First results on impact of large celestial body on Jupiter

Washington, May 20 (ANI): Scientists have published the first results dealing with the impact of a celestial body on the planet Jupiter last July.

The results of the research, conducted by Planetary Sciences Group at the UPV/EHU-University of the Basque Country with its headquarters at the Faculty of Engineering in Bilbao and led by Professor Agustín Sánchez Lavega, have appeared in Astrophysical Journal Letters.

An amateur Australian astronomer came across the presence of a large, black spot close to the polar region of the planet Jupiter, the biggest in the Solar System, on July 19, 2009.

The impact had taken place at a very high latitude close to the planet”s South Pole barely 3 or 4 hours before the spot was seen on Jupiter”s dark side (at night), and this prevented it from being observed directly.

The trajectory was in the opposite direction of the fragments of the Shoemaker-Levy 9 comet that crashed into Jupiter exactly 15 years previously, in July 1994.

After the world”s large observatories had been alerted, the confirmation came through in a matter of hours that the spot consisted of the remains of ash left behind following the impact of a comet or asteroid.

The world”s main observatories, including the Hubble space telescope among others, immediately set about analysing the phenomenon.

After several months” work the first two papers dealing with the conclusions about the nature of the impact and its effect on the planet”s atmosphere have been published.

The University of the Basque Country”s Planetary Sciences Group has shared this science scoop with researchers from the United States.

According to the studies, the main spot, a very black cloud comprising the waste materials produced by the impact, reached a size of about 5,000 km in the atmosphere of Jupiter, even though it was surrounded by a halo caused by the falling of the material expelled from the atmosphere of up to 8,000 km, slightly smaller than the size of the Earth.

It is not known whether the thick cloud consisting of very fine particles (barely a thousandth of a millimetre) and very black, is a product of the waste materials of the object or whether these particles were produced by the extremely high temperatures generated by the impact in Jupiter”s atmosphere.

Over the days that followed the ash was blown by Jupiter”s winds -which are gentle at these latitudes- in a way similar to the ash being blown from the Icelandic volcano currently erupting.

There are doubts as to whether the celestial body that crashed onto the surface of Jupiter was a comet or an asteroid. Assuming that it was of a comet type, -in other words, mainly made up of ice substances-, the size of the meteorite would have been in the region of 500 metres.

This second clearly detected impact on Jupiter seems to suggest that objects ranging between 0.5 and 1 km in size fall onto the planet more frequently than originally thought: until now an impact was reckoned to take place on average once every 50 to 250 years, but with the new findings events like this one could well be occurring every 10 to 15 years.

The study of the impacts on planets helps us to get a better understanding of those that could happen on Earth. (ANI)

Hubble observes star eating a planet

Washington, May 21 (ANI): A new instrument on NASA’s Hubble Space Telescope, called the Cosmic Origins Spectrograph (COS), has observed that the hottest known planet in the Milky Way galaxy being eaten by its parent star.

The planet may only have another 10 million years left before it is completely devoured.

The planet, called WASP-12b, is so close to its Sun-like star that it is superheated to nearly 2,800 degrees Fahrenheit and stretched into a football shape by enormous tidal forces.

The atmosphere has ballooned to nearly three times Jupiter’s radius and is spilling material onto the star.

The planet is 40 percent more massive than Jupiter.

This effect of matter exchange between two stellar objects is commonly seen in close binary star systems, and this is the first time it has been seen so clearly for a planet.

“We see a huge cloud of material around the planet which is escaping and will be captured by the star. We have identified chemical elements never before seen on planets outside our own solar system,” said team leader Carole Haswell of The Open University in Great Britain.

A study last year predicted that the planet’s surface would be distorted by the star’s gravity, and that gravitational tidal forces make the interior so hot that it greatly expands the planet’s outer atmosphere.

Now Hubble has confirmed this prediction.

WASP-12 is a yellow dwarf star located approximately 600 light-years away in the winter constellation Auriga.

The exoplanet was discovered by the United Kingdom’s Wide Area Search for Planets (WASP) in 2008.

The automated survey looks for the periodic dimming of stars from planets passing in front of them, an effect called transiting.

The hot planet is so close to the star it completes an orbit in 1.1 days.

The unprecedented ultraviolet (UV) sensitivity of COS enabled measurements of the dimming of the parent star’s light as the planet passed in front of the star.

The UV spectral observations showed that absorption lines from aluminum, tin, manganese, among other elements became more pronounced as the planet transited the star, meaning that these elements exist in the planet’s atmosphere as well as the star’s.

The fact the COS could detect these features on a planet offers strong evidence that the planet’s atmosphere is greatly extended because it is so hot.

The UV spectroscopy was also used to calculate a light curve to precisely show just how much of the star’s light is blocked out during transit.

The depth of the light curve allowed the COS team to accurately calculate the planet’s radius.

They found that the UV-absorbing exosphere is much more extended than that of a normal planet that is 1.4 times Jupiter’s mass.

It is so extended that the planet’s radius exceeds its Roche lobe, the gravitational boundary beyond which material would be lost forever from the planet’s atmosphere.

