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Quantum fluctuations in science, space and society, from quarks to Hubble and Mars. Served up by Alan Boyle, NBC News Digital science editor. E-mail Alan, or connect via Facebook, Twitter or Google+.

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  • 13
    Dec
    2011
    3:19pm, EST

    Camera captures light particles moving through space

    M. Scott Brauer

    Media Lab postdoc Andreas Velten, left, and Associate Professor Ramesh Raskar with the experimental setup they used to produce slow-motion video of light scattering through a plastic bottle.

    By John Roach, Contributing Writer, NBC News

    A new imaging system that captures visual data at a rate of one-trillion-frames per second is fast enough to create virtual super-slow-motion videos of light particles traveling and scattering through space.

    For reference, light particles — photons — travel about a million times faster than a speeding bullet.


    While that's fast, researchers at MIT's Media Lab have developed a system for capturing data on the movement of photons through space and time and then stitching that data together in a computer to create virtual slow-motion videos.

     

    An imaging solution allows researchers to visualize the propagation of light at an effective rate of one trillion frames per second.

    Watch on YouTube

    In the video above, for example, a burst of laser light is seen traveling through a soda bottle and bouncing off the cap. Other videos show a ripple of laser light move across a table, over and into a tomato, and up a wall.

    "What you see in the videos is an average of many pulses," Andreas Velten, a researcher in MIT's Media Lab who is leading the effort, explained to me Tuesday. "If we capture one pulse, we don't get enough information. First of all because it is too faint and second because we only see one line at a time." 

    The technique to create the videos relies on what's called a streak camera. The aperture — opening — of this camera is a narrow slit that provides a reasonable field of view in the horizontal direction, but very limited view in the vertical — essentially a line, or row of pixels. 

    "It can only see one line, but it gives you a very high frame rate — a trillion-frames-per second," Velten said. This allows the researchers to make a movie of one scan line. Several pulses of light are used to compose each scan line movie to improve image quality, he noted.

    Then, a system of mirrors in front of the camera changes the field of view slightly so that a movie of the next line can be made. The process continues for each line of a scene, such as a pulse of light moving through a bottle. Then, the computer uses all this information to create the virtual slow-motion movies.

    "So what you are seeing is actually an average of many pulses, but because our camera and laser are synchronized very well, all the pulses look exactly the same," Velten said. "That's basically the trick."

    According to the researchers, it takes only a nanosecond — a billionth of a second — for light to scatter through a bottle, but it takes nearly an hour to collect enough data to stitch together a video.

    While watching photons move through soda bottles and across tables is visually cool and educational, the technology could be used to study the properties of materials, as well in scientific and medical imaging, even "ultrasound with light," the researchers suggest.

    For more on this technology, check out the video below featuring Velten and his adviser, Ramesh Raskar. 

    MIT Media Lab researchers have created a new imaging system that can acquire visual data at a rate of one trillion frames per second. That's fast enough to produce a slow-motion video of light traveling through objects.

    Watch on YouTube

    More on high-tech camera technology:

    • New camera always takes perfectly focused photos
    • Foam ball snaps panoramic images in the air
    • Smart fiber can act as a camera
    • Insects, animals captured with high-speed photography

    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.

    Where nations used to compete to get into space, now the competition focuses on private businesses, pouring hundreds of millions of dollars into next-generation spaceships. Msnbc.com science editor Alan Boyle reports from inside the rocket factories on the future of spaceflight.

     

    18 comments

    Nice coke commercial.

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  • 6
    Dec
    2011
    2:29pm, EST

    Computer mimics human ability to match images

    Thibault Camus / AP

    In this file photo, tourists pose in front of the Eiffel Tower in Paris. A computer can match up photos and paintings based on the uniqueness of features such as the Eiffel Tower.

    By John Roach, Contributing Writer, NBC News

    Every year, thousands of tourists stand in front of Paris' Eiffel Tower to have their picture taken, painted, or sketched. Though every image is different, each contains the sky piercing tower. Now, a computer can match up all those images based on that one identifying feature.

    This could be useful, for example, to someone who is wondering how the Eiffel Tower and its surroundings have changed since their grandparents had their picture painted in front of it on their honeymoon. In this case, the computer could find a match to the painting by searching online for a modern match.

