Mysterious ‘dark flow’ might be tug of another Universe

Washington, March 19 (ANI): Scientists say that a mysterious dark cosmic flow, which is carrying along many galaxy clusters in the universe, might be the tug of another universe.

Recent research has found that the universe is not only expanding, it’s being swept along in the direction of constellations Centaurus and Hydra at a steady clip of one million miles per hour, pulled, perhaps, by the gravity of another universe.

Scientists have no idea what’s tugging at the known world, except to say that whatever it is likely dates back to the fraction of the second between the universe’s explosive birth 13.7 billion years ago and its inflation a split second later.

“At this point, we don’t have enough information to see what it is, or to constrain it. We can only say with certainty that somewhere very far away the world is very different than what we see locally. Whether it”s ‘another universe’ or a different fabric of space-time we don’t know,” Alexander Kashlinsky at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, told Discovery News.

Kashlinsky and colleagues have spent years building up evidence for what they call “the dark flow.”

They look at how the relic radiation from the Big Bang explosion scatters as it passes through gases in galaxy clusters, a process that is something akin to looking at stars through the bubble of Earth’s atmosphere.

With data on more than 1,000 galaxy clusters, including some as distant as 3 billion light-years from Earth, the measurements show the universe’s steady flow is clearly not a statistical fluke, according to Kashlinsky.

The force and direction of the flow holds steady across space and through time.

“It’s the same flow at a distance of a hundred million light-years as it is at 2.5 billion light-years and it points in the same direction and the same amplitude. It looks like the entire matter of the universe is moving from one direction to the next,” Kashlinsky said.

The observation fits theoretical models of how our universe might be impacted by sibling universes, predicted by string theory that we cannot directly detect.

It’s like our universe is a box and everything that it contains is inside it like milk in a carton, physicist Laura Mersini-Houghton with University of North Carolina at Chapel Hill, told Discovery News.

“If our universe is all that’s there, then the liquid in the box shouldn’t be sliding. Whatever is pulling it has to be bigger than the size of the box,” she said.

“There is a structure beyond the horizon of our universe and that structure is exerting a force on our universe and creating this flow,” she added. (ANI)

Lava carved ancient Martian riverbed

Washington, March 10 (ANI): A new American research has revealed that an ancient “riverbed” in Mars was not made by the flow of water but was carved by molten lava.

The 270-km long Martian channel near the Ascraeus Mons volcano does not seem to have been made by water.

“We started seeing that, instead of this [liquid] cutting into an existing surface, it was building a surface—it built a ridge up to 40 meters [130 feet] high” millions of years ago, explained study co-author Jacob Bleacher of NASA”s Goddard Space Flight Center in Greenbelt, Maryland.

The channel is also roofed over in some areas and lined with vents, characterises usually linked to lava tubes.

Bleacher said: “You don”t see this on Earth in [river] settings.

“But you see it all the time in volcanic settings. So that”s kind of our smoking gun.”

However, Bleacher, who presented his work last week at the 41st Lunar and Planetary Science Conference, said this does not mean water never existed on the red planet.

But it does mean scientists may have to reconsider when and where they believe water might have existed on Mars.

According to Laszlo Kestay, a planetary geologist on the NASA team that produced the new images of the channel, the findings are also exciting because they shed new light on Mars” volcanic history.

“I think there are some very clearly water-formed features on Mars, but there are other things that are more puzzling. Jake and colleagues make a very compelling case that at least this one is volcanic,” National Geographic News quoted Kestay, as saying.

And chances are bright that other channels in the Ascraeus Mons area will turn out to be lava-made as well, said Kestay, who works with the U.S. Geological Survey”s Astrogeology Science Center.

According to him, the new image data are “revealing not just these channels but a whole suite of smaller volcanic features and showing that volcanism is more widespread spatially than people thought.” (ANI)

Moon”s biggest crater exposes its hidden lower crust

Washington, March 5 (ANI): Reports indicate that the biggest and deepest crater on the Moon can provide glimpses of the hidden lower crust of Earth”s natural satellite.

Shortly after the Moon formed, an asteroid smacked into its southern hemisphere and gouged out a truly enormous crater, the South Pole-Aitken basin, almost 1,500 miles across and more than five miles deep.

