Scientists find meteorite that came from innermost asteroid belt between Mars and Jupiter

Washington, September 18 (ANI): In a very rare finding, scientists have discovered an unusual kind of meteorite in the Western Australian desert and have uncovered that it came from the innermost main asteroid belt between Mars and Jupiter.

Meteorites are the only surviving physical record of the formation of our Solar System.

However, information about where individual meteorites originated, and how they were moving around the Solar System prior to falling to Earth, is available for only a dozen of around 1100 documented meteorite falls over the past two hundred years.

According to Dr Phil Bland from the Department of Earth Science and Engineering at Imperial College London, the lead author of the study, “We are incredibly excited about our new finding. Meteorites are the most analysed rocks on Earth, but it’s really rare for us to be able to tell where they came from.”

The new meteorite, which is about the size of cricket ball, is the first to be retrieved since researchers from Imperial College London, Ondrejov Observatory in the Czech Republic, and the Western Australian Museum, set up a trial network of cameras in the Nullarbor Desert in Western Australia in 2006.

The researchers aim to use these cameras to find new meteorites, and work out where in the Solar System they came from, by tracking the fireballs that they form in the sky.

The new meteorite was found on the first day of searching using the new network, by the first search expedition, within 100m of the predicted site of the fall.

The meteorite appears to have been following an unusual orbit, or path around the Sun, prior to falling to Earth in July 2007, according to the researchers’ calculations.

The team believes that it started out as part of an asteroid in the innermost main asteroid belt between Mars and Jupiter.

It then gradually evolved into an orbit around the Sun that was very similar to Earth’s.

The new meteorite is also unusual because it is composed of a rare type of basaltic igneous rock.

According to the researchers, its composition, together with the data about where the meteorite comes from, fits with a recent theory about how the building blocks for the terrestrial planets were formed.

This theory suggests that the igneous parent asteroids for meteorites like today’s formed deep in the inner Solar System, before being scattered out into the main asteroid belt.

Asteroids are widely believed to be the building blocks for planets like the Earth, so the new finding provides another clue about the origins of the Solar System. (ANI)

Ancient Egyptian temples followed astronomy to set their calendars

London, September 9 (ANI): A new study has indicated that ancient Egyptian temples were aligned so precisely with astronomical events that people could set their political, economic and religious calendars by them.

According to a report in New Scientist, the study was of 650 temples, some dating back to 3000 BC.

For example, New Year coincided with the moment that the winter-solstice sun hit the central sanctuary of the Karnak temple in present-day Luxor, according to archaeological astronomer Juan Belmonte of the Canaries Astrophysical Institute in Tenerife, Spain.

Hieroglyphs on temple walls have hinted at the use of astronomy in temple architecture, including depictions of the “stretching of the cord” ceremony in which the pharaoh marked out the alignment for the temple with string.

But there had been little evidence to support the drawings.

Belmonte and Mosalam Shaltout of the Helwan Observatory in Cairo found that the temples are all aligned according to an astronomically significant event, such as a solstice or equinox, or the rising of Sirius, the brightest star in the sky.

“Somebody would have had to go to the prospective site during a solar, stellar or lunar event – as we did – to mark out the position that the temple axis should take,” Belmonte said.

“For the most important temples, this may well have been the pharaoh, as the temple drawings show,” he added. (ANI)

Chinese scientists claim to have filmed ‘UFO for 40 minutes’

London, Sep 7 (ANI): Chinese scientists claim that they filmed an unidentified flying object for about 40 minutes, during the solar eclipse on July 22.

Researchers at the Purple Mountain Observatory in Nanjing have said that they will spend the next 12 months studying the footage before reaching any conclusions.

In an interview with sina.com, Ji Hai-sheng, the director of the observatory, said that scientists would not be speculating publicly on the nature of what was captured on film until it had been properly studied.

“‘Purple Mountain Observatory and Chinese Academy of Sciences said that during the July 22 total solar eclipse observation, China had discovered near the sun, by observing staff, an unidentified object, it’s physical nature remains to be further studied,” the Telegraph quoted him as saying.

“Currently manpower is being organized to deal with this data, complete the data analysis and reveal the scientific results and this will take at least one year’s time to finalise,” he added.

The incident comes after a series of UFO sightings in China, which eventually led to the object being captured on film by students in Deqing.

The footage, featured on Chinese television, apparently shows the object repeatedly changing shape after initially appearing as a glowing blue sphere. (ANI)

Biggest earthquake in nine years hit Northeast

New Delhi, Sep 4 (ANI): A moderate earthquake measuring 5.9 on the Richter Scale, the biggest in nine years, shook the North-East early on Friday, officials at the Central Seismological Observatory said.

The quake took place at 1:21 a.m. local time and was centered 96 km east-southeast of Imphal, the capital of Manipur.

