Scientists find ‘modern’ galaxies amongst ancient galaxy clusters

Washington, May 13 (ANI): A team of astronomers has discovered a young cluster, born just 2.8 billion years after the Big Bang, that appears very similar to the much older present-day galaxy clusters.

“We were looking for clusters of galaxies when the Universe was still very young,” says Carnegie’s Ivelina Momcheva, who did the spectroscopic analysis that led to the discovery of the cluster.

“One might think that the clusters we find would look young as well. However, in this cluster we found a number of surprisingly ancient-looking galaxies. This cluster resembles modern-day clusters, which are nearly 10 billion years older.”

“It is like we dug an archaeological site in Rome and found pieces of modern Rome in amongst the ruins,” adds lead author Casey Papovich of Texas A&M University.

The cluster is called CLG J02182-05102 and contains approximately 60 galaxies, including several enormous red galaxies at its centre holding 10 times as many stars as the Milky Way.

Unable to find using NASA’s Spitzer Space Telescope if its galaxies are indeed gravitationally bound, the team used an advanced spectrograph.

Post analysis, they found that the cluster now looks the way it looked 9.6 billion years ago and since then, has moved away as the universe expanded. Today, it stands at a distance of 15 billion light years.

The new discovery will help researchers understand how galaxies evolve and form clusters. CLG J02182-05102’s large red galaxies are unexpected because most galaxies at that time were still rapidly forming stars, and, as a result, appear smaller and their emitted light bluer.

“We are witnessing the youth of truly massive cluster of galaxies,” says Momcheva. “ClG J02182-05102 will continue growing, accreting more galaxies and slowly aging. By the present day it has probably grown to be a large metropolis of a cluster like our neighbour, the Coma cluster.” (ANI)

No US big bang on India N-trade

American firms, which played a key role in the passage of Indo-US civilian nuclear deal, are unlikely to engage in atomic trade with India if New Delhi does not become party to the Convention on Supplementary Compensation for Nuclear Damage, which has not yet entered into force, a Congressional report has said.

“US companies have not yet started nuclear trade with India. New Delhi had reportedly insisted that India and the United States conclude an agreement on a reprocessing facility in India before New Delhi would sign contracts with US nuclear firms. However, the countries announced March 29 that they had concluded the agreement,” said a latest report on the civil nuclear deal released by Congressional Research Service.

“The Administration must submit the subsequent arrangement to Congress, but has not yet done so. The proposed arrangement shall not take effect if Congress adopts a joint resolution of disapproval,” said the CRS report ‘US Nuclear Cooperation with India: Issues for Congress’.

CRS is the independent research wing of the US Congress.

“It is worth noting that US firms will likely be very reluctant to engage in nuclear trade with India if the government does not become party to the Convention on Supplementary Compensation for Nuclear Damage, which has not yet entered into force,” said the 47-page report, dated April 8, a copy of which has been obtained by PTI.

The civil-nuclear bill requires that, before the Nuclear Regulatory Commission can issue licenses for US nuclear exports to India, the President must determine and certify to Congress that New Delhi’s IAEA safeguards agreement has entered into force and that India’s declaration of its nuclear facilities to the agency “is not materially inconsistent with the facilities and schedule” described in a separation plan that New Delhi has provided to Washington.

India’s safeguards agreement entered into force May 11, 2009, and New Delhi has filed the declaration with the IAEA.

Obama submitted the required certification to Congress on February 3, 2010, determining that India has satisfied the legal requirement described above.

“Nevertheless, US firms will likely be very reluctant to engage in nuclear trade with India if the government does not become party to the Convention on Supplementary Compensation for Nuclear Damage (CSC), which has not yet entered into force,” it said.

In a letter, the then Foreign Secretary Shivshankar Menon in September 2008, said: “It is the intention of the Indian Government to take all steps necessary to adhere to the Convention on Supplementary Compensation for Nuclear Damage prior to the commencement of international civil nuclear cooperation under” the US-India agreement.

Emma Thompson walks the blue carpet at Nanny McPhee premiere with pig!

