“Ancient city of ”modern” galaxies” discovered

Washington, May 12 (ANI): Astronomers led by Texas A&M scientists have identified what may be called the “ancient city of ”modern” galaxies”.

The group of roughly 60 galaxies, called CLG J02182-05102, is nearly 10 billion years old, and possibly the earliest, most distant cluster of galaxies ever detected.

However, it”s not the size nor the age of the cluster that amazes the team of researchers led by Dr. Casey Papovich, an assistant professor in the Texas A&M Department of Physics and Astronomy and member of the George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy.

Rather, it”s the surprisingly modern appearance of CLG J02182-05102 that has them baffled – a huge, red collection of galaxies typical of only present-day galaxies.

Papovich said: “It”s like we dug an archaeological site in Rome and found pieces of modern Rome amongst the ruins.”

While its neighbouring galaxies appear vastly smaller and far fainter, Papovich says CLG J02182-05102 stands out as a densely populated bundle of ancient galaxies.

Enormous red galaxies at the centre contain almost 10 times as many stars as our Milky Way, he notes, combining for a total size that rivals that of the most monstrous galaxies of our nearby universe.

Before now, Papovich says, such a finding would be considered by many astronomers to be highly unlikely, considering the time frame in which they were found.

Papovich said: “The predictions are that these things should be very rare when the universe was 4 billion years old, and yet, we found them.

“Not only did we find them, it looks for all intents and purposes like they had already formed completely and evolved into the large concentrations of galaxies that we see in clusters today.”

Exactly why these particular galaxies are fully formed that early is what Papovich and his collaborators – which include astronomers from NASA”s Jet Propulsion Laboratory at the California Institute of Technology (Caltech) as well as Carnegie Observatories – hope to one day uncover, but for now, studying CLG J02182-05102 could help them and other researchers better understand how galaxies form and cluster in general.

The study will appear in Astrophysical Journal. (ANI)

‘Potentially dangerous’ asteroid spotted passing Earth on April 19

Washington, April 30 (ANI): An asteroid on the list of potentially dangerous space passed Earth last week at a distance of 1.5 million miles.

The near-Earth asteroid named 2005 YU55 was observed with the Arecibo Telescope’s planetary radar on April 19, 2010, according to Michael Nolan, director of the Arecibo Observatory.

The Arecibo telescope is located in Arecibo, Puerto Rico, and it is managed by Cornell University on behalf of the National Science Foundation.

Arecibo radar imaging of 2005 YU55 at 25-ft resolution showed that this asteroid is about 400 meters (1,300 feet) in size — about a quarter-mile long — and about twice as large as previously estimated.

This object is on the list of “potentially hazardous asteroids” maintained by the Minor Planet Center, of the Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass.

High-precision radar astrometry reduced orbit uncertainties by 50 percent. This improvement eliminated any possibility of an impact with the Earth for the next 100 years, and it was removed from the “Risk Page” maintained by NASA’s Near-Earth Object Program Office at the Jet Propulsion Laboratory.

After circling the Sun, 2005 YU55 will next approach the Earth to about 0.8 lunar distances on Nov. 8, 2011. It will pose no impact hazard at that time. Robert McMillan of the Spacewatch asteroid detection program discovered the asteroid on December 28, 2005.

President Barack Obama has proposed that NASA’s ‘Near Earth Object Observations’ program be increased from 3.7 million dollars in 2009 to 20.3 million dollars in 2011.

NASA has indicated that it intends to provide support to the Arecibo radar program if that funding remains in the budget.

Rep. Jose Serrano, D-N.Y., added 2 million dollars to NASA’s near-Earth object research program in 2010 for support of the Arecibo research work. These funds will offset reduced funding from the National Science Foundation. (ANI)

New NASA robot works tirelessly inside oceans, drawing power from water

London, April 24 (ANI): NASA has developed a new robot that can tirelessly work inside oceans, feeding on the heat of water.

