NASA’s Mars rovers set new longevity record

Washington, May 20 (ANI): NASA”s Mars Exploration Rover Project has set a longevity record on the Red Planet.

The Opportunity rover will surpass the duration record set by NASA”s Viking 1 Lander, which operated on Martian soil for six years and 116 days.

Although Spirit began working on Mars three weeks before Opportunity, it has been out of communication since March 22.

Only if it awakens from hibernation and resumes communication, will it attain the Martian surface longevity record.

NASA”s Mars Odyssey, in orbit since in 2001, has been working at Mars longer than any other current mission and is on track to take the Mars longevity record later this year.

Discoveries by the Mars Exploration Rover have included Opportunity finding the first mineralogical evidence that Mars had liquid water and Spirit finding evidence for hot springs or steam vents and a past environment of explosive volcanism. (ANI)

Newly discovered exoplanet may have water

Washington, March 19 (ANI): Scientists have suggested that the newly discovered planet Corot-9b is temperate enough to allow the presence of liquid water.

Corot-9b was found on 16 May 2008 and orbits its star every 95.274 days, a little longer than Mercury takes to go round the Sun.

It is the first transiting planet to have both a longer period and a near-circular orbit.

A transit is a kind of eclipse and occurs when a celestial body passes in front of its host star and blocks some but not all of the star’s light.

Corot-9b’s orbit is slightly elliptical but at closest approach to its parent star it reaches a distance of 54 million kilometers.

Although that is only about the distance of Mercury in our Solar System, it is by far the largest orbit of any transiting planet found so far.

Because it orbits a star cooler than our Sun, calculations estimate that Corot-9b’s temperature could lie somewhere between -23 degrees C and 157 degrees C.

Corot-9b has a radius around 1.05 times that of Jupiter but only 84 percent of the mass. This leads to a density of 0.90 g/cc, or 68 percent that of Jupiter.

“Corot-9b is the first exoplanet that is definitely similar to a planet in our Solar System,” said Hans Deeg, a researcher at the Instituto de Astrofisica de Canarias.

The similarity is caused by the fact that Corot-9b is sufficiently far from its star to prevent tidal forces from heating its interior.

Tidal forces are created by the strength of gravity weakening from the front to back of the celestial body.

When the difference between the near side and the far side is great, the tidal force can prevent the planet from spinning quickly, forcing it to only show one face to the star.

It can also provide heat to the interior of the planet, changing its physical condition.

Based on calculations, neither of these is possible in this case.

“Although we don’t know, because we can’t see the planet directly, there is reason to believe that this planet has a normal day-night cycle,” said Malcolm Fridlund, ESA Project Scientist for Corot.

It means that lacking a tidal heat source, Corot-9b’s interior is likely to have remained similar to the gas giants in our Solar System. (ANI)

New evidence confirms presence of oceans on Earth 4 bln yrs ago

Sydney, March 15 (ANI): A study of crystals found in Greenland has provided for new evidence of the theory that oceans covered the Earth four billion years ago.

According to a report by ABC Science, the Australian and Swedish researchers, led by geochronologist Dr Chris Kirkland, from the Western Australian Department of Mines and Petroleum, have found evidence from sandstones in the Moræneso Formation in North Greenland, which confirms the presence of oceans on the early Earth.

The researchers analysed the ratio of heavy to light isotopes of oxygen in zircons ranging from 900 to 3900 million years old.

They compared this isotopic ratio to the current average isotopic ratio of oceans called the ‘standard mean ocean water’.

“The nice thing is there is one grain that confirms the Jack Hills results and that is really critical in science,” said study co-author Dr Martin Van Kranendonk, also from the Department of Mines and Petroleum.

“Before we only had that data from one locality, now we have the same result literally from the other side of the world,” he added.

The isotopic composition of this grain shows that it must have been altered by low temperature, near surface conditions, which points to weathering by liquid water.

“Rain is probably not enough to give this sort of a signature because we are dealing with large areas of exposed rocks and they have been significantly altered (by weathering),” said Van Kranendonk.

“The volume of water must have been significant,” he added.

Since subduction is needed to drag water into the crust, the finding also confirms that plate tectonics, the cycling of the Earth’s crust, was happening at this time, albeit in a different way, according to the researchers.

Van Kranendonk said that the evidence points to a weaker, hotter crust sinking at a shallower angle into the underlying mantle.

The research also confirms a suspected shift in the composition of the Earth’s crust 2.5 billion years ago.

