Friday 28 February 2014

Cancer targeted treatments from space station discoveries

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Invasive and systemic cancer treatment is a necessary evil for many people with the devastating diagnosis. These patients endure therapies with ravaging side effects, including nausea, immune suppression, hair loss and even organ failure, in hopes of eradicating cancerous tissues in the body. If treatments targeted a patient's cancerous tissues, it could provide clinicians with an alternative to lessen the delivery of toxic levels of chemotherapy or radiation. Imagine the quality of life from such therapies for patients. Remarkably, research that began in space may soon result in such options here on Earth.

via Science Daily

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NASA's Curiosity Mars Rover views striated ground

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NASA's Curiosity Mars rover has reached an area where orbital images had piqued researchers' interest in patches of ground with striations all oriented in a similar direction.

via Science Daily

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Radar images of near-Earth Asteroid 2006 DP14

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A collage of radar images of near-Earth asteroid 2006 DP14 was generated by NASA scientists using the 230-foot (70-meter) Deep Space Network antenna at Goldstone, Calif., on the night of Feb. 11, 2014.

via Science Daily

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Closest, brightest supernova in decades is also a little weird

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The closest and brightest supernova in decades, SN 2014J, brightens faster than expected for Type Ia supernovae, the exploding stars used to measure cosmic distances, according to astronomers. Another recent supernova also brightened faster than expected, suggesting that there is unsuspected new physics going on inside these exploding stars. The finding may also help physicists improve their use of these supernovae to measure cosmic distance.

via Science Daily

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Möbius Arch Moonrise

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Only two days past full, February's moon shines through thin clouds, rising on the left in this fisheye night skyscape. The moonlight illuminates a weathered, rounded foreground in the Alabama Hills, conveniently located east of Mt. Whitney along the Sierra Nevada range in California, USA, planet Earth. Orion the Hunter stands at the right, a familiar northern winter constellation. Bright Jupiter, the solar system's ruling gas giant, is near center at the top of the frame. Below Jupiter, Sirius, alpha star of the Big Dog, poses above a bowed and twisted landform known as Möbius Arch, its curve reminiscent of the mathematically famous surface with only one side. Of course, instead of using rock, wind, and weather, a Möbius strip is easier to make with paper, scissors, and tape.

Zazzle Space Gifts for young and old

Deal of the Day: Bushnell Legend Ultra HD 10x 42mm Roof Prism Binocular

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Expires Mar 1, 2014

Thursday 27 February 2014

Fat or flat: Getting galaxies into shape

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Australian astronomers have discovered what makes some spiral galaxies fat and bulging while others are flat discs—and it's all about how fast they spin.



Zazzle Space market place

NASA's Kepler mission announces a planet bonanza, 715 new worlds

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NASA's Kepler mission announced Wednesday the discovery of 715 new planets. These newly-verified worlds orbit 305 stars, revealing multiple-planet systems much like our own solar system. Nearly 95 percent of these planets are smaller than Neptune, which is almost four times the size of Earth. This discovery marks a significant increase in the number of known small-sized planets more akin to Earth than previously identified exoplanets, which are planets outside our solar system.

via Science Daily

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Hubble monitors supernova in nearby galaxy M82

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Astronomers have taken a Hubble Space Telescope composite image of a supernova explosion designated SN 2014J in the galaxy M82. At a distance of approximately 11.5 million light-years from Earth it is the closest supernova of its type discovered in the past few decades. The explosion is categorized as a Type Ia supernova, which is theorized to be triggered in binary systems consisting of a white dwarf and another star -- which could be a second white dwarf, a star like our sun, or a giant star.

via Science Daily

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Daytime Moon Meets Morning Star

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Venus now appears as planet Earth's brilliant morning star standing above the eastern horizon before dawn. For most, the silvery celestial beacon rose in a close pairing with an old crescent Moon on February 26. But seen from locations in western Africa before sunrise, the lunar crescent actually occulted or passed in front of Venus, also in a crescent phase. Farther to the east, the occultation occurred during daylight hours. In fact, this telescopic snapshot of the dueling crescents was captured just before the occultation began under an afternoon's crystal clear skies from Yunnan Province, China. The unforgettable scene was easily visible to the naked eye in broad daylight.

Zazzle Space Gifts for young and old

Hubble Monitors Supernova in Nearby Galaxy M82



Get larger image formats

This is a Hubble Space Telescope composite image of a supernova explosion designated SN 2014J in the galaxy M82, at a distance of approximately 11.5 million light-years from Earth. Astronomers using a ground-based telescope discovered the explosion on January 21, 2014. This Hubble photograph was taken on January 31, as the supernova approached its peak brightness.




via HubbleSite NewsCenter -- Latest News Releases

http://hubblesite.org/newscenter/archive/releases/2014/13/

Wednesday 26 February 2014

How small cosmic seeds grow into big stars

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New images provide the most detailed view yet of stellar nurseries within the Snake nebula. These images offer new insights into how cosmic seeds can grow into massive stars. Stretching across almost 100 light-years of space, the Snake nebula is located about 11,700 light-years from Earth in the direction of the constellation Ophiuchus.