Asteroid bombardment over billions of years has left the lunar surface pockmarked with craters of all sizes, and covered with solidified lava, rubble, and dust.

Glimpses of the original surface, or crust, are rare, and views into the deep crust are rarer still.

Fortunately, a crater on the edge of the South Pole-Aitken basin may provide just such a view.

According to Noah Petro of NASA”s Goddard Space Flight Center in Greenbelt, Maryland, “We believe the central part of the Apollo Basin may expose a portion of the Moon”s lower crust. If correct, this may be one of just a few places on the Moon where we have a view into the deep lunar crust, because it”s not covered by volcanic material as many other such deep areas are.”

“Just as geologists can reconstruct Earth”s history by analyzing a cross-section of rock layers exposed by a canyon or a road cut, we can begin to understand the early lunar history by studying what”s being revealed in Apollo,” he said.

Petro and his team made the discovery with the Moon Mineralogy Mapper (M3), a NASA instrument on board India”s Chandrayaan-1 lunar-orbiting spacecraft.

Analysis of the light (spectra) in images from this instrument revealed that portions of the interior of Apollo have a similar composition to the impact melt in the South Pole-Aitken (SPA) basin.

As you go deeper into the Moon, the crust contains minerals have greater amounts of iron. When the Moon first formed, it was largely molten.

Minerals containing heavier elements, like iron, sank down toward the core, and minerals with lighter elements, like silicon, potassium, and sodium, floated to the top, forming the original lunar crust.

“The asteroid that created the SPA basin probably carved through the crust and perhaps into the upper mantle. The impact melt that solidified to form the central floor of SPA would have been a mixture of all those layers,” said Petro.

“We expect to see that it has slightly more iron than the bottom of Apollo, since it went deeper into the crust. This is what we found with M3,” he said.

“However, we also see that this area in Apollo has more iron than the surrounding lunar highlands, indicating Apollo has uncovered a layer of the lunar crust between what is typically seen on the surface and that in the deepest craters like SPA,” he added. (ANI)

NASA’s lunar reconnaissance orbiter begins detailed mapping of moon’s south pole

Washington, September 18 (ANI): NASA’s Lunar Reconnaissance Orbiter, or LRO, has successfully completed its testing and calibration phase and entered its mapping orbit of the moon’s south pole.

The spacecraft already has made significant progress toward creating the most detailed atlas of the moon’s south pole to date.

“The LRO mission already has begun to give us new data that will lead to a vastly improved atlas of the lunar south pole and advance our capability for human exploration and scientific benefit,” said Richard Vondrak, LRO project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

LRO is scheduled for a one-year exploration mission in a polar orbit of about 31 miles above the lunar surface, the closest any spacecraft has orbited the moon.

During the next year, LRO will produce a complete map of the lunar surface in unprecedented detail, search for resources and safe landing sites for human explorers, and measure lunar temperatures and radiation levels.

“The LRO instruments, spacecraft, and ground systems continue to operate essentially flawlessly,” said Craig Tooley, LRO project manager at Goddard

“The team completed the planned commissioning and calibration activities on time and also got a significant head start collecting data even before we moved to the mission’s mapping orbit,” he added.

The south pole of the moon is of great interest to explorers because potential resources such as water ice or hydrogen may exist there.

Permanently shadowed polar craters that are bitterly cold at their bottoms may hold deposits of water ice or hydrogen from comet impacts or the solar wind.

The deposits may have accumulated in these “cold-trap” regions over billions of years.

If enough of these resources exist to make mining practical, future long-term human missions to the moon potentially could save the considerable expense of hauling water from Earth.

First results from LRO’s Lunar Exploration Neutron Detector, or LEND, indicate that permanently shadowed and nearby regions may harbor water and hydrogen.

According to the first measurements from the Diviner instrument, large areas in the permanently shadowed craters are about minus 400 degrees Fahrenheit (33 Kelvin), more than cold enough to store water ice or hydrogen for billions of years.

Additional observations will be needed to confirm this.

LEND relies on a decrease in neutron radiation from the lunar surface to indicate the presence of water or hydrogen.

“If these deposits are present, an analysis of them will help us understand the interaction of the moon with the rest of the solar system,” Vondrak said. (ANI)

NASA’s Swift satellite makes best-ever ultraviolet portrait of Andromeda galaxy

Washington, September 17 (ANI): NASA’s Swift satellite has acquired the highest-resolution view of a neighboring spiral galaxy ever attained in the ultraviolet.