There were no reports of damage or causalities. This is the fourth time earthquakes hit the northeast region of India within a month’s time.

People ran out of their houses as the quake rocked buildings and houses triggering panic. There was, however, no damage to property, police said.

Te quake lasted for around 20 seconds; its after-shocks were felt for over two minutes.

Two moderate intensity quakes, one measuring 5.6 on the Richter Scale and another measuring 4.9 had shook the region on 12th August and 19th August. Another measuring 5.3 was recorded on 31st August. (ANI)

Now a model to predict when stock markets will crash

London, August 29 (ANI): A team of physicists and financiers have shown that it is possible to predict when growth in any stock exchange will become unsustainable and the market will crash, by successfully predicting a steep fall in the Shanghai Stock Exchange.

Used for the purpose was a model that employed concepts from the physics of complex atomic systems, developed by Didier Sornette of the Financial Crisis Observatory in Zurich, Switzerland, and Wei-Xing Zhou of the East China University of Science and Technology in Shanghai.

Sornette, Zhou, and colleagues have revealed that their idea was that if a plot of the logarithm of the market’s value over time would deviates upwards from a straight line, it’s a clear warning that people are investing simply because the market is rising rather than paying heed to the intrinsic worth of companies.

The researchers say that projecting this trend may be helpful in predicting when growth will become unsustainable, and the market will crash.

They applied their model to the Shanghai Composite Index, which tracks the combined worth of all companies listed on the Shanghai Stock Exchange, the world’s second largest.

The index gained 50 per cent in just four months earlier this year.

It was in July that the team predicted that the index would start to fall sharply by August 10, and the index duly began to slide on August 4, falling almost 20 per cent in the subsequent two weeks.

The researchers, however, warn that anyone hoping to exploit the model for profit should think twice.

“If enough investors take action based on our predictions, the evolution of prices will probably be affected,” New Scientist magazine quoted Zhou as saying. (ANI)

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Indian expedition to Antarctica approved

New Delhi, Aug 27 (ANI): The Cabinet Committee on Economic Affairs (CCEA) today accorded its approval for the continuation of the project “Polar Science; Expedition to Antarctica” during the XI Five Year Plan period at an estimated cost of Rs.230.01 crore.

The scientific expeditions which started in 1981 have contributed substantially to the growth of polar science in the country.

Experiments mounted by Indian scientists in disciplines such as atmospheric sciences and meteorology, earth sciences and glaciology, biology and environmental sciences have also contributed directly to global experiments mounted under the aegis of the Scientific Committee on Antarctic Research (SCAR).

The Indian Antarctic research base “Maitri” (70o 45′ 56.9″S : 11o 44′ 08.62″E) is one of the few active permanent research stations in the Central Donning Maudland (CDML) of East Antarctica from where systematic scientific experiments are conducted on a year-round basis.

The facilities available at this research base include a weather observatory, geomagnetic station; a permanent seismological observatory, GPS station, ice-core drilling facilities and laboratories for environmental, human health and communication research.

The entire activities related to the planning, coordination and implementation of the Indian Antarctic Programme is managed by the Ministry of Earth Sciences (MoES) through the National Centre for Antarctic and Ocean Research (NCAOR), Goa, an autonomous institute under the Ministry, established in 1998.

The objectives of this Programme are to continue the long-term scientific pursuits undertaken to understand the global processes and phenomena some of which are directly pertinent to our needs having potential applications.

The continuation emphasizes our perceptible and influential presence in Antarctica to uphold the country’s strategic interests in the Polar region and the surrounding oceans. (ANI)

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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)

‘Noisy’ stars mask planet’s true size

Sydney, July 10 (ANI): A German study has suggested that astronomers observing exoplanets around other stars may be underestimating their size because of active stars that add ‘noise’ to the observation of exoplanets using the transit method.

The transit method detects exoplanets as they pass in front of their parent star, reducing the amount of light reaching telescopes on, and orbiting, Earth.

Although the transit method isn’t the best method for detecting exoplanets, it provides a reliable estimate of its size and mass.

According to a report by ABC News, PhD student Stefan Czesla of the Hamburg Observatory in Germany, and colleagues, examined the giant exoplanet Corot-2b, using data from the French COROT satellite.

Discovered in 2007, Corot-2b is three and a half times the mass of Jupiter and orbits its star in just 1.74 days.

After closely examining the light curves recorded by COROT, which involved splitting them into their red, green and blue components, the researchers determined that the exoplanet is 3 percent bigger than previously thought.

Czelsa and colleagues believe this discrepancy may be true for other exoplanets around active stars.

“For planets found around active stars, the determination of their exact physical parameters is considerably complicated by stellar activity,” said Czesla.