via Science Daily

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'Super-Earths' may be dead worlds: Being in habitable zone is not enough

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In the last 20 years the search for Earth-like planets around other stars has accelerated, with the launch of missions like the Kepler space telescope. Using these and observatories on the ground, astronomers have found numerous worlds that at first sight have similarities with the Earth. A few of these are even in the ‘habitable zone’ where the temperature is just right for water to be in liquid form and so are prime targets in the search for life elsewhere in the universe. New results suggest that for some of the recently discovered super-Earths, such as Kepler-62e and -62f, being in the habitable zone is not enough to make them habitats.

via Science Daily

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SMA unveils how small cosmic seeds grow into big stars

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New images from the Smithsonian's Submillimeter Array (SMA) telescope provide the most detailed view yet of stellar nurseries within the Snake nebula. These images offer new insights into how cosmic seeds can grow into massive stars.



Zazzle Space market place

The Carina Nebula Posters

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

after scouring the Zazzle market place for a while, I settled on this as my choice for today. By toemann09, another talented creative from the Zazzle community!


tagged with: carina nebula, nebula, space, stars, astronomy, telescope, hubble

This is a stunning image of The Carina Nebula taken by the Hubble Space Telescope.

»visit the toemann09 store for more designs and products like this
Click to customize with size, paper type etc.
via Zazzle Astronomy market place

Aurora over New Zealand

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Sometimes the more you look at an image, the more you see. Such may be the case for this beautiful nighttime panorama taken last week in New Zealand. Visible right off, on the far left, are common clouds, slightly altered by the digital fusion of combining 11 separate 20-second exposures. More striking, perhaps, is the broad pink aurora that dominates the right part of the image, a less common auroral color that is likely tinted by excited oxygen atoms high in Earth's atmosphere. Keep looking and you might notice a bright light just beyond the mountain on the left. That is the rising Moon -- and an even closer look will reveal faint crepuscular rays emanating from it. Musing over the image center may cause you to notice the central band of the Milky Way Galaxy which here appears to divide, almost vertically, the left clouds from the right aurora. Inspecting the upper right of the image reveals a fuzzy patch, high in the sky, that is the Small Magellanic Cloud. Numerous stars discretely populate the distant background. Back on Earth, the image foreground features two domes of the Mt. John University Observatory and a camera tripod looking to capture much of this scene over a serene Lake Tekapo.
Tomorrow's picture: open space
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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)
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Zazzle Space Gifts for young and old

A Nobel laureate's formula for the universe



Nobel laureate François Englert at CERN last week. The equation on the blackboard describes the Brout-Englert-Higgs mechanism that gives particles mass (Image: Maximilien Brice)




A Nobel laureate and a blackboard at CERN is all you need to explain the fundamental physics of the universe. At least, that's what François Englert convinced us on his visit to CERN last week.


Englert shared the 2013 Nobel prize in physics with Peter Higgs "for the theoretical discovery of a mechanism that contributes to our understanding of the origin of mass of subatomic particles". In the video below, he explains how he and Higgs manipulated equations containing mathematical constructs called scalar fields to predict the existence of the Brout-Englert-Higgs field.


Nobel laureate François Englert explains the Brout-Englert-Higgs mechanism that gives particles mass, with the help of a blackboard (Video: CERN)


According to Englert, the equation describing this mechanism is built in two parts. One part consists of scalar fields; the other consists of constructs called gauge fields. Englert explains that a big problem in particle physics in the 1960s was to find a gauge field that had mass. Solving that problem - working out how a gauge field could have mass -would help to explain other problems in physics, such as how to mathematically describe short-range interactions inside the nuclei of atoms. But Englert says that you cannot easily just add mass to a gauge field "off-hand". He needed another theoretical approach.


The key was to add a new part – a new scalar field – to the equation describing the mass mechanism. Part of this new scalar field could be mathematically simplified. What came out of the algebraic manipulation was a term that gave rise to "a condensate spread out all over the universe". Then, the interaction between the condensate and another part of the equation could be generalized, says Englert, to give mass to elementary particles. Easy peasy!


"I know this is extremely abstract," says a modest Englert of his explanation. "But if I have two minutes [to explain it], I can hardly do more!"


Find out more about the Higgs boson in the pages below.





via CERN: Updates for the general public

http://home.web.cern.ch/about/updates/2014/02/nobel-laureates-formula-universe

Constellations Poster

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

after scouring the Zazzle market place for a while, I settled on this as my choice for today. By vladstudio, another talented creative from the Zazzle community!


tagged with: artsprojekt, constellations, unitization, orion, constellation, network topology, asterism, astronomy, chunking, unitisation, celestial sphere, redundancy, night sky, topology, list of constellations, configuration, international astronomical union, plan, ptolemy, design, almagest, nicolas louis de lacaille, former constellations, chinese constellation, nakshatra, astrology

Space is never-ending source of inspiration for me! I wanted to draw a map of constellations in Photoshop, so I found suitable projection in Internet and used it as a reference.

