
Each fluid reveals a different letter.
What’s the News: Scientists have developed a chip that can instantaneously identify fluids applied to it, just from their unique surface tension. In a handheld device, it could help toxic site remediators figure out what that ominous clear liquid is. And there’s a bonus for the kids-in-the-treehouse user demographic: different secret messages can appear on the chip depending on what fluid is applied.
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Fiordland National Park in New Zealand, the location of the study
What’s the News: Researchers have mapped out the detailed geological history of a 300-square-mile chunk of New Zealand, from 2.5 million years ago to the present day. The study showed how glaciers carved out the area’s distinctive valleys using a little-known technique called thermochronometry, which involves shooting proton beams onto rocks and making note of what happens—along with some impressive analytical skills.
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Walking the halls of one of the world’s great art museums, it’s easy to regard familiar classic paintings as eternal and unchanging. But this is not the case. Paintings are a mix not only of color but of chemistry—and chemistry changes. In some of Vincent van Gogh’s works, the striking, sunny yellows have faded and turned brownish, robbing the Dutch master’s art of some of its trademark intensity. So a European team of scientists decided to find out exactly what was happening on those canvases.
Using sophisticated X-ray machines, they discovered the chemical reaction to blame — one never before observed in paint. Ironically, van Gogh’s decision to use a lighter shade of yellow paint mixed with white is responsible for the unintended darkening, according to a study published online Monday in the journal Analytical Chemistry. [Los Angeles Times]
Vincent loved yellow. In particular, he loved chrome yellow, a 19th century invention that shone brighter than previously available hues of paint. Art preservationists have known that the lead-based paint fades under intense sunlight, so they’ve done what they can to keep van Goghs and similar works out of intense light. What’s curious about his paintings, however, is that some yellows have faded while others have not.
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We humans are great at making ethanol from grains. We’ve been doing it for thousands of years to make beer and liquor, and our expertise is one reason that corn ethanol has been the biofuel of choice so far. But the biofuels of the future, experts say, will come not from the starch in corn but from the cellulose in grasses and other abundant green plants. There’s just one problem: We’re not good at breaking down the tough structure of cellulose to get at the sugars inside.
But cows are.
Cows, like termites and leafcutter ants, love to eat tough plant material, and host bacteria with the molecular machinery to do so in their guts. Scientists, in their attempts to get better at breaking down cellulose, have tried to copy nature by studying the enzymes that allow those grass-eating animals to do their thing. And now researchers say they have found a treasure trove of new microbe-produced enzymes inside a cow that could help them in their quest.
In a study published Thursday in the peer-reviewed journal Science, researchers described how they incubated bags of switchgrass inside cow rumens and from that found 27,755 “candidate genes” with the potential for efficiently breaking down plant cellulose into usable sugar that can then become ethanol. [MSNBC]
Eddy Rubin and his team executed this chemical excursion by surgically opening a hole into the first of the cow’s four stomachs.
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The weights, they are a-changin’.
What we’re taught in school science classes is a streamlined version of a muddier and more complicated reality, and it’s no different with something as iconic as the periodic table of elements. This week the venerable chart’s overseers decided to fiddle with the atomic weights of 10 elements, changing their values from a single set number to a range of numbers, which is messier but more accurately resembles the messy real world.
The reason for the change is that atomic weights are not always as concrete as most general-chemistry students are taught, according to the University of Calgary, which made the announcement, and the snappily named International Union of Pure and Applied Chemistry‘s Commission on Isotopic Abundances and Atomic Weights, which oversees such weighty matters. [CNET]
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Akira Suzuki, Ei-ichi Negishi, and Richard Heck.
These three scientists won the Nobel Prize for Chemistry this morning for their discoveries that made it easier and cheaper to build long carbon chains in the lab, and use those chains to develop new drugs, build electronics, and more.
Despite the ubiquity of carbon chains in nature, they’re hard to make in the lab at room temperature. The three chemists independently created essentially the same way to skirt this problem, using palladium to link carbon atoms through a process called palladium-catalyzed cross coupling. The palladium is a go-between, bonding to carbon to bring its atoms closer to one another than they could go on their own. The carbons then break their attachment to palladium and bond together in chains.