The galaxy, known as M31 in the constellation Andromeda, is the largest and closest spiral galaxy to our own.

“Swift reveals about 20,000 ultraviolet sources in M31, especially hot, young stars and dense star clusters,” said Stefan Immler, a research scientist on the Swift team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

“Of particular importance is that we have covered the galaxy in three ultraviolet filters. That will let us study M31′s star-formation processes in much greater detail than previously possible,” he added.

M31, also known as the Andromeda Galaxy, is more than 220,000 light-years across and lies 2.5 million light-years away.

On a clear, dark night, the galaxy is faintly visible as a misty patch to the naked eye.

Between May 25 and July 26, 2008, Swift’s Ultraviolet/Optical Telescope (UVOT) acquired 330 images of M31 at wavelengths of 192.8, 224.6, and 260 nanometers.

The images represent a total exposure time of 24 hours.

The task of assembling the resulting 85 gigabytes of images fell to Erin Grand, an undergraduate student at the University of Maryland at College Park who worked with Immler as an intern this summer.

“After ten weeks of processing that immense amount of data, I’m extremely proud of this new view of M31,” she said.

Several features are immediately apparent in the new mosaic.

The first is the striking difference between the galaxy’s central bulge and its spiral arms.

“The bulge is smoother and redder because it’s full of older and cooler stars,” Immler explained. “Very few new stars form here because most of the materials needed to make them have been depleted,” he added.

Dense clusters of hot, young, blue stars sparkle beyond the central bulge.

M31′s disk and spiral arms contain most of the gas and dust needed to produce new generations of stars.

Star clusters are especially plentiful in an enormous ring about 150,000 light-years across.

“Swift is surveying nearby galaxies like M31 so astronomers can better understand star- formation conditions and relate them to conditions in the distant galaxies where we see gamma-ray bursts occurring,” said Neil Gehrels, the mission’s principal investigator at NASA Goddard. (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)

NASA scientist makes first full assessment of Africa’s mangrove forests

Washington, August 21 (ANI): A NASA scientist has made what is believed to be the first full assessment of the African continent’s mangrove forests.

Environmental scientist Lola Fatoyinbo of NASA’s Jet Propulsion Laboratory (JPL) developed and employed a method that can be used across the continent, overcoming expensive, ad hoc, and inconsistent modes of ground-based measurement.

“We’ve lost more than 50 percent of the world’s mangrove forests in a little over half a century; a third of them have disappeared in the last 20 years alone,” said Fatoyinbo, whose earlier study of Mozambique’s coastal forests laid the groundwork for the continent-wide study.

“Hopefully, this technique will offer scientists and officials a method of estimating change in this special type of forest,” she added.

Mangroves are the most common ecosystem in coastal areas of the tropics and sub-tropics.

The swampy forests are essential, especially in densely-populated developing countries, for rice farming, fishing and aquaculture (freshwater and saltwater farming), timber, and firewood.

Some governments also increasingly depend on them for eco-tourism.

The large, dense root systems are a natural obstacle that helps protect shorelines against debris and erosion.

Mangroves are often the first line of defense against severe storms, tempering the impact of strong winds and floods.

These coastal woodlands also have a direct link to climate, sequestering carbon from the atmosphere at a rate of about 100 pounds per acre per day, which is comparable to the per acre intake by tropical rainforests (though rainforests cover more of Earth’s surface).

“To my knowledge, this study is the first complete mapping of Africa’s mangroves, a comprehensive, historic baseline enabling us to truly begin monitoring the welfare of these forests,” said Assaf Anyamba, a University of Maryland-Baltimore County expert on vegetation mapping, based at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

Fatoyinbo’s research combines multiple satellite observations of tree height and land cover, mathematical formulas, and “ground-truthing” data from the field to measure the full expanse and makeup of the coastal forests.

Her measurements yielded three new kinds of maps of mangroves: continental maps of how much land the mangroves cover; a three-dimensional map of the height of forest canopies across the continent; and biomass maps that allow researchers to assess how much carbon the forests store.

