Tuesday 2 June 2015

An inexpensive rival to graphene aerogels

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A team of researchers set out to design a cheaper material with properties similar to a graphene aerogel--in terms of its conductivity, as well as a lightweight, anticorrosive, porous structure. The researchers have describe the new material they created and its performance.
via Science Daily

Alice instrument's ultraviolet close-up provides a surprising discovery about comet's atmosphere

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A close-up of Comet 67P/Churyumov-Gerasimenko by NASA's ultraviolet instrument surprised scientists by revealing that electrons close to the comet's surface -- not photons from the sun as had been believed -- cause the rapid breakup of water and carbon dioxide molecules spewing from the surface.
via Science Daily
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Improving the delivery of chemotherapy with graphene

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A new study has proposed using graphene as an alternative coating for catheters to improve the delivery of chemotherapy drugs.
via Science Daily

Major advance in mastering the extraordinary properties of an emerging semiconductor

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A team of researchers is the first to succeed in preventing two-dimensional layers of black phosphorus from oxidating. In so doing, they have opened the doors to exploiting their striking properties in a number of electronic and optoelectronic devices.
via Science Daily

Researchers use stars to infer mass of Milky Way

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What if your doctor told you that your weight is somewhere between 100 and 400 lbs.? With any ordinary scale every patient can do better at home. Yet, one patient can't: the Milky Way. Even though today we peer deeper into space than ever before, our home galaxy's weight is still unknown to about a factor of four. Researchers at Columbia University's Astronomy Department have now developed a new method to give the Milky Way a more precise physical checkup.

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Earth organisms survive under low-pressure Martian conditions

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Methanogens – among the simplest and oldest organisms on Earth – could survive on Mars, new research suggests. Methanogens, microorganisms in the domain Archaea, use hydrogen as their energy source and carbon dioxide as their carbon source, to metabolize and produce methane, also known as natural gas. Methanogens live in swamps and marshes, but can also be found in the gut of cattle, termites and other herbivores as well as in dead and decaying matter.
via Science Daily
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Quantum dot light emitting diodes meet wearable devices

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An ultra-thin wearable quantum dot light emitting diodes (QLEDs) has been developed by scientists. The electronic tattoo is based on current quantum dot light emitting diode (QLED) technology. Colloidal quantum dot (QLED’s) have attracted great attention as next generation displays. The quantum dots (QDs) have unique properties such as the color tunability, photo/air stability, and are printability on various substrates. The device is paper thin and can be applied to human skin like a sticker.
via Science Daily

New heterogeneous wavelength tunable laser diode for high-frequency efficiency

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A novel ultra-compact heterogeneous wavelength tunable laser diode has been developed by scientists. The heterogeneous laser diode was realized through a combination of silicon photonics and quantum-dot technology, and demonstrates a wide-range tuning-operation.
via Science Daily

Custom Name, Deep Space Phenomena Cigar Galaxy Wrapping Paper

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tagged with: agmet, chandra, messier 82, cigar galaxy, active galaxies, outer space images, deep space photography, hubble astronomy, sky watching, outer space star telescope images

Galaxies, Stars and Nebulae series Composite of images of the active galaxy Messier 82 from the three Great Observatories: Hubble Space Telescope, Chandra X-Ray Observatory, and Spitzer Space Telescope. X-ray data recorded by Chandra appears here in blue, infrared light recorded by Spitzer appears in red. Hubble's observation of hydrogen emission appears in orange. Hubble's bluest observation appears in yellow-green.
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image code: agmet

Image credit: Hubble Space Telescope, Chandra X-Ray Observatory, Spitzer Space Telescope

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Monogram - Sculpted Region of the Orion Nebula Classic Round Sticker

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


tagged with: peel off, envelope sealers, galaxies and stars, orion nebula detail, sculpted gas clouds, sgcion, stellar winds, sculpting trapezium stars, messier 42, messier 43

Galaxies, Stars and Nebulae series A region within the Orion Nebula showing the sculpting effect that stars can have on any surrounding gas clouds. This glowing region reveals arcs and bubbles formed when stellar winds - streams of charged particles ejected by the nearby Trapezium stars - collide with material.

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image code: sgcion

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

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LHC Season 2: First physics at 13 TeV to start tomorrow

In the early morning of Wednesday 3 June, the Large Hadron Collider (LHC) at CERN is set to start delivering physics data to its experiments for the first time in 27 months.