The SOLO-TREC is a wax-filled buoy that draws power by the temperature differences in the water around it.

It has been tirelessly diving to depths of 500 metres off the Hawaiian coast thrice a day since last November.

The float collects data on temperature and salinity to improve studies of ocean currents.

The SOLO-TREC uses thermal energy from the ocean whenever it travels from the cold depths to the warmer surface.

A compartment comprising with two different waxes surrounds oil tubes on its shell. They flip from solid to liquid when the sea temperature rises over 10 °C, and expand by 13 per cent.

The expanding wax squeezes oil from the tubes into the float”s interior, where it is stored at high pressure.

Thereafter, the oil is released to work a generator and charge batteries.

They power the pumps that take on and drive out water so the buoy can dive and surface, as well as the float”s GPS receiver, sensors and the transmitter that beams data to satellites when at the surface.

“Each full dive generates about 200 watts for 30 seconds,” the New Scientist quoted Jack Jones, one of the project”s leaders at the Jet Propulsion Laboratory in Pasadena, California, as saying.

The buoy can recharge as it travels to the warm surface. Each dive generates about 200 watts for 30 seconds

Jones and his team now hope to develop several floats to boost existing monitoring of oceanic conditions, which aid in weather and climate prediction. (ANI)

Venus still hot and active

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

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

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

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

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

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

Similar to Hawaii

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

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

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

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

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

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

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

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

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

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

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

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

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

Future mission

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

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

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

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

A decision on SAGE is expected within a year.

NASA’s Opportunity rover examines weird-looking material near Martian crater

Washington, March 25 (ANI): Reports indicate that NASA’s Opportunity rover on Mars recently examined weird coatings on rocks beside a young crater.

The rover spent six weeks investigating the crater called “Concepcion” before resuming its long journey this month.

The crater is about 10 meters (33 feet) in diameter.

Dark rays extending from it, as seen from orbit, flagged it in advance as a target of interest because the rays suggest the crater is young.

The rocks ejected outward from the impact that dug Concepcion are chunks of the same type of bedrock Opportunity has seen at hundreds of locations since landing in January 2004, namely, soft, sulfate-rich sandstone holding harder peppercorn-size dark spheres like berries in a muffin.

The little spheres, rich in iron, gained the nickname “blueberries.”

“It was clear from the images that Opportunity took on the approach to Concepcion that there was strange stuff on lots of the rocks near the crater,” said Steve Squyres of Cornell University, Ithaca, New York, principal investigator for Opportunity and its twin rover, Spirit.

“There’s dark, grayish material coating faces of the rocks and filling fractures in them. At least part of it is composed of blueberries jammed together as close as you could pack them. We’ve never seen anything like this before,” he added.

Opportunity used tools on its robotic arm to examine this unusual material on a rock called “Chocolate Hills.”

In some places, the layer of closely packed spheres lies between thinner, smoother layers.

“It looks like a blueberry sandwich,” said Matt Golombek, a rover science-team member at NASA’s Jet Propulsion Laboratory, Pasadena, California.

“Initial analysis of the coating’s composition does not show any obvious component from whatever space rock hit Mars to dig the crater, but that is not a surprise,” he said.

“The impact is so fast, most of the impactor vaporizes. Thin films of melt get thrown out, but typically the composition of the melt is the stuff that the impactor hit, rather than the impactor material,” he added.

The composition Opportunity found for the dark coating material fits at least two hypotheses being evaluated, and possibly others.

One is that the material resulted from partial melting of blueberry-containing sandstone from the energy of the impact.

Another is that it formed from filling of fractures in this type of rock before the impact occurred.

“It’s possible that when you melt this rock, the sandstone melts before the blueberries do, leaving intact blueberries as part of a melt layer,” Squyres said. (ANI)

NASA”s Mars rover gets smarter with age

Washington, March 24 (ANI): Reports indicate that NASA”s Mars Exploration Rover Opportunity is becoming smarter as it gets older, as it now has a new capability to make its own choices about whether to make additional observations of rocks that it spots on arrival at a new location.

