Archive for martian surface

Curiosity Makes Its Way to First Mars Experiment

This mosaic from the Mast Camera on NASA's Curiosity rover shows the view looking toward its first science destination, the Glenelg area, where three different types of Martian terrain come together. (Image: NASA/JPL-Caltech/MSSS)

This mosaic from the Mast Camera on NASA’s Curiosity rover shows the view looking toward its first science destination, the Glenelg area, where three different types of Martian terrain come together. (Image: NASA)

The Mars rover Curiosity is about to undertake its first major scientific experiment on the Red Planet.Before Curiosity heads off to its primary destination, the foothills of Mount Sharp, scientists want to learn more about the terrain surrounding the rover’s landing site.

The Mars mission team members are  fascinated with the geology of the area, according to Rob Manning, the Mars Science Laboratory’s (MSL) chief engineer.  They’ve noticed  the surface is covered with a type of gravelly material, rocks called cobbles and various collections of compressed soil.

“It may very well be that we’re on a place that has been affected by water in the past, and that’s very exciting because that’s what we had hoped for,”  Manning said.

Photo of the Martian surface that includes a map of the route driven by NASA's Mars rover Curiosity from it's landing site on the first day of its trip to the Glenelg area through the 43rd Martian day, or sol, of the rover's mission on Mars (Sept. 19, 2012). The image used for the map is from an observation of the landing site by the High Resolution Imaging Science Experiment (HiRISE) instrument on NASA's Mars Reconnaissance Orbiter. (Image: NASA/JPL-Caltech/Univ. of Arizona)

Photo of the Martian surface, including a map of the route driven by NASA’s Mars rover on its trip to the Glenelg area on the 43rd Martian day of Curiosity’s mission on Mars – Sept. 19, 2012.  (Image: NASA)

Since landing seven weeks ago, Curiosity has traveled about 290 meters, approximately the length of an American football field. The rover is now traveling in a different direction toward a location called Glenelg, which lies about 400 meters east-southeast of Curiosity’s landing site.

One  type of terrain  scientists want to learn more about is a kind of bedrock which could be suitable for eventual drilling by Curiosity.

The next is an area  marked by many small craters and scientists believe it might represent an older or harder Martian surface.

The third terrain is similar to  the type where the rover landed.  It’s of particular interest to team members because they’d like to determine if it contains rocks with the same kind of texture as those found in an area close to the landing site where blasts from the descent stage rocket engines scoured away some of the surface.

On its way to Glenelg this week, the rover came across an unusual pyramid-shaped rock. The rover team is planning to touch this mystery rock with a spectrometer to determine its basic composition. They’ll also use an arm-mounted camera to take close-up photographs.  This encounter will likely be the first time  the rover  uses its robotic arm to touch a Martian rock.

Curiosity will then continue on its voyage to Glenelg, where the team will choose another rock for the rover’s first analysis of powder drilled from interiors of rocks.

On it's trip to the Glenelg area the Curiosity recently came accross this interesting pyramid shaped rock that's about 25 centimeters tall and 40 centimeters wide. The rover team has assessed it as a suitable target for the first use of Curiosity's contact instruments on a rock. (Photo:  NASA/JPL-Caltech)

On it’s trip to Glenelg, Curiosity came across this pyramid-shaped rock, which NASA says will be a suitable target for the first use of the rover’s contact instruments. (Photo: NASA)

Once the rover’s side trip to Glenelg concludes, Curiosity will head toward its primary destination, Mount Sharp, which may take a year or two to reach.

Manning tells us everything on the rover has worked perfectly so far except for one of Curiosity’s wind sensors, which was damaged when Martian pebbles hit it.  Since the rover has other wind sensors, the mission should not be impacted.

In fact, the mission is going so well the rover team is amazed everything is working so much better on Mars than it did while undergoing testing here on Earth.

Manning says the rover experienced problem after problem during testing. After seeing the rover perform so well on the Red Planet, the MSL team has concluded Curiosity would rather be on Mars than on its home planet.

And it’s a good thing because Curiosity’s visit there could be extended.

The rover’s older sibling,  Opportunity, has continued to roam and examine the planet, long after the planned end of its mission. Manning expects Curiosity will do likewise.

There are several factors which justify that optimism. The rover’s power source, according to Manning, is producing more energy than expected. The team also found the Martian climate is better than was anticipated so the unit doesn’t need as much heating as was first thought.  Also, with NASA’s orbiting spacecraft flying overhead, the rover has been able to save a great deal of energy while sending back information, which could allow Curiosity to operate longer.

