Updates Mars Science Laboratory (Curiosity)

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Universe Today: Curiosity Shows Off Its Credentials

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Plaque on the exterior of Mars Science Laboratory, aka “Curiosity” (NASA/JPL-Caltech/MSSS)


690461main_pia15882_Flag_FINAL-43_946-710.jpg

Curiosity’s “stars and stripes” American flag mobility logo (NASA/JPL-Caltech/MSSS)​
 

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NASA / NASA JPL:
Curiosity Finishes Close Inspection of Rock Target

September 24, 2012

Mars Science Laboratory Mission Status Report

PASADENA, Calif. -- NASA's rover Curiosity touched a Martian rock with its robotic arm for the first time on Sept. 22, assessing what chemical elements are in the rock called "Jake Matijevic."

After a short drive the preceding day to get within arm's reach of the football-size rock, Curiosity put its Alpha Particle X-Ray Spectrometer (APXS) instrument in contact with the rock during the rover's 46th Martian day, or sol. The APXS is on a turret at the end of the rover's 7-foot (2.1-meter) arm. The Mars Hand Lens Imager (MAHLI), on the same turret, was used for close-up inspection of the rock. Both instruments were also used on Jake Matijevic on Sol 47 (Sept. 23).

{colsp=2}
Click on images for details​
| This image combines photographs taken by the Mars Hand Lens Imager (MAHLI) at three different distances from the first Martian rock that NASA's Curiosity rover touched with its arm.
Image credit: NASA/JPL-Caltech/MSSS​
| This image shows the robotic arm of NASA's Mars rover Curiosity with the first rock touched by an instrument on the arm.
Image credit: NASA/JPL-Caltech​
This engineering animation depicts the moves that NASA's rover Curiosity made on Sept. 22, 2012, when the rover touched a Martian rock with its robotic arm for the first time.


The Chemistry and Camera (ChemCam) instrument, which shoots laser pulses at a target from the top of Curiosity's mast, also assessed what chemical elements are in the rock Jake Matijevic. Using both APXS and ChemCam on this rock provides a cross calibration of the two instruments.

With a final ChemCam laser testing of the rock on Sol 48 (Sept. 24), Curiosity finished its work on Jake Matijevic. The rover departed the same sol, with a drive of about 138 feet (42 meters), its longest yet. Sol 48, in Mars local mean solar time at Gale Crater, ended at 3:09 p.m. Sept. 24, PDT.

{...}



SPACE.com: Curiosity Rover Touches 1st Martian Rock, Makes Longest Drive Yet
 

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42 meters in one day is not bad at all, really :thumbup:
 

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Phobos really deserves its name there !
 

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Stream-bed on Mars!

WOAH, THIS IS BIG NEWS! :jawdrops:

RELEASE: 12-338

NASA ROVER FINDS OLD STREAMBED ON MARTIAN SURFACE

PASADENA, Calif. -- NASA's Curiosity rover mission has found evidence
a stream once ran vigorously across the area on Mars where the rover
is driving. There is earlier evidence for the presence of water on
Mars, but this evidence - images of rocks containing ancient
streambed gravels - is the first of its kind.

Scientists are studying the images of stones cemented into a layer of
conglomerate rock. The sizes and shapes of stones offer clues to the
speed and distance of a long-ago stream's flow.

"From the size of gravels it carried, we can interpret the water was
moving about 3 feet per second, with a depth somewhere between ankle
and hip deep," said Curiosity science co-investigator William
Dietrich of the University of California, Berkeley. "Plenty of papers
have been written about channels on Mars with many different
hypotheses about the flows in them. This is the first time we're
actually seeing water-transported gravel on Mars. This is a
transition from speculation about the size of streambed material to
direct observation of it."

The finding site lies between the north rim of Gale Crater and the
base of Mount Sharp, a mountain inside the crater. Earlier imaging of
the region from Mars orbit allows for additional interpretation of
the gravel-bearing conglomerate. The imagery shows an alluvial fan of
material washed down from the rim, streaked by many apparent
channels, sitting uphill of the new finds.

