Wednesday 16 July 2014

X-ray laser gives buckyballs a big kick

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Scientists at SLAC have been blowing up “buckyballs” – soccer-ball-shaped carbon molecules – with an X-ray laser to understand how they fly apart. The results, they say, will aid biological studies by improving the analysis of X-ray images of tiny viruses, individual proteins and other important biomolecules. The experiment was carried out at SLAC’s Linac Coherent Light Source (LCLS) X-ray laser, a DOE Office of Science user facility, and the results appear in the June 27 issue of Nature Communications. “It’s sort of a Catch-22: You need the X-ray laser focus to be extremely intense and bright to get a good picture,” says Nora Berrah, an experimental physicist at the University of Connecticut. “But the X-rays also trigger unexpectedly rapid and substantial damage and motion in the atoms, resulting in a blurred image.” Berrah led the research with Robin Santra, a theorist from the Center for Free-Electron Laser Science at Germany’s DESY lab. Because buckyballs are composed entirely of carbon – the backbone of all life on Earth – they are a good stand-in for biological molecules, many of which also have strong atomic bonds. They got their formal name, “buckminsterfullerene,” for their resemblance to the geodesic domes invented by R. Buckminster Fuller. Within 20

The post X-ray laser gives buckyballs a big kick has been published on Technology Org.

 
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Asteroid Vesta to reshape theories of planet formation

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Researchers have a better understanding of the asteroid Vesta and its internal structure, thanks to numerical simulations and data from the space mission Dawn. Their findings question contemporary models of rocky planet formation, including that of Earth.

via Science Daily

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NASA's Van Allen Probes show how to accelerate electrons

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One of the great, unanswered questions for space weather scientists is just what creates two gigantic donuts of radiation surrounding Earth, called the Van Allen radiation belts. Recent data from the Van Allen Probes -- two nearly identical spacecraft that launched in 2012 -- address this question.

via Science Daily

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Compressed diamond sheds light on mega-planets

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Physicists in the United States on Wednesday reported they had compressed diamond to a density greater than that of lead, a technical feat that yields insights into the secrets of giant planets.



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Supercomputers reveal strange, stress-induced transformations in world's thinnest materials

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Interested in an ultra-fast, unbreakable, and flexible smart phone that recharges in a matter of seconds? Monolayer materials may make it possible. These atom-thin sheets -- including the famed super material graphene -- feature exceptional and untapped mechanical and electronic properties. But to fully exploit these atomically tailored wonder materials, scientists must pry free the secrets of how and why they bend and break under stress. Supercomputer simulations have revealed unexpected transitions in graphene and other promising super materials under strain.

via Science Daily

Planets and dwarf planets poster

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


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Planets and dwarf planets of the solar system

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HIV re-emerges in 'cured' US girl

Science Focus

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A child born in the US with HIV and believed cured after very early treatment has now been found to still harbour the virus, doctors say. 
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 » see original post http://www.bbc.co.uk/news/health-28257768#sa-ns_mchannel=rss&ns_source=PublicRSS20-sa
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Jamming with the cosmos: CERN and the music of physics

The Moon Eclipses Saturn

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Out There: Stalking the Shadow Universe

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It has long been theorized that it is dark matter that provides the scaffolding for stars and galaxies. Now, scientists are using computer simulations to show us the universe we can’t see.















via New York Times

3-D nanostructure could benefit nanoelectronics, gas storage: functional advantages of 3-D boron nitride predicted

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A three-dimensional porous nanostructure would have a balance of strength, toughness and ability to transfer heat that could benefit nanoelectronics, gas storage and composite materials that perform multiple functions, according to engineers.

