Archive for high resolution imaging science experiment – Page 2

Orbiter View of Curiosity From Nearly Straight Overhead

Details such as the shadow of the mast on NASA’s Mars rover Curiosity appear in an image taken Aug. 17, 2012, by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter, from more directly overhead than previous HiRISE images of Curiosity.

In this product, cutouts showing the rover and other hardware or ground markings from the landing of the Mars Science Laboratory spacecraft are presented across the top of a larger, quarter-resolution overview keyed to the full-resolution cutouts. North is up. The scale bar is 200 meters (one-eighth of a mile).

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Ultra-Sharp Color Photo Reveals Mars Rover From Space




NASA's Mars Reconnaissance Orbiter snapped this color photo of the Curiosity rover from space.

This color-enhanced view of NASA’s Curiosity rover on the surface of Mars was taken by the High Resolution Imaging Science Experiment (HiRISE) on NASA’s Mars Reconnaissance Orbiter as the satellite flew overhead. Colors have been enhanced to show the subtle color variations near the rover, which result from different types of materials.
CREDIT: NASNASA/JPL-Caltech/University of Arizona


A NASA spacecraft in orbit around Mars snapped a new, incredibly crisp color photo of the Curiosity rover on the surface of the Red Planet.

The photo was taken by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter, which has been circling the Red Planet since 2006. The new image shows Curiosity at its Gale Crater landing site, with the effects of its rocket-powered descent to the surface clearly visible.

“The rover appears as double bright spot plus shadows from this perspective, looking at its shadowed side, set in the middle of the blast pattern from the descent stage,” Alfred McEwen, HiRISE principal investigator at the University of Arizona in Tucson, said in a statement. “This image was acquired from an angle looking 30 degrees westward of straight down. We plan to get one in a few days looking more directly down, showing the rover in more detail and completing a stereo pair.”



The photo also reveals spectacular details of the layered bedrock at Gale Crater, NASA officials said. As part of its mission, Curiosity will examine the crater’s layers of rock and soil to determine whether Mars has an environment that is, or ever was, suitable for microbial life.

Engineers at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, Calif. recently upgraded Curiosity’s computers and software to prepare the rover for driving and using the tools on its robotic arm. Mission operators affectionately called this four-day procedure a “brain transplant,” since it involved transitioning Curiosity from landing to now operating on the Martian surface. [Gallery: Curiosity's 1st Photos of Mars]

“We have successfully completed the brain transplant,” Mike Watkins, Curiosity’s mission manager at JPL, said in a statement. “Now we are moving on to a new phase of functional checkouts of the science instruments and preparations for a short test drive.”

Curiosity is expected to take its first drive within roughly a week. The rover’s first outing will likely include short motions forward and in reverse, and a turn, NASA officials said. Mission controllers will prepare and test each of the wheels’ drive and steering motors before Curiosity is moved for the first time.

“It’s fair to say that the scientists, not to mention the rover drivers, are itching to move,” said Ashwin Vasavada, deputy project scientist for the Curiosity mission at JPL.

Curiosity, which is also known as the Mars Science Laboratory, touched down on Mars on the night of Aug. 5 (PDT; Aug. 6 EDT). NASA’s Mars Reconnaissance Orbiter captured photos of the rover on its parachute as it descended to the Martian surface, and also observed the robotic explorer at Gale Crater one day after landing.

NASA's Curiosity rover and its parachute were spotted by NASA's Mars Reconnaissance Orbiter as Curiosity descended to the surface on Aug. 5 PDT (Aug. 6 EDT).

Scientists have been combing through photos taken by HiRISE and Curiosity’s own cameras to narrow down potential areas for the rover to drive to and investigate in the future. Ultimately, Curiosity will explore a mysterious mountain, called Mount Sharp, which rises up three miles (4.8 kilometers) from roughly the center of Gale Crater.

“The science and operations teams are evaluating several potential routes that would take us to Mount Sharp, with perhaps a few waypoints to inspect some of the different terrains we’ve identified as we map the landing area,” Vasavada said. “As we have reported many times before, it’s going to take us a good part of our first year to make it to the layered sediments on Mount Sharp.”

The $2.5 billion Curiosity rover will spend two years on the Red Planet investigating the Martian terrain. The 1-ton rover is NASA’s most ambitious planetary science mission attempted to date.