The rounded shape of some stones in the conglomerate indicates
long-distance transport from above the rim, where a channel named
Peace Vallis feeds into the alluvial fan. The abundance of channels
in the fan between the rim and conglomerate suggests flows continued
or repeated over a long time, not just once or for a few years.

The discovery comes from examining two outcrops, called "Hottah" and
"Link" with the telephoto capability of Curiosity's mast camera
during the first 40 days after landing. Those observations followed
up on earlier hints from another outcrop, which was exposed by
thruster exhaust as Curiosity, the Mars Science Laboratory Project's
rover, touched down.

"Hottah looks like someone jack-hammered up a slab of city sidewalk,
but it's really a tilted block of an ancient streambed," said Mars
Science Laboratory Project Scientist John Grotzinger of the
California Institute of Technology in Pasadena.

The gravels in conglomerates at both outcrops range in size from a
grain of sand to a golf ball. Some are angular, but many are rounded.

"The shapes tell you they were transported and the sizes tell you they
couldn't be transported by wind. They were transported by water
flow," said Curiosity science co-investigator Rebecca Williams of the
Planetary Science Institute in Tucson, Ariz.

The science team may use Curiosity to learn the elemental composition
of the material, which holds the conglomerate together, revealing
more characteristics of the wet environment that formed these
deposits. The stones in the conglomerate provide a sampling from
above the crater rim, so the team may also examine several of them to
learn about broader regional geology.

The slope of Mount Sharp in Gale Crater remains the rover's main
destination. Clay and sulfate minerals detected there from orbit can
be good preservers of carbon-based organic chemicals that are
potential ingredients for life.

"A long-flowing stream can be a habitable environment," said
Grotzinger. "It is not our top choice as an environment for
preservation of organics, though. We're still going to Mount Sharp,
but this is insurance that we have already found our first
potentially habitable environment."

During the two-year prime mission of the Mars Science Laboratory,
researchers will use Curiosity's 10 instruments to investigate
whether areas in Gale Crater have ever offered environmental
conditions favorable for microbial life.

For more about Curiosity, visit:

http://www.nasa.gov/msl
 

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NASA / NASA JPL:
NASA Rover Finds Old Streambed on Martian Surface

September 27, 2012

PASADENA, Calif. -- NASA's Curiosity rover mission has found evidence a stream once ran vigorously across the area on Mars where the rover is driving. There is earlier evidence for the presence of water on Mars, but this evidence -- images of rocks containing ancient streambed gravels -- is the first of its kind.

Scientists are studying the images of stones cemented into a layer of conglomerate rock. The sizes and shapes of stones offer clues to the speed and distance of a long-ago stream's flow.

"From the size of gravels it carried, we can interpret the water was moving about 3 feet per second, with a depth somewhere between ankle and hip deep," said Curiosity science co-investigator William Dietrich of the University of California, Berkeley. "Plenty of papers have been written about channels on Mars with many different hypotheses about the flows in them. This is the first time we're actually seeing water-transported gravel on Mars. This is a transition from speculation about the size of streambed material to direct observation of it."

The finding site lies between the north rim of Gale Crater and the base of Mount Sharp, a mountain inside the crater. Earlier imaging of the region from Mars orbit allows for additional interpretation of the gravel-bearing conglomerate. The imagery shows an alluvial fan of material washed down from the rim, streaked by many apparent channels, sitting uphill of the new finds.