    The technique differs from photo-matching methods that focus on similarities in shapes, colors, or composition, which work well when searching for exact or very close matches but fail when applied across domains, such as a picture taken in different seasons or a painting and a picture.


    "The language of a painting is different than the language of a photograph," Alexei Efros, an associate professor of computer science and robotics at Carnegie Mellon University in Pittsburgh, Penn., said in a news release. "Most computers latch onto the language, not what's being said."

    In the video below that explains how this all works, for example, a standard computer algorithm tasked to find images similar to a painting of a temple returns images of clouds and the ground that most closely match the image, not the temple that's of most interest to humans.

    The goal of this work is to find visually similar images even if they appear quite different at the raw pixel level. This task is particularly important for matching images across visual domains, such as photos taken over different seasons or lighting conditions, paintings, hand-drawn sketches,

    Watch on YouTube

    Efros and his colleagues programmed a computer to find the unique element that sets an image apart from others in a sample and then uses that uniqueness to match it with similar images. 

    The uniqueness is computed based on a dataset of randomly selected images. So, to use the Eiffel Tower example, the person standing in front of the tower is likely similar to other people in other photos and thus given little weight, but the tower itself is unlike anything else in the other photos.

    Efros said the approach is the "best approximation" yet achieved to how humans compare images.

    The technique can be used for automated image searches, for example, or combined with a GPS-tagged photo collection to determine where a particular painting of a landmark such as the Eiffel Tower was painted.

    In the following video, the team shows off how the program can also be used to assemble what they call a "visual memex" — a dataset that explores the visual similarities and contexts of a set of photos. It shows a graph of 200 images of Medici Fountain, another Paris landmark, from various distances. 

    This video demonstrates Visual-Memex graph traversal. Graph is built using our similarity metric.

    Watch on YouTube

    More on photo matching technology:

    • Police use facial recognition technology to match rioters
    • How to turn off Facebook's creepy face recognition
    • Google image search can't tell Obama from Bush
    • U.S. spies seek geotagging software

    Efros and colleagues will present their findings Dec. 14 at SIGGRAPH Asia, a computer graphics and interactive techniques conference in Hong Kong.

    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.

    Kids' play has moved to tablets and PCs. In this new age, toy makers and researchers alike are sorting out the benefits — and detriments — of playful educational interaction in virtual space.

     

    5 comments

    A human child can draw a crude picture of a pig out of magic marker. Any other human child (who knows what a pig is) can recognize it. A computer can't look at that crude drawing, compare it to a database of actual photographs of animals, and determine it is a pig. It might try to match the colors f …

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  • 28
    Nov
    2011
    1:37pm, EST

    Navy's twin stealth drone takes flight

    Northrop Grumman Corp.

    The availability of two X-47B unmanned aircraft enables the UCAS-D program to conduct a faster and more productive flight test program.

    By John Roach, Contributing Writer, NBC News

    Two is better than one, especially when it comes to flight testing a stealth drone designed to take off and land from moving aircraft carriers at sea. The U.S. Navy announced today it has reached that milestone in its X-47B program.

    The second tail-less unmanned aircraft — named Air Vehicle 2 — took to the skies from Edwards Air Force Base in California on Nov. 22 and flew a few racetrack patterns over Rogers Dry Lake at an altitude of 5,000 feet, said Northup Grumman, who is building the plane, in a news release.


    The first flight of the original X-47B took place in February. That aircraft successfully retracted its landing gear and flew in cruise configuration in September, allowing photographers to snap images that make the plane look like a UFO from a 1950s cartoon.

    Having a second plane will allow for the collection of more performance data and keep the program on development schedule, the aerospace company said. 

    Northrop Grumman Corp.

    The second X-47B demonstrator aircraft for the Navy's UCAS-D program completed its first flight on Nov. 22 at Edwards Air Force Base, Calif.

    The computer-controlled unmanned aircraft takes off and flies a pre-programmed mission and then returns to base in response to mouse clicks from a mission operator. The operator monitors the flight, but doesn't actively control it remotely, as for other drones.

