NASA’s Swift satellite makes best-ever ultraviolet portrait of Andromeda galaxy

Washington, September 17 (ANI): NASA’s Swift satellite has acquired the highest-resolution view of a neighboring spiral galaxy ever attained in the ultraviolet.

The galaxy, known as M31 in the constellation Andromeda, is the largest and closest spiral galaxy to our own.

“Swift reveals about 20,000 ultraviolet sources in M31, especially hot, young stars and dense star clusters,” said Stefan Immler, a research scientist on the Swift team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

“Of particular importance is that we have covered the galaxy in three ultraviolet filters. That will let us study M31′s star-formation processes in much greater detail than previously possible,” he added.

M31, also known as the Andromeda Galaxy, is more than 220,000 light-years across and lies 2.5 million light-years away.

On a clear, dark night, the galaxy is faintly visible as a misty patch to the naked eye.

Between May 25 and July 26, 2008, Swift’s Ultraviolet/Optical Telescope (UVOT) acquired 330 images of M31 at wavelengths of 192.8, 224.6, and 260 nanometers.

The images represent a total exposure time of 24 hours.

The task of assembling the resulting 85 gigabytes of images fell to Erin Grand, an undergraduate student at the University of Maryland at College Park who worked with Immler as an intern this summer.

“After ten weeks of processing that immense amount of data, I’m extremely proud of this new view of M31,” she said.

Several features are immediately apparent in the new mosaic.

The first is the striking difference between the galaxy’s central bulge and its spiral arms.

“The bulge is smoother and redder because it’s full of older and cooler stars,” Immler explained. “Very few new stars form here because most of the materials needed to make them have been depleted,” he added.

Dense clusters of hot, young, blue stars sparkle beyond the central bulge.

M31′s disk and spiral arms contain most of the gas and dust needed to produce new generations of stars.

Star clusters are especially plentiful in an enormous ring about 150,000 light-years across.

“Swift is surveying nearby galaxies like M31 so astronomers can better understand star- formation conditions and relate them to conditions in the distant galaxies where we see gamma-ray bursts occurring,” said Neil Gehrels, the mission’s principal investigator at NASA Goddard. (ANI)

Climate change will lead to less ultraviolet radiation over northern high latitudes

Imphal, Sep.16 (ANI): “Move onward with the Lord within your heart and with the footprints of your ancestors in your eyes’ is the greatest moral teaching from Heigru Hidongba ceremony held every year in Manipur.

Heigru Hidongba, a socio-religious ceremony, to exhibit the firm devotion of the descendants of the Great Grand Mantri Anandashai of Lord Bejoy Govindajee was recently held in Imphal.

Devotees brought offerings of Heigru (Amla) fruit to the almighty on the 11th day of Langban Manipuri month which coincides with September to bring prosperity to the community.

During this festival a special boat race ‘Hiyang Tanaba’ is held in the sacred Thangapat Moat of Sagolband, Bejoy Govinda in Imphal amidst singing of devotional songs and a lot of clamour.

It attracted a huge number of spectators on this occasion. “We have organized the ceremony so that we can come and pray together so that the ills of the society will be removed and also for peace to be restored in our land that is filled with violence. In other places, it is celebrated anytime as a festival but we celebrate it as it is our custom,” said Boshana, organiser of the Heigru Hidongba festival.

“This is the 231st Heigru Hidongba Festival. The main theme of the festival is about preserving the age old traditional beliefs and customs of our culture,” said Magochandra, a local resident.

Devotees converged at the Bijoygobinda Moat at Sagoband to witness the ceremony symbolising the unity, which was once deeply rooted amongst the Manipuris’ ancestors and for their struggle for peace and freedom.

Devotees, today, believe that the ceremony brings prosperity to the State and overcomes ills of the society. (ANI)

Scientists unravel chemistry of Titan’s hazy atmosphere

Washington, September 16 (ANI): In a new research, a team of scientists has unraveled the chemical evolution of the orange-brownish colored atmosphere of Saturn’s moon Titan, the only solar system body besides Venus and Earth with a solid surface and thick atmosphere.

Scientists at University of Hawai’i at Manoa carried out the research.

The UH Manoa team, including Xibin Gu and Seol Kim, conducted simulation experiments mimicking the chemical reactions in Titan’s atmosphere utilizing crossed molecular beams in which the consequence of a single collision between molecules can be followed.

