Looking for (Former) Lakeshore Property? HiRISE Finds It on Mars

This is reconstructed landscape showing the Shalbatana lake on Mars as it may have looked roughly 3.4 billion years ago. Data used in reconstruction are from NASA and the European Space Agency. Credit: Image credit: G. Di Achille, University of Colorado

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If you’re in the market for some remote lakeshore property where you can get away from it all, this might be just what you’re looking for. Located in a secluded, pristine setting, this must-see property might be one of a kind. It’s very remote; – did I mention this lakeshore is on Mars? And, oh — it happens to be a former lakeshore.

While lakeshore property on Mars might sound like the biggest real estate swindle ever, the news of the first definitive lakeshore on Mars is momentous. Using images from the HiRISE Camera on the Mars Reconnaissance Orbiter, a University of Colorado at Boulder research team has discovered indications of a deep, ancient lake, estimated to be more than 3 billion years old.

The lake appears to have covered as much as 80 square miles and was up to 460 meters (1,500 feet) deep — roughly the equivalent of Lake Champlain bordering the United States and Canada, said CU-Boulder Research Associate Gaetano Di Achille, who led the study. The shoreline evidence, found along a broad delta in a region called Shalbatana Vallis, includes a series of alternating ridges and troughs thought to be surviving remnants of beach deposits.

“This is the first unambiguous evidence of shorelines on the surface of Mars,” said Di Achille. “The identification of the shorelines and accompanying geological evidence allows us to calculate the size and volume of the lake, which appears to have formed about 3.4 billion years ago.”

HiRISE image from Shalbatana Vallis. Credit: NASA/JPL/ U of AZ
HiRISE image from Shalbatana Vallis. Credit: NASA/JPL/ U of AZ

An analysis of the HiRISE images indicate that water carved a 50 km (30 mile) -long canyon that opened up into a valley, depositing sediment that formed a large delta. This delta and others surrounding the basin imply the existence of a large, long-lived lake, said team member Brian Hynek, also from CU-Boulder.
“Finding shorelines is a Holy Grail of sorts to us,” said Hynek.

In addition, the evidence shows the lake existed during a time when Mars is generally believed to have been cold and dry, which is at odds with current theories proposed by many planetary scientists, he said. “Not only does this research prove there was a long-lived lake system on Mars, but we can see that the lake formed after the warm, wet period is thought to have dissipated.”

Planetary scientists think the oldest surfaces on Mars formed during the wet and warm Noachan epoch from about 4.1 billion to 3.7 billion years ago that featured a bombardment of large meteors and extensive flooding. The newly discovered lake is believed to have formed during the Hesperian epoch and postdates the end of the warm and wet period on Mars by 300 million years, according to the study.

The deltas adjacent to the lake are of high interest to planetary scientists because deltas on Earth rapidly bury organic carbon and other biomarkers of life, according to Hynek. Most astrobiologists believe any present indications of life on Mars will be discovered in the form of subterranean microorganisms.

Close-up of region in Shalbatana Vallis. Credit: NASA/JPL/U of A
Close-up of region in Shalbatana Vallis. Credit: NASA/JPL/U of A

But in the past, lakes on Mars would have provided cozy surface habitats rich in nutrients for such microbes, Hynek said.

The retreat of the lake apparently was rapid enough to prevent the formation of additional, lower shorelines, said Di Achille. The lake probably either evaporated or froze over with the ice slowly turning to water vapor and disappearing during a period of abrupt climate change, according to the study.

Di Achille said the newly discovered pristine lake bed and delta deposits would be would be a prime target for a future landing mission to Mars in search of evidence of past life.

“On Earth, deltas and lakes are excellent collectors and preservers of signs of past life,” said Di Achille. “If life ever arose on Mars, deltas may be the key to unlocking Mars’ biological past.”

The team’s paper has been published online in Geophysical Research Letters, a publication of the American Geophysical Union.