Visit SPACE.com for complete coverage of NASA’s Mars rover Curiosity. Follow SPACE.com on Twitter @Spacedotcom. We’re also on Facebook and Google+.

Article source: http://www.space.com/17117-mars-rover-curiosity-color-photo-from-space.html

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Scientists Find Clues of Plate Tectonics on Mars

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Caption: Valles Marineris NASA World Wind Map Mars Credit: NASA

Until now, Earth was thought to be the only planet with plate tectonics. But a huge “crack” in Mars’ surface — the massive Valles Marinaris — shows evidence of the movement of huge crustal plates beneath the planet’s surface, meaning Mars may be showing the early stages of plate tectonics. This discovery can perhaps also shed light on how the plate tectonics process began here on Earth.

Valles Marineris is no ordinary crack on the Martian surface. It is the longest and deepest system of canyons in the Solar System. Stretching nearly 2,500 miles, it is nine times longer than Earth’s Grand Canyon.

An Yin, a planetary geologist and UCLA professor of Earth and space sciences, analyzed satellite images from THEMIS (Thermal Emission Imaging System), on board the Mars Odyssey spacecraft, and from the HIRISE (High Resolution Imaging Science Experiment) camera on NASA’s Mars Reconnaissance Orbiter.

“When I studied the satellite images from Mars, many of the features looked very much like fault systems I have seen in the Himalayas and Tibet, and in California as well, including the geomorphology,” he said.

The two plates that Yin calls Valles Marineris North and Valles Marineris South are moving approximately 93 miles horizontally relative to each other. By comparison, California’s San Andreas Fault, which is similarly over the intersection of two plates, has moved about twice as much, because Earth is about twice the size of Mars.

Yin believes Mars has no more than two plates whereas Earth has seven major plates and dozens of smaller ones. As Yin puts it “Earth has a very broken ‘egg shell,’ so its surface has many plates; Mars’ is slightly broken and may be on the way to becoming very broken, except its pace is very slow due to its small size and, thus, less thermal energy to drive it. This may be the reason Mars has fewer plates than on Earth.”

Mars also has several long, straight chains of volcanoes, including three that make up the Tharsis Montes, three large shield volcanoes which includes Olympus Mons, the tallest mountain in the Solar System at 22 km high. These volcanic chains may have formed from the motion of a plate sitting over a “hot spot” in the Martian mantle, in the same way the Hawaiian Islands are thought to have formed here on Earth. Yin also identified a steep cliff similar to cliffs in California’s Death Valley, which are generated by a fault, as well as a very smooth and flat side of a canyon wall which Yin says is also strong evidence of tectonic activity.

Yin also suggests that the fault is shifting occasionally, and may even produce “Marsquakes” every now and again. “I think the fault is probably still active, but not every day. It wakes up every once in a while, over a very long duration — perhaps every million years or more,” he said.

It is not known how far beneath the surface the plates on Mars are located. Yin admits “I don’t quite understand why the plates are moving with such a large magnitude or what the rate of movement is; maybe Mars has a different form of plate tectonics,” Yin said. “The rate is much slower than on Earth.”

“Mars is at a primitive stage of plate tectonics,” Yin added. “It gives us a glimpse of how the early Earth may have looked and may help us understand how plate tectonics began on Earth.”

Yin’s study was published in the August issue of the journal Lithosphere and he also plans to publish a follow-up paper hoping to shed more light on plate tectonics on both Mars and Earth.

Read the abstract.

Find out more at the

Article source: http://www.universetoday.com/96856/scientists-find-clues-of-plate-tectonics-on-mars/

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Mars Reconnaissance Orbiter will spy for you, HiRise camera taking requests

Mars Reconnaissance Orbiter

NASA

This artist’s animation of the NASA Mars Reconnaissance Orbiter.

Smile for the Mars Reconnaissance Orbiter! HiRISE, a camera aboard the MRO orbiting spacecraft, is taking requests with an online wishlist of what earthlings want to see on Mars.

NASA’s Curiosity is getting up close and personal with the surface of the red planet, but the eye in the sky that helped get it there could be looking beyond the Gale Crater, if you ask it nicely, and in the right way.

The HiWish program, which began in January 2010, announced “the people’s camera” would be open to public suggestion, and started delivering images of civilian-selected locales within a few months.

