Showing posts with label Mount Sharp. Show all posts
Showing posts with label Mount Sharp. Show all posts

Thursday, November 20, 2014

NASA Mars Curiosity Rover Examines selected rocks

This small ridge, about 3 feet long, appears to resist wind erosion more than the flatter plates around it. 

Such differences are among the traits NASA's Curiosity Mars rover is examining at selected rock targets at the base of Mount Sharp. Curiosity's Mastcam acquired this view on Oct. 7, 2014.

Image Credit: NASA /JPL-Caltech /MSSS

NASA's Curiosity Mars rover has completed a reconnaissance "walkabout" of the first outcrop it reached at the base of the mission's destination mountain and has begun a second pass examining selected rocks in the outcrop in more detail.

Exposed layers on the lower portion of Mount Sharp are expected to hold evidence about dramatic changes in the environmental evolution of Mars. That was a major reason NASA chose this area of Mars for this mission.

The lowermost of these slices of time ascending the mountain includes a pale outcrop called "Pahrump Hills."

It bears layers of diverse textures that the mission has been studying since Curiosity acquired a drilled sample from the outcrop in September.

In its first pass up this outcrop, Curiosity drove about 360 feet (110 meters), and scouted sites ranging about 30 feet (9 meters) in elevation.

It evaluated potential study targets from a distance with mast-mounted cameras and a laser-firing spectrometer.

This patch of Martian bedrock, about 2 feet (70 centimeters) across, is finely layered rock with some pea-size inclusions. 

It lies near the lowest point of the "Pahrump Hills" outcrop, which forms part of the basal layer of Mount Sharp. Curiosity's Mastcam acquired this view on Nov. 9, 2014.

Image Credit: NASA/JPL-Caltech/MSSS

"We see a diversity of textures in this outcrop -- some parts finely layered and fine-grained, others more blocky with erosion-resistant ledges," said Curiosity Deputy Project Scientist Ashwin Vasavada of NASA's Jet Propulsion Laboratory, Pasadena, California.

"Overlaid on that structure are compositional variations. Some of those variations were detected with our spectrometer. Others show themselves as apparent differences in cementation or as mineral veins. There's a lot to study here."

During a second pass up the outrcrop, the mission is using a close-up camera and spectrometer on the rover's arm to examine selected targets in more detail.

The second-pass findings will feed into decisions about whether to drill into some target rocks during a third pass, to collect sample material for onboard laboratory analysis.

A wheel track cuts through a windblown ripple of dusty sand in this Nov. 7, 2014, image from the Mastcam on NASA's Curiosity rover

The view spans about four feet across. This experiment was planned for yielding a view of the inside of the ripple for assessment of particle sizes and composition.

Image Credit: NASA/JPL-Caltech/MSSS

"The variations we've seen so far tell us that the environment was changing over time, both as the sediments were laid down and also after they hardened into bedrock," Vasavada said.

"We have selected targets that we think give us the best chance of answering questions about how the sediments were deposited, in standing water? flowing water? sand blowing in the wind? -- and about the composition during deposition and later changes."

The first target in the second pass is called "Pelona," a fine-grained, finely layered rock close to the September drilling target at the base of Pahrump Hills outcrop. The second is a more erosion-resistant ledge called "Pink Cliffs."

Before examining Pelona, researchers used Curiosity's wheels as a tool to expose a cross section of a nearby windblown ripple of dust and sand.

One motive for this experiment was to learn why some ripples that Curiosity drove into earlier this year were more difficult to cross than anticipated. 

Wednesday, November 5, 2014

NASA Mars Curiosity Rover discovers mineral match

This image shows the first holes drilled by NASA's Mars rover Curiosity at Mount Sharp. 

The loose material near the drill holes is drill tailings and an accumulation of dust that slid down the rock during drilling. 

Credit: NASA/JPL-Caltech/MSSS

Reddish rock powder from the first hole drilled into a Martian mountain by NASA's Curiosity rover has yielded the mission's first confirmation of a mineral mapped from orbit.

"This connects us with the mineral identifications from orbit, which can now help guide our investigations as we climb the slope and test hypotheses derived from the orbital mapping," said Curiosity Project Scientist John Grotzinger, of the California Institute of Technology in Pasadena.

Curiosity collected the powder by drilling into a rock outcrop at the base of Mount Sharp in late September.

The robotic arm delivered a pinch of the sample to the Chemistry and Mineralogy (CheMin) instrument inside the rover.

This sample, from a target called "Confidence Hills" within the "Pahrump Hills" outcrop, contained much more hematite than any rock or soil sample previously analyzed by CheMin during the two-year-old mission.

Hematite is an iron-oxide mineral that gives clues about ancient environmental conditions from when it formed.

In observations reported in 2010, before selection of Curiosity's landing site, a mineral-mapping instrument on NASA's Mars Reconnaissance Orbiter (MRO) provided evidence of hematite in the geological unit that includes the Pahrump Hills outcrop.

The landing site is inside Gale Crater, an impact basin about 96 miles (154 kilometers) in diameter with the layered Mount Sharp rising about three miles (five kilometers) high in the center.

