Glistening galaxies tend to cluster in busiest parts of universe

Washington, May 20 (ANI): Glistening galaxies preferentially occupy regions of the universe containing more dark matter, astronomers have found.

Using a super-sensitive camera/spectrometer on the Herschel Space
Observatory, astronomers, including a UC Irvine team led by Asantha
Cooray, have mapped the skies as they appeared 10 billion years ago.

The UCI scientists found that these glistening galaxies preferentially occupy regions of the universe containing more dark matter and that collisions probably caused the abundant star production.

Cooray, associate professor and Chancellor”s Fellow in physics & astronomy, said: “Thanks to the superb resolution and sensitivity of the SPIRE [Spectral & Photometric Imaging Receiver] instrument on Herschel, we managed to map in detail the spatial distribution of massively star-forming galaxies in the early universe.

“All indications are that these galaxies are…crashing, merging, and possibly settling down at centers of large dark-matter halos.”

This information will enable scientists to adapt conventional theories of galaxy formation to accommodate the strange, star-filled versions.

The European Space Agency”s Herschel observatory carries the largest astronomical telescope operating in space today; it collects data at far-infrared wavelengths invisible to the naked eye.

One of three cameras on Herschel, SPIRE has let Cooray and colleagues survey large areas of the sky – about 60 times the size of the full Moon – in the constellations of Ursa Major and Draco.

The data analysed in this study was among the first to come from the Herschel Multi-Tiered Extragalactic Survey, the space observatory”s largest project. UCI is one of only four U.S. educational institutions involved in Herschel using the SPIRE instrument.

Seb Oliver, a University of Sussex professor who leads the survey, said: “It”s just the kind of thing we were hoping for from Herschel…and was only possible because we can see so many thousands of galaxies. It will certainly give the theoreticians something to chew over.”

The study will be published in a special issue of Astronomy & Astrophysics dedicated to the first scientific results from Herschel. (ANI)

The hidden side of star formation revealed

Washington, May 7 (ANI): ESA’s Herschel infrared space observatory has released new images that reveal previously hidden details of star formation.

One snapshot reveals what researchers called an ”impossible” star caught in the act of forming.

The images show thousands of these galaxies and beautiful star-forming clouds draped across the Milky Way.

The results, presented during a major scientific symposium held at the European Space Agency (ESA), challenge old ideas of star birth, and open new roads for future research.

Herschel’s observation of the star-forming cloud RCW 120 has revealed an embryonic star, which looks set to turn into one of the biggest and brightest stars in our Galaxy within the next few hundred thousand years.

It already contains eight to ten times the mass of the Sun and is still surrounded by an additional 2000 solar masses of gas and dust from which it can feed further.

“This star can only grow bigger. According to our current understanding, you should not be able to form stars larger than eight solar masses,” said Annie Zavagno, Laboratoire d’Astrophysique de Marseille.

Massive stars are rare and short-lived. To catch one during formation presents a golden opportunity to solve a long-standing paradox in astronomy.

This is because the fierce light emitted by such large stars should blast away their birth clouds before any more mass can accumulate. But somehow they do form.

Many of these ‘impossible’ stars are already known, some containing up to 150 solar masses, but now that Herschel has seen one near the beginning of its life, astronomers can use the data to investigate how it is defying their theories.

Herschel is the largest astronomical telescope ever to be placed into space. The diameter of its main mirror is four times larger than any previous infrared space telescope and one and a half times larger than Hubble. (ANI)

Scientists unveil largest atlas of nuclear galactic rings

Washington, Apr 30 (ANI): The most complete atlas of nuclear rings, enormous star-forming ring-shaped regions that circle certain galactic nuclei, has been unveiled by an international team of astrophysicists.

The catalogue, published in the Monthly Notices of the Royal Astronomical Society, includes 113 such rings in 107 galaxies.

“AINUR (the Atlas of Images of Nuclear Rings) is the most complete atlas of nuclear rings created to date”, Sébastien Comerón, a researcher at the Institute of Astrophysics of the Canary Islands (IAC), and co-author of the joint study with other scientists from the universities of La Laguna, Oulu (Finland) and Alabama (United States), tells SINC.

The atlas has just been published in the journal Monthly Notices of the Royal Astronomical Society, and covers 113 nuclear rings in 107 different galaxies. Six are dust rings in elliptical galaxies, while the rest (the majority) are star-forming rings in disc galaxies.

