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  • The spirit of Carl Sagan Day

    "A Glorious Dawn": Carl Sagan's words are set to music by SymphonyofScience.com.

    It was 77 years ago today that astronomer Carl Sagan was born, and 15 years ago that he passed away after a long struggle with bone marrow disease. For a while, Sagan's rich legacy was commemorated on the date of his death, but in recent years, his fans have wisely focused on his birthdate instead. In celebration of his life, Saganites are screening episodes of his well-known TV documentary series, "Cosmos" ... planning parties with cosmic speakers ... and making apple pies from scratch. (First step: Invent the universe).

    If anything, the astronomer's legacy has grown in recent years, as a new generation gets in touch with his easy way of communicating scientific perspectives to the public as well as his deep spirituality. Spirituality? That may come as a surprise to some, who view Sagan as a sharp-edged critic of religion in a "Demon-Haunted World." But his meditation on our "Pale Blue Dot" could well rank as one of the most spiritual essays of the 20th century. To find out more of that side of Sagan's legacy, check out "The Varieties of Scientific Experience," a book based on a series of talks he gave in 1985.

    There'll be more for Saganites to cheer in the years ahead: A new version of "Cosmos" is being readied for prime-time TV in 2013, with astronomer Neil deGrasse Tyson as host. Back in August, Tyson told me that he would bring his own style to the new show while preserving the Sagan spirit. "What people remember the most about 'Cosmos,' and what it did best, and what I don't think has been duplicated, is the effort to convey the meaning of science to a citizen of planet Earth," Tyson said. "'Cosmos' brought science to the public in a way that meant something to their relationship to each other, to the world and to the universe."

    What does Sagan's legacy mean to you? Feel free to share your thoughts on this Sagan Day, in the comment space below.

    More reflections on Carl Sagan Day:


    Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter or following the Cosmic Log Google+ page. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for new worlds.

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  • EV gets 350 mpg, wins race

    Gordon Murray Design

    Gordon Murray Design's T.27 (right) won the Royal Automobile Club's Future Car Challenge, getting the equivalent of 350 miles per gallon on the just under 60 mile course.

    An electric vehicle designed by a former Formula 1 racecar designer sipped its way to first place in a showcase race for cars of the future by getting the equivalent of 350 miles per gallon on the 57.13 mile course.

    The two-seater T.27 by Gordon Murray Design covered the route from Brighton to London within the allocated time of the Royal Automobile Club's Future Car Challenge, which includes a pit-stop at Central Sussex College.


    The winner isn't the first to cross the finish line; it's the team that does it using the least amount of energy. Gordon Murray's car bested entries from major manufacturers including the Nissan, BMW, Toyota, Volkswagen and Peugeot. 

    The T.27 completed the course using just 7 kilowatt hours of electricity, which the company says is 64 pence ($1.03) worth of energy and the equivalent of 350 miles per gallon. 

    The car's actual battery has a range of just 100 miles, similar to the Nissan Leaf, though at about half the size takes 4 hours to charge on a domestic socket.

    Second place in the competition went to a Jaguar E-Type from Germany that consumed 8.5 kilowatt hours and third place a smart fortwo coup EV, which sipped 9.7 kilowatt hours. (Full results here.)

    Murray's advantage over other cars includes a lightweight design and a proprietary manufacturing process that brings Formula One technology to everyday motorists. Lightweight materials, he notes, are the most powerful tool for solving the world's energy problems.

    This sentiment has been seen elsewhere in the automotive sector, including the package delivery company UPS, which is road-testing trucks made with composite body panels that make it 1,000 pounds lighter than comparable models.

    [Via: Forbes]

    More on cars of the future:


    John Roach is a contributing writer for msnbc.com. To learn more about him, check out his website. For more of our Future of Technology series, watch the featured video below.

     

     

    As the over-65 population expands, new gadgets and systems will allow seniors to live at home and receive improved healthcare. From sleep-sensing beds to robots piloted by grandchildren, we look at how "health surveillance" can improve quality of life.

  • Are alien probes lost in space?

    NASA file

    An alien artifact like the Voyager probes' "Golden Record," which contains coded information about Earth as well as recordings of earthly sights and sounds, would probably elude our attention if it were in our solar system. In fact, we might not even detect the Voyager probes.

    After analyzing our capability to detect objects in the solar system, researchers have come to a conclusion that should be fairly obvious: Even if extraterrestrials left something in our solar system like the artifacts we’ve sent out into deep space, we almost certainly wouldn’t know they were there.

    "The vastness of space, combined with our limited searches to date, implies that any remote unpiloted exploratory probes of extraterrestrial origin would likely remain untouched," Penn State researchers Jacob Haqq-Misra and Ravi Kumar Kopparapu write in a paper accepted for publication by the journal Acta Astronautica.

    The claim that there are plenty of places where alien robots or monoliths could lurk comes as no surprise to Douglas Vakoch, director of interstellar message composition at the California-based SETI Institute. "That's standard wisdom in the field," he told me today.

    Our messages to the cosmos
    The latest research quantifies just how unexplored different parts of our solar system are, but the bottom line is that we haven't searched the prime areas closely enough — particularly if we're looking for objects ranging from 1 to 10 meters (3 to 33 feet) in size. That's roughly the size range for the human-made objects that are on their way out of the solar system, including the Pioneer and Voyager probes.

    Those particular '70s-era spacecraft were equipped with objects that could conceivably tell extraterrestrial civilizations that intelligent entities inhabited at least one planet in our solar system: The Pioneer 10 and 11 probes carried plaques that bore pictures of a human male and female, along with symbols representing our cosmic location. The Voyager spacecraft had "Golden Records," pictogram-bearing phonograph records that could be played to reveal the sights and sounds of Earth.

    Haqq-Misra and Kopparapu imply that if the aliens were like us, they wouldn't be able to pick out the Pioneer and Voyager spacecraft, let alone the plaques and the records. "Few if any of the attempts would be capable of detecting a 1 to 10 meter probe," they write.

    Even if an alien object were left on Earth, it's not 100 percent certain that it could be found. "The surface of the Earth is one of the few places in the solar system that has been almost completely examined at a spatial resolution of less than 3 feet," the researchers write. Nevertheless, non-terrestrial objects could lurk on the ocean floor, or in the depths of a jungle, or inside a deep cave. There's even a chance that the probe would just look like a rock.

    And when you're talking about the whole solar system, the task is analogous to "finding a needle in a thousand-ton haystack," the researchers write.

    Signals vs. artifacts
    Vakoch said that's why scientists involved in the search of extraterrestrial intelligence, or SETI, tend to focus on radio signals (or laser pulses) rather than physical artifacts. "It's much less energetically expensive," he said. "In a way, it's easier to search for intelligence across the galaxy than it is in our backyard."

    Similarly, SETI researchers don't hold out much hope that E.T. will come across our the Pioneer plaques or the Golden Records, much less figure them out. "There's a minuscule chance that any of the things we've sent so far will ever be detected by even the hardiest extraterrestrial civilizations," Vakoch said.

    Vakoch observed that the research suggests "one possible response to the Fermi Paradox." Back in 1950, physicist Enrico Fermi and his colleagues discussed the prospects for alien life, and speculated that if intelligent beings could arise in other planetary systems, there should have been enough time for them to visit Earth many times over millions of years. "Where are they?" Fermi is said to have asked.

    Haqq-Misra and Kopparapu propose an answer of sorts: "Searches to date of the solar system are sufficiently incomplete that we cannot rule out the possibility that non-terrestrial artifacts are present and may even be observing us," they write.

    Maybe there's a cast-off alien plaque sitting just over a hill somewhere on Mars ("We Came in Peace for All Blurxkind"). Or maybe the latest "Transformers" movie had it right after all. What do you think? Feel free to weigh in with your comments below.

    More on the alien search:


    Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter or following the Cosmic Log Google+ page. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for new worlds.

  • Passing asteroid puts on a show

    Watch a six-frame video showing the spin of asteroid 2005 YU55 on Nov. 7 as it closed in for an encounter with Earth. The radar imagery was produced by NASA's Goldstone radio telescope.

    Astronomers watched the asteroid 2005 YU55 spin as it zoomed harmlessly past Earth, and everybody else was looking over their shoulders. You can expect to see a huge pile of pictures now that the coal-dark space rock has passed by.

    Even before the closest pass, NASA's Jet Propulsion Laboratory provided a six-frame "movie" based on radar data acquired by the Goldstone radio telescope on Monday. This sequence was captured from a distance of 860,000 miles (1.38 million kilometers).

    The closest approach to Earth came at 6:28 p.m. ET Tuesday, when the quarter-mile-wide (400-meter-wide) asteroid slipped just barely within the orbit of the moon at a distance of 198,000 miles (319,000 kilometers). YU55 is due to come closest to the moon at 2:14 a.m. ET Wednesday, NASA said.

    Neither the moon nor Earth was at risk during this flyby, but the information gathered this time around could help astronomers know what they're dealing with during potentially riskier encounters.


    Here's a parting shot of YU55 from the 25-inch telescope at the Clay Center Observatory in Massachusetts, which tracked the asteroid as it swept past at 29,000 mph:

    Clay Center Observatory

    The speck near the center of this image is 2005 YU55 at the time of closest approach. The bright streaks are background stars.

    In a Twitter update, NASA said that YU55 will make its next Earth flyby in 2015, "but at a greater distance than today." Today's encounter wasn't close enough to perturb the near-Earth asteroid's orbit, but experts are wondering whether a close flyby of Venus in 2029 will change its orbital path slightly.

    Even if that Venus encounter does cause a change, Earth is in no danger from this particular space rock, at least for the next 100 years or so. Which is a good thing. If an object the size of YU55 were to hit land, experts say it would blast a 4-mile-wide, 1,700-foot-deep crater and set off a 7.0 earthquake. If it hit at sea, it would create a catastrophic tsunami with 70-foot-high waves.

    NBC's George Lewis reports on asteroid 2005 YU55's flyby.

    The last time an asteroid as big as YU55 came this close was in 1976, and the next time will be in 2028 — or could it be sooner? Scientists recently estimated that thousands of asteroids around the size of YU55 remain to be discovered, so learning about this rock's composition and motion could help us deal with many other rocks to come. 

    YU55 is particularly interesting because it has a high carbon content, which makes it coal-black. Such carbonaceous chondrites have been found to contain amino acids, and may have played a role in the origin of life on Earth. NASA's Osiris-Rex mission, due for launch in 2016, will target a carbonaceous asteroid called 1999 RQ36 and try to bring a sample back to Earth for study.

    NASA's current space vision calls for sending astronauts to a near-Earth asteroid sometime in the mid-2020s, and the head of NASA's Near Earth Object Program, Don Yeomans, said that if he got the chance to decide the destination, he'd pick a carbon-bearing rock like YU55.

    "This would be an ideal object," he told The Associated Press.

