Your farts could cure high blood pressure

London, July 3 (IANS) Though most of us may find it quite embarrassing in case we were caught breaking wind, a new study has in fact suggested flatulence could help patients with high blood pressure.

Scientists at Johns Hopkins University, in Bal

timore, Maryland, US, have found that hydrogen sulphide in flatus – informally known as a fart – is also produced by an enzyme in blood vessels where it relaxes them and lowers blood pressure, The Sun reported.

Hydrogen sulphide — a toxic gas generated by bacteria living in the human gut — has been shown to control blood pressure in mice. Those with higher levels of the gas had lower blood pressure than rodents with less.

Researchers at a Chinese university in Nanjing are trying to work out whether this could be used to create a treatment for people suffering from high blood pressure.

Yao Yuyu from the university’s Zhongda Hospital said: “Despite the treatment’s potential, using gas to treat high blood pressure has yet to be tested on humans.

“The effective dosage could prove difficult to establish due to the difference in size between humans and mice.”

Soon: a floating hotel that could fly you around the world!

Melbourne, April 29(ANI): A UK-based designer has come up with a concept of a flying hotel called the “Aircruise”.

Nick Talbot’s design shows a vertical air ship, 30-metre tall, complete with penthouse, four duplex apartments, five smaller ones and glass viewing floors.

The structure will be lifted by hydrogen and propelled by solar power, leaving no carbon footprint.

Also referred to as “clipper in the clouds””, the cruise will fly at a leisurely 145k/h, which means a trip from London to New York will take 37 hours.

“Nick”s ideas are very impressive and take our thinking into the next generation of travel products,”” News.com.au quoted conference convenor Tony Charters as saying, in a statement.

He added: “It could be a very exciting leap forward for tourism, and I hope it will inspire the Australian industry to push forward with creative and innovative ideas to help reinvigorate the industry.””

The Aircruise, which will carry a maximum of 100 passengers, will take off with the aid of four envelopes on the outside, each containing modular self-sealing bags.

Tablot will present his design at the Tourism Futures conference in Brisbane from July 5 to 7. (ANI)

Toxic seaweed to go

Work to remove piles of rotting seaweed from Port Geographe in south-west Western Australia is due to start this month.

The Department of Transport has been forced to take on the job of removing 120,000 cubic metres of sand and weed after Port Geographe developers, responsible for the clean-up, failed to take action.

Concerns were raised after a report by the Department of Health found the mounds were releasing harmful levels of hydrogen sulphide.

Work will start on April 19 and is expected to take between six and eight weeks.

90 percent of distant galaxies have gone undiscovered, say astronomers

Washington, March 26 (ANI): Astronomers, using two of the four giant 8.2-metre telescopes that make up ESO’s Very Large Telescope (VLT), have determined that 90 percent of galaxies whose light took 10 billion years to reach us have gone undiscovered.

Astronomers frequently use the strong, characteristic “fingerprint” of light emitted by hydrogen known as the Lyman-alpha line, to probe the amount of stars formed in the very distant Universe.

Yet there have long been suspicions that many distant galaxies go unnoticed in these surveys.

The new VLT survey demonstrates for the first time that this is exactly what is happening.

Most of the Lyman-alpha light is trapped within the galaxy that emits it, and 90 percent of galaxies do not show up in Lyman-alpha surveys.

“Astronomers always knew they were missing some fraction of the galaxies in Lyman-alpha surveys, but for the first time we now have a measurement. The number of missed galaxies is substantial,” explained Matthew Hayes, the lead author of the research paper.

To figure out how much of the total luminosity was missed, Hayes and his team used the FORS camera at the VLT and a custom-built narrowband filter to measure this Lyman-alpha light, following the methodology of standard Lyman-alpha surveys.

Then, using the new HAWK-I camera, attached to another VLT Unit Telescope, they surveyed the same area of space for light emitted at a different wavelength, also by glowing hydrogen, and known as the H-alpha line.

They specifically looked at galaxies whose light has been travelling for 10 billion years, in a well-studied area of the sky, known as the GOODS-South field.

“This is the first time we have observed a patch of the sky so deeply in light coming from hydrogen at these two very specific wavelengths, and this proved crucial,” said team member Goran Ostlin.

The survey was extremely deep, and uncovered some of the faintest galaxies known at this early epoch in the life of the Universe.

The astronomers could thereby conclude that traditional surveys done using Lyman-alpha only see a tiny part of the total light that is produced, since most of the Lyman-alpha photons are destroyed by interaction with the interstellar clouds of gas and dust.