The results were published in the latest issue of The Astrophysical Journal Letters. (ANI)

Amateur astronomers and Cassini spacecraft capture Saturn storm

Washington, Apr 30 (ANI): For the first time, amateur astronomers used the composite infrared spectrometer instrument aboard NASA’s Cassini spacecraft to look at a massive blizzard in Saturn’s atmosphere.

The instrument collected the most detailed data to date of temperatures and gas distribution in that planet’s storms.

The data showed a large, turbulent storm, dredging up loads of material from the deep atmosphere and covering an area at least five times larger than the biggest blizzard in this year’s Washington, D.C.-area storm front nicknamed “Snowmageddon.”

“We were so excited to get a heads-up from the amateurs. Data from the storm cell would have been averaged out,” said Gordon Bjoraker, a composite infrared spectrometer team member based at NASA’s Goddard Space Flight Center in Greenbelt, Md. Normally.

Cassini’s radio and plasma wave instrument and imaging cameras have been tracking thunder and lightning storms on Saturn for years in a band around Saturn’s mid-latitudes nicknamed “storm alley.”

But storms can come and go on a time scale of weeks, while Cassini’s imaging and spectrometer observations have to be locked in place months in advance.

The radio and plasma wave instrument regularly picks up electrostatic discharges associated with the storms, so team members have been sending periodic tips to amateur astronomers, who can quickly go to their backyard telescopes and try to see the bright convective storm clouds.

Amateur astronomers including Anthony Wesley, Trevor Barry and Christopher Go got one of those notices in February and were able to take dozens of pictures over the next several weeks.

In late March, Wesley sent Cassini scientists an e-mail with a picture of the storm.

“I wanted to be sure that images like these were being seen by the Cassini team just in case this was something of interest to be imaged directly by Cassini or the Hubble Space Telescope,” wrote Wesley.

Cassini scientists eagerly pored through the images, including a picture of the storm at its peak on March 13 by Go, who lives in the Philippines.

And luckily, the composite infrared spectrometer happened to be targeting the latitude of the storms.

The instrument’s scientists knew there could be storms there, but didn’t know when they might be active.

Data obtained by the spectrometer on March 25 and 26 showed larger than expected amounts of phosphine, a gas typically found in Saturn’s deep atmosphere and an indicator that powerful currents were dredging material upward into the upper troposphere.

The spectrometer data also showed another signature of the storm: the tropopause, the dividing line between the serene stratosphere and the lower, churning troposphere, was about 0.5 Kelvin (1 degree Fahrenheit) colder in the storm cell than in neighboring areas.

“A balloonist floating about 100 kilometers down from the bottom of
Saturn’s calm stratosphere would experience an ammonia-ice blizzard with the intensity of Snowmageddon. These blizzards appear to be powered by violent storms deeper down — perhaps another 100 to 200 kilometers down — where lightning has been observed and the clouds are made of water and ammonia,” said Brigette Hesman, a composite infrared spectrometer team member who is an assistant research scientist at the University of Maryland. (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)

Hubble celebrates 20 years of launch

Washington, April 24 (ANI): The starry-eyed Hubble Space Telescope is today celebrating 20 years of awe and discovery – after it was launched on April 24, 1990.

Exactly two decades ago the Space Shuttle and crew of STS-31 were launched to deploy the NASA/ESA”s now famous space observatory into a low-Earth orbit.

Hubble”s unprecedented capabilities have made it one of the most powerful science instruments ever conceived by humans, and certainly the one most embraced by the public.

Its discoveries have revolutionised nearly all areas of current astronomical research, from planetary science to cosmology.

At times Hubble”s space odyssey has went on with broken equipment, a bleary-eyed primary mirror and even a Space Shuttle rescue/repair mission cancellation.

But the ingenuity and dedication of Hubble scientists, engineers, and NASA and ESA astronauts have allowed the observatory to rebound time and time again.

Its crisp vision continues to challenge scientists with exciting new surprises and to enthral the public with ever more evocative colour images.

NASA, ESA and the Space Telescope Science Institute (STScI) are celebrating Hubble”s journey of exploration with a stunning new picture.

Another exciting component of the anniversary will be the launch of the revamped European website for Hubble, spacetelescope.org.

ESA will also be sponsoring the Hubble Pop Culture Contest that calls for fans to search for examples of the observatory”s presence in everyday life.

The brand new Hubble anniversary image highlights a small portion of one of the largest observable regions of starbirth in the galaxy, the Carina Nebula.

Towers of cool hydrogen laced with dust rise from the wall of the nebula.

The scene is reminiscent of Hubble”s classic Pillars of Creation photo from 1995, but even more striking in appearance.

The image captures the top of a pillar of gas and dust, three light-years tall, which is being eaten away by the brilliant light from nearby bright stars.

The pillar is also being pushed apart from within, as infant stars buried inside it fire off jets of gas that can be seen streaming from towering peaks like arrows sailing through the air.

To date, Hubble has looked at over 30 000 celestial targets and amassed over half a million pictures in its archive.

The last heroic astronaut-servicing mission to Hubble in May 2009 made the telescope 100 times more powerful than when it was launched. (ANI)

Galaxy merger dilemma solved

Washington, April 21 (ANI): A long-standing dilemma about the mass of infrared bright merging galaxies has finally been solved by scientists at the Naval Research Laboratory (NRL).