»visit the vladstudio store for more designs and products like this
Click to customize with size, paper type etc.
via Zazzle Astronomy market place

New approach to chip design could yield light speed computing

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Researchers are the first to create a device that integrates both optical and electronic signals to perform the most elementary computational operations that could inform 'light speed' computing.

via Science Daily

Technique to create holes in graphene could improve water filters, desalination

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A new technique produces highly selective filter materials that could lead to more efficient desalination. Scientists succeeded in creating subnanoscale pores in a sheet of the one-atom-thick material, which is one of the strongest materials known.

via Science Daily

Graphene's bonding effect on platinum nanoparticles characterized: Lower costs in fuel cell production?

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Physicists have found that platinum nanoparticles limit their size and organize into specific patterns when bonded to freestanding graphene. While displaying this behavior, the bonded platinum nanoparticles maintain an effective surface area functioning as a catalyst for chemical reactions, a discovery that could lower the production costs of platinum-catalyzed fuel cells.

via Science Daily

Microanalysis technique makes the most of small nanoparticle samples

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Sensitive chemical analyses of minute samples of nanoparticles can be done by, essentially, roasting them on top of a quartz crystal, new research demonstrates. Chemical analysis of nanoparticles is a challenging task, and not just because they're small. They're also complicated. The technique, 'microscale thermogravimetric analysis,' holds promise for studying nanomaterials in biology and the environment, where sample sizes often are quite small and larger-scale analysis won't work.

via Science Daily

Tuesday 25 February 2014

Bullying black holes force galaxies to stay red and dead

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Astronomers have discovered massive elliptical galaxies in the nearby Universe containing plenty of cold gas, even though the galaxies fail to produce new stars. Comparison with other data suggests that, while hot gas cools down in these galaxies, stars do not form because jets from the central supermassive black hole heat or stir up the gas and prevent it from turning into stars. Giant elliptical galaxies are the most puzzling type of galaxy in the Universe.

via Science Daily

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Water detected in a planet outside our solar system

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Water has been detected in the atmosphere of a planet outside our solar system with a new technique that could help researchers to learn how many planets with water, like Earth, exist throughout the universe. The team of scientists that made the discovery detected the water in the atmosphere of a planet as massive as Jupiter that is orbiting the nearby star tau Boötis.

via Science Daily

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Rare form of nitrogen detected in comet ISON

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Astronomers observed the Comet ISON during its bright outburst in the middle of November 2013. Subaru Telescope's High Dispersion Spectrograph has detected two rare forms of nitrogen in the comet ISON. Their results support the hypothesis that there were two distinct reservoirs of nitrogen the massive, dense cloud ("solar nebula") from which our Solar System may have formed and evolved.

via Science Daily

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How to create selective holes in graphene

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Researchers have devised a way of making tiny holes of controllable size in sheets of graphene, a development that could lead to ultrathin filters for improved desalination or water purification.



The team of researchers at MIT, Oak Ridge National Laboratory, and in Saudi Arabia succeeded in creating subnanoscale pores in a sheet of the one-atom-thick material, which is one of the strongest materials known. Their findings are published in the journal Nano Letters.



The concept of using graphene, perforated by nanoscale pores, as a filter in desalination has been proposed and analyzed by other MIT researchers. The new work, led by graduate student Sean O’Hern and associate professor of mechanical engineering Rohit Karnik, is the first step toward actual production of such a graphene filter.



Making these minuscule holes in graphene — a hexagonal array of carbon atoms, like atomic-scale chicken wire — occurs in a two-stage process. First, the graphene is bombarded with gallium ions, which disrupt the carbon bonds. Then, the graphene is etched with an oxidizing solution that reacts strongly with the disrupted bonds — producing a hole at each spot where the gallium ions struck. By controlling how long the graphene sheet is left in the oxidizing solution, the MIT researchers can control the average size of the pores.



A big limitation in existing nanofiltration and reverse-osmosis desalination plants, which use filters to separate salt from seawater, is their low permeability: Water flows very slowly through them. The graphene filters, being much thinner, yet very strong, can sustain a much higher flow. “We’ve developed the first membrane that consists of a high density of subnanometer-scale pores in an atomically thin, single sheet of graphene,” O’Hern says.



For efficient desalination, a membrane must demonstrate “a high rejection rate of salt, yet a high flow rate of water,” he adds. One way of doing that is decreasing the membrane’s thickness, but this quickly renders conventional polymer-based membranes too weak to sustain the water pressure, or too ineffective at rejecting salt, he explains.



With graphene membranes, it becomes simply a matter of controlling the size of the pores, making them “larger than water molecules, but smaller than everything else,” O’Hern says — whether salt, impurities, or particular kinds of biochemical molecules.



The permeability of such graphene filters, according to computer simulations, could be 50 times greater than that of conventional membranes, as demonstrated earlier by a team of MIT researchers led by graduate student David Cohen-Tanugi of the Department of Materials Science and Engineering. But producing such filters with controlled pore sizes has remained a challenge. The new work, O’Hern says, demonstrates a method for actually producing such material with dense concentrations of nanometer-scale holes over large areas.