Curiosity's primary destination, the base of Mount Sharp. (Photo: ASA/JPL-Caltech/MSSS)

Curiosity’s primary destination, the base of Mount Sharp. (Photo: NASA)

If  Curiosity’s time on Mars is extended, Manning expects the rover to continue its voyage up Mount Sharp, which is made up of various layers of material, with the oldest at the bottom of the mountain and the youngest at its peak.

At each of these layers, Manning says that, there will be an opportunity to look back in time into the Martian geological history.  So as long as the rover keeps working and NASA extends its mission, “we will continue going up and explore and explore and there is a chapter, chapter and chapter of books telling us about Mars just ahead of us.”

This weekend on the radio edition of Science World, Rob Manning joins us to provide an update with the latest on Curiosity’s mission.

Check out the right column for scheduled air-times or listen now to the interview below.

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Article source: http://blogs.voanews.com/science-world/2012/09/22/curiosity-makes-its-way-to-first-mars-experiment/

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Hot Mars Theory suggests life never had a chance on the Red Planet


George Dvorsky

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Hot Mars Theory suggests life never had a chance on the Red Planet As NASA’s Curiosity rover scours the Martian surface in search of signs that Mars was once capable of fostering complex life, a team of researchers from the University of Poitiers, France, and Caltech have issued a paper that casts serious doubt on the notion that the planet was once habitable.

The new theory, which was published in Nature Geoscience, indicates that clay found on the Martian surface was formed in water-rich magma — water that would be way too hot to support life.

To make their case, a research team led by Alain Meunier studied clay minerals and rocks collected from an old A-bomb test site in French Polynesia. The geologists discovered that the clay minerals bore a remarkable resemblance to the ones observed on Mars. But unlike the South Pacific clays, which were products of weathering by liquid water, the ones on Mars were formed directly from water-rich molten rock as they cooled.

Reporting for the BBC, Jonathan Amos explains further:

It is interesting because it strikes at the heart of the notion that the Red Planet was awash with water, perhaps at its surface, more than 3.75 billion years ago – an idea that has been put forward to explain the great abundance of some clay deposits observed from orbit by satellites.

However, the process of clay production at Mururoa, if replicated and widespread on early Mars, would remove the need for such large volumes of water, and with it possibly a more benign environment for life to establish itself on the planet.

“Mars was not as warm and wet in its earliest time as some have suggested. I do not believe in an early ocean on Mars,” Prof Meunier told BBC News.

But [The Mururoa process] explains only the earliest generation of clays on Mars, in the early Noachian period. In later periods, liquid water has existed on Mars’ surface; that is undoubtedly the case.”

And as the LA Times’ Amina Khan notes, this has serious implications for Martian habitability:

On Earth, clays are remarkably good at trapping organic material. So if organic compounds existed on Mars, clays would be a good place to find them.

If either of the prevailing theories about water is true, the Martian environment could have been hospitable for life, Ehlmann said. Superheated water and magma? Not so much.

“The clays would form as the lava cools from 1,500 degrees Celsius,” she said. “That would not be a good habitat.”

But as Khan notes, the study leaves a number of questions unanswered:

“It’s certainly a different take on trying to explain the origin of some clay minerals on Mars,” [said planetary scientist Ralph Milliken] “It does have some merit, and alternative hypotheses need to be considered fully.”

But he said the story laid out in the new paper doesn’t explain why the Martian surface appears to have tracks cut by flowing liquid. Nor does it account for blueberry-shaped mineral deposits of hematite that scientists believe may have formed when water ran past them.

Again, Meunier is not claiming that surface water has never existed on Mars — merely that it wasn’t present during its early Noachian period (a time that might have been critical to the spawning of life). The jury, therefore, is still very much out on this one.

Read the entire paper here.

Other sources: BBC.

Top image: A three-dimensional image of the Nili Fossae region of Mars showing clays presence of abundant clays minerals (in magenta and blue hues) via NASA/JPL/JHUAPL.

Article source: http://io9.com/5941964/hot-mars-theory-suggests-life-never-had-a-chance-on-the-red-planet

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New Mars rover targets red planet’s biggest mysteries

(SPACE.com) Mars, our next-door neighbor in the solar system, hasn’t given up many of its secrets yet. But when NASA’s newest Mars rover, Curiosity, lands on the Red Planet next week, scientists hope to unlock a few more.

