Planck spacecraft obtains first peek of big bang’s ‘afterglow’

London, September 18 (ANI): European Space Agency’s (ESA’s) Planck spacecraft has obtained its first peek at the afterglow of the big bang, revealing it in unprecedented detail.

The ESA spacecraft was launched into space on May 14 this year. It is observing the glow of hot gas from just 380,000 years after the big bang, called the cosmic microwave background (CMB).

According to a report in New Scientist, the detailed properties of this background may contain hints of hidden extra dimensions or multiple universes, as well as providing clues to what caused a brief, early period of incredibly rapid cosmic expansion.

Planck began surveying the microwave background on August 13, a few weeks after reaching its planned perch 1.5 million kilometres from Earth at a point called L2 and cooling its detectors to within 0.1 degrees Celsius above absolute zero.

Now, the Planck team has released the probe’s first image, an observational strip covering about 5 per cent of the sky.

Slight variations in temperature from place to place in the early universe give the image its mottled appearance.

“With a few per cent of the data in, you can see it’s working well and delivering good stuff,” said team member George Efstathiou of the University of Cambridge.

Planck is expected to provide the most detailed all-sky map of the cosmic microwave background yet, improving on the best current map, obtained by NASA’s Wilkinson Microwave Anisotropy Probe (WMAP), which launched in 2001.

Planck’s detectors have more than 10 times the sensitivity of WMAP’s, and about 2.5 times the angular resolution.

“Every strip that Planck scans, we’re getting data that is many, many times more sensitive than WMAP,” Efstathiou told New Scientist.

Although Planck was only designed to observe the sky for 15 months, the team believes it could last for more than 30 months, based on new estimates of how long its coolant will last.

The extra time will allow Planck to measure the radiation with even greater precision, since it will scan the entire sky four times – two more than originally planned. (ANI)

Iggy Pop to be honoured with living legend award

London, September 16 (ANI): Iggy Pop, often referred to as “the Godfather of Punk”, is set to be honoured with a living legend trophy at the Marshall Classic Rock Roll of Honour awards.

The rocker and former lead singer of ‘The Stooges’ will join previous recipients including Ozzy Osbourne, Jimmy Page and Alice Cooper on November 2 in London.

“All those years of banging away in the dives and palaces of the weird universe of rock are finally adding up to something,” the BBC quoted him as saying.

“The other people who have received this award are absolutely awesome, and I feel very lucky to be included,” he added.

Readers of Classic Rock magazine will vote for other awards at the ceremony. (ANI)

New model of quantum gravity may rewrite Einstein’s theory of general relativity

Washington, August 25 (ANI): Scientists at Texas A and M University in the US have developed a controversial new model of quantum gravity, which might reproduce Albert Einstein’s theory of general relativity.

The theory, which Einstein developed in the early 20th century, says that matter curves spacetime, and it is this curvature which deflects massive bodies – an effect that we interpret as the influence of gravity.

The theory has been tested to extremely high accuracy and without it, our satellite global positioning system would be off by about 10 km per day.

Despite the success of general relativity, one of the most important problems in modern physics is finding a theory of quantum gravity that reconciles the continuous nature of gravitational fields with the inherent ‘graininess’ of quantum mechanics.

Recently, Petr Horava at Lawrence Berkeley Lab proposed such a model for quantum gravity that has received widespread interest, in no small part because it is one of the few models that could be experimentally tested.

In Horava’s model, Lorentz symmetry, which says that physics is the same regardless of the reference frame, is violated at small distance scales, but remerges over longer distance scales

The team at Texas A and M, which includes Hong Lu, Jianwei Mei and Christopher Pope, report their investigations into how the modifications proposed in Horava’s theory will broadly affect the solutions of general relativity.

Lu and his team’s calculations suggest that Horava’s model only reproduces general relativity on unobservable scales, “larger than the size of the Universe”.

