Hot Rap Tracks for the 4/10/2010 issue

Now Last Weeks Peak

1 1 15 1 Say Something – Timbaland Featuring Drake (/Interscope)

2 3 10 2 Nothin’ On You – B.o.B Featuring Bruno Mars (/Atlantic)

3 2 20 1 BedRock – Young Money Featuring Lloyd (/UMRG)

4 4 20 2 How Low – Ludacris (/IDJMG)

5 5 6 5 My Chick Bad – Ludacris Featuring Nicki Minaj (/IDJMG)

6 8 4 6 Over – Drake (/Universal Motown)

7 6 22 6 Steady Mobbin’ – Young Money Featuring Gucci Mane (/UMRG)

8 9 10 8 Lemonade – Gucci Mane (/Warner Bros.)

9 10 17 7 O Let’s Do It – Waka Flocka Flame (/Warner Bros.)

10 7 13 5 On To The Next One – Jay-Z + Swizz Beatz ()

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Cracks on Mars a result of evaporating lakes in ancient times

Washington, September 16 (ANI): Networks of giant polygonal troughs etched across crater basins on Mars have been identified as desiccation cracks caused by evaporating lakes, providing further evidence of a warmer, wetter Martian past.

The findings were presented at the European Planetary Science Congress by PhD student M. Ramy El Maarry of the Max Planck Institute for Solar System Research.

The polygons are formed when long cracks in the surface of the Martian soil intersect.

El Maarry investigated networks of cracks inside 266 impact basins across the surface of Mars and observed polygons reaching up to 250 meters in diameter.

Polygonal troughs have been imaged by several recent missions but, until now, they have been attributed to thermal contractions in the Martian permafrost.

El Maarry created an analytical model to determine the depth and spacing of cracks caused by stresses building up through cooling in the Martian soil.

He found that polygons caused by thermal contraction could have a maximum diameter of only about 65 meters, much smaller than the troughs he was seeing in the craters.

“I got excited when I saw that the crater floor polygons seemed to be too large to be caused by thermal processes. I also saw that they resembled the desiccation cracks that we see on Earth in dried up lakes,” said El Maarry.

“The stresses that build up when liquids evaporate can cause deep cracks and polygons on the scale I was seeing in the craters,” he added.

El Maarry identified the crater floor polygons using images taken by the MOC camera on Mars Global Surveyor and the HiRISE and Context cameras on Mars Reconnaissance Orbiter.

The polygons in El Maarry’s survey had an average diameter of between 70 and 140 kilometers, with the width of the actual cracks ranging between 1 and 10 meters.

Evidence suggests that between 4.6 and 3.8 billion years ago, Mars was covered in significant amounts of water.

Rain and river water would have collected inside impact crater basins, creating lakes that may have existed for several thousand years before drying out.

However, according to El Maarry, in the northern hemisphere, some of the crater floor polygons could have been formed much more recently.

“When a meteorite impacts with the Martian surface, the heat can melt ice trapped beneath the Martian crust and create what we call a hydrothermal system. Liquid water can fill the crater to form a lake, covered in a thick layer of ice. Even under current climatic conditions, this may take many thousands of years to disappear, finally resulting in the desiccation patterns,” said El Maarry. (ANI)

NASA all set to launch infrared eye to hunt for dark asteroids

Sydney, September 3 (ANI): NASA is preparing to launch an infrared telescope that will hunt down dark asteroids that have slipped beneath our radar.

According to a report by ABC Science, the Wide-field Infrared Survey Explorer (WISE) spacecraft recently arrived at Vandenberg Air Force Base in California ahead of its launch later this year.

With a quartet of infrared sensors and a wide view, WISE is designed to survey the whole sky in infrared light.

It’s not the first telescope to do so, but scientists expect WISE’s observations will be 500 times sharper than a survey conducted in 1980s by IRAS, the Infrared Astronomical Satellite, according to astronomer Martin Cohen of the University of California at Berkeley.

The data will be complied into an all-sky infrared atlas, a tome that is expected to include about 300 million objects, including around 100,000 asteroids.

Many of the asteroids seen by WISE will be known objects.

Scientists hope to use the new observations to nail down details, such as an asteroid’s diameter and surface reflectivity.

“With ground-based scopes, it’s just a point source. You can’t tell size directly,” said University of Texas astronomer Dr Robert McMillan who leads Spacewatch, an asteroid-survey project.