    Still more about the encounter:


    Correction for 3:45 p.m. ET: I originally wrote that the Clay Center Observatory's telescope was a 15-incher, but it's actually a 25-incher.

    Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter or following the Cosmic Log Google+ page. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for new worlds.

  • Poop-to-power projects pumped up

    Vickie Chachere / USF News

    University of South Florida associate professor Daniel Yeh has worked on developing the NEWgenerator, which harvests clean water, methane and nutrients from sewage, for nearly a decade.

    Innovators from around the world who see power in steaming piles of poop are getting serious money from Microsoft billionaire Bill Gates' foundation to help the world's 2.1 billion urban dwellers without access to sewers live safer, more sanitary and electrified lives.

    Grantee Daniel Yeh, a civil and environmental engineer at the University of South Florida, for example, will use the funds to field test an advanced technology that harvests nutrients, energy, and water from wastewater.


    Known as the NEW generator, it uses anaerobic microorganisms — those that live in the absence of oxygen — to convert organic material into methane, which is natural gas, and a membrane that filters out viruses and bacteria, leaving only water enriched with the nutrients ammonia and phosphorous.

    "In the lab, we can already turn wastewater into methane and we can already recover the ammonia and phosphorus into a clean water solution that looks crystal clear, just like tap water," Yeh told me. "The only difference is it has ammonia and phosphorus in it."

    Those two nutrients are crucial for growing crops. So this water would be ideal for irrigation, freeing farmers from synthetic ammonia fertilizer, which is energy intensive to make, and phosphorus, which is a finite mined resource, Yeh added.

    He and his colleagues will use the $100,000 grant from the Bill and Melinda Gates Foundation to build a field unit and demonstrate the technology at the environmentally progressive Learning Gate Community School in Florida.

    Sanitation grants
    The project is one of 31 announced Monday by the Seattle-based global health organization for its next generation sanitation technologies as part of a larger round of grants awarded in the Grand Challenges Explorations program.

    Untreated fecal sludge contaminates water used for everything from irrigation and bathing to dishwashing and drinking. An estimated 1.6 million children die each year from diarrheal disease, many caused by fecal-oral contamination, according to the Bill and Melinda Gates Foundation.

    Among the 30 other projects receiving funding for next generation sanitation technologies are:

    • Entrepreneur Jason Aramburu's re:char technology that aims to convert human waste into biochar, which can be used as a replacement for chemical fertilizer or charcoal.
    • Environmental and sustainability engineer Zhiyong Ren at the University of Colorado Denver will develop a low-cost and easy-to-operate bioelectric system that uses microbes to breakd waste and convert it to useable electricity.
    • Chemist Steven Cobb at Durham University in the United Kingdom aims to develop a "macroporous" scaffold that can support bacterial cells and metal nanoparticles that work together to catalyze conversion of fecal sludge into hydrogen for electricity.
    • Roboticist Ioannnis Ieropoulos at the University of Bristol will test the ability of microbial fuel cells to convert urine and sludge into electrical energy while purifying water and killing pathogens.
    • And engineer Yinije Tang at Washington University in St. Louis will develop a genetically engineered fungal species that can convert fecal sludge into butanol, a biofuel similar to gasoline.

    While we've seen plenty of poop to power projects over the years, all of the ideas fit the Gates Foundation's requirement for proposals designed for low income urban settings, where demand for fecal sludge emptying and treatment are high.

    According to the Gates Foundation, the indiscriminate dumping of a truckload of fecal sludge is the equivalent of 5,000 people openly defecating. Harvesting the energy and nutrients in that sludge, noted Yeh, could help solve some of the world's greatest challenges: energy and food.

    "Wherever people live, there's wastewater. It's a 24/7 thing," he said. "Why don't we connect the whole picture together and close the loop."

    More on poop to power:


    John Roach is a contributing writer for msnbc.com. To learn more about him, check out his website. For more from our Future of Technology series, watch the featured video below.

    As the over-65 population expands, new gadgets and systems will allow seniors to live at home and receive improved healthcare. From sleep-sensing beds to robots piloted by grandchildren, we look at how "health surveillance" can improve quality of life.

     

  • Your guide to the asteroid encounter

    NASA releases a new radar image of asteroid 2005 YU55 as it approaches Earth for a Tuesday close encounter. Watch Brian Williams' report for "NBC Nightly News."

    Last updated 5:25 p.m. ET Nov. 8

    The asteroid 2005 YU55 will pose no threat to Earth when it zooms by on Tuesday, but it will spark a frenzy of picture-taking and online chatting. So where do you find the good stuff?

    The hottest action will be up in the sky: This space rock (which we'll call YU55 from here on out) is about a quarter-mile (400 meters) wide, which makes it wider than an aircraft carrier. It's due to zoom past us at 30,000 mph (50,000 kilometers per hour) at a minimum distance of 198,000 miles (319,000 kilometers) at 6:28 p.m. ET. That would bring it just within the orbit of the moon. But don't worry: YU55 is on course to miss the moon as well as Earth, and even if it did hit the lunar surface, the only thing that'd happen would be a fantastic fireworks show.


    Aerospace engineers from Analytical Graphics Inc. created this animation of the asteroid flyby, including a comparison of the asteroid's size with an aircraft carrier. (Courtesy of AGI)

    If YU55 did smash into Earth, it could conceivably turn a city into a smoking crater, or stir up a destructive tsunami. But the asteroid's orbital path doesn't pose any risk in the foreseeable future. It's not expected to have any effect on Earth's tides, or on seismic activity. From the cosmic perspective, this is no big deal. In fact, YU55 has come even closer to Earth over the centuries, but went undetected until just six years ago.

    The fact that YU55 went unnoticed for so long does raise a question, however: What else are we missing out there?

    The science team for NASA's Wide-field Infrared Survey Explorer recently estimated that more than 90 percent of the near-Earth asteroids wider than a kilometer (0.6 miles) have been identified, but that thousands of asteroids in YU55's size range still remain to be detected. That's why astronomers around the world are so interested in watching for YU55 during this go-round. Getting a close look at this space rock should provide good practice for monitoring other potentially hazardous asteroids.

    Asteroid experts say the last time a space rock as big as YU55 came this close was in 1976, and the next time will be in 2028.

    Watching it pass by
    You won't be able to see YU55 zoom by with your naked eye. Even at its closest approach, the asteroid will be no brighter than magnitude 11 — much dimmer than the magnitude-6.5 threshold for naked-eye observations. Astronomers say you'd need something on the order of a 6-inch telescope, and you'd have to know exactly where to look.

    Sky & Telescope's editors have offered viewing advice as well as charts that show YU55's progress through the constellations. If you have your telescope aimed in the right place, you should be able to see a starlike point moving from west to east. "It will be gliding fast enough to move along in real time as you watch using a moderately high-magnification eyepiece," Sky & Telescope says.

    Sky & Telescope

    Best seen from North America, the asteroid 2005 YU55 will race far across the constellations in just 11 hours on the night of Nov. 8-9. The times shown on this chart are GMT. Subtract five hours for Eastern Standard Time. Click on the image for a larger view.

    Some amateur astronomers are involved in an effort to monitor variations in the asteroid's brightness during the encounter. Those variations can be used to determine how YU55 is rotating as it flies by. Check out this Sky & Telescope webpage for details.

    Most of us won't be peering through telescopes when 6:28 p.m. ET rolls around. Instead, we'll be looking for pictures from the professionals. The best pictures are expected to come from radar observations: NASA's Goldstone radio telescope in California and the Arecibo observatory in Puerto Rico are the big guns in this field, but the National Radio Astronomy Organization will be putting other assets on the case as well, including the Green Bank Telescope in West Virginia, the Very Large Array in New Mexico, and the Very Long Baseline Array.

    Other telescopes around the world will be watching as well. The Clay Center Observatory in Massachusetts, which became known for its telescopic imagery of high-flying SpaceShipOne, is planning to track the asteroid on video. Stay tuned for that imagery, which will be streamed online via msnbc.com as well as on Ustream and other outlets.

    Watching it on the Web
    NASA is offering two main portals to asteroid imagery: Asteroid and Comet Watch on the main NASA site, and Asteroid Watch on the Jet Propulsion Laboratory's website. Both those sites should feature the latest and greatest images available to the space agency, and you should be able to see movies of YU55's encounter by late Tuesday or Wednesday.

    NASA has just released a new radar view of the asteroid, produced from Goldstone data at 2:45 p.m. ET Monday when it was about 860,000 miles (1.38 million kilometers) from Earth. The image looks pretty pixellated, but it nevertheless reveals what appear to be lumps and craters on the surface. Arecibo is due to join the observing campaign on Tuesday, and the pictures should get progressively better as the asteroid zooms closer.

    NASA / JPL-Caltech

    The radar image at left shows the asteroid 2005 YU55, as imaged by NASA's Goldstone radio telescope from a distance of 860,000 miles. At right, a diagram shows the asteroid's trajectory past Earth and the moon.

    Another popular place to look for space imagery is SpaceWeather.com, which is already passing along intelligence for the flyby. If amateurs come up with cool pictures of YU55, you can bet some of them will appear on that website. Space.com is keeping close watch on the asteroid encounter, and we'll be sharing the best of their coverage.

    French astrophotographer Thierry Legault has made a name for himself as the chronicler of fast-moving space phenomena, ranging from space shuttles and the International Space Station to high-flying satellites. I'd be surprised if he didn't at least attempt to catch YU55 on video as it flies by. And if you can read German, you'll enjoy science writer Daniel Fischer's live blog of the flyby.

    Share what you see
    Have you got questions about the asteroid, or about asteroids in general? The Washington Post's website is hosting a live online chat at 1:30 p.m. ET Tuesday with Thomas Statler, a planetary scientist with the National Science Foundation. The chat follows up on last week's online encounter with NSF's Scott Fisher and NASA's Don Yeomans.

    JPL's Lance Benner explains what's going on with asteroid 2005 YU55.

    There's a growing buzz about the YU55 encounter on Facebook: You can easily find a whole bunch of event pages. And some wag has already set up a Twitter account for @AsteroidYU55 ("Uncomfortably Close"). For the real lowdown in tweets, do a search on YU55 or #YU55.

    If you've made a great sighting, or even if you've found a great site on the Web, I hope you'll share it with the rest of the class. You can pass along links or observations in your comments below. You can also share comments or pictures via the Cosmic Log Facebook page or our brand-new Google+ page. We may use your submissions in our own follow-up coverage of the Great Asteroid Encounter.

    Update for 11 p.m. ET: Discovery News' Ian O'Neill lets fly with an "Angry Asteroid" mashup.

    More about the encounter:


    Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter or following the Cosmic Log Google+ page. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for new worlds.

  • Gamers create scientific 'recipes'

    UW Center for Game Science / Baker Lab

    Foldit players learn to resolve structural conflicts in a protein molecule due to amino acid size (indicated by spiky red balls in this game visualization).