After nearly two years of maintenance and repair, as well as several months of re-commissioning, the experiments at the world's largest particle accelerator are now ready to take data at the unprecedented energy of 13 teraelectronvolts (TeV) – almost double the collision energy of the LHC's first, three-year run. Data taking will mark the start of season 2 at the LHC, opening the way to new frontiers in physics.


For all the day's action, follow our Live Blog "LHC Season 2: New frontiers in physics" where we'll be posting all the latest from the CERN Control Centre, starting at 7am CEST.


The blog will guide you through key moments in the day, from injecting the counter-rotating beams of protons into the LHC and ramping their energy to 6.5 TeV each, to eventual particle collisions and the start of data taking at 13 TeV. A live webcast will also be available through the live blog.

For more about the big questions that the LHC experiments are tackling, check out “New frontiers in physics” and follow the scientists at the forefront of particle physics.

For more about the LHC and its second run, check out "LHC Season 2: Facts & figures" and "LHC Season 2: A stronger machine"


via CERN: Updates for the general public
http://home.web.cern.ch/about/updates/2015/06/lhc-season-2-first-physics-13-tev-start-tomorrow

Polaris and Comet Lovejoy

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Zazzle Space Gifts for young and old

Ultraviolet study reveals surprises in comet coma

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Rosetta’s continued close study of Comet 67P/Churyumov–Gerasimenko has revealed an unexpected process at work, causing the rapid breakup of water and carbon dioxide molecules spewing from the comet’s surface.


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

Research pair find a way to measure electrical conductance at sites on individual atoms

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(Phys.org)—A pair of researchers with the University of Tokyo has found a way to improve on scanning tunneling microscope (STM) technology where it is now possible to measure electrical conductance at individual sites on and between individual atoms. In their paper published in Physical Review Letters, Howon Kim and Yukio Hasegawa describe the changes they made and what they found using the newly improved device.

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New electronics? Black Phosphorus Reveals Its Secrets

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Scientists have succeeded in preventing two-dimensional layers of black phosphorus from oxidating. In so doing, they have opened the doors to exploiting their striking properties in a number of electronic and optoelectronic devices.
via Science Daily

Purple Galaxy Cluster Powis iPad Air 2 Case

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!


tagged with: blue, purple, nasa, hubble, space, images, stars, pretty, galaxies, galaxy cluster macs j0717

Galaxy Cluster MACS J0717 thanks to NASA and Hubble program.

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LHC Season 2: CERN computing ready for data torrent

The CERN Data Centre

This week, the experiments at the Large Hadron Collider (LHC) will start taking data at the new energy frontier of 13 teraelectonvolts (TeV) - nearly double the energy of collisions in the LHC's first three-year run. These collisions, which will occur up to 1 billion times every second, will send showers of particles through the detectors.

With every second of run-time, gigabytes of data will come pouring into the CERN Data Centre to be stored, sorted and shared with physicists worldwide. To cope with this massive influx of Run 2 data, the CERN computing teams focused on three areas: speed, capacity and reliability.

"During Run 1, we were storing 1 gigabyte-per-second, with the occasional peak of 6 gigabytes-per-second," says Alberto Pace, who leads the Data and Storage Services group within the IT Department. "For Run 2, what was once our "peak" will now be considered average, and we believe we could even go up to 10 gigabytes-per-second if needed."

At CERN, most of the data is archived on magnetic tape using the CERN Advanced Storage system (CASTOR) and the rest is stored on the EOS disk pool system – a system optimized for fast analysis access by many concurrent users. Magnetic tapes may be seen as an old-fashioned technology. They are actually a robust storage material, able to store huge volumes of data and thus ideal for long-term preservation. The computing teams have improved the software of the tape storage system CASTOR, allowing CERN's tape drives and libraries to be used more efficiently, with no lag times or delays. This allows the Data Centre to increase the rate of data that can be moved to tape and read back.

Reducing the risk of data loss - and the massive storage burden associated with this - was another challenge to address for Run 2. The computing teams introduced a data 'chunking' option in the EOS storage disk system. This splits the data into segments and enables recently acquired data to be kept on disk for quick access. "This allowed our online total data capacity to be increased significantly," Pace continues. "We have 140 petabytes of raw disk space available for Run 2 data, divided between the CERN Data Centre and the Wigner Data Centre in Budapest, Hungary. This translates to about 60 petabytes of storage, including back-up files."