The nuclear rings are ring-shaped, star-forming configurations located around galactic nuclei. They range in size on average from between 500 to 3,000 light years, and they are very bright because they contain an abundance of young stars, including some extremely massive ones. This kind of star has a short lifetime but shines very brightly before exploding as a supernova.

To find the rings, the astrophysicists used images from around 500 galaxies observed by the Hubble space telescope, which belongs to NASA and the European Space Agency, as well as using other references. (ANI)

Venus still hot and active

The Earth’s nearest planetary neighbour might still be geologically active, according to a new study.

Venus is sometimes called Earth’s sister planet because they’re almost the same size and composition. But it’s a twisted sister, with temperatures hot enough to melt lead, sulphuric acid rain, and a crushing atmospheric pressure 100 times greater than Earth’s.

Now a team of scientists led by Dr Suzanne Smrekar from NASA’s Jet Propulsion Laboratory in California has found new evidence for recently active volcanoes on Venus.

Its report, which appears today in the journal Science, identifies hot spots on Venus that indicate young rocks with abnormally high level of heat compared to their surroundings.

“It shows the rocks haven’t degraded despite exposure to the harsh Venusian weather,” said Dr Smrekar.

“It means the hotspots are recently active volcanoes, with lava flows younger than 2.5 million years.”

Similar to Hawaii

Dr Smrekar and colleagues used surface heat data gathered by sensors aboard the European Space Agency’s Venus Express spacecraft.

Data collected by NASA’s Magellan spacecraft in the 1990s identified nine hot spots similar to those found on the islands of Hawaii.

Broad topographic rises and gravity anomalies found at these hot spots suggest there could be active mantle plumes close to the surface.

Using the visible and infrared thermal imaging spectrometer aboard Venus Express, Dr Smrekar’s team examined three of these hot spots.

“They’re places geologically like Hawaii, and so are the most likely sites for volcanic activity. They could be active now but there’s no evidence that they’re currently erupting,” Dr Smrekar said.

“The clue was finding basalt rock that hasn’t been weathered or chemically changed. Even on Earth when lava erupts on the surface, it interacts with the atmosphere and changes composition at the crust.

“On Venus, because it’s so hot with a dense carbon dioxide and sulphur dioxide atmosphere, we expect lava to quickly react when it hits the surface undergoing chemical and mineral changes.”

But Dr Smrekar says that process has not yet happened at these hot spots.

“We believe that means these are relatively fresh,” he said.

Because of the small number of impact craters on Venus, scientists know the planet’s surface is not much more than half a billion years old.

Dr Smrekar says that is a relatively young surface, like the Earth’s, and much younger than Mars. But unlike Earth, there is no evidence of plate tectonic activity on Venus or Mars.

“It means Venus is a lot like Earth, but not exactly the same. It’s kind of a laboratory for understanding how the Earth works,” she said.

“As we find more planets around other stars, maybe we’ll find out what’s more typical, Earth or Venus.”

Future mission

According to Dr Smrekar, a new mission to visit the surface of Venus is currently being considered for funding.

Called Surface and Atmospheric Geochemical Explorer (SAGE), the lander will have a tough time surviving the journey to the surface.

During the 1970s, a number of Soviet spacecraft landed on the Venusian surface, but lasted no more than a hour before being cooked and crushed in the hostile environment.

Dr Smrekar says SAGE could answer a number of questions relating to Venus and help scientists better understand data from orbiting spacecraft such as Venus Express.

A decision on SAGE is expected within a year.

New boreal forest biomass maps produced from radar satellite data

Paris, March 27 (ANI): A new processing algorithm has been developed using stacks of images from the Advanced Synthetic Aperture Radar (ASAR) on ESA’s (European Space Agency’s) Envisat satellite that allows for the retrieval of boreal forest biomass well beyond the levels that have been previously reported.

Forests play a crucial role in Earth’s carbon cycle by absorbing carbon from the atmosphere and storing it in biomass.

Undisturbed forests are carbon sinks as they absorb carbon, while forests that are logged or burnt down become carbon sources as they release carbon into the atmosphere.

Boreal forests and woodlands are estimated to cover approximately 14.5 percent of Earth’s land surface, comprising an area of nearly 16 million sq km (about the size of the contiguous 48 states of the US).

The boreal forest ecosystem, which spans Russia, northern Europe, Canada and Alaska, comprises interrelated habitats made up of forests, lakes, wetlands, rivers and tundra.