“Beyond density or geographical size of the forests, the measurements get to the heart of the structure, or type, of mangroves,” explained Fatoyinbo. (ANI)

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

NASA and NOAA’S GOES-O satellite launched successfully

Washington, June 28 (ANI): The latest Geo-stationary Operational Environmental Satellite, GOES-O, soared into space Saturday after a successful launch from Space Launch Complex 37 at the Cape Canaveral Air Force Station in Florida.

The GOES-O spacecraft lifted off at 6:51 p.m. EDT on a Delta IV rocket.

The National Oceanic and Atmospheric Administration’s GOES-O satellite will improve weather forecasting and monitor environmental events around the world.

The satellite is the second to be launched in the GOES N series of geo-stationary environmental weather satellites.

“All indications are that GOES-O is in a normal orbit, with all spacecraft systems functioning properly,” stated Andre Dress, GOES deputy project manager at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

“We are proud of our support teams and pleased with the performance of the Delta IV launch vehicle,” he added.

Approximately four hours and twenty-one minutes after the launch, the spacecraft separated from the launch vehicle.

The Universal Space Network Western Australia tracking site in Dongara monitored the spacecraft separation.

On July 7, GOES-O will be placed in its final orbit and renamed GOES-14.

Approximately 24 days after launch, Boeing Space and Intelligence Systems will turn engineering control over to NASA.

About five months later, NASA will transfer operational control of GOES-14 to NOAA. The satellite will be checked out, stored in orbit and available for activation should one of the operational GOES satellites degrade or exhaust its fuel.

NASA contracted with Boeing to build and launch the GOES-O spacecraft.

NASA’s Launch Services Program at NASA’s Kennedy Space Center in Florida supported the launch in an advisory role.

The NOAA manages the GOES program, establishes requirements, provides all funding and distributes environmental satellite data for the United States.

Goddard procures and manages the design, development and launch of the satellites for NOAA on a cost-reimbursable basis. (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)

NASA’s lunar mission successfully enters Moon orbit

Washington, June 23 (ANI): NASA’s Lunar Reconnaissance Orbiter, or LRO, has successfully entered orbit around the moon after a four and a half day journey from the Earth.

Engineers at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, confirmed the spacecraft’s lunar orbit insertion at 6:27 a.m. EDT on Tuesday.

During transit to the moon, engineers performed a mid-course correction to get the spacecraft in the proper position to reach its lunar destination.

Since the moon is always moving, the spacecraft shot for a target point ahead of the moon.

When close to the moon, LRO used its rocket motor to slow down until the gravity of the moon caught the spacecraft in lunar orbit.

“Lunar orbit insertion is a crucial milestone for the mission,” said Cathy Peddie, LRO deputy project manager at Goddard.

“The LRO mission cannot begin until the moon captures us. Once we enter the moon’s orbit, we can begin to buildup the dataset needed to understand in greater detail the lunar topography, features and resources. We are so proud to be a part of this exciting mission and NASA’s planned return to the moon,” she added.

A series of four engine burns over the next four days will put the satellite into its commissioning phase orbit.

During the commissioning phase, each of its seven instruments is checked out and brought online.

The commissioning phase will end approximately 60 days after launch, when LRO will use its engines to transition to its primary mission orbit.

For its primary mission, LRO will orbit above the moon at about 31 miles, or 50 kilometers, for one year.

The spacecraft’s instruments will help scientists compile high resolution, three-dimensional maps of the lunar surface and also survey it at many spectral wavelengths.

The satellite will explore the moon’s deepest craters, examining permanently sunlit and shadowed regions, and provide understanding of the effects of lunar radiation on humans.

It is speculated that LRO will return more data about the moon than any previous mission. (ANI)

NASA’s new lunar mission to hunt for water on Moon

Washington, June 19 (ANI): NASA’s Lunar Reconnaissance Orbiter (LRO), which will hunt for water on the Moon, launched aboard an Atlas V rocket on June 18.

The satellite, launched from Cape Canaveral Air Force Station in Florida, will relay more information about the lunar environment than any other previous mission to the moon.

The spacecraft will be placed in low polar orbit about 31 miles, or 50 kilometers, above the moon for a one-year primary mission.

High-resolution imagery from LRO’s camera will help identify landing sites for future explorers and characterize the moon’s topography and composition.

The hydrogen concentrations at the moon’s poles will be mapped in detail, pinpointing the locations of possible water ice.