The team’s experiments indicate that triacetylene can be formed by a single collision of a “radical” ethynyl molecule and a diacetylene molecule.

An ethynyl radical is produced in Titan’s atmosphere by the photodissociation of acetylene by ultraviolet light.

Photodissociation is a process in which a chemical compound is broken down by photons.

“Surprisingly, the photochemical models show inconsistent mechanisms for the production of polyynes,” said Kaiser, who is the principal investigator of this study.

The mechanism involved in the formation of triacetylene, was also confirmed by accompanying theoretical calculations by Alexander Mebel, a theoretical chemist at Florida International University.

These theoretical computations also provide the 3D distribution of electrons in atoms and thus the overall energy level of a molecule.

To apply these findings to the real atmosphere of Titan, Danie Liang and Yuk Yung, planetary scientists at Taiwan’s Academia Sinica and California Institute of Technology (Caltech), respectively, performed photochemical modeling studies of Titan’s atmosphere.

All data together suggest that triacetylene may serve as a building block to form more complex and longer polyynes and produce potential precursors for the aerosol-based layers of haze surrounding Titan.

The study demonstrated for the first time that a sensible combination of laboratory simulation experiments with theory and modeling studies can shed light on decade old unsolved problems crucial to understand the origin and chemical evolution of the solar system.

The researchers hope to unravel next the mystery of the missing ethane lakes on Titan – postulated to exist for half a century, but not detected conclusively within the framework of the Cassini-Huygens mission.

In the future, the UH Manoa team will combine the research results with terrestrial-based observations of Titan’s atmosphere. (ANI)

Vitamin C can help protect DNA damage of skin cells

Washington, Sept 10 (ANI): Researchers at the University of Leicester and Institute for Molecular and Cellular Biology in Portugal have found that vitamin C can help protect DNA damage of skin cells and lead to better skin regeneration.

Previous research has shown that DNA repair is upregulated in people consuming vitamin C supplements.

In the new study, the researchers have provided some mechanistic evidence.

The researchers used affymetrix microarray, for looking at gene expression, and the ‘Comet’ assay to study DNA damage

“The exposure to solar ultraviolet radiation increases in summer, often resulting in a higher incidence of skin lesions. Ultraviolet radiation is also a genotoxic agent responsible for skin cancer, through the formation of free radicals and DNA damage,” said lead researcher Tiago Duarte, formerly of the University of Leicester, and now at the Institute for Molecular and Cellular Biology in Portugal.

“Our study analysed the effect of sustained exposure to a vitamin C derivative, ascorbic acid 2-phosphate (AA2P), in human dermal fibroblasts.

“We investigated which genes are activated by vitamin C in these cells, which are responsible for skin regeneration.

“The results demonstrated that vitamin C may improve wound healing by stimulating quiescent fibroblasts to divide and by promoting their migration into the wounded area. Vitamin C could also protect the skin by increasing the capacity of fibroblasts to repair potentially mutagenic DNA lesions,” Duarte added.

The researchers hope that the results will be of great relevance to the cosmetics industry.

“The study indicates a mechanism by which vitamin C could contribute to the maintenance of a healthy skin by promoting wound healing and by protecting cellular DNA against damage caused by oxidation,” said Dr Marcus S. Cooke from the Department of Cancer Studies and Molecular Medicine and Department of Genetics, at the University of Leicester.

“These findings are particular importance to our photobiology interests, and we will certainly be looking into this further,” Cooke added.

The findings have been published in the journal Free Radical Biology and Medicine. (ANI)

‘Laughing gas’ leaves ozone layer in splits

Washington, August 28 (ANI): A new study has determined that nitrous dioxide, popularly known as ‘laughing gas’, has now become the largest ozone-depleting substance emitted through human activities, and is expected to remain the largest throughout the 21st century.

The study was authored by A.R. Ravishankara, J.S. Daniel and Robert W. Portmann of the NOAA Earth System Research Laboratory (ESRL) chemical sciences division.

For the first time, this study has evaluated nitrous oxide emissions from human activities in terms of their potential impact on Earth’s ozone layer.

As chlorofluorocarbons (CFCs), which have been phased out by international agreement, ebb in the atmosphere, nitrous oxide will remain a significant ozone-destroyer, the study found.

Today, nitrous oxide emissions from human activities are more than twice as high as the next leading ozone-depleting gas.

Nitrous oxide is emitted from natural sources and as a byproduct of agricultural fertilization and other industrial processes.