Boreal forests – including forest soil – store a third more carbon stocks per hectare as tropical forests, making them one of the most significant carbon sinks in the world.

These regions are considered global hotspots, that is, areas of increased warming, which represent possible important tipping points for abrupt climate change.

“Biomass, one of the most essential climate variables defining the functions of the Earth system, is the big unknown factor in the carbon cycle. Since no biomass maps exist with a high level of accuracy, we do not know how much is changing and cannot do calculations with any certainty,” said Professor Christiane Schmullius with the Friedrich Schiller University Jena.

“With this new algorithm, it is the first time that we have something in hand that may be a first step to a global biomass map,” she added.

The BIOMASAR project, sponsored by ESA’s Support to Science Element (STSE), has fully validated the algorithm using ASAR data, which is capable of acquiring images regardless of darkness and cloud cover, with existing in-situ information.

To validate the algorithm, several test sites were chosen in Scandinavia, Siberia and Canada, where both extensive datasets of ASAR images, acquired in ScanSAR mode at mid-resolution, and in-situ measurements were available.

The results show that the retrieval of forest growing stock volume (GSV) – the amount of wood expressed in cubic metres per hectare – is possible from Envisat ASAR data in boreal forests well beyond the levels that have been reported previously, that is, up to 500 cubic metres per hectare.

Using this method, Envisat archives can be exploited to generate global maps of GSV yearly over the entire boreal ecozone with a resolution of 10 km and accuracies of 20 percent. (ANI)

Hurtling star could fire comets at Earth!

London, March 16 (ANI): New calculations have suggested that a hurtling star is on its path to enter our solar system in about 1.5 million years, scattering millions of comets into paths that cross Earth’s orbit.

According to a report in New Scientist, Vadim Bobylev of the Pulkovo Observatory in St Petersburg, Russia, modelled the paths of neighbouring stars using data from the European Space Agency’s Hipparcos satellite and from ground-based measurements of the speeds of stars.

He found four previously unidentified stars that will pass within roughly 9.5 light years of Earth.

They will tug on the Oort cloud, a diffuse cloud of icy objects around the solar system thought to be a reservoir of comets.

However, the biggest threat comes from another star, Gliese 710, an orange dwarf now some 63 light years away but zooming our way at 14 kilometres per second.

Previous studies have suggested that Gliese 710 could pass through the Oort cloud in about 1.5 million years.

Bobylev’s calculations suggest that Gliese 710 has an 86 per cent chance of passing through the Oort cloud.

This could scatter millions of comets into paths that cross Earth’s orbit.

Fortunately, previous work on the effect of a star tangling with the Oort cloud hints the comets would arrive in a trickle, with only one entering an Earth-crossing orbit per year.

Gliese 710 also has a 1 in 10,000 probability of coming within 1000 astronomical units – 1 AU being the distance from the Earth to the sun.

Such a path could jostle objects in the Oort cloud, the Kuiper belt – a swarm of icy objects beyond Neptune’s orbit – as well as others that orbit in a disc between the two regions.

“The star could also change Neptune’s orbit a fraction,” said Paul Weissman of NASA’s Jet Propulsion Laboratory in Pasadena, California. “It would be a very significant event,” he added. (ANI)

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)

Solar wind strips off water from Venus

Washington, September 16 (ANI): Observations by the European Space Agency’s (ESA’s) Venus Express mission have provided strong new evidence that the solar wind has stripped away significant quantities of water from Earth’s twin planet Venus.

The SPICAV and VIRTIS instruments carried by the spacecraft have been used to measure concentrations of water vapor in the Venusian atmosphere at altitudes ranging from the lowest 10 km up to 110 km, high above the cloud tops.

Studies led by scientists from Belgium and Russia have found that the ratio of heavy water, which contains the isotope deuterium instead of hydrogen, to normal water is nearly twice as high above the clouds compared to its value in the lower atmosphere.

According to Dr. Emmanuel Marcq of the LATMOS laboratory in France, “Water vapor is a very rare species in the Venusian atmosphere: if it were in liquid form now, it would cover the surface of Venus with just a few centimeters of water. However, we believe Venus once had large volumes of water that have since escaped into space or stripped away by the solar wind.”

“These results from Venus Express demonstrate that the heavier water containing deuterium has not been able to escape Venus’s gravity as easily as normal H2O. This enrichment of heavy water provides strong evidence that water loss is occurring in the upper atmosphere and that Venus was probably more humid and Earth-like in the distant past,” he said.