"We've reached the part of the crater where we have the mineralogical information that was important in selection of Gale Crater as the landing site," said Ralph Milliken of Brown University,

Providence, Rhode Island. He is a member of Curiosity's science team and was lead author of that 2010 report in Geophysical Research Letters identifying minerals based on observations of lower Mount Sharp by the orbiter's Compact Reconnaissance Imaging Spectrometer for Mars (CRISM).

"We're now on a path where the orbital data can help us predict what minerals we'll find and make good choices about where to drill. Analyses like these will help us place rover-scale observations into the broader geologic history of Gale that we see from orbital data."

This image from NASA's Curiosity rover shows a sample of powdered rock extracted by the rover's drill from the "Confidence Hills" target, the first rock drilled after Curiosity reached the base of Mount Sharp in September 2014. 

Credit: NASA/JPL-Caltech/MSSS

Much of Curiosity's first year on Mars was spent investigating outcrops in a low area of Gale Crater called "Yellowknife Bay," near the spot where the rover landed.

The rover found an ancient lakebed. Rocks there held evidence of wet environmental conditions billions of years ago that offered ingredients and an energy source favourable for microbial life, if Mars ever had microbes.

Clay minerals of interest in those rocks at Yellowknife Bay had not been detected from orbit, possibly due to dust coatings that interfere with CRISM's view of them.

The rover spent much of the mission's second year driving from Yellowknife Bay to the base of Mount Sharp.

The hematite found in the first sample from the mountain tells about environmental conditions different from the conditions recorded in the rocks of Yellowknife Bay.

The rock material interacted with water and atmosphere to become more oxidized.

The rocks analyzed earlier also contain iron-oxide minerals, mostly magnetite. One way to form hematite is to put magnetite in oxidizing conditions.

The latest sample has about eight percent hematite and four percent magnetite. The drilled rocks at Yellowknife Bay and on the way to Mount Sharp contain at most about one percent hematite and much higher amounts of magnetite.

"There's more oxidation involved in the new sample," said CheMin Deputy Principal Investigator David Vaniman of the Planetary Science Institute in Tucson, Arizona.

This side-by-side comparison shows the X-ray diffraction patterns of two different samples collected from rocks on Mars by NASA's Curiosity rover. 

The images present data obtained by Curiosity's Chemistry and Mineralogy instrument (CheMin). 

At left is a pattern of data from analysis of the "Cumberland" rock target in the "Yellowknife Bay" area investigated by Curiosity in 2013. 

The pattern at right is from the "Confidence Hills" target that was the first rock drilled after Curiosity reached the base of Mount Sharp in September 2014. 

A label in the right image of the annotated view points out evidence for the mineral hematite in this rock. 

Credit: NASA/JPL-Caltech

The sample is only partially oxidized, and preservation of magnetite and olivine indicates a gradient of oxidation levels.

That gradient could have provided a chemical energy source for microbes.

The Pahrump HIlls outcrop includes multiple layers uphill from its lowest layer, where the Confidence Hills sample was drilled.

The layers vary in texture and may also vary in concentrations of hematite and other minerals.

The rover team is now using Curiosity to survey the outcrop and assess possible targets for close inspection and drilling.

This view shows the path and some key places in a survey of the "Pahrump Hills" outcrop by NASA's Curiosity Mars rover in autumn of 2014. The outcrop is at the base of Mount Sharp within Gale Crater. 

The mission's in-place investigation of the layered mountain began at the low edge of the Pahrump Hills outcrop, at the target "Confidence Hills." 

Curiosity collected a drilled sample of rock powder at that target in September 2014 and delivered portions of the powder into analytical instruments inside the rover. 

Then the mission began a "walkabout" of the outcrop, similar to the way field geologists on Earth walk across an outcrop to choose the best places on it to examine in detail. 

The dashed gold line indicates the path the rover drove during the walkabout. Names are shown for a few of the features visited and observed by the rover. 

Red dots indicate stops at the end of a day's drive. White dots indicate locations of stops made during the drives to collect observations of the Pahrump Hills outcrop. 

The mission completed the walkabout at the site labeled "Whale Rock," and the team is now examining the observations acquired during the walkabout to decide where to return for more detailed analysis. Credit: NASA/JPL-Caltech/MSSS

The mission may spend weeks to months at Pahrump Hills before proceeding farther up the stack of geological layers forming Mount Sharp.

Those higher layers include an erosion-resistant band of rock higher on Mount Sharp with such a strong orbital signature of hematite, it is called "Hematite Ridge."

The target drilled at Pahrump Hills is much softer and more deeply eroded than Hematite Ridge.

Another NASA Mars rover, Opportunity, made a key discovery of hematite-rich spherules on a different part of Mars in 2004.

That finding was important as evidence of a water-soaked history that produced those mineral concretions.

The form of hematite at Pahrump Hills is different and is most important as a clue about oxidation conditions. Plenty of other evidence in Gale Crater has testified to the ancient presence of water.

Wednesday, August 20, 2014

NASA Mars Curiosity Rover Stalled by 'Hidden Valley' Sand Trap








Click on the picture to see the full image.

NASA’s Curiosity rover looks back to ramp with 4th drill site target at ‘Bonanza King’ rock outcrop in ‘Hidden Valley’ in this photo mosaic view captured on Aug. 6, 2014, Sol 711. 