Calculating the effect on the ozone layer now and in the future, NOAA researchers found that emissions of nitrous oxide from human activities erode the ozone layer and will continue to do so for many decades.

ESRL tracks the thickness of the ozone layer, as well as the burden of ozone-depleting compounds in the atmosphere. It maintains a large portion of the world air sampling and measurement network.

NOAA scientists also conduct fundamental studies of the atmosphere and atmospheric processes to improve understanding of ozone depletion and of the potential for recovery the ozone layer.

“The dramatic reduction in CFCs over the last 20 years is an environmental success story. But manmade nitrous oxide is now the elephant in the room among ozone-depleting substances,” said Ravishankara, lead author of the study and director of the ESRL Chemical Sciences Division in Boulder, Colorado.

The ozone layer serves to shield plants, animals and people from excessive ultraviolet light from the sun.

Thinning of the ozone layer allows more ultraviolet light to reach the Earth’s surface where it can damage crops and aquatic life and harm human health.

Though the role of nitrous oxide in ozone depletion has been known for several decades, the new study is the first to explicitly calculate that role using the same measures that have been applied to CFCs, halons and other chlorine- and bromine-containing ozone-depleting substances.

According to scientists, nitrous oxide is also a greenhouse gas, so reducing its emission from manmade sources would be good for both the ozone layer and climate. (ANI)

Stressed crops emit more methane emissions than previously thought

Washington, August 18 (ANI): Scientists at the University of Calgary (U of C) in Canada have found that methane emission by stressed crops could be a bigger problem in global warming than previously thought.

According to a U of C study, when crops are exposed to environmental factors that are part of climate change – increased temperature, drought and ultraviolet-B radiation – some plants show enhanced methane emissions.

Methane is a very potent greenhouse gas; 23 times more effective in trapping heat than carbon dioxide (CO2).

“Most studies just look at one factor. We wanted to mix a few of the environmental factors that are part of the climate change scenario to study a more true-to-life impact climate change has on plants,” said David Reid, a professor in the Department of Biological Sciences, who co-authored a paper with research associate Mirwais Qaderi in the advanced on-line edition of the journal Physiologia Plantarum.

Reid and Qaderi analyzed methane emissions from six important Canadian crops – faba bean, sunflower, pea, canola, barley and wheat – that were exposed to combinations of three components of global climate change: temperature, ultraviolet-B radiation and water stress (drought).

What they found was troubling.

These stresses caused plants to emit more methane. In a warmer, drier world, methane might be a bigger contributor in global warming than previously thought.

When it comes to the greenhouse effect, methane could be considered the misunderstood and often overlooked orphan greenhouse gas.

Much of the attention has been focused on carbon dioxide, but more recently it has been realized that methane should also be considered as a very significant greenhouse gas.

Its concentrations have more than doubled since pre-industrial times.

While the growth rate of methane concentrations has slowed since the early 1990s, some scientists say this is only a temporary pause.

“Our results are of importance in the whole climate warming discussion because methane is such a potent greenhouse warming gas,” said Qaderi.

“It points to the possibility of yet another possible feedback phenomena which could add to global warming,” 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)

New handheld device detects anthrax with outstanding accuracy and reliability

Washington, June 26 (ANI): Scientists have developed a handheld device that can detect anthrax with outstanding accuracy and reliability.

The device, called Ceeker (pronounced “seeker”), was made by scientists at Veritide Ltd., a developer of innovative biological identification and detection solutions.

It can discriminate between anthrax spores and similar-looking hoax substances.

The data show that in over two weeks of testing at the Midwest Research Institute in Florida, the company’s Ceeker scanner accurately identified 100 percent of the anthrax samples used and was correct in 95 percent of tests involving hoax substances.

“We knew that our innovative Ceeker is capable of producing outstanding results in distinguishing between anthrax and look-alike hoax substances, and now we have definitive data confirming its performancem,” said Andrew Rudge, Chief Executive Officer of Veritide.

“Even better, these extraordinary results were generated by a small portable handheld system that requires no special skills or training to operate and that can produce a result within minutes, enabling first responders to rapidly determine whether the situation is a nuisance or a major threat to public health,” he added.

The Ceeker employs optical detection technology developed at New Zealand’s University of Canterbury.

It uses ultraviolet light and special algorithms to detect bacterial spores and provides test results within minutes, without the need for wet chemistry or analytic processes that can be difficult to handle in the field.