The centerpiece of the Mars Science Laboratory mission, the Curiosity rover comes packed with a slew of instruments to study not only today’s Martian surface, but also the surface of the past.

The overarching strategy of NASA’s Mars Exploration Program has long been to follow the water, and Curiosity is no exception. Following up on clues provided by previous missions, the newest rover will seek answers to questions about climate, geology, human exploration, and of course, whether or not the Red Planet could have once hosted life.

Where might Martian life make its home?

Curiosity won’t be searching for life directly. Project scientist John Grotzinger pointed out that such a search would require more sophisticated scientific equipment than even the advanced rover carries, if not a full-scale sample return mission. Instead, Curiosity will be searching for places where life could have evolved. [11 Amazing Things NASA's Huge Mars Rover Can Do]

“Curiosity is not a life mission,” Grotzinger told SPACE.com. “What we are doing in this mission is exploring for habitable environments.”

Because water is considered essential for the development of the only life known to exist — life on Earth — scientists are focusing on wet areas, past and present.

A potentially habitable environment would also contain chemical and mineralogical signatures suggesting the presence of an energy source that microorganisms could have used at some point. It might also boast signs of organic carbon, thought to be one of the building blocks of life.

The previous rovers, Spirit and Opportunity, were equipped to search for only water in the environments they explored. Grotzinger compared them to robotic geologists.

“Curiosity is both a robotic geologist and a robotic geochemist,” able to look for more than just water, he said.

Of course, even if Curiosity finds ample environments where life could have flourished, that doesn’t necessarily mean that it did.

“It’s entirely possible to find a habitable environment that was never inhabited, because life never originated,” Grotzinger said.

Either way, the rover can help pinpoint some of the best Martian environments to search for life on future missions, perhaps making them less hit-and-miss.

What made a wet Mars dry?

In its distant past, a warmer Mars likely sported a thicker, wetter atmosphere, with water running across its surface. Today, the planet is dry and dusty, with most of its water thought to be trapped beneath the surface.

Curiosity will land at the base of Mount Sharp, which rises 3 miles (5 kilometers) from the center of the Gale Crater. Named for planetary geologist Robert Sharp, the mountain has layers that will be open to exploration by the rover.

Grotzinger described these layers as pages in a book, with the first layers similar to the oldest chapters. As Curiosity ascends the mountain, it will explore the history of the planet embedded within the rocks.

“By the time we get done, we’ll get this great story on how the environment of Mars changed,” he said.

At the same time, the rover will explore shifts in the geology of the planet over millions of years, also folded into the rocks. Earlier rovers were able to find clues that water once existed on the surface of the planet, but Curiosity aims to dig deeper.

“With Spirit and Opportunity, we were only able to determine that water was there,” Grotzinger said. “We didn’t get so much insight into how the water was produced or the environments in which the rocks were formed.”

Studying the layers will provide hints about the geological activities that shaped and molded the Martian crust. [7 Biggest Mysteries of Mars]

But Curiosity won’t just be sampling the climate of the past. While exploring the Martian surface, the rover will analyze the composition of the planet’s climate today, measuring the temperature of the air, the ground, and the movement of the wind in its local area. When combined with the more regional measurements from space, the information should help provide a broader understanding of how the climate varies on the planet.

How much radiation will humans experience?

Some day, whether in the near or distant future, humans will travel to Mars. Before they arrive, they’ll want to know how much radiation they’ll have to deal with while on the ground. Readings taken by Curiosity should help solve that mystery.

On Earth, much of the radiation emitted by the sun is blocked by the thick atmosphere. However, Mars has less of a shield protecting it.

“No mission has ever measured the actual radiation on the surface before,” Grotzinger pointed out.

Knowing how much solar and cosmic radiation makes it to the ground will help future explorers know just how much protection they will need to don.

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Copyright 2012 SPACE.com, a TechMediaNetwork company. All rights reserved. This material may not be published, broadcast, rewritten or redistributed.