Inset shows results of brushing on Aug. 17, Sol 722, that revealed gray patch beneath red dust. Note the rover’s partial selfie, valley walls, deep wheel tracks in the sand dunes and distant rim of Gale crater beyond the ramp. Navcam camera raw images stitched and colorized. 

Credit: NASA/JPL-Caltech/Ken Kremer-kenkremer.com/Marco Di Lorenzo


This image, taken by NASA's Mars rover Curiosity in August 2014, looks across the northeastern end of sandy "Hidden Valley" to the lower slopes of Mount Sharp on the horizon.

Credit: NASA/JPL-Caltech

NASA's Mars rover Curiosity may have to choose a new route to the base of a huge Red Planet mountain.

The 1-ton Curiosity rover had been heading for Mount Sharp, a 3.4-mile-high (5.5 kilometers) mountain in the center of Mars' Gale Crater, via "Hidden Valley," a sandy swale that's about the length of a football field.

But Curiosity turned back shortly after entering the valley's northeastern end earlier this month, finding the sand surprisingly slippery, NASA officials said.

"We need to gain a better understanding of the interaction between the wheels and Martian sand ripples, and Hidden Valley is not a good location for experimenting," Curiosity project manager Jim Erickson, of NASA's Jet Propulsion Laboratory (JPL) in Pasadena, California, said in a statement.

This photo taken on Aug. 12, 2014 by NASA's Curiosity Mars rover shows an outcrop that includes the "Bonanza King" rock under consideration as a drilling target.

Credit: NASA/JPL-Caltech/MSSS

There is no way out of Hidden Valley save exits at its northeastern and southwestern ends, NASA officials said.

The mission team is now assessing possible alternative routes that would take Curiosity north of the valley.

The goal is to get Curiosity to Mount Sharp, which has been the rover's ultimate science destination since before its August 2012 touchdown.

Mission scientists want the six-wheeled robot to climb up through the mountain's foothills, reading a history in the rocks of Mars' transition from a warm and wet planet in the ancient past to the cold, dry world we know today.

The chief goal of the $2.5 billion Curiosity mission is to determine if the Red Planet could ever have supported microbial life.

The team has already checked off this goal, finding that an area near Curiosity's landing site called Yellowknife Bay was a habitable lake-and-stream system billions of years ago.

Researchers came to this conclusion last year after analyzing samples Curiosity drilled from two different rocks in Yellowknife Bay.

Friday, August 15, 2014

NASA Curiosity Mars Rover Prepares for Fourth Rock Drilling

In this image from NASA's Curiosity Mars rover looking up the ramp at the northeastern end of "Hidden Valley," a pale outcrop including drilling target "Bonanza King" is at the center of the scene. 

The rover's Navcam captured this northward view on Aug. 4, 2014, from the valley's sandy floor.

Image Credit: NASA/JPL-Caltech

The team operating NASA's Curiosity Mars rover has chosen a rock that looks like a pale paving stone as the mission's fourth drilling target, if it passes engineers' evaluation.

They call it "Bonanza King."

It is not at the "Pahrump Hills" site the team anticipated the rover might reach by mid-August.

Unexpected challenges while driving in sand prompted the mission to reverse course last week after entering a valley where ripples of sand fill the floor and extend onto sloping margins.

However, the new target outcrop's brightness and its position within the area's geological layers resemble the Pahrump Hills outcrop.

This Aug. 14, 2012, image from the Mastcam on NASA's Curiosity Mars rover shows an outcrop that includes the "Bonanza King" rock under consideration as a drilling target. 

Raised ridges on the flat rocks are visible at right. 

Tread marks from a rover wheel are in the lower half.

Image Credit: NASA/JPL-Caltech/MSSS

"Geologically speaking, we can tie the Bonanza King rocks to those at Pahrump Hills. Studying them here will give us a head start in understanding how they fit into the bigger picture of Gale Crater and Mount Sharp," said Curiosity Deputy Project Scientist Ashwin Vasavada of NASA's Jet Propulsion Laboratory in Pasadena, California.

Mount Sharp is the mission's long-term science destination, offering a stack of layers holding evidence about environmental changes on ancient Mars.

The mountain rises from inside Gale Crater, where Curiosity landed in August 2012.

All three rocks the rover has drilled so far have been geologically associated with the crater floor, rather than the mountain.

Sample material pulled from the first two and delivered to Curiosity's onboard analytical laboratories in 2013 provided evidence for ancient environmental conditions favorable for microbial life.

A drilled sample from Bonanza King may add understanding about how environments varied and evolved.

This image from NASA's Curiosity Mars rover looks down the ramp at the northeastern end of "Hidden Valley" and across the sandy-floored valley to lower slopes of Mount Sharp on the horizon. 

The rover's Navigation Camera captured this southward view on Aug. 12, 2014, after exiting the valley. 

Image Credit: NASA/JPL-Caltech

Monday, August 4, 2014

NASA Mars Rover Curiosity nears mountain-base outcrop

This full-circle panorama of the landscape surrounding NASA's Curiosity Mars rover on July 31, 2014, offers a view into sandy lower terrain called "Hidden Valley," which is on the planned route ahead. 

It combines several images from Curiosity's Navigation Camera (NavCam). South is at the center. 

Credit: NASA/JPL-Caltech 

As it approaches the second anniversary of its landing on Mars, NASA's Curiosity rover is also approaching its first close look at bedrock that is part of Mount Sharp, the layered mountain in the middle of Mars' Gale Crater.