“We think this oxygen isotope value shows changes in the style of continental crust, and reflects the continents getting stiffer,” Van Kranendonk said. (ANI)

How life might evolve with “exotic” biochemistry and solvents

London, September 18 (ANI): Scientists at a new interdisciplinary research group in Austria are working to uncover how life might evolve with “exotic” biochemistry and solvents, such as sulfuric acid instead of water.

The research group for Alternative Solvents as a Basis for Life Supporting Zones in (Exo-) Planetary Systems was established by the University of Vienna.

Traditionally, planets that might sustain life are looked for in the ‘habitable zone’, the region around a star in which Earth-like planets with carbon dioxide, water vapor and nitrogen atmospheres could maintain liquid water on their surfaces.

Consequently, scientists have been looking for biomarkers produced by extraterrestrial life with metabolisms resembling the terrestrial ones, where water is used as a solvent and the building blocks of life, amino acids, are based on carbon and oxygen.

However, these may not be the only conditions under which life could evolve.

“It is time to make a radical change in our present geocentric mindset for life as we know it on Earth,” said scientist Johannes Leitner.

“Even though this is the only kind of life we know, it cannot be ruled out that life forms have evolved somewhere that neither rely on water nor on a carbon and oxygen based metabolism,” he added.

One requirement for a life-supporting solvent is that it remains liquid over a large temperature range.

Water is liquid between 0 degree Celsius and 100 degrees C, but other solvents exist which are liquid over more than 200 degrees C.

Such a solvent would allow an ocean on a planet closer to the central star.

The reverse scenario is also possible. A liquid ocean of ammonia could exist much further from a star.

Furthermore, sulfuric acid can be found within the cloud layers of Venus and it is now known that lakes of methane/ethane cover parts of the surface of the Saturnian satellite Titan.

Consequently, the discussion on potential life and the best strategies for its detection is ongoing and not only limited to exoplanets and habitable zones.

The newly established research group at the University of Vienna, together with international collaborators, will investigate the properties of a range of solvents other than water, including their abundance in space, thermal and biochemical characteristics as well as their ability to support the origin and evolution of life supporting metabolisms. (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)

Mars quite similar to planet Earth

Washington, July 3 (ANI): A new research has determined that many characteristics of Mars are quite similar to planet Earth, including its landscape, history of water, soil and even its weather.

The research, by Mark Lemmon, a professor of atmospheric sciences, Texas A and M University, US, points out that last year’s Phoenix Mars Lander mission keeps revealing secrets about the planet, answering some questions but raising other big ones.

“Phoenix landed in a place that has access to Martian ice, which is exciting by itself,” Lemmon said of the Mars probe, which landed May 25, 2008.

The mission goals were to investigate the suitability of Mars for past or present life, but Phoenix was incapable of detecting life itself.

“Phoenix was designed to verify and investigate subsurface ice, and it found it almost instantly,” explained Lemmon. “The entire area where it landed has water ice just a few inches under the soil. The area is cold now, but it has been warmer in the past,” he added.

“No water in a liquid state has been found yet, but there is new evidence that Mars had liquid water billions of years ago,” said Lemmon.

Using its robotic arm, the Mars Lander was able to scoop up dirt, which was mixed with ice, and analyze it.

“Where it landed is a barren place that resembles the dry valleys of Antarctica. The area has mounds and troughs, and just like in Antarctic valleys, there is no liquid water but plenty of ice,” said Lemmon.

“Some of these patches are fairly pure. Others have the ice mixed with soil containing energy sources and nutrients that could be used if there were life,” he added.

According to Lemmon, the soil has perchlorate, a form of chlorine that is considered hazardous, but certain types of bacteria are able to live on it here.

“The interesting thing is, the soil has a potential energy source and oxygen source for life on Mars,” he said.

Traces of calcite were also found, which shows a presence of liquid water at some time in the past, Lemmon notes.

Phoenix also found weather patterns similar to those on Earth, including cold fronts that bring in gusty winds and sub-freezing temperatures.

Another bonus: Phoenix saw small Martian snowflakes, which leads the team to believe that snowfall on Mars was once a common occurrence.

“To sum it up, we found a place on Mars that is similar to cold, dry environments on Earth, and those environments are capable of supporting life,” Lemmon explained. (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)

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)

New technique could find water and life on Earth-like planets

Washington, May 26 (ANI): Using instruments aboard the Deep Impact spacecraft, a team of astronomers and astrobiologists has devised a technique to tell whether an Earth-like exoplanet harbors liquid water, which in turn could tell whether it might be able to support life.