    One of the twin aircraft will transition to the Naval Air Station Patuxent River, Md., by the end of 2011, to begin testing of precision carrier approaches, arresting landings and "roll-out" catapult landings, according to the release. 

    The tests will also include testing of recently installed guidance, navigation and control software that will enable the aircraft to land on a moving carrier deck, considered among the harshest aviation environments.

    The second craft will remain in California to continue envelop expansion flights, which are used to demonstrate the aircraft performance under a range of range, speed, and fuel-load conditions. 

    The first carrier launches are planned for 2013 and autonomous refueling demonstrations are slated for 2014. 

    More on Navy technology:

    • UFO-like drone hits cruise mode
    • New, stealthy Navy drone makes its maiden flight
    • Navy gets fix for speed need
    • Navy sees spying, not flying, future with drones

     


    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.

     

    Kids' play has moved to tablets and PCs. In this new age, toy makers and researchers alike are sorting out the benefits — and detriments — of playful educational interaction in virtual space.

     

    6 comments

    How does this thing get any yaw stabilization without a vertical stabilizer anyway?

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  • 4
    Aug
    2011
    2:09pm, EDT

    Spies seek geotagging software

    Getty Images / Getty Images

    Pakistanis and international and local media gather outside Osama Bin Laden's compound, where he was killed during a raid by U.S. Special Forces on May 3 in Abottabad, Pakistan. Bin Laden was killed during a U.S. military mission May 2)

    By John Roach, Contributing Writer, NBC News

    Osama bin Laden regularly taunted with propaganda photos and videos that left us asking: where in the world is he? U.S. spy agencies want software that analyzes and quickly identifies where such imagery was made.

    Currently, human intelligence analysts pore over propaganda imagery to tease out clues from things such as the geography, vegetation and even the style of clothes worn and gadgets used, and try to match them up with existing images taken from satellites and on the ground.


    But this is "an extremely time-consuming and labor-intensive activity that often meets with limited success," notes the U.S. Intelligence Advanced Research Projects Agency in its announcement for the Finder Program.

    The agency is the intelligence community's DARPA, the secretive military research agency that funds similar futuristic-sounding initiatives such as machines that are able to think for themselves.

    Computer programmers have already come up with a bunch of fancy tools to manipulate and find information in images, including animation software to trace faces through the years, Facebook's facial recognition program , and a search engine that IDs stars in photos of the night sky.

    Google recently launched an image search engine billed as being able to do the type of task IARPA wants, but it's full of kinks. It can't even distinguish George W. Bush from Barack Obama. Reverse image search engine TinyEye  is designed to perform a similar function.

    IARPA says these types of consumer-oriented systems are limited because they "tend to work best in geographic areas with significant population densities or that are well traveled by tourists, and where the query image or video contains notable features such as mountains or buildings."

    The Finder Program, as its wished-for software is called, "will deliver rigorously tested solutions for the image/video geolocation task in any outdoor terrestrial location."

    Work on the program is scheduled to kick off in earnest next January. That hoped-for solution isn't expected until 2016. But when it comes, and even as researchers work on the task, terrorists will have to be ever more careful about what to include in their propaganda imagery.

     


    Tip o' the Log to The Telegraph.

    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

     

    Comment

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  • 29
    Jun
    2011
    1:10pm, EDT

    African volcano spied from space

    Robert Simmon, using EO-1 ALI data

    The Nabro volcano has been erupting in the African nation of Eritrea since June 13. This image made with data from a NASA satellite is giving scientists one of their most detailed views of the remote, little-studied volcano.

    By John Roach, Contributing Writer, NBC News

    A NASA satellite captured this spectacular false-color image of the Nabro volcano erupting in a remote region of the northeastern African country of Eritrea.

    The bright red portions of the image indicate hot surfaces, NASA explains in an advisory. That's why the hot volcanic ash spewing out of the volcano's caldera glows red.


    To the west of the ash cloud, portions of the lava flow are visible. The front edge is particularly hot, thus red. The speckled bits upstream in the lava flow are likely regions where the cool, hardened crust is splitting and exposing fluid lava as the flow advances.