The mission made important discoveries during its first year by finding evidence of ancient lake and river environments.

During its second year, it has been driving toward long-term science destinations on lower slopes of Mount Sharp.

Those destinations are in an area beginning about 2 miles (3 kilometers) southwest of the rover's current location, but an appetizer outcrop of a base layer of the mountain lies much closer, less than one-third of a mile (500 meters) from Curiosity. The rover team is calling the outcrop "Pahrump Hills."

"We're coming to our first taste of a geological unit that's part of the base of the mountain rather than the floor of the crater," said Curiosity Project Scientist John Grotzinger of the California Institute of Technology, Pasadena. "We will cross a major terrain boundary."

For about half of July, the rover team at NASA's Jet Propulsion Laboratory in Pasadena, California, drove Curiosity across an area of hazardously sharp rocks called "Zabriskie Plateau."

Damage to Curiosity's aluminum wheels from driving across similar terrain last year prompted a change in route planning to skirt such rock-studded terrain wherever feasible.

The one-eighth mile (200 meters) across Zabriski Plateau was one of the longest stretches without a suitable detour on the redesigned route toward the long-term science destination.

The main map shows landforms near NASA's Curiosity Mars rover as the rover's second anniversary of landing on Mars nears. 

The gold traverse line ends at Curiosity's position as of July 31, 2014 (Sol 705).

The inset shows the entire traverse and the remaining distance to Murray Buttes. Credit: NASA/JPL-Caltech 

"The wheels took some damage getting across Zabriskie Plateau, but it's less than I expected from the amount of hard, sharp rocks embedded there," said JPL's Jim Erickson, project manager for Curiosity.

"The rover drivers showed that they're up to the task of getting around the really bad rocks. There will still be rough patches ahead."

"We didn't imagine prior to landing that we would see this kind of challenge to the vehicle, but we're handling it."

Another recent challenge appeared last week in the form of unexpected behavior by an onboard computer currently serving as backup.

Curiosity carries duplicate main computers. It has been operating on its B-side computer since a problem with the A-side computer prompted the team to command a side swap in February 2013.

Work in subsequent weeks of 2013 restored availability of the A-side as a backup in case of B-side trouble.

Last week, fresh commanding of the rover was suspended for two days while engineers confirmed that the A-side computer remains reliable as a backup.

Curiosity landed inside Gale Crater on Aug. 5, 2012, PDT (Aug. 6, 2012, EDT). During its first year of operations, it fulfilled its major science goal of determining whether Mars ever offered environmental conditions favorable for microbial life.

Clay-bearing sedimentary rocks on the crater floor in an area called Yellowknife Bay yielded evidence of a lakebed environment billions of years ago that offered fresh water, all of the key elemental ingredients for life, and a chemical source of energy for microbes, if any existed there.

NASA's Mars Science Laboratory Project continues to use Curiosity to assess ancient habitable environments and major changes in Martian environmental conditions.

The destinations on Mount Sharp offer a series of layers that recorded different chapters in the environmental evolution of early Mars.

Tuesday, July 1, 2014

Mars Curiosity Rover: Travels outside landing ellipse

Nasa Curiosity Rover treks across Martian dunes and drives outside landing ellipse here, in this photo mosaic view captured on Sol 672, June 27, 2014. 

Distant eroded rim of Gale Crater seen in background. Navcam camera raw images stitched and colorized. 

Credit: NASA /JPL-Caltech /Marco Di Lorenzo /Ken Kremer

NASA's intrepid robot Curiosity is roving rapidly across the sandy ripples of the Red Planet in her quest to reach mysterious Mount Sharp and just drove outside her landing ellipse!

The six wheeled rover marked a major milestone on Sol 672, June 27, 2014, by driving beyond her targeted landing ellipse for the first time since touchdown nearly two years ago on August 5, 2012.

"On yestersol's drive [June 27], I left my landing ellipse, the 20×25 km area I targeted for landing," Curiosity tweeted across interplanetary space.

See our new Sol 672 photo mosaic above showing Curiosity's glorious view marking this major achievement just days ago.

Since switching paths to smoother, sandier terrain with less sharp edged rocks, Curiosity continues rolling across the floor of her Gale Crater landing site.

"After traversing 82 meters the rover stopped because it determined that it was slipping too much," wrote mission scientist Ken Herkenhoff in an update.

"Coincidentally, the rover stopped right on the landing ellipse, a major mission milestone!"

"The vehicle was designed to be able to traverse far enough to drive out of the region defined by the uncertainty in the landing location, and has now achieved that laudable goal."

Curiosity treks to Mount Sharp in this photo mosaic view captured on Sol 669, June 24, 2014. 

Navcam camera raw images stitched and coloured. 

Credit: NASA /JPL-Caltech /Marco Di Lorenzo /Ken Kremer

The SUV sized rover automatically stopped when it encountered soft sand and sensed that it wasn't making enough progress. It's been programmed with this built in safety check to avoid being trapped in a quagmire.

Earlier last week, Curiosity celebrated another milestone anniversary on June 24 (Sol 669), 1 Martian Year on Mars!

A Martian year is equivalent to 687 Earth days, or nearly two Earth years.

Curiosity crosses landing ellipse on Sol 672. 