“Liquid water on the surface of a planet is the gold standard that people are looking for,” said Nicolas Cowan, a University of Washington doctoral student in astronomy and lead author of a paper explaining the new technique.

As part of NASA’s Extrasolar Planet Observation and Characterization mission, the scientists obtained two separate 24-hour observations of light intensity from Earth in seven bands of visible light, from shorter wavelengths near ultraviolet to longer wavelengths near infrared.

Earth appears gray at most wavelengths because of cloud cover, but it appears blue at short wavelengths because of the same atmospheric phenomenon that makes the sky look blue to people on the surface.

The researchers studied small deviations from the average color caused by surface features like clouds and oceans rotating in and out of view.

They found two dominant colors, one reflective at long, or red, wavelengths and the other at short, or blue, wavelengths.

They interpreted the red as land masses and the blue as oceans.

According to Cowan, the analysis was undertaken “as if we were aliens looking at Earth with the tools we might have in 10 years” and did not already know Earth’s composition.

“You sum up the brightness into a single pixel in the telescope’s camera, so it truly is a pale blue dot,” he said.

Since Earth’s colors changed throughout the 24-hour-long observations, the scientists made maps of the planet in the dominant red and blue colors and then compared their interpretations with the actual location of the planet’s continents and oceans.

“You could tell that there were liquid oceans on the planet,” Cowan said.

“The idea is that to have liquid water the planet would have to be in its system’s habitable zone, but being in the habitable zone doesn’t guarantee having liquid water,” he added.

The observations on March 18 and June 4, 2008 were made when the spacecraft was between 17 million and 33 million miles from Earth, and while it was directly above the equator.

“Observations from above a polar region likely would show up as white,” Cowan said.

“It will be some years before the launch of space telescopes capable of making similar observations for Earth-sized exoplanets, but devising this technique now could guide the construction of those instruments,” he explained. (ANI)

New technique will detect water on earth-like planets

Washington, May 26 (IANS) Since the early 1990s, astronomers have discovered more than 300 planets orbiting far away stars, nearly all of them being gas giants like Jupiter. Now, powerful telescopes, similar to NASA’s recently launched Kepler Mission, will help spot much smaller rocky extrasolar planets, or exoplanets with water, more similar to earth.

Seen from dozens of light years away, an exoplanet will appear a little more than a “pale blue dot,” the term coined by late astronomer Carl Sagan to describe how earth appeared in a 1990 photograph taken by the Voyager spacecraft from near the edge of the solar system.

Using instruments aboard the Deep Impact spacecraft, a team of astronomers and astrobiologists has devised a technique to tell whether such a planet harbours liquid water, which in turn could tell whether it might be able to support life.

“Liquid water on the surface of a planet is the gold standard that people are looking for,” said Nicolas Cowan, University of Washington (UW) doctoral astronomy student who led the study.

As part of NASA’s Extrasolar Planet Observation and Characterisation mission, scientists obtained two separate 24-hour observations of light intensity from earth in seven bands of visible light, from shorter wavelengths near ultraviolet to longer wavelengths near infrared.

The analysis was undertaken “as if we were aliens looking at earth with the tools we might have in 10 years” and did not already know earth’s composition, Cowan said. “You sum up the brightness into a single pixel in the telescope’s camera, so it truly is a pale blue dot.”

“You could tell that there were liquid oceans on the planet,” Cowan said. “The idea is that to have liquid water the planet would have to be in its system’s habitable zone, but being in the habitable zone doesn’t guarantee it having liquid water.”

The observations on March 18 and June 4, 2008 were made when the spacecraft was between 17 million and 33 million miles from Earth, and while it was directly above the equator.

Observations from above a polar region likely would show up as white, Cowan said, according to an UW release.

These findings will be published in Astrophysical Journal.

Scientists see evidence of young and vast river valleys on Mars

Washington, May 7 (ANI): A team of scientists has reported evidence of young and vast river valleys on Mars, which date back to 1.8 billion years.

Most river valley systems on Mars existed only during the early history of the planet, before a major climate transition to colder, drier conditions.

Now, J. L. Dickson, C. I. Fassett, J. W. Head, from the Department of Geological Sciences, Brown University, Providence, Rhode Island, US, have reported evidence of younger fluvial valley systems that formed during the middle to late Amazonian epoch, which extends from about 1.8 billion years ago to the present.