{colsp=2}
Click on images for details​
|
Remnants of Ancient Streambed on Mars
NASA's Curiosity rover found evidence for an ancient, flowing stream on Mars at a few sites, including the rock outcrop pictured here, which the science team has named "Hottah" after Hottah Lake in Canada's Northwest Territories.
Image credit: NASA/JPL-Caltech/MSSS​
|
Curiosity's Roadside Discoveries
This map shows the path on Mars of NASA's Curiosity rover toward Glenelg, an area where three terrains of scientific interest converge.
Image credit: NASA/JPL-Caltech/Univ. of Arizona​
|
Where Water Flowed Downslope
This image shows the topography, with shading added, around the area where NASA's Curiosity rover landed on Aug. 5 PDT (Aug. 6 EDT).
Image credit: NASA/JPL-Caltech/UofA​
|
Downslope of the Fan
This false-color map shows the area within Gale Crater on Mars, where NASA's Curiosity rover landed on Aug. 5, 2012 PDT (Aug. 6, 2012 EDT).
Image credit: NASA/JPL-Caltech/ASU​


The rounded shape of some stones in the conglomerate indicates long-distance transport from above the rim, where a channel named Peace Vallis feeds into the alluvial fan. The abundance of channels in the fan between the rim and conglomerate suggests flows continued or repeated over a long time, not just once or for a few years.

The discovery comes from examining two outcrops, called "Hottah" and "Link," with the telephoto capability of Curiosity's mast camera during the first 40 days after landing. Those observations followed up on earlier hints from another outcrop, which was exposed by thruster exhaust as Curiosity, the Mars Science Laboratory Project's rover, touched down.

{colsp=2}
Click on images for details​
|
Best View of Goulburn Scour
This image from NASA's Curiosity Rover shows a high-resolution view of an area that is known as Goulburn Scour, a set of rocks blasted by the engines of Curiosity's descent stage on Mars.
Image credit: NASA/JPL-Caltech/MSSS​
|
Link to a Watery Past
In this image from NASA's Curiosity rover, a rock outcrop called Link pops out from a Martian surface that is elsewhere blanketed by reddish-brown dust.
Image credit: NASA/JPL-Caltech/MSSS​
|
Rock Outcrops on Mars and Earth
This set of images compares the Link outcrop of rocks on Mars (left) with similar rocks seen on Earth (right).
Image credit: NASA/JPL-Caltech/MSSS and PSI​
|
Dry Streambed on Alluvial Fan in Northern Chile
This image shows a dry streambed on an alluvial fan in the Atacama Desert, Chile, revealing the typical patchy, heterogeneous mixture of grain sizes deposited together.
Image credit: UC Berkeley​


"Hottah looks like someone jack-hammered up a slab of city sidewalk, but it's really a tilted block of an ancient streambed," said Mars Science Laboratory Project Scientist John Grotzinger of the California Institute of Technology in Pasadena.

The gravels in conglomerates at both outcrops range in size from a grain of sand to a golf ball. Some are angular, but many are rounded.

"The shapes tell you they were transported and the sizes tell you they couldn't be transported by wind. They were transported by water flow," said Curiosity science co-investigator Rebecca Williams of the Planetary Science Institute in Tucson, Ariz.

The science team may use Curiosity to learn the elemental composition of the material, which holds the conglomerate together, revealing more characteristics of the wet environment that formed these deposits. The stones in the conglomerate provide a sampling from above the crater rim, so the team may also examine several of them to learn about broader regional geology.

The slope of Mount Sharp in Gale Crater remains the rover's main destination. Clay and sulfate minerals detected there from orbit can be good preservers of carbon-based organic chemicals that are potential ingredients for life.

"A long-flowing stream can be a habitable environment," said Grotzinger. "It is not our top choice as an environment for preservation of organics, though. We're still going to Mount Sharp, but this is insurance that we have already found our first potentially habitable environment."

{...}



NASA News Release: RELEASE : 12-338 - NASA Rover Finds Old Streambed On Martian Surface

SpaceRef: Remnants of Ancient Streambed Discovered on Mars

SPACE.com:
Universe Today: Curiosity Finds Evidence of An Ancient Streambed on Mars

Aviation Week: Curiosity Finds Evidence Of Flowing Water On Mars

CBS News Space: Mars rover finds ancient streambed frozen in conglomerate rock

Florida Today:
Discovery News: Mars Rover Finds Bed of Ancient Flowing Stream

RIA Novosti: Mars Rover Curiosity Finds Old Streambed
 

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The media briefing about the discovery from NASAtelevision:
 

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NASA / NASA JPL:
NASA Mars Curiosity Rover Prepares to Study Martian Soil

October 04, 2012

PASADENA, Calif. -- NASA's Curiosity rover is in a position on Mars where scientists and engineers can begin preparing the rover to take its first scoop of soil for analysis.