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The silicon from which most electronics are built is a useful, durable material up to about 350 degrees Fahrenheit (but don’t go sticking your iPhone in the oven). Three hundred fifty isn’t bad, says engineer Alton Horsfall of Newcastle University in the U.K., but not nearly good enough for his mission: monitoring volcanoes. Horsfall and colleague Nick Wright say their research into a different material, silicon carbide (SiC), shows that it could work at temperatures in excess of 1,000 degrees F, and might be just what they need to keep watch on inhospitable places like the blazing-hot mouth of a volcano.
The silicon and carbon in silicon carbide bond very strongly, permitting them to survive extreme temperatures. But the material’s pricey and hard to work with for the same reason. So while organizations like NASA have done silicon carbide research, the material hasn’t spread to a multitude of applications.
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If you’re a tobacco hornworm caterpillar, your own spit can come back to bite you: That plant you tried to eat for dinner can use your own saliva to summon larger animals that might like to make you their dinner.
According to a study in Science, the tobacco plant has evolved a clever defense against hungry insects—it calls in the insects’ predators for help:
When a leaf is wounded, plants immediately release a “bouquet” of distress chemicals known as green leaf volatiles (GLVs) into the air. GLVs are formed when long fatty acid chains in the cell membranes are chopped up into six-carbon molecules as a result of damage. These molecules can exist in two different shapes, or isomers, depending on the position of a double bond between two of the carbons [The Scientist].
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Researchers have found the secret to improving a robot’s sense of smell: Shove frog eggs up its nose. A team at the University of Tokyo has developed a sensor made from a genetically modified frog egg that can help a robot pick out insect smells and pheromones.
As useful as a moth-smelling robot may seem, researchers believe the study published yesterday in Proceedings of the National Academy of Sciences is just one step towards an inexpensive but sensitive chemical detector. Study coauthor Shoji Takeuchi explains that such a device could pick out gases like carbon dioxide:
“When you think about the mosquito, it is able to find people because of carbon dioxide from the human. So the mosquito has CO2 receptors. When we can (extract) DNA (from the mosquito) we can put this DNA into the frog eggs to detect CO2.” [Reuters]
Here’s how they did it.
Step 1 — Get Some Frog Eggs
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Wet. Dry. Wet. Dry. You’d think the moon were a vacuum cleaner infomercial.
A series of studies in the last few years has raised our hopes that the moon is not completely dry—researchers have said that it’s still drier than the driest places on Earth, but some small amount of water ice is there. Then, this afternoon, along comes another study to reassert that the interior of the moon is drier than bone-dry.
For his paper in Science, Zachary Sharp peered into the lunar samples brought back to Earth by the Apollo missions. Where previous studies of those Apollo rocks suggested water ice was locked inside the minerals, Sharp’s assessment focuses on the chlorine in the sample because it could tell him about the moon’s history.
Most scientists think the moon was born when a huge object roaming the inner solar system — something about the size of Mars — smashed into the embryonic Earth. Debris from the collision coalesced to form the moon. As it cooled, an ocean of magma covering its surface began to crystallize. Sharp and his colleagues studied what happened to two isotopes of the element chlorine during that process [Science News].
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Looking at a planetary nebula 6,500 light years away, scientists recognized an old friend: the buckyball. The large, soccer ball-shaped molecule–made from bonding 60 carbon atoms together–was first seen in a lab in 1985. In a paper published today in Science, scientists confirm the first known extraterrestrial existence of the rare carbon balls.

The buckyballs’ planetary nebula, called TC 1, surrounds a white dwarf star. Using NASA’s Spitzer Space Telescope, a team led by Jan Cami of the University of Western Ontario observed traces of the the 60-atom balls and their 70-atom cousins while looking at light coming from the white dwarf.
When light hits molecules and atoms, they will vibrate in specific, measurable ways–a field of science known as spectroscopy. One of Cami’s colleagues, who was studying Tc 1, found some unfamiliar fingerprints in the nebula’s infrared light. Cami recognized them as carbon’s 60-atom configuration and its favored 70-atom carbon partner. [Discovery News]
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Around the United States, state governments are rushing to enact bans on K2, the hot new (and still mostly legal) drug made with synthetic cannabinoids: lab-created compounds designed to mimic the effects of THC, the active ingredient in marijuana.