Article source: http://www.cbsnews.com/8301-205_162-57483404/new-mars-rover-targets-red-planets-biggest-mysteries/

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NASA’s Huge New Mars Rover Targets Biggest Red Planet Mysteries




Hubble photo of Mars

NASA’s Hubble Space Telescope snapped this shot of Mars on Aug. 26, 2003, when the Red Planet was 34.7 million miles from Earth. The picture was taken just 11 hours before Mars made its closest approach to us in 60,000 years.
CREDIT: NASA/ESA


Mars, our next-door neighbor in the solar system, hasn’t given up many of its secrets yet. But when NASA’s newest Mars rover, Curiosity, lands on the Red Planet next week, scientists hope to unlock a few more.

The centerpiece of the Mars Science Laboratory mission, the Curiosity rover comes packed with a slew of instruments to study not only today’s Martian surface, but also the surface of the past.

The overarching strategy of NASA’s Mars Exploration Program has long been to follow the water, and Curiosity is no exception. Following up on clues provided by previous missions, the newest rover will seek answers to questions about climate, geology, human exploration, and of course, whether or not the Red Planet could have once hosted life.



Where might Martian life make its home?

Curiosity won’t be searching for life directly. Project scientist John Grotzinger pointed out that such a search would require more sophisticated scientific equipment than even the advanced rover carries, if not a full-scale sample return mission. Instead, Curiosity will be searching for places where life could have evolved. [11 Amazing Things NASA's Huge Mars Rover Can Do]

“Curiosity is not a life mission,” Grotzinger told SPACE.com. “What we are doing in this mission is exploring for habitable environments.”

Because water is considered essential for the development of the only life known to exist — life on Earth — scientists are focusing on wet areas, past and present.

A potentially habitable environment would also contain chemical and mineralogical signatures suggesting the presence of an energy source that microorganisms could have used at some point. It might also boast signs of organic carbon, thought to be one of the building blocks of life.

The previous rovers, Spirit and Opportunity, were equipped to search for only water in the environments they explored. Grotzinger compared them to robotic geologists.

“Curiosity is both a robotic geologist and a robotic geochemist,” able to look for more than just water, he said.

Of course, even if Curiosity finds ample environments where life could have flourished, that doesn’t necessarily mean that it did.

“It’s entirely possible to find a habitable environment that was never inhabited, because life never originated,” Grotzinger said.

Either way, the rover can help pinpoint some of the best Martian environments to search for life on future missions, perhaps making them less hit-and-miss.

Artist's Conception of Curiosity Mars RoverWhat made a wet Mars dry?

In its distant past, a warmer Mars likely sported a thicker, wetter atmosphere, with water running across its surface. Today, the planet is dry and dusty, with most of its water thought to be trapped beneath the surface.

Curiosity will land at the base of Mount Sharp, which rises 3 miles (5 kilometers) from the center of the Gale Crater. Named for planetary geologist Robert Sharp, the mountain has layers that will be open to exploration by the rover.

Grotzinger described these layers as pages in a book, with the first layers similar to the oldest chapters. As Curiosity ascends the mountain, it will explore the history of the planet embedded within the rocks.

“By the time we get done, we’ll get this great story on how the environment of Mars changed,” he said.

At the same time, the rover will explore shifts in the geology of the planet over millions of years, also folded into the rocks. Earlier rovers were able to find clues that water once existed on the surface of the planet, but Curiosity aims to dig deeper.

“With Spirit and Opportunity, we were only able to determine that water was there,” Grotzinger said. “We didn’t get so much insight into how the water was produced or the environments in which the rocks were formed.”

Studying the layers will provide hints about the geological activities that shaped and molded the Martian crust. [7 Biggest Mysteries of Mars]

But Curiosity won’t just be sampling the climate of the past. While exploring the Martian surface, the rover will analyze the composition of the planet’s climate today, measuring the temperature of the air, the ground, and the movement of the wind in its local area. When combined with the more regional measurements from space, the information should help provide a broader understanding of how the climate varies on the planet.

How much radiation will humans experience?

Some day, whether in the near or distant future, humans will travel to Mars. Before they arrive, they’ll want to know how much radiation they’ll have to deal with while on the ground. Readings taken by Curiosity should help solve that mystery.

On Earth, much of the radiation emitted by the sun is blocked by the thick atmosphere. However, Mars has less of a shield protecting it.

“No mission has ever measured the actual radiation on the surface before,” Grotzinger pointed out.

Knowing how much solar and cosmic radiation makes it to the ground will help future explorers know just how much protection they will need to don.