A miniaturized radar system will image the poles and test communication capabilities.

“During the 60 day commissioning period, we will turn on spacecraft components and science instruments,” explained Cathy Peddie, LRO deputy project manager at Goddard.

“All instruments will be turned on within two weeks of launch, and we should start seeing the moon in new and greater detail within the next month,” she added.

“We learned much about the moon from the Apollo program, but now it is time to return to the moon for intensive study, and we will do just that with LRO,” said Richard Vondrak, LRO project scientist at Goddard.

LRO’s instruments will help scientists compile high-resolution three-dimensional maps of the lunar surface and also survey it at many spectral wavelengths.

The satellite will explore the moon’s deepest craters, exploring permanently sunlit and shadowed regions, and provide understanding of the effects of lunar radiation on humans.

“Our job is to perform reconnaissance of the moon’s surface using a suite of seven powerful instruments,” said Craig Tooley, LRO project manager at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

“NASA will use the data LRO collects to design the vehicles and systems for returning humans to the moon and selecting the landing sites that will be their destinations,” he added.

“This is a very important day for NASA,” said Doug Cooke, associate administrator for NASA’s Exploration Systems Mission Directorate in Washington, which designed and developed both the LRO and LCROSS missions.

“We look forward to an extraordinary period of discovery at the moon and the information LRO will give us for future exploration missions,” he added.

All LRO initial data sets will be deposited in the Planetary Data System, a publicly accessible repository of planetary science information, within six months of launch. (ANI)

NASA’s new lunar mission to hunt for water on Moon

NASA’s new lunar mission to hunt for water on MoonWashington, June 19 : NASA’s Lunar Reconnaissance Orbiter (LRO), which will hunt for water on the Moon, launched aboard an Atlas V rocket on June 18.

The satellite, launched from Cape Canaveral Air Force Station in Florida, will relay more information about the lunar environment than any other previous mission to the moon.

The spacecraft will be placed in low polar orbit about 31 miles, or 50 kilometers, above the moon for a one-year primary mission.

High-resolution imagery from LRO’s camera will help identify landing sites for future explorers and characterize the moon’s topography and composition.

The hydrogen concentrations at the moon’s poles will be mapped in detail, pinpointing the locations of possible water ice.

A miniaturized radar system will image the poles and test communication capabilities.

“During the 60 day commissioning period, we will turn on spacecraft components and science instruments,” explained Cathy Peddie, LRO deputy project manager at Goddard.

“All instruments will be turned on within two weeks of launch, and we should start seeing the moon in new and greater detail within the next month,” she added.

“We learned much about the moon from the Apollo program, but now it is time to return to the moon for intensive study, and we will do just that with LRO,” said Richard Vondrak, LRO project scientist at Goddard.

LRO’s instruments will help scientists compile high-resolution three-dimensional maps of the lunar surface and also survey it at many spectral wavelengths.

The satellite will explore the moon’s deepest craters, exploring permanently sunlit and shadowed regions, and provide understanding of the effects of lunar radiation on humans.

“Our job is to perform reconnaissance of the moon’s surface using a suite of seven powerful instruments,” said Craig Tooley, LRO project manager at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

“NASA will use the data LRO collects to design the vehicles and systems for returning humans to the moon and selecting the landing sites that will be their destinations,” he added.

“This is a very important day for NASA,” said Doug Cooke, associate administrator for NASA’s Exploration Systems Mission Directorate in Washington, which designed and developed both the LRO and LCROSS missions.

“We look forward to an extraordinary period of discovery at the moon and the information LRO will give us for future exploration missions,” he added.

All LRO initial data sets will be deposited in the Planetary Data System, a publicly accessible repository of planetary science information, within six months of launch.

Scientists pinpoint the impact epicenter of earthbound space storms

Washington, May 29 (ANI): Using data from NASA’s THEMIS mission, a team of University of Alberta researchers has pinpointed the impact epicenter of an earthbound space storm as it crashes into the atmosphere, and given an advance warning of its arrival.

The team’s study reveals that magnetic blast waves can be used to pinpoint and predict the location where space storms dissipate their massive amounts of energy.

These storms can dump the equivalent of 50 gigawatts of power, or the output of 10 of the world’s largest power stations, into Earth’s atmosphere.