Often marketed as incense, K2 — which is also known as Spice, Demon or Genie — is sold openly in gas stations, head shops and, of course, online. It can sell for as much as $40 per gram. The substance is banned in many European countries, but by marketing it as incense and clearly stating that it is not for human consumption, domestic sellers have managed to evade federal regulation [The New York Times].
Missouri is the most recent state to move against K2, the origin of which dates back to the work of Clemson University scientist John Huffman, who was developing these synthetic compounds in the 1990s. Scientifically, the chemicals are interesting for their potential to mimic some of the pain-relieving aspects of marijuana, which advocates of medical marijuana legality point to, without the negative health effects that come with setting a plant on fire and inhaling the smoke. The chemical used in most varieties of K2 is called JWH-018.
Huffman was interviewed by The Guardian last year when K2 was spreading around Europe. Now in his late 70s, he seems to understand something that many politicians can’t seem to get through their heads: Risk-taking teenagers will go to about any length, legal or illegal, to get high. Huffman says he wouldn’t oblige the numerous enterprising types who asked him how to make his substances, and that the substances are always labeled not for human consumption. But he figured someone was going to figure it out sooner or later, especially considering the chemical doesn’t show up on drug tests.
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Who needs poppy plants to produce morphine? Last month scientists said they’d isolated the genes those plants use to synthesize the narcotic chemical and made it themselves in a lab. Now, in a study in the Proceedings of the National Academy of Sciences, another team has suggested that we mammals might possess the pathway to create our own morphine.
Because we have receptors for the opiate in our brains (which makes it such an effective and addictive painkiller), and because morphine traces show up in our urine, scientists had long wondered if animals could produce the drug themselves. But studies using living animals yielded inconclusive results because of possible contamination from external sources of morphine in their food or in the environment [Nature]. In addition, the body breaks down and changes morphine, which complicates the task.
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A little square that has been left blank on the periodic table for all these years might finally be filled in. A team of American and Russian scientists have just reported the synthesis of a brand new element–element 117. Says study coauthor Dawn Shaughnessy: “For a chemist, it’s so fundamentally cool” to fill a square in that table [The New York Times].
If other scientists confirm the discovery, the still-unnamed element will take its place between elements 116 and 118, both of which have already been tracked down. A paper about element 117 will soon be published in Physical Review Letters, and scientists say the new element appears to point the way toward a brew of still more massive elements with chemical properties no one can predict [The New York Times].
Element 117 was born in a particle accelerator in Russia, where the scientists smashed together calcium-48 — an isotope with 20 protons and 28 neutrons — and berkelium-249, which has 97 protons and 152 neutrons. The collisions spit out either three or four neutrons, creating two different isotopes of an element with 117 protons [Science News].
The new element 117, takes it place between two superheavy elements that scientists know to be very radioactive and that decay almost instantly. But many researchers think it is possible that even heavier elements may occupy an “island of stability” in which superheavy atoms stick around for a while [Science News]. If this theory holds up, scientists say, the work could generate an array of strange new materials with as yet unimagined scientific and practical uses [New York Times].
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Since NASA’s Stardust mission returned in 2006 from its trip of billions of miles collecting the dust of a comet called Wild2 and dropped it samples down to Earth in the Utah desert, the samples have raised all sorts of questions about how comets formed and what the early solar system was like. In a study this week in Science, there’s a new surprise. Scientists say that the comet sample contains chemicals that must have formed in our home turf, the inner solar system.
Lead researcher Jennifer Matzel studies a tiny particle taken from Stardust’s sample, a piece just five micrometers across. In it her team found the mark of materials that would have formed under high temperatures. Matzel, who specializes in using the decay rates of radioactive chemical elements to assess ancient dates, determined that the Stardust particle must have crystallized just 1.7 million years after the oldest solid rocks in the solar system were forming [San Francisco Chronicle]. After that, the researchers says, the particle must have been flung out to the Kuiper Belt, the region of icy comets revolving around the sun at a distance far past Neptune.
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