“We bombard the graphene with gallium ions at high energy,” O’Hern says. “That creates defects in the graphene structure, and these defects are more chemically reactive.” When the material is bathed in a reactive oxidant solution, the oxidant “preferentially attacks the defects,” and etches away many holes of roughly similar size. O’Hern and his co-authors were able to produce a membrane with 5 trillion pores per square centimeter, well suited to use for filtration. “To better understand how small and dense these graphene pores are, if our graphene membrane were to be magnified about a million times, the pores would be less than 1 millimeter in size, spaced about 4 millimeters apart, and span over 38 square miles, an area roughly half the size of Boston,” O’Hern says.



With this technique, the researchers were able to control the filtration properties of a single, centimeter-sized sheet of graphene: Without etching, no salt flowed through the defects formed by gallium ions. With just a little etching, the membranes started allowing positive salt ions to flow through. With further etching, the membranes allowed both positive and negative salt ions to flow through, but blocked the flow of larger organic molecules. With even more etching, the pores were large enough to allow everything to go through.



Scaling up the process to produce useful sheets of the permeable graphene, while maintaining control over the pore sizes, will require further research, O’Hern says.



Karnik says that such membranes, depending on their pore size, could find various applications. Desalination and nanofiltration may be the most demanding, since the membranes required for these plants would be very large. But for other purposes, such as selective filtration of molecules — for example, removal of unreacted reagents from DNA — even the very small filters produced so far might be useful.



“For biofiltration, size or cost are not as critical,” Karnik says. “For those applications, the current scale is suitable.”



Bruce Hinds, a professor of materials engineering at the University of Kentucky who was not involved in this work, says, “Previous groups had tried just ion bombardment or plasma radical formation.” The idea of combining these methods “is nice and has the potential to be fine-tuned.” While more work needs to be done to refine the technique, he says, this approach is “promising” and could ultimately help to lead to applications in “water purification, energy storage, energy production, [and] pharmaceutical production.”



The work also included Jing Kong, the ITT Career Development Associate Professor of Electrical Engineering; MIT graduate students Michael Boutilier and Yi Song; researcher Juan-Carlos Idrobo of the Oak Ridge National Laboratory; and professors Tahar Laoui and Muataz Atieh of the King Fahd University of Petroleum and Minerals (KFUPM). The project received support from the Center for Clean Water and Clean Energy at MIT and KFUPM and the U.S. Department of Energy.



via MIT News

Crab Nebula Astronomy and Science Poster

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

after scouring the Zazzle market place for a while, I settled on this as my choice for today. By walgenn, another talented creative from the Zazzle community!


tagged with: astronomy, astronomer, scientist, science, space, gift, space gift, astronomy gift, science gift, nebula, star, universe, hubble, hubble space telescope, nasa, astrophysicist, astrophysics, super nova, space exploration, big bang, birthday gift, graduation gift, unique gift idea, poster, print, astronomy poster, space poster, hubble poster, nebula poster, crab nebula, supernova

Crab Nebula a supernova explosion remnant - this striking image by the Hubble Space Telescope, is a unique gift idea for the space science, astronmer and astrophysics enthusiast on you Holiday gift list or a special gift for any occasion.

»visit the walgenn store for more designs and products like this
Click to customize with size, paper type etc.
via Zazzle Astronomy market place

The Pleiades Deep and Dusty

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The well known Pleiades star cluster is slowly destroying part of a passing cloud of gas and dust. The Pleiades is the brightest open cluster of stars on Earth's sky and can be seen from almost any northerly location with the unaided eye. The passing young dust cloud is thought to be part of Gould's belt, an unusual ring of young star formation surrounding the Sun in the local Milky Way Galaxy. Over the past 100,000 years, part Gould's belt is by chance moving right through the older Pleiades and is causing a strong reaction between stars and dust. Pressure from the star's light significantly repels the dust in the surrounding blue reflection nebula, with smaller dust particles being repelled more strongly. A short-term result is that parts of the dust cloud have become filamentary and stratified, as seen in the above deep-exposure image.
Tomorrow's picture: down over
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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)
NASA Official: Phillip Newman Specific rights apply.
NASA Web Privacy Policy and Important Notices
A service of: ASD at NASA / GSFC
& Michigan Tech. U.



Zazzle Space Gifts for young and old

CVD graphene suitable for transistors and surface chemistry studies

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With exceptional carrier mobilities, mechanical strength, and optical transparency, graphene is a leading material for next-generation electronic devices. However, for most applications, graphene will need to be integrated with other materials, which motivates efforts to understand and tune its surface chemistry. In recent work, published in the scientific journal Small, scientists from the University of Groningen in the Netherlands studied surface chemistry and self assembly of organic molecular wires on Graphenea's CVD graphene.


