Mars Rover Curiosity

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Sols 928-929 Checking Out Garden City

Mon, 16 Mar 2015

By Lauren Edgar

Over the weekend, Curiosity bumped closer to the target "Garden City" located in "Artist's Drive."  "Garden City" is an intriguing target because it contains a lot of really big veins, captured here in this Mastcam image from Sol 926.

Today's plan is focused on characterizing "Garden City" and getting ready for contact science on Wednesday.  The plan includes ChemCam observations on the targets "Ouray" and "Hoskinnini" to characterize the composition of the light and dark parts of the veins, as well as several Mastcam multispectral observations.  There are also several Navcam and Mastcam activities to monitor atmospheric opacity and search for dust devils.  Furthermore, this plan includes several important SAM activities to prepare for and analyze the previously acquired "Telegraph Peak" sample.

I'll be the Geology Science Theme Lead on Wednesday so I dialed in to the planning meetings to prepare for what is shaping up to be a very busy day of arm activities!

--Lauren is a Research Geologist at the USGS Astrogeology Science Center and a member of MSL science team.

Dates of planned rover activities described in these reports are subject to change due to a variety of factors related to the Martian environment, communication relays and rover status.

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03.24.2015

Curiosity Rover Finds Biologically Useful Nitrogen on Mars

A team using the Sample Analysis at Mars (SAM) instrument suite aboard NASA's Curiosity rover has made the first detection of nitrogen on the surface of Mars from release during heating of Martian sediments.

A team using the Sample Analysis at Mars (SAM) instrument suite aboard NASA's Curiosity rover has made the first detection of nitrogen on the surface of Mars from release during heating of Martian sediments. The nitrogen was detected in the form of nitric oxide, and could be released from the breakdown of nitrates during heating. Nitrates are a class of molecules that contain nitrogen in a form that can be used by living organisms. The discovery adds to the evidence that ancient Mars was habitable for life.
Nitrogen is essential for all known forms of life, since it is used in the building blocks of larger molecules like DNA and RNA, which encode the genetic instructions for life, and proteins, which are used to build structures like hair and nails, and to speed up or regulate chemical reactions.

However, on Earth and Mars, atmospheric nitrogen is locked up as nitrogen gas (N2) - two atoms of nitrogen bound together so strongly that they do not react easily with other molecules. The nitrogen atoms have to be separated or "fixed" so they can participate in the chemical reactions needed for life. On Earth, certain organisms are capable of fixing atmospheric nitrogen and this process is critical for metabolic activity. However, smaller amounts of nitrogen are also fixed by energetic events like lightning strikes.

Nitrate (NO3) - a nitrogen atom bound to three oxygen atoms - is a source of fixed nitrogen. A nitrate molecule can join with various other atoms and molecules; this class of molecules is known as nitrates.

There is no evidence to suggest that the fixed nitrogen molecules found by the team were created by life. The surface of Mars is inhospitable for known forms of life. Instead, the team thinks the nitrates are ancient, and likely came from non-biological processes like meteorite impacts and lightning in Mars' distant past.

Features resembling dry riverbeds and the discovery of minerals that only form in the presence of liquid water suggest that Mars was more hospitable in the remote past. The Curiosity team has found evidence that other ingredients needed for life, such as liquid water and organic matter, were present on Mars at the Curiosity site in Gale Crater billions of years ago.

"Finding a biochemically accessible form of nitrogen is more support for the ancient Martian environment at Gale Crater being habitable," said Jennifer Stern of NASA's Goddard Space Flight Center in Greenbelt, Maryland. Stern is lead author of a paper on this research published online in the Proceedings of the National Academy of Science March 23.

The team found evidence for nitrates in scooped samples of windblown sand and dust at the "Rocknest" site, and in samples drilled from mudstone at the "John Klein" and "Cumberland" drill sites in Yellowknife Bay. Since the Rocknest sample is a combination of dust blown in from distant regions on Mars and more locally sourced materials, the nitrates are likely to be widespread across Mars, according to Stern. The results support the equivalent of up to 1,100 parts per million nitrates in the Martian soil from the drill sites. The team thinks the mudstone at Yellowknife Bay formed from sediment deposited at the bottom of a lake. Previously the rover team described the evidence for an ancient, habitable environment there: fresh water, key chemical elements required by life, such as carbon, and potential energy sources to drive metabolism in simple organisms.