The energy that drives space storms originates on the Sun. The stream of electrically charged particles in the solar wind carries this energy toward Earth. The solar wind interacts with Earth’s magnetic field.

Scientists call the process that begins with Earth’s magnetic field capturing energy and ends with its release into the atmosphere a geomagnetic substorm.

“Substorm onset occurs when Earth’s magnetic field suddenly and dramatically releases energy previously captured by the solar wind,” said David Sibeck, project scientist for the Time History of Events and Macroscale Interactions During Substorms (THEMIS) mission at NASA Goddard Spaceflight Center in Greenbelt, Maryland.

Physicists Jonathan Rae and Ian Mann lead the University of Alberta research team that recently located a substorm’s epicenter of the impact.

The team uses ground-based observatories spread across northern Canada and the five satellites of the THEMIS mission to detect magnetic disturbances as storms crash into the atmosphere.

Using a technique the researchers call “space seismology,” they look for the eye of the storm hundreds of thousands of miles above Earth.

High-energy, electrically charged particles released by space storms can damage spacecraft.

On Earth, disturbances caused by the particles and the electrical currents they carry can interrupt radio communications and global positioning system (GPS) navigation, and damage electric power grids.

Rae and Mann’s team has also determined that the magnetic tremors show that the space storm impact into the atmosphere has a unique epicenter, with the eye of the storm located in space beyond the low-Earth orbits of most communication satellites.

Guided by Earth’s magnetic field, the magnetic tremors rocket through space toward Earth.

These geomagnetic substorms trigger magnetic sensors on the ground as they impact the atmosphere.

The effects of these storms, and the most spectacular displays of the Northern Lights, follow a few minutes later.

The objective of NASA’s pioneering multi-spacecraft THEMIS mission is to determine what causes geomagnetic substorms. (ANI)

NASA uses satellite to improve global crop forecasting

Washington, May 27 (ANI): NASA researchers are using satellite data to cultivate the most accurate estimates of soil moisture, which would improve global crop forecasting.

Soil moisture is essential for seeds to germinate and for crops to grow. But, record droughts and scorching temperatures in certain parts of the globe in recent years have caused soil to dry up, crippling crop production.

The falling food supply in some regions has forced prices upward, pushing staple foods out of reach for millions of poor people.

Now, NASA researchers are using satellite data to deliver a kind of space-based humanitarian assistance.

They are cultivating the most accurate estimates of soil moisture and improving global forecasts of how well food will grow at a time when the world is confronting shortages.

In this context, NASA scientist John Bolten described a new modeling product that uses data from the Advanced Microwave Scanning Radiometer for EOS (AMSR-E) sensor on NASA’s Aqua satellite to improve the accuracy of West African soil moisture.

The group produced assessments of current soil moisture conditions, or “nowcasts,” and improved estimates by 5 percent over previous methods.

“Though seemingly small and incremental, the increase can make a big difference in the precision of crop forecasts,” Bolten said.

The modeling innovation comes at a time when crop analysts at agencies like the U.S. Department of Agriculture (USDA) are working to meet the food shortage problem head on.

They combine soil moisture estimates with weather trends to produce up-to-date forecasts of crop harvests.

Those estimates help regional and national officials prepare for and prevent food crises.

“The USDA’s estimates of global crop yields are an objective, timely benchmark of food availability and help drive international commodity markets,” said Bolten, a physical scientist at NASA’s Goddard Space Flight Center, Greenbelt, Maryland.

Crop analysts must estimate root-zone soil moisture, the amount of water beneath the surface available for plants to absorb.

But estimating the amount of water in soil has posed challenges and data gaps.

Under a new NASA-USDA collaboration known as the Global Agriculture Monitoring Project, Bolten and colleagues from the USDA’s Agricultural Research Service are using AMSR-E to fill the data gaps with daily soil moisture “snapshots.”

Since its launch in 2002, the instrument has “seen” through clouds, and light vegetation like crops and grasses to detect the amount of soil moisture beneath Earth’s surface.

Bolten says that results from AMSR-E are just a precursor to dramatic new improvements in data and prediction accuracy researchers expect from the Soil Moisture Active and Passive satellite, slated to launch in 2013. (ANI)

NASA twin spacecraft may reveal how our moon was born

Washington, April 10 (ANI): Two identical NASA spacecraft are preparing to enter a point in the universe that may eventually answer the question of how our moon originated.