The research team’s paper is an important contribution to testing the Horava model and shows that a good deal of work remains to understand its full implications. (ANI)

Most scientifically accurate and advanced planetarium show on display in US

Washington, August 21 (ANI): High-performance computing systems, visualization resources, and software tools provided by the National Science Foundation TeraGrid helped make the Hayden Planetarium’s new space show the most scientifically accurate and advanced planetarium show ever produced.

The Hayden Planetarium is a public planetarium located on Central Park West, New York City, next to and organizationally part of the American Museum of Natural History.

“Journey to the Stars,” which debuted this summer at the American Museum of Natural History, is being hailed as the most beautiful planetarium show to date.

Narrated by Whoopi Goldberg, the 25-minute presentation takes viewers on a journey through the universe.

The space show projects cutting-edge visualizations of the universe onto the 87-foot, seven-million-pixel dome of the museum’s Hayden Sphere at the Rose Center for Earth and Space in New York City.

Piecing together a new narrative of life’s origins, the space show explains how dark matter’s gravity gathered the primordial gas in the universe to form the first stars, and how these massive stars exploded, seeding the galaxy with new stars and the chemical elements that made life possible.

The centerpiece of the show, and the most difficult sequence to depict scientifically, is a flight into the center of the Sun.

The visuals of the Sun were produced using supercomputing resources provided by the NSF TeraGrid, a national cyberinfrastructure for open scientific research.

According to Ro Kinzler, the show’s producer, “We wanted to treat the Sun in a terrific and powerful way to [not just] reveal the surface, but to take our audience into the Sun, through the convective layer and into the core.”

“The results are beautiful. No one has seen the Sun in this way, and the software from NCAR and computational resources from TACC made it possible,” he said.

The visual sequences are based on the research of Juri Toomre, a professor of astrophysics at the University of Colorado at Boulder, and run on TACC’s Ranger supercomputer.

“It’s not enough to know what comes out of the surface,” Toomre said.

“We would like to understand how the magnetic engine of a star works, how it churns away and how it builds orderly fields. This is one of the top 10 questions in physics,” Toomre added.

“A very dramatic moment in the show is when we actually peel away the surface of the Sun, revealing the dynamic convective motion below,” Kinzler said. “We take the audience through the convective region and into the Sun’s core,” he added. (ANI)

Dark energy may not actually exist

London, August 18 (ANI): A new research by scientists has claimed that dark energy – the mysterious substance thought to make up three-quarters of the universe – may not actually exist.

The concept of dark energy was created by cosmologists to fit Albert Einstein’s General Theory of Relativity into reality after modern space telescopes discovered that the Universe was not behaving as it should.

According to Einstein’s work, the speed at which the Universe is expanding following the Big Bang should be slower than it actually is and this unexplained anomaly threatened to turn the whole theory upside down.

In order to reconcile this problem, the concept of dark energy was invented.

But now, according to a report in the Telegraph, Blake Temple and Joel Smoller, mathematicians at the University of California and the University of Michigan, believe they have come up with a whole new set of calculations that allow for all the sums to add up without the need for this controversial substance.

The research could change the way astronomers view the composition of our Universe, as it may prove that dark energy doesn’t exist at all.

The Standard Model of Cosmology, which describes the evolution of the Universe, begins with the Big Bang.

Astronomers have recently observed that the galaxies are accelerating as they move away from each other, and cosmologists have sought to explain this unexpected acceleration by introducing the concept of dark energy, which permeates space, propels matter, and accounts for nearly 75 percent of the mass-energy in our Universe.

The new research is likely to be equally controversial as the work it purports to challenge especially as it relies on our galaxy being at the centre of the Universe – a concept that has been generally disregarded in modern science.

According to Dr Malcom Fairbairn, particle cosmologist at King’s College London, “Ever since the concept of dark energy was first mentioned, people have been trying to explain it or explain it away. It is a mystery and an inconvenience.”