London, Mar 25 (ANI): British actress Emma Thompson was spotted walking down the blue carpet at the world premiere of ‘Nanny McPhee And The Big Bang’ leading a pig.

Thompson, 50, had written and starred in the movie, which sees the magical nanny come to the aid of a mother struggling to run a farm and look after her children while her husband is at war.

Among the cast who attended the screening of the sequel in London’s Leicester Square, were comedian Bill Bailey and Maggie Gyllenhaal, who praised Thompson for her acting.

“I’m her biggest fan and I know I’m not alone in thinking she is a brilliant genius. I would like to work with her on everything,” the Telegraph quoted her as saying. (ANI)

Galaxy in early Universe went through ‘teenage growth spurt’

Washington, March 22 (ANI): Reports indicate that an international team of scientists has found a massive galaxy in the early Universe creating stars like our sun up to 100 times faster than the modern-day Milky Way, which they have described as “a teenager going through a growth spurt”.

Due to the amount of time it takes light to reach Earth, the scientists observed the galaxy as it would have appeared 10 billion years ago – just three billion years after the Big Bang.

They found four discrete star-forming regions within the galaxy known as SMM J2135-0102.

Each region was more than 100 times brighter than star-forming regions in the Milky Way, such as the Orion Nebula.

The researchers suggested that star formation was more rapid and vigorous in the early Universe as galaxies went through periods of huge growth.

The findings provide a unique insight into how stars formed in the early Universe, the scientists added.

According to lead author Dr Mark Swinbank, in the Institute for Computational Cosmology, at Durham University, “This galaxy is like a teenager going through a growth spurt. If you could see it today as an adult, you’d find the galactic equivalent of the football player Peter Crouch.”

“We don’t fully understand why the stars are forming so rapidly but our results suggest that stars formed much more efficiently in the early Universe than they do today,” he said.

“Galaxies in the early Universe appear to have gone through rapid growth and stars like our sun formed much more quickly than they do today,” he added.

The scientists estimate that the observed galaxy is producing stars at a rate equivalent to 250 suns per year. (ANI)

Antonio Banderas beds beauty 20 years his junior – in new film!

London, March 10 (ANI): Antonio Banderas’ luck has not left him even when he’s about to hit 50 – the actor recently got a chance to bed Autumn Resser, 20 years his junior, for his new flick The Big Bang.

Resser, 29, is taking the big leap from the small screen to Hollywood after winning accolades for playing Taylor Townsend on the Fox series The OC, reports the Sun.

The movie is the story of a private detective who has been given the task of finding a missing stripper, but things turn ugly when everyone he questions is killed.

The film also stars Snoop Dogg and former Dawson”s Creek actor James Van Der Beek. (ANI)

FlexMonkeyTM 1.0 GA Now Available From Gorilla Logic

Open-Source Functional Testing Tool for Adobe Flex Applications – New and
Improved!
BROOMFIELD, Colo.–(Business Wire)–
Gorilla Logic, an enterprise IT consulting services firm known for its top
consulting talent, today announced the availability of FlexMonkeyTM 1.0 GA. With
a rapidly growing user base that recently surpassed 5,000 registered users,
FlexMonkey is a de facto standard for automated functional testing of Flex
applications. After eight months of maturing in a beta status, FlexMonkey is now
available for production use by developers and quality assurance professionals
everywhere.

“FlexMonkey has been invaluable for us in testing Adobe Air applications. It has
found bugs and regressions on several occasions, preventing them from ever
reaching customers. And…I had everything I needed to add FlexMonkey tests into
our continuous integration environment,” said Michael Portuesi, Principal
Engineer, Zoodles.com.