Since all atoms in graphene are surface atoms, a natural approach to tune graphene’s electronic properties is to use surface interactions. In particular, the modification of graphene via functionalization with organic molecules holds promise for tuning the electronic properties of graphene, controlling interfaces with other materials, and tailoring surface chemical reactivity.


Recently, a number of studies on self-assembly of organic molecules on graphene have been reported, albeit with few reports combining both the surface organization and its effect on the electrical performance of graphene devices. The scarcity of combined studies is likely to be due to the specific limitations presented by each source of graphene used. For example, mechanically exfoliated flakes of graphene on an insulating substrate, such as the commonly used silicon dioxide, allow fabrication of electronic devices, but are very challenging to approach with the tip of a scanning tunneling microscope (STM) due to their small dimensions. On the other hand, large-area graphene grown epitaxially from silicon carbide or grown by chemical vapor deposition (CVD) on a metal is suitable for studying self-assembly, but is not readily used in field-effect transistors due to the lack of a back gate electrode in the substrate.


In contrast, graphene grown by CVD and subsequently transferred to silicon/silicon dioxide wafers combines the accessibility of large-area graphene with the utility of a back gate present in the substrate. Furthermore, waferscale CVD graphene transferred to silicon/silicon dioxide has become widely available. In the work detailed in the Small publication, the team led by Prof. Ben L. Feringa used our commercially available CVD graphene on silicon/silicon dioxide. High quality CVD graphene on this substrate is available from Graphenea on wafer sizes ranging from 10mm x 10mm to a full 4'' diameter wafer, or on any other custom-sized wafer or substrate material.



Figure: Molecular wires grown on a graphene layer, imaged by scanning tunneling microscopy (from Small, a Wiley publication)


The research team discovered several surprising features of molecular wire self-assembly on graphene. Notably, it is found that the wires grow in patches oriented at 60 degrees to each other (see figure, part b), indicating the the atomic structure of graphene (a honeycomb lattice with 60 degree symmetry) plays a role in the self-assembly process, reflecting on the macroscopic topology of the wires. A second surprising finding is that the performance (doping level and mobility) of graphene transistors becomes better when they are covered by the layer of organic molecular wires. The performance increase is attributed mostly to cleaning of the graphene by the solvents used in the chemistry process.


In conclusion, this top-ranking publication confirms the importance of surface properties of graphene, studying the important interaction of the graphene surface with organic molecules. Importantly, the results show that CVD graphene is compatible with graphene transistor technology, touting a quality high enough to investigate surface chemistry effects. Combined with the ability to grow wafer-scale layers, CVD graphene is so far the most serious contender for fast graphene electronics and precise sensors.




via Graphenea

How to create selective holes in graphene

more »

Researchers have devised a way of making tiny holes of controllable size in sheets of graphene, a development that could lead to ultrathin filters for improved desalination or water purification.



The team of researchers at MIT, Oak Ridge National Laboratory, and in Saudi Arabia succeeded in creating subnanoscale pores in a sheet of the one-atom-thick material, which is one of the strongest materials known. Their findings are published in the journal Nano Letters.



The concept of using graphene, perforated by nanoscale pores, as a filter in desalination has been proposed and analyzed by other MIT researchers. The new work, led by graduate student Sean O’Hern and associate professor of mechanical engineering Rohit Karnik, is the first step toward actual production of such a graphene filter.



Making these minuscule holes in graphene — a hexagonal array of carbon atoms, like atomic-scale chicken wire — occurs in a two-stage process. First, the graphene is bombarded with gallium ions, which disrupt the carbon bonds. Then, the graphene is etched with an oxidizing solution that reacts strongly with the disrupted bonds — producing a hole at each spot where the gallium ions struck. By controlling how long the graphene sheet is left in the oxidizing solution, the MIT researchers can control the average size of the pores.



A big limitation in existing nanofiltration and reverse-osmosis desalination plants, which use filters to separate salt from seawater, is their low permeability: Water flows very slowly through them. The graphene filters, being much thinner, yet very strong, can sustain a much higher flow. “We’ve developed the first membrane that consists of a high density of subnanometer-scale pores in an atomically thin, single sheet of graphene,” O’Hern says.



For efficient desalination, a membrane must demonstrate “a high rejection rate of salt, yet a high flow rate of water,” he adds. One way of doing that is decreasing the membrane’s thickness, but this quickly renders conventional polymer-based membranes too weak to sustain the water pressure, or too ineffective at rejecting salt, he explains.



With graphene membranes, it becomes simply a matter of controlling the size of the pores, making them “larger than water molecules, but smaller than everything else,” O’Hern says — whether salt, impurities, or particular kinds of biochemical molecules.



The permeability of such graphene filters, according to computer simulations, could be 50 times greater than that of conventional membranes, as demonstrated earlier by a team of MIT researchers led by graduate student David Cohen-Tanugi of the Department of Materials Science and Engineering. But producing such filters with controlled pore sizes has remained a challenge. The new work, O’Hern says, demonstrates a method for actually producing such material with dense concentrations of nanometer-scale holes over large areas.