Credit: NASA/JPL

During Year 1 on Mars, Earth's emissary has already accomplished her primary objective of discovering a habitable zone on the Red Planet that contains the minerals necessary to support microbial life in the ancient past.

So there's no stopping Curiosity on her way to Mount Sharp, which dominates the center of Gale Crater and reaches 3.4 miles (5.5 km) into the Martian sky, taller than Mount Rainier.



Curiosity rover panorama of Mount Sharp captured on June 6, 2014 (Sol 651) during traverse inside Gale Crater

Note rover wheel tracks at left. She will eventually ascend the mountain at the ‘Murray Buttes’ at right later this year. 

Assembled from Mastcam colour camera raw images and stitched by Marco Di Lorenzo and Ken Kremer. 

Credit: NASA /JPL /MSSS /Marco Di Lorenzo /Ken Kremer

Driving, Driving, Driving, that's Curiosity's number one priority as she traverses across the surface of Gale Crater towards towering Mount Sharp on an expedition in search of the chemical ingredients of life that could support Martian microbes if they ever existed.

Curiosity still has about another 2.4 miles (3.9 kilometers) to go to reach the entry way at a gap in the dunes at the foothills of Mount Sharp sometime later this year.

To date, Curiosity's odometer totals over 5.1 miles (8.4 kilometers) since landing inside Gale Crater on Mars in August 2012. She has taken over 162,000 images.

Monday, June 9, 2014

NASA Mars Rover Curiosity: New Mount Sharp panorama in transit


Curiosity rover panorama of Mount Sharp captured on June 6, 2014 (Sol 651) during traverse inside Gale Crater. Note rover wheel tracks at left. 

She will eventually ascend the mountain at the ‘Murray Buttes’ at right later this year. 

Assembled from Mastcam color camera raw images and stitched by Marco Di Lorenzo and Ken Kremer. 

Credit: NASA /JPL /MSSS /Marco Di Lorenzo

Within the past Martian day on Friday, June 6, NASA's rover Curiosity captured a stunning new panorama of towering Mount Sharp and the treacherous sand dunes below which she must safely traverse before reaching the mountains foothills, while in transit to her primary destination.

See our brand new Mount Sharp photo mosaic above – taken coincidentally by humanity's emissary on Mars on the 70th anniversary of D-Day on Earth.

Basically she's eating desiccated dirt while running a Martian marathon.

Having said 'Goodbye Kimberley' after drilling her third bore hole deep into a cold red slab of enticing bumpy textures of Martian sandstone in the name of science, our intrepid mega Rover Curiosity is trundling along with all deliberate speed towards the inviting slopes of sedimentary rocks at the base of mysterious Mount Sharp which hold clues to the habitability of the Red Planet.

The sedimentary layers of Mount Sharp, which reaches 3.4 miles (5.5 km) into the Martian sky, is the six wheeled robots ultimate destination inside Gale Crater because it holds caches of water altered minerals.

Such minerals could possibly mark locations that sustained potential Martian microbial life forms, past or present, if they ever existed.

The 1 ton robot is driving on a path towards the Murray Buttes which lies across the dunes on the right side of Mount Sharp as seen in our photo mosaic above, with wheel tracks on the left side.

She will eventually ascend the mountain at the 'Murray Buttes' after crossing the sand dunes.



Mars Rover Curiosity’s panoramic view departing Mount Remarkable and ‘The Kimberley Waypoint’ where rover conducted 3rd drilling campaign inside Gale Crater on Mars. 

The navcam raw images were taken on Sol 630, May 15, 2014, stitched and colorized. 

Credit: NASA/JPL-Caltech

Mars Rover Curiosity still has roughly another 4 kilometers of driving to go to reach the foothills of Mount Sharp sometime later this year.

Approximately four weeks ago, Curiosity successfully completed her 3rd drilling campaign since landing at the science waypoint region called "The Kimberley" on May 5, Sol 621, into the 'Windjana' rock target at the base of a 16 foot tall ( 5 Meter) hill called Mount Remarkable.

Mars was far wetter and warmer – and more conducive to the origin of life – billions of years ago.

The fresh hole drilled into "Windjana" was 0.63 inch (1.6 centimeters) in diameter and about 2.6 inches (6.5 centimeters) deep and resulted in a mound of dark grey coloured drill tailings piled around. It looked different from the initial holes drilled at Yellowknife Bay in the spring of 2013.

Composite photo mosaic shows deployment of NASA Rover Curiosity robotic arm and two holes after drilling into ‘Windjana’ sandstone rock on May 5, 2014, Sol 621, at Mount Remarkable as missions third drill target for sample analysis by rover’s chemistry labs. 

The Navcam raw images were stitched together from several Martian days up to Sol 621, May 5, 2014 and coloured. 

Credit: NASA/JPL-Caltech

Windjana lies some 2.5 miles (4 kilometers) southwest of Yellowknife Bay.

Curiosity then successfully delivered pulverized and sieved samples to the pair of onboard miniaturised chemistry labs; the Chemistry and Mineralogy instrument (CheMin) and the Sample Analysis at Mars instrument (SAM), for chemical and compositional analysis.

Before departing, Curiosity blasted the hole multiple times with her million watt laser on the Mast mounted Chemistry and Camera (ChemCam) instrument , leaving no doubt of her capabilities or intentions.