Dr. Barry Rothberg along with Dr. Jacqueline Fischer used new data from the 8-meter Gemini-South telescope in Chile along with earlier results from the W. M. Keck-2 10-meter and University of Hawaii 2.2-meter telescopes in Hawaii and archival data from the Hubble Space Telescope, to solve the problem.

Galaxies in the Universe generally come in two shapes, spiral, like our own Milky Way, and elliptical, in which the stars move in random orbits.

The largest galaxies in the Universe are elliptical in shape and how they formed is central to our understanding how the Universe has evolved over the last 15 billion years.

The long-standing theory has been that spiral galaxies merge with each other forming most of the elliptical galaxies in the Universe.

Spiral galaxies contain significant amounts of cold hydrogen gas. When they merge, the beautiful spiral patterns are destroyed and the gas is converted into new stars and with it, large amounts of dust. The dust is heated by the young stars and radiates energy at infrared wavelengths.

Until recently scientists thought that these infrared bright merging galaxies were not massive enough to be the precursors of most elliptical galaxies in the Universe.

The conventional method of measuring mass in dusty IR-bright galaxies uses near-infrared light, which can penetrate dust, to measure the random motions of old-stars.

The larger the random motions, the more mass is present. When spirals merge, gas from both galaxies forms a central rotating disk which then forms new stars.

These young stars outshine the old stars at near-infrared wavelengths making it appear as if the old stars have less random motion. Rothberg and Fischer instead observed the random motions of old stars at shorter wavelengths effectively using the dust to block the light from the young stars.

Their new results showed that the old stars in merging galaxies have large random motions, which means they will eventually become very massive elliptical galaxies.

The new research has been published in the Astrophysical Journal. (ANI)

Awesome power of supermassive black holes revealed

Washington, April 17 (ANI): Nottingham University researchers have shed new light on the super destructive capacity of black holes.

For the study, Asa Bluck in the School of Physics and Astronomy and colleagues, used images of unprecedented depth and resolution from the Hubble Space Telescope and the Chandra X-Ray Observatory to detect black holes in distant galaxies.

Scientists looked for galaxies emitting high levels of radiation and x-rays – a classic signature of black holes devouring gas and dust through accretion, or attracting matter gravitationally.

As this matter swirls around the event horizon of a black hole it heats up and radiates energy – as an accretion disc.

In supermassive black holes this radiation can reach huge proportions, emitting X-ray radiation in far greater quantities then is emitted by the rest of the objects in the galaxy combined – meaning that the black hole ”shines” far brighter than the entire galaxy it lies at the heart of.

In fact, the amount of energy released is sufficient to strip the galaxy of gas at least 25 times over.

Results have also demonstrated that the vast majority of the X-ray radiation present in the universe is produced in these accretion discs surrounding supermassive black holes, with a small proportion produced by all other objects, including galaxies and neutron stars.

The accretions discs surrounding supermassive black holes produce so much energy that they heat up the cold gases lying at the heart of massive galaxies.

The accretion disc shines across all wavelengths – from radio waves to gamma waves.

This speeds up the random motions of the gas, making it rise in temperature and pushing it away from the galactic centre, where it becomes less dense.

Gas needs to be cold and dense to collapse under gravity to form new stars, this resulting hot, low-density material must cool down before gravity will take effect – a process which would take longer than the age of the universe to achieve.

Old stars are therefore left to die out with no new stars replacing them, leaving the galaxy to grow dark and die.

And by pushing gas away from the galactic centre, the accretion disc starves the supermassive black hole of new material to devour, leading to its eventual demise.

Asa Bluck, a PhD student at the University and a Fellow of the Royal Astronomical Society, said: “It”s thought that black holes form inside their host galaxies and grow in proportion to them, forming an accretion disc which will eventually destroy the host. In this sense they can be described as viral in nature.

“Massive galaxies are in the minority in our visible universe – about one in a thousand galaxies is thought to be massive, but it may be much less. And at least a third of these have supermassive black holes at their centre. That”s why it”s so interesting that this type of black hole produces most of the X-ray light in the universe. They are the minority but they dominate energy output.”

The study, a collaboration between researchers at The University of Nottingham and Imperial College London, was presented at the Royal Astronomical Society National Astronomy Meeting in Glasgow. (ANI)

Astronomers confirm Einstein’s theory of general relativity

Washington, March 26 (ANI): An international team of astronomers has confirmed Albert Einstein’s theory of general relativity and that the expansion of the universe is accelerating after looking at data from the largest-ever survey conducted by the Hubble Space Telescope.

The astronomers studied more than 446,000 galaxies to map the matter distribution and the expansion history of the universe.

This study enabled them to observe precisely how dark matter evolved in the universe and to reconstruct a three-dimensional map of the dark matter and use this to test Albert Einstein’s theory of general relativity.

“Our results confirmed that there is an unknown source of energy in the universe which is causing the cosmic expansion to speed up, stretching the dark matter further apart exactly as predicted by Einstein’s theory,” said Van Waerbeke, an associate professor in the Dept. of Physics and Astronomy.

Einstein’s theory of general relativity predicts that space and time is a soft geometrical structure of which the shape and evolution are entirely determined by the matter within it.