    Researchers say that players of a protein-folding game called Foldit are coming up with molecular "recipes" that rival their own complex algorithms.

    One of the recipes — a computerized tool called "Blue Fuse," which checks whether a protein molecule is in its highest-scoring configuration — knocked Foldit's creators for a loop. "When I saw the Blue Fuse algorithm, I recognized immediately that it was almost identical in concept to the best algorithm that we developed in my research group over a period of years," David Baker, a biochemist at the University of Washington, told me today.

    It took the players of the Foldit game only about seven months to come up with their version, and they're continuing to improve the recipe.

    "We were shocked to find state-of the art algorithms," Zoran Popovic, director of UW's Center for Game Science and the game's co-creator, said in a university news release.

    UW computer scientist Seth Cooper, Foldit's other co-creator as well as lead designer/developer, said the findings demonstrate the power of collaborative game play for solving scientific problems. "It's a great thing to show what kinds of things video games and gamers can accomplish," he told me.

    The science behind the recipe-writing process is detailed in a research paper published online this week in the Proceedings of the National Academy of Sciences.


    More than a game
    Protein-folding isn't just a game: The structures of protein molecules are the keys to a wide range of biological processes. In a sense, proteins literally serve as "keys" and "locks" to open up cellular pathways, to admit or block viruses, to start or stop the machinery of life. If scientists can gain a better understanding of how those keys and locks work, they could actually design their own molecules for future medications and nanomachines.

    That's where Foldit and other protein-folding software tools can play a huge role. Foldit is a social game based on a computerized molecule-manipulation program called Rosetta, which was developed a decade ago by Baker and his colleagues at UW. The Foldit game has enlisted hundreds of thousands of players who can work together (or compete against each other) to twist and turn virtual molecules and rack up high scores. The scores are based on how well players can fold molecules to produce the lowest-energy state — the state that is preferred in nature.

    Just a couple of months ago, UW researchers credited Foldit players with figuring out the right structure for an enzyme from an AIDS-like virus found in rhesus monkeys. The latest research focuses on the processes used by the players rather than the results.

    Players trade recipes
    Starting in mid-2009, Foldit's developers made it possible for players to create and share their own algorithms for manipulating molecules automatically. The gamers refer to these software routines as "recipes."

    "A lot of them have been shared with their own teammates, of course, and also with the players that they're competing against," UW biochemist Firas Khatib, a co-author for the paper, told me. "In some of the descriptions, they say, 'You might want to put the kettle on for this one,' or 'You might want to let this one run for a few days.'"

    Over the months that followed, Foldit players tinkered with the recipes to produce tastier molecules with less time and effort.

    "The whole thing was a social process," Cooper explained. "It's really drawing on the collective intelligence of the Foldit players as a whole, to come up with the algorithms and also decide which ones are useful."

    Blue Fuse became one of the most popular recipes among the gamers. Khatib said the software tool takes the code for a molecule folded in a particular way, and bends the rules of the game temporarily to check whether there's an even better solution to the puzzle. If there is, the software slowly brings the rules back and heads for that better solution instead. "That's literally how simple the algorithm is, which is why it's so brilliant," Khatib said.

    Researchers conduct cook-off
    It turned out that Blue Fuse was similar to an algorithm in the more sophisticated Rosetta program, known as Fast Relax. That algorithm was a new, improved (but unpublished) version of an older software tool called Classic Relax. The researchers staged a recipe cook-off to see how the three algorithms compared. Blue Fuse took less time to come up with a low-energy solution to a given protein puzzle than Classic Relax, but more time than the improved Fast Relax.

    That wasn't the end of the cook-off, however. "One of the reviewers for our paper pointed out that that's a completely unfair competition," Khatib said.

    The reviewer observed that Fast Relax was taking advantage of software routines in Rosetta that were not available in Foldit. When the UW researchers adapted Fast Relax for the Foldit program, they found that Blue Fuse identified low-energy puzzle solutions faster — although Fast Relax could find even lower-energy solutions if it was allowed to run for more than 200 seconds of CPU time. (The average Blue Fuse runtime during gameplay was 122 seconds.)

    "For 200 seconds and less, Blue Fuse is actually better than Fast Relax," Khatib said. "It optimizes faster."

    Baker said the next step is to give the gamers more power. "What we're doing now is taking many more of the Rosetta options and parameters and exposing them to Foldit players, so that they can use them. ... I'm really excited to see what Foldit players can do once they have access to the full palette of options," he told me.

    He said it won't be all that long before the Foldit players are recruited not only to solve protein-folding puzzles, but also to try out molecular designs that could lead to "new virus inhibitors, new carbon-fixation pathways, new routes to vaccines."

    "We're now learning enough of the rules that we can actually make our own proteins," Baker said.

    Update for 5:45 p.m. ET: The creator of the Blue Fuse "recipe," a Foldit player known as Vertex, was kind enough to answer a few of my questions via email. (Foldit players traditionally prefer not to be identified by their real-world names.) Here's an edited version of the Q&A:

    Cosmic Log: What’s your background? Are you the sort of person who deals with molecule-manipulating algorithms for your day job, or is this something generally foreign to you?

    Vertex: I'm a retired software engineer, so I know nothing about biochemistry. I wrote Blue Fuse primarily to launch new Foldit puzzles — light the blue fuse and stand back. It was quickly taken up by the Foldit community as a credibility test on new protein shapes generated by the rebuild toolset. Its success in this role is far beyond anything I originally imagined or expected, but this is the key strength of the Foldit democracy — it is natural selection at its very best. Dozens of bright ideas are brought to life through the vision, creativity and collaboration of the players. And then, in recipe form, the scripts fly or die when others use them.

    Blue Fuse spawned from Acid Tweeker, a brilliant grandfather script from the genius of Stephen Pletsch, and now has many children of its own. To 'Fuze' has even become a Foldit verb. It's a crazy success story for Blue Fuse, but Foldit is a place where game play meets bioengineering and the next flash of inspiration can come from literally anywhere.

    Q: What process did you use to come up with the algorithm? Is it a question of math, or a question of visualization?

    A: The development of Blue Fuse was a small exercise in statistics. In Foldit there is an adjustable parameter, "clash behavior," that controls how well the Foldit toolset tolerates proximity between protein side chains. Setting the clash behavior low allows the protein to compress, but at the expense of the overall energy score. Blue Fuse manipulates the clash behavior through various compressions and relaxations. I tried different clash values on the start positions of three puzzles and recorded the scores for a wide range of samples. An unexpected result was the discovery that the best clash values were significantly different for the three puzzles, so I had to choose values that on probability gave a good outcome. I could have made Blue Fuse a bigger script with more combinations, but I wanted a quick answer more than anything else.

    Q: Could you explain for a newbie like me exactly what the algorithm does?

    A: The core idea is that the clash behavior is adjusted down to a carefully selected level, and the protein is allowed to compress and is then shaken. The clash behaviour is then set back to normal, and the protein is allowed to decompress. This is very much more gentle on the overall shape of the protein than the scripts that use "bands" to compress the structure — which can cause undesired distortions. Blue Fuse is a deliberately simple set of actions based on this core idea. It has been developed to be fast. It will very quickly let you discover if a new shape is fundamentally OK or not.

    Q: Has the tool evolved substantially since its creation?

    A: Blue Fuse itself has not changed since I posted it, but there are many children citing Blue Fuse as parent, using variations on the core idea. Firas could say how many, but I think it may be as many as 60. I too have a design for a new version of Blue Fuse that will improve its performance — I can't ignore the challenge that Fast Relax is out ahead right now.

    Q: The paper indicates that Blue Fuse and other recipes are used in conjunction with human-guided manipulation, and that it’s not a strictly automatic process. Is that pretty much the way it works? How long does it generally take to run the tool?

    A: Correct. Blue Fuse is typically used by Foldit players to test the results of the rebuild tool. The choice of what section of the protein to rebuild, and which outcomes are worth testing, are normally human decisions. There are very sophisticated recipes that automate these selection tasks and embed "Fuzers" to test outcomes, but they are generally used to fine-tune a shape rather than perform major surgery. A primary goal of Foldit is to capture ways of automating the human element, and huge progress has been made on this, but judgment of good shape remains our edge over the machine.

    The time taken by Blue Fuse varies enormously, depending on the size of the protein and the power of the player's computer. For me it typically takes about a minute. This is fast for a Foldit script.

    Q: I’m wondering if there are things that could be adapted from Blue Fuse to Fast Relax or other tools used in other protein-folding software, or more generally, to mathematics and engineering challenges that aren’t directly connected to protein folding.

    A: Yes. Blue Fuse (and children) and Fast Relax are actually convergent. Everyone competes and collaborates at the same time. Evolution and natural selection will decide the best script.

    Foldit is part of the GWAP ("games with a purpose") world. There are many ways that crowdsourcing through game-play is already bringing a fresh approach to all kinds of academic challenge. Foldit does this supremely well for protein structure. It's an amazing tool. The Foldit community has already solved important biological proteins that previously had unknown structures, and has helped design new proteins for medical research. I would expect this important work to continue strongly in the future, and we will get better at it. I would also expect substantial progress to be made in the automation of protein structure prediction tools — both in Foldit and in the broader academic world, of course.

    More about Foldit and other games with a purpose:


    In addition to Khatib, Cooper, Popovic and Baker, co-authors of "Algorithm Discovery by Protein Folding Game Players" include Michael Tyka, Kefan Xu, Ilya Makedon and Foldit players.  The Foldit project was developed by the UW Center for Game Science in collaboration with UW's Baker Laboratory, with funding from the Defense Advanced Research Projects Agency, the National Science Foundation, the Howard Hughes Medical Institute, Adobe and Microsoft Corp. (Microsoft and NBC Universal are partners in the msnbc.com joint venture.)

    Connect with the Cosmic Log community by "liking" the log's Facebook page or following @b0yle on Twitter. You can also add me to your Google+ circle, and check out "The Case for Pluto," my book about the controversial dwarf planet and the search for new worlds.

  • Tech tracks individuals in a crowd

    EPFL's Computer Vision Laboratory has developed an advanced system for continuous tracking of athletes on the field as well as passers by on the street without the need for RFID tags, even when the subjects overlap or are hidden.

    Ever lost track of your favorite player while watching the game on TV? That frustration could come to an end thanks to a new tracking technology that might also watch your moves at the shopping mall.

    The technology involves multiple cameras and computer algorithms that detect players, predict their trajectories, and identify them based on their uniform color and the number on their shirt.


    On the TV screen, the athletes are represented with a superimposed image bearing their jersey color and number, so that spectators along with referees and coaches can easily follow individuals without mixing them up even when they get buried under a pile of bodies or crouch behind another player.

    This is all done without the aid of RFID chips or other gear that are prohibited by international sporting bodies.