Other studies by groups at the LESIA laboratory and the University of Oxford show that concentrations of water vapor decline from around 44 parts per million in the hot lower atmosphere to 25 parts per million at an altitude of 30-40 km.

At this level, the amounts of water vapor vary according to the overlying sulfuric acid cloud cover, with regions of thicker cloud containing less water vapor. (ANI)

Space Shuttle Discovery returns to Earth after successful mission

Washington, September 12 (ANI): Space shuttle Discovery and its crew of seven astronauts has returned to Earth after a successful mission called STS-128, in which the team delivered two refrigerator-sized science racks to the International Space Station (ISS).

One rack will be used to conduct experiments on materials such as metals, glasses and ceramics.

The results from these experiments could lead to the development of better materials on Earth. The other rack will be used for fluid physics research.

Understanding how fluids react in microgravity could lead to improved designs for fuel tanks, water systems and other fluid-based systems.

STS-128 Commander Rick Sturckow was joined on the mission by Pilot Kevin Ford, Mission Specialists Pat Forrester, Jose Hernandez, Danny Olivas and European Space Agency astronaut Christer Fuglesang.

NASA astronaut Nicole Stott flew to the complex aboard Discovery to begin a nearly three-month mission as a station resident, replacing Tim Kopra, who returned home on Discovery.

In addition to carrying a new station crew member, Discovery and the crew also delivered a new sleeping compartment, an air purification system and a treadmill named after comedian Stephen Colbert.

The mission included three spacewalks that replaced experiments outside the European Space Agency’s Columbus laboratory and an empty ammonia storage tank. eather concerns prevented the crew from returning to NASA’s Kennedy Space Center in Florida, the primary end-of-mission landing site.

In 7-10 days, Discovery will be transported approximately 2,500 miles from California to Florida on the back of a modified 747 jumbo jet.

Once at Kennedy, Discovery will be separated from the aircraft to begin processing for its next flight, targeted for March 2010. (ANI)

‘Smell of space’ strong, metallic and unique, say NASA astronauts

Washington, September 7 (ANI): NASA astronauts aboard the US space shuttle Discovery have said that the smell of space, which is regarded as the final frontier, is strong, metallic and unique.

“There is one smell up here that is really unique though and that is the smell, we just call it ‘the smell of space’,” said NASA engineer and astronaut Gregory Chamitoff, who is on board US space shuttle Discovery.

“I haven’t had a chance to do a spacewalk yet, but when the other guys did and they came back in, there’s this really, really strong metallic smell,” he added.

For rookie astronaut Kevin Ford, Discovery’s pilot, both the sounds and smells of space have surprised him.

“It’s like something I haven’t ever smelled before, but I’ll never forget it,” he said. “You know how those things stick with you,” he added.

Chamitoff and Ford are among 13 astronauts on board the International Space Station and US space shuttle Discovery.

Astronauts from Discovery have concluded a third and final spacewalk, installing new equipment on the International Space Station (ISS), though failing to connect some of the cables.

The spacewalkers deployed a new payload attachment system, replaced a failed gyro assembly, installed two GPS antennae and did some work to prepare for the installation of the Node 3 “Tranquility” module next year.

Built in Italy by the European Space Agency, Node 3 “Tranquility” is scheduled to be flown to the ISS next February.

It contains the most advanced life support systems designed to recycle waste water and generate oxygen. (ANI)

Scientists design “gravity tractor” to save earth from asteroids

London, Aug 30 (ANI): British space scientists have designed a special spacecraft that can save the earth from a catastrophic asteroid collision.

The 10 tonne spacecraft named “gravity tractor” would be deployed to intercept an asteroid en route to the earth and has the ability to fly 160 ft alongside it.

Once near an asteroid the craft will use gravitational force to pull the rock towards itself.

Gradually the gravity tractor will be able to change the asteroids path and thus make sure it misses the earth.

According to rough estimates of the American space agency NASA, there are more than 100,000 asteroids orbiting near the Earth and have the capacity to destroy cities.

The engineers of space company EADS Astrium, which designs crafts for NASA and the European Space Agency, have made the gravity tractor.

The team believes the craft could successfully divert the course of asteroids up to 430 yards across, which can release 100,000 times more than the Hiroshima bomb.