Scientists posit that the universe is composed of dark matter and normal matter with a third constituent called “dark energy,” which over the past two billion years has been the force behind the accelerated expansion of the universe.

“The data from our study are consistent with these predictions and show no deviation from Einstein’s theories,” said Van Waerbeke, who is also a scholar in the Cosmology and Gravity program of the Canadian Institute for Advanced Research. (ANI)

Teledyne Infrared Sensors Survey the Universe

THOUSAND OAKS, Calif.–(Business Wire)–
Teledyne Technologies Incorporated (NYSE:TDY) announced today that its
subsidiary, Teledyne Scientific & Imaging, LLC (TS&I), has a key role in NASA`s
Wide-field Infrared Survey Explorer (WISE), with two of Teledyne`s megapixel
imaging sensors at the heart of the WISE infrared camera. The mission will be
the most sensitive infrared survey ever made of the universe.

Operating in a sun-synchronous low Earth orbit, WISE is designed to scan the
entire sky in infrared light, picking up the glow of hundreds of millions of
objects and producing millions of images. It is anticipated that objects never
seen before will be discovered, including the coolest stars, the universe`s most
luminous galaxies and some of the darkest near-Earth asteroids and comets. Its
vast catalogs will help answer fundamental questions about the origins of
planets, stars and galaxies, and provide a mountain of data for astronomers to
mine for decades to come. The WISE catalog will guide the observations of the
Hubble Space Telescope (HST), ground-based observatories, and the James Webb
Space Telescope (JWST).

The WISE observatory is hundreds of times more sensitive than previous space
missions due in part to its advanced detector technology. There are four
megapixel infrared sensors in WISE and Teledyne provided two of them (each is
1024×1024 pixels). The Teledyne sensors detect light at bands centered at 3.4
and 4.6 microns; 5 to 7 times longer than the longest wavelengths that can be
detected by the human eye. At these wavelengths, WISE will detect the thermal
emission of cooler objects, such as brown dwarf stars, and will see the visible
light from distant galaxies that has been stretched into infrared wavelengths by
the expansion of the universe (known as “redshift”).

The Teledyne infrared detectors are made from an advanced detector technology
pioneered by Teledyne called “substrate-removed HgCdTe.” The detector material
is a crystal lattice that is specially grown from the elements mercury, cadmium
and tellurium. This type of detector provides improved infrared sensitivity with
the lowest noise, vital for detecting the faint signals from distant objects.
Teledyne`s sensors with this advanced technology have already been critical to
the success of several NASA missions. A megapixel sensor was installed in May
2009 in the HST Wide Field Camera 3 (WFC3) instrument, a combined
visible-infrared sensor operated in the Moon Mineralogy Mapper that discovered
water on the moon, and fifteen 4-megapixel sensors from Teledyne will be used in
the JWST. Teledyne`s substrate-removed HgCdTe focal plane array is the baseline
technology for several future space astronomy and Earth observation missions,
and is now the standard for ground-based astronomy.

The most sensitive infrared surveys of the universe must be made from space to
avoid the high level of infrared light produced by the Earth`s atmosphere and to
avoid the absorption of infrared light by the atmosphere. In spite of the
limitations of ground-based observations, the most thorough all-sky infrared
survey to date has been the Two Micron All-Sky Survey (2MASS) that was conducted
by the University of Massachusetts and the California Institute of Technology
during 1997-2001. The 2MASS used telescopes located in Arizona and Chile with
the largest infrared arrays that were available at the time; each infrared
camera had three Teledyne sensors of 256×256 pixels, one-sixteenth the size of
the WISE sensors. 2MASS produced a catalog of over 500 million objects that has
guided infrared astronomy for the past decade.

JPL manages WISE for NASA`s Science Mission Directorate. The mission was
competitively selected under NASA`s Explorers Program, which NASA`s Goddard
Space Flight Center in Greenbelt, Md., manages. The Space Dynamics Laboratory in
Logan, Utah, built the science instrument, and Ball Aerospace & Technologies
Corp. of Boulder, Colo., built the spacecraft. Science operations and data
processing take place at the Infrared Processing and Analysis Center at the
California Institute of Technology in Pasadena. Caltech manages JPL for NASA.
For more information about WISE, visit http://www.nasa.gov/wise and
http://wise.astro.ucla.edu and http://www.jpl.nasa.gov/wise.

Teledyne Technologies is a leading provider of sophisticated electronic
components, instrumentation and communication products, engineered systems,
aerospace engines, and energy and power generation systems. Teledyne
Technologies` operations are primarily located in the United States, the United
Kingdom and Mexico. For more information, visit Teledyne Technologies` website
at www.teledyne.com.

Teledyne Technologies Incorporated
Investor Contact:
Jason VanWees, 805-373-4542
or
Media Contact:
Robyn E. McGowan, 805-373-4540

Copyright Business Wire 2010

Rejuvenated Hubble captures images of eerie “pillar of creation” and “butterfly” nebula

Washington, September 10 (ANI): NASA’s Hubble Space Telescope, which has been declared fully rejuvenated, has captured colorful, multi-wavelength pictures of far-flung galaxies, a densely packed star cluster, an eerie “pillar of creation,” and a “butterfly” nebula.