“This is one attempt at it. Whether it is right only time will tell,” he said. (ANI)

NASA scientists make first discovery of life’s building block in comet

Washington, August 18 (ANI): NASA scientists have discovered glycine, a fundamental building block of life, in samples of comet Wild 2 returned by NASA’s Stardust spacecraft.

“Glycine is an amino acid used by living organisms to make proteins, and this is the first time an amino acid has been found in a comet,” said Dr. Jamie Elsila of NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

“Our discovery supports the theory that some of life’s ingredients formed in space and were delivered to Earth long ago by meteorite and comet impacts,” he added.

“The discovery of glycine in a comet supports the idea that the fundamental building blocks of life are prevalent in space, and strengthens the argument that life in the universe may be common rather than rare,” said Dr. Carl Pilcher, Director of the NASA Astrobiology Institute, which co-funded the research.

Stardust passed through dense gas and dust surrounding the icy nucleus of Wild 2 on January 2, 2004.

As the spacecraft flew through this material, a special collection grid filled with aerogel – a novel sponge-like material that’s more than 99 percent empty space – gently captured samples of the comet’s gas and dust.

The grid was stowed in a capsule, which detached from the spacecraft and parachuted to Earth on January 15, 2006.

Since then, scientists around the world have been busy analyzing the samples to learn the secrets of comet formation and our solar system’s history.

“We actually analyzed aluminum foil from the sides of tiny chambers that hold the aerogel in the collection grid,” said Elsila.

“As gas molecules passed through the aerogel, some stuck to the foil. We spent two years testing and developing our equipment to make it accurate and sensitive enough to analyze such incredibly tiny samples,” he added.

Earlier, preliminary analysis in the Goddard labs detected glycine in both the foil and a sample of the aerogel.

However, since glycine is used by terrestrial life, at first the team was unable to rule out contamination from sources on Earth.

The new research used isotopic analysis of the foil to rule out that possibility.

“We discovered that the Stardust-returned glycine has an extraterrestrial carbon isotope signature, indicating that it originated on the comet,” said Elsila.

According to Dr. Daniel Glavin of NASA Goddard, “Based on the foil and aerogel results it is highly probable that the entire comet-exposed side of the Stardust sample collection grid is coated with glycine that formed in space.” (ANI)

World’s largest and most technologically advanced telescope to debut on July 24

Washington, July 14 (ANI): The world’s largest, most technologically advanced telescope is all set to make its formal debut on July 24 in Spain’s Canary Islands.

Known as the Gran Telescopio Canarias, the telescope has a 10.4-meter diameter mirror, and has more light-collecting area than any other telescope.

Perched 7,874 feet above sea level on a mountain on the island of La Palma, the GTC has 6 square meters more light collecting area than any of the roughly one dozen 8- to 10-meter telescopes worldwide.

With a mirror composed of 36 hexagonal segments thought to have the smoothest surfaces ever made, it is also the world’s most technologically advanced optical telescope.

Sensors keep the mirrors aligned to counteract the force of gravity, with the result that they act as a single surface, even as the telescope is rotated and aligned in place.

According to Stan Dermott, chairman of UF’s (University of Florida’s) astronomy department, the GTC’s size and technical attributes enable it not only to gather more light than any other telescope, but also resolve the light into sharper and clearer focus.

“For astronomers, those capabilities make it a powerful tool to study cosmic origins – the early days of the universe and the very early moments in the mysterious births of stars, planets and galaxies,” he said.

“The interpretation of the structure of the disks where new planets form is highly dependent on the quality of the image,” he said, adding that the GTC also will enable the discoveries of new planets, possibly including the first habitable planet.

At the inauguration of the telescope, officials and astronomers from the University of Florida, the only US institution that is part of the project, will join more than 500 astronomers, journalists and celebrities in a ceremony presided over by Spain’s King Juan Carlos I and Queen Sofia. (ANI)

Herschel’s first insight into space reveals spectacular results

Paris, July 11 (ANI): The Herschel Space Observatory has carried out the first test observations with all its instruments, revealing spectacular results, finding water and carbon and revealing dozens of distant galaxies.