Mars Rover’s Underbelly Panorama

Panorama underneath the Spirit rover. Credit: NASA/JPL

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The Spirit rover has now taken two sets of close-up images showing the ground where it has been stuck for several weeks. Spirit used the microscopic imager on the robotic arm to peer underneath her own belly in an attempt to determine how the vehicle is embedded, and if there might be something obstructing the rover. Sure enough, the images appear to show a rock or mound of dirt that might be in the way, but more pictures and tests are needed before the rover team can develop a strategy for getting the rover out of its current predicament. Rover project manager John Callas said using the robotic arm for this purpose was never in the original design book, but it appears to have worked quite well.

Spirit is dug in over halfway up her wheels in soil that varies from one side of the rover to the other. The rover engineers and drivers have been worried that Spirit has dug herself down so deep that her belly might be sitting on rocks, and one wheel may be jammed by a rock.

The camera normally take close-up images of Martian rocks and soil. The technique for using it to look underneath the rover was tested on Spirit’s twin, Opportunity, and it worked well. The first set of images are a little out of focus, but according to an article in New Scientist, Spirit took additional images on Tuesday which showed one possible obstruction, but it wasn’t clear whether it was a rock or just a mound of dirt, and it also wasn’t obvious if the object was hitting the rover’s underside.

In an article in Universe Today last week, Callas said that even though this is one of the worst predicaments either rover has ever been in, he is optimistic about getting Spirit unstuck. “We saw that even on the last drive that the rover was still moving, even though it was only fractionally, based on the wheel spin. So, that tells us material is still being transported underneath the wheels. Given enough time and enough wheel spinning we should be able to get out. If that changes, if we get a situation where we have a hundred per cent slip, then we’re in trouble. But we’re not at that point yet, — even if we’re at 99.9%, that makes a big difference between 100%.”

And if this latest attempt doesn’t work, Callas says they have some other ideas up their robotic arm sleeves. “There are some exotic things we would consider if the more traditional methods don’t work,” he said. We have a lot of arrows in our quiver, or tools in our toolbelt to try first. ”

Sources: New Scientist, previous interview/article with John Callas

Dear JPL: I Have an Idea on How to Rescue the Spirit Rover

Drawing submitted to JPL by 7-year old Julian. Used by permission.

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We’re all concerned about the Spirit rover, currently stuck in some soft soil on Mars. But some people are actually working hard to figure out how to rescue the rover. That includes a 7-year old boy named Julian who sent this drawing in to JPL with his idea of how help Spirit: use the robotic arm as a “tripod” to lift the rover up and help move it out of the spot where it is embedded. Julian, you have a bright future ahead of you as an engineer! “We are getting a lot of interesting suggestions from the public,” said JPL’s John Callas, MER project manager, “and we think that’s wonderful. It shows people are interested in these rovers. We certainly are canvassing the full range of possibilities to get Spirit unstuck.”

And Callas said they are actually planning to use the robotic arm to help get Spirit unstuck, but not quite the way Julian had in mind.

“We’re doing a parallel approach,” Callas told Universe Today, “doing things both on Earth and on Mars. Spirit is using her instruments to assess the terrain and the nature of the materials where she is stuck. Just last night we made the decision to use the robotic arm to look underneath the belly of the rover to see if we can determine how the vehicle is embedded and if it may be high centered on some small rocks under the rover. We’ll also look at the wheels to see how the middle wheels are dug in.”

Callas said this is a technique the robotic arm was never designed to do. “So, we tested it first on Opportunity and it worked quite well, so that’s the plan for what we’ll do with Spirit this weekend.”

Spirit has also been busy taking remote sensing images of the surrounding terrain with all its instruments to try to characterize the soils and their properties. Callas said “soils” because there actually appears to be two different types of materials where the rover is stuck, with a different type of soil on the left side of the rover from the right.