via Science Daily

ucsdnews.ucsd.edu/archives/date/290614

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Researchers at the University of California, San Diego School of Medicine have discovered a widely distributed group of marine bacteria that produce compounds nearly identical to toxic man-made fire retardants. Among the chemicals produced by the ocean-dwelling microbes, which have been found in habitats as diverse as sea grasses, marine sediments and corals, is a potent endocrine disruptor that mimics the human body’s most active thyroid hormone. The study is published in the June 29 online issue of Nature Chemical Biology. “We find it very surprising and a tad alarming that flame retardant-like chemicals are biologically synthesized by common bacteria in the marine environment,” said senior author Bradley Moore, PhD, a professor at the UC San Diego Skaggs School of Pharmacy and Pharmaceutical Sciences and Scripps Institution of Oceanography. The toxic compounds are known as polybrominated diphenyl ethers (PBDEs), a subgroup of brominated flame retardants that are combined into foam, textiles and electronics to raise the temperature at which the products will burn. Certain formulations of PBDEs are no longer used in automobile and home products in the United States, but testing by the Environmental Protection Agency indicates that most Americans and Canadians carry traces of the chemicals. Indeed, levels exceed

The post ucsdnews.ucsd.edu/archives/date/290614 has been published on Technology Org.

 
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Helix Nebula in space Poster

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


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This infrared image from NASA's Spitzer Space Telescope shows the Helix Nebula, a cosmic starlet often photographed by amateur astronomers for its vivid colors and eerie resemblance to a giant eye. The nebula, located about 700 light-years away in the constellation Aquarius, belongs to a class of objects called planetary nebulae. Discovered in the 18th century, these colorful beauties were named for their resemblance to gas-giant planets like Jupiter. Planetary nebulae are the remains of stars that once looked a lot like our sun. When sun-like stars die, they puff out their outer gaseous layers. These layers are heated by the hot core of the dead star, called a white dwarf, and shine with infrared and visible colors. Our own sun will blossom into a planetary nebula when it dies in about five billion years. In Spitzer's infrared view of the Helix nebula, the eye looks more like that of a green monster's. Infrared light from the outer gaseous layers is represented in blues and greens. The white dwarf is visible as a tiny white dot in the center of the picture. The red color in the middle of the eye denotes the final layers of gas blown out when the star died. The brighter red circle in the very center is the glow of a dusty disk circling the white dwarf (the disk itself is too small to be resolved). This dust, discovered by Spitzer's infrared heat-seeking vision, was most likely kicked up by comets that survived the death of their star. Before the star died, its comets and possibly planets would have orbited the star in an orderly fashion. But when the star blew off its outer layers, the icy bodies and outer planets would have been tossed about and into each other, resulting in an ongoing cosmic dust storm. Any inner planets in the system would have burned up or been swallowed as their dying star expanded. So far, the Helix nebula is one of only a few dead-star systems in which evidence for comet survivors has been found.

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Orion Nebula and Trapezium Stars Sticker

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


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Galaxies, Stars and Nebulae series A gorgeous picture from the deep universe featuring the bubbling, seething mass of gas and dust that is the Orion Nebula, 1500 light years away and the closest star-forming region to us. The nebula is a star nursery in which there are birthing, new-born, young and adult stars. Look carefully in the brightest central region and you'll see the Trapezium, four of the most massive stars in Orion.

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Image credit: NASA, ESA, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team

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Solar Flair Wall Skins

Here's a great wall decal featuring a beautiful image from deep space


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Stunning Solar Flair iPad Air with sun flares, earth and nebulas. Psalm 19:1 The heavens declare the glory of God; the skies proclaim the work of his hands.

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Dwarf Galaxy Holmberg IX iPad Mini Covers

Here's a great iPad case from Zazzle featuring a Hubble-related design. Maybe you'd like to see your name on it? Click to personalize and see what it's like!


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"This loose collection of stars is actually a dwarf irregular galaxy, called Holmberg IX. It resides just off the outer edge of M81, a large spiral galaxy in Ursa Major. This image was taken with Hubble's Advanced Camera for Surveys in early 2006. Holmberg IX is of the so-called Magellanic type of galaxy, as its size and irregularity in structure are similar to the Small Magellanic Cloud, a neighbor to our own Milky Way. Holmberg IX was first discovered by astronomer Sidney van den Bergh in 1959, and cataloged as DDO 66. The galaxy received its "Holmberg IX" naming when it was discussed in Eric Holmberg's study of groups of galaxies ten years later. It is suspected that the dwarf galaxy was created as a result of a galactic interaction between M81 and neighboring galaxy M82."

(qtd. from Hubblesite.org NewsCenter release STScI-2008-02)

Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

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