140 petabytes (which is equal to 140 million gigabytes) is a very large number indeed - equivalent to over a millenium of full HD-quality movies.

Now, in addition to the regular "replication" approach - whereby a duplicated copy is kept for all data - experiments will now have an option to scatter the data across multiple disks. This "chunking" approach breaks the data into pieces. Use of reconstruction algorithms means that content will not be lost even if multiple disks fail. This not only decreases the probability of data loss, but also cuts in half the space needed for back-up storage. Finally, the EOS system has also been further improved to achieve the goal of more than 99.5% availability for the duration of Run 2.

From quicker storage speeds to new storage solutions, CERN is well-prepared for all of the fantastic challenges of Run 2.

 

 


via CERN: Updates for the general public
http://home.web.cern.ch/about/updates/2015/06/lhc-season-2-cern-computing-ready-data-torrent

The Acid Test

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Earth’s air pollution and climate change issues are linked to combustion and its detrimental byproducts: greenhouse gases such

The post The Acid Test has been published on Technology Org.

 
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Microgravity experiments may help lighten the load of joint diseases

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Going into space might wreak havoc on our bodies, but a new set of microgravity experiments may help shed light on new approaches for treating cartilage diseases on Earth. A team of scientists suggests that our cartilage--tissue that serves as a cushion between bones--might be able to survive microgravity relatively unscathed.
via Science Daily
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Name, Flame Nebula in Orion, intriguing deep space Wrapping Paper

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tagged with: star forming, orion constellation, young stars clusters, orions belt, orion the hunter, flame nebula, astronomy pictures, deep space image, star galaxies, hrbstslr hfflmnb, heavens, european southern observatory, eso, vista

Galaxies, Stars and Nebulae series A gorgeous outer space picture featuring the spectacular star-forming region known as the Flame Nebula, or NGC 2024, in the constellation of Orion (the Hunter) and its surroundings.
In views of this evocative object in visible light the core of the nebula is completely hidden behind obscuring dust, but in this VISTA view, taken in infrared light, the cluster of very young stars at the object’s heart is revealed. The wide-field VISTA view also includes the glow of the reflection nebula NGC 2023, just below centre, and the ghostly outline of the Horsehead Nebula (Barnard 33) towards the lower right.
The bright bluish star towards the right is one of the three bright stars forming the Belt of Orion. The image was created from VISTA images taken through J, H and Ks filters in the near-infrared part of the spectrum.
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image code: hfflmnb

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

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Monogram, Butterfly Nebula, Scorpius Constellation Classic Round Sticker

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


tagged with: envelope sealers, galaxies and stars, stellar winds, btbgneb, butterfly nebula, bug nebula, scorpius constellation, ngc 6302, sculptured gas clouds, monogram initials

Galaxies, Stars and Nebulae series NGC 6302, more popularly called the Bug Nebula or the Butterfly Nebula, lies within our Milky Way galaxy, roughly 3,800 light-years away in the constellation of Scorpius.
The central dying star cannot be seen because it's hidden within a doughnut-shaped ring of dust, which appears as a dark band pinching the nebula in the centre. The thick dust belt constricts the star's outflow, creating the classic "bipolar" or hourglass shape displayed by some planetary nebulae.
The nebula's reddish outer edges are largely due to light emitted by nitrogen, which marks the coolest gas visible in the picture. The white-coloured regions are areas where light is emitted by sulphur. These are regions where fast-moving gas overtakes and collides with slow-moving gas that left the star at an earlier time, producing shock waves in the gas (the bright white edges on the sides facing the central star).

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image code: btbgneb

image credit: NGC 6302 was imaged on 27 July 2009 with Hubble's Wide Field Camera 3 in ultraviolet and visible light. Filters that isolate emissions from oxygen, helium, hydrogen, nitrogen and sulphur were used to create this composite image.

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Orion Nebula Powis iPad Air 2 Case

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!


tagged with: orion, nebula, rust, aqua, green, space, cosmic, astronomy, images, nasa, hubble

A lovely image of the Orion Nebula thanks to NASA/Hubble Space Telescope.

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