Follow SPACE.com on Twitter @Spacedotcom. We’re also on Facebook  Google+

Article source: http://www.space.com/16819-mars-mysteries-nasa-curiosity-rover.html

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Mars Life Could Leave Traces in Red Planet’s Air: Study




Hubble photo of Mars

NASA’s Hubble Space Telescope snapped this shot of Mars on Aug. 26, 2003, when the Red Planet was 34.7 million miles from Earth. The picture was taken just 11 hours before Mars made its closest approach to us in 60,000 years.
CREDIT: NASA/ESA


If life exists on Mars, scientists may be able to detect it by measuring the amounts of hydrogen and methane in the Red Planet’s atmosphere, a new study suggests.

Finding lots of methane but relatively little hydrogen could be an indicator of active Martian life, according to the study. And scientists could make the needed measurements soon if they wanted to, researchers said.

“What’s really nice about this is that it is an incredibly simple method,” lead author Christopher Oze, of the University of Canterbury in New Zealand, said in a statement. “All you need to do is measure the methane and hydrogen levels on Mars, something that can easily be done now.”



The cold, dry and radiation-blasted Martian surface is generally viewed as inhospitable to life as we know it. But there could be oases of good habitat on the planet, in the form of hydrothermal systems, researchers say.

Scientists think hydrothermal systems — which bring together water and energy — have existed on Mars at some points in the planet’s history. NASA’s Spirit and Opportunity rovers, for example, have found strong evidence of them in rocks that date back billions of years.

Oze and his colleagues spent the last three years investigating the possible signatures organisms living in hydrothermal systems here on Earth might give off. Specifically, they zeroed in on the dynamics of hydrogen and methane production.

Experiments in the lab revealed the levels of these substances that could be expected where life is absent. The team then looked at data from hydrothermal systems in the field that were packed with organisms.

There was a clear difference, researchers said.

“From our calculations, low hydrogen-methane [ratios] could indicate that there might be life, if it’s similar to that on Earth,” Oze said.

The original 'Face on Mars' image taken by NASA's Viking 1 orbiter, in grey scale, on July, 25 1976. Image shows a remnant massif located in the Cydonia region.

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More Quizzes

If life thrives in Martian hydrothermal systems, scientists should be able to pick it up — even if it’s underground, the researchers said .

“Lifeforms on Mars may be under the surface of the planet, where no probe can currently go right now,” Oze said. “But methane and hydrogen formed in specific hydrothermal systems are eventually released at the surface, so all that needs to be done is for an analysis to be made at a vent to measure the gas that is released.”

Oze and his team published their results June 7 in the journal Proceedings of the National Academy of Sciences (PNAS).

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Article source: http://www.space.com/16284-mars-life-atmosphere-hydrogen-methane.html

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Mars, Facts and Information about the Planet Mars

Martian Surface Similar to Earth and Moon

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Mars rocks indicate relatively recent quakes, volcanism, on Red Planet

Images of a martian landscape offer evidence that the Red Planet’s surface not only can shake like the surface of Earth, but has done so relatively recently. If marsquakes do indeed take place, said the scientists who analyzed the high-resolution images, our nearest planetary neighbor may still have active volcanism, which could help create conditions for liquid water.

With High Resolution Imaging Science Experiment (HiRISE) imagery, the research team examined boulders along a fault system known as Cerberus Fossae, which cuts across a very young (few million years old) lava surface on Mars.

By analyzing boulders that toppled from a martian cliff, some of which left trails in the coarse-grained soils, and comparing the patterns of dislodged rocks to such patterns caused by quakes on Earth, the scientists determined the rocks fell because of seismic activity. The martian patterns were not consistent with how boulders would scatter if they were deposited as ice melted, another means by which rocks are dispersed on Mars.

Gerald Roberts, an earthquake geologist with Birkbeck, an institution of the University of London, who led the study, said that the images of Mars included boulders that ranged from two to 20 meters (6.5 to 65 feet) in diameter, which had fallen in avalanches from cliffs.

The size and number of boulders decreased over a radius of 100 kilometers (62 miles) centered at a point along the Cerberus Fossae faults.
“This is consistent with the hypothesis that boulders had been mobilized by ground-shaking, and that the severity of the ground-shaking decreased away from the epicenters of marsquakes,” Roberts said.

The study, by Roberts and his colleagues, will be published Thursday in the Journal of Geophysical Research-Planets, a publication of the American Geophysical Union (AGU).