“Bright and dark spots on the star can modify the transit light curves, something that isn’t accounted for in models currently used to calculate an exoplanet’s size,” he explained.

According to Dr John Greenhill of the University of Tasmania, the research also highlights the limitation of the transit method in detecting exoplanets, particularly those smaller than Jupiter.

“The two techniques that have netted the most planets, the radial velocity technique and the transit method, are limited by the noisiness of stars,” he said.

“In principle, it looks like we won’t be able to detect planets the size of Neptune and Uranus, and even Saturn using these methods because of that limit,” he added. (ANI)

Astronomers see high-speed galaxy collision in action

Washington, July 10 (ANI): Astronomers at the Chandra X-ray Observatory have spotted a galaxy collision in action, with one galaxy passing through the core of other galaxies at almost 2 million miles per hour.

The image obtained is of Stephan’s Quintet, a compact group of galaxies discovered about 130 years ago and located about 280 million light years from Earth.

Four of the galaxies in the group are visible in the optical image from the Canada-France-Hawaii Telescope.

A labeled version identifies these galaxies (NGC 7317, NGC 7318a, NGC 7318b and NGC 7319) as well as a prominent foreground galaxy (NGC 7320) that is not a member of the group.

The galaxy NGC 7318b is passing through the core of galaxies at almost 2 million miles per hour, and is thought to be causing the ridge of X-ray emission by generating a shock wave that heats the gas.

Additional heating by supernova explosions and stellar winds has also probably taken place in Stephan’s Quintet.

A larger halo of X-ray emission, detected by ESA’s (European Space Agency’s) XMM-Newton could be evidence of shock heating by previous collisions between galaxies in this group.

Some of the X-ray emissions are likely caused by binary systems containing massive stars that are losing material to neutron stars or black holes.

Stephan’s Quintet provides a rare opportunity to observe a galaxy group in the process of evolving from an X-ray faint system dominated by spiral galaxies to a more developed system dominated by elliptical galaxies and bright X-ray emission.

According to scientists, being able to witness the dramatic effect of collisions in causing this evolution is important for increasing the understanding of the origins of the hot, X-ray bright halos of gas in groups of galaxies.

Stephan’s Quintet shows an additional sign of complex interactions in the past, notably the long tails visible in the optical image.

These features were probably caused by one or more passages through the galaxy group by NGC 7317. (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)

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)

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)

“Cosmic blobs” a result of growing supermassive black holes

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Astronomers obtain first detection of magnetic field on bright star Vega

Paris, June 24 (ANI): Astronomers, using the NARVAL spectropolarimeter of the Bernard-Lyot telescope in France, have obtained the first detection of a magnetic field on the bright star Vega.

According to an article in the journal Astronomy and Astrophysics, astronomers clearly observe the magnetically-induced effect in the spectrum of Vega, thereby showing that the star possesses a magnetic field, something unknown so far.

Using the high-sensitivity NARVAL spectropolarimeter installed at the Bernard-Lyot telescope at the Pic du Midi Observatory in France, a team of astronomers detected the effect of a magnetic field (known as the Zeeman effect) in the light emitted by Vega.

Vega is a famous star among amateur and professional astronomers. Located at only 25 light years from Earth in the Lyra constellation, it is the fifth brightest star in the sky. It has been used as a reference star for brightness comparisons.

Vega is twice as massive as the Sun and has only one-tenth its age.

Because it is both bright and nearby, Vega has been often studied but it is still revealing new aspects when it is observed with more powerful instruments.

Vega rotates in less than a day, while the Sun’s rotation period is 27 days.

The intense centrifugal force induced by this rapid rotation flattens its poles and generates temperature variations of more than 1000 degrees Celsius between the polar (warmer) and the equatorial regions of its surface.

Astronomers analyzed the polarization of light emitted by Vega and detected a weak magnetic field at its surface.

This is really not a big surprise because one knows that the charged particle motions inside stars can generate magnetic fields, and this is how solar and terrestrial magnetic fields are produced.

However, for more massive stars than the Sun, such as Vega, theoretical models cannot predict the intensity and the structure of the magnetic field, so that astronomers had no clue to the strength of the signal they were looking for.

After many unsuccessful attempts in past decades, both the high sensitivity of NARVAL and the full dedication of an observing campaign to Vega have made this first detection possible.

he strength of Vega magnetic field is about 50 micro-tesla, which is close to that of the mean field on Earth and on the Sun.

This first observational constraint opens the way to in-depth theoretical studies about the origin of magnetic fields in massive stars.

Astronomers believe that this discovery will be a key step in understanding stellar magnetic fields and their influence on stellar evolution. (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)

Astronomers probe close to supermassive black hole’s edge

Paris, May 28 (ANI): Astronomers have used new data from ESA’s (European Space Agency’s) XMM-Newton spaceborne observatory, to probe closer than ever to a supermassive black hole lying deep at the core of a distant active galaxy.