The samples were first heated to release molecules bound to the Martian soil, then portions of the gases released were diverted to the SAM instruments for analysis. Various nitrogen-bearing compounds were identified with two instruments: a mass spectrometer, which uses electric fields to identify molecules by their signature masses, and a gas chromatograph, which separates molecules based on the time they take to travel through a small glass capillary tube -- certain molecules interact with the sides of the tube more readily and thus travel more slowly.

Along with other nitrogen compounds, the instruments detected nitric oxide (NO -- one atom of nitrogen bound to an oxygen atom) in samples from all three sites. Since nitrate is a nitrogen atom bound to three oxygen atoms, the team thinks most of the NO likely came from nitrate which decomposed as the samples were heated for analysis. Certain compounds in the SAM instrument can also release nitrogen as samples are heated; however, the amount of NO found is more than twice what could be produced by SAM in the most extreme and unrealistic scenario, according to Stern. This leads the team to think that nitrates really are present on Mars, and the abundance estimates reported have been adjusted to reflect this potential additional source.

"Scientists have long thought that nitrates would be produced on Mars from the energy released in meteorite impacts, and the amounts we found agree well with estimates from this process," said Stern.

The SAM instrument suite was built at NASA Goddard with significant elements provided by industry, university, and national and international NASA partners. NASA's Mars Science Laboratory Project is using Curiosity to assess ancient habitable environments and major changes in Martian environmental conditions. NASA's Jet Propulsion Laboratory in Pasadena, California, a division of Caltech, built the rover and manages the project for NASA's Science Mission Directorate in Washington. The NASA Mars Exploration Program and Goddard Space Flight Center provided support for the development and operation of SAM. SAM-Gas Chromatograph was supported by funds from the French Space Agency (CNES). Data from these SAM experiments are archived in the Planetary Data System.

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Changes in Scars From 2012 Mars Landing

Spacecraft that land in dusty areas of Mars create dark blast zone patterns where bright dust is blown away by the landing. Monitoring with the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter shows these dark patterns fade over time in a surprising way. Four sequences of images span two-and-a-half years beginning in the week after the August 2012 landing of NASA's Curiosity Mars rover inside Gale Crater.

The first series shows a repeating sequence of seven images of the scar where the Mars Science Laboratory's descent stage hit the ground. The descent stage, or "sky crane," had lowered Curiosity onto the ground and then flown approximately 2,100 feet (650 meters) away and impacted the ground. The fading of the dark blast zone resembles what has been observed at other Mars landing sites, presumably because bright dust is settling on the surface and masking the blast zones. Scientists thought they could model this fading and predict how long it would take for the patterns to disappear entirely. However, the most recent image, taken in February 2015, shows that this blast zone is not fading as quickly as expected, and may even be darkening. This indicates that understanding is still incomplete about processes that move dust around on the Martian surface.

Figure A is a sequence showing the spacecraft's back shell and parachute. Wind causes changes in the shape of the parachute as well as fading of the dark zone visible around the back shell in initial frames.

The Figure B sequence shows where the rover itself landed. Curiosity disappears after the first two of the seven frames because it drove away. Its wheel tracks heading generally east (toward the left) can be seen in subsequent frames, and they also fade over time.

Figure C is a five-frame sequence of the location where the spacecraft's heat shield hit the ground.

The images in these sequences have not been adjusted for differences in viewing angle or lighting conditions. Without such image processing, some features on the ground appear to shift slightly from frame to frame.

The first image in each of the four sequences is from HiRISE observation ESP_028335_1755, taken on Aug. 12, 2012, six days after Curiosity's landing. A different product from this observation, mapping where various hardware hit the ground, is at http://photojournal.jpl.nasa.gov/catalog/pia16001 . Additional image products from this observation are available at http://www.uahirise.org/ESP_028335_1755 . Subsequent images in these sequences are from HiRISE observations ESP_028401_1755, on Aug. 17, 2015; ESP_030313_1755, on Jan. 13, 2013; ESP_034572_1755, on Dec. 11, 2013; ESP_036128_1755, from April 2014; ESP_037117_1755, from June 27, 2014; and ESP_040269_1755, from February 2015. The two observations in 2014 did not include the heat shield location.

HiRISE is one of six instruments on NASA's Mars Reconnaissance Orbiter. The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.

Changes in Scars: Figure A - Backshell

This sequence of images shows a blast zone where the sky crane from NASA's Curiosity rover mission hit the ground after setting the rover down in August 2012, and how that dark scar's appearance changed over the subsequent 30 months. The images are from HiRISE on NASA's Mars Reconnaissance Orbiter.