Now, Opportunity”s computer can examine images that the rover takes with its wide-angle navigation camera after a drive, and recognize rocks that meet specified criteria, such as rounded shape or light color.

It can then center its narrower-angle panoramic camera on the chosen target and take multiple images through color filters.

The new system is called Autonomous Exploration for Gathering Increased Science, or AEGIS.

Without it, follow-up observations depend on first transmitting the post-drive navigation camera images to Earth for ground operators to check for targets of interest to examine on a later day.

Because of time and data-volume constraints, the rover team may opt to drive the rover again before potential targets are identified or before examining targets that aren”t highest priority.

The first images taken by a Mars rover choosing its own target show a rock about the size of a football, tan in color and layered in texture.

It appears to be one of the rocks tossed outward onto the surface when an impact dug a nearby crater.

Opportunity pointed its panoramic camera at this unnamed rock after analyzing a wider-angle photo taken by the rover”s navigation camera at the end of a drive on March 4.

Opportunity decided that this particular rock, out of more than 50 in the navigation camera photo, best met the criteria that researchers had set for a target of interest: large and dark.

“It found exactly the target we would want it to find,” said Tara Estlin of NASA”s Jet Propulsion Laboratory, Pasadena, California.

“This checkout went just as we had planned, thanks to many people”s work, but it”s still amazing to see Opportunity performing a new autonomous activity after more than six years on Mars,” she added.

Opportunity can use the new software at stopping points along a single day”s drive or at the end of the day”s drive.

This enables it to identify and examine targets of interest that might otherwise be missed.

The developers anticipate that the software will be useful for narrower field-of-view instruments on future rovers.

Other upgrades to software on Opportunity and its twin, Spirit, since the rovers” first year on Mars have improved other capabilities.

These include choosing a route around obstacles and calculating how far to reach out a rover”s arm to touch a rock. (ANI)

20-yr-old study reveals precise estimates of Earth’s tectonic plate movements

Washington, March 23 (ANI): A 20 year-long study by scientists has yielded precise estimates of the interlocking tectonic plates that account for about 97 percent of Earth’s surface.

The study was carried out by Rice University geoscientist Richard Gordon and collaborators Chuck DeMets of the University of Wisconsin-Madison and Donald Argus of NASA’s Jet Propulsion Laboratory in Pasadena, California.

The 25 tectonic plates that form Earth’s surface are rigid, but they are in constant motion because they float atop the planet’s interior.

The plates constantly grind together and slide past one another.

When two plates crash into each other, they form mountain ranges like the Himalayas. When they slide past one another, they cause earthquakes like the one that struck Haiti this year.

“We live on a dynamic planet, and it’s important to understand how the surface of the planet changes,” said Gordon.

“The frequency and magnitude of earthquakes depend upon how the tectonic plates move. Understanding how plates move can help researchers understand surface processes like mountain-building and subsurface processes like mantle convection,” he added.

The new model of Earth, dubbed “MORVEL” for “mid-ocean ridge velocities,” was developed by Gordon and longtime collaborators DeMets and Argus.

“This model can be used to predict the movement of one plate relative to any other plate on the Earth’s surface,” said DeMets, the lead author of the MORVEL paper.

“Plate tectonics describes almost everything about how the Earth’s surface moves and deforms, but it’s remarkably simple in a mathematical way,” he added.

About three-quarters of the MORVEL data come from Earth’s mid-ocean ridges, undersea boundaries between tectonic plates.

At these ridges, new crust forms constantly as magma wells up from beneath the planet”s surface while the plates spread apart.

To judge how fast the plates are spreading, the team uses data from scanners that look at the magnetic profile of the crust that”s formed at mid-ocean ridges.

When Earth’s magnetic field changes polarity, it leaves a magnetic mark in the crust that”s akin to a tree ring.

These polarity changes occur at irregular intervals – the last being about 780,000 years ago.