    The system was developed by researchers at Ecole Polytechnique Fédérale de Lausanne in Switzerland and was unveiled today at the International Conference on Computer Vision in Barcelona. Team member Horesh Ben Shitrit describes how this all works in the video at the top of this post. 

    The technology is currently being used to track multiple basketball players in a world championship so that researchers can better understand their behavior. And studying behavior off the court also has appeal.

    "Other applications, like tracking pedestrians to monitor traffic in an area, or following the movement of clients in a store for marketing purposes, are being planned," Ben Shitrit noted in a media release.

    More stories on tracking technology:


    John Roach is a contributing writer for msnbc.com. To learn more about him, check out his website. For more of our Future of Technology series, watch the featured video below.

    As the over-65 population expands, new gadgets and systems will allow seniors to live at home and receive improved healthcare. From sleep-sensing beds to robots piloted by grandchildren, we look at how "health surveillance" can improve quality of life.

     

  • Google wishes scientist Marie Curie a happy 144th birthday

    Google

    Marie Curie was a pioneer in radioactivity research, the first woman to be awarded a Nobel Prize, and the first person to receive Nobel Prizes in two different fields (one in physics and one in chemistry). And while it may pale in comparison to her many other accomplishments, today — on what would've been her 144th birthday — she also becomes a Google doodle honoree.

    You're probably aware by now that a Google doodle — a redesigned version of the Google home page logo — is the highest honor the search engine can bestow on a significant date. Some of the more elaborate ones we've seen in recent memory include a Freddie Mercury birthday video, an animated interpretation of John Lennon's "Imagine," and a playable/recordable Les Paul guitar.

    Next to those particular Google doodles, Curie's is plain — it is not interactive or animated — but it is somehow fitting for the scientist. A visit to the Google homepage reveals an illustration of Curie sitting at a workbench covered with various flasks. She appears to be in the middle of an experiment as the Google logo casts a shadow behind her.

    We're glad to see this simple yet poignant logo mark the addition of Curie to the short list of scientists who have been honored with Google doodles. She's in pretty good company with physiologist Albert Szent-Gyorgyi, geneticist Gregor Mendel, chemist Robert Bunsen, inventor Thomas Edison and several others.

    Related stories:

    Want more tech news, silly puns or amusing links? You'll get plenty of all three if you keep up with Rosa Golijan, the writer of this post, by following her on Twitter, subscribing to her Facebook posts, or circling her on Google+.

  • Genes tell a tale as big as Africa

    Courtesy of William Holland

    William Holland, a family researcher from Georgia, tours a village in the Oku region of Cameroon.

    Over the past year, William Holland's African-American family tale has grown in the telling, thanks to genetic testing and a whole lot of trans-Atlantic travel. The latest twist is a doozy: The Georgia resident has turned his research into a story that goes back to the seventh century.

    Holland says he has found links to ancestors who lived in the Cameroonian region of Oku, who were captured by neighboring tribes and taken as slaves in Virginia. His story illustrates how the descendants of slaves can go beyond a painful chapter of American history and find their place in the broader sweep of world history. But the outcome isn't as precise as a paternity test.

    "You have to put together the science and the history to make sense of it," he told me after his latest trips to West Africa. "To be honest, this is not an easy thing to do. You have to understand history, you have to understand migration patterns, you also have to understand culture. Most people would say, 'This is too much, because it's too complicated.' I would say this is a master's degree-level task."


    Real families, real feelings
    And it's not just an academic exercise. We're talking real families here. A year ago, Holland thought the genetic linkages showed a strong tie to royalty in a Cameroonian region known as Mankon. But after additional genetic tests and consultations with historians in Africa — including Samuel N. Wambeng, Nji Oumarou Nchare and Aboubakar Mgbekoum — he has focused on Oku instead. In fact, some of the people living around Mankon just might be the descendants of tribes that were involved in the slave trade.

    "In Mankon, there were people who were dealers in trading people," Holland said. "They didn't trade their own people, but they were trading people from outside their community. So now it makes sense that I was not directly related to the palace in Mankon. Did my people come from there? No. Did they pass through there? Yes."

    Even though the abduction from Africa happened in the 1770s, that part of the story has sparked bad feelings between Holland and some of the Cameroonians he came to know. "I didn't speak to them for a month," Holland told me. "It's still painful. ... Have you ever had a bad dream about being chained up in the bottom of a ship?"

    Solving family mysteries
    Unraveling history can leave scars, but it can also solve family mysteries. For example, the historians told Holland something that meshed with his memory of his sister's nickname. "Her name is Delores, but we always call her 'Nene,'" he said. "In Oku, 'Nene' basically means 'Mother.' That name was given to her by my father. These are very old names."

    The DNA tests that Holland has taken mark marked the beginning of Holland's story, not the end. Most recently, Holland took a Y-chromosome test from Ancestry.com that looked at 46 genetic markers, and then he plugged the results into a database on the Sorenson Molecular Genealogy Foundation website. In some cases, comparisons with African test subjects in the database produced 33 matches out of 36 common markers.

    "Normally they'll say, 'We're not related to someone,'" Holland observed. "Now the results show that, guess what, something must have occurred in those days for them to have nearly the same DNA as myself. Thirty-three out of 36 is pretty high."

    Holland followed up by contacting the likeliest candidates for his kin.

    "Genetics will only get you to the airport, but now where do you go?" he said. "You have to really find all the links. I'm lucky to have the information to find the links to the old names. With the names, people in Africa can say, 'This person was from this kingdom.' It's just like when people decide to go back to Scotland or Ireland, depending on whether your name begins with an 'M-A-C' or an 'M-C.'"

    I can relate to that: I took a Y-chromosome test a decade ago in hopes of tracing my genetic roots in Ireland. I still haven't found a match close enough to confirm family ties in the old country, but the historical record provides enough information to make for a good tale about my great-grandfather's escape from western County Clare in 1847, during the Great Famine.

    From Arabia to Virginia
    Here's Holland's story, based on his visits to Ghana and Cameroon as well as the genetic results and the reports from the historians:

    "We left Saudi Arabia around 622 when the time of Prophet Mohammed was implementing Islam.  A war ensued, and the Mboum people left and went to Egypt, then to the Sudan, then in the Tigray area of Ethiopia.  The city was in a town called Axum. Please note the Tigray province and the current tribal name of Tikar/Tikari.  From Ethiopia, the Mboum people went to the valley in Lake Chad in the north of Cameroon and arrived finally in 933 in the Adamawa region. The village that was set up in the Adamawa region was called Ngan-Ha, and Nya Sana was the first Fon [king]. The story told to me was that he (Nya Sana) was the youngest of the leaders that arrived from Ethiopia, but became the king because he retrieved the most powerful idol that fell from the sky.  There were a total of four leaders that came from Ethiopia, and all got their hands on one of the idols that fell from the sky.  These idols were in Mecca (Makah) in Arabia that flew from there and headed to Egypt then to the Sudan, Ethiopia and finally to Ngan-Ha.

    "Took Gokor ruled from 1186 to 1217, as he was a direct descendant from Nya Sana. Princess Wouten (Wou-Ten or Betaka) ruled around 1201-1246, during which she founded the Tinkala kingdom. So the tribal name change was from Mboum to Tinkala and finally to Tikari/Tikar. The Tikar kingdom was created around 1300.  The migration pattern was from Ngan-Ha to Tibati, Ina and finally Bankim or Kimi.  Kimi and Bankim are names that are used interchangeably when referring to this ancient area of various tribes in Cameroon. Around 1387, Fon Mbe left Bankim due to chieftancy disputes, and also he did not want to be killed while ruling. Nchare Yen supposedly had the right to become the next Fon, but was passed over by his half brother. Mbe, Ngonnso and Nchare Yen were siblings from the same mother and father. They left in fear, founding the kingdoms of Bankim, Foumban and Banso.  Ngonnso founded Banso, while Nchare Yen founded Foumban.  Nchare was the youngest of the siblings.

    "I believe my common ancestor [linked to the royalty] lived around 1550, during the time when Fon Ngang was on the throne.  He ruled from 1540 to 1588.  According to the SMGF DNA results, the time period for the common ancestor was about 440 years ago. Also, there is a possibility that it could have been in Foumban. The eighth Fon of Foumban founded Banka, and his name was Ngapna (1590-1629).  The familes that are in Banka and Bafang must have descended from the Prince of Ngapna. 

    "The Wambeng family of Oku descends from the third Fon, who was named Ney. Oku was founded around 1650, so the third Fon would be close to accurate for the 1770s time period. The people of Bali were hired by the coastal slavers, who gave them guns to capture individuals for the Virginia plantation owners. Bali is not too far away from Mankon.  I asked the elder about this whole scenario, and he told me the year adds up to when Ney was ruling.  Those who were captured, including my ancestor, were guards of the palace.

    "The Bali people came with guns and created quite a scene, resulting in the capture of my ancestor. They were taken to the coast, and the rest is history.  Meanwhile, in Foumban, the 11th Fon also lost children due to the fighting that was going on at the same time.  It's very possible that when all of them arrived in Bimbia, they knew they were the same people, but spoke different languages and could not communicate with each other.  I was told that the slavers arranged things intentionally so that you would be separated if you spoke the same language/dialect, to prevent insurrection on the ship. 
     
    "Because of Ngonnso, the kingdoms of Oku, Banso (Kumbo) and Mbiame are related, and also Kom would have to be included.  There is a good relationship between all of them today, and who knows? Maybe a big party would happen if we all go back to meet the family in Oku."

    So now what? Holland is still working on the later chapters of his family's story — the part that includes his slave ancestors in Virginia, including one ancestor who was taken into the Confederate Army for a time. But the chapters that excite Holland the most are the ones that go way back into the past.

    "I guess I'll always have a curious gene in there, a gene that makes me want to find out," he told me. "Will I stop after this? Hopefully there's be a different thing to work on. I'd like to go to the east — to Egypt, and Ethiopia."

    Earlier chapters in the African-American saga:


    Connect with the Cosmic Log community by "liking" the log's Facebook page or following @b0yle on Twitter. You can also add me to your Google+ circle, and check out "The Case for Pluto," my book about the controversial dwarf planet and the search for new worlds.

  • Rover spots the 'new thing' on Mars

    NASA / JPL / Stuart Atkinson

    A close-up from NASA's Opportunity rover shows the line of light-colored rocks known as "Homestake" or "The Vein." Components of Opportunity's robotic arm are visible in the left foreground.

    NASA's Opportunity rover has come across a light-colored line of rocks that could serve as solid evidence for Mars' watery past — and help set the stage for the next Mars mission, due for launch this month.

    The formation, nicknamed "Homestake" or "The Vein," showed up in pictures that the rover sent back from the rim of Endeavour Crater early this week. It looks like a few paving bricks, sticking edge up from the surrounding soil. Not all that impressive, but it caught the attention of the rover science team as well as the amateur observers who are following Oppy's every move.