These observations show that Herschel’s instruments are working beyond expectations. They promise a mission of rich discoveries for waiting astronomers.

On June 24, Herschel’s Spectral and Photometric Imaging Receiver (SPIRE) was trained on two galaxies for its first look at the Universe.

The galaxies showed up prominently, providing astronomers with their best images yet at these wavelengths, and revealing other, more distant galaxies in the background of the images.

The pictures show galaxies M66 and M74 at a wavelength of 250 microns, longer than any previous infrared space observatory, but still the shortest SPIRE wavelength.

SPIRE is designed to look at star formation in our own Galaxy and in nearby galaxies. It will also search for star-forming galaxies in the very distant Universe.

Because these galaxies are so far away, their light has taken a very long time to reach us; so by detecting them, we are looking into the past and learning how and when galaxies like our own were formed.

Herschel’s primary mirror is 3.5 m in diameter, nearly four times larger than any previous infrared space telescope.

These images prove that Herschel enables a giant leap forward in scientists’ ability to study celestial objects at far infrared wavelengths.

Scientists used Herschel’s Heterodyne Instrument for the Far-Infrared (HIFI) on June 22 to look for warm molecular gas heated by newborn massive stars in the DR21 star-forming region in Cygnus.

HIFI provided excellent data in two different observing modes, returning information on the composition of the region with unprecedented accuracy and resolution.

It works by ‘zooming in’ on specific wavelengths, revealing different spectral ‘lines’ that represent the fingerprints of atoms and molecules and even the physical conditions of the object observed.

This makes it a powerful tool to study the role of gas and dust in the formation of stars and planets and the evolution of galaxies.

Using HIFI, scientists observed ionized carbon, carbon monoxide, and water in DR21.

These different molecular lines contribute to a more complete understanding of what is happening deep in space.

The high quality of these first observations promises great new insights into the process of star formation.

Following these images, Herschel is now in the performance verification phase, where the instruments will be further tested and calibrated. (ANI)

Earliest stars in Universe may have been twins

Washington, July 10 (ANI): Astrophysicists, using extremely detailed computer simulations, have determined that the earliest stars in the universe formed not only as individuals, but sometimes also as twins.

The robust simulations of the early universe were created by astrophysicists Matthew Turk and Tom Abel of the Kavli Institute for Particle Astrophysics and Cosmology, and Brian O’Shea of Michigan State University.

“We used to think that these stars formed by themselves, but now we see from our computer simulations that sometimes they have siblings,” said Turk.

“These stars provide the seeds of next generation star formation, so by understanding them we can better understand how other stars and galaxies formed,” he added.

To make this discovery, the researchers created an extremely detailed computer simulation of early star formation.

Into this virtual universe, they sprinkled primordial gas and dark matter as it existed soon after the Big Bang, data they obtained from observations of the cosmic microwave background.

This mostly uniform radiation – a faint glow of radio waves spread across the entire sky – contains subtle variations that reflect the beginning of all structure in the universe.

The simulations focused on the first Population III stars: massive, hot stars thought to have formed a mere several hundred million years after the Big Bang.

As the researchers watched their simulated universe evolve, waves of gas and dark matter swirled through the hot, dense universe.

As the universe cooled, gravity began to draw the matter together into clumps. In areas rich with matter, stars began to form.

In one out of the researchers’ five simulations, a single cloud of dust and dark matter formed into “twin” stars: one with a mass equivalent to about 10 suns, and one with a mass equivalent to about 6.3 suns.

Both of them were still growing at the end of the calculation and will likely grow to many times that mass.

“We ran five of these calculations starting from the beginning of the universe, and to our surprise one of them was special,” said Abel.

“This opens a whole new realm of research possibilities. These stars could evolve into two black holes, which could have created gravitational waves we could detect with an instrument like the Laser Interferometer Gravitational Wave Observatory,” he added.