    The volcano is located in an isolated region of Eritrea near its border with Ethiopia. Scientists believe it began erupting on June 13. Ash from the volcano has disrupted flights and cut short Secretary of State Hilary Clinton's recent trip to Africa.

    Despite these impacts, scientists say they know very little about the volcano. When it was first detected, in fact, scientists thought it was the nearby Dubbi volcano. Imagery such as this photo from NASA's Earth Observing-1 satellite acquired on June 24 is providing the most detailed look at the eruption to date.

    More on African volcanoes:

    • Airlines watching East Africa volcanic ash cloud
    • Volcanic eruption cuts short Clinton African trip
    • Giant crack in Africa may create a new ocean
    • Science explodes at African lake

    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    5 comments

    Great, there's great imagery of a new volcano and some redneck uses the opportunity to slime Hillary Clinton. You're a standup schmuck, friend.

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  • 17
    Jun
    2011
    12:37pm, EDT

    A Martian moon slips by Jupiter

    ESA / DLR / FU Berlin (G. Neukum)

    Three frames from the series of 104 taken by Mars Express during the Phobos–Jupiter conjunction on 1 June 2011.

    By John Roach, Contributing Writer, NBC News

    Alignments of planets, moons and stars as seen from Earth always get us excited. This close-up view of the Martian moon Phobos lined up with Jupiter ups the ante – it was seen by a spacecraft orbiting Mars.


    Phobos is only 23 kilometers wide, whereas Jupiter is 142,000 kilometers across, but at the moment of the alignment on June 1, the European Space Agency's Mars Express orbiter was only 11,389 kilometers away from the lumpy moon. Jupiter was a further 529 million kilometers away.

    The High Resolution Stereo Camera on Mars Express was kept fixed on Jupiter for the conjunction, ensuring that the planet remained static in the frame. The operation returned a total of 104 images over a period of 68 seconds, all of them taken using the camera’s super-resolution channel.

    These images have been stitched together as a movie, seen below.

    On June 1 2001, Mars express watched as Phobos (the inner and larger of Mars' two moons) slipped past distant Jupiter.

    Watch on YouTube

    Beyond the cool factor of the chance alignment, the observations are helping astronomers refine their knowledge about the orbit of Phobos, which varies with time because of its small mass and extreme proximity to Mars, the Planetary Society's Emily Lakdawalla explains.

    Mars Express is studying Phobos to help out the planned Russian Phobos-Grunt mission to land a spacecraft on the moon and snag a sample for return to Earth, which is due for launch in November.

    More on Phobos:

    • Orbiter gets a fresh 3-D look at Phobos 
    • Martian moon in spotlight 
    • Martian moons pictured together for first time 
    • Phobos likely forged by catastrophic blast 

    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    16 comments

    So does Jupiter actually appear as a disc from Mars?

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  • 16
    Jun
    2011
    3:33pm, EDT

    NASA / ESA / Hubble Heritage collaboration

    Dark lanes of dust crisscross the giant elliptical galaxy Centaurus A where a firestorm of star formation is occurring due to a merger with another galaxy.

    Hubble spies a firestorm of star birth

    By John Roach, Contributing Writer, NBC News

    Dark clouds of gas and dust bring out a sense of storminess in this region of active star formation in the elliptical galaxy Centaurus A, located 11 million light years from Earth.


    The composite image was made with the Wide Field Camera 3 on the Hubble Space Telescope, which spans wavelengths from ultraviolet through near infrared to reveal the vibrant glow of young, blue star clusters in regions normally obscured by dust.

    The dustiness and warped shape of Centaurus A are evidence of a past collision and merger with another galaxy. Such smashups cause hydrogen gas clouds to compress, triggering a firestorm of star formation. These regions are visible as the red patches in this image, according on an image advisory.

    The galaxy also harbors a supermassive black hole at its nucleus that ejects jets of high speed gas into space. Neither the supermassive black hole or the jets is visible in this image.

