Tuesday 27 October 2015

Artificial intelligence finds messy galaxies

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An astrophysics student has turned to artificial intelligence to help her to see into the hearts of galaxies. She was inspired by neural networks to create a program to single out from thousands of galaxies the subjects of her study -- the most turbulent and messy galaxies.
via Science Daily
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Graphene flakes as an ultra-fast stopwatch

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Scientists have developed a new optical detector from graphene which reacts very rapidly to incident light of all different wavelengths and even works at room temperature. It is the first time that a single detector has been able to monitor the spectral range from visible light to infrared radiation and right through to terahertz radiation. The scientists use the new graphene detector for the exact synchronization of laser systems.
via Science Daily

Wall-less Hall thruster may power future deep space missions

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To prolong the lifespan of Hall thrusters, scientists have experimentally optimized the operation of a novel, wall-less thruster prototype developed a year ago by the same team. The preliminary performance results were satisfactory, the team said, and pave the way toward developing a high-efficiency wall-less Hall thruster suitable for long-duration, deep space missions.
via Science Daily
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Probing the mysteries of Europa, Jupiter's cracked and crinkled moon

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New research, using spectrographic data, shows what are likely deposits from Europa's sub-surface ocean on it's so-called 'chaos terrain.'
via Science Daily
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Why Earth is so much bigger than Mars: Rocky planets formed from 'pebbles'

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Using a new process in planetary formation modeling, where planets grow from tiny bodies called 'pebbles,' scientists can explain why Mars is so much smaller than Earth. This same process also explains the rapid formation of the gas giants Jupiter and Saturn, as reported earlier this year.
via Science Daily
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Engineering students 'talk' to satellite

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With the help of enthusiastic European ham radio operators, engineering students now have two-way communication with their home-built ESA-sponsored satellite AAUSAT5 that was sent into orbit around Earth from the International Space Station (ISS) on October 5.
via Science Daily
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Bright from the Heart Nebula

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Zazzle Space Gifts for young and old

Graphene Biosensors

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Graphene for sensor applications has received considerable attention due to the material's unique physicochemical properties, such as large surface to volume ratio, high mechanical strength, biocompatibility, excellent thermal and electrical conductivity, low cost, safety and ease of production. Graphene also exhibits a broad electrochemical potential and low charge-transfer resistance, making it almost ideal for multifunctional fast sensors. Another important feature required in optical biosensors is the ability to be functionalized. Both graphene and graphene oxide (GO) are versatile materials for functionalization.

 

This multitude of favorable properties has led to a wide array of investigations into graphene use for biosensing. Particularly interesting configurations are graphene field-effect transistors (GFETs) and graphene enhanced surface plasmon resonance (SPR). These types of graphene sensors have been used for DNA, protein, glucose, and bacteria detection.

 

Figure: Sketch of GFET sensor (Reproduced from Chem. Sci., 2012,3, 1764, with permission of The Royal Society of Chemistry).

 

Graphene field effect transistors (GFET)


GFET is a modification of the classic silicon field-effect transistor, ubiquitous in modern electronics. In traditional transistors, silicon acts as a thin conducting channel, the conductivity of which can be tuned with applied voltage. GFETs perform in a similar manner, except that the silicon is replaced with graphene, which yields a much thinner and hence more sensitive channel region. Due to the broad electrochemical potential and ability to be functionalized, GFETs present an attractive device for biomolecules to attach to, and because of graphene's ultimate thinness and extreme surface-to-volume ratio, even the smallest concentration of attached molecules changes the channel conductivity. GFET biosensors are available for sensing enzymes, hydrogen peroxides, dopamine, and reduced b-nicotinamide adenine dinucleotide (NADH) molecules.

 

Surface plasmon polariton detectors


In a different configuration, graphene or GO is used in conjunction with surface plasmon polaritons (SPPs) on metal films to enhance biosensor performance. SPP-based sensors utilize the confinement of optical waves on the surface of metals to make small-volume chemical and biological sensors. The sensing volume is given by the tightly confined surface wave, boosting sensitivity of optical detection. Standard metals used in this type of sensor are gold and silver, due to their favorable SPP propagation properties. However, silver corrodes quickly, and gold has poor adsorption properties. Placing a layer of graphene on top of the gold results in superior adsorption, and GO is in particular good at binding proteins, due to its high covalent binding affinity. GO multiplies the sensitivity of SPP sensors in this label-free detection system. In conjunction with microfluidics technology, researchers have shown that they can detect a single cancer cell. In a most recent result, scientists announced that GO-based chips could be used for detection of HIV. The selectivity of the GO SPP sensor was enhanced by adding streptavidin to the GO coating. Adding selectivity to GO SPP sensors has been a rising trend in research, with several recent reports on the topic. Selectivity can also be improved by utilizing several graphene measurement modes at once, such as mechanical, electrical, and optical.

 

Figure: SPP sensor enhanced with graphene (Reproduced from Optics Express 18, 14395 (2010) with permission from the Optical Society of America).

 

Aside from GFETs and SPPs, several other types of graphene-enhanced sensors are on the rise, such as for example micromechanical (MEMS) and pressure sensors.


via Graphenea

Common chemical makeup at largest cosmic scales

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A new survey of hot, X-ray-emitting gas in the Virgo galaxy cluster shows that the elements needed to make stars, planets and people were evenly distributed across millions of light-years early in cosmic history, more than 10 billion years ago.
via Science Daily
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