FlexMonkey is an open source testing tool providing record/playback functional
testing of Adobe Flex applications. FlexMonkey 1.0 GA delivers the features and
improvements most requested by the FlexMonkey user community including:

* “Wait For” handling – removes reliance on the PauseCommand by defining
conditions that pause a script until true
* Fuzzy Bitmap Compare – the Verify command for bitmap images now allows for
user- controlled tolerances in color comparisons
* Simplified Setup – new easier process for configuring FlexMonkey testing of an
application
* Compatability – out of the box compatibility with multiple Flex SDKs (3.3,
3.4.1 and 3.5)
* Code Compiling – easier customization and compilation of FlexMonkey source

“FlexMonkey keeps me from becoming exactly that – a monkey chained to a desk
manually testing our software,” said Max Cameron, Co-Founder, Big Bang
Technology, Inc. “Simply put, FlexMonkey kicks ass. It softens the enormous
overhead of functional testing, and more importantly, it let`s my engineers get
some sleep at night.”

FlexMonkey is well-suited for use by both developers and QA testers. It provides
for regression and functional testing, and can be run from popular build systems
and continuous integration environments, like CruiseControl.

“FlexMonkey 1.0 GA marks a major milestone for the FlexMonkey open source
project and the Flex community who have come to rely on it. We encourage all
existing users to upgrade to this new version which paves the way for our
upcoming FlexMonkey releases for Flex 4, as well as our FlexMonkey/Selenium
bridge,” said Stu Stern, CEO, Gorilla Logic.

FlexMonkey 1.0 GA is available today at www.gorillalogic.com/flexmonkey. Gorilla
Logic also offers complete FlexMonkey training and testing services. Customers
interested in early access to FlexMonkey for the Flex 4 SDK and the
FlexMonkey/Selenium bridge should contact Gorilla Logic at
www.gorillalogic.com/who-we-are/contact.

About Gorilla Logic

Gorilla Logic is an enterprise application development services and consulting
firm known industry-wide for providing “gorilla” consultants that can
dramatically improve development team productivity. Gorilla Logic has long
demonstrated their industry-leading expertise in enterprise Java / JEE
development, Adobe Flex / RIA development, and mobile device application
development, including the iPhone. Gorilla Logic has been engaged to ensure the
success of their most mission critical projects by Fortune 500 companies as well
as small and mediums-zed businesses and startups in industries ranging from
financial services to entertainment to aerospace and the government sector.

Gorilla Logic also develops open source tools for Java, Flex, and iPhone
developers.

FoneMonkey (www.gorillalogic.com/fonemonkey)

FlexMonkey (www.gorillalogic.com/flexmonkey)

MonkeyWrench (www.gorillalogic.com/monkeywrench)

OpenGXE (www.gorillalogic.com/opengxe)

For more information about Gorilla Logic, please visit www.gorillalogic.com or
email info@gorillalogic.com.

Gorilla Logic Media Contact
Chad Sanderson
303.974.7088 ext. 7002
chad.sanderson@gorillalogic.com

Copyright Business Wire 2010

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)

Scientists make major advance in understanding evolution of the universe

Washington, August 20 (ANI): In a new research, a team of scientists has achieved a significant advance in the understanding of the early evolution of the universe, by putting new constraints on the details of how the universe looked in its earliest moments.

The research was conducted by a team of scientists associated with the LIGO (Laser Interferometer Gravitational-Wave Observatory) Scientific Collaboration and the Virgo Collaboration.

The new measurements by LIGO directly probe the gravitational wave background in the first minute of its existence, at time scales much shorter than accessible by the cosmic microwave background.

“Our results are a major step toward the detection of primordial gravitational waves – ripples in the fabric of space and time – that were created as the universe expanded in its earliest moments,” said Lee Samuel Finn, a Penn State professor of physics and of astronomy and astrophysics.

“This type of information would provide vital clues to understanding how the structure of the universe evolved. For example, why is our universe clumped into galaxies? This information also would tell us whether some of the fantastical proposals are correct about the way our universe came to be,” he said.

The Big Bang is believed to have created a flood of gravitational waves that still fill the universe and carry information about the universe as it existed immediately after the Big Bang.

These waves would be observed as the “stochastic background,” analogous to a superposition of many waves of different sizes and directions on the surface of a pond.

The amplitude of this background is directly related to the parameters that govern the behavior of the universe during the first minute after the Big Bang.