“We bombard the graphene with gallium ions at high energy,” O’Hern says. “That creates defects in the graphene structure, and these defects are more chemically reactive.” When the material is bathed in a reactive oxidant solution, the oxidant “preferentially attacks the defects,” and etches away many holes of roughly similar size. O’Hern and his co-authors were able to produce a membrane with 5 trillion pores per square centimeter, well suited to use for filtration. “To better understand how small and dense these graphene pores are, if our graphene membrane were to be magnified about a million times, the pores would be less than 1 millimeter in size, spaced about 4 millimeters apart, and span over 38 square miles, an area roughly half the size of Boston,” O’Hern says.



With this technique, the researchers were able to control the filtration properties of a single, centimeter-sized sheet of graphene: Without etching, no salt flowed through the defects formed by gallium ions. With just a little etching, the membranes started allowing positive salt ions to flow through. With further etching, the membranes allowed both positive and negative salt ions to flow through, but blocked the flow of larger organic molecules. With even more etching, the pores were large enough to allow everything to go through.



Scaling up the process to produce useful sheets of the permeable graphene, while maintaining control over the pore sizes, will require further research, O’Hern says.



Karnik says that such membranes, depending on their pore size, could find various applications. Desalination and nanofiltration may be the most demanding, since the membranes required for these plants would be very large. But for other purposes, such as selective filtration of molecules — for example, removal of unreacted reagents from DNA — even the very small filters produced so far might be useful.



“For biofiltration, size or cost are not as critical,” Karnik says. “For those applications, the current scale is suitable.”



Bruce Hinds, a professor of materials engineering at the University of Kentucky who was not involved in this work, says, “Previous groups had tried just ion bombardment or plasma radical formation.” The idea of combining these methods “is nice and has the potential to be fine-tuned.” While more work needs to be done to refine the technique, he says, this approach is “promising” and could ultimately help to lead to applications in “water purification, energy storage, energy production, [and] pharmaceutical production.”



The work also included Jing Kong, the ITT Career Development Associate Professor of Electrical Engineering; MIT graduate students Michael Boutilier and Yi Song; researcher Juan-Carlos Idrobo of the Oak Ridge National Laboratory; and professors Tahar Laoui and Muataz Atieh of the King Fahd University of Petroleum and Minerals (KFUPM). The project received support from the Center for Clean Water and Clean Energy at MIT and KFUPM and the U.S. Department of Energy.



via MIT News

Astronomers spot record-breaking lunar impact

more »

A meteorite with the mass of a small car crashed into the Moon last September, according to Spanish astronomers. The impact, the biggest seen to date, produced a bright flash and would have been easy to spot from Earth.

via Science Daily

Zazzle Space Exploration market place

Hubble's Ultra Deep Field Image Poster

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

so many products with fantastic designs on Zazzle... which to choose today? How about this one from HubbleView, another talented creative from the Zazzle community!


tagged with: hubble, ultra deep field, ultra, deep, field, astronomical, astronomy, distant, galaxies, ancient, red shift, space images

This view of nearly 10,000 galaxies is called the Hubble Ultra Deep Field. The snapshot includes galaxies of various ages, sizes, shapes, and colors. The smallest, reddest galaxies may be among the most distant known, existing when the universe was just about 800 million years old. The nearest galaxies - the larger, brighter, well-defined spirals and ellipticals - thrived about 1 billion years ago, when the cosmos was 13 billion years old. The image required 800 exposures taken over the course of 400 Hubble orbits around Earth. The total amount of exposure time was 11.3 days, taken between Sept. 24, 2003 and Jan. 16, 2004. Credit: NASA, ESA, and S. Beckwith (STScI) and the HUDF Team For more information, visit http://hubblesite.org/newscenter/archive/releases/2006/12/image/b/

»visit the HubbleView store for more designs and products like this
Click to customize with size, paper type etc.
via Zazzle Astronomy market place

Monday 24 February 2014

Rose Galaxy iPad Mini Cases

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!

wow! This one caught my eye, I hope you like it. By A_Peace_of_Joy,
another talented creative from the Zazzle community!


tagged with: rose, galaxy, rose galaxy, hubble, space, telescope, hubble space telescope

Depicting the Rose Galaxy, courtesy of NASA's Hubble Space Telescope.

»visit the A_Peace_of_Joy store for more designs and products like this
The Zazzle Promise: We promise 100% satisfaction. If you don't absolutely love it, we'll take it back!

Pale Blue Dot Print

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

could this be the design you've been looking for? It features the creativeness of ThatGuy042, another talented creative from the Zazzle community!


tagged with: pale blue dot, carl sagan, earth, astronomy, cosmology, voyager 1

The world famous photograph of earth taken 3.7 billion miles away from home as Voyager 1 exited the solar system with Carl Sagan's beautiful words overlaid beneath it.

