Friday, 12 June 2015

Mission possible: This device will self-destruct when heated

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Where do electronics go when they die? Most devices are laid to eternal rest in landfills. But what

The post Mission possible: This device will self-destruct when heated has been published on Technology Org.

 
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Center of Milky Way in Sagittarius Print

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


tagged with: astronomy, background, celestial bodies, milky way, natural sciences, natural world, nobody, outer space, physical science, sagittarius, sciences, stars, zodiac

ImageID: RR016935 / Roger Ressmeyer / CORBIS / Center of Milky Way in Sagittarius /

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Why combining Mentos and Coke creates a sugary volcano, and other cool candy tricks

Science Focus

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How to make sparks fly in your mouth

We're issuing a science-based exception to the "don't chew with your mouth open" rule for this one. If you crunch Wint-O-Green Life Savers with your mouth open in the dark in front of a mirror, you should see some sparks start to fly. The light you see is due to a phenomenon called "triboluminescence."

When you chomp down on a mint, your teeth are fracturing crystals of sugar. This fracturing happens all the way down at the molecular level, where chemical bonds are broken. Because of the structure of the sugar crystal, the breaking of these chemical bonds causes a build-up of electrons that creates a miniature electrical field. Eventually, the electrons glom onto molecules like oxygen or nitrogen in the air, and emit a bit of light in the process. Usually we can't see this light because it's in the ultraviolet part of the spectrum. But wintergreen candies contain a compound called methyl salicylate that fluoresces, converting that UV light into visible blue light.

(More from World Science Festival: Remembering polio vaccine pioneer Jonas Salk)

Why do Pop Rocks pop?

Carbon dioxide gas is the chemical key to making Pop Rocks crackle in your mouth. Pop Rocks are made by heating a mixture of carbon dioxide and candy (a combination of sugar, corn syrup, lactose, and flavoring) to temperatures above 320 degrees Fahrenheit inside a pressurized chamber. While there's still 600 pounds per square inch of pressure on the mixture, the candy-carbon dioxide combination is cooled. After cooling, the pressure is released and the candy shatters into pieces full of tiny bubbles of carbon dioxide gas.

When you stick some Pop Rocks in your mouth, the candy melts and the carbon dioxide bubbles escape from their sugary prisons with satisfying pops.

And, despite any rumors you might have heard, eating Pop Rocks and drinking soda together won't cause your stomach to explode. That urban legend seems to have spread based on the false notion that pop rocks and soda would combine like an acid and a base and react violently — but since they both just get their fizz from carbon dioxide, the worst thing that would happen to you would be a really big burp.

Why do Mentos and Diet Coke create a geyser?

While you won't get much of a thrill from mixing Pop Rocks and Coke, if you pop some Mentos mints into a bottle of Diet Coke, you'll get to see an impressive geyser:

In some ways, the reaction looks like a science fair volcano. But unlike a baking soda-vinegar geyser, the candy isn't combining with the Coke in an acid-base reaction (none of the ingredients in Mentos are basic). Instead, the Mentos serves as a little factory and launchpad for carbon dioxide bubbles — supercharging the normal bubble-formation process in the Coke. The mint's rough surface has thousands of tiny pores, an ideal landscape for lots of bubbles to form (a process called nucleation). As the bubbles grow they become more buoyant and float up to the top of the soda. The process keeps chugging along, creating more and more bubbles until it explodes out the top of the bottle in a foamy overflow.

Certain ingredients in Mentos, like aspartame and potassium benzoate, also speed the process by acting as surfactants — chemicals that lower the surface tension of the soda. This makes it even easier for bubbles to form on the candy. Too much surface tension in a liquid doesn't allow for much bubble formation — the attractions between molecules in the liquid are strong enough that the molecules at the surface resist moving up and away. Adding a surfactant, like Mentos in Coke or soap in water, loosens the liquid molecules' hold on each other a little bit, allowing for bubbles to form.

Appalachian State University physicist Tonya Coffey wrote an in-depth paper on the science behind the Coke-Mentos reaction published in the American Journal of Physics in 2008. Coffey found that combining Diet Coke and Fruit Mentos yielded the most impressive horizontal spray distance, flinging the soda nearly 17 feet from the bottle.