“A big object that is dark and a small object that is bright are going to look like they have the same brightness,” he added.

The solar system contains several million asteroids, most of which reside in the main asteroid belt between Mars and Jupiter.

About 7000 asteroids have been identified that cross or come close to Earth’s orbit.

WISE will be able to spot asteroids emitting heat due to direct exposure from the Sun, as opposed to visible-light searches that find asteroids that are reflecting sunlight.

“Those are two different physical effects,” said McMillan. “An asteroid that has very dark colour in invisible light is going to get heated up more, just like a black car in a parking lot is going to get heated up more than a white car,” he added.

Scientists hope to get enough positioning information to follow up targets with ground-based observations.

McMillan expects that WISE will discover a few hundred new asteroids.

The information will be folded into ongoing surveys to map asteroids that could impact Earth and cause widespread damage.

Other WISE targets include brown dwarfs, which are Jupiter-sized stars that never got their nuclear fusion engines running, and ultra-luminous galaxies, which pump out the equivalent of about 1000 Sun-sized stars every year. (ANI)

ISRO to launch Mars mission by 2013

New Delhi, Aug 31 (ANI):Indian Space research Organisation (ISRO) chairman G. Madavan Nair said on Monday that India would launch a mission to Mars by 2013.

The ISRO has begun the preparations for sending a spacecraft to Mars.

Earlier on Aug 13 the Union Government sanctioned seed money of Rs 10 crore for Mars project, to carry out various studies on experiments to be conducted, route of the mission and other related details necessary to scale the new frontier.

On Sunday ISRO called off the maiden Lunar mission after Indian Deep Space Network at Byalalu near Bangalore lost control over the Chndrayaan -I spacecraft.

Though Chandrayaan- I was slated to be a two-year mission, Nair claimed that ISRO scientists have achieved nearly 95% of Chandrayaan’s scientific goals in less than a year. (ANI)

ISRO formally calls off India’s first moon mission

Panaji. Aug 31 (ANI): Indian Space Research Organisation (ISRO) has formally called off Chandrayaan-1, India’s first moon mission, after it lost contact with the craft. ink with the Chandrayaan-1 craft broke down early on Saturday.

Talking to reporters here on Sunday, ISRO Chairman G Madhavan Nair said, “The net result is that the lunar has lost radio contact with the craft and we are not receiving any signal. So we had to terminate the mission with this sequence…we made all attempts but our attempts were not succeed.”

Nair claimed that though the moon mission terminated much before its two-year lifetime it was a great success.

“About 95 percent of the objectives of the scientific experiments have been completed and we have more than 70,000 images of the moon, especially the most critical regions are in our custody,” he added.

The 79-million dollar mission was launched amid national euphoria last October, putting India in the Asian space race alongside China.

A probe vehicle landed on the moon a month later and sent back images of the lunar surface.

But a critical sensor in the main craft, orbiting the moon, malfunctioned in July, raising fears that the two-year mission might have to be curtailed.

One of the mission’s main aims was to look for Helium 3, an isotope which is very rare on earth but could be an energy source in the future in nuclear fusion.

ISRO has plans to send a manned mission to space in four years’ time and eventually on to Mars. (ANI)

“Mars spectacular” event on August 27 a hoax, say astronomers

Washington, August 27 (ANI): Astronomers have confirmed that an email promising a “Mars spectacular” event on August 27, when the Red Planet will look as large as the full moon, is nothing but a hoax.

According to a report in National Geographic News, the anonymous message from an unknown part of the globe says that the red planet “will look as large as the full moon” in the night sky, and that “no one alive today will ever see this again.”

The claim has been bombarding people’s inboxes worldwide every summer for five years.

Today, the Mars hoax has grown into a kind of cyber legend-one that astronomers are still struggling to debunk.

“The possibility of seeing Mars as large as the moon strikes the imagination,” said Marc Jobin, staff astronomer at the Montreal Planetarium in Quebec.

“The sad reality is that a lot of people have little comprehension of astronomy and are unable to call the hoax,” he added.

But, there is a thread of truth that inspired the prank several years ago.

Planets are not on perfectly circular orbits, and during their elliptical paths around the sun, planets can vary in their exact distances to each other over time.

On August 27, 2003, Mars made a historically tight approach to Earth, coming about 56 million kilometers away.