Workers at JPL start digging to replicate Spirit's situation on Mars. Image credit: NASA/JPL
Workers at JPL start digging to replicate Spirit's situation on Mars. Image credit: NASA/JPL

The rover team will use the data to create a soil simulant to be used in the JPL test bed, basically a large sandbox where an engineering model of the rover identical to Spirit and Opportunity can be used to simulate Spirit’s predicament. There, the team can experiment with how best to get the rover out.

However, the test has been held up because of problems with work station that controls the test facility, but Callas said they are hoping by later today (Friday) to get started with the simulations.

They’ll start by putting the simulated Mars regolith, which is called baghouse dust, (ground basaltic material, Callas said) and use enough to test just one wheel of the rover. “If it exhibits the same characteristics we’re seeing on Mars, then we’ll truck in tons of that material to do the tests with the rover,” said Callas. If not, they’ll have to go back to the drawing board.

Spirit's wheels embedded in the Martian regolith. Credit: NASA/JPL
Spirit's wheels embedded in the Martian regolith. Credit: NASA/JPL

Spirit has long been without the use of her right front wheel, which doesn’t help the situation, and recently the left middle wheel was jammed, but now appears to be working again. The one piece of good news is that Mars itself provided a little help by sending a gust of wind Spirit’s way, cleaning off the solar panels, making more energy available to the rover. Spirit now has over 80% of its potential power, with 843 watt hours available, as opposed to earlier where the rover was operating at less than 200 watt hours.

Callas said he is optimistic about getting Spirit unstuck. “We saw that even on the last drive that the rover was still moving, even though it was only fractionally, based on the wheel spin. So, that tells us material is still being transported underneath the wheels. Given enough time and enough wheel spinning we should be able to get out. If that changes, if we get a situation where we have a hundred per cent slip, then we’re in trouble. But we’re not at that point yet, — even if we’re at 99.9%, that makes a big difference between 100%.”

And if this latest attempt doesn’t work, Callas says they have some other ideas up their robotic arm sleeves. “There are some exotic things we would consider if the more traditional methods don’t work,” he said. We have a lot of arrows in our quiver, or tools in our toolbelt to try first. ”

And they always have Julian to rely on, too.

Source: Interview with John Callas
Julian’s picture on Twitpic — check out the comments!

Fly Over the Potential Landing Sites For Next Mars Rover (Video)


Hang on and take a bird’s eye look at the four different proposed landing sites for the Mars Science Lab! At a briefing yesterday, Dr. Richard Zurek presented a flyover video of the potential landing sites for the next Mars rover, set to launch in 2011. The video is now available, and Zurek narrates the excellent flyover footage of each site, created by images taken by the HiRISE camera on the Mars Reconnaissance Orbiter. Enjoy the video, and find out a little more on each of the proposed sites below.
Continue reading “Fly Over the Potential Landing Sites For Next Mars Rover (Video)”

Mars Rover Has a New Name

Artist concept of MSL. Credit: JPL

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The Mars Science Laboratory rover, scheduled for launch in 2011, now has a new name, thanks to a sixth-grade student from Kansas. Twelve-year-old Clara Ma submitted the winning entry, “Curiosity” in the name-the-rover contest for schoolchildren, sponsored by NASA. “We have been eager to call the rover by name,” said Pete Theisinger, who manages the JPL team building and testing Curiosity. “Giving it a name worthy of this mission’s quest means a lot to the people working on it.”

For winning the naming contest, Clara gets to sign her name directly on the rover. But you can send your name to Mars with Curiosity, too.

Find out more about sending your name to Mars.

A NASA panel selected the name following a nationwide student contest that attracted more than 9,000 proposals via the Internet and mail. The panel primarily took into account the quality of submitted essays. Name suggestions from the Mars Science Laboratory project leaders and a non-binding public poll also were considered.