“This will help us fine-tune our models for how structure in the universe formed and evolved. Understanding the very early stars helps us understand what we see today,” Turk said. (ANI)

Milky Way’s “dark matter” mystery solved by astrophysicists

Washington, July 9 (ANI): A team of astrophysicists has solved a mystery that led some scientists to speculate that the distribution of certain gamma rays in our Milky Way galaxy was evidence of a form of undetectable “dark matter” believed to make up much of the mass of the universe.

In two separate scientific papers, the astrophysicists show that this distribution of gamma rays can be explained by the way “antimatter positrons” from the radioactive decay of elements, created by massive star explosions in the galaxy, propagate through the galaxy.

Thus, the scientists said, the observed distribution of gamma rays is not evidence for dark matter.

“There is no great mystery,” said Richard Lingenfelter, a research scientist at UC San Diego’s Center for Astrophysics and Space Sciences who conducted the studies with Richard Rothschild, a research scientist also at UCSD, and James Higdon, a physics professor at the Claremont Colleges.

“The observed distribution of gamma rays is in fact quite consistent with the standard picture,” he added.

Over the past five years, gamma ray measurements from the European satellite INTEGRAL have perplexed astronomers, leading some to argue that a “great mystery” existed because the distribution of these gamma rays across different parts of the Milky Way galaxy was not as expected.

To explain the source of this mystery, some astronomers had hypothesized the existence of various forms of dark matter, which astronomers suspect exists, but have not yet found.

What is known for certain is that our galaxy and others are filled with tiny subatomic particles known as positrons, the antimatter counterpart of typical, everyday electrons.

The scientists calculated that most of the gamma rays should be concentrated in the inner regions of the galaxy, just as was observed by the satellite data.

“The observed distribution of gamma rays is consistent with the standard picture where the source of positrons is the radioactive decay of isotopes of nickel, titanium and aluminum produced in supernova explosions of stars more massive than the Sun,” said Rothschild.

The scientists point out that a basic assumption of one of the more exotic explanations for the purported mystery – dark matter decays or annihilations – is flawed, because it assumes that the positrons annihilate very close to the exploding stars from which they originated.

“We clearly demonstrated this was not the case, and that the distribution of the gamma rays observed by the gamma ray satellite was not a detection or indication of a ‘dark matter signal’,” said Lingenfelter. (ANI)

Cosmic ‘whips’ may be detected with gravitational waves

London, July 6 (ANI): A new research has determined that cosmic ‘whips’, which are topological defects in space-time larger than the observable universe, can be detected with the help of gravitational waves.

Many theories predict the existence of cosmic strings.

They say that space-time should have universe-sized snags called ‘cosmic strings’ running across it, but none have yet been found.

That could be because they broke into a tangle of smaller strings and beads soon after the big bang, say scientists.

The imprint of their extremely high gravity was expected to be seen in the cosmic microwave background – the radiation left over from the big bang – or as gravitational lenses that bend distant light towards us.

But, no convincing evidence has been seen.

Ben Shlaer of Tufts University in Medford, Massachusetts, and colleagues, told New Scientist that the lack of evidence could be because the strings were unstable and split into smaller and smaller pieces soon after they formed.

The first strings could have been gigantic closed loops or extremely large fragments that terminated in “beads”.

These beads would have been so-called monopoles – analogous to a magnet’s north or south pole without its partner.

As the strings broke, the team’s analysis shows that their split ends would have been capped off by more monopoles, eventually leading to a universe filled with fragmented strings with beads at their ends.

In an infant universe, these high-tension strings would have been whipping around, accelerating the massive beads to relativistic speeds.

These would have generated tight beams of gravitational waves, which could still be traveling through space-time.

“It’s possible that if you wait long enough, one of those highly focused bursts would hit the Earth, and that would cause one of our gravitational wave detectors to chirp,” said Shlaer.

The first cosmic strings were unstable and split into small pieces capped by monopoles.

Those detectors include the Laser Interferometer Gravitational Observatory, which is currently being upgraded, and the upcoming Laser Interferometer Space Antenna.