Such a near pass hadn’t happened in nearly 60,000 years, and it won’t happen again until August 28, 2287.

In 2003, planetariums had sent out notices alerting stargazers of the real astronomical event.

“At the time, through the telescope, Mars looked as large as the full moon would with the naked eye,” explained Geza Gyuk, astronomer at the Adler Planetarium in Chicago, Illinois.

Through a backyard telescope with a high-power eyepiece, viewers could even make out many surface features on Mars’s disk.

With the naked eye, Mars still appeared as nothing more than a brilliant orange-colored star in the sky.

Still, an email hoax was born.

If the red planet actually did appear as huge as purported in the Mars hoax email, the planet would be just 750,000 kilometers from Earth, or about twice as far away as the moon.

According to Jobin, at that distance, life on Earth would likely be doomed.

Given the interplay of gravity between the planets and the sun, a much closer Mars “would have extreme consequences on the shape of the Earth’s orbit, with our planet swinging much closer and much farther away from the sun,” he said. (ANI)

NASA successfully tests eco-friendly rocket propellant

Washington, August 22 (ANI): NASA and the Air Force Office of Scientific Research, or AFOSR, have successfully launched a small rocket using an environmentally-friendly, safe propellant comprised of aluminum powder and water ice, called ALICE.

“This collaboration has been an opportunity for graduate students to work on an environmentally-friendly propellant that can be used for flight on Earth and used in long distance space missions,” said NASA Chief Engineer Mike Ryschkewitsch at NASA Headquarters in Washington.

“These sorts of university-led experimental projects encourage a new generation of aerospace engineers to think outside of the box and look at new ways for NASA to meet our exploration goals,” he added.

Using ALICE as fuel, a nine-foot rocket soared to a height of 1,300 feet over Purdue University’s Scholer farms in Indiana earlier this month.

ALICE is generating excitement among researchers because this energetic propellant has the potential to replace some liquid or solid propellants.

When it is optimized, it could have a higher performance than conventional propellants.

“By funding this collaborative research with NASA, Purdue University and the Pennsylvania State University, AFOSR continues to promote basic research breakthroughs for the future of the Air Force,” said Dr. Brendan Godfrey, director of AFOSR.

ALICE has the consistency of toothpaste when made. It can be fit into molds and then cooled to -30 degree Celsius 24 hours before flight.

The propellant has a high burn rate and achieved a maximum thrust of 650 pounds during this test.

“A sustained collaborative research effort on the fundamentals of the combustion of nanoscale aluminum and water over the last few years led to the success of this flight,” said Dr. Steven F. Son, a research team member from Purdue.

“ALICE can be improved with the addition of oxidizers and become a potential solid rocket propellant on Earth. Theoretically, ALICE can be manufactured in distant places like the moon or Mars, instead of being transported to distant locations at high cost,” he added. (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)

Scientists identify lake shorelines on Mars

Washington, August 9(ANI): A team of scientists, using images from the High Resolution Imaging Science Experiment (HiRISE) camera on board NASA’s Mars Reconnaissance Orbiter, have reported direct evidence of lake shorelines in the Shalbatana Vallis in Mars.

Scientists generally believe that warm, wet conditions existed on Mars until only about 3.7 billion years ago.

In recent years, however, remote sensing studies have hinted at the existence of Martian lakes during the Hesperian epoch (about 3.5 billion to 1.8 billion years ago).

Now, sub-meter-scale images from NASA’s Mars Reconnaissance Orbiter show clear, unambiguous evidence of shorelines of a lake more than 450 meters (1,476 feet) deep that formed about 3.4 billion years ago.

The study indicates that conditions favorable for flowing water and lake formation may have existed for thousands of years on Mars during the Hesperian epoch, which has been thought to be a period during which surface conditions did not allow significant hydrological activity.

According to the researchers, the sedimentary deposits associated with the lake in Shalbatana Vallis should be considered a priority for further study by future landed Mars missions. (ANI)

Giant Martian egg cups could be used to trace the Red Planet’s climate

London, July 14 (ANI): A new study has suggested that craters embedded on pedestals that tower above the Martian landscape like giant egg cups could be used to trace the planet’s climate.

‘Pedestal’ craters were gouged out by impacts, like other craters, but stand out because they sit atop plateaus that loom an average of 50 metres above the Martian surface.