Hubble’s suite of new instruments allows it to study the universe across a wide swath of the light spectrum, from ultraviolet all the way to near-infrared.

In addition, scientists released spectroscopic observations that slice across billions of light-years to probe the cosmic-web structure of the universe and map the distribution of elements that are fundamental to life as we know it.

“This marks a new beginning for Hubble,” said Ed Weiler, associate administrator for NASA’s Science Mission Directorate at NASA Headquarters in Washington. The telescope was given an extreme makeover and now is significantly more powerful than ever, well-equipped to last into the next decade,” he added.

The new instruments are more sensitive to light and, therefore, will improve Hubble’s observing efficiency significantly.

It is able to complete observations in a fraction of the time that was needed with prior generations of Hubble instruments.

The space observatory today is significantly more powerful than it ever has been.

“The targets we’ve selected to showcase the telescope reveal the great range of capabilities in our newly upgraded Hubble,” said Keith Noll, leader of a team at the Space Telescope Science Institute in Baltimore, which planned the early release observations.

These results are compelling evidence of the success of the STS-125 servicing mission in May, which has brought the space observatory to the apex of its scientific performance.

Two new instruments, the Wide Field Camera 3 and Cosmic Origins Spectrograph, were installed, and two others, the Advanced Camera for Surveys and Space Telescope Imaging Spectrograph, were repaired at the circuit board level.

Hubble now enters a phase of full science observations.

Observations will range from studying the population of Kuiper Belt objects at the fringe of our solar system to surveying the birth of planets around other stars and probing the composition and structure of extrasolar planet atmospheres.

There are ambitious plans to take the deepest-ever near-infrared portrait of the universe to reveal never-before-seen infant galaxies that existed when the universe was less than 500 million years old.

Other planned observations will attempt to shed light on the behavior of dark energy, a repulsive force that is pushing the universe apart at an ever-faster rate. (ANI)

Warped debris disks around stars a result of interstellar wind

Washington, August 29 (ANI): In a new research, a team of scientists has determined that the warped shapes of the dust-filled disks where new planets may be forming around other stars, may be due to interstellar wind.

The dust-filled disks where new planets may be forming around other stars occasionally take on some difficult-to-understand shapes.

Now, a team led by John Debes at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, has found that a star’s motion through interstellar gas can account for many of them.

“The disks contain small comet- or asteroid-like bodies that may grow to form planets,” Debes said. “These small bodies often collide, which produces a lot of fine dust,” he added.

As the star moves through the galaxy, it encounters thin gas clouds that create a kind of interstellar wind.

“The small particles slam into the flow, slow down, and gradually bend from their original trajectories to follow it,” said Debes.

Far from being empty, the space between stars is filled with patchy clouds of low-density gas.

When a star encounters a relatively dense clump of this gas, the resulting flow produces a drag force on any orbiting dust particles.

The force only affects the smallest particles – those about one micrometer across, or about the size of particles in smoke.

“This fine dust is usually removed through collisions among the particles, radiation pressure from the star’s light and other forces,” explained Debes. “The drag from interstellar gas just takes them on a different journey than they otherwise would have had,” he said.

Working with Alycia Weinberger at the Carnegie Institution of Washington and Goddard astrophysicist Marc Kuchner, Debes was using the Hubble Space Telescope to investigate the composition of dust around the star HD 32297, which lies 340 light-years away in the constellation Orion.

He noticed that the interior of the dusty disk – a region comparable in size to our own solar system – was warped in a way that matched a previously known warp at larger distances.

“Other research indicated there were interstellar gas clouds in the vicinity. The pieces came together to make me think that gas drag was a good explanation for what was going on,” Debes said.

“It looks like interstellar gas helps young planetary systems shed dust much as a summer breeze helps dandelions scatter seeds,” Kuchner said.

As dust particles respond to the interstellar wind, a debris disk can morph into peculiar shapes determined by the details of its collision with the gas cloud. (ANI)

Future astronauts may be sent to ‘gravity holes’

London, August 29 (ANI): If scientists have their way, then space missions in the future might see astronauts being sent to ‘gravity holes’.

Gravitational “sweet spots” called Lagrange points lie at least 1 million kilometres away.

These points are great swathes of space where the gravitational acceleration from the Earth and the sun are exactly equal, letting objects stick there with very little effort.

Because they’re far from warm stars and planets, they make useful havens for ultra-cold telescopes that measure fluctuations in the temperature of deep space.

The Wilkinson Microwave Anisotropy Probe (WMAP), which measures radiation from the big bang, is located at a Lagrange point called L2 more than 1 million kilometres away.

The successor to the Hubble Space Telescope, the massive James Webb Space Telescope, will also be sent to the spot, which lies in line with the sun and Earth.

“If you look at our list of future space telescope concepts, just about all of them are going to go to L2,” said Dan Lester of the University of Texas, Austin. “That’s going to be a very busy place out there,” he added.

But what would humans do there?

According to a report in New Scientist, one useful task is repairing and upgrading the new telescopes, like astronauts have done five times with Hubble.

“If we want to have humans having anything to do with these new telescopes, we really have to think about Lagrange points,” Lester said.