The data suggests that these fluvial valley systems, located in the Lyot crater in the northern midlatitudes, are tens of kilometers in length and are among the youngest river valley systems of this size reported to date.

Past research indicates that conditions overall on Mars during the middle to late Amazonian were too cold to support liquid water.

However, the researchers propose that in the microenvironment of the Lyot crater, high surface pressure due to low elevation, combined with local temperature conditions, at times made possible the melting of surface ice.

They suggest that observed glacial deposits in the crater indicate that glaciers provided the continuous melt water needed to form these fluvial valley systems. (ANI)

Orange stars may have planets having life

London, May 7 (ANI): A new analysis has suggested that the best bet that scientists have in finding life in the Universe may be around stars a little less massive than the sun, called ‘orange dwarfs’.

According to a report in New Scientist, these stars live much longer than sun-like stars, and have safer habitable zones – where liquid water can exist – than those of lighter red dwarf stars.

Stars similar in mass to the sun, categorised as a yellow dwarf, have received the most attention from planet hunters.

Edward Guinan of Villanova University in Pennsylvania, US, leads a team that has been studying how the properties of stars vary with mass.

But, recent research suggests orange dwarfs may provide an even better hunting ground for life-bearing planets.

The team is using observations from a variety of sources, such as archival measurements from the ROSAT X-ray satellite, and more recent measurements from ground-based telescopes.

The results confirm that red dwarf stars, which weigh between 10 and 50 percent as much as the sun, are far more prone to unleashing powerful flares that can deliver deadly radiation to nearby planets.

This activity declines as the red dwarfs age, and scientists have not ruled out red dwarf planets as potential abodes for life, but any such life would certainly face some big challenges.

Orange dwarfs, on the other hand, with masses between 50 and 80 percent that of the sun, have only a little bit more flare activity than sun-like stars.

They would also provide a haven for life for a much longer time – roughly double the 10-billion-year lifetime of a sun-like star.

Moreover, they change very little in brightness compared to sun-like stars.

The odds of intelligent life arising may be better on planets around orange dwarfs than sun-like stars, given the extra time available for it to evolve.

That makes orange dwarfs not only good targets for habitable planet searches, but for the search for extraterrestrial intelligence (SETI) as well, according to Guinan.

“There are old ones around – some are 8 to 9 billion years old, and could have planets that are more evolved,” he told New Scientist.

Orange dwarfs are about three to four times as abundant as sun-like stars, making planet searches easier.

Some planets have already been found around orange dwarfs, though outside the stars’ habitable zones.

But, according to Gregory Laughlin of the University of California, Santa Cruz, it should be possible with current technology to find Earth-mass planets in the habitable zones of nearby orange dwarfs.

“They do seem to be a sweet spot for prospects of actually detecting habitable planets,” he said. (ANI)

Flowers may bloom on Jupiter’s icy moon Europa

London, May 6 (ANI): Scientists have suggested that spacecraft should hunt for signs of life on Jupiter’s ice-covered moon Europa, since it would be detectable there in the form of blooming flowers.

Europa, which is thought to have an ocean of liquid water beneath its icy shell, has long been a target for astrobiologists, who suspect the interior could be salubrious for life.

But, digging deep into the moon’s icy shell could be difficult. Estimates of the thickness of the ice have ranged between less than a kilometre to more than 100 km.

Life could be visible from orbiting spacecraft, however, if it made a home in cracks in Europa’s shell that connect the surface to the interior, Physicist and futurist Freeman Dyson told New Scientist.

Such life might take the form of flowers with a parabolic shape that focuses the dim sunlight falling on Europa on the interior of the plant.

Flowers with such shapes are found in Arctic climes on Earth, where the plants have evolved to maximize solar energy.

According to Dyson, Europa flowers could be detectable through a phenomenon called retroreflection, in which light gets reflected back to its source.

This optical effect is seen in light reflected from animals’ eyes, and was used in the design of road signs and mirrors left behind on the moon by Apollo astronauts.

Although Dyson’s ‘sunflowers’ may get their start on Europa, they could conceivably spread elsewhere in the solar system.

“You can imagine once you have flowers that get nourished from below, they could evolve in the direction of being independent,” Dyson said.

“If plants spread to smaller, more distant objects in the solar system’s two cometary reservoirs, the Kuiper belt and the Oort cloud, they would be less subject to gravity and could easily grow in size to maximize solar collection,” he added.