It’s not clear exactly how the pedestals formed.

According to a report in New Scientist, a comprehensive catalogue of the objects is lending weight to the idea that the pedestals may conceal ice-rich soil from previous eras, when the planet’s spin axis tilted at a different angle than it does today.

Seth Kadish of Brown University in Providence, Rhode Island, and colleagues identified 2696 pedestal craters in the planet’s mid- and low-latitudes from images taken primarily by the thermal imager aboard NASA’s Mars Odyssey spacecraft.

The craters seem to be concentrated at the mid-latitudes, with very few found at the planet’s equator.

About 3 per cent of them have depressions around their bases that resemble areas in Antarctica where permafrost ice vaporizes, creating pits in the soil left behind.

The team said that strengthens the hypothesis that the pedestals were created from soil that was enriched in ice during a period when the Martian poles pointed more towards the sun and its mid-latitudes were colder.

Because Mars does not have a massive satellite that stabilises it, like Earth’s moon, the tilt of its axis is thought to change regularly on scales of tens of thousands of years.

When the planet is tilted most drastically on its side, the planet’s poles receive a lot of sunshine. Any water locked in ice there is thought to vaporize and move towards the equator, where it falls as snow.

Tens of metres of snow are thought to be deposited on the planet’s mid-latitudes during these episodes.

Pedestal craters may preserve regions with this ancient snow.

The researchers suspect the impact of the meteorite that created each pedestal crater could somehow ‘armour’ the ground in the area, producing a top layer that protected ice from sublimating into gas during warmer periods.

The unprotected ice surrounding the armoured area, however, would eventually disappear when the planet’s tilt changed and the area warmed.

That would leave behind the modern-day, ice-laden pedestals that can be more than 100 metres thick.

“These pedestals represent almost like a cookie-cutter section of past icy, dust-rich layers,” Kadish said. (ANI)

Factors other than trapped ice limit dune movement on Mars

Washington, July 8 (ANI): A study has determined that snow and ice trapped inside dunes on Mars does not entirely stop their movement, a finding which indicates that other factors are limiting the dune movement.

Planetary scientists have monitored some Martian sand dunes for more than 30 years, and the dunes have not moved during that time, leading scientists to question whether snow and ice trapped inside the dunes might be preventing movement.

However, a recent study, led by Mary Bourke, a senior research scientist at the Tucson-based Planetary Science Institute, shows that snow and ice are not enough in themselves to stop dune movement.

While trapped ice and snow impedes movement of sand dunes in polar climates, compared to their counterparts in warmer areas, this does not entirely stop dune movement, the study shows.

“This indicates that other factors are limiting dune movement,” said Bourke.

Bourke also showed that two small dunes recently disappeared on Mars. The dunes, which were 20 meters wide (about 65 feet) and located in the north polar region of Mars, were completely eroded away over a period of 5.7 Earth years.

“This (dune disappearance) is fantastic new data, showing that sand is transported on Mars where and when the wind energy is available,” Bourke said. “But the bigger, larger dunes on Mars are not moving, at least in the areas we studied,” she added.

In the most recent study, Bourke and her colleagues used vertical aerial photos and LiDAR (Light Detection and Ranging) data to estimate dune migration rates in Antarctica’s Victoria Valley dune field.

The photos, taken between 1961 and 2001, came from the USGS Antarctic Resource Center.

These dunes are known to be covered by seasonal snowfalls and have snow and ice layers trapped inside.

Bourke found that the dunes migrated about 1.5 meters (5 feet) per year, which is small compared to the distance covered by dunes in warm deserts, which can be as high as 30-70 meters (about 100 to 230 feet) a year.

Factors limiting dune movement on Mars would include the planet’s thin atmosphere, which requires very high wind speeds to provide the force needed to move sand, and the water and carbon-dioxide frosts that cover dunes in Mars’ polar regions for 70 percent of the year. (ANI)

Robotic grasshopper to help explore Mars’ rocky geography

London, July 6 (ANI): Scientists have come up with the first robotic grasshopper based on the spring mechanism the insect has to propel itself, which may help explore Mars’ rocky terrain.

The Jollbot was masterminded by Rhodri Armour, who spent a year building the robot with colleagues at the University of Bath.

The robot, which can jump and roll, enjoys an edge over other machines due to its ability to launch itself over obstacles.