Making candy dance

For a less explosive demonstration of the powers of carbon dioxide fizziness, you can drop a few pieces of various kinds of candy or food into a glass of clear soda and see what happens. Anything with a rough surface — like raisins, or Valentine's Day conversation hearts — should provide a good surface for bubbles to form, as we saw with the Mentos. If the candy (or raisin) is light enough, the carbon dioxide bubbles should be able to buoy it up to the surface; when the bubble pops, the candy (or raisin) falls back down again. This up-and-down "dance" should last until the soda goes flat.

See the spectrum in black jellybeans

Plunk a wet black jellybean down on a piece of filter paper, and you'll be able to see that its blackness is actually made from a combination of hues. The various dyes in the bean will travel different distances away from the jellybean on the filter paper due to their different properties. Some shades of dye are more water-soluble, meaning they dissolve more easily and can be carried along the paper further. Some colors will be more attracted to the paper. The resulting rings of colors are called a separation pattern — something chemists use all the time to figure out what different chemical ingredients are in a mixture. You can try this same experiment with other colors of jellybeans and with other candies as well.

(More from World Science Festival: Getting sleep in the wild)

How to grow giant gummy bears

If you leave gummy bears in tap water for a while, they'll swell up into something more like Gummy Grizzlies. The reason for this is the process of osmosis — the tendency for water to perform a balancing act where it flows from a solution with fewer molecules dissolved into it into a solution that has more molecules in it (provided the two solutions are accessible to each other through a semipermeable membrane that allows certain molecules to cross its border, but which screens out others).

Gummy bears are actually a solution of water. These candies start out as a liquid mixture of water and gelatin, which is heated and then cooled, a process that draws water out of the bear and hardens it into a chewier texture. But there's still some water trapped in the matrix of gelatin that forms the bear. When you stick a gummy bear in water, osmotic pressure forces water molecules into the gummy bear, making the candy swell up like a sponge.

How to take the M off an M&M

If you leave an M&M or a Skittle in water for a little while, the 'M' or 'S' should peel off and float up to the surface. That's because the letters on the candy are made out of white edible ink that doesn't dissolve, unlike the dyes that color the candy shell.

Making soap bubbles with candy corn

This is one experiment you won't be able to do at home, unless you happen to live in a low-gravity environment:

NASA astronaut Don Pettit used his special stash of candy corn on the International Space Station to model how soap works. Soap molecules have a hydrophobic (water-hating) end and a hydrophilic (water-loving) end. When you scrub something with soap, the hydrophobic ends of the soap molecules automatically point towards little globules of grease and oil on your clothes (or your dishes, or your skin); eventually, the particles of grease are encased in little bubbles of soap and can be rinsed off with water.

(More from World Science Festival: How fear happens)

With his candy corn experiment, Pettit did the same trick, but in reverse: He coated one end of his candy corn pieces with oil, making it hydrophobic, then started adding kernels to a floating sphere of water. The hydrophobic ends naturally oriented themselves away from the center. After Pettit added enough candy corn, the sphere reached what's known as the "critical micelle concentration." The candy corn sphere wasn't mushy anymore, but behaved like a solid ball — or like a soap-coated grease globule ready to be rinsed off and away.

Why microwaved marshmallows puff up

Put a couple marshmallows in the microwave for about a minute, and you'll see them puff up. This is because the heat from the microwave softens the sugar in the marshmallow, and also causes the air pockets inside the sweet to expand. Because the sugary walls of the marshmallow are softer, the marshmallow puffs up. When cooled, the marshmallow shrinks down again — but is usually a bit crunchier than before, probably because some of the water inside it evaporated in the heat of the microwave.

 
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 » see original post http://theweek.com/articles/442667/why-combining-mentos-coke-creates-sugary-volcano-other-cool-candy-tricks
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NASA wants to cut travel time to Mars “in half” with new propulsion tech

Science Focus

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Speaking at an Aerojet Rocketdyne plant, NASA administrator Charles Bolden said that NASA is looking into advanced propulsion technologies that can cut the current eight-month journey to Mars "in half." Technologies such as solar-electric propulsion are definitely on the cards, but NASA may look towards more unconventional solutions such as nuclear rockets, too.