This effect is dramatically more significant for Lyman-alpha than for H-alpha light. As a result, many galaxies, a proportion as high as 90 percent, go unseen by these surveys.

“If there are ten galaxies seen, there could be a hundred there,” Hayes said. (ANI)

New evidence points towards water on Moon

London, September 19 (ANI): Two separate lunar missions have found evidence which indicates that the polar regions of the moon are chock full of water-altered minerals.

According to a report in Nature News, early results from NASA’s Lunar Reconnaissance Orbiter (LRO), launched on June 18, are offering a wide array of watery signals.

The Moon, in fact, has water in all sorts of places: not just locked up in minerals, but scattered throughout the broken-up surface, and, potentially, in blocks or sheets of ice at depth.

“We are on the verge of a renaissance in our thinking about the poles of the Moon, including how water ice gets there,” said Anthony Colaprete, principal investigator for the Lunar Crater Observation and Sensing Satellite (LCROSS), which on October 9, will slam into a polar crater with the intention of ploughing up a plume of water ice for many telescopic eyes to see.

The initial LRO results confirm what was long suspected as a way for ice to stay trapped on the Moon for billions of years.

A thermal mapping instrument showed that permanently shadowed regions within deep polar craters are as cold as 35o Kelvin (-238o Celsius).

Project scientist Richard Vondrak said that they are the coldest spots in the Solar System – even colder than the surface of Pluto.

Variations in the flux of neutrons suggests variability in water content among craters.

But, the surprise comes from a different instrument on LRO, which counts slow-moving neutrons as a way of measuring hydrogen abundance in the top metre or so of the surface.

This hydrogen is often interpreted as a proxy for water ice, although it could also be molecular hydrogen or hydrogen trapped in other molecules.

The LRO instrument has already found a significant excess of hydrogen at the poles.

But, with added resolution, it is seeing surprising variability within the polar regions. Some of the craters appear enriched in hydrogen. Others are not.

Stranger still, some areas outside the crater walls, which were thought to get too hot for water to linger, show an excess of hydrogen.

Vondrak said this shows that the water could have arrived more recently, or that it can persist if buried as impacts till the lunar soil.

If the LCROSS impact spews up ice, it will eliminate the last vestiges of doubt about water on the Moon.

It could also start a new hunt: to find a record of impact events, such as water-rich comet strikes, that put the ice there in the first place. (ANI)

Catalyst simulations for fuel cells may make clean cars a reality

Washington, Sep 18 (ANI): University of Wisconsin-Madison researchers are working towards developing better catalyst for fuel cells in a bid to make clean cars a reality.

If successful, the researchers could make a car that runs on hydrogen from solar power, and produces water instead of carbon emissions.

Materials science and engineering assistant professor Dane Morgan and Ph.D. student Edward (Ted) Holby have developed a computational model that could optimise an important component of fuel cells, making it possible for the technology to have a more widespread use.

The researchers investigated how particle size is related to the overall stability of a material, and showed with their model that increasing the particle size of a fuel cell catalyst decreases degradation and therefore increases the useful lifetime of a fuel cell.

Fuel cells are electrochemical devices that facilitate a reaction between hydrogen and oxygen, producing electrical power and forming water.

In the type of fuel cells Morgan is researching, called proton exchange membrane fuel cells (PEMFCs), hydrogen is split into a proton and electron at one side of the fuel cell (the anode).

The proton moves through the device while the electron is forced to travel in an external circuit, where it can perform useful work, while at the other side of the fuel cell (the cathode), the protons, electrons and oxygen combine to form water, which is the only waste product.

One of the many hurdles to producing efficient fuel cells for widespread use is the catalyst added to aid the reaction between protons, electrons and oxygen at the cathode.

Current fuel cells use platinum and platinum alloys as a catalyst. While platinum can withstand the corrosive fuel cell environment, it is expensive and not very abundant.

Thus, to maximize platinum use, researchers use catalysts made with platinum particles as small as two nanometers, which are approximately 10 atoms across.

These tiny structures have a large surface area on which the fuel cell reaction occurs.

However, platinum catalysts this small degrade very quickly, which means that the fuel cell doesn’t last long.

The researchers have found a possible solution to the rapid degradation problem-when it comes to catalyst particle size, sometimes smaller isn’t better.

In their modelling work, they showed that if the particle size of a platinum catalyst is increased to four or five nanometers, which is approximately 20 atoms across, the level of degradation significantly decreases.

This means the catalyst and the fuel cell as a whole can continue to function for much longer than if the particle size was only two or three nanometers.