“The possible frequency range of the waves is exceptionally large, “raising the hope of detection” of cosmic strings,” said theoretical physicist Henry Tye at Cornell University in Ithaca, New York. (ANI)

International Year of Astronomy raises millions of eyes to the skies

Berlin, July 2 (ANI): The International Year of Astronomy 2009 (IYA2009) has achieved a milestone of sorts, in the sense that over a million people have already looked at the sky through a telescope for the first time, and even more have newly engaged in astronomy in just six months this year.

This is just one of many achievements, as countless ongoing projects and planned initiatives indicate that the IYA2009 is well on the way towards achieving many of its goals.

UNESCO and the International Astronomical Union (IAU) launched 2009 as the International Year of Astronomy under the theme “The Universe, Yours to Discover”.

The IYA2009 is a global celebration of astronomy and its contributions to society and culture, with events at national, regional and global levels throughout the whole of 2009.

Now, halfway through 2009, much has been achieved and even more can be expected in the future.

With the aim of providing low-cost telescopes that offer views far better than those obtained by Galileo Galilei some 400 years ago, the venture has picked up significant pace since the IYA2009 began.

By the end of July, the first 60,000 Galileoscopes will have been shipped, and a further 100,000 are currently in production.

More than 4000 Galileoscopes have been generously donated by the IYA2009 and individuals to organizations and schools in developing countries.

This gesture aptly demonstrates the commitment of astronomy enthusiasts to the IYA2009 goal of making the skies accessible to all.

But perhaps the most impressive figures for the IYA2009 have come from the national activities that have brought together hundreds of thousands of people in many countries for astronomy-themed events.

According to IAU President Catherine Cesarsky, “It’s amazing to see just how far the International Year of Astronomy 2009 has progressed over the last six months. The hard work put in by professional and amateur astronomers is making the IYA2009′s theme, ‘The Universe, Yours to Discover’ a reality.” (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)

Milky Way survived ancient heat wave because of dark matter

Washington, July 1 (ANI): A new theory by scientists says that our Milky Way galaxy survived intense heat generated by the “ignition” of the Universe about half-a-billion years after the Big Bang, because it was already immersed in a large clump of dark matter that trapped gases inside it.

Tiny galaxies, inside small clumps of dark matter, were blasted away by the heat that reached approximate temperatures of between 20,000 and 100,000 degrees centigrade, according to the scientists, including experts at Japan’s University of Tsukuba.

The researchers said that the early Milky Way, which had begun forming stars, held on to the raw gaseous material from which further stars would be made.

This material would otherwise have been evaporated by the high temperatures generated by the “ignition”.

Using computer simulations carried out by the international Virgo Consortium (which is led by Durham), the scientists examined why galaxies like the Milky Way have so few companion galaxies or satellites.

Astronomers have found a few dozen small satellites around the Milky Way, but the simulations revealed that hundreds of thousands of small clumps of dark matter should be orbiting our galaxy.

Dark matter is thought to make up 85 per cent of the Universe’s mass and is believed to be one of the building blocks of galaxy formation.

The scientists said the heat from the early stars and black holes rendered this dark matter barren and unable to support the development of satellite star systems.

According to Joint lead investigator Professor Carlos Frenk, Director of the Institute for Computational Cosmology, at Durham University, “The validity of the standard model of our Universe hinges on finding a satisfactory explanation for why galaxies like the Milky Way have so few companions.”

“The simulations show that hundreds of thousands of small dark matter clumps should be orbiting the Milky Way, but they didn’t form galaxies,” he explained.

“We can demonstrate that it was almost impossible for these potential galaxies to survive the extreme heat generated by the first stars and black holes,” he added.

“The heat evaporated gas from the small dark matter clumps, rendering them barren. Only a few dozen front-runners which had a head start on making stars before the Universe ignited managed to survive,” he further added.