Over the past few years, there's been a lot of attention on getting astronauts on Mars, mostly fuelled by crazy projects like Mars One, the success of the Curiosity rover, and heavyweights like Elon Musk saying he wants to colonise Mars.

The main problem with getting humans to Mars is that, with our current liquid-fuelled rocket engines, it takes a very long time to get there; about eight months or so. If we can cut the journey in half, we significantly reduce the amount of food and water needed—which in turn cuts down the weight of the spacecraft, which in turn reduces the amount of fuel needed, which in turn feeds a very positive feedback loop. Less time in outer space means astronauts will be bombarded by less radiation, too.

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 » see original post http://feeds.arstechnica.com/~r/arstechnica/science/~3/p3HY9HpJAE4/
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On-demand X-rays at Synchrotron Light Sources

Science Focus

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Consumers are now in the era of “on-demand” entertainment, in which they have access to the books, music

The post On-demand X-rays at Synchrotron Light Sources has been published on Technology Org.

 
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 » see original post http://feedproxy.google.com/~r/TechnologyOrgPhysicsNews/~3/gHcpE_hyIyw/
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Helix Nebula, Galaxies and Stars Star Sticker

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tagged with: star nurseries, star clusters, galaxies, stars, astronomy, nebulae, helixneb, helix nebula, starfields, european southern observatory, eso, vista

Galaxies, Stars and Nebulae series A fantastic colour-composite image of the Helix Nebula (NGC 7293). It was created from images obtained using the Wide Field Imager (WFI), an astronomical camera attached to the 2.2-metre Max-Planck Society/ESO telescope at the La Silla observatory in Chile.

The blue-green glow in the centre of the Helix comes from oxygen atoms shining under effects of the intense ultraviolet radiation of the 120 000 degree Celsius central star and the hot gas.

Further out from the star and beyond the ring of knots, the red colour from hydrogen and nitrogen is more prominent. A careful look at the central part of this object reveals not only the knots, but also many remote galaxies seen right through the thinly spread glowing gas.
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ESO/J. Emerson/VISTA www.eso.org
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Blind quantum computing method surpasses efficiency 'limit'

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(Phys.org)—Demonstrating that limits were made to be broken, physicists have overcome what was previously considered to be a natural and universal limit on the efficiency of a quantum cryptography task called blind quantum computing. The new method offers significant efficiency improvements and, in some cases, requires exponentially fewer communication resources to implement than previous methods did.

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The Medusa Nebula

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Braided, serpentine filaments of glowing gas suggest this nebula's popular name, The Medusa Nebula. Also known as Abell 21, this Medusa is an old planetary nebula some 1,500 light-years away along the southern border of the constellation Gemini. Like its mythological namesake, the nebula is associated with a dramatic transformation. The planetary nebula phase represents a final stage in the evolution of low mass stars like the sun, as they transform themselves from red giants to hot white dwarf stars and in the process shrug off their outer layers. Ultraviolet radiation from the hot star powers the nebular glow. An unrelated, bright, foreground star is near center in this close-up, telescopic view, while the Medusa's transforming central star is actually the dimmer star below center and toward the right-hand part of the frame. The Medusa Nebula is estimated to be over 4 light-years across.

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LHC physicists preserve Native American voices

NASA's Great Observatories Witness a Galactic Spec iPad Mini Case

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tagged with: new, image, two, tangled, galaxies, has, been, released, nasa's, great, observatories., antennae, located, about, million, light-years, from, earth, are, shown, this, composite, chandra, x-ray, observatory, blue, hubble, space, telescope, gold, brown, spitzer, red, take, their, name, long, antenna-like, arms, seen

A new image of two tangled galaxies has been released by NASA's Great Observatories. The Antennae galaxies, located about 62 million light-years from Earth, are shown in this composite image from the Chandra X-ray Observatory (blue), the Hubble Space Telescope (gold and brown), and the Spitzer Space Telescope (red). The Antennae galaxies take their name from the long, antenna-like arms seen in wide-angle views of the system. These features were produced in the collision.