“Fuel cells are just one of many energy technologies – solar, battery, etc. – with enormous potential to reduce our dependence on oil and our carbon emissions. Computer simulation offers a powerful tool to understand and develop new materials at the heart of these energy technologies,” said Morgan. (ANI)

New method to monitor early sign of oxidative stress that triggers cancer

Washington, Sept 12 (ANI): Scientists from University of Michigan have developed a new method to monitor early sign of oxidative stress that triggers cancer spread.

Lead researcher Kate Carroll suggests that being able to monitor a marker of oxidative stress that is associated with the activation of tumor cell growth pathways, particularly at an early stage, and then tailor treatments accordingly would allow for more targeted studies and might improve the odds of success with antioxidants and pro-oxidants.

The new method detects sulfenic acid in proteins-a tip off to early oxidative stress and to a specific protein modification associated with cell growth pathways.

Sulfenic acid is produced when a particular oxidant, hydrogen peroxide, reacts with the protein building block cysteine. But because the chemical modification involved is so small and transient, it has been difficult to detect.

To get around that problem, Carroll and Seo used a chemical probe that “traps” sulfenic acid and tags it for recognition by an antibody.

The antibody is labeled with a fluorescent dye that glows when observed with a fluorescence microscope.

The researchers then used the method to assess sulfenic acid levels as a marker of oxidative stress in several systems, including a panel of breast cancer cell lines.

“For each line, we saw a very distinct pattern of sulfenic acid modifications,” indicating different oxidative stress levels and hinting at differences in the underlying molecular events associated with tumor growth,” said Carroll, assistant professor of chemistry and a research assistant professor in the Life Sciences Institute.

“Whether the patterns we see will correlate with response to antioxidant treatment or other therapies that modulate oxidative stress level remains to be seen, but now we at least have a way to investigate that question,” the expert added.

The study appears in Proceedings of the National Academy of Sciences. (ANI)

Pak Qaeda hand in 2006 trans-Atlantic bomb plot revealed

London, Sep.8 (ANI): New evidence put before a British jury during a retrial of three Brit Muslim convicts suggests that the men used code words to discuss their plans with an al-Qaeda fixer based in Pakistan.

The e-mails and conversations suggest that the plot was in its final stages, possibly days away from execution in 2006.

The seven daily flights highlighted by the three plotters were: 14.15 United Airlines Flight 931 to San Francisco; 15.00 Air Canada Flight 849 to Toronto; 15.15 Air Canada Flight 865 to Montreal; 15.40 United Airlines Flight 959 to Chicago; 16.20 United Airlines Flight 925 to Washington; 16.35 American Airlines Flight 131 to New York; 16.50 American Airlines Flight 91 to Chicago.

According to The Telegraph and the Daily Express, the batteries the gang planned to use as part of their detonators were bought in Pakistan.

An ingredient in the bomb mix was the orange soft drink Tang – sold in Pakistan – which had a high sugar content to aid the explosion.

A British intelligence source said: “The use of drink bottles sold in Pakistan and batteries sold in Pakistan underline the plot’s ties to that country. The foot soldiers were from Britain – but the organisers were in Pakistan.”

A security source said of the conspiracy: “It was very clever and the airport scanners would not have picked up the devices at all.”

Prosecutor Peter Wright told the Woolwich Crown Court in South East London how the would-be bombers were “a cell of home-grown terrorists activated and directed by a designated leader in Pakistan.”

That was confirmed by a government source in Pakistan, who said the plot was believed to have originated “with al-Qaeda in Afghanistan.”

Seized e-mails showed the chain of terror stretched from there, across the lawless border to Pakistan, to London and to the woods of High Wycombe where explosives were buried.

The aim was to mirror the 1988 bombing of Pan Am Flight 103 over Lockerbie, which killed 259 passengers and 11 in the Scottish town.

Aliases exposed during the trial revealed the terror kingpin in Pakistan was dubbed “Paps” or “Papa”.

Ali called himself Imran and Chacha and also set up email accounts in the bogus names Tippu Khan and Jameel Masood.

His co-conspirators used aliases such as Fatty, Arro and Nigga.

Hydrogen peroxide was known as “aftershave”, police surveillance as “skin problems” and martyrdom videos were referred to as “wedding tapes”.

It is also thought that the bomb makers received training at an al-Qaeda camp in Pakistan.

A mystery Pakistani, thought to be a top al-Qaeda envoy, made contact with the three would-be suicide bombers during a flying visit to Britain in June 2006.

Experts who tested the explosive mix on the aircraft were horrified.