According to Finn, “Space-time is the living stage upon which the drama of the universe plays out. The primordial stochastic gravitational waves are the warps, twists, and bends in space-time that were laid down as the universe expanded from its earliest moments to the present.”

“The observations we report in this paper are the closest direct examination of the framework of the living, breathing universe, he said.

“Gravitational waves are the only way to directly probe the universe at the moment of its birth; they’re absolutely unique in that regard,” said David Reitze, a professor of physics at the University of Florida and spokesperson for the LIGO Scientific Collaboration.

“We simply can’t get this information from any other type of astronomy. This is what makes this result in particular, and gravitational-wave astronomy in general, so exciting,” 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)

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)

Probe to look out for gravity waves emitted 14 billion years ago

Washington, May 16 (ANI): A new probe is going to look for the cosmic microwave background (CMB) radiation, which is the afterglow of the Big Bang, that may still carry a faint signature of gravitational waves, which rippled through the very fabric of space-time nearly 14 billion years ago.

A tiny fraction of a second following the Big Bang, the universe allegedly experienced the most inflationary period it has ever known.

“During this inflationary era, space expanded faster than the speed of light. It sounds crazy, but it fits a variety of cosmological observations made in recent years,” said University of Chicago physicist Bruce Winstein.

“Theorists take it to be true, but we have to prove it,” said Winstein, the Samuel K. Allison Distinguished Service Professor in Physics at the University of Chicago. “It needs a real test, and that test is whether or not gravity waves were created,” he added.

“The CMB is probably our best handle on the overall structure of the universe and how it was born,” he further added.

Winstein and his Chicago associates are part of the international QUIET (Q/U Imaging ExperimenT; the Q and U stand for radiation parameters called Stokes parameters) collaboration that has devised such a test.

QUIET’s goal is to detect remnants of the radiation emitted at the earliest moments of the universe, when gravity waves rippled through the very fabric of space-time itself.

The intensive gravitational fields that existed at these earliest moments, according to Einstein, produced gravity waves that alternatively compressed and expanded space, first in one direction, then another.

The QUIET experiment began operating last October with an antenna array that contains 19 detectors.

Since then, QUIET collaborators at the Jet Propulsion Laboratory in California have produced 91 detectors sensitive to the radiation at a higher frequency.

Over the past several months, the Chicago collaboration has assembled and calibrated these 91 detectors in the basement of the Laboratory for Astrophysics and Space Research.

Winstein’s team has tested each detector, adjusting 10 critical voltages for each to yield the best performance.

According to Winstein, correctly optimized voltages can improve detector performance by a large factor, making it possible to observe in one day what would have otherwise required a week.

This newer, more sensitive array will begin operating in June. (ANI)

Antonio Banderas to star as detective in The Big Bang

Washington, May 11 (ANI): Antonio Banderas is all set to star in the Tony Krantz-directed neo-noir detective story, ‘The Big Bang’.

Richard Rionda Del Castro, Krantz and Erik Jendresen will produce the film, which is based on a script by Jendresen, who also penned ‘Band of Brothers’.

The production of ‘The Big Bang’ will start in Spokane, Washington, in September, reports Variety magazine.

In the film, Banderas would be seen playing an L.A. private detective who’s hired to find a missing stripper.

The track leads to the New Mexico desert, where he finds a trail of bodies and contends with a brutal Russian boxer, three LAPD detectives and an aging billionaire looking to perfect the nuclear physics equivalent of the Big Bang.

The film’s executive producers will be Patricia Eberle, Richard Salvatore, and Ross Dinerstein.

And Rionda Del Castro’s Hannibal Pictures is financing and handling foreign sales at Cannes.

U.S. representation is being handled by WMA and Endeavor.

The project would be the first theatrical feature for Krantz, one of the few ex-agents to make that leap. (ANI)

‘Big Bang’ machine almost ready to run again

London, May 4 (ANI): The Large Hadron Collider (LHC), which is the biggest atom-smashing machine ever built, is almost ready to run again.