    NASA / JPL-Caltech / Stuart Atkinson

    This stereo view from NASA's Opportunity rover shows the view looking out past Cape York to Endeavour Crater. Use red-blue glasses to see the 3-D effect. Click on the image for a larger view.

    Cornell astronomer Steve Squyres, the principal investigator for the Opportunity and Spirit rover missions, told the Planetary Society's A.J.S. Rayl that he and his colleagues have been keeping an eye on similar light-colored veins of rock for months during Opportunity's dash to the crater rim. Squyres said tracing the veins to find Homestake was a "real triumph of geology."

    "These are different from anything we've ever seen with either rover, a completely new thing on Mars, never seen anywhere," Squyres said. "And we're pretty charged up about it."

    Stuart Atkinson, a British educator, author and amateur astronomer who has been working up wonderful imagery from the rover missions for years, produced more than a dozen pictures over the past few days documenting Opportunity's surroundings, and particularly what's happening with Homestake. The rover has already been taking a close look at the formation with its microscopic imager.

    NASA / JPL-Caltech / Stuart Atkinson

    Opportunity's microscopic imager looks at the Homestake rock formation and its surroundings in detail.

    So what is it? Squyres isn't willing to "hazard a guess" yet, but the speculation is that the rock could point the way to minerals that are linked to Mars' wetter, warmer past. Five years ago, the now-defunct Spirit rover churned up light-colored, silica-rich dirt that had to have been formed in the presence of water.

    The Opportunity team has also been looking for phyllosilicates, clay minerals that have already been detected through orbital observations. Such minerals are an important clue to Mars' geological history, since they form in water that's not as acidic as the water that gave rise to Spirit's silica. A less acidic environment would be more hospitable to life.

    It may be too early to say what Homestake is, but based on the buzz, it's likely to be something interesting.

    More buzz will be stirred up in the weeks to come over the Curiosity rover's upcoming $2.5 billion mission to Mars. The car-sized rover, also known as the Mars Science Laboratory, is due to be launched on Nov. 25 with Mars' Gale Crater as its objective.

    Gale Crater should be a candy store for geologists, because it boasts a 3-mile-high (5-kilometer-high) mound of phyllosilicates and sulfates. The composition of the soil at different elevations could help scientists document a billion years of geological and climate history. It could even point to particular eras when Mars was actually habitable by life as we know it. And if those conditions still exist underground ... well, that would be a vein of pure gold for astrobiologists.

    By the time Curiosity touches down on the Martian surface next summer, Squyres and his colleagues may well have unraveled Homestake's secrets, and the lessons learned from one rover mission will carry over to the next. Stay tuned...


    Tip o' the Log to Discovery News' Jason Major. Special thanks to Stuart Atkinson for sharing his processed images of Opportunity's views.

    Connect with the Cosmic Log community by "liking" the log's Facebook page or following @b0yle on Twitter. You can also add me to your Google+ circle, and check out "The Case for Pluto," my book about the controversial dwarf planet and the search for new worlds.

  • How driving can light up cities

    New Energy Technologies

    Cars can help generate electricity to light up city streets by rolling over these rumble strip-like speed bumps as the come to a stop. The technology was recently demonstrated in Roanoke, Va.

    The roads of the future may be lined with speed bumps if a Maryland company succeeds in wide-scale deployment of a technology that harvests kinetic energy from cars and trucks and converts it to electricity.

    The technology essentially helps slow vehicles down as they roll over rumble strip-like treadles that capture energy that is otherwise lost as heat when drivers step on the brakes. 


    This harvested energy is used to generate electricity that can power streetlights, nearby buildings and keep emergency communications equipment charged up, for example.

     

    The MotionPower strip is being developed by Maryland-based New Energy Technologies. They recently demonstrated it at an event center in Roanoke, Virginia, where stopping cars lit up a series of lights.

    A total of 580 cars drove over the strip in a 6-hour period, generating enough electricity to power an average U.S. home for a day, according to the company.

    The concept of harvesting energy from people as they move around is nothing new. We've seen an energy harvesting backpack, pair of shoes, and a knee brace, for example, as well as pavers that light up when people step on them a la the late Michael Jackson in his "Billie Jean" video.

    New Energy Technologies envisions their system as a way to generate clean and green energy for cities and, at the same time, help them shave costs off their electricity bills.

    Assuming the technology works as advertised, there's the question of economics. How much does the system cost to install and maintain and what's the payback in terms of a city's savings on utility bills? A spokesman said hard numbers aren't yet available.

    More on energy harvesting technologies:


    John Roach is a contributing writer for msnbc.com. To learn more about him, check out his website. For more of our Future of Technology series, watch the featured video below.

     

     

    Disposable computers for hurling into infernos, underwater robots that team up for search and rescue, and other new tools are coming to the aid of emergency responders during calamities.

     

  • What's next for a make-believe Mars

    ESA

    Diego Urbina, one of the six volunteers who have been cooped up in a Moscow lab during a 520-day simulated mission to Mars, looks out from a hatch inside the Mars500 "spacecraft."

    The end of a 520-day simulated mission to Mars marks one more step in a succession of make-believe trips to Mars, leading up to the real thing. And who knows? You might even be able to get in on a "sim."

    Measured by length and expense, the Mars500 exercise is the most ambitious earthly simulation to date: In June of last year, the $15 million experiment put six male volunteers from Europe, Russia and China in a windowless mobile home that was set up inside Moscow's Institute for Biomedical Problems. Crew members "landed" at their destination in February, and walked out into a make-believe Mars roughly the size of an indoor tennis court.

    After a months-long simulation of the return trip, the crew is scheduled to "land" back on Earth on Friday and climb out of their isolation compartment. "The longest night in the world is about to finish," simulation crew member Diego Urbina wrote today in a Twitter update. You can watch the hatch opening via the European Space Agency's website at 6 a.m. ET (11:00 CET).


    Space.com

    'We come in peace'
    The whole idea of this simulation was to see what kinds of interpersonal problems might come up during a real 520-day mission to Mars, due to the confined space, delays in back-and-forth communication, once-a-week showers and the sense of separation from the home base. If the aim was to see whether a six-person team could survive the simulated trip without lashing out at each other, this team passed with flying colors. 

    "They have had their ups and downs, but these were to be expected," Patrik Sundblad, a life sciences specialist at the European Space Agency, said in an online recap of the mission. "In fact, we anticipated many more problems, but the crew has been doing surprisingly well. August was the mental low point: It was the most monotonous phase of the mission, their friends and family were on vacation and didn't send so many messages, and there was also little variation in food."

    The crew's spirits lifted with the approach of the end, and Urbina could indulge in a little space levity as the final hours ticked by. "'We come in peace' ... I always wanted to say that," he wrote.

    But this simulation left out some of the most important challenges that would face real Mars-bound astronauts: for example, the bone and muscle loss that comes along with spending months in zero gravity, and the risk posed by radiation exposure between here and the Red Planet. Some of those issues will be addressed in the simulated Mars missions to come.

    Simulations in space
    The biggest and most expensive "simulation" of a mission to Mars isn't a simulation at all: It's the multibillion-dollar operation known as the International Space Station. This month marks 11 years of continuous human presence aboard the station, and during all that time, much has been learned about coping with weightlessness. (One big problem that's come up is vision impairment. Possible coping mechanisms: artificial gravity and hibernation.)

    The next few years are expected to bring additional experiments aimed at testing the waters for Mars missions. NASA has been talking about setting up time delays in Earth-to-space communications, to reflect the minutes-long light-speed travel times between Mission Control and a spaceship heading for Mars. A 10-minute time delay is on the space station's tentative science agenda for next year. Several experts have suggested attaching prototype Mars modules to the station for future test runs.

    Russian space officials are thinking about conducting a Mars500-style experiment aboard the space station sometime after 2014, the Itar-Tass news agency reported today. "We are interested in staging such an experiment in actual conditions of zero gravity," Vitaly Davydov, deputy chief of Russia's Federal Space Agency, told Itar-Tass. "It is too early to say when such an experiment could be made."

    If the plan goes forward, at least two astronauts would spend at least 18 months in orbit. That timetable is much longer than the typical four- to five-month tour of duty — and would set a new record for time spent in space. The current endurance record is 437 days and 18 hours, set in 1995 by Soviet cosmonaut Valery Polyakov aboard the Mir space station. Polyakov was said to suffer some low moods during his record-setting stint in space, but there were no lasting physical impairments, and by all accounts he's still healthy at the age of 69.

    "I was able to stand up and walk on Earth after being in zero gravity," he told an interviewer at the New Mexico Museum of Space History in 2007, "so it should be easy to stand up and walk on Mars."

    Experiments on Earth and Mars
    More make-believe Mars missions will be getting under way here on the home planet. Next month, the nonprofit Mars Society will begin its 11th field season at the Mars Desert Research Station near Hanksville, Utah. Teams of volunteers cycle through tours of duty at a lonely-looking habitat in a Marslike desert environment. Part of the job is to go out in faux spacesuits and simulate surface exploration, but there are also experiments aimed at testing technologies and procedures that could come into play during a real Mars mission.

    The deadline has passed for this season's crew selection, but if you want to volunteer, there's always next year. If you're selected to participate, you'll have to pay a fee and cover some of your travel expenses. The project's organizers also say you'll definitely have a "leg up" in the selection process if you're working on a research project that could yield publishable results.

    During the summer, the Haughton-Mars Project provides a home away from home for researchers on Devon Island in the Canadian Arctic, one of the most Marslike places on Earth. Researchers from around the world have conducted Mars analog experiments at Haughton Crater for more than a decade.

    So what about the real Mars? NASA's timetable for human exploration calls for astronauts to visit the low-gravity moons of Mars in the mid-2030s, followed by forays to the planet's surface. There's lots to be done between now and then, not only to solve the challenges facing interplanetary space travelers, but also to do the robotic reconnaissance that's required in advance of human missions.

    Two robotic missions are set to blast off toward the Red Planet in the next month: Russia is due to launch its Phobos-Grunt probe from the Baikonur Cosmodrome in Kazakhstan on Nov. 8, with a landing on the Martian moon Phobos expected in 2013. NASA's Mars Curiosity rover arrived at its Florida launch pad today, in preparation for a Nov. 25 launch.

    And then what? Some observers worry that NASA's budget woes will put a huge crimp in planetary exploration, including future missions to Mars. Scientists would love to have samples of Martian soil returned to Earth for study, but the crystal ball seems to be providing less clarity as time goes on. Will we be stuck in simulation mode forever? Feel free to weigh in with your comments below.

    More about Mars:


    Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter or adding me to your Google+ circle. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for other worlds.

  • Manned electric 'multi-copter' takes flight

    A pilot in Germany completes the first manned flight of the E-volo multicopter which takes off and lands like a helicopter. Msnbc.com's Dara Brown reports.

    A group of German tinkerers have successfully completed what it claims is the world's first manned flight with an electric-powered "multi-copter" — a contraption that resembles a helicopter but with 16 rotors.