The remote-controlled Jollbot runs on a motor connected to a battery pack and a series of springs around the circumference, which help it leap up to half a metre.

Weighing only one kilogram, it has been made from soft plastic, and borrows dynamics from insects when it bounces on landing.

Armour said: “I was inspired by the way insects like the grasshopper jump around in extremely rough environments. Even with their comparatively long legs, an insect’s small size limits the possibility of using its muscles to directly provide the contraction needed for take-off.”

The researcher added: “That means all insects and smaller jumping animals use some sort of spring mechanism to store muscle energy and release it when required. It’s a bit like a mechanical catapult – with a lengthy energy storage phase and rapid release.”

The boffin further revealed that the project was meant to be low-cost, adding: “Jollbot was always intended to be inexpensive and as such many could be sent on exploratory missions in place of a single conventional robot. This would allow for some of them to fail.”

Dr David Williams, director general of the British National Space Centre, said that the University of Bath’s research helped boost homegrown innovation in space exploration.

He added: “We wish the project all the best.” (ANI)

Martian climate was life-friendly more recently than thought

Washington, July 1 (ANI): In a new research, scientists have found evidence that indicates the Martian climate was life-friendly more recently than thought.

Matthew Balme, a research scientist with the Tucson-based Planetary Science Institute and a research fellow at the United Kingdom’s Open University, discovered signs of melting permafrost in images from NASA’s HiRISE (High Resolution Imaging Science Experiment) camera, which is flying aboard the Mars Reconnaissance Orbiter.

The images show that landforms once thought to be shaped by volcanism were actually modified by the expansion and contraction of ice due to freeze/thaw cycles, according to Balme.

Balme studied an outflow channel that was active as recently as 2 to 8 million years ago.

The channel contains polygonal patterns, branched channels, blocky debris and mound/cone formations, all of which are similar to formations found where permafrost melts on Earth.

“These observations demonstrate that ice melted near the Martian equator within the past few million years and then refroze,” Balme said. “This probably happened over many freeze/thaw cycles,” he added.

Since liquid water is essential to life as we know it, this equatorial channel would be an ideal place to hunt for traces of past or present Martian life, Balme added. (ANI)

Mars had warmer weather in its recent past than previously thought

London, June 30 (ANI): A new research led by a UK scientist has indicated that Mars had significantly warmer weather in its recent past than previously thought.

Dr. Matthew Balme, from The Open University, made the new discovery by studying detailed images of equatorial landforms that formed by melting of ice-rich soils.
is work indicates that the Martian surface experienced “freeze thaw” cycles as recently as 2 million years ago, and that Mars has not been locked in permafrost conditions for billions of years as had been previously thought.

The high-resolution images, which show a variety of interesting landforms, were taken with NASA’s HiRISE (High Resolution Imaging science Experiment) which is onboard the Mars Reconnaissance Orbiter (MRO) mission.

According to Dr. Balme, “The features of this terrain were previously interpreted to be the result of volcanic processes. The amazingly detailed images from HiRISE show that the features are instead caused by the expansion and contraction of ice, and by thawing of ice-rich ground. This all suggests a very different climate to what we see today.”

All of the landforms observed are in an outflow channel, thought to have been active as recently as 2 million to 8 million years ago.

Since the landforms exist within, and cut across, the pre-existing features of the channel, this suggests that they too were created within this timeframe.

The pictures show polygonally patterned surfaces, branched channels, blocky debris and mound/cone structures.

All of these features are similar to landforms on Earth typical of areas where permafrost terrain is melting.

“These observations demonstrate not only that there was ice near the Martian equator in the last few million years, but also that the ice melted to form liquid water and then refroze. And this probably happened for many cycles,” Dr. Balme said.

“Given that liquid water seems to be essential for life, these kinds of environments could be a great place to look for evidence of past life on Mars,” he added.

According to Professor Keith Mason, CEO of the Science and Technology Facilities Council (STFC), “Understanding current processes on the surface of Mars and the past and present role of climate improves our knowledge of the planet’s history and thus the chances of one day detecting evidence for past or present life.” (ANI)

Native seeds may feed future human colonies in space

Sydney, June 29 (ANI): An Australian experiment with native plant seeds has raised hopes for self-sustaining human colonies in space, with the seeds, taken into space last year, showing no signs of “fatigue” or damage after surviving more than 28,000 orbits of the earth.