The team compared the pattern of boulder falls, and faulting of the martian surface, with those seen after a 2009 earthquake near L’Aquila, in central Italy. In that event, boulder falls occurred up to approximately 50 km (31 miles) from the epicenter. Because the area of displaced boulders in the marsscape stretched across an area approximately 200 km124-miles) long, the quakes were likely to have had a magnitude greater than 7, the researchers estimated.

By looking at the tracks that the falling boulders had left on the dust-covered martian surface, the team determined that the marsquakes were relatively recent – and certainly within the last few percent of the planet’s history – because martian winds had not yet erased the boulder tracks.

Trails on Mars can quickly disappear – for instance, tracks left by NASA robotic rovers are erased within a few years by martian winds, whereas other, sheltered tracks stick around longer. It is possible, the scientists concluded, that large-magnitude quake activity is still occurring on Mars.

The existence of marsquakes could be significant in the ongoing search for life on Mars, the researchers stated. If the faults along the Cerberus Fossae region are active, and the quakes are driven by movements of magma related to the nearby volcano, Elysium Mons, the energy provided in the form of heat from the volcanic activity under the surface of Mars could be able to melt ice. The resulting liquid water, they noted, could provide habitats friendly to life.

“Possible evidence of palaeomarsquakes from fallen boulder populations, Cerberus Fossae, Mars” Gerald P. Roberts: Department of Earth and Planetary Sciences, Birkbeck, University of London, United Kingdom; Brian Matthews: Department of Physics and Astronomy, The Open University, Milton Keynes, United Kingdom; Christ Bristow: Department of Earth and Planetary Sciences, Birkbeck, University of London, United Kingdom and Hyder Consulting, London, United Kingdom; Luca Guerrieri: Geological Survey of Italy, ISPRA – High Institute for the Environmental Protection and Research, Rome, Italy; Joyce Vetterlein: Department of Earth and Planetary Sciences, Birkbeck, University of London, United Kingdom.

Article source: http://www.marsdaily.com/reports/Mars_rocks_indicate_relatively_recent_quakes_volcanism_on_Red_Planet_999.html

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Mars, the Red Planet, Fourth Planet from the Sun

Martian Surface Similar to Earth and Moon

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NASA Orbiter Catches Mars Sand Dunes in Motion

/PRNewswire-USNewswire/ — Images from NASA’s Mars Reconnaissance Orbiter (MRO) show sand dunes and ripples moving across the surface of Mars at dozens of locations and shifting up to several yards. These observations reveal the planet’s sandy surface is more dynamic than previously thought.

(Logo: http://photos.prnewswire.com/prnh/20081007/38461LOGO)

“Mars either has more gusts of wind than we knew about before, or the winds are capable of transporting more sand,” said Nathan Bridges, planetary scientist at the Johns Hopkins University’s Applied Physics Laboratory in Laurel, Md., and lead author of a paper on the finding published online in the journal Geology. “We used to think of the sand on Mars as relatively immobile, so these new observations are changing our whole perspective.”

While red dust is known to swirl all around Mars in storms and dust devils, the planet’s dark sand grains are larger and harder to move. Less than a decade ago, scientists thought the dunes and ripples on Mars either did not budge or moved too slowly for detection.

MRO was launched in 2005. Initial images from the spacecraft’s High Resolution Imaging Science Experiment (HiRISE) camera documented only a few cases of shifting sand dunes and ripples, collectively called bedforms. Now, after years of monitoring the martian surface, the spacecraft has documented movements of a few yards or meters per year in dozens of locations across the planet.

The air on Mars is thin, so stronger gusts of wind are needed to push a grain of sand. Wind-tunnel experiments have shown that a patch of sand would take winds of about 80 mph to move on Mars compared with only 10 mph on Earth. Measurements from the meteorology experiments on NASA’s Viking landers in the 1970s and early 1980s, in addition to climate models, showed such winds should be rare on Mars.

The first hints that Martian dunes move came from NASA’s Mars Global Surveyor, which operated from 1997 to 2006. But the spacecraft’s cameras lacked the resolution to definitively detect the changes. NASA’s Mars Exploration Rovers also detected hints of shifting sand when they touched down on the red planet’s surface in 2004. The mission team was surprised to see grains of sand dotting the rovers’ solar panels. They also witnessed the rovers’ track marks filling in with sand.

“Sand moves by hopping from place to place,” said Matthew Golombek, a co-author of the new paper and a member of the Mars Exploration Rover and MRO teams at NASA’s Jet Propulsion Laboratory in Pasadena, Calif. “Before the rovers landed on Mars, we had no clear evidence of sand moving.”