Curiosity is the centerpiece of the two-year Mars Science Laboratory mission. The rover's ability to put soil samples into analytical instruments is central to assessing whether its present location on Mars, called Gale Crater, ever offered environmental conditions favorable for microbial life. Mineral analysis can reveal past environmental conditions. Chemical analysis can check for ingredients necessary for life.

"We now have reached an important phase that will get the first solid samples into the analytical instruments in about two weeks," said Mission Manager Michael Watkins of NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Curiosity has been so well-behaved that we have made great progress during the first two months of the mission."

{colsp=3}
Click on images for details​
| |
Wheel Scuff Mark at 'Rocknest'
NASA's Mars rover Curiosity cut a wheel scuff mark into a wind-formed ripple at the "Rocknest" site to give researchers a better opportunity to examine the particle-size distribution of the material forming the ripple.
Image Credit: NASA/JPL-Caltech​
|
Curiosity's Travels Through Sol 56
This map shows the route driven by NASA's Mars rover Curiosity through the 56th Martian day, or sol, of the rover's mission on Mars (Oct. 2, 2012).
Image Credit: NASA/JPL-Caltech/Univ. of Arizona​
|
View on the Way to 'Glenelg'
This 360-degree panorama from NASA's Mars rover Curiosity shows the rocky terrain surrounding it as of its 55th Martian day, or sol, of the mission (Oct. 1, 2012). The base of Mount Sharp can be seen at upper left.
Image Credit: NASA/JPL-Caltech​
| |
'Rocknest' From Sol 52 Location
This patch of windblown sand and dust downhill from a cluster of dark rocks is the "Rocknest" site, which has been selected as the likely location for first use of the scoop on the arm of NASA's Mars rover Curiosity.
Image credit: NASA/JPL-Caltech/MSSS​
|
CHIMRA: Scoops, Sieves and Delivers Samples
This false-color engineering drawing shows the Collection and Handling for In-Situ Martian Rock Analysis (CHIMRA) device, attached to the turret at the end of the robotic arm on NASA's Curiosity Mars rover.
Image Credit: NASA/JPL-Caltech​
|
Internal Chambers of CHIMRA
This cutaway view shows the internal chambers of the Collection and Handling for In-Situ Martian Rock Analysis (CHIMRA) device, attached to the turret at the end of the robotic arm on NASA's Curiosity Mars rover.
Image Credit: NASA/JPL-Caltech​


The rover's preparatory operations will involve testing its robotic scooping capabilities to collect and process soil samples. Later, it also will use a hammering drill to collect powdered samples from rocks. To begin preparations for a first scoop, the rover used one of its wheels Wednesday to scuff the soil to expose fresh material.

Next, the rover twice will scoop up some soil, shake it thoroughly inside the sample-processing chambers to scrub the internal surfaces, then discard the sample. Curiosity will scoop and shake a third measure of soil and place it in an observation tray for inspection by cameras mounted on the rover's mast. A portion of the third sample will be delivered to the mineral-identifying chemistry and mineralogy (CheMin) instrument inside the rover. From a fourth scoopful, samples will be delivered to both CheMin and to the sample analysis at Mars (SAM) instrument, which identifies chemical ingredients.

"We're going to take a close look at the particle size distribution in the soil here to be sure it's what we want," said Daniel Limonadi of JPL, lead systems engineer for Curiosity's surface sampling and science system. "We are being very careful with this first time using the scoop on Mars."

The rinse-and-discard cycles serve a quality-assurance purpose similar to a common practice in geochemical laboratory analysis on Earth.