Changes in Scars: Figure B - Curiosity Rover

This sequence of images shows a blast zone where the sky crane from NASA's Curiosity rover mission hit the ground after setting the rover down in August 2012, and how that dark scar's appearance changed over the subsequent 30 months. The images are from HiRISE on NASA's Mars Reconnaissance Orbiter.

Changes in Scars: Figure C - Heat Shield

This sequence of images shows a blast zone where the sky crane from NASA's Curiosity rover mission hit the ground after setting the rover down in August 2012, and how that dark scar's appearance changed over the subsequent 30 months. The images are from HiRISE on NASA's Mars Reconnaissance Orbiter.

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04.01.2015

NASA's Curiosity Eyes Prominent Mineral Veins on Mars

NASA's Curiosity Mars rover has climbed uphill from an outcrop it studied for six months and found a site with two-tone mineral veins forming "ice-cream sandwich" ridges.

Fast Facts:
-- Exposed mineral veins at "Garden City" tell of a wet environment after lake-bed deposits became rock
-- Drilled sample from "Telegraph Peak" contains cristobalite, a silica mineral


This view from the Mars Hand Lens Imager (MAHLI) on the arm of NASA's Curiosity Mars rover is a close-up of a two-tone mineral vein at a site called "Garden City" on lower Mount Sharp. Credit: NASA/JPL-Caltech/MSSS

Two-tone mineral veins at a site NASA's Curiosity rover has reached by climbing a layered Martian mountain offer clues about multiple episodes of fluid movement. These episodes occurred later than the wet environmental conditions that formed lake-bed deposits the rover examined at the mountain's base.
Curiosity has analyzed rock samples drilled from three targets lower on the mountain in the past seven months. It found a different mineral composition at each, including a silica mineral named cristobalite in the most recent sample. These differences, together with the prominent veins seen in images taken a little farther uphill, illustrate how the layers of Mount Sharp provide a record of different stages in the evolution of the area's ancient environment.

The two-tone veins are at the site called "Garden City." They appear as a network of ridges left standing above the now eroded-away bedrock in which they formed. Individual ridges range up to about 2.5 inches (6 centimeters) high and half that in width, and they bear both bright and dark material.

"Some of them look like ice-cream sandwiches: dark on both edges and white in the middle," said Linda Kah, a Curiosity science-team member at the University of Tennessee, Knoxville. "These materials tell us about secondary fluids that were transported through the region after the host rock formed."

Veins such as these form where fluids move through cracked rock and deposit minerals in the fractures, often affecting the chemistry of the rock surrounding the fractures. Curiosity has found bright veins composed of calcium sulfate at several previous locations. The dark material preserved here presents an opportunity to learn more. Kah said, "At least two secondary fluids have left evidence here. We want to understand the chemistry of the different fluids that were here and the sequence of events. How have later fluids affected the host rock?"

Some of the sequence is understood: Mud that formed lake-bed mudstones Curiosity examined near its 2012 landing site and after reaching Mount Sharp must have dried and hardened before the fractures formed. The dark material that lines the fracture walls reflects an earlier episode of fluid flow than the white, calcium-sulfate-rich veins do, although both flows occurred after the cracks formed.

Garden City is about 39 feet (12 meters) higher than the bottom edge of the "Pahrump Hills" outcrop of the bedrock forming the basal layer of Mount Sharp, at the center of Mars' Gale Crater. The Curiosity mission spent about six months examining the first 33 feet (10 meters) of elevation at Pahrump Hills, climbing from the lower edge to higher sections three times to vertically profile the rock structures and chemistry, and to select the best targets for drilling.

"We investigated Pahrump Hills the way a field geologist would, looking over the whole outcrop first to choose the best samples to collect, and it paid off," said David Blake of NASA's Ames Research Center, Moffett Field, California, principal investigator for the Chemistry and Mineralogy (CheMin) analytical laboratory instrument inside the rover.

Analysis is still preliminary, but the three drilled samples from Pahrump Hills have clear differences in mineral ingredients. The first, "Confidence Hills," had the most clay minerals and hematite, both of which commonly form under wet conditions. The second, "Mojave," had the most jarosite, an oxidized mineral containing iron and sulfur that forms in acidic conditions. The third is "Telegraph Peak." Examination of Garden City has not included drilling a sample.