“Explore Mars, one giant image at a time,” is the HiRISE (High-Resolution Imaging Science Experiment) motto, and project researchers continue to look to the home planet for input about where to point the camera.

Earth-tethered explorers can help HiRISE decide what should be photographed next by searching existing images, browsing known targets, and suggesting new ones. 

Operated out of the Lunar Planetary Laboratory at the University of Arizona, HiRISE has “huge capability to do detailed imaging,” JPL’s Guy Webster told KPCC, noting that the camera could capture on the surface of Mars something “the size of a washing machine.” 

Amid the current commotion, Webster said he hoped people would be reminded about what an “amazing instrument” HiRISE is, and take advantage of the public possibilities, even with Curiosity phoning home photos from the surface.

KPCC asked Webster if combining perspectives with Curiosity’s data would paint a more complete picture of the rover’s landscape. As one would hope, he was way ahead of us. 

Webster told KPCC that there isn’t an inch for miles around Curiosity’s landing area that hasn’t already been photographed by the HiRISE camera, calling its image database of the area, “comprehensive.”

What morsel of Mars do you want to see?

Article source: http://www.scpr.org/blogs/news/2012/08/16/9436/smile-reconnaissance-orbiter-hirise-taking-mars-ph/

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Image of the Day: Mars’ Valles Marineris –Evidence of Plate Tectonics, A Key …

Yin made the discovery during his analysis of satellite images from a NASA spacecraft known as THEMIS (Time History of Events and Macroscale Interactions during Substorms) and from the HIRISE (High Resolution Imaging Science Experiment) camera on NASA’s Mars Reconnaissance Orbiter. He analyzed about 100 satellite images — approximately a dozen were revealing of plate tectonics.

Yin has conducted geologic research in the Himalayas and Tibet, where two of the Earth’s seven major plates divide.* “When I studied the satellite images from Mars, many of the features looked very much like fault systems I have seen in the Himalayas and Tibet, and in California as well, including the geomorphology,” said Yin, a planetary geologist.

For example, he saw a very smooth, flat side of a canyon wall, which can be generated only by a fault, and a steep cliff, comparable to cliffs in California’s Death Valley, which also are generated by a fault. Mars has a linear volcanic zone, which Yin said is a typical product of plate tectonics.

“You don’t see these features anywhere else on other planets in our solar system, other than Earth and Mars,” said Yin, whose research is featured as the cover story in the August issue of the journal Lithosphere.

The surface of Mars contains the longest and deepest system of canyons in our solar system, known as Valles Marineris (image at top and bottom of the page–Latin for Mariner Valleys and named for the Mariner 9 Mars orbiter of 1971, which discovered it). It is nearly 2,500 miles long — about nine times longer than the Earth’s Grand Canyon. Scientists have wondered for four decades how it formed. Was it a big crack in Mars’ shell that opened up?

“In the beginning, I did not expect plate tectonics, but the more I studied it, the more I realized Mars is so different from what other scientists anticipated,” Yin said. “I saw that the idea that it is just a big crack that opened up is incorrect. It is really a plate boundary, with horizontal motion. That is kind of shocking, but the evidence is quite clear.* “The shell is broken and is moving horizontally over a long distance. It is very similar to the Earth’s Dead Sea fault system, which has also opened up and is moving horizontally.”

The two plates divided by Mars’ Valles Marineris have moved approximately 93 miles horizontally relative to each other, Yin said. California’s San Andreas Fault, which is over the intersection of two plates, has moved about twice as much — but the Earth is about twice the size of Mars, so Yin said they are comparable.

Yin, whose research is partly funded by the National Science Foundation, calls the two plates on Mars the Valles Marineris North and the Valles Marineris South.

“Earth has a very broken ‘egg shell,’ so its surface has many plates; Mars’ is slightly broken and may be on the way to becoming very broken, except its pace is very slow due to its small size and, thus, less thermal energy to drive it,” Yin said. “This may be the reason Mars has fewer plates than on Earth.”

Mars has landslides, and Yin said a fault is shifting the landslides, moving them from their source.

“I think so,” he said. “I think the fault is probably still active, but not every day. It wakes up every once in a while, over a very long duration — perhaps every million years or more.”

Yin is very confident in his findings, but mysteries remain, he said, including how far beneath the surface the plates are located.* “I don’t quite understand why the plates are moving with such a large magnitude or what the rate of movement is; maybe Mars has a different form of plate tectonics,” Yin said.

