار خواهند شد و همچنین فرصت مرکز گذراندن دوره شش ماه در آزمایشگاههای خارج از کشور که با مرکز مهندسی عصبی همکاری پژوهشی دارند را برای دانشجویان فراهم خواهد ساخت. 


شرایط عمومی: 


  • مهارت برقراری ارتباط علمی و توانایی انجام کار تیمی از قبیل بحث های علمی هفتگی و ماهانه
  • تسلط به زبان انگلیسی و ارتباط مکالمه اسکایپ با اساتید خارجی
  • کار تمام وقت در آزمایشگاه
  • علاقه به رشته علوم اعصاب

شرایط تخصصی: 

  • برای دانشجویان دکتری رشته مهندسی کامپیوتر، مهارتهای برنامه نویسی، آشنایی با متدولوژی مهندسی نرم افزار و پیش زمینه در یکی از فیلدهای بازشناسی الگو، یادگیری ماشین، یا پردازش تصویر ضروری است.
  • برای دانشجویان دکتری رشته مهندسی برق، پیش زمینه در الکترونیک، دانش در زمینه های VLSI و MEMSs، و مهارتهای پردازش سیگنال دیجیتال ضروری است.
  • برای دانشجویان رشته علوم اعصاب، پیش زمینه قوی در زیست یا فیزیولوژی، دانش عمومی الکتروفیزیولوژی، و آشنایی با پردازش سیگنال در زبان متلب ضروری است.
  • برای دانشجویان دکتری رشته ریاضی، مهارتهای برنامه نویسی و آشنایی با روشهای عمومی مدلهای ریاضی پدیده های زیستی (مثل آمار، احتمال، سیستمهای دینامیکی، نظریه گراف و توپولوژی) ضروری است.


تماس: دانشجویان متقاضی در صورت تمایل به فعالیت پژوهشی در مرکز مهندسی عصبی، رزومه و خلاصه ای از فعالیت تحقیقاتی گذشته خود به همراه دو توصیه نامه را به آدرس ایمیل rezalashgari@ipm.ir ارسال نمایند. 




Ph.D Research Opportunities 

  • Brain Engineering Research Center


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Revealing Saturn: Cassini Science Highlights and the Grand Finale

Revealing Saturn: Cassini Science Highlights and the Grand Finale

September 22 & 23

The Cassini mission’s findings have revolutionized our understanding of Saturn, its complex rings, the amazing assortment of moons and the planet’s dynamic magnetic environment. The robotic spacecraft arrived in 2004 after a 7-year flight from Earth, dropped a parachuted probe named Huygens to study the atmosphere and surface of Saturn’s big moon Titan, and commenced making astonishing discoveries that continue today.

Cassini’s current mission extension has led to some remarkable discoveries and more are expected when Cassini repeatedly dives between the innermost ring and the top of Saturn’s atmosphere during its final six months starting in April 2017. Late last year Cassini completed its final equatorial tour of Saturn’s icy satellites, culminating in a series of Enceladus encounters including a daring pass through the icy moon’s southern jets and plume.

The mission then began executing a series of Titan flybys, each of which increases the spacecraft’s inclination until it finally reaches nearly 64 degrees. At that point, in late November, the Cassini mission will embark on its final set of orbits: 20 F ring orbits with a periapsis just outside Saturn’s F ring, 22 Proximal orbits, the Grand Finale, with periapsis between the innermost D ring and Saturn, and finally, entry into Saturn’s atmosphere in September 2017.

What new puzzles will Cassini solve before it plunges into Saturn’s atmosphere rather than risk crashing into one of Saturn’s ocean worlds and contaminating it? Come and hear the story of recent science discoveries and the upcoming excitement during the final orbits. Dr. Linda Spilker, Cassini Project Scientist, will present highlights of Cassini’s ambitious inquiry at Saturn and an overview of science observations in the final orbits. Dr. Earl Maize will discuss Cassini’s exciting challenges and promise of the final year of the mission, ultimately flying through a region where no spacecraft has ever flown before.

This flagship mission is a cooperative undertaking by NASA, the European Space Agency (ESA), and the Italian space agency (Agenzia Spaziale Italiana (ASI)).

Speaker:
Dr. Earl Maize, Cassini Project Manager, JPL
Dr. Linda Spilker, Cassini Project Scientist, JPL

JPL
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What 10 Years at Mars Can Tell Us About the Planet In the Blink of the Eye: What 10 Years at Mars Can Tell Us About the Planet

What 10 Years at Mars Can Tell Us About the Planet

In the Blink of the Eye: What 10 Years at Mars Can Tell Us About the Planet

March 24 & 25

Our eyes in the sky at Mars include the Mars Reconnaissance Orbiter, which has been orbiting Mars for 10 years. 

The orbiter has sent back thousands of high-resolution images and more data than all Mars missions combined and: 

• Found the strongest evidence yet that liquid water flows intermittently on present-day Mars
• Found evidence of diverse watery environments on early Mars, some more habitable than others
• Caught avalanches and dust storms in action
• Seen seasonal changes and longer-term changes over the last decade 

On Aug. 12, 2005, the Mars Reconnaissance Orbiter (MRO) lifted off from Cape Canaveral Air Force Station. Seven months later, the orbiter arrived at Mars. Thus began an incredible journey of exploration, guided by the Mars Exploration Program’s “follow-the-water” theme. 