By matching up the marks from the polarity shifts at different points along mid-ocean ridges worldwide, the team can judge how quickly new crust is being formed. (ANI)

Hurtling star could fire comets at Earth!

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

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

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

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

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

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

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

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

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

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

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

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

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)

Global warming may cause Earth’s axis to tilt in coming century

London, August 21 (ANI): A new study has suggested that gloabal warming may heat up oceans to the extent that it could cause Earth’s axis to tilt in the coming century.

According to a report in New Scientist, the warming effect was previously thought to be negligible, but researchers now say the shift will be large enough that it should be taken into account when interpreting how the Earth wobbles.

The Earth spins on an axis that is tilted some 23.5 degrees from the vertical. But this position is far from constant – the planet’s axis is constantly shifting in response to changes in the distribution of mass around the Earth.

“The Earth is like a spinning top, and if you put more mass on one side or other, the axis of rotation is going to shift slightly,” said Felix Landerer of NASA’s Jet Propulsion Laboratory in Pasadena, California.

The changing climate has long been known to move Earth’s axis. The influx of fresh water from shrinking ice sheets also causes the planet to pitch over.

Landerer and colleagues estimate that the melting of Greenland’s ice is already causing Earth’s axis to tilt at an annual rate of about 2.6 centimetres – and that rate may increase significantly in the coming years.

Now, they calculate that oceans warmed by the rise in greenhouse gases can also cause the Earth to tilt – a conclusion that runs counter to older models, which suggested that ocean expansion would not create a large shift in the distribution of the Earth’s mass.

The researchers modelled the changes that would occur if moderate projections made by the Intergovernmental Panel on Climate Change – a doubling of carbon dioxide levels between 2000 and 2100 – were to become reality.

The team found that as the oceans warm and expand, more water will be pushed up and onto the Earth’s shallower ocean shelves.

Over the next century, the subtle effect is expected to cause the northern pole of Earth’s spin axis to shift by roughly 1.5 centimetres per year in the direction of Alaska and Hawaii.

The motion is strong enough that it needs to be taken into account when interpreting shifts in Earth’s axis.

Tracking the motion of the poles could help place limits on the total amount of sea level rise over decades.

“The oceans take up at least 80 per cent of the heat that is added from greenhouse gases,” Landerer told New Scientist. “They have a huge heat capacity, so this effect is going to be there for quite a bit,” he said. (ANI)

‘Spiderbots’ inside Mount St Helens may detect impending volcanic eruption

Washington, August 15 (ANI): NASA scientists have placed about a dozen monitoring ‘spiderbots’ inside the volcanic crater in Mount St Helens in the US, which are high-tech devices that can detect an impending eruption.

Mount St. Helens is one of the most active volcanoes in the US. Its most devastating eruption in 1980, and the most recent seen here in 2004.

According to a report in National Geographic News, about a dozen so-called Spiders were placed on Mount St. Helens in July.

The pods, designed to go where no human can, were lowered by helicopter inside and around the volcano center.

“We can detect the differences between snow falling off of a branch, an animal running by, wind, a thunderstorm and the very subtle signatures of magma moving at depth, perhaps even kilometers beneath the surface of the earth,” said Steve Chien, Principal Scientist, Autonomous Systems, NASA Jet Propulsion Laboratory .

The pods form a virtual wireless network and communicate with each other and a NASA satellite called Earth Observing-1, or EO-1.

Each pod contains a seismometer, a GPS receiver, an infrared sounder to sense explosions, and a lightning detector.

According to Chien, “They have the ability to recognize different kinds of events such as seismic events, earthquakes, that are basically indications that something is happening at the volcano.”

“In the context of volcano monitoring, we want to have the best educated guess to make decisions that will save life and properties,” said Sharon Kedar, Geophysicist, NASA /Jet Propulsion Laboratoy.