    More about Centaurus A and galactic mergers:

    • Giant cannibal galaxy caught in mid-gobble
    • Snapshot reveals a black hole's jets
    • Monster black holes result of galaxies' collision
    • Hubble photo shows stretched out galaxy

    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    11 comments

    11 million LY's away?? Looks like a stones throw away. The HST is a marvel that has earned it's place in history. Oh and the "red patches" are hydrogen alpha regions (Hll regions) of star formation. They are pinky red because that is the wavelength of the light of ionized hydrogen gas in t …

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  • 15
    Jun
    2011
    2:00pm, EDT

    NASA / JPL / Caltech

    NASA's Spitzer Space Telescope spots a glowing emerald nebula in the murky clouds encircled by the tail of the constellation Scorpius. These bubbles are thought to be common throughout the Milky Way.

    Space telescope spies Green Lantern's ring

    By John Roach, Contributing Writer, NBC News

    A green ring fit for a Green Lantern, the superhero protectors of peace and justice throughout the universe, has been spied by NASA's Spitzer Space Telescope in the murky clouds encircled by the tail of the constellation Scorpius.

    The ring glows in infrared colors invisible to the naked eye, but show up brightly in the telescope's infrared detectors. Astronomers believe the rings are sculpted by bubbles of hot gas and dust blown by the powerful light of "O" stars, the most massive stars known to exist.


    The difference in colors — and thus the reason for the green ring — stems from how the light and wind are interacting with the gas and dust, explained Sean Carey, a Spitzer scientist at the California Institute of Technology.

    "The main reason that there is no green inside the bubble is that the smallest dust grains, the polycyclic aromatic hydrocarbons which produce the green emission, are destroyed in the inside of the bubble by a combination of the ultraviolet radiation and the shocks driving through the gas," he said.

    The slightly larger dust grains remaining inside the bubble are heated up by the radiation from the O stars and glow red. The green ring, by contrast, is where the green glowing hydrocarbons and larger grains are still present.

    According to Spitzer scientists, these bubbles are common throughout our Milky Way galaxy, similar to the way that many Green Lanterns patrol different sectors of space. The small objects at the lower right area of the image may, in fact, be similar regions seen at a much great distance across the galaxy.

    NASA hopes to learn more about these bubbles and you can help them by joining The Milky Way Project where you can find and catalog bubbles in our galaxy. Ultimately, the project will give us all a better understanding about the life cycle of stars.

    More images of stars and bubbles:

    • Hubble captures image of star-forming lab
    • Witness the glorious birth and death of stars
    • Infrared portrait traces the life cycle of stars
    • Hot new stars featured in cosmic portrait

    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    6 comments

    When I see pictures like this I always get sad because I am stuck on this planet unable to go out into space and explore all the amazingly beautiful things out in the Universe.

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  • 26
    May
    2011
    1:17pm, EDT

    NASA / JPL-Caltech / L. Lanz (Harvard-Smithsonian CfA)

    This montage shows three examples of colliding galaxies from a new photo atlas of galactic "train wrecks." The new images combine observations from NASA's Spitzer Space Telescope, which observes infrared light, and NASA's Galaxy Evolution Explorer (GALEX) spacecraft, which observes ultraviolet light.

    Galactic train wrecks show our future

    By John Roach, Contributing Writer, NBC News

    Five billion years from now our galaxy, the Milky Way, will collide with the Andromeda galaxy, triggering the birth of stars from smashed together clouds of cosmic gas and dust. This is old news, but exactly what the galactic wreckage will look like is unknown.


    Part of the problem is that these mergers take place over millions to billions of years, which is much too long for anyone to witness the whole process. As a work around, astronomers study a variety colliding galaxies at various stages of merging to piece together the picture of what will happen to us.

    They've now gotten enough data to assemble an atlas of the galactic train wrecks from start to finish.

    "This atlas is the first step in reading the story of how galaxies form, grow, and evolve," Lauranne Lanz of the Harvard Smithsonian Center for Astrophysics, said in a news release announcing the accomplishment.

    She and colleagues combined recent data from NASA's Galaxy Evolution Explorer (GALEX) spacecraft and Spitzer Space Telescope and presented the images Wednesday at a meeting of the American Astronomical Society in Boston.

    GALEX observes in ultraviolet light, which captures emission from hot young stars. Spitzer sees the infrared emission from warm dust heated by those stars, as well as from stellar surfaces. The combined data highlight areas where stars are forming most rapidly, and together permit a more complete census of the new stars.