The Ceeker is capable of producing test results from very small amounts of sample and does not consume or destroy the sample being tested, allowing it to be re-analyzed later for forensic applications.

In contrast, existing detection approaches require longer and more complex processing to distinguish anthrax from other substances (between 30 minutes and three days). Their accuracy is inferior to the Ceeker and the sample is typically destroyed during testing.

According to Professor Lou Reinisch, an inventor of the Ceeker technology, “These new data definitively confirm the validity of the detection concepts underlying the Ceeker and should help fuel its wider use among such first responders as fire and police departments, HazMat teams, postal services, port and airport security, and defense and military authorities.”

The Ceeker has also been previously validated by forensic laboratory ESR, which conducted multiple rounds of testing using anthrax simulants and hoax substances.

The successful US test results have triggered significant sales from US customers who had pre-ordered the Ceeker but were waiting for positive direct anthrax testing results before proceeding. (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)

Satellites’ launch to give boost to NASA’s ‘return to Moon’ mission

Washington, May 22 (ANI): NASA’s return to the moon will get a boost in June with the launch of two satellites that will return a wealth of data about Earth’s nearest neighbor.

On May 21, the agency outlined the upcoming missions of the Lunar Reconnaissance Orbiter, or LRO, and the Lunar Crater Observation and Sensing Satellite, or LCROSS.

The spacecraft will launch together June 17 aboard an Atlas V rocket from Cape Canaveral Air Force Station in Florida.

Using a suite of seven instruments, LRO will help identify safe landing sites for future human explorers, locate potential resources, characterize the radiation environment and test new technology.

LCROSS will seek a definitive answer about the presence of water ice at the lunar poles.

It will use the spent second stage Atlas Centaur rocket in an unprecedented way that will culminate with two spectacular impacts on the moon’s surface.

“These two missions will provide exciting new information about the moon, our nearest neighbor,” said Doug Cooke, associate administrator of NASA’s Exploration Systems Mission Directorate in Washington.

“Imaging will show dramatic landscapes and areas of interest down to one-meter resolution. The data also will provide information about potential new uses of the moon. These teams have done a tremendous job designing and building these two spacecraft,” he added.

LRO’s instruments will help scientists compile high resolution, three-dimensional maps of the lunar surface and also survey it in the far ultraviolet spectrum.

The satellite’s instruments will help explain how the lunar radiation environment may affect humans and measure radiation absorption with a plastic that is like human tissue.

LRO’s instruments also will allow scientists to explore the moon’s deepest craters, look beneath its surface for clues to the location of water ice, and identify and explore both permanently lit and permanently shadowed regions.

High-resolution imagery from its camera will help identify landing sites and characterize the moon’s topography and composition.

A miniaturized radar will image the poles and test the system’s communications capabilities.

“LRO is an amazingly sophisticated spacecraft,” said Craig Tooley, LRO project manager at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

“Its suite of instruments will work in concert to send us data in areas where we’ve been hungry for information for years,” he added. (ANI)

Child’s ghostly image caught on new spirit-catching camera

London, May 13 (ANI): British spook hunter Paul Rowland has revealed that he might have invented a device by which he can capture spirits on camera, especially after he captured the ghostly image of a child with it.

The instrument works by using ultraviolet and infrared lights to enhance images other cameras miss, and the chilling discovery was made while taking a picture with the camera at the Welsh mansion he was working in.

“You can see a child-like figure and what appears to be an arm reaching out towards me,” the Sun quoted him as saying.

“I was standing with my back against the window ledge, just a metre away.

“This picture is my prized-possession,” he said.

The eerie shape was spotted at the haunted Plas Teg mansion, which is popular with paranormal groups, and 49-year-old Rowland said that he developed the gadget after watching TV shows like Most Haunted.

“I used to shout at the screen ‘why don’t you use this, or that’,” he said.

“But when I researched I found the technologies simply didn’t exist – so I started inventing them.

“The equipment I build is specifically for the purpose of paranormal investigations, unlike the borrowed technology used by other investigators.

“My belief is it will take new technology to reveal new evidence,” he added.

Rowland’s ghost-cam device is yet to get a proper name.

“The idea came about because I wanted to be able to carry technology around in one unit,” he said.

“I use blue and ultraviolet lights to enhance our capability in the dark.

“It also has a digital stills camera and camcorder – both of which can see in ultraviolet light.