Originally slated for a two-year prime science mission followed by a two-year relay mission, MRO has logged more than a decade of science operations and support for surface missions. MRO has probed the planet’s atmosphere, surface and subsurface with unprecedented spatial resolution and coverage. Its seven science investigations and six instruments have returned more than 250 terabits of data, enabling numerous discoveries. Among them, MRO has found evidence for a variety of water-laden environments dating to early Mars, and enough carbon dioxide ice buried in the south polar cap to double the current atmosphere if it were released in gaseous form. The orbiter has revealed a planet with a surface that is active today, decorated by moving dunes and mysterious strips that appear to be brine flows. 

At the same time, MRO has rendered invaluable service to landers and rovers at Mars. It not only delivered critical information for the selection of landing sites, but captured crucial data and historic images during the arrivals of the Phoenix lander and Mars Science Laboratory. Since then, MRO has frequently served as a relay for data and commands between those spacecraft and Earth. As NASA’s Mars Exploration Program looks to the future, MRO continues to characterize and certify new landing sites for both NASA and the European Space Agency, while preparing to cover critical events and landed operations for the InSight lander, Mars 2020 rover, and future missions.

Speaker:
Dr. Leslie Tamppari, MRO deputy project scientist

Webcast:
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Is the Solar System's Galactic Motion Imprinted in the Phanerozoic Climate

A new δ18O Phanerozoic database, based on 24,000 low-Mg calcitic fossil shells, yields a prominent 32 Ma oscillation with a secondary 175 Ma frequency modulation. The periodicities and phases of these oscillations are consistent with parameters postulated for the vertical motion of the solar system across the galactic plane, modulated by the radial epicyclic motion.

The Milky Way is a barred spiral galaxy. As a consequence, the solar system revolves around the galaxy and carries out a small oscillation in the direction perpendicular to the dense galactic disk, with a period much shorter than its orbital period




http://www.nature.com/articles/srep06150

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ESA Citizens’ Debate Project

article (495×330)


On 10 September 2016 about 2000 citizens from 22 European countries will

participate in the first Citizens’ Debate on Space for Europe.In the course of the day, citizens will have the opportunity to learn, debate, have their say and participate by suggesting priorities on all aspects of current and future space programmes.

This consultation on an unprecedented scale will take place simultaneously in all 22 Member States of the European Space Agency (ESA).  Missions Publiques, the company that has been brought in by ESA to organise this consultation and conduct the debate, will gather approximately 100 citizens per Member State at various locations. Those selected will be as representative as possible of the population of their country according to socio-demographic criteria.  The results of the consultation will be collated – as early as 48 hours after the debate takes place – and communicated to ESA.

Referring to this initiative, ESA Director General Jan Woerner, emphasised his commitment to ESA being more open to society and to further engaging in a dialogue with European  citizens, and said, “Spaceflight, space science, exploration, Earth observation, telecommunication, satellite navigation, space technology and innovation can all help respond to societal challenges and be a source of inspiration to future generations. European citizens can help us  better assess our priorities”.

The Citizens’ Debate on Space for Europe is a major first – never before has the future of space activities been addressed in such an event held across so many countries.

For more information,  and to apply  to take part in the debate, visit http://citizensdebate.space


About the European Space Agency

The European Space Agency (ESA) provides Europe’s gateway to space.

ESA is an intergovernmental organisation, created in 1975, with the mission to shape the development of Europe’s space capability and ensure that investment in space delivers benefits to the citizens of Europe and the world.

ESA has 22 Member States: Austria, Belgium, the Czech Republic, Denmark, Estonia, Finland, France, Germany, Greece, Hungary, Ireland, Italy, Luxembourg, the Netherlands, Norway, Poland, Portugal, Romania, Spain, Sweden, Switzerland and the United Kingdom, of whom 20 are Member States of the EU.

ESA has established formal cooperation with seven other Member States of the EU. Canada takes part in some ESA programmes under a Cooperation Agreement.

By coordinating the financial and intellectual resources of its members, ESA can undertake programmes and activities far beyond the scope of any single European country. It is working in particular with the EU on implementing the Galileo and Copernicus programmes.

ESA develops the launchers, spacecraft and ground facilities needed to keep Europe at the forefront of global space activities.

Today, it develops and launches satellites for Earth observation, navigation, telecommunications and astronomy, sends probes to the far reaches of the Solar System and cooperates in the human exploration of space.

Learn more about ESA at www.esa.int

About Missions Publiques

Missions Publiques is a company specialised in citizen participation and policy dialogue with more than fifteen years of experience in this innovative field. Its team has expertise at local, national, European and global level. Missions Publiques has cooperated with 20 different organisations  in helping  to implement  the Citizens' Debate on Space for Europe across ESA Member States.

For further information, please contact:

Nathalie Meusy

ESA Citizens’ Debate Project Manager

Email: contact@citizensdebate.space


The Citizens' Debate on Space for Europe is a unique - indeed the first instance of a - consultation organized in every member state of the European Space Agency. Over 2000 citizens selected to reflect the socio-demographic diversity of their country will debate on space matters during a day-long meeting. In order to consolidate the 22 national results reports into one European report, all debates will follow the same instructions and answer the same set of questions. 
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This consultation on unprecedented scale is organised by Missions Publiques, a company specialised in citizen participation, with 20 partners, on behalf of ESA. ESA intends to take in new actors to develop its future orientation and nurture its strategy. It is crucial to the Agency to involve more actors, especially citizens, in choices that will respond to societal challenges, put space at their service and impact coming generations through space innovation, exploration and international space cooperation.

http://www.citizensdebate.space/en_GB
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