Europa will be one of two moons explored in depth by a planned collaboration between NASA and the European Space Agency beginning in 2026,when a pair of orbiters are set to reach Jupiter. (ANI)

Salt in ice plume on Enceladus points to presence of liquid ocean

London, April 30 (ANI): Scientists, studying measurements made by Cassini spacecraft, have found salt in the ice plumes that bloom above Saturn’s moon Enceladus, which suggest the presence of a liquid ocean on the satellite.

The Cassini spacecraft flew through a plume on October 9, 2008, and measured the molecular weight of chemicals in the ice.

According to a report in New Scientist, Frank Postberg of the Max Planck Institute for Nuclear Physics in Heidelberg, Germany, and colleagues, found traces of sodium in the form of salt and sodium bicarbonate.

The chemicals would have originated in the rocky core of Enceladus, so to reach a plume they must have leached from the core via liquid water.

Observations from Earth in 2007 spotted no sign of sodium, casting doubt on such a subsurface sea.

Although the salt could have been leached out by an ancient ocean which since froze solid, that freezing process would concentrate most of the salt very far from the surface of the moon’s ice, according to Julie Castillo of NASA’s Jet Propulsion Laboratory in Pasadena, California.

“It is easier to imagine that the salts are present in a liquid ocean below the surface,” she said. “That’s why this detection, if confirmed, is very important,” she added. (ANI)

Mars domes may be mud volcanoes

London, March 27 (ANI): Scientists at NASA have identified dozens of mounds or domes in the northern plains of Mars, which they say bear a striking resemblance to mud volcanoes.

According to a report by BBC News, the domes on the Red Planet were detected using images taken by NASA’s Mars Odyssey spacecraft, and Carlton Allen and Dorothy Oehler of NASA’s Johnson Space Center in Houston.

Infrared data also show the domes cool more quickly at night than the surrounding rock, as one might expect if they were made of sediment.

Together with David Baker from Brown University, the researchers used instruments on NASA’s Mars Reconnaissance Orbiter (MRO) to observe several of these structures in a northern region known as Acidalia Planitia.

Data from the MRO’s Crism experiment indicate that the material in the domes is more oxidised than the rock of the surrounding plains.

This might suggest the presence of iron oxides, which form in the presence of liquid water.

They also took pictures of the structures with the HiRise camera on MRO; the images show the bright domes standing out against the dark basaltic rock of the surrounding plains.

Dr Allen told BBC News the structures resembled smooth cones with “no breaks”, which visibly feathered out towards the margins.

The observations, he said, were consistent with material that is “smooth, soft and easily eroded”.

On Earth, the largest concentration of mud volcanoes is in Azerbaijan and the adjacent Caspian Sea. But, they have been found at more than 40 sites on land and at more than 20 locations beneath the sea.

They are formed when pressurized gas and liquid from as much as several kilometers down, breach the surface. They belch out slurries of fluid, mud and rocks, as well as gases such as methane.

“In Azerbaijan, there is so much methane coming out that they can catch fire,” said Dr Allen.

This raises the possibility that mud volcanoes could contribute to the methane observed in the Martian atmosphere.

Methane should last for only a short time in the atmosphere until it is destroyed by sunlight, so its continued presence means it is being replenished by some unknown process.

According to Dr Allen, the team had found no evidence that the domes could be active today, as most show clear evidence of erosion. But, he suggested they could have formed in the last 10 million years.

Researchers suggest that, if life does exist deep beneath the Martian surface, mud volcanoes could be one of the best ways to get at the evidence. (ANI)

Life might be bubbling in Martian mud

London, March 21 (ANI): Using images from the Mars Odyssey spacecraft, NASA scientists have discovered what could be mud volcanoes on the planet, in which life might be bubbling in muddy squirts.

According to a report in New Scientist, Dorothy Oehler and Carlton Allen of NASA’s Johnson Space Center in Houston, Texas, identified dozens of mounds at a site in the northern plains of Mars that bear a striking resemblance to mud volcanoes on Earth.

These form a distinctive large hill of sediment with a central crater.

Further evidence comes from infrared images of the Martian mounds, which show that they cool down more quickly at night than rock should, suggesting they are made of a fine-grained sediment such as mud.

Together with David Baker of Brown University in Providence, Rhode Island, Allen and Oehler also took a fresh look at some possible mud volcanoes identified previously by other researchers, about 1000 kilometers further north.

Using light spectra of the mounds recorded by the Mars Reconnaissance Orbiter, they found hints of iron oxides, which form in the presence of liquid water.