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140224

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Zazzle Space Gifts for young and old

Rosetta’s selfie

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Space science image of the week: As Rosetta flew by Mars 7 years ago, its lander, Philae, took this incredible self-portrait

via ESA Space Science

http://bit.ly/1fgHkjk

Space Walk 1 Poster

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

so many products with fantastic designs on Zazzle... which to choose today? How about this one from kcoop, another talented creative from the Zazzle community!


tagged with: space, walk, earth, station, astronaut, skylab, astronomy

Space Walk 1

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The Hubble showdown: Starbursts versus monsters

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The dominating figure in the middle of this new Hubble image is a galaxy known as MCG-03-04-014. It belongs to a class of galaxies called luminous infrared galaxies -- galaxies that are incredibly bright in the infrared part of the spectrum.

via Science Daily

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Sunday 23 February 2014

Earth at Night Posters

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

after scouring the Zazzle market place for a while, I settled on this as my choice for today. By kcoop, another talented creative from the Zazzle community!


tagged with: earth, night, astronomy, space

Earth at Night

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Stellar Nurseries RCW120 Rectangle Sticker

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


tagged with: envelope sealers, nebulae, gstlnrsr, rcw120, breathtaking astronomy images, star nurseries, ionised gas clouds, star forming regions, european southern observatory, clusters of stars, galaxies, starfields, eso, vista

Galaxies, Stars and Nebulae series

A fantastic set of stickers, with a monogram for you to change, featuring a colour composite image of RCW120.

It reveals how an expanding bubble of ionised gas about ten light-years across is causing the surrounding material to collapse into dense clumps where new stars are then formed.

The 870-micron submillimetre-wavelength data were taken with the LABOCA camera on the 12-m Atacama Pathfinder Experiment (APEX) telescope. Here, the submillimetre emission is shown as the blue clouds surrounding the reddish glow of the ionised gas (shown with data from the SuperCosmos H-alpha survey). The image also contains data from the Second Generation Digitized Sky Survey (I-band shown in blue, R-band shown in red).

All items with this image
All items in the Galaxies, Stars and Nebulae series

Image code: gstlnrsr

ESO/J. Emerson/VISTA www.eso.org
Reproduced under the Creative Commons Attribution 3.0 Unported license.

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Cassini Spacecraft Crosses Saturn's Ring Plane

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If this is Saturn, where are the rings? When Saturn's "appendages" disappeared in 1612, Galileo did not understand why. Later that century, it became understood that Saturn's unusual protrusions were rings and that when the Earth crosses the ring plane, the edge-on rings will appear to disappear. This is because Saturn's rings are confined to a plane many times thinner, in proportion, than a razor blade. In modern times, the robot Cassini spacecraft orbiting Saturn now also crosses Saturn's ring plane. A series of plane crossing images from 2005 February was dug out of the vast online Cassini raw image archive by interested Spanish amateur Fernando Garcia Navarro. Pictured above, digitally cropped and set in representative colors, is the striking result. Saturn's thin ring plane appears in blue, bands and clouds in Saturn's upper atmosphere appear in gold. Details of Saturn's rings can be seen in the high dark shadows across the top of this image, taken back in 2005. Moons appear as bumps in the rings.
Tomorrow's picture: open space
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Zazzle Space Gifts for young and old

Beautiful Heart of The Milky Way Galaxy Poster

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

so many products with fantastic designs on Zazzle... which to choose today? How about this one from Galactica, another talented creative from the Zazzle community!


tagged with: nasa, galaxies, galaxy, space, prints, posters, poster, print, milky way, stars, nebula, fantasy, science fiction

A never-before-seen view of the turbulent heart of our Milky Way galaxy is being unveiled by NASA on Nov. 10. This event will commemorate the 400 years since Galileo first turned his telescope to the heavens in 1609. In celebration of this International Year of Astronomy, NASA is releasing images of the galactic center region as seen by its Great Observatories to more than 150 planetariums, museums, nature centers, libraries, and schools across the country. The sites will unveil a giant, 6-foot-by-3-foot print of the bustling hub of our galaxy that combines a near-infrared view from the Hubble Space Telescope, an infrared view from the Spitzer Space Telescope, and an X-ray view from the Chandra X-ray Observatory into one multiwavelength picture. Experts from all three observatories carefully assembled the final image from large mosaic photo surveys taken by each telescope. This composite image provides one of the most detailed views ever of our galaxy's mysterious core. Participating institutions also will display a matched trio of Hubble, Spitzer, and Chandra images of the Milky Way's center on a second large panel measuring 3 feet by 4 feet. Each image shows the telescope's different wavelength view of the galactic center region, illustrating not only the unique science each observatory conducts, but also how far astronomy has come since Galileo. The composite image features the spectacle of stellar evolution: from vibrant regions of star birth, to young hot stars, to old cool stars, to seething remnants of stellar death called black holes. This activity occurs against a fiery backdrop in the crowded, hostile environment of the galaxy's core, the center of which is dominated by a supermassive black hole nearly four million times more massive than our Sun. Permeating the region is a diffuse blue haze of X-ray light from gas that has been heated to millions of degrees by outflows from the supermassive black hole as well as by winds from massive stars and by stellar explosions. Infrared light reveals more than a hundred thousand stars along with glowing dust clouds that create complex structures including compact globules, long filaments, and finger-like "pillars of creation," where newborn stars are just beginning to break out of their dark, dusty cocoons.Courtesy: NASA.