    In general, galaxy collisions trigger star formation, though some mergers trigger few stars than others. Lanz and her colleagues want to figure out what differences in physical processes cause these varying outcomes, which will help guide computer simulations of these smashups.

    "We're working with the theorists to give our understanding a reality check," she said in the news release. "Our understanding will really be tested in five billion years when the Milky Way experiences its own collision."

    More stories on galactic collisions:

    • Head-on galactic collision is an impressive sight
    • Black hole knocked off axis by galaxy collision
    • Andromeda involved in galactic collision
    • Galacitc merger could boot our solar system

    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    16 comments

    Our future? Do they really think a species as bent on self destruction as this one is going to be around even a fraction of the time before the 'train wreck'? I'd like to think humans can stop being so self absorbed and be survival oriented and work for a future but the daily news makes that a fanta …

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  • 12
    May
    2011
    12:07pm, EDT

    NASA / ESA and the Hubble Heritage Team. Acknowledgment: R. O’Connell (University of Virginia) and the WFC3 Scientific Oversi

    Galaxy NGC 4214, pictured here in an image from the NASA/ESA Hubble Space Telescope's newest camera, is an ideal location to study star formation and evolution. Dominating much of the galaxy is a huge glowing cloud of hydrogen gas in which new stars are being born.

    Hubble captures image of star-forming lab

    By John Roach, Contributing Writer, NBC News

    The Hubble telescope captured this crystal-clear optical and near-infrared view of a dwarf galaxy that is glowing brightly with hot, young stars and gas clouds, making it an ideal laboratory for studying star formation and evolution, astronomers reported Thursday.

    The image shows that even in the scale of galaxies, great things come in small packages.


    "Dwarf galaxy NGC 4214 may be small, but what it lacks in size it makes up for in content. It is packed with everything ... an astronomer could ask for," the European Space Agency noted in an image advisory.

    The galaxy is located around 10 million light-years away in the constellation of Canes Venatici ("The Hunting Dogs"). Inside the hole of the large, heart-shaped cavity at the center of the image lies a large cluster of massive, young stars ranging in temperature from 10,000 to 50,000 degrees C. Their strong stellar winds blew the cavity clear of gas, which prevents any further star formation.

    Other regions of the galaxy contain large amounts of star-forming gas, seen glowing red in this image. The area with the most hydrogen gas, and thus the youngest cluster of stars, about 2 million years old, lies in the upper portion of this image. This region is visible due to ionization of the surrounding gas by ultraviolet light of a young cluster of stars within.

    Clusters of much older, red supergiant stars in a late stage of their evolution are also dotted across the galaxy. The variety of stars at different stages in their evolution indicate that the recent and ongoing starburst periods are by no means the first, and the galaxy's abundant supply of hydrogen means star formation will continue into the future.

    The image was made with the Wide Field Camera 3 instrument on the Hubble Space Telescope.


    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    23 comments

    Simply beautiful. I have been in search of a new desktop background.

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  • 9
    May
    2011
    12:32pm, EDT

    ESA / AOES Medialab

    An artist's impression shows a galaxy with a molecular outflow. Herschel has discovered that such outflows can travel at 1000 km/s, which could deplete the galaxy of the gas needed for further star formation within 1 million to 100 million years.

    Raging winds strip galaxies of gas

    By John Roach, Contributing Writer, NBC News

    Raging winds up to 10,000 times more powerful than a terrestrial hurricane have been detected streaming away from galaxies and stripping them of star-forming gas, according to a new study.

    The strongest winds, observed with the European Space Agency's Herschel infrared space observatory, reach up to 1,000 kilometers per second (2.2 million miles per hour).


    The winds could be generated by the intense emission of light and particles from newly formed stars, the shockwaves of stellar explosions, or by the black holes at the center of galaxies, the agency notes in a media advisory.

    The finding may help explain why some galaxies suddenly stop forming new stars. Scientists studying the data infer that about 1,200 times the mass of our sun is being lost each year from the galaxies with the most vigorous outflows. That is sufficient to strip them of star-forming gas in as little as a million years.