According to a report in The Sydney Morning Herald, the seedlings of the golden wattle, waratah, flannel flower and wollemi pine accompanied NASA astronaut Dr Gregory Chamitoff on his six-month space odyssey.

At the request of NSW’s (New South Wales’) Botanic Gardens Trust, Dr Chamitoff took the seeds on the Space Shuttle Discovery mission to the International Space Station in May 2008.

While tests are still being conducted on the seedlings, which returned to earth in November last year, conservationists are encouraged by preliminary findings.

The seeds are being germinated and “fast-track” aged at the Trust’s NSW Seedbank at Mount Annan Botanic Garden in Sydney’s southwest.

“With habitats under increasing threat, seedbanking on earth, and perhaps in space, will be part of an integrated conservation program for species threatened by extinction due to global warming or other sudden changes to their habitat,” said Trust executive director Dr Tim Entwisle.

“As a species (humans) have an impact upon the other species of the world and we have the possibility of damaging the environment where we lose the biodiversity because of our actions,” said Entwisle.

“We also are a species that understands these things and, therefore, I think we have a moral imperative to do these kinds of things and protect the environment.” he added.

For NASA, the findings also present the opportunity to plan for possible space colonies.

“As soon as we get back to the moon and even before we reach Mars, we’re going to have to figure out how to recycle as much as we can and provide as much food sources as we can in space,” Dr Chamitoff said.

“From NASA’s perspective, we are interested in seeds that might be hardy enough to survive long duration exposure to the space environment and then germinate in greenhouses in Space or on other planets,” he added.

“Ultimately, this will be essential to support self-sustaining outposts or colonies in Space with food and oxygen,” he explained.

The NSW Seedbank tests on the seedlings will monitor their growth, vigour and life span compared to control seeds. (ANI)

Traces of microbes in shallow ice layers may help find life on icy worlds

Washington, June 26 (ANI): A new research has indicated that living microorganisms and the food that sustained them can be detected in shallow ice layers, which will help find life on icy worlds.

The research is a part of the Project SLIce, which means, Signatures of Life in Ice.

Dominique Tobler and Jennifer Eigenbrode of NASA Goddard Space Science Laboratory, and Liane Benning of the University of Leeds, UK, show that not only living micro-organisms, but also traces of long-dead ones, and the food that sustained them can be detected in shallow ice layers, using methods rigorously tested in one of our own planet’s most extreme environments.

“With SLIce, we wanted to figure out the nature of the organic matter in ice and how what we find on Earth can be the basis for comparisons with organic matter on Mars,” explained Benning.

“The organic matter we find could be alive or dead, representing extant or extinct life, or even the nutrients that made life possible, and we want to identify the biological signals that point towards ice-dwelling life,” she added.

The SLIce team went to a glacial region of Svalbard to try taking ice samples in exactly the way it would be done on Mars, using a sequence of procedures and tests that they had developed as part of the AMASE project, a long-running international research program that has established Svalbard as a test bed for planetary exploration.

“We’re using sample devices, primarily to be operated from a rover, but we’re also testing how we go about taking and testing samples and keeping them separate,” said Benning.

“For SLIce, we applied the protocol we had developed to take ice cores, process them and analyze them in the field just as would happen on a rover on Mars, and then of course we took them back to the lab and did a much wider range of tests, so we really knew what we had found,” she said.

“There could be microbes living in the ice, but there could also be the dead bodies of microbes that used to live there, and there could be biological molecules that blew in from dust and micrometeorites. We need to identify what we’ve got, so that we know what it’s telling us,” she added. (ANI)

Snoop Dogg, Buzz Aldrin team up for rap single Rocket Experience

London, June 25 (ANI): Snoop Dogg has teamed up with Apollo astronaut Buzz Aldrin to record a rap single Rocket Experience.

Aldrin, the second man to set foot on the moon, said he had reached his second mission of becoming a rap star, thanks to the collaboration with the hip hop artist.

Aldrin has continued his attempts to revive interest in space exploration and the track video, he revealed, was one such step.

“Young people have lost any interest in space that isn’t in a video game or a movie house. Many don’t really know that Man has stood on the Moon,” Times Online quoted him as saying.