A witness said: “It was absolutely devastating.” (ANI)

Image of different regions of Trifid Nebula captured by European Southern Observatory

Munich, August 27 (ANI): A new image by the European Southern Observatory (ESO) has captured the different regions of the Trifid Nebula, which is a rare combination of three nebula types, as seen in visible light.

This massive star factory is so named for the dark dust bands that trisect its glowing heart, revealing the fury of freshly formed stars and presaging more star birth.

Smoldering several thousand light-years away in the constellation of Sagittarius (the Archer), the Trifid Nebula presents a compelling portrait of the early stages of a star’s life, from gestation to first light.

The heat and “winds” of newly ignited, volatile stars stir the Trifid’s gas and dust-filled cauldron.

In time, the dark tendrils of matter strewn throughout the area will themselves collapse and form new stars.

The French astronomer Charles Messier first observed the Trifid Nebula in June 1764, recording the hazy, glowing object as entry number 20 in his renowned catalogue.

Observations made about 60 years later by John Herschel of the dust lanes that appear to divide the cosmic cloud into three lobes inspired the English astronomer to coin the name “Trifid”.

Made with the Wide-Field Imager camera attached to the MPG/ESO 2.2-meter telescope at ESO’s La Silla Observatory in northern Chile, the new image prominently displays the different regions of the Trifid Nebula as seen in visible light.

In the bluish patch to the upper left of the image, called a reflection nebula, gas scatters the light from nearby, Trifid-born stars.

The largest of these stars shines most brightly in the hot, blue portion of the visible spectrum.

This, along with the fact that dust grains and molecules scatter blue light more efficiently than red light, imbues this portion of the Trifid Nebula with an azure hue.

Below, in the round, pink-reddish area typical of an emission nebula, the gas at the Trifid’s core is heated by hundreds of scorching young stars until it emits the red signature light of hydrogen, the major component of the gas, just as hot neon gas glows red-orange in illuminated signs all over the world.

The gases and dust that crisscross the Trifid Nebula make up the third kind of nebula in this cosmic cloud, known as dark nebulae, courtesy of their light-obscuring effects.

Within these dark lanes, the remnants of previous star birth episodes continue to coalesce under gravity’s inexorable attraction.

The rising density, pressure and temperature inside these gaseous blobs will eventually trigger nuclear fusion, and yet more stars will form. (ANI)

Aliens in no mood to response to SETI right now

London, August 19 (ANI): The SETI (Search For Extraterrestrial Intelligence) telescope has produced its first scientific results, but unfortunately it’s still waiting for a response from the aliens.

The project, called the Allen Telescope Array (ATA) after benefactor and Microsoft co-founder Paul Allen, went live in 2007.

It was designed to scan for broadcasts from alien civilizations with more consistency and a wider field of view than any previous effort.

Run jointly by the SETI Institute and the University of California, Berkeley, from a site in northern California, the ATA is ultimately intended to comprise 350 dishes.

But, even with its current complement of 42, it has an impressively wide field of view. It uses relatively small, 6-metre dishes that together can take in five square degrees of sky at a time – a box as wide as 10 full moons.

“At any one moment, you look into a very large piece of the sky,” said Jill Tarter, director of the SETI Institute. “At 350 (telescopes), the ATA just blows any other survey telescope out of the water. Even at 42, it’s interesting,” she told New Scientist.

According to Joeri van Leeuwen, an ATA team member who presented the project’s first results at a conference in the Netherlands in June, “You can see entire galaxies within one shot.”

One question the ATA aims to answer is a mystery of missing gas.

Star-forming regions don’t seem to have enough molecular gas to keep up the star-formation rates we observe.

Some researchers think atomic hydrogen might make up the difference.

ATA team members have searched for it in four groups of galaxies so far, but have not yet found any new intergalactic gas, deepening the mystery.

“This paper was our first science paper, so we’ve answered some questions, but we’re finding new questions again. This paper really shows that our setup is working, we have all the algorithms working, and we could easily upgrade to a more powerful system still,” van Leeuwen said.

Such surveys do not distract from the search for aliens, which – if they exist and are attempting to communicate – may send out broadcasts at wavelengths not commonly emitted by astrophysical objects. (ANI)

US navy chemists try to turn seawater into jet fuel

London, August 19 (ANI): In a new experiment, US navy chemists have processed seawater into unsaturated short-chain hydrocarbons that with further refining could be made into kerosene-based jet fuel.

According to a report by New Scientist, the process involves extracting carbon dioxide (CO2) dissolved in the water and combining it with hydrogen – obtained by splitting water molecules using electricity – to make a hydrocarbon fuel.