And she completed an up close examination of the texture and composition of 'Windjana' with the MAHLI camera and spectrometers at the end of her 7-foot-long (2 meter) arm to glean every last drop of science before moving on.

Wednesday, May 7, 2014

NASA's Curiosity rover drills sandstone slab Windjana on Mars

This May 5, 2014, image from the Navigation Camera on NASA's Curiosity Mars rover shows two holes at top centre drilled into a sandstone target called "Windjana." 

The farther hole was created by the rover's drill while it collected rock-powder sample material from the interior of the rock. 

Credit: NASA/JPL-Caltech

Portions of rock powder collected by the hammering drill on NASA's Curiosity Mars rover from a slab of Martian sandstone "Windjana," will be delivered to the rover's internal instruments.

Rover team members at NASA's Jet Propulsion Laboratory, Pasadena, Calif., received confirmation early today (Tuesday) of Curiosity's third successful acquisition of a drilled rock sample, following the drilling Monday evening (PDT).

The fresh hole in the rock target "Windjana," visible in images from the rover, is 0.63 inch (1.6 centimeters) in diameter and about 2.6 inches (6.5 centimeters) deep.

The full-depth hole for sample collection is close to a shallower test hole drilled last week in the same rock, which gave researchers a preview of the interior material as tailings around the hole.

Jim Bell
"The drill tailings from this rock are darker-toned and less red than we saw at the two previous drill sites," said Jim Bell of Arizona State University, Tempe, deputy principal investigator for Curiosity's Mast Camera (Mastcam).

"This suggests that the detailed chemical and mineral analysis that will be coming from Curiosity's other instruments could reveal different materials than we've seen before. We can't wait to find out!"

The mission's two previous rock-drilling sites, at mudstone targets in the Yellowknife Bay area, yielded evidence last year of an ancient lakebed environment with key chemical elements and a chemical energy source that long ago provided conditions favourable for microbial life.

The rover's current location is at a waypoint called "The Kimberley," about 2.5 miles (4 kilometers) southwest of Yellowknife Bay, and along the route toward the mission's long-term destination on lower slopes of Mount Sharp.

Sample material from Windjana will be sieved, then delivered in coming days to onboard laboratories for determining the mineral and chemical composition: the Chemistry and Mineralogy instrument (CheMin) and the Sample Analysis at Mars instrument (SAM).

The analysis of the sample may continue as the rover drives on from The Kimberley toward Mount Sharp. One motive for the team's selection of Windjana for drilling is to analyze the cementing material that holds together sand-size grains in this sandstone.

Wednesday, April 30, 2014

NASA Mars Curiosity Rover: MAHLI Captures a mosaic of Mars

A mosaic of MSL MAHLI images acquired on Sol 613. CLICK on the photo to see the full image

Credit: NASA /JPL-Caltech /MSSS

This is Curiosity's latest "selfie," a mosaic made up of about a dozen images acquired with the rover's Mars Hand Lens Imager (MAHLI) instrument on April 27-28, 2014 (Sol 613).

The 5.5-km-high Mount Sharp (Aeolis Mons) rising in the background.

There are plenty of discrepancies in the mosaic tiling but, some say, it imparts some character to Curiosity.

Visible in the mosaic are Curiosity's cylindrical RUHF antenna and a bit of her Radioisotope Thermoelectric Generator (RTG) visible in the lower center.

Tuesday, March 25, 2014

NASA Mars Curiosity rover finds sandstone variations

Sandstone layers with varying resistance to erosion are evident in this Martian scene recorded by the Mast Camera on NASA's Curiosity Mars rover on Feb. 25, 2014, about one-quarter mile (about 400 meters) from a planned waypoint called "the Kimberley." 

Credit: NASA /JPL-Caltech /MSSS

Variations in the stuff that cements grains together in sandstone have shaped the landscape surrounding NASA's Curiosity Mars rover and could be a study topic at the mission's next science waypoint.

On a journey with many months yet to go toward prime destinations on the lower slope of Mount Sharp, Curiosity is approaching a site called "the Kimberley."

Scientists on the team picked this location last year as a likely place to pause for investigation.

Its informal name comes from a northwestern Australia region known as the Kimberley. The Martian site's geological appeal, based on images taken from orbit, is that four types of terrain with different rock textures intersect there.

Ashwin Vasavada
"The orbital images didn't tell us what those rocks are, but now that Curiosity is getting closer, we're seeing a preview," said Curiosity Deputy Project Scientist Ashwin Vasavada of NASA's Jet Propulsion Laboratory, Pasadena, Calif.

"The contrasting textures and durabilities of sandstones in this area are fascinating.

While superficially similar, the rocks likely formed and evolved quite differently from each other."

The rocks that the Curiosity mission has studied most intensively so far are finer-grain mudstone, rather than sandstone.

The rover found evidence for an ancient lakebed environment favorable for microbial life when it analyzed sample powder drilled from mudstone last year in an area called "Yellowknife Bay."

The rover team is eager to inspect sandstone at the planned waypoint, now just 282 feet (86 meters) south of the rover.

The pause for investigations at this site might include time for collecting rock-sample material with the rover's drill, for delivery to the laboratory instruments inside the vehicle.