“Students from every state suggested names for this rover. That’s testimony to the excitement Mars missions spark in our next generation of explorers,” said Mark Dahl, the mission’s program executive at NASA Headquarters in Washington. “Many of the nominating essays were excellent and several of the names would have fit well. I am especially pleased with the choice, which recognizes something universally human and essential to science.”

Clara Ma
Clara Ma

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

“I was really interested in space, but I thought space was something I could only read about in books and look at during the night from so far away,” Ma said. “I thought that I would never be able to get close to it, so for me, naming the Mars rover would at least be one step closer.”

“Curiosity is an everlasting flame that burns in everyone’s mind. It makes me get out of bed in the morning and wonder what surprises life will throw at me that day,” Ma wrote in her winning essay. “Curiosity is such a powerful force. Without it, we wouldn’t be who we are today. Curiosity is the passion that drives us through our everyday lives. We have become explorers and scientists with our need to ask questions and to wonder.”

Source: JPL

More Researchers Say Liquid Water Present on Mars Now

Blobs of something "growing" on the Phoenix lander's legs.

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Finding perchlorates on Mars was not only surprising for the Phoenix lander science team, it also has created a bit of a rift among the researchers. In March, Ian reported on one scientist who used strictly photographic evidence to say that blobs appearing on the lander’s legs were actually water. Other scientists, however, including principal investigator Peter Smith were dubious about the “water on Mars now” claims. But now, a group of researchers at the University of Arkansas say they have now demonstrated a potential stable liquid on present-day Mars in the immediate environment of the lander.

The salts formed from perchlorates discovered at the Phoenix landing site act as “anti-freeze” and have the potential to be found in a liquid solution under the temperature and pressure conditions on present-day Mars, say professor Vincent F. Chevrier and graduate students Jennifer Hanley and Travis S. Altheide. Their research is published in the current issue of Geophysical Research Letters.

“Under real, observed Martian conditions, you can have a stable liquid,” said Chevrier.

The researchers studied the properties of sodium and magnesium perchlorates, salts detected by the Phoenix lander, under the temperature, pressure and humidity conditions found at the landing site. The discovery of perchlorates on Mars by the Phoenix mission surprised scientists – the compounds are rare on Earth, found mostly in extremely arid environments such as the Atacama Desert in Chile.

This image was taken by the Phoenix land on the 97th day of the mission.  Credit: NASA/JPL
This image was taken by the Phoenix land on the 97th day of the mission. Credit: NASA/JPL


The scientists studied the properties of these salts at varying temperatures using the Andromeda Chamber in the W.M. Keck Laboratory for Space Simulation – a chamber that can imitate the pressure and atmospheric conditions found on Mars. They also performed thermodynamic calculations to determine the state of salt and water combinations on the Martian surface and to see if there was any potential for liquid to be found.

The extreme temperatures found on Mars typically lead to either crystallization or evaporation of water, making it difficult to imagine that water could be found in liquid form. However, salts have been shown to lower the freezing point of water – which is why street crews use salt on the roads to melt ice, Hanley said. Some salts, like perchlorates, lower the freezing point substantially. It turns out that the temperature for the liquid phase of magnesium perchlorate – 206 degrees Kelvin – is a temperature found on Mars at the Phoenix landing site. Based on temperature findings from the Phoenix lander, conditions would allow this perchlorate solution to be present in liquid form for a few hours each day during the summer.

“The window for liquid is very small,” Hanley said. Nevertheless, this finding further supports the possibility of finding life on Mars.

“You don’t necessarily need to have a lot of water to have life,” Chevrier said. “But you need liquid water at some point.”

Source: University of Arkansas

Opportunity Reveals Long-time Water, Winds at Victoria

A sizable collaboration of researchers has unveiled an enormous set of data from NASA’s Opportunity rover today — data that testify to the rover’s lucky longevity, and paint a picture of climate events that have shaped Victoria Crater, shown in this NASA/JPL-Caltech image.