The Telegraph quoted Dr Ralph Cordey, science and exploration business development manager at Astrium as saying: “Anything bigger than 30m (32 yards) across is a real threat to the Earth.

“Unfortunately it is a matter of when rather than if one of them hits us.

“The gravity tractor exploits the principals of very basic physics – every object with a mass has its own gravity that affects objects around it. It can move fairly large objects 300 metres (984ft) to 400 metres (1,312ft) across.

“These asteroids are hurtling around our solar system at 10km per second, so when you scale that up, you just need a tiny nudge to send it off course.” (ANI)

NASA’s space shuttle Discovery launched successfully

Washington, August 29 (ANI): NASA’s space shuttle Discovery, with its seven-member crew, launched successfully from the space agency’s Kennedy Space Center in Florida on August 28.

The shuttle will deliver supplies, equipment and a new crew member to the International Space Station.

Inside the shuttle’s cargo bay is the Leonardo Multi-Purpose Logistics Module, a pressurized “moving van” that will be temporarily installed to the station.

The module will deliver storage racks; materials and fluids science racks; a freezer to store research samples; a new sleeping compartment; an air purification system; and a treadmill named after comedian Stephen Colbert.

The name “Colbert” received the most entries in NASA’s online poll to name the station’s Node 3. NASA named the node Tranquility.

Shortly before liftoff, Commander Rick Sturckow said, “Thanks to everyone who helped prepare for this mission. Let’s go step up the science on the International Space Station!”

The 13-day flight will include three spacewalks to replace experiments outside the European Space Agency’s Columbus laboratory, install a new ammonia storage tank and return the used one.

Ammonia is needed to move excess heat from inside the station to the radiators located outside.

Sturckow is joined on the STS-128 mission by Pilot Kevin Ford, Mission Specialists Pat Forrester, Jose Hernandez, Danny Olivas and European Space Agency astronaut Christer Fuglesang.

NASA astronaut Nicole Stott will fly to the complex aboard Discovery to begin a three-month mission as a station resident.

She replaces NASA’s Tim Kopra, who will return home on Discovery. Ford, Hernandez and Stott are first-time space fliers.

The mission marks the start of the transition from assembling the space station to using it for continuous scientific research.

Assembly and maintenance activities have dominated the available time for crew work.

As completion nears, additional facilities and the crew members to operate them will enable a measured increase in time devoted to research as a national and multinational orbiting laboratory.

Discovery’s first landing opportunity at Kennedy is scheduled for Thursday, Sept. 10.

This mission is the 128th space shuttle flight, the 30th to the station, the 37th for Discovery and the fourth in 2009. (ANI)

Mars simulation mission focuses on improving work performance on Red Planet

Washington, July 14 (ANI): A six-man international crew has completed a 105-day Mars simulation mission that was full of realistic scenarios, with experiments evaluating solutions to conditions that impact work performance.

The experiment was carried out in an isolation chamber in Moscow from March 31 to July 14.

The crew, composed of four Russians and two Europeans, simulated the 105-day Mars mission full of experiments and realistic mission scenarios, including emergency situations and 20-minute communications delays.

US participation in the mission consisted of three research teams with experiments evaluating solutions to conditions that impact work performance.

The projects evaluated lighting interventions to counter sleep disruption due to shift work or long hours, tested two objective methods of measuring the impact of stress and fatigue on performance, and assessed interactions between crew members and mission control.

“The mission allowed us to look at the feasibility of certain technologies developed for improving performance by deploying them in an extremely demanding work environment. In this realistic setting, will crews use the technologies and will we get good data?” said Dr. David F. Dinges, leader of the NSBRI group funded from University of Pennsylvania School of Medicine and Rutgers.

“Additional goals were to see how different mission situations affected the various performance measures and to evaluate whether the interventions could indeed improve performance,” he added.

The 105-Day Mars Mission, a partnership between Russia’s Institute of Biomedical Problems and the European Space Agency, is the precursor to a 520-Day mission scheduled for 2010.

The isolation facility consists of several interconnected, modules containing medical and scientific research areas, living quarters, a kitchen, greenhouse and exercise facility.

For researchers, the opportunity to run experiments in this type of environment was invaluable.

“We’ve done experiments in the sleep lab to test the efficacy of lighting interventions, but that is a highly controlled environment,” said Dr. Charles A. Czeisler, leader of the NSBRI project funded from Harvard Medical School, Brigham and Women’s Hospital, and University of Colorado.