    The one-minute-and-30-second flight was proof of concept for the machine that could one day find use for tasks such as inspecting wind turbines and pipelines or taking aerial photographs — in addition to giving aviation geeks a good time.


    Though most similar to a helicopter, the team says the E-volo is superior due to the "simplicity of its engineered construction without complicated mechanics, and its redundant engines."

    Should something go wrong, it can land even if four of its 16 rotors fail, for example. And since there is no propeller above the pilot, a safety parachute could also be deployed.

    Sans pilot, the machine weighs 176 pounds (80 kilograms), light enough to be classified as an ultralight. 

    What makes it different from other helicopter-like flying machines with multiple rotors is the electric power source — lithium-ion batteries. In its current configuration, there's enough juice for 20 minutes of flight.

    We've recently seen other electric flying machines, such as the electric-powered plane that took flight this summer at EAA AirVenture show in Wisconsin. And students at the University of Maryland are working on a human-powered helicopter.

    Compared to flying a plane, the E-volo is simple to operate — it is controlled with a joystick — potentially opening up this aviation thrill to the masses.

    Future designs could include multi-seat machines that zip along quickly enough to replace the helicopters we see flying around today.

    More on flying contraptions:


    John Roach is a contributing writer for msnbc.com. To learn more about him, check out his website. For more of our Future of Technology series, watch the featured video below.

     

    Disposable computers for hurling into infernos, underwater robots that team up for search and rescue, and other new tools are coming to the aid of emergency responders during calamities.

     

  • Reality check for starships

    Les Bossinas / NASA

    An artist's conception shows a starship entering a wormhole to travel to a distant galaxy.

    Last month's "100-Year Starship" conference, backed by NASA and the Pentagon's Defense Advanced Research Projects Agency, threw a huge spotlight on the idea of sending spacecraft far beyond our solar system — but how realistic is that idea? Check out what one of the world's top experts on the subject has to say on "Virtually Speaking Science."

    Marc Millis, the researcher behind NASA's Breakthrough Propulsion Physics Project and the nonprofit Tau Zero Foundation, was my guest on tonight's show, which is available as a podcast via BlogTalkRadio and iTunes.


    Millis estimates that it'll take 200 years to get in position for the first missions to stars beyond our own, but he says there are lots of small steps we can take starting tomorrow to "chip away" at the challenge. Experiments with solar sails have already started, and Millis says the next step there is to figure out the business case for more ambitious light-powered trips.

    There are all sorts of potential breakthroughs to consider: Could the recent reports of faster-than-light neutrinos point to a way to break the speed limit set by special relativity? Could laser experiments let scientists warp the fabric of space-time on a small scale? "What creates the properties of an inertial frame, and how does that relate to space travel?" Millis asked.

    Is it worth spending money on precursor missions — for example, sending a "Super-Hubble" space telescope beyond the edge of our solar system to look outward, and inward? "What would it take to do that? How much would it cost?" Millis said.

    Here's an edited transcript of my pre-show Q&A with Millis:

    Cosmic Log: More people are aware that interstellar flight is on the agenda, in part because of the 100-Year Starship conference. So is anyone building a starship anytime soon? What's the next step?

    Millis: No one's building a starship anytime soon, although a lot of people would like to attempt that. The workshop had about 1,000 people there. It was open to the public, and I was glad to see some very intelligent questions from the public. It was an introductory look at not only the technology, but also some of the social issues, and how you would do financing.

    The next step by DARPA is that there's a competition out to award the remaining funds of about $500,000 [out of an original $1 million] as seed money to whoever can suggest the best organizational structure to carry forward with the 100-Year Starship image. That will be an organization that will work for at least a century to develop the technology and financing to ultimately enable starships.

    Q: Do you see Tau Zero as that organization?

    A: Tau Zero is making a proposal. To gauge our chances, I would have to know what all the other competitors are proposing, and that's hard to do.

    Q: Could it be that the social issues are actually more challenging than the technological issues?

    A: Theoretically, it would be possible to send a probe to the nearest neighboring star in less than a century, so you could actually get your data back. But the required expense is beyond what I think our society could commit to right now.

    Q: What's the ballpark figure for the cost?

    A: There isn't one, because it's so beyond what we can do.

    Based on the progression of society ... if we don't change anything that we're doing, it looks as if it might take another two centuries to have an interstellar probe that's fast enough to complete a mission within a human lifespan. Not that there's people on board, but that the people who launched the mission could get the data back before they retire. We have a long way to go.

    The important issue to figure out today is to make sure we have a sane comparison of the real challenges and the real state of the art, so we're proceeding wisely here. Then, from that, ask, "OK, if that's where we are, what can we start tomorrow to chip away at those issues?" We can't build the starship tomorrow, but we can identify the correct questions to ask, and begin seeking answers to those questions. When it looks more promising, and the advancements are there, fine.

    On the social issues ... when you think of leaving the planet, and representing Earth, that requires a high degree of political will and collaboration. I don't consider that impossible, and things are certainly looking up in terms of nations collaborating on major space topics. But I don't know how long it will take to really bring this collaboration to bear. Now this doesn't preclude any one sufficiently able and wealthy team from launching their own mission, on their own. Would that be ethical or not?

    Then, suppose we did identify a habitable planet. Is it really ours to consider colonizing?

    There are a lot of huge questions: What's the optimal population for an interstellar trip? What are the governance models? What's the meaning of life? When you start thinking about "world ships," where we're sending people instead of just robotic probes, that provides a venue that's far enough out that you can rationally discuss these questions. It's an interesting opportunity that we really haven't tapped into yet.

    Q: I guess one of those big questions would be, "Why travel to other star systems?" How would you answer that one?

    A: The ultimate, highest-priority benefit of star flight is the survival of the human species beyond the fate of our own solar system and our home planet. In the meantime, the progress we make to try to turn all this stuff into a reality will result in profound improvements in energy conversion, transportation, self-supporting life support — things that would be very useful for life on Earth. And then there's the social aspect. This effort can give us hope for a better future, expand our opportunities — and hopefully give people a frontier to conquer, rather than being left with no option other than to conquer each other.

    More about interstellar flight:

    Podcasts from 'Virtually Speaking Science':


    Last update: 10:30 p.m. ET Nov. 2.

    Many thanks to the Meta Institute for Computational Astrophysics for co-sponsoring tonight's Second Life talk at the Stella Nova auditorium.

    Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter or adding me to your Google+ circle. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for other worlds.

  • Will Japan build a backup Tokyo?

    Issei Kato / Reuters

    Onlookers get a panoramic view of the city of Tokyo from the first observatory deck during a media preview of the Tokyo Sky Tree tower this week. Some Japanese lawmakers have proposed constructing a "backup city" that could take on the capital's functions in the event of a catastrophe.

    It sounds like a story ripped from the parody-filled pages of The Onion, but some Japanese lawmakers really do want to build a "backup city" that would take over the functions of Tokyo, including tourism, in the event of a catastrophe.

    The idea was floated last month at a Tokyo luncheon, with a follow-up in The Telegraph last week. "The idea of being able to have a backup, a spare battery for the functions of the nation ... isn't this really a good idea?" Hajime Ishii, a parliamentarian representing the ruling Democratic Party of Japan, was quoted as saying.


    Support for creating an urban Plan B has grown in the wake of the earthquake and tsunami that devastated Japan in March and led to the Fukushima nuclear crisis. "Preparations are already under way at various levels to find ways of mitigating possible far-reaching consequences of a much-expected earthquake striking Tokyo," the Foreign Correspondents Club of Japan said.

    The lawmakers' plan calls for building an urban center known as IRTBBC (Integrated Resort, Tourism, Business and Backup City) or NEMIC (National Emergency Management International City) on the 1,236-acre site currently occupied by Osaka International Airport at Itami. Today, Itami is used only as a secondary hub for domestic flights, operating in the shadow of the newer Kansai airport.

    The new city would take on all the functions of the capital city in the event of an emergency. It would boast office complexes, resort facilities, parks and even casinos. The city's centerpiece would be a tower that would rank among the tallest in the world, coming in at just over 650 meters (2,133 feet). It'd be built to house 50,000 residents and accommodate a workday population of around 200,000 people from the Osaka region, The Telegraph reported.

    If the plan goes forward, it would rank among history's most ambitious backup plans. The backers haven't calculated the cost of building the city. For now, Ishii and his fellow lawmakers — including the Democratic Party's Banri Kaieda, Shizuka Kamei of the People's New Party and Ichiro Aisawa of the Liberal Democrats — are merely seeking 14 million yen ($180,000) for a feasibility study.

    So far, the reaction has been mixed: Osaka's governor, Toru Hashimoto, has been quoted as saying that his region is willing to accept the capital backup role, while Tokyo Governor Shintaro Ishihara has voiced opposition. And he may not be the only one: It just seems to me that most emergency-management officials, if not most politicians, would prefer to fortify what they have rather than building a whole new complex someplace else. Of course, I could be wrong about that.

    More about Japan's future:


    Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter or adding me to your Google+ circle. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for other worlds.

  • Ant frying tech could make solar cheap

    Chris Giebink, Penn State

    An LSC is illuminated by a laser beam (central spot) resulting in luminescence that is emitted from the edges and projected onto a white business card. The faintly visible concentric rings and different colors of light on the business card result from microcavity effects.

    Admit it. You fried an ant under a magnifying glass. It's OK. We did it too. Now scientists are reporting a breakthrough in a similar technology that could bring down the cost of solar power.

    About 50 percent of the cost of solar power is due to the materials and manufacturing of solar cells, essentially pieces of silicon that convert sunlight into electricity. By concentrating the sunlight, you can get the same amount of power with fewer cells.


    One way to do this is with a magnifying glass, like we do when we fry ants. But this is a bit tricky when we want to concentrate sunlight all day long because we have to make sure the glass is directly aligned with the sun. 

    "In order to do that, you have to track the sun … and that drives up the cost of your concentrating system," Chris Giebink, an assistant professor of electrical engineering at Pennsylvania State University, told me today.

    Luminescent solar concentrators
    The approach he and his colleagues are improving upon is a decades old technology called luminescent solar concentrators. These contraptions concentrate light by absorbing it with special dyes that re-emit about 75 percent of the light within the confines of a transparent slab of material.

    The trapping effect is similar to the way optical fibers use light to transmit data. "It is trapped so it is guided towards the edges and that's where you stick your solar cells," Giebink explained.

    The bigger you make the LSC, the more concentrated the light that's fed to the solar cells on the edges. In theory, these things can concentrate the light to the power of 100 suns — all without tracking the sun since they work at any angle and even concentrate diffuse light on cloudy days.

    "On paper, it sounds really good," Giebink said. "In practice, the reason you don't see these things is because they don't work very well."