    The fastest of the winds appear to come from galaxies that have the brightest galactic nuclei in which a black hole is feeding from its surroundings, a finding that could be a step towards explaining how elliptical galaxies are formed.

    Elliptical galaxies are vast islands of stars that have stopped producing appreciable numbers of new stars because they have exhausted their gas supplies.

    ESA explains that as smaller galaxies interact and merge with each other, more food is supplied to the central black hole, making it larger and more active. This, in turn, could result in a more powerful wind, which removes the molecular gas and halts star formation, leading to an elliptical galaxy.

    The inhibition of star formation in a galaxy is known as negative feedback.

    "By catching molecular outflows in the act, Herschel has finally yielded long-sought-after evidence that powerful processes with negative feedback do take place in galaxies and dramatically affect their evolution," Goran Pilbratt, ESA Herschel project scientist, said in the media advisory.

    More stories on violent galactic processes:

    • Stars form within black hole's destructive reach
    • Starburst galaxy unleashes gassy 'superwind'
    • Starbirth goes wild in 'cosmic hurricane'
    • Blackholes are a turnoff for star formation
    • Giant cannibal galaxy caught in mid-gobble

    'Massive molecular outflows and negative feedback in ULIRGs observed by Herschel-PACS,' by Sturm et al., is published in Astrophysical Journal Letters, vol. 733, page L16.

    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    6 comments

    I love astronomy. It's one of the few fields in science where all of the rules are not etched in stone.

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  • 4
    May
    2011
    9:57am, EDT

    Telescopes snag Meathook Galaxy

    ESO

    This picture of the Meathook Galaxy was taken by the Wide Field Imager on the MPG/ESO 2.2-metre telescope at La Silla, Chile. This view includes the whole galaxy and the surrounding sky, and clearly shows the asymmetric spiral arms. The longer of the two arms has intense star formation, which is visible here as a pink glow.

    By John Roach, Contributing Writer, NBC News

    Two complementary views of the so-called Meathook Galaxy, released today, show how astronomers are piecing together the history of this lopsided group of stars.

    The galaxy, located about 50 million light years away in the southern constellation Volans (The Flying Fish), is recognized for its asymmetrical spiral arms. One is tightly folded in on itself and host to a recent supernova, and the other is dotted with new star formation and extends far out from the nucleus. 


    NASA / ESA / ESO

    This close-up Hubble view of the Meathook Galaxy focuses on the more compact of its two asymmetric spiral arms as well as the central regions. The spiral arm was the location of a supernova that exploded in 1999. These Hubble observations were made in 2006 in order to study the aftermath of this supernova. Ground-based data from MPG/ESO 2.2-metre telescope were used to fill out parts of the edges of this image.

    The broa- view image above was taken by the Wide Field Imager the MPG/ESO 2.2-meter telescope at La Silla, Chile. It clearly shows the double hook shape that gives NGC 2442, as it the galaxy is officially known, its nickname.

    The lopsided appearance is thought to be due to the gravitational interactions of another galaxy, though the culprit remains unknown, the European Space Agency noted in an image advisory. This interaction is probably responsible for an episode of recent star formation, seen as the patches of pink and red, particularly in the longer of the two spiral arms.

    These colors come from hydrogen gas in star forming regions, ESA explains. As the powerful radiation of newborn stars excites the gas in the clouds they formed from, it glows in a bright shade of red.

    The close-up view from the Hubble Space Telescope focuses on the nucleus of the Meathook and the more compact of its two spiral arms. Not seen in the image is a massive star that exploded at the end of its life in a supernova, witnessed in 1999. By comparing older ground-based observations, previous Hubble images and these made in 2006, astronomers have been able to study the details of the star's violent death. By the time this image was made, the supernova had faded.


    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    34 comments

    I've always wondered how much "distortion" is in perspectives like this Meathook galaxy. If the light from stars on the far side left 80-100,000 years earlier than the light from the near side, how much difference in their positions would there be ?

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John Roach, Contributing Writer, NBC News

John Roach is a contributing writer for NBC News. From climate change and mass extinctions to human evolution and deep space, his writing explores life on Earth and its place in the universe. He was a staff writer at the Environmental News Network for several years and has contributed to National Geographic News for more than a decade.

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