It uses a variant of a chemical reaction called the Fischer-Tropsch process, which is used commercially to produce a gasoline-like hydrocarbon fuel from syngas, a mixture of carbon monoxide and hydrogen often derived from coal.

Robert Dorner, a Naval Research Laboratory chemist in Washington DC and first author of a new paper on the technique, said that CO2 is rarely used in the Fischer-Tropsch process because of its chemical stability.

“But CO2′s abundance, combined with concerns about global warming, make it an attractive potential feedstock,” Dorner said.

“Although the gas forms only a small proportion of air – around 0.04 per cent – ocean water contains about 140 times that concentration,” he added.

The navy team has been experimenting to find out how to steer the CO2-producing process away from producing unwanted methane to produce more of the hydrocarbons wanted.

In the conventional Fischer-Tropsch process, carbon monoxide and hydrogen are heated in the presence of a catalyst to initiate a complex chain of reactions that produce a mixture of methane, waxes and liquid fuel compounds.

Dorner and colleagues found that using the usual cobalt-based catalyst on seawater-derived CO2 produced almost entirely methane gas.

Switching to an iron catalyst resulted in only 30 per cent methane being produced, with the remainder short-chain hydrocarbons that could be refined into jet fuel.

According to Heather Willauer, the navy chemist leading the project, the efficiency needs to be much improved, perhaps by finding a different catalyst. (ANI)

Radiation from massive stars may trigger many more stars than previously thought

Washington, August 13 (ANI): A new study from two of NASA’s Great Observatories has shown that radiation from massive stars may trigger the formation of many more stars than previously thought.

While astronomers have long understood that stars and planets form from the collapse of a cloud of gas, the question of the main causes of this process has remained open.

One option is that the cloud cools, gravity gets the upper hand, and the cloud falls in on itself.

The other possibility is that a “trigger” from some external source – like radiation from a massive star or a shock from a supernova – initiates the collapse.

Some previous studies have noted a combination of triggering mechanisms in effect.

By combining observations of Cepheus B from the Chandra X-ray Observatory and Spitzer Space Telescope, researchers have taken an important step in addressing this question.

Cepheus B is a cloud of mainly cool molecular hydrogen located about 2,400 light years from the Earth.

There are hundreds of very young stars inside and around the cloud – ranging from a few millions years old outside the cloud to less than a million in the interior – making it an important testing ground for star formation.

“Astronomers have generally believed that it’s somewhat rare for stars and planets to be triggered into formation by radiation from massive stars,” said Konstantin Getman of Penn State University, and lead author of the study. “Our new result shows this belief is likely to be wrong,” he added.

This particular type of triggered star formation had previously been seen in small populations of a few dozen stars, but the latest result is the first time it has been clearly observed in a rich population of several hundred stars.

The new study suggests that star formation in Cepheus B is mainly triggered by radiation from one bright, massive star outside the molecular cloud.

According to theoretical models, radiation from this star would drive a compression wave into the cloud triggering star formation in the interior, while evaporating the cloud’s outer layers.

The Chandra-Spitzer analysis revealed slightly older stars outside the cloud while the youngest stars with the most protoplanetary disks congregate in the cloud interior – exactly what is predicted from the triggered star formation scenario.

“We essentially see a wave of star and planet formation that is rippling through this cloud,” said co-author Eric Feigelson, also of Penn State. “Outside the cloud, the stars probably have newly born planets while inside the cloud the planets are still gestating,” he added. (ANI)

Your cars may soon be powered by urine

New York, July 15 (ANI): Could it be possible to run your car on urine? Well, it may be, if Ohio University scientists are to be believed.

And their confidence stems from the fact that they have found a novel way to produce hydrogen energy from urine.

According to Discovery News, the scientists used a nickel-based electrode to make cheap hydrogen from urine.

When the research team led by professor Gerardine Botte stuck the electrode into a pool of urine, and applied an electrical current, hydrogen gas was released, which was used in fuel cells.

The prototype is about three inches by three inches, and is capable of generating 500 milliwatts of power.

The scientists hope to create commercial versions of the technology.

Botte expects that the fuel-cell urine-powered car could theoretically travel 90 miles per gallon.

“One cow can provide enough energy to supply hot water for 19 houses. Soldiers in the field could carry their own fuel,” the New York Daily News quoted him as saying.

The researchers focussed their study on urea, a urine by-product.

“Urea is a byproduct of a lot of cities and farms, but even if you take all the people and all the animals, there’s not enough to run the world,” said University of Georgia professor John Stickney.

He added that though applications using urine won’t be available to consumers for quite some time, it’s definitely worth developing.