Astronauts may not have to go as far as L2 to be useful.

Lagrange points exist in the Earth-moon system, and every other planet in the solar system also boasts Lagrange points with the sun.

It takes surprisingly little energy to travel between these points, because massive bodies like the sun and planets have gravitational fields that resemble mountains and hills, but Lagrange points are all at gravitational lowlands.

Once set on the right path, spacecraft can coast along the gravitational contours of space between these lowlands, as if travelling on an interplanetary superhighway.

“Going back and forth between Earth-sun Lagrange points and Earth-moon Lagrange points is pretty much a matter of giving the thing a swift kick,” Lester told New Scientist.

Future astronauts could repair telescopes at a staging area at the nearest Earth-moon Lagrange point and send them sailing back to L2 when they’re done.

They could also assemble large telescopes or spaceships at the staging area and then send them out to farther-flung destinations.(ANI)

Astronomers spot a pair of solar systems in the making

Washington, July 2 (ANI): Two University of Hawaii astronomers have found a binary star-disk system in which each star is surrounded by the kind of dust disk that is frequently the precursor of a planetary system, which makes them solar systems in the making.

The astronomers in question are doctoral student Rita Mann and Dr. Jonathan Williams, who used the Submillimeter Array on Mauna Kea, Hawaii, to make the observations.

A binary star system consists of two stars bound together by gravity that orbit a common center of gravity.

Most stars form as binaries, and if both stars are hospitable to planet formation, it increases the likelihood that scientists will discover Earth-like planets.

This binary system, 253-1536, stands out as the first known example of two optically visible stars, each surrounded by a disk with enough mass to form a planetary system like our own.

It lies 1,300 light-years from Earth, in the famous Orion Nebula, the kind of rich cluster of stars that is a common birth environment for most stars in our Milky Way galaxy, including our Sun.

One of the disks was discovered in an image taken with the Hubble Space Telescope, but the other disk was hidden in the glare of the star.

Hubble saw only the disk shadow, so the amount of material and its capability for planet formation was unknown until the UH team made the SMA observations.

The two stars are 400 times farther from each other than Earth is from the Sun.

They would take 4,500 years, or about the length of human recorded history, to complete one orbit around their common center.

Both stars are only about a third the mass of our Sun and are much cooler and redder in color.

The larger disk in 253-1536 is also the most massive found in the Orion Nebula so far.

The discovery of this massive disk and the binary disk system improve our understanding of how common planet formation is in our Galaxy and place our Solar System in context. (ANI)

Hubble Servicing Mission 4 comes to an end with successful landing

Washington, May 25 (ANI): The historic and successful Hubble Servicingission 4 – the fifth and final visit of the Space Shuttle to the NASA/ESA Hubble Space Telescope – came to an end with a perfect landing at Edwards Air Force Base in California on Sunday.

During a series of unprecedented spacewalks, Space shuttle Atlantis’ astronauts replaced and repaired a total of four instruments.

The Wide Field Camera 3 and Cosmic Origins Spectrograph were installed and the Advanced Camera for Surveys and Space Telescope Imaging Spectrograph were successfully repaired.

Servicing Mission 4 was an intense, 13-day undertaking that revitalized Hubble, making the telescope more capable than ever.

All mission objectives were accomplished during five spacewalks that totalled 36 hours, 56 minutes.

“This is not the end of the story but the beginning of another chapter of discovery by Hubble,” said Ed Weiler, associate administrator for Science at NASA Headquarters.

“Hubble will be more powerful than ever, continue to surprise, enlighten, and inspire us all and pave the way for the next generation of observatories,” Weiler added. (ANI)

Hubble Servicing Mission 4 comes to an end with successful landing

Washington, May 25 (ANI): The historic and successful Hubble Servicing Mission 4 – the fifth and final visit of the Space Shuttle to the NASA/ESA Hubble Space Telescope – came to an end with a perfect landing at Edwards Air Force Base in California on Sunday.

During a series of unprecedented spacewalks, Space shuttle Atlantis’ astronauts replaced and repaired a total of four instruments.

The Wide Field Camera 3 and Cosmic Origins Spectrograph were installed and the Advanced Camera for Surveys and Space Telescope Imaging Spectrograph were successfully repaired.

Servicing Mission 4 was an intense, 13-day undertaking that revitalized Hubble, making the telescope more capable than ever.

All mission objectives were accomplished during five spacewalks that totalled 36 hours, 56 minutes.

“This is not the end of the story but the beginning of another chapter of discovery by Hubble,” said Ed Weiler, associate administrator for Science at NASA Headquarters.

“Hubble will be more powerful than ever, continue to surprise, enlighten, and inspire us all and pave the way for the next generation of observatories,” Weiler added. (ANI)

Shuttle landing postponed again – NASA NEWS

Shuttle landing postponed again Washington – Inclement weather has forced the Atlantis space shuttle to forgo its initial attempt at a return to Earth Sunday, though three more chances remain, according to US space agency officials.

NASA, the US space agency, said that weather conditions remained too unstable at the Kennedy Space Centre in Florida for the first scheduled landing time, at 1411 GMT.

Of the three remaining windows of opportunity for a return on Sunday, two are at Edwards Air Force Base in California. It remains unclear if a Florida or California landing is more likely.