The LHC straddles the borders of France and Switzerland and is operated by CERN, the European particle physics laboratory near Geneva.
It is designed to simulate the “Big Bang”, which started the universe 15 billion years ago, by smashing sub-atomic particles together at energies never before achieved.
But, it suffered a catastrophic malfunction soon after being switched on last September amid a fanfare of publicity.

In the accident in September, a weld between two sections of the superconducting wire failed.
In the minutes after the accident, several tonnes of liquid helium used to cool the magnets vaporized, creating a pressure build-up that wrenched magnets from their concrete stands.

As a result, 53 of the magnets used to accelerate sub-atomic particles around the machine’s 17-mile underground tunnel had to be brought to the surface for repair or cleaning.

Now, according to a report in The Sun, the last of 53 replacement magnets have been lowered into the LHC, which stands in a 16-mile tunnel on the Swiss-French border.

Reports indicate that the massive machine would be ready by autumn this year.

Through experiments at the LHC, physicists hope to find the elusive “God’s Particle” – Higgs Boson – which would explain the existence of mass. (ANI)

Giant galaxies born 6-7 billion years earlier than expected

Washington, April 24 (ANI): Astronomers have discovered large galaxies that have not changed much in size for the last 9 billion years, which suggests these cosmic giants were born 6-7 billion years earlier than expected.

The most popular model for galaxy formation is a bottom-up or hierarchical model in which small galaxies gradually develop into larger ones over a long period of time.

The model predicts that smaller galaxies would merge to form larger ones, growing to 90 percent of their size about 11 billion years after the Big Bang.

This means that smaller galaxies would be older and larger ones, younger.

A team of astrophysicists, led by Professor Chris Collins from Liverpool John Moores University (LJMU), used observations from the Subaru Telescope, as well as the XMM-Newton to collect data about galaxies that existed two-thirds of the way back in time since the Universe began.

By being able to extend the baseline of their data so far back in time, they have a foundation for concluding that large galaxies were almost fully formed 4-5 billion years after the Big Bang, 6-7 billion years earlier than the hierarchical model would forecast.

According to Dr. John Stott, who carried out the photometry and data analysis, “We were surprised to find that the largest and brightest galaxies in the universe have remained essentially unchanged for the last 9 billion years, having grown rapidly soon after the Big Bang.”

The galaxies examined in the observations were brightest cluster galaxies (BCGs), located at the centers of galaxy clusters.

Because they are so bright and uniform, they are often used as beacons for studying the universe.

At the beginning of their research, the scientists examined the ages of the stars in the galaxies. Their findings indicated a consistent epoch of formation for the majority of the stars – about 2-3 billion years after the Big Bang.

Since the galaxies they studied were almost fully formed 4-5 billion years after the Big Bang, they concluded that they probably grew rapidly and formed much sooner than the hierarchical model of galaxy evolution suggests. (ANI)

Maggie Gyllenhaal joins cast of ‘Nanny McPhee and the Big Bang’

Washington, Apr 15 (ANI): American actress Maggie Gyllenhaal has joined the cast of ‘Nanny McPhee and the Big Bang’, a sequel to Working Title’s 2005 hit ‘Nanny McPhee’.

Gyllenhaal, 31, will be starring alongside Rhys Ifans, Maggie Smith and Asa Butterfield.

Ralph Fiennes is said to be in talks for an uncredited cameo, reports Variety magazine.

Brit actress Emma Thompson will be penning the script, exec producing, and reprising her role as a magic-wielding governess.

Brit television director Susanna White will be making her feature-directing debut with the movie, whose story is based on a group of kids who are evacuated from the city to a farm during wartime.

Working Title co-toppers Eric Fellner and Tim Bevan are producing along with Lindsay Doran, and Debra Hayward and Liza Chasin will exec produce the series based on Christianna Brand’s popular “Nurse Matilda” tyke books. (ANI)

Discovery of recently formed galaxies poses challenge to galaxy formation theories

Washington, April 11 (ANI): A team of astronomers has found a sample of massive galaxies with properties that suggest they may have formed relatively recently, a discovery that poses challenge to galaxy formation theories.