“We are going to have to put together a lot of greener ways to collect energy that don’t produce greenhouse gases and don’t require us to go to war,” he added. (ANI)

Omega Nebula’s ‘watercolors’ revealed in new image

Munich, July 8 (ANI): A new image captured by the European Southern Observatory (ESO) has reveled the Omega Nebula, a stellar nursery where infant stars illuminate and sculpt a vast pastel fantasy of dust and gas, in all its glory.

The Omega Nebula, sometimes called the Swan Nebula, is a dazzling stellar nursery located about 5500 light-years away towards the constellation of Sagittarius (the Archer).

An active star-forming region of gas and dust about 15 light-years across, the nebula has recently spawned a cluster of massive, hot stars.

The intense light and strong winds from these hulking infants have carved remarkable filigree structures in the gas and dust.

When seen through a small telescope, the nebula has a shape that reminds some observers of the final letter of the Greek alphabet, omega, while others see a swan with its distinctive long, curved neck.

Swiss astronomer Jean-Philippe Loys de Cheseaux discovered the nebula around 1745. The French comet hunter Charles Messier independently rediscovered it about twenty years later and included it as number 17 in his famous catalogue.

In a small telescope, the Omega Nebula appears as an enigmatic ghostly bar of light set against the star fields of the Milky Way.

In recent years, astronomers have discovered that the Omega Nebula is one of the youngest and most massive star-forming regions in the Milky Way.

Active star-birth started a few million years ago and continues through today.

The newly released image, obtained with the EMMI instrument attached to the ESO 3.58-metre New Technology Telescope (NTT) at La Silla, Chile, shows the central region of the Omega Nebula in exquisite detail.

The NASA/ESA Hubble Space Telescope has also imaged small parts of this nebula.

At the left of the image, a huge and strangely box-shaped cloud of dust covers the glowing gas.

The fascinating palette of subtle color shades across the image comes from the presence of different gases (mostly hydrogen, but also oxygen, nitrogen and sulfur) that are glowing under the fierce ultraviolet light radiated by the hot young stars. (ANI)

Cardiac drug research may get a boost from new way to detect nitroxyl

Washington, July 6 (ANI): Wake Forest University scientists have identified unique chemical markers for detecting the presence of a compound called nitroxyl in biological systems, an achievement that can boost cardiac drug research.

The researchers point out that nitroxyl-a cousin to the blood-vessel relaxing compound nitric oxide-has already been shown to strengthen canine heart beats in previous studies.

However, they add, research into its potential benefits for humans has been slowed by a lack of specific detection methods.

“I think this is a very powerful tool to help in the development of new drugs for congestive heart failure,” said S. Bruce King, a professor of chemistry at Wake Forest who leads the team that conducted the research.

The researchers say that nitroxyl can be generated from precursor chemicals under controlled conditions, but studying the molecule’s activity in cells is difficult because its constituent elements-nitrogen, oxygen and hydrogen-react so readily with other molecules.

King and colleagues used compounds that are not present in normal cell biology to produce a reaction that yields the identifying chemical markers.

While the researchers have established that the human body naturally produces nitric oxide, natural production of nitroxyl is suspected but has not been demonstrated.

King said that the new chemical markers could help answer that question, as well.

A research article on this study has been published online in the American Chemical Society’s journal Organic Letters. (ANI)

Astronomers unveil largest map of cold cosmic dust

Berlin, July 2 (ANI): Astronomers have unveiled the largest map of cold cosmic dust, which are peppered in the inner regions of the Milky Way galaxy, and are the potential birthplaces of new stars.

Made using observations from the APEX telescope in Chile, this will prove an invaluable map for observations made with the forthcoming ALMA telescope, as well as the recently launched ESA Herschel space telescope.

This new guide for astronomers, known as the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) shows the Milky Way in submillimeter-wavelength light.

Images of the cosmos at these wavelengths are vital for studying the birthplaces of new stars and the structure of the crowded galactic core.

“ATLASGAL gives us a new look at the Milky Way. Not only will it help us investigate how massive stars form, but it will also give us an overview of the larger-scale structure of our galaxy,” said Frederic Schuller from the Max Planck Institute for Radio Astronomy, leader of the ATLASGAL team.

The area of the new submillimeter map is approximately 95 square degrees, covering a very long and narrow strip along the galactic plane two degrees wide (four times the width of the full Moon) and over 40 degrees long.

The Universe is relatively unexplored at submillimeter wavelengths, as extremely dry atmospheric conditions and advanced detector technology are required for such observations.

The interstellar medium – the material between the stars – is composed of gas and grains of cosmic dust, rather like fine sand or soot.