NASA would like to someday use this same technology on the surface of Mars to study atmospheric events like dust storms, which are mini-tornadoes, as well as seismic activity. (ANI)

Mars had a wetter and warmer climate in the recent past

Washington, July 3 (ANI): Findings by NASA’s Phoenix Mars mission indicates that the Red Planet had a wetter and warmer climate in the recent past, and could again in the future.

Phoenix ended communications in November 2008 as the approach of Martian winter depleted energy from the lander’s solar panels.

“Not only did we find water ice, as expected, but the soil chemistry and minerals we observed lead us to believe this site had a wetter and warmer climate in the recent past – the last few million years – and could again in the future,” said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson.

A paper about Phoenix water studies, for which Smith is the lead author with 36 coauthors from six nations, cites clues supporting an interpretation that the soil has had films of liquid water in the recent past.

The evidence for water and potential nutrients “implies that this region could have previously met the criteria for habitability” during portions of continuing climate cycles, according to the researchers.

The mission’s biggest surprise was finding a multi-talented chemical named perchlorate in the Martian soil.

“This Phoenix finding caps a growing emphasis on the planet’s chemistry,” said Michael Hecht of NASA’s Jet Propulsion Laboratory, Pasadena, California, who has 10 coauthors on a paper about Phoenix’s soluble-chemistry findings.

“The study of Mars is in transition from a follow-the-water stage to a follow-the-chemistry stage,” Hecht said. “With perchlorate, for example, we see links to atmospheric humidity, soil moisture, a possible energy source for microbes, even a possible resource for humans,” he added. (ANI)

Most successful space mission finally ends

Paris, July 1 (ANI): Ulysses, the joint ESA/NASA solar orbiter mission, one of the longest and most successful space missions ever conducted, has finally ended, with ground controllers sending commands to shut down the satellite’s communications on June 30.

The mission had been predicted to end in July 2008, when the satellite’s weakened power supply was expected to fall below the minimum required to keep fuel lines from freezing, without which Ulysses would be uncontrollable.

At that time, the ESA/NASA operations team planned to continue operating the spacecraft in a reduced capacity for a few more weeks.

However, through smart engineering and real time innovation, controllers determined they could keep the lines from freezing by briefly firing the thrusters every few hours.

In fact, Ulysses has continued gathering valuable scientific data throughout most of the past year – until June 30, after a decision was taken to end the mission due to continuing weak power and the unavailability of ground station time.

The joint ESA/NASA mission operations team under Nigel Angold, ESA Mission Operations Manager, monitored the final activity from the Ulysses Mission Support Area (MSA) at NASA’s Jet Propulsion Laboratory (JPL), California, USA.

Launched by Space Shuttle Discovery on 6 October 1990, the 18-year, 8-month mission has returned a wealth of scientific data on the space environment above and below the poles of the Sun.

At the time of sending the last commands, Ulysses was located approximately 1.5 astronomical units from Earth and the one-way radio signal time was approximately 45 minutes.

“This has been an amazing adventure. Although we have said a sad farewell, Ulysses will remain a unique landmark in the exploration of space, something we can all be incredibly proud of,” said Richard Marsden, ESA’s Ulysses Project Scientist and Mission Manager.

During its life, Ulysses made nearly three complete orbits of the Sun.

The probe revealed for the first time the three-dimensional character of galactic cosmic radiation, energetic particles produced in solar storms and the solar wind.

Not only has Ulysses allowed scientists to map constituents of the heliosphere in space, its longevity enabled the Sun to be observed over a longer period of time than ever before. (ANI)

NASA releases new extensive digital topographic map of Earth

Washington, June 30 (ANI): NASA, along with Japan’s Ministry of Economy, Trade and Industry, known as METI, have released a new digital topographic map of Earth that covers more of our planet than ever before.

The map was produced with detailed measurements from NASA’s Terra spacecraft.

The new global digital elevation model of Earth was created from nearly 1.3 million individual stereo-pair images collected by the Japanese Advanced Spaceborne Thermal Emission and Reflection Radiometer, or ASTER, instrument aboard Terra.