The rate is much slower than on Earth.”* The Earth has a broken shell with seven major plates; pieces of the shell move, and one plate may move over another. Yin is doubtful that Mars has more than two plates.

“We have been able to identify only the two plates,” he said. “For the other areas on Mars, I think the chances are very, very small. I don’t see any other major crack.”

Did the movement of Valles Marineris North and Valles Marineris South create the enormous canyons on Mars? What led to the creation of plate tectonics on Earth?*

Yin, who will continue to study plate tectonics on Mars, will answer those questions in a follow-up paper that he also plans to publish in the journal Lithosphere.

            Mars-plate-tectonics

Image credit top of page: With thanks to space artist, Walter Myers

Image Credit bottom of page: from Google Mars created by MOLA Science Team) View full size image

Article source: http://www.dailygalaxy.com/my_weblog/2012/08/image-of-the-day-mars-.html

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Scientist discovers plate tectonics on Mars

For years, many scientists had thought that plate tectonics existed nowhere in our solar system but on Earth. Now, a University of California, Los Angeles (UCLA), scientist has discovered that the geological phenomenon, which involves the movement of huge crustal plates beneath a planet’s surface, also exists on Mars.

“Mars is at a primitive stage of plate tectonics. It gives us a glimpse of how the early Earth may have looked and may help us understand how plate tectonics began on Earth,” said researcher An Yin.

Yin made the discovery during his analysis of satellite images from a NASA spacecraft known as THEMIS (Time History of Events and Macroscale Interactions during Substorms) and from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter (MRO). He analyzed about 100 satellite images, and approximately a dozen were revealing of plate tectonics.

Yin has conducted geologic research in the Himalayas and Tibet, where two of Earth’s seven major plates divide.

“When I studied the satellite images from Mars, many of the features looked very much like fault systems I have seen in the Himalayas and Tibet, and in California as well, including the geomorphology,” said Yin.

For example, he saw a smooth, flat side of a canyon wall, which can be generated only by a fault, and a steep cliff, comparable to cliffs in California’s Death Valley, which also are generated by a fault. Mars has a linear volcanic zone, which Yin said is a typical product of plate tectonics.

“You don’t see these features anywhere else on other planets in our solar system, other than Earth and Mars,” said Yin.

The surface of Mars contains the longest and deepest system of canyons in our solar system, known as Valles Marineris. It is nearly 2,500 miles (4,000 kilometers) long — about nine times longer than Earth’s Grand Canyon. Scientists have wondered for four decades how it formed. Was it a big crack in Mars’ shell that opened up?

“In the beginning, I did not expect plate tectonics, but the more I studied it, the more I realized Mars is so different from what other scientists anticipated,” Yin said. “I saw that the idea that it is just a big crack that opened up is incorrect. It is really a plate boundary with horizontal motion. That is kind of shocking, but the evidence is quite clear. The shell is broken and is moving horizontally over a long distance. It is very similar to the Earth’s Dead Sea fault system, which has also opened up and is moving horizontally.”

The two plates divided by Mars’ Valles Marineris have moved approximately 93 miles (150km) horizontally relative to each other, said Yin. California’s San Andreas Fault, which is over the intersection of two plates, has moved about twice as much — but Earth is about twice the size of Mars, so Yin said they are comparable. Yin calls the two plates on Mars the Valles Marineris North and the Valles Marineris South.

“Earth has a very broken ‘egg shell,’ so its surface has many plates; Mars’ is slightly broken and may be on the way to becoming very broken, except its pace is very slow due to its small size and, thus, less thermal energy to drive it,” Yin said. “This may be the reason Mars has fewer plates than on Earth.”

Mars has landslides, and Yin said a fault is shifting the landslides, moving them from their source.

Does Yin think there are Marsquakes?

“I think so,” he said. “I think the fault is probably still active, but not every day. It wakes up every once in a while over a very long duration — perhaps every million years or more.” Yin is very confident in his findings, but mysteries remain, he said, including how far beneath the surface the plates are located.

“I don’t quite understand why the plates are moving with such a large magnitude or what the rate of movement is — maybe Mars has a different form of plate tectonics,” Yin said. “The rate is much slower than on Earth.”