Not all of the sand on Mars is blowing in the wind. The study also identifies several areas where the bedforms did not move.

“The sand dunes where we didn’t see movement today could have larger grains, or perhaps their surface layers are cemented together,” said Bridges, who also is a member of the HiRISE team. “These studies show the benefit of long-term monitoring at high resolution.”

According to scientists, the seemingly stationary areas might move on much larger time scales, triggered by climate cycles on Mars that last tens of thousands of years. The tilt of Mars’ axis relative to its orbital plane can vary dramatically. This, combined with the oval shape of Mars’ orbit, can cause extreme changes in the Martian climate, much greater than those experienced on Earth. Mars may once have been warm enough that the carbon dioxide now frozen in the polar ice caps could have been free to form a thicker atmosphere, leading to stronger winds capable of transporting sand.

HiRISE is operated by the University of Arizona in Tucson. The instrument was built by Ball Aerospace Technologies Corp. of Boulder, Colo. The Mars Exploration Rovers Opportunity and Spirit were built by JPL. JPL also manages the MRO and Mars Exploration Rover projects for NASA’s Science Mission Directorate in Washington. Lockheed Martin Space Systems of Denver is NASA’s industry partner for the MRO Project and built the spacecraft.

MRO images and additional information is available online at:

http://www.nasa.gov/mission_pages/MRO

For more information about NASA Mars missions, visit the Web at:

www.nasa.gov/mars

SOURCE NASA

Article source: http://www.sacbee.com/2011/11/17/4062930/nasa-orbiter-catches-mars-sand.html

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Mars Rover Curiosity: NASA Prepares For Launch Of Mars Science Laboratory …

The day after Thanksgiving, the Mars Science Laboratory (MSL), NASA’s car-sized, nuclear-powered rover called Curiosity, will blast off for a nine-month journey to the Red Planet.

When it lands next August, after traveling 354 million-miles, the MSL will spend nearly two years analyzing rock samples and exploring the Martian surface for signs that microbial life may have once existed.

“This is a Mars scientist’s dream machine,” Ashwin Vasavada, MSL deputy project scientist at NASA’s Jet Propulsion Laboratory said, according to AFP. “This is the most capable scientific explorer we have ever sent out…We are super excited.”

According to NASA, Curiosity is about twice as long and five times as heavy as the Opportunity and Spirit, the twin Mars rovers that NASA launched in 2003. But unlike the Opportunity and Spirit, the Curiosity is equipped with tools to gather and analyze samples from the Martian surface and ground.

The six-wheeled craft will be able to maneuver over obstacles that are more than two-feet high and travel about 600 feet per day. The Spirit and Opportunity were solar-powered, but Curiosity runs on a plutonium-powered battery.

“It requires a fancy power supply in order to do the job,” Dr. Pam Conrad, deputy principal investigator for Mars Science Laboratory said in a statement. “This enables us to make measurements all day, every day, at night, in the winter.”

The Mars Science Laboratory, which Reuters reports cost $2.5 billion, is currently in a payload fairing atop an Atlas V rocket. Although the launch is scheduled for November 25 at 10:21 a.m. EST, weather or other factors could delay it, so the launch window extends to December 18.

From USA Today::

It will land in unprecedented fashion, first using a braking heat shield, then high-speed parachute and finally a rocket-powered “sky crane” to safely deposit the rover on the martian surface. “It is clearly not risk-free,” says Peter Theisinger, mission chief of NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, Calif.

A NASA video, available above, shows a simulation of the rover landing and working on Mars.

The rover will land near the base of a 3-mile high mountain inside the Gale crater.

“Gale gives us a superb opportunity to test multiple potentially habitable environments and the context to understand a very long record of early environmental evolution of the planet,” John Grotzinger, project scientist for the Mars Science Laboratory said in a statement. “The portion of the crater where Curiosity will land has an alluvial fan likely formed by water-carried sediments. Layers at the base of the mountain contain clays and sulfates, both known to form in water.”

NASA has since lost contact with the Spirit, but the Opportunity is continuing to study while spending the winter on the rim of Endeavour Crater.

LOOK: Pictures of the Mars Science Laboratory, also known as the Curiosity Rover:


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Article source: http://www.huffingtonpost.com/2011/11/16/mars-rover-curiosity-nasa_n_1097949.html

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