NASA and Japan’s METI developed the data set. It is available online to users everywhere at no cost.

“This is the most complete, consistent global digital elevation data yet made available to the world,” said Woody Turner, ASTER program scientist at NASA Headquarters in Washington.

“This unique global set of data will serve users and researchers from a wide array of disciplines that need elevation and terrain information,” he added.

According to Mike Abrams, ASTER science team leader at NASA’s Jet Propulsion Laboratory in Pasadena, California, the new topographic information will be of value throughout the Earth sciences and has many practical applications.

“ASTER’s accurate topographic data will be used for engineering, energy exploration, conserving natural resources, environmental management, public works design, firefighting, recreation, geology and city planning, to name just a few areas,” Abrams said.

Previously, the most complete topographic set of data publicly available was from NASA’s Shuttle Radar Topography Mission.

That mission mapped 80 percent of Earth’s landmass, between 60 degrees north latitude and 57 degrees south.

The new ASTER data expands coverage to 99 percent, from 83 degrees north latitude and 83 degrees south. Each elevation measurement point in the new data is 98 feet apart.

“The ASTER data fill in many of the voids in the shuttle mission’s data, such as in very steep terrains and in some deserts,” said Michael Kobrick, Shuttle Radar Topography Mission project scientist at the Jet Propulsion Laboratory.

“NASA is working to combine the ASTER data with that of the Shuttle Radar Topography Mission and other sources to produce an even better global topographic map,” he added. (ANI)

‘Stuck’ Martian rover uses opportunity to learn about Red Planet’s ecological history

Washington, June 26 (ANI): NASA’s Mars rover Spirit, lodged in Martian soil that is causing traction trouble, is taking advantage of the situation by learning more about the Red Planet’s environmental history.

In April, Spirit entered an area composed of three or more layers of soil with differing pastel hues hiding beneath a darker sand blanket.

Scientists dubbed the site “Troy.”

Spirit’s rotating wheels dug themselves more than hub deep at the site.

The rover team has spent weeks studying Spirit’s situation and preparing a simulation of this Martian driving dilemma to test escape maneuvers using an engineering test rover at NASA’s Jet Propulsion Laboratory in Pasadena, California.

A rock seen beneath Spirit in images from the camera on the end of the rover’s arm may be touching Spirit’s belly.

Scientists believe it appears to be a loose rock not bearing the rover’s weight.

While Spirit awaits extraction instructions, the rover is keeping busy examining Troy, which is next to a low plateau called Home Plate, approximately 3.2 kilometers (2 miles) southeast of where Spirit landed in January 2004.

“By serendipity, Troy is one of the most interesting places Spirit has been,” said Ray Arvidson of Washington University in St. Louis.

“We are able here to study each layer, each different color of the interesting soils exposed by the wheels,” he added.

Spirit has been using tools on its robotic arm to examine tan, yellow, white and dark-red sandy soil at Troy. Stretched-color images from the panoramic camera show the tints best.

“The layers have basaltic sand, sulfate-rich sand and areas with the addition of silica-rich materials, possibly sorted by wind and cemented by the action of thin films of water. We’re still at a stage of multiple working hypotheses,” said Arvidson.

“This may be evidence of much more recent processes than the formation of Home Plate, or isome Plate being slowly stripped back by wind, and we happened to stir up a deposit from billions of years ago before the wind got to it?” he added.

Team members from NASA’s Johnson Space Center in Houston feel initial readings suggest that iron is mostly present in an oxidized form as ferric sulfate and that some of the differences in tints at Troy observed by the panoramic camera may come from differences in the hydration states of iron sulfates.

While extraction plans for the rover are developed and tested during the coming weeks, the team plans to have Spirit further analyze the soil from different depths. (ANI)

NASA’s lunar map sheds new light on Moon’s darkest craters

Washington, June 19 (ANI): NASA scientists have created a new lunar topography map with the highest resolution of the Moon’s rugged south polar region, which provides new information on some of out natural satellite’s darkest craters.