The climate history is vast and compelling, including dramatic floods and terrain-shaping winds spanning billions of years. The data appear in today’s issue of the journal Science.

Because of the Mars rovers’ ability to move from place to place and also because of their unexpected long lives, the mission scientists have been able to study Mars in situ in a way they weren’t anticipating.

“There’s no way Spirit and Opportunity could have made all of these discoveries without the longevity that they’ve had,” said principal investigator Steve Squyres, of Cornell University in Ithaca, N.Y. “Mars has been good to us, but more than anything else, I think their longevity is testimony to the excellence of the work that was done by the team that built these vehicles so many years ago.”

Pancam false-color image of the east face of Cape Verde, showing typcal impact-related stratigraphy. Credit: NASA/JP
Pancam false-color image of the east face of Cape Verde, showing typcal impact-related stratigraphy. Credit: NASA/JP

The Opportunity rover has been able to study in detail three different craters located over three miles apart.  Data and images from the rover show similar patterns in sedimentary rocks in each crater, patterns that could only have been laid down by ancient water flow. According to Squyres and his team, this discovery means that water once covered the entire area and helped shape that region of the planet long ago.

The rover revealed that water repeatedly came and left billions of years ago. Wind persisted much longer, heaping sand into dunes between ancient water episodes. These activities still shape the landscape today. At Victoria, steep cliffs and gentler alcoves alternate around the edge of a bowl about 0.8 kilometers (half a mile) in diameter. The scalloped edge and other features indicate the crater once was smaller than it is today, but wind erosion has widened it gradually. 

More layering in Victoria Crater. Credit: NASA/JPL
More layering in Victoria Crater. Credit: NASA/JPL

“What drew us to Victoria Crater is the thick cross-section of rock layers exposed there,” Squyres said. “The impact that excavated the crater millions of years ago provided a golden opportunity, and the durability of the rover enabled us to take advantage of it.” 

Imaging the crater’s rim and interior, Opportunity inspected layers in the cliffs around the crater, including layered stacks more than 10 meters (30 feet) thick. Distinctive patterns indicate the rocks formed from shifting dunes that later hardened into sandstone, according to Squyres and 33 co-authors.

Instruments on the rover’s arm studied the composition and detailed texture of rocks just outside the crater and exposed layers in one alcove called “Duck Bay.” Rocks found beside the crater include pieces of a meteorite, which may have been part of the impacting space rock that made the crater. 

Inside Duck Bay, the rover found that the lower layers showed less sulfur and iron, more aluminum and silicon. This composition matches patterns Opportunity found earlier at the smaller Endurance Crater, about 6 kilometers (4 miles) away from Victoria, indicating the processes that varied the environmental conditions recorded in the rocks were regional, not just local.

Squyres said there were specific minerals and specific patterns in the geochemistry of the crater walls. In all three craters, Eagle, Endurance and Victoria, the round, iron-rich spherules — BB-like structures — which the scientists nicknamed “blueberries,” were found embedded in the rock. The scientists have concluded that these were created from mineral deposits emerging from a watery solution inside the rock.

Opportunity gained more than 30 meters (98 feet) of elevation travelling from Endurance to Victoria, and the amount of “blueberries” decreased with the elevation. But once the rover entered Victoria crater, which is about 75 meters (246 feet) deep — and 750 meters in diameter — the spherules reappeared in the soil.

The spherules in rocks deeper in the crater are larger than those in overlying layers, suggesting the action of groundwater was more intense at greater depth. 

Opportunity’s first observations showed interaction of volcanic rock with acidic water to produce sulfate salts. Dry sand rich in these salts blew into dunes. Under the influence of water, the dunes hardened to sandstone. Further alteration by water produced the iron-rich spherules, mineral changes and angular pores left when crystals dissolved away. 

A rock from space blasted a hole about 600 meters (2,000 feet) wide and 125 meters (400 feet) deep. Wind erosion chewed at the edges of the hole and partially refilled it, increasing the diameter by about 25 percent and reducing the depth by about 40 percent. 