The galaxy – known as 1H0707-495 – was observed during four 48-hr-long orbits of XMM-Newton around Earth, starting in January 2008.

The black hole at its center was thought to be partially obscured from view by intervening clouds of gas and dust, but these current observations have revealed the innermost depths of the galaxy.

“We can now start to map out the region immediately around the black hole,” said Andrew Fabian, at the University of Cambridge, who headed the observations and analysis.

X-rays are produced as matter swirls into a supermassive black hole.

The X-rays illuminate and are reflected from the matter before its eventual accretion. Iron atoms in the flow imprint characteristic iron lines on the reflected light.

XMM-Newton detected two bright features of iron emission in the reflected X-rays that had never been seen together in an active galaxy.

These bright features are known as the iron L and K lines, and they can be so bright only if there is a high abundance of iron.

Seeing both in this galaxy suggests that the core is much richer in iron than the rest of the galaxy.

The direct X-ray emission varies in brightness with time. During the observation, the iron L line was bright enough for its variations to be followed.

A painstaking statistical analysis of the data revealed a time lag of 30 seconds between changes in the X-ray light observed directly, and those seen in its reflection from the disc.

This delay in the echo enabled the size of the reflecting region to be measured, which leads to an estimate of the mass of the black hole at about 3 to 5 million solar masses.

The observations of the iron lines also reveal that the black hole is spinning very rapidly and eating matter so quickly that it verges on the theoretical limit of its eating ability, swallowing the equivalent of two Earths per hour.

This new technique will enable the astronomers to map out the process in all its glorious complexity, taking them to previously unseen regions at the very edges of this and other supermassive black holes. (ANI)

World’s largest space telescope aims to explore depths of the Universe

Berlin, May 12 (ANI): Herschel, the largest space telescope ever built, would explore the depths of the Universe, once it launches into orbit aboard the latest ESA (European Space Agency) mission on May 14th.

In 1.5 million kilometers distance from Earth, the space probe will orbit the Sun for 3 and a half years.

With its three instruments, it will especially detect and analyze infrared radiation, which contains information on a wide range of phenomena in the Universe, like the evolution of distant galaxies and the existence of water in our solar system.

The Universe reveals many of its secrets in the infrared.

Just like every object on Earth, the icy nebulae, galaxies and stars from the depths of the Universe emit infrared heat radiation.

The Earth’s atmosphere is impervious to these wavelengths.

The instruments aboard the Herschel space probe investigate space in the wavelength range between 55 and 672 micrometers.

No other infrared observatory so far has offered such a bandwidth in combination with the spatial resolution of a 3.5-meter telescope.

For the first time, the scientists are able to resolve the cosmic infrared background into its individual sources and thus to determine the development of the Universe.

The evolution of stars and galaxies, the formation of planetary systems, the history of our own solar system and the chemical composition of molecular clouds, stars and galaxies are the most important topics on which Herschel will provide information.

“With the start of this space telescope a dream comes true for which we have worked hard for more than ten years”, said Eckhard Sturm from Max Planck Institute (MPE).

“With Herschel, we will resolve the cosmic infrared background into individual galaxies and so be able to study the most active stage of star formation in the history of the Universe,” said Dieter Lutz, Sturm’s colleague.

Herschel also opens up new opportunities for our understanding of the trans-Neptunian region – remains of the disc from which our planets formed. (ANI)

Astronomers to search for precursors to life in cosmic dust

Washington, May 6 (ANI): A University of Michigan astronomer has decided to use the Herschel Space Observatory to study the organic molecules that make up life on Earth in new detail in the warm clouds of gas and dust around young stars.

The astronomer in question is Ted Bergin, an associate professor in the Department of Astronomy, University of Michigan.

He hopes to gain insights into how organic molecules form in space, and possibly, how life formed on Earth.

“The chemistry of space makes molecules that are the precursors of life. It’s possible that the Earth didn’t have to make these things on its own, but that they were provided from space,” said Bergin.

Herschel, a European Space Agency mission with NASA participation, is scheduled to launch on May 14.

An orbiting telescope that will unlock new wavelengths on the electromagnetic spectrum, it will allow astronomers to observe at the far-infrared wavelengths where organic molecules and water emit their chemical signatures.

“We’ll be studying the full extent of chemistry in space and we hope to learn what types of organics are out there as a function of their distance from a star,” Bergin said. “And we want to understand the chemical machinery that led to the formation of these organics,” he added.

In faraway galaxies and stellar nurseries, astronomers have detected complex organic sugar and hydrocarbon molecules that are key components in chlorophyll in plants and RNA.

Bergin expects to detect tens if not hundreds of these kinds of compounds – some of which have never been found before outside the Earth. (ANI)