The Earth has a broken shell with seven major plates; pieces of the shell move, and one plate may move over another. Yin is doubtful that Mars has more than two plates. “We have been able to identify only the two plates,” he said. “For the other areas on Mars, I think the chances are very, very small. I don’t see any other major crack.”

Did the movement of Valles Marineris North and Valles Marineris South create the enormous canyons on Mars? What led to the creation of plate tectonics on Earth?

Yin, who will continue to study plate tectonics on Mars, will answer those questions in a follow-up paper.

Article source: http://www.astronomy.com/~/link.aspx?_id=d66f48a7-7783-4a31-a9d7-e20312eccca4

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Orbiter images NASA’s martian landscape additions

Late Monday night, an image from the High Resolution Imaging Science Experiment (HiRISE) camera aboard NASA’s Mars Reconnaissance Orbiter (MRO) captured the Curiosity rover and the components that helped it survive its seven-minute ordeal from space to its present location in Mars’ Gale Crater.

“This latest image is another demonstration of the invaluable assistance the MRO team, and its sister team with the Mars Odyssey orbiter, have provided the Curiosity rover during our early days on the Red Planet,” said Mike Watkins from NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California. “The image not only satisfies our curiosity, but also can provide important information on how these vital components performed during entry, descent, and landing, and exactly locate the rover’s touchdown site within Gale Crater.”

The Curiosity rover is in the center of the image. To the right, approximately 4,900 feet (1,500 meters) away, lies the heat shield, which protected the rover from the 3800° Fahrenheit (2100° Celsius) temperatures it encountered during its fiery descent. On the lower left, about 2,020 feet (615m) away, are the parachute and back shell. The parachute has a constructed diameter of 71 feet (21.5m) and an inflated diameter of 51 feet (16m). The back shell remains connected to the chute via 80 suspension lines that are 165 feet (50m) long. To the upper left, approximately 2,100 feet (650m) away from the rover, is a discoloration of the Mars surface consistent with what would have resulted when the rocket-powered Sky Crane impacted the surface.

“This is the first of what I imagine will be many portraits HiRISE will be taking of Curiosity on the surface of Mars,” said Sarah Milkovich from JPL. “The image was taken Monday at about 10:30 p.m. Pacific when MRO was at an altitude of about 186 miles (300 kilometers), and we are getting resolution on the surface down to 1.3 feet (39 centimeters) per pixel.”

As more of Curiosity’s instruments are coming online, more “first images” are being downlinked from the rover’s 17 cameras. The latest to come in is from the Mars Hand Lens Imager (MAHLI). The focusable color camera is located on the tool-bearing turret at the end of Curiosity’s robotic arm. Researchers will use it for magnified, close-up views of rocks and soils and also for wider scenes of the ground, the landscape, or even the rover.

“It is great to have our first MAHLI image under our belt,” said Ken Edgett from Malin Space Science Systems in San Diego. “We tested the focus mechanism and imager, and the whole system is looking good. We are looking forward to getting up close and personal with Mars.”

The team plans for Curiosity checkout Tuesday included raising the rover’s mast and continued testing of the high-gain antenna.

Curiosity carries 10 science instruments with a total mass 15 times as large as the science payloads on the Mars rovers Spirit and Opportunity. Some of the tools, such as a laser-firing instrument for checking rocks’ elemental composition from a distance, are the first of their kind on Mars. Curiosity will use a drill and scoop, which is located at the end of its robotic arm, to gather soil and powdered samples of rock interiors, then sieve and parcel out these samples into the rover’s analytical laboratory instruments.

To handle this science toolkit, Curiosity is twice as long and five times as heavy as Spirit or Opportunity. The Gale Crater landing site places the rover within driving distance of layers of the crater’s interior mountain. Observations from orbit have identified clay and sulfate minerals in the lower layers, indicating a wet history.

Article source: http://www.astronomy.com/~/link.aspx?_id=609e264b-e834-47c3-8ead-5198c3c7e214

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Mars orbiter captures mysterious hollows in the ice on surface of planet – are …

  • Holes in planet are ‘wrong shape’ for normal meteorite
  • Layer of pure ice seems to have been exposed
  • Has ice ‘boiled off’ into space to cause weird shapes?

By
Rob Waugh

04:33 EST, 25 May 2012

|

04:53 EST, 25 May 2012

The surface of Mars is dotted with craters – but when the HiRise camera aboard the Mars Reconnaissance Orbiter captured ‘holes’ in the ice of the planet, scientists were puzzled.