“By transitioning studies into an operational environment, like the 105-Day Mission, we have the opportunity to learn how to best deploy interventions in a realistic mission setting. This analog is a great intermediate step before implementation on an actual spaceflight,” he added.

Participation from the crew and mission controllers was excellent. All three NSBRI projects received data throughout the mission.

Final data will be received in the coming weeks, and the teams will begin detailed data analysis. (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)

Astronomers discover new class of black holes

London, July 2 (ANI): An international team of astronomers has discovered a new class of black hole, more than 500 times the mass of the Sun.

Astronomers made the finding in a distant galaxy approximately 290 million light years from Earth.

Until now, identified black holes have been either super-massive in the centre of galaxies, or about the size of a typical star (between three and 20 Solar masses).

The new discovery is the first solid evidence of a new class of medium-sized black holes.

A black hole is a remnant of a collapsed star with such a powerful gravitational field that it absorbs all the light that passes near it and reflects nothing.

It had been long believed by astrophysicists that there might be a third, intermediate class of black holes, with masses between a hundred and several hundred thousand times that of the Sun.

However, such black holes had not been reliably detected until now.

The team, led by astrophysicists at the Centre d’Etude Spatiale des Rayonnements in France, detected the new black hole with the European Space Agency’s XMM-Newton X-ray space telescope.

“While it is widely accepted that stellar mass black holes are created during the death throes of massive stars, it is still unknown how super-massive black holes are formed,” said the lead author of the research paper, Dr. Sean Farrell, now based at the Department of Physics and Astronomy at the University of Leicester, UK.

“One theory is that super-massive black holes may be formed by the merger of a number of intermediate mass black holes. To ratify such a theory, however, you must first prove the existence of intermediate black holes,” he added.

“This is the best detection to date of such long sought after intermediate mass black holes. Such a detection is essential. While it is already known that stellar mass black holes are the remnants of massive stars, the formation mechanisms of supermassive black holes are still unknown,” said Farrell.

“The identification of HLX-1 is therefore an important step towards a better understanding of the formation of the super-massive black holes that exist at the centre of the Milky Way and other galaxies,” he added.

HLX-1 (Hyper-Luminous X-ray source 1), lies towards the edge of the galaxy ESO 243-49.

It is ultra-luminous in X-rays, with a maximum X-ray brightness of approximately 260 million times that of the Sun. (ANI)

Mars may have a water table hidden underground

London, June 27 (ANI): A new hypothesis has suggested that Mars may have a water table hidden underground, despite satellite data suggesting otherwise.

Today the small amount of water detected on the planet is locked in the polar ice caps, but recently discovered geological features suggest liquid water once flowed on its surface.

This could now be hiding beneath the rocky crust.

According to a report in New Scientist, the European Space Agency’s Mars Express satellite has used ground-penetrating radar in some areas to look for a water table but found no evidence for one, despite research that concluded any water would be found within 9 kilometres of the surface, which is well within the reach of the probe’s instruments.

Planetary scientist Bill Farrell of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and colleagues say that scientists should not give up the search for the Martian water table just yet.

The satellite’s radar signal should bounce back from shiny surfaces like water.

But, the team calculates that if the layer of rock and icy soil above the water table is particularly conductive, it could be absorbing enough energy from the radar to obscure a telltale signal.

According to Farrell, the work will be useful for missions to other icy bodies too.

“We don’t want future geologists to look at their radar data and say no reflectance means no aquifer,” he said. (ANI)

Astronaut to telecast freefall experiment via live link-up from space station

Paris, June 23 (ANI): ESA (European Space Agency) astronaut Frank De Winne, in a live link-up with the ISS (International Space Station), scheduled for September 21, will perform a simple experiment in space to demonstrate the effects of freefall.

The event is enabled by ESA’s Directorate of Human Spaceflight and its Erasmus Centre and will be co-hosted by four European science museums.

The ‘Take your classroom into space’ activity is one of several education activities planned during De Winne’s ongoing six-month OasISS mission on the International Space Station (ISS). e Winne is part of a crew of six living and working on the ISS.

De Winne will perform the curriculum-relevant demonstration inside the European Columbus laboratory using a standalone education kit.

The experiment was selected from ideas proposed by European educators in response to a call for experiments that can be carried out on the ISS to demonstrate the effects of freefall.