“And there’s a live EVP (electronic voice phenomenon) system hooked up to it.

“With all great respect to mediums, nobody else can hear what’s going on.

“But I believe my devices can – through feedback – let people hold yes/no conversations with the dead.

“It’s almost as if the machine senses an energy build-up in the room and records it,” he added.

Rowland will be leading an investigation called The Paradox Experience in Scotland running until May 17. (ANI)

Sun’s new solar cycle will be weakest since 1928

London, May 11 (ANI): A panel of international experts has predicted that the Sun’s new solar cycle, which is thought to have begun in December 2008, will be the weakest since 1928.

Solar activity waxes and wanes every 11 years.

Cycles can vary widely in intensity, and there is no foolproof way to predict how the sun will behave in any given cycle.

In 2007, an international panel of 12 experts split evenly over whether the coming cycle of activity, dubbed Cycle 24, would be stronger or weaker than average.

The group did agree the sun would probably hit the lowest point in its activity in March 2008 before ramping up to a new cycle that would reach its maximum in late 2011 or mid-2012.

But, the sun did not bear out those predictions.

Instead, it entered an unexpectedly long lull in activity with few new sunspots. It is thought to have reached its minimum in December 2008, and now seems to be slowly waking up.

According to a report in New Scientist, one such sign is two new active regions captured this week by the ultraviolet camera on one of NASA’s twin STEREO probes.

“There’s a lot of indicators that Cycle 24 is ready to burst out,” said panel chair Doug Biesecker of the National Oceanic and Atmospheric Administration Space Weather Prediction Center in Boulder, Colorado.

The panel now expects the sun’s activity will peak about a year late, in May 2013, when it will boast an average of 90 sunspots per day.

That is below average for solar cycles, making the coming peak the weakest since 1928, when an average of 78 sunspots was seen daily.

Sunspots are Earth-sized blotches that coincide with knotty magnetic fields. They are a common measure of solar activity.

The higher the number of sunspots, the higher the probability of a major storm that could wreak havoc on Earth.

A lower number of sunspots could mean space weather will be relatively mild in the coming years. (ANI)

The “fashionable way” to stave off skin cancer

Washington, May 5 (ANI): Just applying sunscreen doesn’t guarantee full protection in the summer, and thus researchers have now offered insight into how some of today’s hottest fashion trends can help play it safe in the sun without leaving you feeling like a well-greased baking pan.

Dr. Susan Y. Chon, assistant professor in The University of Texas M. D. Anderson’s Department of Dermatology, has explained how the hottest trends from the spring/summer 2009 runway shows also can provide skin cancer prevention and maximize clothing’s sun protection power.

Sunglasses:

The most fabulous, current sunglass styles are those with extra-large frames that help protect the delicate skin around the eyes from skin cancer and aging. Sunglasses also should have broad ultraviolet (UV) protection that absorbs at least 99 percent of UV rays for maximum cancer prevention benefits.

Leggings:

Leggings have now become a runway staple and can go under dresses and tunics even in hot weather because they aren’t as heavy as pants. They are a great way to defend legs from UVA and UVB rays while running errands or at an outdoor barbeque.

Long Dresses:

Another leg-saving fashion trend that is extremely popular on the runways for spring/summer 2009 is the move from “mini” to “maxi”-long dresses are everywhere, and are being worn for day and night.

Hats:

Modern, wide-brimmed sun hats shield the face, neck, ears and chest from the sun. The trend this season on the runway-the bigger the brim, the better! Sun hats also should be tightly woven.

Tunic Tops:

Pretty, “boho” style beach cover-ups with long sleeves are a great way to save a person’s skin from being over exposed in a teeny-bikini. Tunic tops are not only perfect on the beach but also can transition from day to night when worn with the right accessories, like chunky bracelets, necklaces and belts.

Scarves:

Summery shawls and scarves in lightweight fabrics are back again this season.

“Women are usually pretty good about applying sunscreen to their face, but generally forget their necks and the ‘v’ of their chests. A light scarf is a great way to cover neglected skin that gets a lot of sun exposure during summer months,” said Chon.

One Piece Bathing Suits:

The new trend of one-piece bathing suits gives skin on the stomach an extra layer of protection. One-piece suits also provide more coverage of the lower back, an area often missed while applying sunscreen.

Maximize clothing’s sun protection power

“There are certain colours and fabrics that will offer more protection than others,” said Chon.