The ‘holes’ aren’t the circular shape of a ‘normal’ meteorite impact – they have two levels, a small inner crater, surrounded by a shallow depression extending outward from the inner crater. 

The craters seem to have exposed a layer of shallow ice that was mapped by the Mars Odyssey spacecraft.

The pictures were captured by the High Resolution Imaging Science Experiment - HiRISE - camera on board the Mars Reconnaissance orbiter.

The pictures were captured by the High Resolution Imaging Science Experiment – HiRISE – camera on board the Mars Reconnaissance orbiter.

This image is located at 50 degrees north latitude, where shallow ice has been mapped by the Mars Odyssey spacecraft. 

The scientists now think that the layer of ice might have ‘boiled off’ into space after being exposed by meteoriste impacts.

MRO has detected newly-formed impact craters in this broad region that exposed shallow ice, and also revealed that it is nearly pure ice.

One interpretation of the expanded craters visible here is that a group of small impacts, probably secondary craters from a much larger primary crater, exposed the clean, shallow ice in this region.

Once exposed, the ice is unstable and sublimates (passes directly from ice to gas), and the shallow depressions could gradually expand.

The pictures were captured by the High Resolution Imaging Science Experiment – HiRISE – camera on board the Mars Reconnaissance orbiter.

They are just one of several new features uncovered by the orbiter in recent weeks.

The 'snails' are liable to be rather crunchy, however - they are actually lava flows in the planet's Elysium region in spiral patterns that resemble snail or nautilus shells.

The ‘snails’ are liable to be rather crunchy, however – they are actually lava flows in the planet’s Elysium region in spiral patterns that resemble snail or nautilus shells.

The new result came from ongoing research into whether there was once water in the Elysium volcanic province of Mars.

‘I was interested in Martian outflow channels and was particularly intrigued by Athabasca Valles and Cerberus Palus, both part of Elysium,’ says Arizona State University graduate student Andrew Ryan.

‘Athabasca Valles has a very interesting history,’ Ryan says.

‘There’s an extensive literature on the area, as well as an intriguing combination of seemingly fluvial and volcanic features.’

Among the features are large slabs or plates that resemble broken floes of pack ice in the Arctic Ocean on Earth.

In the past, a few scientists have argued that the plates in Elysium are in fact underlain by water ice.

‘One evening,’ Ryan says, ‘I was making a second pass over the HiRISE images when I first noticed puzzling spiral patterns in an image near the southern margin of Cerberus Palus. I actually nearly overlooked that particular frame, thinking that it might not be too useful, being so far away from main study area farther north.’

He notes, ‘The coils become noticeable in the full-resolution HiRISE image only when you really zoom in. They also tend to blend in with the rest of the light-gray terrain — that is, until you stretch the contrast a bit.

The new result came from ongoing research into whether there was once water in the Elysium volcanic province of Mars

Snails from space! The new result came from ongoing research into whether there was once water in the Elysium volcanic province of Mars

‘I don’t find it surprising that these were overlooked in the past. I nearly missed them too.’

On Earth, lava coils can be found on the Big Island of Hawaii, mainly on the surface of ropey pahoehoe lava flows. They have also been seen in submarine lava flows near the Galapagos Rift on the Pacific Ocean floor.

As Ryan explains, ‘The coils form on flows where there’s a shear stress — where flows move past each other at different speeds or in different directions. Pieces of rubbery and plastic lava crust can either be peeled away and physically coiled up — or wrinkles in the lava’s thin crust can be twisted around.’

Similarly, he notes that scientists have documented the formation of rotated pieces of oceanic crust at mid-ocean ridge spreading centers. ‘Since the surface of active lava lakes, such as those on Hawaii, can have crustal activity like spreading centers do, it’s conceivable that lava coils may form there in a similar way, but at a smaller scale.’

The size of Martian lava coils came as a surprise.

‘On Mars the largest lava coil is 100 feet across. That’s bigger than any known lava coils on Earth,’ he says. Ryan and Christensen’s work has inventoried nearly 200 lava coils in the Cerberus Palus region alone.

Looking ahead, Ryan says, ‘Lava coils may be present in other Martian volcanic provinces or in outflow channels mantled by volcanic features. I expect that we’ll find quite a few more in Elysium as the HiRISE image coverage grows over time.’
 image coverage grows over time.’