One of the two best experiment ideas, which were proposed independently by five teachers, ‘Do objects have weight in space?’ and ‘Exploring Capillarity’ will be demonstrated by De Winne during the live link-up.

Using the ‘Take your classroom into space’ Education Kit, which contains all the elements needed to perform the same demonstrations on the ground, secondary school students (14 to 18 years old) will compare their results with those obtained by De Winne in space, helping them to learn about the conditions of freefall.

During the live link-up with the Station, De Winne will also answer questions from the students.

The event will be co-hosted by four European science museums and centres located close to the home cities of the five teachers who proposed the winning ‘Take your classroom into space’ ideas. (ANI)

Herschel telescope obtains images of ‘whirlpool galaxy’ as first test observation

Paris, June 20 (ANI): Herschel, the largest infrared space telescope ever flown, has obtained images of the famous ‘whirlpool galaxy’ for a first test observation.

European Space Agency’s (ESA’s) Herschel opened its ‘eyes’ on June 14 and the Photoconductor Array Camera and Spectrometer obtained images of M51, which is popularly dubbed the ‘whirlpool galaxy’.

Scientists obtained images in three colours, which clearly demonstrate the superiority of Herschel, the largest infrared space telescope ever flown.

This image shows the ‘whirlpool galaxy’, first observed by Charles Messier in 1773, who provided the designation Messier 51 (M51).

This spiral galaxy lies relatively nearby, about 35 million light-years away, in the constellation Canes Venatici. M51 was the first galaxy discovered to harbour a spiral structure.

The image is a composite of three observations taken at 70, 100 and 160 microns, taken by Herschel’s Photoconductor Array Camera and Spectrometer (PACS) on June 14 and 15, immediately after the satellite’s cryocover was opened on June 14.

Herschel, launched only a month ago, is still being commissioned and the first images from its instruments were planned to arrive only in a few weeks.

But, engineers and scientists were challenged to try to plan and execute daring test observations as part of a ‘sneak preview’ immediately after the cryocover was opened.

The objective was to produce a very early image that gives a glimpse of things to come.

To the left is the best image of M51, taken by NASA’s Spitzer Space Telescope, with the Multiband Imaging Photometer for Spitzer (MIPS), juxtaposed with the Herschel observation on 14 and 15 June at 160 microns.

The obvious advantage of the larger size of the telescope is clearly reflected in the much higher resolution of the image. Herschel reveals structures that cannot be discerned in the Spitzer image.

These images clearly demonstrate that the shorter the wavelength, the sharper the image, which is a very important message about the quality of Herschel’s optics, since PACS observes at Hersche”s shortest wavelengths.

Produced from the very first test observation, these images lead scientists to conclude that the optical performance of Herschel and its large telescope is so far meeting their high expectations. (ANI)

Sun using Earth’s solar defense to steal its atmosphere

Washington, May 30 (ANI): A new study has suggested that the Sun is slowly stealing Earth’s atmosphere, with our planet’s main solar defense acting as a double agent, aiding and abetting the thievery.

According to a report in National Geographic News, typically hailed as a protective buffer from the sun’s brute power, Earth’s magnetosphere is actually helping the sun’s energized particles strip away a tiny fraction of Earth’s atmosphere.

“We’re, in fact, losing more oxygen and more hydrogen than even Venus is today,” said Chris Russell, a professor of space physics at the University of California, Los Angeles.

“We often tell our colleagues and ourselves that we are fortunate living on this planet, because we have this magnetic shield that protects us,” he added.

“It certainly does help, but we’ve come to the realization that, when it comes to the atmosphere, that’s not true,” he further added.

An international team of researchers has been tracking planetary atmospheres using the European Space Agency’s (ESA’s) Mars Express mission for Venus and Mars and NASA’s Small Explorer Mission (SMEX) for Earth.

SMEX also harbors an instrument for measuring magnetic activity on Earth.

“On Earth, the magnetosphere acts like an energy collector that interacts with the material that’s coming from the sun and can draw energy out of the solar wind,” Russell said.

But then, Earth’s magnetic field funnels and guides that energy to the upper atmosphere, heating the atmosphere and allowing bits of it to escape along the very same funnels that guided the energy in.

“The precise physics have yet to be worked out, but there’s no cause for alarm,” Russell said.

“At the current rate, our present atmospheric inventory can last at least until the sun-midway through its life now-turns into a red giant and engulfs Earth,” he explained.

“At that point, the loss of atmosphere becomes moot,” he added. (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)