The spacecraft duet, called Solar Terrestrial Relations Observatory, or Stereo, are nearing a zone known as the Lagrangian points.

At these points, the gravity of the Sun and Earth combine to form gravitational wells where asteroids and space dust tend to gather.

The 18th-century mathematician Joseph-Louis Lagrange realized there were five such wells in the Sun-Earth system.

The twin probes are about to pass through two of them, named L4 and L5.

During their journey, the spacecraft will use a wide-field-of-view telescope to look for asteroids orbiting the region.

Scientists will be able to identify if a dot of light is an asteroid because it will shift its position against stars in the background as it moves in its orbit.

“These points may hold small asteroids, which could be leftovers from a Mars-sized planet that formed billions of years ago,” said Michael Kaiser, Stereo project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

According to Edward Belbruno and Richard Gott at Princeton University, about 4.5 billion years ago, when the planets were still growing, a hypothetical world called Theia may have been nudged out of L4 or L5 by the increasing gravity of other developing planets like Venus, sending it on a collision course with Earth.

“The resulting impact blasted the outer layers of Theia and Earth into orbit, which eventually coalesced under their own gravity to form the moon,” they added.

This concept is a modification of a scientific “giant impact” theory of the moon’s origin. The theory explains puzzling properties of the moon, such as its relatively small iron core.

At the time of the giant impact, Theia and Earth would have been large enough to be molten, enabling heavier elements, like iron, to sink to the center to form their cores.

An impact would have stripped away the outer layers of the two worlds, containing mostly lighter elements like silicon.

The moon eventually formed from this material. (ANI)

‘Halo effect’ causes formation of unusually bright patches of sky

London, March 31 (ANI): A new research has shown that unusually bright patches of sky, observed up to several kilometers away from clouds, are a result of the ‘halo effect’, which is light reflected off the cloud and bouncing off the particles in the air.

This seemingly innocuous finding could have a surprisingly big knock-on effect because it means there may be fewer cooling particles in the sky than previously thought, and that could change the way climate change is modeled.

According to a report in New Scientist, to discover why the air near clouds appears so aglow, Tamas Varnai and Alexander Marshak at the NASA Goddard Space Flight Center in Greenbelt, Maryland, used MODIS satellite observations from a piece of sky above the Atlantic just southeast of the UK.

To work out the amount of particles suspended in the air, Marshak’s team looked at the number of clear sky pixels picked up by MODIS and subtracted the reflection that was estimated to come from the planet’s surface and air molecules.

“This leaves us with the remaining reflection bouncing off aerosol particles, and so we can estimate their density,” explained Marshak.

Using this idea, it makes sense to assume that where the sky appears brighter, light must be being reflected off more or bigger aerosol particles.

In their current analysis, Marshak and Varnai found that the bright sky effect was stronger on the sunlit sides of clouds or when the clouds were denser.

Because more light reflects off a denser or sunlit cloud, this suggests that the clear sky brightness near clouds is caused by extra light reflecting off the clouds sideways and then scattering again between the particles in the clear sky area before reaching the satellite.

“It’s essentially extra energy bouncing off the clouds that enhances the glow of the clear sky,” he said.

This effect – called 3D radiative interaction – had been previously identified as a factor cranking up the sky’s brightness, but the new data elevates it to the most important factor.

This, in turn, means that many estimates of aerosol density may be plain wrong, because most clear sky analyses are close enough to clouds to be affected by the effect, according to Marshak.

“Overestimating aerosol density means that climate models will be wrong if they assume a certain amount of aerosol is needed, when in fact it is less,” said Varnai. (ANI)

Watery asteroids may explain why life is ‘left-handed’

London, March 17 (ANI): A new study has suggested that watery asteroids hurtling through the solar system gave a boost to left-handed proteins on Earth, which explains why life on our planet is ‘left-handed’.

Curiously, almost every living organism on Earth uses left-handed amino acids instead of their right-handed counterparts.

According to a report in New Scientist, the new research suggests that water on asteroids amplified left-handed amino acid molecules, making them dominate over their right-handed mirror images.

In the 1990s, scientists found that meteorites contain up to 15 percent more of the left version too.

That suggests space rocks bombarding the early Earth biased its chemistry so that life used left-handed amino acids instead of right.