This runs counter to the widely-held belief that massive, luminous galaxies (like our own Milky Way Galaxy) began their formation and evolution shortly after the Big Bang, some 13 billion years ago.

Further research into the nature of these objects could open new windows into the study of the origin and early evolution of galaxies.

As part of the research, the team of astronomers, led by IU (Indiana University) astronomer John Salzer, uncovers the unique properties of 15 galaxies.

According to John Salzer, principal investigator for the study, the 15 galaxies in the sample exhibit luminosities (a measure of their total light output) that indicate that they are massive systems like the Milky Way and other so-called “giant” galaxies.

However, these particular galaxies are unusual because they have chemical abundances that suggest very little stellar evolution has taken place within them.

Their relatively low abundances of “heavy” elements (elements heavier than helium, called “metals” by astronomers) imply the galaxies are cosmologically young and may have formed recently.

The chemical abundances of the galaxies, combined with some simple assumptions about how stellar evolution and chemical enrichment progress in galaxies in general, suggest that they may only be 3 or 4 billion years old, and therefore formed 9 to 10 billion years after the Big Bang.

Most theories of galaxy formation predict that massive, luminous systems like these should have formed much earlier.

If this overall interpretation proves correct, the galaxies may allow astronomers to investigate phases of the galaxy formation and evolution process that have been difficult to study because they normally occur at such early times in the Universe, and therefore at very large distances from us.

“These objects may represent a unique window on the process of galaxy formation, allowing us to study relatively nearby systems that are undergoing a phase in their evolution that is analogous to the types of events that, for most galaxies, typically occurred much earlier in the history of the Universe,” Salzer said.

The discoveries are the result of a multi-year survey of more than 2,400 star-forming galaxies called the Kitt Peak National Observatory International Spectroscopic Survey (KISS).

The survey was designed to collect basic observational data for a large number of extragalactic emission-line sources. (ANI)

Universe’s biggest galaxies may have fed on dark matter to grow quick

London, April 7 (ANI): In a new research, scientists have determined that some of the biggest galaxies in the early universe seem to have grown quicker than thought possible and may have bulked up on streams of gas flowing along filaments of dark matter.

Monster galaxies have long been thought to take a long time to form, growing slowly by gobbling up smaller galaxies like a giant amoeba absorbing food.

According to a report in New Scientist, a new research performed using the Subaru telescope in Hawaii, has suggested that overeating in this way cannot explain why some of the brightest galaxies at the heart of five clusters dating from relatively soon after the big bang – more than 8 billion years ago – grew so large.

Models suggest that if they snacked only on other galaxies, those ancient leviathans should have been just a fifth as massive as the biggest galaxies in similar clusters today that have had longer to eat their smaller neighbours.

But instead the ancient galaxies appear to be roughly 90 per cent as massive as their present-day counterparts.

“It could be the tip of the iceberg. It might mean the simulations (of the early universe) need to be significantly altered,” said Chris Collins of Liverpool John Moores University in Birkenhead, UK.

“Either simulations of large galaxies gobbling up smaller ones have misjudged some physical principles, like star formation and the behaviour of gas, or the rapid growth was fed by a completely different diet,” said Collins.

There is a limit on how quickly galaxies can draw in gas needed to fuel star formation, since pulling it in too fast raises its temperature to create a shock-wave-like barrier that prevents more gas from entering.

However, simulations published earlier this year suggest early galaxies could feed more quickly if they were situated on filaments of dark matter that act like pipes, allowing gas to flow rapidly into a galaxy while staying cool.

These filaments may already have been spotted in mystery blobs of hydrogen recently found surrounding other galaxies, according to Collins.

Finding such features in the dust around these large galaxies could be additional evidence that dark matter may be responsible.