Monday, March 3, 2014

NASA Curiosity rover captures spectacular Mount Sharp from Junda rocks

Martian landscape scene with rows of striated rocks in the foreground and spectacular Mount Sharp on the horizon. 

NASA’s Curiosity Mars rover paused mid drive at the Junda outcrop to snap the component images for this coloured navcam camera photomosaic on Sol 548 (Feb. 19, 2014) and then continued traveling southwards towards mountain base. 

NASA’s Curiosity Mars rover's UHF Antenna are visoble on the very right of the picture. 

Credit: NASA /JPL-Caltech /Marco Di Lorenzo /Ken Kremer

Like any good tourist, NASA's rover Curiosity apparently couldn't resist the photobug urge from a gorgeous Martian mountain scene she happened by recently and decided to pull over and enjoy the view.

So she stopped the dune buggy mid-drive on the sandy road to her daily destination one Sol last week on Feb. 19, powered up the camera suite and excitedly snapped a spectacular landscape view of a striated rock field dramatically back dropped by towering Mount Sharp on the horizon.

The sedimentary foothills of Mount Sharp, which reaches 3.4 miles (5.5 km) into the Martian sky, is the 1 ton robots ultimate destination inside Gale Crater because it holds caches of water altered minerals.

And just for good measure, Curiosity also snapped a series of breathtaking look back photos showing her tracks in the dune filled terrain from whence she came since straddling through the Dingo Gap gateway.

The panoramic mountain view taken on Sol 548 shows rows of striated rocks all oriented in a similar direction in the foreground with Mount Sharp in the background.

Scientists directed Curiosity to drive by the rock rows nicknamed "Junda" after their interest was piqued by orbital images taken by the powerful telescopic camera on NASA's Mars Reconnaissance Orbiter (MRO) circling overhead.

The six wheeled rover paused during the planned Feb. 19 drive of 328 feet (100 meters) to capture the imagery.

She then pushed forward to finish the day's drive and snapped another fabulous look back view – see our mosaic below.

And the next day on Feb. 20 (Sol 549), she also completed her second 100 meter drive in reverse.

Her handlers are occasionally commanding Curiosity to drive backwards in a newly tested bid to minimize serious damage to the six 20 inch diameter wheels in the form of rips and tears caused by rough edged Red Planet rocks.

Saturday, November 16, 2013

NASA Mars Curiosity Rover: MSL, where it's been and where it's going - video


The path the Mars Science Laboratory has taken, started in the plains of the Gale crater and ultimately will makes its way through rough roads on the way to a Mount Sharp climb. 

Curiosity project scientist John Grotzinger explains.

Credit: NASA / JPL-Caltech

Thursday, July 18, 2013

NASA Mars Curiosity Rover: New software hastens trek to Mount Sharp

Mount Sharp inside Gale Crater – is the primary destination of NASA’s Curiosity rover mission to Mars since it harbors minerals to support potential life forms. 

Curiosity landed on the right side of the mountain as shown here, near the dune field colored dark blue. Mount Sharp dominates Gale Crater. 

It is 3.4 mile (5.5 km) high. Gale Crater is 154 km wide. This image was taken by the High Resolution Stereo Camera (HRSC) of ESA’s Mars Express orbiter. 

Credit: ESA/DLR/FU Berlin (G. Neukum)

NASA's 1 ton Curiosity Mars rover sets out on her epic trek to the ancient sedimentary layers at the foothills of mysterious Mount Sharp.

The science and engineering teams are diligently working right now to hasten the rovers roughly year long journey to the 3.4 mile (5.5 km) high Martian mountain – which is the mission's chief destination and holds caches of minerals that are key to sparking and sustaining life.

"We have departed Glenelg and the Shaler outcrop and started to Mount Sharp," Jim Erickson, project manager, reported.

Overall the six wheeled rover just exceeded the 1 kilometer (0.62 mile) mark in roving across the Red Planet.

Mount Sharp lies about 5 miles (8 kilometers) distant – as the Martian crow flies.

Curiosity will have to traverse across potentially treacherous dune fields on the long road ahead to the layered mountain.

"Things are going very well and we have a couple of drives under our belt," said Erickson.

Curiosity just completed more than half a year's worth of bountiful science at Glenelg and Yellowknife Bay where she discovered a habitable environment on the Red Planet with the chemical ingredients that could sustain Martian microbes- thereby already accomplishing the primary goal of NASA's flagship mission to Mars.

Curiosity's handlers are upgrading the rovers 'brain' with new driving software, making her smarter, more productive and capable than ever before, and also far more independent since her breathtaking touchdown inside Gale Crater nearly a year ago on Aug. 6, 2012.

"We continue to drive regularly. The next drive is planned tomorrow and will be executed the following day."

As of today (Sol 336, July 17), Curiosity has driven six times since leaving Glenelg on July 4 (Sol 324), totaling more than 180 meters.

Scientists specifically targeted Curiosity to Gale Crater and Mount Sharp because it is loaded with deposits of clay minerals that form in neutral water and that could possibly support the origin and evolution of simple Martian life forms, past or present.

Erickson has worked in key positions on many NASA planetary science missions dating back to Viking.

These include the Galileo mission to Jupiter, both MER rovers Spirit & Opportunity, as well as a stint with the Mars Reconnaissance Orbiter (MRO).