By providing a natural explanation for the origin of galaxies, the simulations support the view that cold dark matter is the best candidate for the mysterious material believed to make up the majority of our Universe. (ANI)

‘Friendly’ Anne Hathaway doling out designer dresses on loan

New York, June 24 (ANI): Everyone should have a friend like Anne Hathaway, for the actress not only knows how to treat her pals well, but also makes sure that they dress well too.

The actress’ ‘Twelfth Night’ co-star Julie White arrived at the L.A. premiere of ‘Transformers: Revenge of the Fallen’ in a dress happily on loan from her.

“I had my dress picked out for the premiere on Monday, and on Sunday night Annie came in with kind of a wadded-up-looking black bag that you get from the deli,” the New York Daily News quoted White as saying.

She added: “And inside of it was this gorgeous Marchesa dress. She’s like, ‘Julie, I think you should wear this.’ I’m not kidding. That’s how good a girl she is.”

When asked whether it’s just like lady friends borrowing clothes from each other, White said: “Yes, except it’s lady friends with access to the greatest clothes in the universe.”

She said: “It’s like Shia – someone who knows they’re in a kind of crazy, charmed position. They just totally share the wealth.”

She added: “Anne “was absolutely right. She has brilliant taste. It looks perfect!” (ANI)

‘Friendly’ Anne Hathaway doling out designer dresses on loan

New York, June 24 (ANI): Everyone should have a friend like Anne Hathaway, for the actress not only knows how to treat her pals well, but also makes sure that they dress well too.

The actress’ ‘Twelfth Night’ co-star Julie White arrived at the L.A. premiere of ‘Transformers: Revenge of the Fallen’ in a dress happily on loan from her.

“I had my dress picked out for the premiere on Monday, and on Sunday night Annie came in with kind of a wadded-up-looking black bag that you get from the deli,” the New York Daily News quoted White as saying.

She added: “And inside of it was this gorgeous Marchesa dress. She’s like, ‘Julie, I think you should wear this.’ I’m not kidding. That’s how good a girl she is.”

When asked whether it’s just like lady friends borrowing clothes from each other, White said: “Yes, except it’s lady friends with access to the greatest clothes in the universe.”

She said: “It’s like Shia – someone who knows they’re in a kind of crazy, charmed position. They just totally share the wealth.”

She added: “Anne “was absolutely right. She has brilliant taste. It looks perfect!” (ANI)

Scientists invent world’s fastest and most sensitive astronomical camera

Munich, June 19 (ANI): Scientists have invented the world’s fastest and most sensitive astronomical camera that can take 1500 finely exposed images per second even when observing extremely faint objects.

The first 240×240 pixel images with the world’s fastest high precision faint light camera were obtained through a collaborative effort between ESO and three French laboratories from the French Centre National de la Recherche Scientifique/Institut National des Sciences de l’Univers (CNRS/INSU).

Cameras such as this are key components of the next generation of adaptive optics instruments of Europe’s ground-based astronomy flagship facility, the ESO Very Large Telescope (VLT).

“The performance of this breakthrough camera is without an equivalent anywhere in the world. The camera will enable great leaps forward in many areas of the study of the Universe,” said Norbert Hubin, head of the Adaptive Optics department at ESO.

OCam will be part of the second-generation VLT instrument SPHERE. To be installed in 2011, SPHERE will take images of giant exoplanets orbiting nearby stars.

A fast camera such as this is needed as an essential component for the modern adaptive optics instruments used on the largest ground-based telescopes.

Telescopes on the ground suffer from the blurring effect induced by atmospheric turbulence.

This turbulence causes the stars to twinkle in a way that delights poets, but frustrates astronomers, since it blurs the finest details of the images.

Adaptive optics techniques overcome this major drawback, so that ground-based telescopes can produce images that are as sharp as if taken from space.

The new generation instruments require these corrections to be done at an even higher rate, more than one thousand times a second, and this is where OCam is essential.

Cameras normally used for very high frame-rate movies require extremely powerful illumination, which is of course not an option for astronomical cameras.