Blake said, "Telegraph Peak has almost no evidence of clay minerals, the hematite is nearly gone and jarosite abundance is down. The big thing about this sample is the huge amount of cristobalite, at about 10 percent or more of the crystalline material." Cristobalite is a mineral form of silica. The sample also contains a small amount of quartz, another form of silica. Among the possibilities are that some process removed other ingredients, leaving an enrichment of silica behind; or that dissolved silica was delivered by fluid transport; or that the cristobalite formed elsewhere and was deposited with the original sediment.

NASA's Mars Science Laboratory Project is using Curiosity to examine environments that offered favorable conditions for microbial life on ancient Mars, if the planet ever has hosted microbes, and the changes from those environments to drier conditions that have prevailed on Mars for more than three billion years.

After investigations in the Telegraph Peak area, the rover team plans to drive Curiosity through a valley called "Artist's Drive" to reach higher layers. Engineers are meanwhile developing guidelines for best use of the rover's drill, following detection of a transient short circuit last month while using the tool's percussion action to shake rock powder into a sample-processing device. Drilling can use both rotary and percussion actions.

"We expect to use percussion as part of drilling in the future while we monitor whether shorts become more frequent," said Steve Lee of NASA's Jet Propulsion Laboratory, Pasadena, California. Lee became deputy project manager for the Mars Science Laboratory Project this month. He previously led the project's Guidance, Navigation and Control Team from design through landing.

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04.16.2015

NASA's Curiosity Rover Making Tracks and Observations

Fast Facts:
-- Curiosity has passed the mission's 10-kilometer mark as it heads for its next science destination, called "Logan Pass"
-- The rover is approaching a corrugated geological unit that overlies the layers examined by Curiosity

NASA's Curiosity Mars rover is continuing science observations while on the move this month. On April 16, the mission passed 10 kilometers (6.214 miles) of total driving since its 2012 landing, including about a fifth of a mile (310 meters) so far this month.
The rover is trekking through a series of shallow valleys between the "Pahrump Hills" outcrop, which it investigated for six months, and the next science destination, "Logan Pass," which is still about 200 yards, or meters, ahead toward the southwest.

"We've not only been making tracks, but also making important observations to characterize rocks we're passing, and some farther to the south at selected viewpoints," said John Grant of the National Air and Space Museum, Washington. Grant is a Curiosity science team member who has been the team's long-term planner in recent days.

A drive of 208 feet (63.5 meters) during the mission's 957th Martian day, early Thursday, took Curiosity past a cumulative 10 kilometers of total Martian ground-distance covered. This is based on mapped distance covered by each drive; by wheel odometery, the rover reached 10 kilometers last week, but the mapped tally is considered a more precise measure of distance covered, excluding wheel slippage.

Curiosity is examining the lower slopes of a layered mountain, Mount Sharp, to investigate how the region's ancient environment evolved from lakes and rivers to much drier conditions. Sites at Pahrump Hills exposed the mountain's basal geological layer, named the Murray formation. Nearby, high-standing buttes are examples of terrain called the Washboard unit, from its corrugated appearance as seen from orbit.

"The trough we're driving through is bounded by exposures of the Washboard unit, with gaps at some places that allow us to see farther south to higher exposures of it," Grant said. "At Logan Pass, we hope to investigate the relationship between the Murray formation and the Washboard unit, to help us understand the ancient depositional setting and how environmental conditions were changing. The observations we're making now help establish the context for what we'll see there."

"The rover's mobility has been crucial, because that's what allows us to get to the best sites to investigate," Grant said. "The ability to get to different sections of the rock record builds more confidence in your interpretation of each section."

From observations made by NASA's Mars Reconnaissance Orbiter, topographically ridged terrain that has beenategorized as the Washboard unit has been mapped at many locations around Mount Sharp -- on the south flank of the mountain as well as the northern flank Curiosity is climbing -- and on the surrounding plains.

"Understanding the Washboard unit and what processes formed it could put what we've been studying into a wider context," Grant said.

Curiosity spent much of its first 12 months on Mars investigating locations close to its landing site north of Mount Sharp. Findings during that period included evidence for ancient rivers and a lakebed environment that offered conditions favorable for microbial life, if Mars has ever hosted life. After leaving the landing vicinity, Curiosity drove to reach Mount Sharp, with a few extended stops at science waypoints along the route before arriving in September 2014.

NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, built the rover and manages the project for NASA's Science Mission Directorate in Washington. For more information about Curiosity, visit:

http://www.nasa.gov/msl
http://mars.nasa.gov/msl/

04.16.2015

Curiosity's Position After 10 Kilometers

A green star marks the location of NASA's Curiosity Mars rover after a drive on the mission's 957th Martian day, or sol, (April 16, 2015). The map covers an area about 1.25 miles (2 kilometers) wide.