However, the gas is mostly hydrogen and relatively difficult to detect, so astronomers often search for these dense regions by looking for the faint heat glow of the cosmic dust grains.

Submillimeter light allows astronomers to see these dust clouds shining, even though they obscure our view of the Universe at visible light wavelengths.

Accordingly, the ATLASGAL map includes the denser central regions of our galaxy, in the direction of the constellation of Sagittarius – home to a supermassive black hole that are otherwise hidden behind a dark shroud of dust clouds.

The newly released map reveals thousands of dense dust clumps, many never seen before, which mark the future birthplaces of massive stars.

The clumps are typically a couple of light-years in size, and have masses of between ten and a few thousand times the mass of our Sun. (ANI)

“Cosmic blobs” a result of growing supermassive black holes

Washington, June 25 (ANI): New data obtained from NASA’s Chandra X-ray Observatory and other telescopes has pinpointed the source of “cosmic blobs” as growing supermassive black holes.

This discovery helps resolve the true nature of gigantic blobs of gas observed around very young galaxies.

About a decade ago, astronomers discovered immense reservoirs of hydrogen gas, which they named “blobs”, while conducting surveys of young distant galaxies.

The blobs are glowing brightly in optical light, but the source of immense energy required to power this glow and the nature of these objects were unclear.

A long observation from Chandra has identified the source of this energy for the first time.

The X-ray data show that a significant source of power within these colossal structures is from growing supermassive black holes partially obscured by dense layers of dust and gas.

The fireworks of star formation in galaxies are also seen to play an important role, thanks to Spitzer Space Telescope and ground-based observations.

“For ten years, the secrets of the blobs had been buried from view, but now we’ve uncovered their power source,” said James Geach of Durham University in the United Kingdom, who led the study.

“Now, we can settle some important arguments about what role they played in the original construction of galaxies and black holes,” he added.

Galaxies are believed to form when gas flows inwards under the pull of gravity and cools by emitting radiation.

This process should stop when the gas is heated by radiation and outflows from galaxies and their black holes.

Blobs could be a sign of this first stage, or of the second.

Based on the new data and theoretical arguments, Geach and his colleagues show that heating of gas by growing supermassive black holes and bursts of star formation, rather than cooling of gas, most likely powers the blobs.

The implication is that blobs represent a stage when the galaxies and black holes are just starting to switch off their rapid growth because of these heating processes.

This is a crucial stage of the evolution of galaxies and black holes – known as “feedback” – and one that astronomers have long been trying to understand.

“We’re seeing signs that the galaxies and black holes inside these blobs are coming of age and are now pushing back on the infalling gas to prevent further growth,” said coauthor Bret Lehmer, also of Durham.

“Massive galaxies must go through a stage like this or they would form too many stars and so end up ridiculously large by the present day,” he added. (ANI)

NASA spacecraft detects ultra fast hydrogen coming from Moon

Washington, June 19 (ANI): NASA’s Interstellar Boundary Explorer (IBEX) spacecraft has made the first observations of very fast hydrogen atoms coming from the Moon, following decades of speculation and searching for their existence.

During spacecraft commissioning, the IBEX team turned on the IBEX-Hi instrument, built primarily by Southwest Research Institute (SwRI) and the Los Alamos National Laboratory, which measures atoms with speeds from about half a million to 2.5 million miles per hour.

Its companion sensor, IBEX-Lo, built by Lockheed Martin, the University of New Hampshire, NASA Goddard Space Flight Center, and the University of Bern in Switzerland, measures atoms with speeds from about one hundred thousand to 1.5 million mph.

“Just after we got IBEX-Hi turned on, the Moon happened to pass right through its field of view, and there they were,” said Dr. David J. McComas, IBEX principal investigator and assistant vice president of the SwRI Space Science and Engineering Division.

“The instrument lit up with a clear signal of the neutral atoms being detected as they backscattered from the Moon,” he added.

From its vantage point in space, IBEX sees about half of the Moon – one quarter of it is dark and faces the nightside (away from the Sun), while the other quarter faces the dayside (toward the Sun).

Solar wind particles impact only the dayside, where most of them are embedded in the lunar surface, while some scatter off in different directions.

The scattered ones mostly become neutral atoms in this reflection process by picking up electrons from the lunar surface.

The IBEX team estimates that only about 10 percent of the solar wind ions reflect off the sunward side of the Moon as neutral atoms, while the remaining 90 percent are embedded in the lunar surface.

Characteristics of the lunar surface, such as dust, craters and rocks, play a role in determining the percentage of particles that become embedded and the percentage of neutral particles, as well as their direction of travel, that scatter.