Bad weather canceled previous attempts at a return to Earth on Friday and Saturday. The shuttle has enough fuel to remain in orbit until Monday.

During its recent space mission, the crew of the shuttle conducted five spacewalks that added a new camera and spectograph to the Hubble Space Telescope, repaired other equipment and replaced its batteries and gyroscopes. (dpa)

CORRECTED – Astronauts tackle last items on Hubble fix-up list

Shuttle Atlantis astronauts returned to the Hubble Space Telescope on Monday for a final spacewalk to install fresh batteries, thermal shields and a sensor to pinpoint celestial targets for research.

Lead spacewalker John Grunsfeld and partner Andrew Feustel left the shuttle’s air lock at about 8:30 a.m. EDT (1230 GMT), almost an hour ahead of schedule.

“OK, Drew. Let’s go and be productive,” Grunsfeld said as they headed out toward Hubble.

Their primary job is to replace three of Hubble’s batteries and one of its star-tracking sensors, which are used to aim the observatory at celestial targets.

The astronauts also hope to make up some work left over from Sunday’s spacewalk by crew mates Michael Massimino and Michael Good, who battled stuck bolts and equipment glitches in their attempt to revive one of Hubble’s dead science instruments.

The Space Telescope Imaging Spectrograph, known as STIS, was used to hunt for black holes and probe the gas and dust between galaxies before a power failure shut it down in 2004.

Tests of the instrument showed the repair was successful, NASA spokesman Rob Navias said.

Grunsfeld and Feustel plan to replace the rest of Hubble’s batteries. Three of the six batteries were replaced on Thursday during the mission’s first spacewalk.

Swapping the remaining three will complete NASA’s primary goals for the mission, the fifth and final servicing call to Hubble before the shuttle fleet is due to be retired next year.

FRIDAY RETURN PLANNED

The Atlantis crew plans to release Hubble back into orbit on Tuesday and return to the Kennedy Space Center in Florida on Friday.

During four previous spacewalks, astronauts installed a new camera and light-splitting spectrograph, replaced Hubble’s positioning system, repaired two instruments and attached a docking ring so a robotic spacecraft can be sent to remove Hubble from orbit at the end of its operational lifetime.

The upgrades are expected to keep Hubble on the cutting edge of scientific exploration for at least five years so it can work in tandem with its replacement, the James Webb Space Telescope.

Grunsfeld and Feustel also hope to have enough time to install metal shields over the telescope’s instrument bays to help protect the observatory from the harsh environment of space. One of the shields was scheduled to be attached on Sunday, but the astronauts ran out of time.

NASA designed covers for three areas of the telescope and hopes to get to at least two of them on Monday.

Spacewalkers tackle final Hubble fix-up tasks

Astronauts finished the last of five complex spacewalks to refurbish the Hubble Space Telescope on Monday, leaving the 19-year-old instrument at the height of its star-gazing prowess.

Three earlier spacewalks during the shuttle Atlantis’ 11-day servicing mission to the bus-sized telescope were beset by frozen bolts and balky equipment that left astronauts cursing and ground controllers scrambling to improvise solutions.

But John Grunsfeld and Andrew Feustel’s seven-hour house call to Hubble on Monday went so smoothly that NASA added a final task: replacing some of the telescope’s thermal insulation.

It was the last time that human hands will ever likely touch Hubble, due to NASA’s plans to retire the shuttle fleet next year.

NASA hopes the improvements will keep Hubble operational until at least 2014 so it can work in tandem with its replacement, the James Webb Space Telescope.

“Hey John, you guys have had a great set of spacewalks. Come on in,” shuttle Commander Scott Altman told Grunsfeld after he and Feustel replaced batteries and a sensor on Hubble.

“I’m on my way,” Grunsfeld said.

Before returning to Atlantis’ airlock, Grunsfeld gave a farewell to Hubble that resembled an address to an old friend.

“I want to wish Hubble its’ own set of adventures and with the new instruments we’ve installed that it may unlock further mysteries of the universe,” Grunsfeld said.

The telescope is now “more powerful then ever” and has the ability to divine the mass of black holes and sample the composition of distant planets, said Jennifer Wiseman, chief of exoplanet and stellar astrophysics at NASA’s Goddard Space Flight Center.

“It’s almost like starting with a brand-new observatory,” Wiseman said.

The scientific gains came at a high cost in sweat and toil for Atlantis’ astronauts, who logged two of the longest spacewalks in NASA history on the Hubble mission.

On two spacewalks, astronauts removed dozens of tiny screws and clamored inside the telescope’s body to remove razor-sharp computer circuit boards that were never designed to be repaired in space, a task that NASA officials likened to brain surgery.

The Atlantis crew plans to release Hubble back into orbit on Tuesday and return to the Kennedy Space Center in Florida on Friday.

Hubble has helped rewrite astronomy text books. Among its key contributions are the discovery that the universe is expanding at an increasingly fast rate and that galaxies formed relatively soon after the Big Bang explosion that created the universe 13.7 billion years ago.