To maximize clothing’s skin cancer prevention powers, wear tightly woven, dark-coloured fabrics.

“You don’t need to wear special UPF clothing to get extra protection, just wear a sunscreen with SPF15 or higher under layers. It is absolutely possible to be fashion conscious and protect yourself from the sun. The trends on the runway this year offer more coverage. We love that! Said Chon. (ANI)

Asteroids age quickly because of a ‘sun tan’

Munich, April 23 (ANI): A new study has revealed that asteroid surfaces age and redden much faster than previously thought – in less than a million years, all thanks to solar winds.

“Asteroids seem to get a ‘sun tan’ very quickly,” said lead author Pierre Vernazza. “But not, as for people, from an overdose of the Sun’s ultraviolet radiation, but from the effects of its powerful wind,” he added.

It has long been known that asteroid surfaces alter in appearance with time.

The observed asteroids are much redder than the interior of meteorites found on Earth, but the actual processes of this “space weathering” and the timescales involved were controversial.

Thanks to observations of different families of asteroids using ESO’s New Technology Telescope at La Silla and the Very Large Telescope at Paranal, as well as telescopes in Spain and Hawaii, Vernazza’s team have now solved the puzzle.

When two asteroids collide, they create a family of fragments with “fresh” surfaces.

The astronomers found that these newly exposed surfaces are quickly altered and change color in less than a million years – a very short time compared to the age of the Solar System.

“The charged, fast moving particles in the solar wind damage the asteroid’s surface at an amazing rate,” said Vernazza.

Unlike human skin, which is damaged and aged by repeated overexposure to sunlight, it is, perhaps rather surprisingly, the first moments of exposure (on the timescale considered) – the first million years – that causes most of the aging in asteroids.

By studying different families of asteroids, the team has also shown that an asteroid’s surface composition is an important factor in how red its surface can become.

After the first million years, the surface “tans” much more slowly. At that stage, the color depends more on composition than on age.

Moreover, the observations reveal that collisions cannot be the main mechanism behind the high proportion of “fresh” surfaces seen among near-Earth asteroids.

Instead, these “fresh-looking” surfaces may be the results of planetary encounters, where the tug of a planet has “shaken” the asteroid, exposing unaltered material.

Thanks to these results, astronomers will now be able to understand better how the surface of an asteroid, which often is the only thing we can observe, reflects its history. (ANI)

Berries may help keep wrinkles at bay

Washington, Apr 22 (ANI): The latest beauty cream that can be added in a woman’s skin care regimen can be found in berries. A new study has found that an antioxidant present in the fruit could help fight skin damage due to ultraviolet (UV) rays.

Using a topical application of the antioxidant ellagic acid, researchers at Hallym University in the Republic of Korea markedly prevented collagen destruction and inflammatory response – major causes of wrinkles – in both human skin cells and the sensitive skin of hairless mice following continuing exposure to UV-B, the sun’s skin-damaging ultraviolet radioactive rays.

Ji-Young Bae, a graduate student in the laboratory of Dr. Young-Hee Kang, presented results of the two-part study on April 21, at the Experimental Biology 2009 meeting in New Orleans. The presentation was part of the scientific program of the American Society for Nutrition.

Ellagic acid is an antioxidant found in numerous fruits, vegetables and nuts, especially raspberries, strawberries, cranberries and pomegranates. Earlier studies have suggested it has a photoprotective effect.

The Kang laboratory found that, in human skin cells, ellagic acid worked to protect against UV damage by blocking production of MMP (matrix metalloproteinase enzymes that break down collagen in damaged skin cells) and by reducing the expression of ICAM (a molecule involved in inflammation).

The scientists then turned to young (four weeks), male, hairless mice – genetically bred types of mice often used in dermatology studies because of the physiological similarities of their skin to that of humans. For eight weeks, the 12 mice were exposed to increasing ultraviolet radiation, such as that found in sunlight, three times a week, beginning at a level sufficient to cause redness or sunburn and increasing to a level that would have definitely caused minor skin damage to human skin.

During these eight weeks, half of the exposed mice were given daily 10 microM topical applications of ellagic acid on their skin surface, even on the days in which they did not receive UV exposure. The other mice, also exposed to UV light, did not receive ellagic acid.

Following the analyses, the mice exposed to UV radiation without the ellagic acid treatment developed wrinkles and thickening of the skin, the researchers found.