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Graphenea secures €2.5 million to install a new production plant

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Graphenea has won a project worth 2.5 million from the EU Horizon 2020 program ‘SME Instrument’. The funding will be used for the construction, installation and commissioning of a new production plant that will multiply production capacity by 200 times and consolidate the firm’s global leadership in the sector. The project was selected among 614 submitted proposals. In addition to construction of the production plant, the project will result in the opening of twenty highly skilled labor jobs.

“It is a very important boost that will accelerate our business plan. It will allow us to grow faster and consolidate our position as the global leader in our industry”, said Jesus de la Fuente, Founder and CEO of Graphenea after receiving the news. “We want to be the best in the world.”

The guarantee: Results and Customers

With this award, the European Commission has recognized Graphenea’s results both in research and production of graphene. The process developed and patented by Graphenea is highly efficient and environmentally friendly.

Graphene is a material under development, with new applications discovered every day, and current uses in advance polymers, battery electrodes and sensors. The world market in 2014 was estimated at about $12 million.

Graphenea currently employs 13 professionals, mostly PhD in Chemistry, and has closed 2014 with more than 400 customers in 50 countries and a turnover of around $1.2 million (~10% of the world market share). Graphenea holds leading international firms like Intel, Nokia, IBM, Philips, Repsol, BASF and Sigma-Aldrich in its customer portfolio.

Operating plant in 24 months

The ‘SME Instrument’ will contribute 1.8 million to the construction, installation and optimization of a pilot production plant of high-quality graphene for industrial applications. This is a relevant milestone in the development of Graphenea in an emerging market that recognizes the high quality of the materials produced by the company.

The construction of the new plant will take 24 months, including installation of equipment. If all goes as planned, the new facility could open in late 2017.

De la Fuente states that “in the first year of implementation of the pilot plant, it will allow us to increase our revenues and address the emerging global market for graphene”. He also said that “if the phase pilot plant is successful, Graphenea will move to an industrial phase that will require a larger investment.”

Photo: Graphenea headquarters.

Regulation

In a first stage, the pilot plant will be limited to an annual production of 1 ton per year imposed by the European regulation of new chemical products. Graphene is a new material that has not yet passed the registration process required by the European regulations for new substances, so its production or import is limited. Graphenea has begun the process of registration and certification of their materials to overcome this regulatory limitation. Thus, the firm will become the first producer of graphene approved for industrial use in Europe.

Presence and investment in USA

The main graphene demand comes from the United States, with large activity concentrated in the Boston area. According to the firm, this geographical area holds the biggest potential for development in the coming years. For that reason, and in parallel to the pilot plant project, Graphenea opened an Applications Laboratory at MIT campus. “We must be close to the market,” concluded Jesus de la Fuente.


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How Longhorned Beetles Find Mr. Right

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Smelling good is just part of what some beetles must do to find a mate. They have to

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Star birth in Carina Nebula from Hubble's WFC3 det Posters

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ImageID: 42-23286264 / STScI / NASA/Corbis / Star birth in Carina Nebula from Hubble's WFC3 detector

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Enlarged Region of The Omega Nebula Square Sticker

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Galaxies, Stars and Nebulae series Like the fury of a raging sea, this bubbly ocean of glowing hydrogen, oxygen, and sulphur gas lies in the extremely massive and luminous molecular nebula Messier 17.
This Hubble photograph captures a small region within Messier 17 (M17), a hotbed of star formation. M17, also known as the Omega or Swan Nebula, is located about 5500 light-years away in the Sagittarius constellation.
Ultraviolet radiation is carving and heating the surfaces of cold hydrogen gas clouds and the warmed surfaces glow orange and red. The intense heat and pressure causes some material to stream away from the surface, creating the glowing veil of even hotter green-coloured gas that masks background structures. The colours in the image represent various gases. Red represents sulphur; green, hydrogen; and blue, oxygen.

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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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