(Additional reporting by Irene Klotz)

Astronauts release Hubble telescope back into space

Astronauts release Hubble telescope back into spaceRejuvenated by hours of repairs in space, the Hubble Space Telescope floated out of shuttle Atlantis’ cargo bay on Tuesday to reclaim its place as the world’s flagship observatory for astronomical research.

Atlantis astronauts spent more than 36 hours over five marathon spacewalks to make upgrades and outfit Hubble with new instruments. These included a panchromatic wide-field camera that should be able to see objects formed just 500 million years after the universe’s birth in the big bang explosion some 13.7 billion years ago.

Using the shuttle’s robot arm, astronaut Megan McArthur gently lifted the 13-tonne observatory from a work platform in Atlantis’ payload bay where it had been positioned since Wednesday.

Holding the telescope high overhead, she released Hubble at 8:57 a.m. EDT (1257 GMT) as the spacecraft soared 350 miles (560 km) over the planet.

“There are folks who thought we couldn’t do this. They told us, ‘You’re too aggressive,’” said lead flight director Tony Ceccacci. “I don’t want to say, ‘We told you so,’ but, ‘We told you so.’”

Atlantis is due to land at the Kennedy Space Center in Florida on Friday.

Watching Hubble resume its solitary voyage in orbit was a bittersweet moment for the U.S. space agency, which has staged four previous shuttle missions to service the observatory, plus a 1990 flight to put it into orbit. The shuttle fleet is being retired next year.

The Atlantis crew completed everything NASA had planned, including the unprecedented repair of two science instruments not designed to be worked on in space. The astronauts, clad in bulky suits and gloves, sometimes struggled with the repair work, and were held up at times by stuck bolts.

‘SHOWTIME’

“It’s showtime for us now,” said Hubble program scientist Eric Smith. “We got everything we asked for.”

NASA plans to release the first images from the refurbished Hubble in September, following extensive tests of its cameras, light-splitting spectrographs and other systems.

“I truly believe this is a very important moment in human history, and I think it’s an important moment for science,” Hubble project scientist David Leckrone said.

“Just using what Hubble’s already done as a starting point, it’s unimaginable that we won’t dramatically go further than that,” he added.

Hubble already has changed astronomers’ understanding of how the universe formed and is evolving. It found ancient galaxies that formed well before scientists believed it was possible for them to exist.

It also provided evidence of an anti-gravity force known as “dark energy” that is inflating all of space at a faster and faster rate.

“There’s almost no area of astronomy that isn’t in some way significantly impacted by Hubble,” Leckrone said.

Added Smith, “I’m really looking forward to what comes next.”

Space shuttle readies for landing, watching weather

Space shuttle readies for landing, watching weatherSpace shuttle Atlantis prepared on Thursday to leave orbit after a successful mission that repaired the Hubble Space Telescope, but poor weather over Florida may delay Friday’s planned homecoming.

Shuttle Commander Scott Altman and his flight crew tested Atlantis’ rocket thrusters and other equipment needed to return through the atmosphere and land.

Touchdown is scheduled for 10 a.m. EDT (1400 GMT) on Friday at the Kennedy Space Center, with a back-up opportunity at 11:39 a.m. (1539 GMT)

The weather, however, may pose a problem. Powerful thunderstorms and heavy rain pummeled central Florida late on Wednesday, leaving cloudy skies and drizzle on Thursday that is expected to linger for several days.

Nevertheless, NASA told the astronauts to be ready to leave orbit in case the weather breaks.

“You know how the weather changes rapidly in Florida,” astronaut Greg Johnson told the crew from Mission Control in Houston. “We’ll plan as it comes.”

The shuttle has enough supplies to remain in orbit until Monday.

NASA said the shuttle is in good condition for landing following several inflight inspections of its heat shield by the crew. Heat shield damage is blamed for the 2003 Columbia disaster.

Atlantis is returning from NASA’s fifth and final servicing call to the 19-year-old Hubble telescope, which has been instrumental in expanding scientists’ understanding of the universe and widening public knowledge of astronomy.

GRUELING SPACEWALKS

Hubble’s unprecedented photographs of celestial objects include pictures of planetary nebula, which are colorful gas shells of exploded stars, and of a dizzying array of galaxies.

NASA is retiring the shuttle fleet next year and no other planned or existing spaceships have the capability of satellite servicing.

Working in teams of two, the Atlantis astronauts completed five occasionally grueling spacewalks to install new cameras, repair broken instruments and replace Hubble’s batteries and positioning gyroscopes.

The telescope also received fresh layers of thermal insulation and a docking ring so that a future spacecraft can hook up and steer the 13-ton observatory out of orbit toward its eventual final resting place in the ocean.

Without the servicing mission, Hubble’s effective operating days had looked short, with two of its main science instruments shut down by power failures and no gyroscopes to spare.

The spinning devices are needed to lock the telescope’s gaze on targets with the accuracy of a laser illuminating a coin several hundred miles (km) away.

The Atlantis crew’s refurbishments should keep the observatory on the cutting edge of scientific research until at least 2014 when its replacement, the infrared-sensitive James Webb Space Telescope, is scheduled to be in orbit.

“We all feel pretty good about what’s been accomplished,” Atlantis flight engineer Megan McArthur said during the crew’s inflight news conference on Wednesday. “But we’re also looking forward to taking a little bit of a break.”