Friday, July 12, 2013

MARS Rover Curiosity (MSL) Heading for Mount Sharp

Image credit: NASA/JPL-Caltech

The lower slopes of Mount Sharp appear at the top of this image taken by the right Navigation Camera (Navcam) of NASA's Mars rover Curiosity at the end of a drive of about 135 feet (41 meters) during the 329th Martian day, or sol, of the rover's work on Mars (July 9, 2013). 

 That was the third drive by Curiosity since finishing observations at the mission's final science target in the "Glenelg" area east of the rover's landing site.

The planned entry point to the lower layers of Mount Sharp, the mission's next major destination, lies about 5 miles (8 kilometers) to the southwest.

The turret of tools at the end of Curiosity's robotic arm is in the foreground, with the rover's rock-sampling drill in the lower left corner of the image. 

Monday, May 6, 2013

NASA Curiosity Rover: Mars Mount Sharp Possibly Built by Wind, Not Water


Researchers based at Princeton University, the California Institute of Technology and Ashima Research suggest that Mars' roughly 3.5-mile high Mount Sharp (above) most likely emerged as strong winds carried dust and sand into Gale Crater where the mound sits. 

If correct, the research could dilute expectations that the mound is the remnant of a massive lake, which would have important implications for understanding Mars' past habitability. 

Credit: NASA/JPL-Caltech/MSSS

A roughly 3.5-mile high Martian mound that scientists suspect preserves evidence of a massive lake might actually have formed as a result of the Red Planet's famously dusty atmosphere, an analysis of the mound's features suggests.

They report in the journal Geology that air likely rises out of the massive Gale Crater when the Martian surface warms during the day, then sweeps back down its steep walls at night.

Though strong along the Gale Crater walls, these "slope winds" would have died down at the crater's center where the fine dust in the air settled and accumulated to eventually form Mount Sharp, which is close in size to Alaska's Mt. McKinley.

This dynamic counters the prevailing theory that Mount Sharp formed from layers of lakebed silt—and could mean that the mound contains less evidence of a past, Earth-like Martian climate than most scientists currently expect.

Evidence that Gale Crater once contained a lake in part determined the landing site for the NASA Mars rover Curiosity.

The rover touched down near Mount Sharp in August with the purpose of uncovering evidence of a habitable environment, and in December Curiosity found traces of clay, water molecules and organic compounds.

Determining the origin of these elements and how they relate to Mount Sharp will be a focus for Curiosity in the coming months.

But the mound itself was likely never under water, though a body of water could have existed in the moat around the base of Mount Sharp, said study co-author Kevin Lewis, a Princeton associate research scholar in geosciences and a participating scientist on the Curiosity rover mission, Mars Science Laboratory.

The quest to determine whether Mars could have at one time supported life might be better directed elsewhere, he said.

Sunday, April 28, 2013

NASA Mars Curiosity Rover Explores 'Yellowknife Bay'

The NASA Mars rover Curiosity used its left Navigation Camera (NavCam) to record this view of the step down into a shallow depression called "Yellowknife Bay." 

Image credit: NASA/JPL-Caltech

The NASA Mars rover Curiosity this week is driving within a shallow depression called "Yellowknife Bay," providing information to help researchers choose a rock to drill.

Using Curiosity's percussive drill to collect a sample from the interior of a rock, a feat never before attempted on Mars, is the mission's priority for early 2013.

After the powdered-rock sample is sieved and portioned by a sample-processing mechanism on the rover's arm, it will be analyzed by instruments inside Curiosity.

Yellowknife Bay is within a different type of terrain from what the rover has traversed since landing inside Mars' Gale Crater on Aug. 5, PDT (Aug. 6, UTC).

The terrain Curiosity has entered is one of three types that intersect at a location dubbed "Glenelg," chosen as an interim destination about two weeks after the landing.

MSL's percussive drill
Curiosity reached the lip of a 2-foot (half-meter) descent into Yellowknife Bay with a 46-foot (14-meter) drive on Dec. 11.

The next day, a drive of about 86 feet (26.1 meters) brought the rover well inside the basin.

Mast Camera (Mastcam)
The team has been employing the Mast Camera (Mastcam) and the laser-wielding Chemistry and Camera (ChemCam) for remote-sensing studies of rocks along the way.

On Dec. 14, Curiosity drove about 108 feet (32.8 meters) to reach rock targets of interest called "Costello" and "Flaherty."

Researchers used the Alpha Particle X-Ray Spectrometer (APXS) and Mars Hand Lens Imager (MAHLI) at the end of the rover's arm to examine the targets.

Mars Hand Lens Imager (MAHLI)
After finishing those studies, the rover drove again on Dec. 17, traveling about 18 feet (5.6 meters) farther into Yellowknife Bay.

That brings the mission's total driving distance to 0.42 mile (677 meters) since Curiosity's landing.

One additional drive is planned this week before the rover team gets a holiday break.

Curiosity will continue studying the Martian environment from its holiday location at the end point of that drive within Yellowknife Bay.

The mission's plans for most of 2013 center on driving toward the primary science destination, a 3-mile-high (5-kilometer) layered mound called Mount Sharp.

NASA's Mars Science Laboratory Project (MSL) is using Curiosity during a two-year prime mission to assess whether areas inside Gale Crater ever offered a habitable environment for microbes.