“Meteorites would have seeded the Earth with some of the prebiotic compounds like amino acids that are needed to get life started, and also biased the origin of life to the left-handed amino acid form,” said Daniel Glavin at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

Some have suggested that polarized starlight preferentially destroyed right-handed amino acids on asteroids.

But, this alone couldn’t explain why the meteorite bias is so strong.

Now, Glavin and colleague Jason Dworkin have shown that water amplified the asymmetry.

They studied an amino acid called isovaline in six meteorites that showed evidence of ancient exposure to liquid water for about 1000 to 10,000 years.

The longer water persisted in the rock, the stronger its left-handed isovaline bias, the team found. (ANI)

Moon craters reveal history of 4-bln yr old asteroid bombardment in solar system

London, March 14 (ANI): A scientist is analyzing the age of craters found on the Moon in the 1990s to find out if they are the same age as the others, which would support the idea that asteroids bombarded the inner solar system about 4 billion years ago.

Most surveys of lunar impact craters have used photos, but Herbert Frey of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, wanted to know if there were any old craters buried beneath younger ones.

So, he studied elevation mapping data from the Clementine mission in the 1990s.

He also used simulations to identify impact signatures, such as a roughly circular crater with a thin crust and a thicker rim.

This approach uncovered 150 craters more than 300 kilometres wide instead of 45.

Frey is now trying to work out the age of the newly found craters. If they are the same age as the others, this would support the idea that asteroids bombarded the inner solar system for a particularly intense period about 4 billion years ago.

“Some esearchers think that life may have existed before this bombardment, but if so, its survival now seems less likely,” said Andrew Valley of the University of Wisconsin, Madison.

“The probability that early primitive life, if it existed, could find refuge, even in sediments beneath he ocean would be reduced,” he added.

Other researchers, however, disagree, arguing that life could have survived the barrage of impacts deep underground.

Frey, who will present the work at the Lunar and Planetary Science Conference in Woodlands, Texas, later this month, expects more subtle features to be discovered when the Asian lunar probes release further data and NASA’s Lunar Reconnaissance Orbiter launches in May. (ANI)

NASA’s Fermi Telescope obtains best ever view of gamma rays in space

Washington, March 12 (ANI): Astronomers have developed a new map combining nearly three months of data from NASA’s Fermi Telescope to obtain the best-ever view of gamma rays in space.

To Fermi’s eyes, the universe is ablaze with gamma rays from sources ranging from within the solar system to galaxies billions of light-years away.

“Fermi has given us a deeper and better-resolved view of the gamma-ray sky than any previous space mission,” said Peter Michelson, the lead scientist for the spacecraft’s Large Area Telescope (LAT) at Stanford University, California.

“We’re watching flares from supermassive black holes in distant galaxies and seeing pulsars, high-mass binary systems, and even a globular cluster in our own,” he added.

“This is the mission’s first major science product, and it’s a big step toward producing our first source catalog later this year,” said David Thompson, a Fermi deputy project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

The LAT scans the entire sky every three hours when operating in survey mode, which is occupying most of the telescope’s observing time during Fermi’s first year of operations.

These snapshots let scientists monitor rapidly changing sources.

The all-sky image shows how the cosmos would look if our eyes could detect radiation 150 million times more energetic than visible light.

The view merges LAT observations spanning 87 days, from August 4 to October 30, 2008.

The map includes one object familiar to everyone: the sun.

“Because the sun appears to move against the background sky, it produces a faint arc across the upper right of the map,” Michelson explained.

During the next few years, as solar activity increases, scientists expect the sun to produce growing numbers of high-energy flares.

“No other instrument will be able to observe solar flares in the LAT’s energy range,” said Michelson.

To better show individual sources, the new map was processed to suppress emissions from gas in the plane of our galaxy, the Milky Way.

As a way of underscoring the variety of the objects the LAT is seeing, the Fermi team created a “top ten” list comprising five sources within the Milky Way and five beyond our galaxy.

The top sources within our galaxy include the sun; a star system known as LSI +61 303, which pairs a massive normal star with a superdense neutron star; PSR J1836+5925, which is one of many new pulsars, a type of spinning neutron star that emits gamma-ray beams; and the globular cluster 47 Tucanae, a sphere of ancient stars 15,000 light-years away. (ANI)