“But these incredible rappers speak to the new generations and know how to reach them. The Americans who will take Man to Mars are already born and they don’t even know that space is Man’s fate,” he added. (ANI)

New instrument may detect groundwater deep inside Mars

Washington, June 25 (ANI): A team of Boulder (US) scientists and engineers has tested a new instrument prototype that might be used to detect groundwater deep inside Mars.

Known as the Mars Time Domain Electromagnetic Sounder (MTDEM), the instrument uses induction to generate electrical currents in the ground, whose secondary magnetic fields are in turn detected at the planetary surface.

In this way, the electrical conductivity of the subsurface can be reconstructed.

“Groundwater that has been out of atmospheric circulation for eons will be very salty,” said the project’s principal investigator Dr. Robert Grimm, a director in the Space Science and Engineering Division at Southwest Research Institute. “It is a near-ideal exploration target for inductive systems,” he added.

The inductive principle of the MTDEM is distinct from the wavelike, surface-penetrating radars MARSIS and SHARAD presently orbiting Mars.

“The radars have been very useful in imaging through ice and through very dry, low-density rock, but they have not lived up to expectations to look through solid rock and find water,” said Grimm.

The time-domain inductive method uses a large, flat-lying loop of wire on the ground to generate and receive electromagnetic signals.

In order to do this robotically, the team developed a launch system that shoots two projectiles, each paying out spooled wire as they fly.

Data taken during the test launches allowed Warden and Grimm to scale the system for a flight mission. The MTDEM prototype deployed to a distance of more than 70 meters.

For Mars, a system deploying a 200-meter loop would be less than 6 kilograms mass and could detect groundwater at depths up to 5 kilometers (3 miles). Most of the instrument’s mass would be in the loop and deployment system.

According to Barry Berdanier, the Ball electrical engineer who built the MTDEM electronics, the flight electronics would comprise just a few hundred grams.

“Electromagnetic induction methods are widely used in groundwater exploration,” said James Pfieffer of Zapata Incorporated, a geophysical firm that provided field support.

“Subsurface, liquid water on Mars could be a habitable zone for microbes. We know that huge volumes of discharged groundwater have shaped Mars’ ancient surface,” said Grimm. (ANI)

Saturn’s moon Enceladus may host a salty ocean

London, June 25 (ANI): A new research by European scientists has provided evidence that an enormous plume of water spurts in giant jets from the south pole of Saturn’s moon Enceladus is fed by a salty ocean, a discovery that may have implications for the search for extraterrestrial life.

The Cassini spacecraft made a surprising discovery about Saturn’s sixth largest moon, Enceladus, on its exploration of the giant ringed planet in 2005.

Enceladus ejects water vapor, gas and tiny grains of ice into space hundreds of kilometers above the moon’s surface.

Enceladus orbits in Saturn’s outermost “E” ring. It is one of only three outer solar system bodies that produce active eruptions of dust and vapor.

Moreover, aside from the Earth, Mars, and Jupiter’s moon Europa, it is one of the only places in the solar system for which astronomers have direct evidence of the presence of water.

New understanding of how this plume is produced was revealed in 2008 by Juergen Schmidt of the University of Potsdam, Germany, and Nikolai Brilliantov of the University of Leicester, and colleagues.

They explained how the water vapor jets are blasted out much faster than the dust particles. To work their theory required that Enceladus has an ocean of liquid water below its surface.

The same team, working with Frank Postberg of the University of Heidelberg and the Max Planck Institute for Nuclear Physics, in Heidelberg, has now found the direct experimental evidence for the presence of this ocean, which was previously lacking.

Current theories of satellite formation suggest that should a moon have a deep liquid ocean in contact with the body’s rocky core, for many millions of years, then it should be a salty ocean.

The team now reports the detection of sodium salts among the dust ejected in the Enceladus plume.

Postberg and colleagues have studied data from the Cosmic Dust Analyzer (CDA) onboard the Cassini spacecraft and have combined this data with laboratory experiments.

They have shown that the icy grains in the Enceladus plume contain substantial quantities of sodium salts, hinting at the salty ocean deep below.

The theory, proposed by Brilliantov and Schmidt, has allowed the team to relate the detected salt in the CDA with the likely concentration in the water vapor above the ocean, which proves the consistency of the experimental data.

The results of the study imply that the concentration of sodium chloride in the ocean can be as high as that of Earth’s oceans and is about 0.1-0.3 moles of salt per kilogram of water. (ANI)