    The biggest problem is that much of the sunlight that is absorbed by the dye and reemitted into the glass either bounces off the glass and gets reabsorbed by the dye and lost or reemitted in a direction where it is no longer trapped, which has about a 25 percent chance of occurring.

    "Since we are bouncing through this thing hundreds of times, that adds up to a big problem. It has prevented these things from getting anywhere close to their theoretical potential," Giebink said.

    Preventing re-absorption
    He and his colleagues have now found a way to prevent the light from being reabsorbed by the dye en route to the edge of the glass.

    To do this, they made an LSC with two very thin films stacked on a layer of glass. 

    The first film — about 100 nanometers thick — is a luminescent layer containing the dye that absorbs and reemits sunlight. This layer sits on top of a low refractive index layer, "which essentially means from the standpoint of light it looks a lot like air," Giebink explained.

    This combination creates what is called a microcavity. The researchers found if they changed the thickness of the luminescent layer, the microcavity would change in a way that prevents the light reemitted by the dye from being reabsorbed when it bounces off the bottom of the glass.

    "We've changed the thickness of one of the films such that light essentially can't fit in that thin film anymore and as a result it is reflected back with very high efficiency, close to 100 percent," Giebink said.

    Their experimental results suggest this approach allows them to get to about 25 suns for a window pane sized collector, which is 2.5 times greater than a conventional LCS.

    Going forward, the researchers need to optimize the design so that it is both cheap to manufacture and has the desired effect. After all, it won't bring down the cost of solar power if the concentrator cost as much as the solar cells it's meant to replace.

    "We've shown the general idea works, but how exactly to build one of these things is not entirely clear," Giebink said.

    Complementary approach
    The breakthough is compatible with another approach to this problem reported by researchers at the Massachusetts Institute of Technology in 2008 that focused on creating dyes that are less susceptible to reabsorbing the light they reemit.

    "We took any dye that you want and decreased the probability of re-absorption a lot just by how we structure the concentrator itself," Giebink explained. "We ought to be able to combine the two approaches. That's the direction we are going now."

    If it all works out, the researchers estimate it could reduce the cost of solar power systems by about a factor of two, he added, which could help make solar energy more price competitive with coal and oil, easing the transition away from fossil fuel energy.

    More on solar power technologies:


    The researchers, who included Giebink and Gary Widerrecht and Michael Wasielewski with Argonne-Northwestern Solar Energy Research Center and Northwestern University, published their findings in current issue of Nature Photonics.

    John Roach is a contributing writer for msnbc.com. To learn more about him, check out his website. For more of our Future of Technology series, watch the featured video below.

    Disposable computers for hurling into infernos, underwater robots that team up for search and rescue, and other new tools are coming to the aid of emergency responders during calamities.

  • Happy Palindrome Day! (Again!)

    Aziz Inan explains this year's palindrome dates.

    If you're mathematically minded enough, every day can be a special day — it's just that today's date, 11-02-2011, makes it more obvious for palindrome fans. Like Aziz Inan, for instance.

    Inan, an engineering professor at the University of Portland, has made a study of dates that run the same numbers forward and backward. Several studies, in fact. Such combinations are considered numerical palindromes, much like the alphabetical palindromes that delight puzzle fans. (One of the most famous examples is the Garden of Eden's first introduction: "Madam, I'm Adam.")


    This year has several date-based palindromes, depending on how you structure them: 1-10-2011, 1-11-11, 11-1-11 ... and if you go by the DD/MM/YYYY notation, Feb. 11 already marked 11-02-2011. Inan told the Los Angeles Times that today (or Feb. 11, if your calendar swings differently) is extra special because 11,022,011 equals another palindrome, 1001 X 11 X 1001.

    Aziz Inan / Univ. of Portland

    Aziz Inan, an engineering professor at the University of Portland, demonstrates the palindromosity of 11-02-2011 with a little help from a mirror image (and Cookie Monster).

    "This is so much fun," Inan told the Times. "Engineering can get pretty boring because you talk about equations, but when I say, 'Do you know today is a special date?' it gets a lot of attention. It helps me change the subject for a few minutes and bring the students back from their dream or their hibernating."

    Next year's Palindrome Days are Feb. 10 (2-10-2012), Feb. 21 (21-02-2012 in day/month/year) and Oct. 2 (2-10-2012 in day/month/year). Then there's 02-02-2020 — which is particularly notable not only because it's the next eight-digit palindrome date but also because it works whether you go with MM/DD/YYYY notation or DD/MM/YYYY.

    But you don't have to wait all that long for the mother of all monodigital dates, which comes next week on Veterans Day. What will you be doing at 11:11 on 11-11-11? Going to the movies?

    Correction for 3:35 p.m. ET: I originally wrote that Aziz's last name was "Anin," but the University of Portland pointed out that it's actually "Inan." Which is disappointing, because I was hoping he'd be the perfect palindromic match for Nina Ziza. The good news is that there's a Nani Ziza out there as well. I've also fixed another glitch: I originally referred to 11-02-2010 as Feb. 2 in day/month/year notation instead of the proper Feb. 11. Sorry about both those errors.

    More calendrical fun:


    Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter or adding me to your Google+ circle. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for other worlds.

  • How strange can space-time get?

    WGBH

    Our own planet twists the fabric of space-time, as shown in this animation from "The Fabric of the Cosmos."

    Theoretical physicist Brian Greene admits that the world he describes in his new public-TV documentary series, "The Fabric of the Cosmos," is nothing like everyday experience. He's not even sure some of the things he describes are for real. For example, how can we possibly know other universes exist? Believe it or not, there are ways to find out.

    The four-part "Nova" series makes its debut on PBS stations on Wednesday night with an episode that delves into the mysteriously substantial properties of empty space. "As it turns out, empty space is not nothing," the Columbia University professor says at the start of the show. "It's something. ... So real, that empty space itself helps shape everything in the world around us, and forms the very fabric of the cosmos."

    That episode is already available for watching over iPhones, iPads and iPod Touch devices, as well as through Amazon Prime instant video. And if you miss seeing it on TV on Wednesday, you'll be able to catch up with it later online. Over succeeding weeks, Greene addresses not only space, but also the nature of time, the weird world of quantum mechanics and the possibility that our universe is just one bubble in the cosmic ocean (or raisin-bread loaf, or cheese wedge) of the multiverse.


    Most of the substance in "The Fabric of the Cosmos" comes from Greene's book of the same name — but the part about the multiverse is more speculative, and is derived from Greene's follow-up book titled "The Hidden Reality." So of course that's where I had to start when I had a chat with Greene this week. Here's an edited transcript of the Q&A:

    Cosmic Log: You must get this question all the time: What sort of proof do you have that any of this stuff is true?

    Brian Greene: Well, the first three episodes — focusing on space, time and quantum mechanics — are much more closely tied to observations and experiments that have already been done. Much of what we describe in those programs is firmly rooted in science that is now largely accepted, even though it's weird. The fourth program is different in that regard, because as the last program in the series, it is looking beyond what we currently know, and surveying the landscape of possibilities that may in the future become accepted science. But not yet.

    That's the multiverse. The multiverse is hard to test because we have access to this universe, and the theory proposes that there are other universes. We can't directly see them. We can't visit them. So how would you ever prove that idea?

    In the program, we tackle that issue head-on. We describe how the multiverse naturally emerged from investigations that were rooted in observations and experiments: things to do with questions of the origin of the universe, the cosmic microwave background radiation, issues surrounding the puzzles of the big bang that can only be resolved through an inflationary view of the universe — which then yields the multiverse. But it won't be a satisfying explanation until we have some kind of direct confirmation.

    To my mind, there's really one main way that could happen in the near future: In this proposal, different universes are like different expanding bubbles in some larger cosmic environment, like bubbles in a bubble bath. And when bubbles in a bubble bath expand, they can run into each other. Similarly, expanding universes can collide. The math indicates that if and when they do, the collision can send ripple-like disturbances through the microwave background radiation — the heat signature left over from the big bang. Those temperature differences of that particular sort are something that people are looking for. Some even claim they've seen the first tentative signals of the pattern. I'm highly skeptical about that, as everybody should be. But this could be a way to subject an idea that seems so foreign to an observational test.

    Q: There's also been some talk about possible observations at the Large Hadron Collider that might suggest energy was "leaking" into other dimensions.

    A: Yes, the notion that there are extra dimensions provides another way in which you could have other universes. Our universe might be one piece of bread in a big cosmic loaf, where the other "slices" are displaced from ours in a new direction, and are actually other universes. One way to check that idea would be to have a very energetic collision of particles in our universe, on our slice of space. The math shows it's possible for energy from those collisions to be ejected off our slice and migrate into the wider cosmos. We would notice that here by seeing that energy was not conserved. The energy after the collision would be a little less than it was before, because some of the energy would have crossed beyond our universe.

    The point is that there are strange ideas about the universe that can nevertheless yield evidence, if we know where to look.

    WGBH

    In "The Fabric of the Cosmos," physicist Brian Greene graphically shows how the "Mona Lisa" ... and even Brian Greene ... could exist in more than one universe.

    Q: One of the points of the series is that there's a deeper level to reality that what we see in everyday life, suggested by mathematics and physics. You use all sorts of animations and graphics to convey a sense of the underlying fabric of the cosmos. Do you have some favorite tricks that you've used in the TV series?

    A: When you're dealing with subjects that are abstract ... these are mind-bending ideas, but what do you point the camera at? That's a funny thing, because everything we do takes place within space, within time. The concepts of space and time are so profoundly interwoven with reality as we know it, and yet science has revealed that there are features of space and time that run completely counter to our intuition — if you examine them on non-human scales, that is, scales that are very tiny, or very big, or when you're moving very fast, or if you're near a very strong, massive gravitational object.

    Since we can't actually go to those exotic realms, we use animation to show what it would be like if you could shrink down to a billionth of a billionth of a meter ... or what it'd be like if you could travel at just a tiny fraction less than the speed of light ... or what it would be like to hover near the edge of a black hole and then come back to Earth. And we use animation to show the largest bird's-eye view of the cosmos if some of these multiverse ideas are correct. That really gives you a visceral understanding of the concepts.

    Q: In fact Einstein used these types of thought experiments as well when he worked on his theories of relativity. He imagined what it would be like to ride a light wave, or to be falling through space in an elevator...

    A: If only Einstein had the tools of animation, who knows how far he would have gone!

    But there's a serious point here: When I do my own work, I'm constantly trying to build a mental image of what's going on. I'm never comfortable if my understanding is just completely in the equations. I feel like I have a storehouse of imagery built up just from the scientific research itself, which then leads to a form that will work in a book or on TV, which requires dressing it up in various ways. The whole idea of trying to visualize abstract equations is something that many of us do as part of our second nature, as researchers.

    Q: Are there any favorite visualizations you keep coming back to?