Since leaving Victoria Crater about eight months ago, Opportunity has been on its way to study a crater named Endeavour that is about 20 times bigger than Victoria. The rover has driven about one-fifth of what could be a 16-kilometer (10-mile) trek to this new destination. 

Sources: NASA and an e-mail exchange with Steve Squyres.

A Cold and Wet History on Early Mars?

Mars. Credit: NASA

 

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Even if an early Mars never got above freezing, the brine on its surface could have stayed liquid and supported life, a new study says.

Lead author Alberto G. Fairen, of NASA Ames Research Center in Moffett Field, California, and his colleagues have analyzed the behavior of Martian chemical concentrations found at various mission landing sites, and revealed that warm temperatures wouldn’t have been necessary to support salt-loving life forms.

The authors point out that many features on the Martian surface are believed to have been formed by flowing water and related mineral activity on the surface. Water is a key ingredient for life, but models were having a hard time envisioning a Mars warm enough to support it.

Much evidence has indicated surface temperatures well below freezing.

According to the new study, life may have fared all right anyway.

“Solutes could depress the melting point of water in a frozen Martian environment, providing a plausible solution to the early Mars climate paradox,” the authors write.

Fairen and his colleagues modeled the freezing and evaporation processes of Martian fluids with a composition resulting from the weathering of basalts, as reflected in the chemical compositions at Mars landing sites of Viking 1, Mars Pathfinder, and the rovers Spirit and Opportunity.

“Our results show that a significant fraction of weathering fluids loaded with Si, Fe, S, Mg, Ca, Cl, Na, K and Al remain in the liquid state at temperatures well below 273 K,” or nearly 32 degrees Fahrenheit (zero C), they write.

“This stability against freezing of Martian fluids can explain saline liquid water activity on the surface of Mars at mean global temperatures well below 273 K.”

Photo credit: NASA

Source: Nature

Spirit Rover Stuck in “Difficult Situation”

Wheel slippage during attempts to extricate NASA's Mars Rover Spirit from a patch of soft ground during the preceding two weeks had partially buried the wheels by the 1,899th Martian day, or sol, of the Spirit's mission on Mars (May 6, 2009). Image credit: NASA/JPL-Caltech

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Of all the perilous situations and technological issues the two Mars rovers dealt with, soft soil wasn’t tops on my list of what might mean the end of roving on Mars. The Spirit rover is stuck in an area of soft sand-like soil, slipping severely during recent attempts to drive, sinking the wheels about halfway into the ground. The rover engineers and scientists has suspended driving Spirit temporarily while studying the ground around the rover and planning simulation tests of driving options with a test rover at NASA’s Jet Propulsion Laboratory, Pasadena, Calif.

“Spirit is in a very difficult situation,” JPL’s John Callas, MER project manager said Monday. “We are proceeding methodically and cautiously. It may be weeks before we try moving Spirit again. Meanwhile, we are using Spirit’s scientific instruments to learn more about the physical properties of the soil that is giving us trouble.”

Spirit has overcome problems with her flash drive, survived climbing and descending Husband Hill with a malfunctioning front wheel, and recently prevailed over problems caused by cosmic ray hit which caused memory problems and “amnesia.” Things were looking up for Spirit as three times in the past month, wind has removed some of the dust accumulated on Spirit’s solar panels, increasing the rover’s capability for generating power.

Spirit has been driving counterclockwise from north to south around a low plateau called “Home Plate” for two months. The rover progressed 122 meters (400 feet) on that route before reaching its current position.

In the past week, the digging-in of Spirit’s wheels has raised concerns that the rover’s belly pan could now be low enough to contact rocks underneath the chassis, which would make getting out of the situation more difficult. The right-front wheel on Spirit stopped working three years ago. Driving with just five powered wheels while dragging or pushing an immobile wheel adds to the challenge of the situation.