Article source: http://www.dailymail.co.uk/sciencetech/article-2149791/Mars-orbiter-captures-mysterious-hollows-ice-surface-planet--wrong-shape-meteorite-impacts.html

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Mars orbiter captures mysterious hollows in the ice on surface of planet – but …

  • Holes in planet are ‘wrong shape’ for normal meteorite
  • Layer of pure ice seems to have been exposed
  • Has ice ‘boiled off’ into space to cause weird shapes?

By
Rob Waugh

04:33 EST, 25 May 2012

|

04:53 EST, 25 May 2012

The surface of Mars is dotted with craters – but when the HiRise camera aboard the Mars Reconnaissance Orbiter captured ‘holes’ in the ice of the planet, scientists were puzzled.

The ‘holes’ aren’t the circular shape of a ‘normal’ meteorite impact – they have two levels, a small inner crater, surrounded by a shallow depression extending outward from the inner crater. 

The craters seem to have exposed a layer of shallow ice that was mapped by the Mars Odyssey spacecraft.

The pictures were captured by the High Resolution Imaging Science Experiment - HiRISE - camera on board the Mars Reconnaissance orbiter.

The pictures were captured by the High Resolution Imaging Science Experiment – HiRISE – camera on board the Mars Reconnaissance orbiter.

This image is located at 50 degrees north latitude, where shallow ice has been mapped by the Mars Odyssey spacecraft. 

The scientists now think that the layer of ice might have ‘boiled off’ into space after being exposed by meteoriste impacts.

MRO has detected newly-formed impact craters in this broad region that exposed shallow ice, and also revealed that it is nearly pure ice.

One interpretation of the expanded craters visible here is that a group of small impacts, probably secondary craters from a much larger primary crater, exposed the clean, shallow ice in this region.

Once exposed, the ice is unstable and sublimates (passes directly from ice to gas), and the shallow depressions could gradually expand.

The pictures were captured by the High Resolution Imaging Science Experiment – HiRISE – camera on board the Mars Reconnaissance orbiter.

They are just one of several new features uncovered by the orbiter in recent weeks.

The 'snails' are liable to be rather crunchy, however - they are actually lava flows in the planet's Elysium region in spiral patterns that resemble snail or nautilus shells.

The ‘snails’ are liable to be rather crunchy, however – they are actually lava flows in the planet’s Elysium region in spiral patterns that resemble snail or nautilus shells.

The new result came from ongoing research into whether there was once water in the Elysium volcanic province of Mars.

‘I was interested in Martian outflow channels and was particularly intrigued by Athabasca Valles and Cerberus Palus, both part of Elysium,’ says Arizona State University graduate student Andrew Ryan.

‘Athabasca Valles has a very interesting history,’ Ryan says.

‘There’s an extensive literature on the area, as well as an intriguing combination of seemingly fluvial and volcanic features.’

Among the features are large slabs or plates that resemble broken floes of pack ice in the Arctic Ocean on Earth.

In the past, a few scientists have argued that the plates in Elysium are in fact underlain by water ice.

‘One evening,’ Ryan says, ‘I was making a second pass over the HiRISE images when I first noticed puzzling spiral patterns in an image near the southern margin of Cerberus Palus. I actually nearly overlooked that particular frame, thinking that it might not be too useful, being so far away from main study area farther north.’

He notes, ‘The coils become noticeable in the full-resolution HiRISE image only when you really zoom in. They also tend to blend in with the rest of the light-gray terrain — that is, until you stretch the contrast a bit.

The new result came from ongoing research into whether there was once water in the Elysium volcanic province of Mars

Snails from space! The new result came from ongoing research into whether there was once water in the Elysium volcanic province of Mars

‘I don’t find it surprising that these were overlooked in the past. I nearly missed them too.’

On Earth, lava coils can be found on the Big Island of Hawaii, mainly on the surface of ropey pahoehoe lava flows. They have also been seen in submarine lava flows near the Galapagos Rift on the Pacific Ocean floor.

As Ryan explains, ‘The coils form on flows where there’s a shear stress — where flows move past each other at different speeds or in different directions. Pieces of rubbery and plastic lava crust can either be peeled away and physically coiled up — or wrinkles in the lava’s thin crust can be twisted around.’