OCam and its CCD220 detector, developed by the British manufacturer e2v technologies, solve this dilemma, by being not only the fastest available, but also very sensitive, making a significant jump in performance for such cameras.

Because of imperfect operation of any physical electronic devices, a CCD camera suffers from so-called readout noise.

OCam has a readout noise ten times smaller than the detectors currently used on the VLT, making it much more sensitive and able to take pictures of the faintest of sources. (ANI)

Depeche Mode’s O2 gig derailed due to tumour scare

London, May 29 (ANI): British electronic music pioneers, Depeche Mode, have cancelled their homecoming gig at the O2 after announcing that its lead singer, Dave Gahan, was recovering from an emergency cancer surgery.

Gahan, 47, had undergone an operation to remove a cancerous tumor from his bladder.

Now he has been ordered to take time off, reports The Sun.

Medics discovered the growth by chance during routine tests after Gahan suffered a nasty stomach bug that has also scuppered nine dates on their Tour Of The Universe.

The heroes had been gearing up to make their grand return at the O2 supershow.

However, a statement released by the band yesterday, said: “On May 12, lead singer Dave Gahan suffered a severe bout of gastroenteritis, leading to his hospitalisation and the cancellation of the Athens concert.

“While in hospital, further medical tests revealed a low­grade malignant tumour in Dave’s bladder, which has since been successfully removed.

“At doctors’ orders, Dave Gahan must take a break until June 8, to ensure that he makes a full recovery. The Leipzig show on June 8 will be the first concert following Dave’s recovery.

“Dave Gahan sincerely thanks his fans for their support, understanding and patience.

“Depeche Mode deeply regret any problems or inconveniences the cancellations and postponements may have caused.” (ANI)

Cosmic “ghost” found lurking around supermassive black hole

Washington, May 29 (ANI): NASA’s Chandra X-ray Observatory has found a cosmic “ghost” lurking around a distant supermassive black hole, which is the first detection of such a high-energy apparition, and may be evidence of a huge eruption produced by the black hole.

The X-ray ghost, so-called because a diffuse X-ray source has remained after other radiation from the outburst has died away, is in the Chandra Deep Field-North, one of the deepest X-ray images ever taken.

The source, a.k.a. HDF 130, is over 10 billion light-years away and existed at a time 3 billion years after the Big Bang, when galaxies and black holes were forming at a high rate.

“We’d seen this fuzzy object a few years ago, but didn’t realize until now that we were seeing a ghost”, said Andy Fabian of the Cambridge University in the United Kingdom.

“It’s not out there to haunt us, rather it’s telling us something – in this case what was happening in this galaxy billions of year ago,” he added.

Fabian and colleagues think the X-ray glow from HDF 130 is evidence for a powerful outburst from its central black hole in the form of jets of energetic particles traveling at almost the speed of light.

When the eruption was ongoing, it produced prodigious amounts of radio and X-radiation, but after several million years, the radio signal faded from view as the electrons radiated away their energy.

However, less energetic electrons can still produce X-rays by interacting with the pervasive sea of photons remaining from the Big Bang – the cosmic background radiation.

Collisions between these electrons and the background photons can impart enough energy to the photons to boost them into the X-ray energy band.

This process produces an extended X-ray source that lasts for another 30 million years or so.

“This ghost tells us about the black hole’s eruption long after it has died,” said co-author Scott Chapman, also of Cambridge University. “This means we don’t have to catch the black holes in the act to witness the big impact they have,” he added.

This is the first X-ray ghost ever seen after the demise of radio-bright jets.

In HDF 130, only a point source is detected in radio images, coinciding with the massive elliptical galaxy seen in its optical image.

This radio source indicates the presence of a growing supermassive black hole.

“This result hints that the X-ray sky should be littered with such ghosts, especially if black hole eruptions are as common as we think they are in the early Universe,” said co-author Caitlin Casey, also of Cambridge. (ANI)