According to McComas, the results also shed light on the “recycling” process undertaken by particles throughout the solar system and beyond.

The solar wind and other charged particles impact dust and larger objects as they travel through space, where they backscatter and are reprocessed as neutral atoms.

These atoms can travel long distances before they are stripped of their electrons and become ions and the complicated process begins again.

The combined scattering and neutralization processes now observed at the Moon have implications for interactions with objects across the solar system, such as asteroids, Kuiper Belt objects and other Moons. (ANI)

Giant laser reactor aims to create nuclear fusion for first time

Washington, May 30 (ANI): A giant laser reactor has been unveiled in California, US, which scientists hope will accomplish nuclear fusion, the Holy Grail of energy sources, which was once thought impossible.

According to a report in Fox News, the National Ignition Facility at Lawrence Livermore National Laboratory will focus 192 laser beams on a hydrogen pellet the size of a bead, heating it to incredible temperatures in an attempt to recreate the power of the sun.

Nuclear fusion would create huge amounts of energy from tiny amounts of fuel. It would produce far less radioactive waste than conventional nuclear reactors.

But, it takes huge amounts of energy to trigger, and so far humans have managed to do so only by detonating atomic bombs.

“We have this big ball, right?” Ed Moses, program director of the National Ignition Facility, explained to Fox News. “And we hold our little targets inside of there, and the light focuses on there, and that’s where all the action happens,” he added.

The “action” aims to trigger a tiny thermonuclear explosion inside the huge target chamber, a blast sparked by the lasers, which bounce off a series of lenses and mirrors, intensifying and multiplying with each pass.

“Pretty soon, you have a lot of ‘em, and we have enough energy to drive our targets, to a point where they get to over 100 million degrees and it’s a pretty warm day,” said Moses.

Eventually turning ultraviolet, the beams push a million miles an hour toward the tiny hydrogen-fuel pellet in the center.

The resulting burst of energy should be so powerful, it could light up the entire country – but for only a split second.

“The facility is designed to do experiments that are confined within in the target chamber,” said project director Brian MacGowen.

“There has been a very thorough analysis of the potential impact of those experiments on the rest of the building and the community. They have all been reviewed extensively and the experiments are perfectly safe,” he added.

But, researchers here are confident their efforts will pay off – and be the game changer for meeting the world’s energy needs.

“It would change how we look at global warming. It would change pollution,” said Moses. “It would change all of those things. This is a small investment for that great payback,” he added. (ANI)

How oxidative stress may help extend lifespan

Washington, May 29 (ANI): Scientists at the University of California, San Diego claim to have identified a mechanism of oxidative stress that prevents cellular damage.

“We may drink pomegranate juice to protect our bodies from so-called ‘free radicals’ or look at restricting calorie intake to extend our lifespan,” said Dr Trey Ideker, chief of the Division of Genetics in the Department of Medicine at UC San Diego’s School of Medicine and professor of bioengineering at the Jacobs School of Engineering.

“But our study suggests why humans may actually be able to prolong the aging process by regularly exposing our bodies to minimal amounts of oxidants,” Ideker added.

Reactive oxygen species (ROS), ions that form as a natural byproduct of the metabolism of oxygen, play important roles in cell signalling. However, due to environmental stress like ultraviolet radiation or heat or chemical exposure the ROS levels can increase dramatically, resulting insignificant damage to cellular damage to DNA, RNA and proteins – cumulating in an effect called oxidative stress.

The scientists claim to have discovered the gene responsible for this effect.

One major contributor to oxidative stress is hydrogen peroxide. While the cell has ways to help minimize the damaging effects of hydrogen peroxide by converting it to oxygen and water, this conversion isn’t 100 percent successful.

During the study, the researchers designed a way to identify genes involved in adaptation to hydrogen peroxide.

To figure out which genes might control this adaptation mechanism, the team ran a series of experiments in which cells were forced to adapt while each gene in the genome was removed, one by one – covering a total of nearly 5,000 genes.

They identified a novel factor called Mga2, which is essential for adaptation.

“This was a surprise, because Mga2 is found at the control point of a completely different pathway than those which respond to acute exposure of oxidative agents,” said Ideker.

“This second pathway is only active at lower doses of oxidation,” Ideker added.

“It may be that adaptation to oxidative stress is the main factor responsible for the lifespan-expanding effects of caloric restriction,” said Ideker.

“Our next step is to figure out how Mga2 works to create a separate pathway – to discover the upstream mechanism that senses low doses of oxidation and triggers a protective mechanism downstream.”

The study is published in PLoS Genetics. (ANI)