The map was created by scientists at NASA’s Jet Propulsion Laboratory, Pasadena, California, who collected the data using the Deep Space Network’s Goldstone Solar System Radar located in California’s Mojave Desert.

The map will help Lunar Crater Observation and Sensing Satellite (LCROSS) mission planners as they target for an encounter with a permanently dark crater near the lunar South Pole.

“Since the beginning of time, these lunar craters have been invisible to humanity,” said Barbara Wilson, a scientist at NASA’s Jet Propulsion Laboratory, and manager of the study.

“Now we can see detailed topography inside these craters down to 40 meters (132 feet) per pixel, with height accuracy of better than 5 meters (16 feet),” she added.

Scientists targeted the Moon’s south polar region using Goldstone’s 70-meter (230-foot) radar dish.

The antenna, three-quarters the size of a football field, sent a 500-kilowatt-strong, 90-minute-long radar stream 373,046 kilometers (231,800 miles) to the Moon.

Signals were reflected back from the rough-hewn lunar terrain and detected by two of Goldstone’s 34-meter (112-foot) antennas on Earth.

The roundtrip time, from the antenna to the Moon and back, was about two-and-a-half seconds.

The scientists compared their data with laser altimeter data recently released by the Japanese Aerospace Exploration Agency’s Kaguya mission to position and orient the radar images and maps.

The new map provides contiguous topographic detail over a region approximately 500 kilometers (311 miles) by 400 kilometers (249 miles). (ANI)

Astronomers discover Jupiter-like planet orbiting one of the smallest stars known

Washington, May 29 (ANI): A long-proposed tool for hunting planets has finally discovered a Jupiter-like planet orbiting one of the smallest stars known.

The technique, called astrometry, was first attempted 50 years ago to search for planets outside our solar system, called exoplanets.

It involves measuring the precise motions of a star on the sky as an unseen planet tugs the star back and forth.

But, the method requires very precise measurements over long periods of time, and until now, has failed to turn up any exoplanets.

A team of two astronomers from NASA’s Jet Propulsion Laboratory, Pasadena, California, has, for the past 12 years, been mounting an astrometry instrument to a telescope at the Palomar Observatory near San Diego.

After careful, intermittent observations of 30 stars, the team has identified a new exoplanet around one of them – the first ever to be discovered around a star using astrometry.

“This method is optimal for finding solar-system configurations like ours that might harbor other Earths,” said astronomer Steven Pravdo of JPL.

“We found a Jupiter-like planet at around the same relative place as our Jupiter, only around a much smaller star. It’s possible this star also has inner rocky planets,” he added. Since more than seven out of 10 stars are small like this one, this could mean planets are more common than we thought,” he further added.

The finding confirms that astrometry could be a powerful planet-hunting technique for both ground- and space-based telescopes.

The newfound exoplanet, called VB 10b, is about 20 light-years away in the constellation Aquila. It is a gas giant, with a mass six times that of Jupiter’s, and an orbit far enough away from its star to be labeled a “cold Jupiter” similar to our own.

In reality, the planet’s own internal heat would give it an Earth-like temperature.

The planet’s star, called VB 10, is tiny. It is what’s known as an M-dwarf and is only one-twelfth the mass of our Sun, just barely big enough to fuse atoms at its core and shine with starlight.

For years, VB 10 was the smallest star known. Now, it has a new title: the smallest star known to host a planet.

In fact, though the star is more massive than the newfound planet, the two bodies would have a similar girth.

Because the star is so small, its planetary system would be a miniature, scaled-down version of our own. (ANI)

6th grader names NASA’s Mars rover ‘Curiosity’

Washington, May 28 (ANI): NASA has selected ‘Curiosity’, the name given by a sixth-grade student from Kansas, US, for its Mars Science Laboratory rover, scheduled for launch in 2011.