    A: Well, sure. A lot of my work has to do with extra dimensions of space. And I readily admit that I cannot picture anything more than three dimensions. So in my own work, I'm constantly doing what we do in the television program, which is to use lower dimensions as analogies — two-dimensional analogies that you can draw and manipulate. You use those as a guide to what's happening in higher-dimensional settings, where the equations of string theory reside.

    You have to be careful. Sometimes a lower-dimensional analogy can be misleading. But you begin to build up the art of knowing what aspects of those visualizations you can trust when you're taking the leap to higher dimensions, and which aspects make you say, "No, no, no, that won't give me insight into my real interest."

    Q: What do you hope viewers will take away from the show?

    A: The main goal is for people to leave the program with a more complete sense that when it comes to the universe, what you see is not what you get. There are layers upon layers of reality that we are unaware of in everyday life. Intuition is built up from experience, and our experiences since we appeared on the planet has been largely dictated by what is beneficial for our survival. Understanding the quantum world, and understanding the possibility of other universes, and understanding the deep nature of time don't help you get the next meal. So there hasn't been any real evolutionary pressure for us to gain intuition about those things. But when we have the luxury of thinking about them mathematically, we learn that there's much more to the universe than meets the eye.

    It's absolutely thrilling to learn that time for me is not the same as time for you; that out there in space, time is elapsing at a different rate near the edge of a black hole; that in the depths of space, there is unavoidable, ferocious quantum activity; that the world is governed by probabilities, not certainty; and then there's entanglement, the idea that what you do over here can have a direct effect on something over there. Wow!

    What is space? "The Fabric of the Cosmos" explains that empty space is not really empty.


    Wow indeed. The TV show is just the tip of the iceberg: The "Fabric of the Cosmos" website offers tons of videos, interactives, intereviews and links to online resources. More than a dozen "Cosmic Cafes" have been organized nationwide to talk about space, time and the multiverse. And the World Science Festival has organized a screening of the first episode at Columbia University at 9 p.m. ET Wednesday, to be followed by a forum featuring Greene, theoretical physicist Leonard Susskind and Nobel laureate Saul Perlmutter.

    Even though the in-person event sold out almost immediately, you can still tune in to live streaming video and join the discussion via Facebook or Twitter. I have an alternate suggestion: Watch the episode in advance, or save it for later, and tune in to "Virtually Speaking Science" at 9 p.m. ET Wednesday for my chat with interstellar-travel expert Marc Millis. Then, at 10 p.m. ET, switch on over to the World Science Festival's forum.

    More cosmic contemplations from Brian Greene:


    Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter or adding me to your Google+ circle. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for other worlds. 

  • City lights could point to E.T.

    David A. Aguilar / CfA

    If an alien civilization builds brightly lit cities like those shown in this artist's conception, future generations of telescopes might allow us to detect them.

    Astronomers suggest that artificial illumination creates a signature that could point to the existence of civilizations on other worlds — and they say we should get started on a survey of the edges of our own solar system, just in case.

    The suggestion comes from Harvard's Abraham Loeb and Princeton's Edwin Turner, in a research paper submitted to the journal Astrobiology. A version of the paper appears on the arXiv.org preprint server and sparked a write-up today on Technology Review's Physics arXiv Blog.

    Loeb, who chairs Harvard's astronomy department and is affiliated with the Harvard-Smithsonian Center for Astrophysics, acknowledged that detecting aliens by looking for the glow of their cities would be a long shot. But he pointed out that the cost of the exercise would be low.


    "We say that we can piggyback on existing surveys that people are doing anyway. There's no need to use extra resources. ... My philosophy is simple: If we can do it, why not do it and check? Why put blinders on ourselves?" Loeb told me today.

    Here's how the idea could work: An object's brightness varies with distance, but the relationship between those two factors will depend on whether the brightness is due to reflected sunlight or due to illumination from the object itself. For a self-illuminated object, the brightness varies by a factor of 1 over the distance squared, but "if you have an object that reflects light from another source ... the flux dies out like 1 over the distance to the fourth power," Loeb said.

    Monitoring the changes in the brightness of an object on the edge of our solar system, in a broad disk of icy material known as the Kuiper Belt, could provide a "very simple test" to determine whether extraterrestrials have turned on the lights, Loeb said.

    "We conclude that existing telescopes and surveys could detect the artificial light from a reasonably brightly illuminated region, roughly the size of a terrestrial city," on a Kuiper Belt object, Loeb and Turner write.

    NASA

    The lights of Cairo, Alexandria and the Nile shine through the night on Oct. 28, 2010, as seen from the International Space Station. Astronomers say such illumination could serve as a tip-off in the search for civilizations on other worlds.

    How likely is it that E.T. would be found on the edges of our own solar system? Not that likely, but Loeb and Turner speculate that it could happen. "Artificially lit KBOs [Kuiper Belt objects] might have originated from civilizations near other stars," they write. "In particular, some small bodies may have traveled to the Kuiper Belt through interstellar space after being ejected dynamically from other planetary systems."

    In addition to the E.T. search, Loeb said the Kuiper Belt survey would also be useful for studying how Kuiper Belt objects reflect light at different points in their orbits. "Even if the answer is, 'No, there is nothing peculiar,' we can still learn something from doing that," he told me. "And if there's something out there worth finding, that could change our perception of our place in the universe."

    The technique could conceivably be extended to other stars once next-generation telescopes such as the James Webb Space Telescope and the Giant Magellan Telescope come online, over the next decade or so. There's been a lot of debate over whether the traditional search for radio signals from alien civilizations might be fruitless if E.T. moved beyond analog radio transmissions — and the search for artificial illumination could be worth checking out as a new frontier.

    Someone could even try looking for the spectral signature of artificial light. (Do aliens use incandescent bulbs, compact fluorescent or LEDs?) But that particular kind of search would not be easy.

    "For this signature to be detectable, the night side needs to have an artificial brightness comparable to the natural illumination of the day side," Loeb and Turner write. And when you consider that Earth's day side is about 600,000 times brighter than the night side, that means E.T. would have to cope with one heck of an electric bill.

    What do you think about the search for E.T.'s city lights? Feel free to add your comment below.

    More about the search for extraterrestrial intelligence:


    Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter or adding me to your Google+ circle. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for other worlds. 

  • Printable sensors detect bombs

    Georgia Tech / Gary Meek

    Krishna Naishadham, left, and Xiaojuan (Judy) Song display two types of wireless ammonia-sensing prototype devices.

    If there's a suspicious package on the doorstep and you want to know if it’s a bomb, you may soon be able to print out a sensor that can do just that.

    The ability to make bomb-detecting sensors with inkjet printer technology could also benefit soldiers on the lookout for roadside bombs and aid agencies working in war-torn countries.


    The technology to do this is under development at the Georgia Institute of Technology, where researchers have created a sensor that communicates its findings wirelessly.

    The manufacturing process requires an inkjet printer that has a "much finer resolution than the standard household printer and it uses special inks," Krishna Naishadham, a research engineer who is leading the project, told me Tuesday.

    The ink for the sensor circuitry is a commercially available emulsion of silver nanoparticles, and the ink for the sensing element consists of bundled carbon nanotubes that have been mixed in a solution of water.

    The team uses a process called sonification which helps this ink achieve an optimal viscosity and homogeneity, allowing it to be easily deposited on a piece of photographic paper.

    The nanotubes — each about one billionth of a meter in diameter, or 1/50,000th the width of a human hair — are coated with a conductive polymer that attracts ammonia, a key ingredient found in many explosives.

    The sensor has been designed to detect trace amounts of ammonia — as low as five parts per million, but since ammonia is also found in non-explosive devices such as fertilizer and urine, more work is needed before the technology is ready for commercialization.

    "In order to develop this fully into an explosive sensor, we need to improve the sensitivity, we need to filter out other materials that might interfere with what we are trying detect — detecting ammonium by itself is not sufficient," Naishadham said.

    More research is also needed to seamlessly integrate a power supply for the sensors. Potential technologies include thin-film batteries, solar cells and energy-harvesting techniques.

    But with two years of research and another year to commercialize, Naishadham said these sensors could be available for as little as tens of dollars each for use in industrial settings, and perhaps a few hundred dollars when tuned up for military applications.

    [Via: Gizmag and Georgia Tech]

    More on bomb-detection technology:


    A presentation on this sensing technology was given this July at the IEEE Antennas and Propagation Symposium in Spokane, Wash., by Hoseon Lee, a Ph.D. student at Georgia Tech.

    John Roach is a contributing writer for msnbc.com. To learn more about him, check out his website. For more of our Future of Technology series, watch the featured video below.

    Disposable computers for hurling into infernos, underwater robots that team up for search and rescue, and other new tools are coming to the aid of emergency responders during calamities.

  • Gecko-inspired robot climbs walls

    Researchers have developed a tank-like robot that has the ability to scale smooth walls, opening up a series of applications ranging from inspecting pipes, buildings, aircraft and nuclear power plants to deployment in search and rescue operations.

    Researchers have built a tank-like robot that can climb smooth walls with the ease of a gecko scurrying about in the middle of the night. In fact, the robot was inspired by a scientific explanation for what makes gecko feet so sticky.

    The robot could find use in applications ranging from inspections of pipes, buildings, and nuclear power plants to search and rescue missions.


    Its tank-like feet are inspired from the millions of tiny, hair-like toe pads on gecko feet that allow the lizards to scurry up trees, walls, and across ceilings without falling down. 

    Previous research explained that tiny toe pads accomplish this thanks to what are known as van der Waals forces, very weak attractive forces between molecules.

    The robot team, led by Jeff Krahn at Simon Fraser University in Burnaby, Canada, recreated these dry but sticky toe pads in the lab using the material polydimethysiloxane (PDMS). The end of each hair-like pad contains a mushroom cap shape that is 17 micrometers wide and 10 micrometers high.

    "While van der Waals forces are considered to be relatively weak, the thin, flexible overhang provided by the mushroom cap ensures that the area of contact between the robot and the surface is maximized," Krahn explained in a news release

    By using the gecko-like pads on the robot, the researchers are able to climb even smooth surfaces such as glass or plastic, materials that are a consistent challenge for robots that use magnets, suction cups, spines and claws to climb.

    The tank-like robot weighs in at 240 grams and can transfer from a flat surface to a wall over inside and outside corners. It has a top speed of 3.4 centimeters per second.

    The robot goes by the name Timeless Belt Climbing Platform (TBCP-II). It is outfitted with sensors that allow it to detect its surroundings and alter its course to navigate obstacles, though Krahn and his team are still improving the control strategy to make it fully autonomous.

    To see the robot climb the wall, be sure to check out the video at the top of this post. Krahn and colleagues describe the robot today in the journal Smart Materials and Structures.

    More on geckoes and robots:


    John Roach is a contributing writer for msnbc.com. To learn more about him, check out his website. For more of our Future of Technology series, watch the featured video below.

     

    Disposable computers for hurling into infernos, underwater robots that team up for search and rescue, and other new tools are coming to the aid of emergency responders during calamities.

     

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