Jack Farmer of Arizona State University in Tempe agrees that the mounds could be mud volcanoes, but cautions that other processes, like the retreat of glaciers, can leave behind similar heaps of sediment.

“Nonetheless, studying the clay from mud volcanoes would be of great interest,” he said.

“Clays have the ability to sequester organic molecules, like ammonia and proteins. They might retain a memory of any organisms that were there,” he added. (ANI)

Liquid saltwater on Mars detected by NASA’s Phoenix Lander

Washington, March 18 (ANI): A new analysis by a group of mission scientists has determined that salty, liquid water has been detected on a leg of the Mars Phoenix Lander and therefore could be present at other locations on the Red Planet.

This is the first time liquid water has been detected and photographed outside the Earth.

“A large number of independent physical and thermodynamical evidence shows that saline water may actually be common on Mars,” said Nilton Renno, a professor in the U-M Department of Atmospheric, Oceanic and Space Sciences and a co-investigator on the Phoenix mission.

“Liquid water is an essential ingredient for life. This discovery has important implications to many areas of planetary exploration, including the habitability of Mars,” he added.

Previously, scientists believed that water existed on Mars only as ice or water vapor because of the planet’s low temperature and atmospheric pressure.

They thought that ice in the Red Planet’s current climate could sublimate, or vaporize, but they didn’t think it could melt.

This analysis shows how that assumption may be incorrect.

“Temperature fluctuation in the arctic region of Mars where Phoenix landed and salts in the soil could create pockets of water too salty to freeze in the climate of the landing site,” Renno said.

Photos of one of the Lander’s legs show droplets that grew during the polar summer.

Based on the temperature of the leg and the presence of large amounts of “perchlorate” salts detected in the soil, scientists believe the droplets were most likely salty liquid water and mud that splashed on the spacecraft when it touched down.

The Lander was guided down by rockets whose exhaust melted the top layer of ice below a thin sheet of soil.

“Some of the mud droplets that splashed on the Lander’s leg appear to have grown by absorbing water from the atmosphere,” Renno said.

Images suggest that some of the droplets darkened, then moved and merged – physical evidence that they were liquid.

Thermodynamic calculations offer additional evidence that salty liquid water can exist where Phoenix landed and elsewhere on Mars.

The calculations also predict a droplet growth rate that is consistent with what was observed. (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)

NASA’s Kepler mission blasts off in search of Earth-like planets

Washington, March 7 (ANI): NASA’s Kepler mission, which would search other Earth-like planets, has been successfully launched into space from Cape Canaveral Air Force Station, Florida, US, aboard a United Launch Alliance Delta II.

Kepler is designed to find the first Earth-size planets orbiting stars at distances where water could pool on the planet’s surface. Liquid water is believed to be essential for the formation of life.

“It was a stunning launch,” said Kepler Project Manager James Fanson of NASA’s Jet Propulsion Laboratory in Pasadena, California.

“Our team is thrilled to be a part of something so meaningful to the human race – Kepler will help us understand if our Earth is unique or if others like it are out there,” he added.

Engineers acquired a signal from Kepler at 12:11 a.m. on March 7th, after it separated from its spent third-stage rocket and entered its final sun-centered orbit, trailing 950 miles behind Earth.

The spacecraft is generating its own power from its solar panels.

“Kepler now has the perfect place to watch more than 100,000 stars for signs of planets,” said William Borucki, the mission’s science principal investigator at NASA’s Ames Research Center at Moffett Field, California.

“Everyone is very excited as our dream becomes a reality. We are on the verge of learning if other Earths are ubiquitous in the galaxy,” he added.

Engineers have begun to check Kepler to ensure it is working properly, a process called “commissioning” that will take about 60 days.

In about a month or less, NASA will send up commands for Kepler to eject its dust cover and make its first measurements.

After another month of calibrating Kepler’s single instrument, a wide-field charge-couple device camera, the telescope will begin to search for planets.

The first planets to roll out on the Kepler “assembly line” are expected to be the portly “hot Jupiters” – gas giants that circle close and fast around their stars.

Neptune-size planets will most likely be found next, followed by rocky ones as small as Earth.

The true Earth analogs – Earth-sized planets orbiting stars like our sun at distances where surface water, and possibly life, could exist – would take at least three years to discover and confirm.

Ground-based telescopes also will contribute to the mission by verifying some of the finds.

In the end, Kepler will give us our first look at the frequency of Earth-size planets in our Milky Way galaxy, as well as the frequency of Earth-size planets that could theoretically be habitable. (ANI)