Monday 13 July 2015

Opening a New Route to Photonics

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A new route to ultrahigh density, ultracompact integrated photonic circuitry has been discovered by researchers with the  Lawrence

The post Opening a New Route to Photonics has been published on Technology Org.

 
#materials 
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Nerve-wracking flyby of Pluto: New Horizons probe begins complicated dance

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The moment is finally here: after a decade of travel, the New Horizons probe is about to encounter Pluto. Flying faster than a speeding bullet -- literally -- the probe has to perform complex maneuvers, and go completely silent before scientists on Earth will hear anything, an astronomer says.
via Science Daily
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Polymer mold makes perfect silicon nanostructures

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In a breakthrough for nanoscience, polymer engineers have made such a mold for nanostructures that can shape liquid silicon out of an organic polymer material. This paves the way for perfect, 3-D, single crystal nanostructures.
via Science Daily

Clay sheets stack to form proton conductors

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A researcher employs a clay typically used for gardening to develop a proton-conducting, bulk nanostructured material.
via Science Daily

Out There: The Telescope of the 2030s

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Facing a funding labyrinth, American university astronomers have called on NASA to begin planning for a supersize version of the Hubble.










via New York Times

White Dwarf Star in Aquarius Print

Here's a great poster featuring a beautiful image from deep space


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ImageID: 42-20484545 / NASA / JPL-Caltech/Corbis / White Dwarf Star in Aquarius

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Using lasers to build molecules instead of tearing them apart

Science Focus

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In general, the world of chemistry is a closed book. Reactions happen, and my understanding is limited to counting electrons and seeing if they add up. Despite this ignorance, there is a particular field of chemistry that I really love: photochemistry, or chemistry driven by light. Nothing gives me more pleasure than setting stuff on fire with a laser—I mean carefully studying light-controlled reactions.

Seriously though, there is this whole field out there where chemists and physicists study and control reactions using light. Or, more accurately, they study how to control the breakup of molecules using light fields. These experiments make use of something called coherent control, where we use light to steer electrons. As a result, the light controls the chemistry. But creating molecules using the same idea has proven to be hard—really hard. That makes a recent publication on the creation of molecules using coherent control reasonably important.

Coherent destruction

One of the easier—and I use that word in the sense of "not impossible"—demonstrations of coherent control involves tearing molecules apart. The reason this is easy is because as long as your laser is powerful enough, you can always tear molecules apart. That means you can always start with a light pulse that does the job, then by tweaking the pulse shape (more on that below), you can increase the efficiency with which you break molecules. Or, you can aim to break particular bonds.

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#science 
 » see original post http://feeds.arstechnica.com/~r/arstechnica/science/~3/MXsRohQEF8Y/
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Can Heat Be Controlled as Waves?

Science Focus

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A growing interest in thermoelectric materials – which convert waste heat to electricity – and pressure to improve

The post Can Heat Be Controlled as Waves? has been published on Technology Org.

 
#physics 
 » see original post http://feedproxy.google.com/~r/TechnologyOrgPhysicsNews/~3/7Z2GP-JgJ6Y/
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Crab Pulsar Time Lapse - Neutron Star Square Sticker

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Galaxies, Stars and Nebulae series

Multiple observations made over several months with NASA's Chandra X-ray Observatory and the Hubble Space Telescope captured the spectacle of matter and antimatter propelled to near the speed of light by the Crab pulsar, a rapidly rotating neutron star the size of Manhattan.

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Image code: crbplsr

Image credit: NASA's Chandra X-ray Observatory and the Hubble Space Telescope

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Last Look at Pluto's Charon Side

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Rosetta: preparing for perihelion

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Rosetta’s investigations of its comet are continuing as the mission teams count down the last month to perihelion – the closest point to the Sun along the comet’s orbit – when the comet’s activity is expected to be at its highest.


via ESA Space Science
http://www.esa.int/Our_Activities/Space_Science/Rosetta/Rosetta_preparing_for_perihelion

Eye in Orion iPad Mini Covers

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Digital artwork inspired by one of NASA/Hubble's images of the Orion Nebula.

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NASA Technology Protects Webb Telescope from Contamination

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Contamination from organic molecules can harm delicate instruments and engineers are taking special care at NASA to prevent

The post NASA Technology Protects Webb Telescope from Contamination has been published on Technology Org.

 
#materials 
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Stonehenge at Night Posters

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ImageID: AX028971 / M. Dillon / CORBIS / Stonehenge at Night /

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Crab Pulsar Time Lapse - Neutron Star Classic Round Sticker

Here's a great sheet of stickers featuring a beautiful image from deep space


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Galaxies, Stars and Nebulae series

Multiple observations made over several months with NASA's Chandra X-ray Observatory and the Hubble Space Telescope captured the spectacle of matter and antimatter propelled to near the speed of light by the Crab pulsar, a rapidly rotating neutron star the size of Manhattan.

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All items in the Galaxies, Stars and Nebulae series

Image code: crbplsr

Image credit: NASA's Chandra X-ray Observatory and the Hubble Space Telescope

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What happens when cosmic giants meet galactic dwarfs?

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According to a new study of more than 20,000 merging galaxies, when two different sized galaxies smash together, the larger galaxy stops the smaller one making new stars.
via Science Daily
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Monogram Barred Spiral Galaxy NGC 1672 iPad Folio Case

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tagged with: monogram initials, star galaxies, deep space astronomy, barred spiral galaxy, starry space picture, galactic arms, supermassive black hole, dust lanes, star forming galaxy, hrbstslr bsgsst

Galaxies, Stars and Nebulae series This NASA Hubble Space Telescope view of the nearby barred spiral galaxy NGC 1672 unveils details in the galaxy's star-forming clouds and dark bands of interstellar dust.
One of the most striking features is the dust lanes that extend away from the nucleus and follow the inner edges of the galaxy's spiral arms. Clusters of hot young blue stars form along the spiral arms and ionize surrounding clouds of hydrogen gas that glow red. Delicate curtains of dust partially obscure and redden the light of the stars behind them by scattering blue light.
Galaxies lying behind NGC 1672 give the illusion they are embedded in the foreground galaxy, even though they are really much farther away. They also appear reddened as they shine through NGC 1672's dust. A few bright foreground stars inside our own Milky Way Galaxy appear in the image as bright and diamond-like objects.
As a prototypical barred spiral galaxy, NGC 1672 differs from normal spiral galaxies, in that the arms do not twist all the way into the center. Instead, they are attached to the two ends of a straight bar of stars enclosing the nucleus. Viewed nearly face on, NGC 1672 shows intense star formation regions especially off in the ends of its central bar.
Astronomers believe that barred spirals have a unique mechanism that channels gas from the disk inward towards the nucleus. This allows the bar portion of the galaxy to serve as an area of new star generation.
NGC 1672 is also classified as a Seyfert galaxy. Seyferts are a subset of galaxies with active nuclei. The energy output of these nuclei can sometimes outshine their host galaxies. This activity is powered by accretion onto supermassive black holes.
NGC 1672 is more than 60 million light-years away in the direction of the southern constellation Dorado. These observations of NGC 1672 were taken with Hubble's Advanced Camera for Surveys in August of 2005. The composite image was made by using filters that isolate light from the blue, green, and infrared portions of the spectrum, as well as emission from ionized hydrogen.
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Image credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration

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