Second, as hypothesized, the exposed mice that received topical application of ellagic acid showed reduced wrinkle formation.

Third, as suggested in the study of human cells, the ellagic acid reduced inflammatory response and MMP secretion due to protection from the degradation of collagen. The ellagic acid also helped prevent an increase of epidermal thickness.

The researchers say the results demonstrate that ellagic acid works to prevent wrinkle formation and photo-aging caused by UV destruction of collagen and inflammatory response. (ANI)

Space “aerobrakes” could bring used rockets back to Earth safely

London, April 18 (ANI): Scientists are working on ways to build a gossamer-thin space sail or “aerobrake” that would help bring back a used rocket back to Earth safely.

According to a report in New Scientist, space-flight engineers Max Cerf and Brice Santerre at the European aerospace firm EADS Astrium have put the idea forward.

Rocket stages are a particular risk to spacecraft because they often contain large amounts of unused fuel, which can explode when sunlight heats the tank. Leaking fuel can also act like a mini-thruster, pushing the rocket into an orbit where it may cause a collision.

One way to tackle the problem is to vent unused fuel in a controlled way, and drain power from the battery, but this is unlikely to eliminate all collisions.

Now, Cerf and Santerre are devising ways to build a sail that would quickly remove a spent rocket from orbit.

The sail or “aerobrake” would be deployed after a rocket has delivered its satellite into low-Earth orbit, slowing it down by friction with the thin atmosphere so that burns up in around 25 years, much earlier than conventional rocket stages, some of which are expected to survive for at least 100 years.

The aerobrake would be deployed after the rocket has delivered its satellite into low-Earth orbit.

For the final stage of an Ariane 5 launcher, the conical sail would need to have an area of about 350 square metres and be supported by an inflatable mast 12 meters long.

Cerf and Santerre propose a number of possible ways to build the mast.

The simplest envisages a woven polymer and aluminium tube that is kept inflated by nitrogen gas.

Another uses a tube made of polymer composite, which after being inflated with nitrogen is set hard by the sun’s ultraviolet rays. A third design uses epoxy resin that is set hard by solvent evaporation.

The pair revealed their designs at this month’s Fifth European Conference on Space Debris in Darmstadt, Germany, organised by the European Space Agency.

According to Peter Roberts, a space-flight engineer at Cranfield University in the UK, who is working on similar technology for small satellites, “It’s a good idea, says Peter Roberts, a space-flight engineer at Cranfield University in the UK.”

“The risk of fragmentation of end-of-life spacecraft due to impacts from other debris can be greatly reduced by deploying a drag sail,” he said. (ANI)

New technique shrinks size of circuitry used in nanotechnology devices

Washington, April 17 (ANI): A University of Colorado at Boulder team, US, has developed a new method of shrinking the size of circuitry used in nanotechnology devices like computer chips and solar cells by using two separate colors of light.

Like current methods in the nanoengineering field, one color of light inscribes a pattern on a substrate, according to CU-Boulder Assistant Professor Robert McLeod of the electrical, computer and energy engineering department.

But, the new system developed by McLeod’s team uses a second color to “erase” the edges of the pattern, resulting in much smaller structures.

“The team used tightly focused beams of blue light to record lines and dots thousands of times smaller than the width of a human hair into patterned lithography on a substrate,” said McLeod.

The researchers then “chopped off the edges” of the lines using a halo of ultraviolet light, trimming the width of the lines significantly.

“We are essentially drawing a line with a marker on a nanotechnology scale and then erasing its edges,” said McLeod.

The method offers potential new approaches in the search for ways to shrink transistor circuitry, a process that drives the global electronic market that is pursuing smaller, more powerful microchips, he added.

For the project, McLeod and his team used a tabletop laser to project tightly focused beams of visible blue light onto liquid molecules known as monomers.

A chemical reaction initiated a bonding of the monomers into a plastic-like polymer solid.

If the beam was focused in one place, it inscribed a small solid dot. If the beam was moving the focus through the material, it created a thin thread, or line.

The researchers then added a second ultraviolet laser focused into a halo, or donut, which surrounded the blue light.

The special monomer formulation was designed to be inhibited by the UV light, shutting down its transformation from a liquid to a solid.

This “halo of inhibition” prevented the edges of the spot or line from developing, resulting in a much finer final structure.

According to McLeod, the new technology has the potential to lead to the construction of a variety of nanotechnology devices, including “nanomotors”.