"It is standard to run a split of your sample through first and dump it out, to clean out any residue from a previous sample," said JPL's Joel Hurowitz, a sampling system scientist on the Curiosity team. "We want to be sure the first sample we analyze is unambiguously Martian, so we take these steps to remove any residual material from Earth that might be on the walls of our sample handling system."

Rocknest is the name of the area of soil Curiosity will test and analyze. The rover pulled up to the windblown, sandy and dusty location Oct. 2. The Rocknest patch is about 8 feet by 16 feet (2.5 meters by 5 meters). The area provides plenty of area for scooping several times. Diverse rocks nearby provide targets for investigation with the instruments on Curiosity's mast during the weeks the rover is stationed at Rocknest for this first scooping campaign.

Curiosity's motorized, clamshell-shaped scoop is 1.8 inches (4.5 centimeters) wide, 2.8 inches (7 centimeters) long, and can sample to a depth of about 1.4 inches (3.5 centimeters). It is part of the collection and handling Martian rock analysis (CHIMRA) device on a turret of tools at the end of the rover's arm. CHIMRA also includes a series of chambers and labyrinths for sorting, sieving and portioning samples collected by the scoop or by the arm's percussive drill.

Following the work at Rocknest, the rover team plans to drive Curiosity about 100 yards (about 100 meters) eastward into the Glenelg area and select a rock as the first target for use of its drill.

{...}



NASA News Release: RELEASE : 12-348 - NASA Mars Curiosity Rover Prepares to Study Martian Soil

SpaceRef: Curiosity Prepares to Study Martian Soil

SPACE.com: Curiosity Rover to Scoop Up 1st Mars Samples This Weekend

The Planetary Society Blog: Curiosity Update, sol 57: Digging in at Rocknest

CBS News Space: Curiosity gets the scoop on Mars

Science Daily: NASA Mars Curiosity Rover Prepares to Study Martian Soil

Discovery News: Mars Rover Ready to Scoop Sand: Big Pic

Universe Today: Curiosity Set for 1st Martian Scooping at ‘Rocknest’ Ripple
 

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[ame="http://www.youtube.com/watch?v=I5b6KSTst-o"]Curiosity Report (Oct. 4, 2012): Rover Gets Set to Scoop - YouTube[/ame]
 

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I wonder why the MSL team did not spent more time at that ancient stream bed? "Hottah"
They just take some amazing photos and that is it.
In my perspective, the gravels in the conglomerates they found, is very important to study extensively.
To my knowledge they did not even used the chemcam laser to study the elements in that outcrop.
Another issue that bother me is the "link" discovery.
If I understand correctly, they already photographed the link outcrop with the 100-millimeter Mast Camera on Sept. 2, 2012, which was the 27th sol, or Martian day of operations.
But they announced it much later on sol 39.
Anyway, it looks like MSL is in for extensive science in Gale crater.
I try to imagine what it looked like when that water steam flowed on Mars some time ago.
It is hard to believe that that site is dead and arid as showed in the images.
Is it possible for fossils (if present on Mars at all) to be preserved in that conglomerate sedimentary like here on Earth?

(I apologize for my crude English)
 
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I wonder why the MSL team did not spent more time at that ancient stream bed?

Simply because the primary goal of the mission is investigating Aeolis Mons, which is now considered even more interesting. The primary mission has a tight schedule.

It is possible to return to the streambeds, once the extended mission starts.

Also, you should remember that Mars also has seasons and weather, while Curiosity isn't as sensitive to the season as the previous rovers, it still can be negatively affected when temperatures drop and dust storms roam over the country, especially when trying to scale a 5 km mountain on Mars (if you think this is easy, try getting on the much smaller Kilimandjaro, you might be surprised). This will be even more important once humans will explore Mars.

Exploration is no pony club.
 
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Well, the way I see it is that everyone is going to want to look here and there and everywhere. We're all gonna wanna see everything, but there is a schedule to follow and the guys in command are calling the shots.

I bet there are guys on the team wanting to do the same thing. This is only one rover and can't get to everything!
 
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