According to Kenneth Rines of Western Washington University in Bellingham, Washington, “Overall, the results are every intriguing. They show the history of these monster galaxies is more complex than we expected.” (ANI)

Computer simulation reveals ‘dawn’ of the cosmos

Washington, Feb 11 (ANI): Scientists have used a computer simulation to come up with images that show the formation of the first big galaxies in the Universe, which is literally the ‘cosmic dawn’.

The images, produced by scientists at Durham University’s Institute for Computational Cosmology, predict what the very early Universe would have appeared like 500 million years after the Big Bang.

The Cosmic Dawn began as galaxies began to form out of the debris of massive stars which died explosively shortly after the beginning of the Universe.

The Durham calculation predicts where these galaxies appear and how they evolve to the present day, over 13 billion years later.

Gravity produced by dark matter is an essential ingredient in galaxy formation and by studying its effects the scientists eventually hope to learn more about what the substance is.

The work combined a massive simulation showing how structures grow in dark matter with a model showing how normal matter, such as gas, behaves to predict how galaxies grow.

Gas feels the pull of gravity from dark matter and is heated up before cooling by releasing radiation and turning into stars.

The simulation images show which galaxies are forming stars most vigorously at a given time.

Although the galaxies are biggest at the present day, the rate at which they are making new stars has dropped greatly compared with the rate in the early Universe.

The calculations of the Durham team, supported by scientists at the Universidad Catolica in Santiago, Chile, can be tested against new observations reaching back to early stages in the history of the Universe almost one billion years after the Big Bang.

According to lead author, Alvaro Orsi, a research postgraduate in Durham University’s Institute for Computational Cosmology (ICC), “We are effectively looking back in time and by doing so we hope to learn how galaxies like our own were made and to understand more about dark matter.”

“The presence of dark matter is the key to building galaxies. Without dark matter, we wouldn’t be here today,” he said.

“Our research predicts which galaxies are growing through the formation of stars at different times in the history of the Universe and how these relate to the dark matter,” said co-author Dr Carlton Baugh, a Royal Society Research Fellow, in the ICC, at Durham University.

“We give the computer what we think is the recipe for galaxy formation and we see what is produced which is then tested against observations of real galaxies,” he added. (ANI)

“Big Bang Machine” to be re-started later this year

London, Feb 9 (ANI): An official statement from CERN indicates that the Large Hadron Collider, popularly known as the “Big Bang Machine”, will be up and running in time to deliver the first batch of data for experts to begin experiments by the end of the year.

The LHC, the biggest atom-smashing machine ever built, straddles the borders of France and Switzerland and is operated by Cern, the European particle physics laboratory near Geneva.

It is designed to simulate the “Big Bang”, which started the universe 15 billion years ago, by smashing sub-atomic particles together at energies never before achieved.

But, it suffered a catastrophic malfunction soon after being switched on last September amid a fanfare of publicity.

Officials and scientists from the European Organization for Nuclear Research (CERN), which built the 4 billion pounds device, have been in talks this week about when to re-start it.

They have also discussed what caused the LHC to grind to a halt and how to prevent similar incidents happening in the future.

According to a report in the Telegraph, CERN have now said that they hope the machine will be up and running in time to deliver the first batch of data for experts to begin experiments by the end of the year.

A final decision on the exact date to switch it back on is expected to be taken soon.

The breakdown on September 19 was blamed on a faulty electrical connection, which led to a leak of super-cold helium causing damage estimated at 20 million pounds.

As a result, 53 of the magnets used to accelerate sub-atomic particles around the machine’s 17-mile underground tunnel had to be brought to the surface for repair or cleaning.

Two further “suspect connections” have since been found and engineers are working to remedy the problem, this week’s meeting in Chamonix was told.

CERN said that if the plans for re-starting the LHC are approved, it will start producing physics data late this year, through to the end of 2010.

“These recommendations represent the best way forward for the LHC and for the field of particle physics in general,” said Steve Myers, CERN’s Director for Accelerators, who chaired the meeting.

“CERN’s priority for 2009 is to get collision data for the experiments, but with caution as the guiding principle. The recommendations made to the CERN management are cautious, while achieving the goal of running this year,” he added. (ANI)