Twelve-year-old Clara Ma from the Sunflower Elementary school in Lenexa submitted the winning entry, “Curiosity.”

As her prize, Ma wins a trip to NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California, where she will be invited to sign her name directly onto the rover as it is being assembled.

A NASA panel selected the name following a nationwide student contest that attracted more than 9,000 proposals via the Internet and mail.

The panel primarily took into account the quality of submitted essays.

Name suggestions from the Mars Science Laboratory project leaders and a non-binding public poll also were considered.

The activity invited ideas from students 5 – 18 years old enrolled in a US school. The contest started in November 2008. Entries were accepted until midnight January 25.

Ma decided to enter the rover-naming contest after she heard about it at her school.

“I was really interested in space, but I thought space was something I could only read about in books and look at during the night from so far away,” Ma said.

“I thought that I would never be able to get close to it, so for me, naming the Mars rover would at least be one step closer,” she added.

“Curiosity is an everlasting flame that burns in everyone’s mind. It makes me get out of bed in the morning and wonder what surprises life will throw at me that day,” Ma wrote in her winning essay.

“Curiosity is such a powerful force. Without it, we wouldn’t be who we are today. Curiosity is the passion that drives us through our everyday lives. We have become explorers and scientists with our need to ask questions and to wonder,” she wrote.

“Students from every state suggested names for this rover. That’s testimony to the excitement Mars missions spark in our next generation of explorers,” said Mark Dahl, the mission’s program executive at NASA Headquarters in Washington.

Curiosity will be larger and more capable than any craft previously sent to land on the Red Planet. It will check to see whether the environment in a selected landing region ever has been favorable for supporting microbial life and preserving evidence of life.

The rover also will search for minerals that formed in the presence of water and look for several chemical building blocks of life. (ANI)

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Herschel and Planck on their way to unlock secrets of the Universe

Washington, May 15 (ANI): The Herschel and Planck spacecraft have successfully blasted into space on May 14 from the Guiana Space Centre in French Guiana, in a mission to unlock the secrets of the Universe.

The European Space Agency (ESA) missions, with significant participation from NASA, hitched a ride together on an Ariane 5 rocket, but now have different journeys before them.

Herschel will explore, with unprecedented clarity, the earliest stages of star and galaxy birth in the universe; it will help answer the question of how our Sun and Milky Way galaxy came to be.

Planck will look back to almost the beginning of time itself, gathering new details to help explain how our universe came to be.

“These two missions have spent a lot of time together,” said Ulf Israelsson, NASA project manager for both Herschel and Planck at NASA’s Jet Propulsion Laboratory, Pasadena, California.

“But now they are going their separate ways, each ready to do what it does best,” he added.

The spacecraft are traveling on separate trajectories to a point in the Earth-Sun system called the second Lagrangian point, four times farther away than the moon’s orbit, or an average distance of 1.5 million kilometers from Earth.

They will spend the rest of their missions independently orbiting this point – located on the other side of Earth from the Sun – as they make their way around the Sun every year.

Herschel will start preparing for science operations while en route toward its operational orbit, which will be reached in about two months.

Four months later, the science mission will begin and is expected to last more than three-and-a-half years.

Planck will reach a similar orbit in roughly two months, with science observations beginning one month later.

The mission’s science operations are scheduled to last a minimum of 15 months, with the possibility of an extension.

Herschel will make the most detailed measurements yet of the cold and dark wombs where the embryos of stars and galaxies have just begun to grow.

It will also be able to detect key elements and molecules involved in a star’s life, tracing their evolution from atoms to potentially life-forming materials.

Planck will see light that has traveled billions of years from the newborn universe to reach us.

This light, called the cosmic microwave background, contains information about the Big Bang that created space and time itself.

According to Charles Lawrence, the NASA Planck project scientist at JPL, “Our previous images of the baby universe were like fuzzy snapshots. Now, we’ll have the cleanest, deepest and sharpest images ever made of the early universe.” (ANI)