“The improved power situation buys us time,” Callas said. “We will use that time to plan the next steps carefully. We know that dust storms could return at any time, although the skies are currently clear.”

Opportunity also had problems with soft soil, running aground in a dune called “Purgatory” back in 2005. Extricating the rover from the dune required more than five weeks of planning, testing, and carefully monitored driving. So, don’t give up hope yet of the engineers figuring out how to get Spirit out of the bind she is in.

We’ll keep you posted.

Source: JPL

‘Dalmatian’ Volcano, Opportunity Rover and Other New Images from HiRISE

Ancient defrosting volcano on Mars, Credit: NASA/JPL/University of Arizona

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Malea Patera isn’t the name of one of the One Hundred and One Dalmatians, but it is the designation of an ancient volcano on Mars located on the outskirts of the Hellas impact basin. This isn’t your typical Martian landscape — just where are the red rocks and soil? — but is reminiscent of the markings on a Dalmatian dog. So what is going on here? This image was taken in early spring for this location in the southern hemisphere and the ground is covered with bright frost except for some dark splotches found in discrete patches. This is where the sunlight has penetrated the frost and initiated defrosting around discrete spots. The HiRISE scientists say that clearly, something is different about the patches, with the defrosting taking place, while the other areas remain frosty. One possibility is that these are (frost covered) dark sand dunes that heat up more easily than the surrounding terrain. However, to find out for sure, HiRISE will need to take a new image in the summer time to really know what is happening here. See below for a full view of this region, plus a few more of a mega-huge batch of images that were released today from the HiRISE camera on the Mars Reconnaissance Orbiter.

Full view of  Malea Patera.  Credit: NASA/JPL/U of AZ
Full view of Malea Patera. Credit: NASA/JPL/U of AZ


Starburst Spider. Credit: NASA/JPL/University of Arizona
Starburst Spider. Credit: NASA/JPL/University of Arizona

We move from dogs to spiders, but this, too is an unusual Mars image. Mars’ seasonal cap of carbon dioxide ice (dry ice) has eroded to create many beautiful terrains as it sublimates every spring. In this region we see troughs that form a starburst pattern.

In other areas these radial troughs have been referred to as “spiders,” simply because of their shape. In this region the pattern looks more dendritic as channels branch out numerous times as they get further from the center. The troughs are believed to be formed by gas flowing beneath the seasonal ice to openings where the gas escapes, carrying along dust from the surface below. The dust falls to the surface of the ice in fan-shaped deposits.

Opportunity Imaged by HiRISE (ESP_011765_1780) Credit: NASA/JPL/University of Arizona
Opportunity Imaged by HiRISE (ESP_011765_1780) Credit: NASA/JPL/University of Arizona


HiRISE spied the Opportunity rover heading through the dunes of Meridiani Planum. This image is about 400 meters across and was taken on January 29, 2009, Opportunity’s 1783rd sol (Mars day) on the Red Planet. Opportunity had driven 130 meters on the previous sol; wheel tracks are visible crossing dark ripples to the upper right of the rover. The ripples, which trend mostly north-south in this area, can be easily crossed by the rover unless they are very large (such as those right of center).

Using the HiRISE images allows the MER scientists to plan out Oppy’s route in great detail, avoiding potential hazards and targeting features of interest (such as the small craters below and left of center). HiRISE images are routinely used by the Opportunity operations team for these purposes, and to plan the route to distant Endeavour Crater, the long-term goal of Opportunity’s mission, about 17 km to the southeast.

Opportunity has been exploring Mars for over 5 (Earth) years; it will probably take another two years to reach Endeavour.

Check out over 600 observations that were just released by the HiIRISE team — 2 terabytes worth of data! And all are Martian eye candy (or is that “Hi” candy?) Hats off to HiRISE and her team!

Source: HiRISE site