“We now have a set of new tools. We believe this is a new way to do nanotechnology,” he said. (ANI)

Planets around cool suns have different mix of life-forming chemicals

Washington, April 8 (ANI): A new study from NASA’s Spitzer Space Telescope hints that planets around stars cooler than our Sun might possess a different mix of potentially life-forming, or “prebiotic,” chemicals.

Astronomers used Spitzer to look for a prebiotic chemical, called hydrogen cyanide, in the planet-forming material swirling around different types of stars.

Hydrogen cyanide is a component of adenine, which is a basic element of DNA.

The researchers detected hydrogen cyanide molecules in disks circling yellow stars like our Sun – but found none around cooler and smaller stars, such as the reddish-colored “M-dwarfs” and “brown dwarfs” common throughout the universe.

“Prebiotic chemistry may unfold differently on planets around cool stars,” said Ilaria Pascucci, lead author of the new study from Johns Hopkins University, Baltimore, Maryland.

Young stars are born inside cocoons of dust and gas, which eventually flatten to disks.

Dust and gas in the disks provide the raw material from which planets form. Scientists think the molecules making up the primordial ooze of life on Earth might have formed in such a disk.

Prebiotic molecules, such as adenine, are thought to have rained down to our young planet via meteorites that crashed on the surface.

“It is plausible that life on Earth was kick-started by a rich supply of molecules delivered from space,” said Pascucci.

But, could the same life-generating steps take place around other stars?

Pascucci and her colleagues addressed this question by examining the planet-forming disks around 17 cool and 44 Sun-like stars using Spitzer’s infrared spectrograph, an instrument that breaks light apart, revealing signatures of chemicals.

The stars are all about one to three million years old, an age when planets are thought to be growing.

The astronomers specifically looked for ratios of hydrogen cyanide to a baseline molecule, acetylene.

They found that the cool stars, both the M-dwarf stars and brown dwarfs, showed no hydrogen cyanide at all, while 30 percent of the Sun-like stars did.

“Perhaps ultraviolet light, which is much stronger around the Sun-like stars, may drive a higher production of the hydrogen cyanide,” said Pascucci.

The team did detect their baseline molecule, acetylene, around the cool stars, demonstrating that the experiment worked.

This is the first time that any kind of molecule has been spotted in the disks around cool stars.

The findings have implications for planets that have recently been discovered around M-dwarf stars. (ANI)

Gamma-ray burst may have caused mass extinction 440 million years ago

Washington, April 4 (ANI): A new study has suggested that a brilliant burst of gamma rays may have caused a mass extinction event on Earth 440 million years ago, and a similar celestial catastrophe could happen again in the future.

Most gamma-ray bursts are thought to be streams of high-energy radiation produced when the core of a very massive star collapses.
According to a report in National Geographic News, the new computer model shows that a gamma-ray burst aimed at Earth could deplete the ozone layer, cause acid rain, and initiate a round of global cooling from as far as 6,500 light-years away.

Such a disaster may have been responsible for the mass die-off of 70 percent of the marine creatures that thrived during the Ordovician period (488 to 443 million years ago), suggests study leader Brian Thomas, an astrophysicist at Washburn University in Kansas.

The simulation also shows that a significant gamma-ray burst is likely to go off within range of Earth every billion years or so, although the stream of radiation would have to be lined up just right to affect the planet.

Currently WR104, a massive star 8,000 light-years away in the constellation Sagittarius, is in position to be a potential threat, according to Thomas.

Study author Thomas’ former graduate advisor, Adrian Melott, first proposed in 2004 that a gamma-ray burst near Earth wiped out Ordovician life.

Since then, both researchers have been tackling pieces of the puzzle.

According to their newest models, gamma radiation from a nearby burst would quickly deplete much of Earth’s protective ozone layer, allowing increased ultraviolet radiation (UV) from the sun to reach the surface.

In the longer term, chemical reactions in the atmosphere would produce dark, nitrogen-based gases that would block the sun’s heat and trigger global cooling, even as the gamma rays continued to deplete ozone and let in UV rays, the authors suggesedt.

Some of the pollution would fall as damaging acid rain, which can severely disrupt ecosystems.

The atmosphere might be able to recover within a decade, and a rise in DNA damage caused by increased UV exposure might pass after a few months or years, the researchers note.

“But other biological impacts-such as reduced ocean productivity-could linger for an unknown length of time,” Thomas said. (ANI)