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Saturday 22 February 2014

Smart SPHERES are about to get a whole lot smarter

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Smart devices -- such as tablets and phones -- increasingly are an essential part of everyday life on Earth. The same can be said for life off-planet aboard the International Space Station. Our reliance on these mobile and social technologies means equipment and software upgrades are an everyday occurrence -- like buying a new pair of shoes to replace a pair of well-worn ones. That's why the Intelligent Robotics Group at NASA's Ames Research Center in Moffett Field, Calif. is working to upgrade the smartphones currently equipped on a trio of volleyball-sized free-flying satellites on the space station called Synchronized Position Hold, Engage, Reorient, Experimental Satellites (SPHERES).

via Science Daily

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Orion testing provides lessons and data for splashdown recovery operations

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The first full joint testing between NASA and the U.S. Navy of Orion recovery procedures off the coast of California was suspended after the team experienced issues with handling lines securing a test version of Orion inside the well deck of the USS San Diego.

via Science Daily

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NASA's IRIS spots its largest solar flare

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On Jan. 28, 2014, NASA's Interface Region Imaging Spectrograph, or IRIS, witnessed its strongest solar flare since it launched in the summer of 2013. Solar flares are bursts of x-rays and light that stream out into space, but scientists don't yet know the fine details of what sets them off.

via Science Daily

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Curiosity Mars rover adds reverse driving for wheel protection

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Terrain that NASA's Curiosity Mars rover is now crossing is as smooth as team members had anticipated based on earlier images from orbit. On Tuesday, Feb. 18, the rover covered 329 feet (100.3 meters), the mission's first long trek that used reverse driving and its farthest one-day advance of any kind in more than three months.

via Science Daily

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NASA Mars Orbiter views Opportunity Rover on ridge

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A new image from a telescopic camera orbiting Mars shows NASA's Mars Exploration Rover Opportunity at work on "Murray Ridge," without any new impact craters nearby.

via Science Daily

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Shocking behavior of a runaway star: High-speed encounter creates arc

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Roguish runaway stars can have a big impact on their surroundings as they plunge through the Milky Way galaxy. Their high-speed encounters shock the galaxy, creating arcs, as seen in a newly released image from NASA's Spitzer Space Telescope.

via Science Daily

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Jupiter will be at its highest point in the sky for many years to come

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In just over a week, Jupiter, the largest planet in the solar system, will be at its highest point in the sky for many years to come. Near their closest to Earth, Jupiter and its moons will appear obvious in the sky, offering fantastic opportunities to view the giant planet through a telescope.

via Science Daily

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Chaotic Sun Poster

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

could this be the design you've been looking for? It features the creativeness of yarddawg, another talented creative from the Zazzle community!


tagged with: sun, solar, star, space, science, astronomy, geek, nerd, solar system

The boiling chaos that is our sun, developed from SOHO imagery. Makes a nice addition to a collection of solar system posters.

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M44: The Beehive Cluster

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A mere 600 light-years away, M44 is one of the closest star clusters to our solar system. Also known as the Praesepe or the Beehive cluster its stars are young though, about 600 million years old compared to our Sun's 4.5 billion years. Based on similar ages and motion through space, M44 and the even closer Hyades star cluster in Taurus are thought to have been born together in the same large molecular cloud. An open cluster spanning some 15 light-years, M44 holds 1,000 stars or so and covers about 3 full moons (1.5 degrees) on the sky in the constellation Cancer. Visible to the unaided eye, M44 has been recognized since antiquity. Described as a faint cloud or celestial mist long before being included as the 44th entry in Charles Messier's 18th century catalog, the cluster was not resolved into its individual stars until telescopes were available. A popular target for modern, binocular-equiped sky gazers, the cluster's few yellowish tinted, cool, red giants are scattered through the field of its brighter hot blue main sequence stars in this colorful stellar group snapshot.

Zazzle Space Gifts for young and old

Vintage Astronomy Celestial Renaissance Moon Stars Poster

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

so many products with fantastic designs on Zazzle... which to choose today? How about this one from YesterdayCafe, another talented creative from the Zazzle community!


tagged with: landscape, antique, constellations, stars, retro, moon, americana, nostalgic, celestial, vintage illustration

Vintage illustration astronomy and celestial black and white Renaissance drawing of a landscape and the moon (lune) in the night sky with stars and constellations. People are standing next to a river, bridge and buildings. Created in 1683 by Allain Manesson Mallet (1630 – 1706), a French cartographer and engineer.

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Friday 21 February 2014

Planet-sized space weather explosions at Venus

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Researchers recently discovered that a common space weather phenomenon on the outskirts of Earth's magnetic bubble, the magnetosphere, has much larger repercussions for Venus. The giant explosions, called hot flow anomalies, can be so large at Venus that they're bigger than the entire planet and they can happen multiple times a day.

via Science Daily

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