Similarly, he notes that scientists have documented the formation of rotated pieces of oceanic crust at mid-ocean ridge spreading centers. ‘Since the surface of active lava lakes, such as those on Hawaii, can have crustal activity like spreading centers do, it’s conceivable that lava coils may form there in a similar way, but at a smaller scale.’

The size of Martian lava coils came as a surprise.

‘On Mars the largest lava coil is 100 feet across. That’s bigger than any known lava coils on Earth,’ he says. Ryan and Christensen’s work has inventoried nearly 200 lava coils in the Cerberus Palus region alone.

Looking ahead, Ryan says, ‘Lava coils may be present in other Martian volcanic provinces or in outflow channels mantled by volcanic features. I expect that we’ll find quite a few more in Elysium as the HiRISE image coverage grows over time.’
 image coverage grows over time.’

Article source: http://www.dailymail.co.uk/sciencetech/article-2149791/Mars-orbiter-captures-mysterious-hollows-ice-surface-planet--wrong-shape-meteorite-impacts.html?ito=feeds-newsxml

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Geological Life on Mars

Sand dunes in Nili Patera. (NASA / HiRISE)

When Percival Lowell first looked at Mars through his telescope in the 1890s, he saw some remarkable patterns: connecting lines crisscrossing the surface, linking distant ends of the planet in a seemingly non-natural way.  Lowell subscribed to Italian astronomer Giovanni Schiaparelli’s interpretation that the lines were canals deliberately constructed by intelligent beings to transport water.  And he felt the need to spread the word, writing an increasingly bold trilogy as his convictions deepened: Mars, Mars and Its Canals, and Mars As the Abode of Life.

Several decades later, the Mariner 4 spacecraft flew past the Red Planet, snapping pictures like a speeding paparazzo.  The results were disappointing: the grainy photographs showed craters frozen in time, evidence of a brutal bombardment in the planet’s past.  And there certainly weren’t any well-constructed canals.

These two examples represent the stark extremes of our perception of Mars, from a world of actively changing surfaces to one of a static, frozen wasteland.  Subsequent missions have pointed to a reality that is somewhere in between, but recent findings from NASA’s Mars Reconnaissance Orbiter mission offer unprecedented resolution on dynamic sand dune activity.

Software engineers and image analysts based at the California Institute of Technology, or Caltech, examined pictures from the High Resolution Imaging Science Experiment (HiRISE) camera.  This camera is a 30 cm-per-pixel powerhouse that, ironically, is better than publically available images of our own planet.  (According to Caltech, images of Earth-based targets taken at a similar resolution are classified information.)

The team looked at HiRISE images taken 105 days apart within the 300 square kilometer Nili Patera dune field and used an advanced processing program to detect subtle changes in dune shape and coverage.  To their surprise, they saw movement – up to 4.5 meters – and not just in isolated cases.  In fact, according to software engineer Francois Ayoub, who contributed to the study, “in the footprint covered by our analysis, all of the dunes imaged are active.  No dune seems static.”

Evidence of morphological changes in the very recent past has been seen before, but the rate and apparent pervasiveness of the dune movement were surprising.  As study leader Jean-Philippe Avouac puts it, “wind activity is indeed a major agent of evolution of the landscape on Mars.  This is important because it tells us something about the current state of Mars and how the planet is working today, geologically.”

Wind is certainly the most prominent cause of erosion on modern Mars, and the breeze would feel pretty intense to any future Mars-walking astronauts.  “Wind speeds on Mars are in the range of speeds found on Earth,” says Ayoub.  Based on the HiRISE imagery, “local wind gusts could reach the speed of what would be considered as a hurricane-force on Earth.”

Needless to say, questions remain.  Do the dunes creep along the surface slowly and incrementally over several-month periods, or do the shifts represent sudden changes from single wind storms?  And just how common are shifting sands?

Fortunately, the Caltech team is already on the case.  The software validation shown in this study proves that even more frequent imaging over a larger portion of the planet could provide answers.  “A more frequent temporal series of images would be needed,” says Ayoub.  “This is something we are working on now as more images are currently acquired.”

The days of planet-paving volcanic eruptions and catastrophic floods may be long past, but Mars remains geologically active as winds continue to re-work the planet’s surface.  As the search for signs of life on Mars continues, fast-moving sand dunes suggest that geologically at least, the Red Planet is very much alive.

Article source: http://www.wired.com/wiredscience/2012/05/geological-life-on-mars/

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