Curiosity landed on Mars in August 2012. The drive on Sol 957 brought the mission's total driving distance past the 10-kilometer mark (6.214 miles). The rover is passing through a series of shallow valleys on a path from the "Pahrump Hills" outcrop, which it investigated for six months, toward its next science destination, called "Logan Pass."

The rover's traverse line enters this map at the location Curiosity reached in mid-July 2014.

The base map uses imagery from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.

More information about Curiosity is online at http://www.nasa.gov/msl and http://mars.nasa.gov/msl/.

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Tough environment... below is wheel wear and tear to date...

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Some stratified rock outcrops... 

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https://www.youtube.com/v/MLFwOBnyvio

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05.08.2015

Quick Detour by NASA Mars Rover Checks Ancient Valley

Researchers slightly detoured NASA's Curiosity Mars rover from the mission's planned path in recent days for a closer look at a hillside site where an ancient valley had been carved out and refilled.
The rover made observations and measurements there to address questions about how the channel formed and filled. Then it resumed driving up Mount Sharp, where the mission is studying the rock layers. The layers reveal chapters in how environmental conditions and the potential to support microbial life changed in Mars' early history.

Two new panoramas of stitched-together telephoto images from Curiosity's Mast Camera (Mastcam) present the increasingly hilly region the rover has been investigating, and more distant portions of Mount Sharp. These large images are online, with pan and zoom controls for exploring them, at:

mars.nasa.gov/msl/multimedia/deepzoom/PIA19397
mars.nasa.gov/msl/multimedia/deepzoom/PIA19398

Curiosity's Path to Some Spring 2015 Study Sites




Curiosity has been exploring on Mars since 2012. It reached the base of Mount Sharp last year after fruitfully investigating outcrops closer to its landing site and then trekking to the mountain. The main mission objective now is to examine successively higher layers of Mount Sharp. Curiosity spent several months examining the lowest levels of the mountain's basal geological unit, the Murray formation, at an outcrop called "Pahrump Hills." Then it set off toward a site called "Logan Pass," where the team anticipates a first chance to place the contact-science instruments at the end of the rover's arm onto a darker geological unit overlying or within the Murray formation.
"In pictures we took on the way from Pahrump Hills toward Logan Pass, some of the geologists on the team noticed a feature that looked like what's called an 'incised valley fill,' which is where a valley has been cut into bedrock and then filled in with other sediment," said Curiosity Project Scientist Ashwin Vasavada of NASA's Jet Propulsion Laboratory, Pasadena, California.

This unusual geometry of the rock layers was noted on the side of a rise called "Mount Shields," which sits northwest of the planned route to Logan Pass. The team chose in late April to divert the rover to the base of Mount Shields.

"We wanted to investigate what cut into the mudstone bedrock, and what process filled it back in," Vasavada said. "The fill material looks like sand. Was the sand transported by wind or by water? What were the relative times for when the mudstone formed, when the valley was cut into it, when the cut was filled in?

"It's exciting to see this on Mars for the first time," he continued. "Features like this on Earth capture evidence of change. What in the environment changed to go from depositing one kind of sediment, to eroding it away in a valley, to then depositing a different kind of sediment? It's a fascinating puzzle that Mars has left for us."

Scientists are examining the evidence collected at Mount Shields as the rover approaches its next study area, at Logan Pass.

JPL, a division of the California Institute of Technology in Pasadena, built the rover and manages the project for NASA's Science Mission Directorate in Washington. For more information about Curiosity, visit:

http://www.nasa.gov/msl
http://mars.nasa.gov/msl/

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05.08.2015

Sunset in Mars' Gale Crater

NASA's Curiosity Mars rover recorded this sequence of views of the sun setting at the close of the mission's 956th Martian day, or sol (April 15, 2015), from the rover's location in Gale Crater.

The four images shown in sequence here were taken over a span of 6 minutes, 51 seconds.

This was the first sunset observed in color by Curiosity. The images come from the left-eye camera of the rover's Mast Camera (Mastcam). The color has been calibrated and white-balanced to remove camera artifacts. Mastcam sees color very similarly to what human eyes see, although it is actually a little less sensitive to blue than people are.

Dust in the Martian atmosphere has fine particles that permit blue light to penetrate the atmosphere more efficiently than longer-wavelength colors. That causes the blue colors in the mixed light coming from the sun to stay closer to sun's part of the sky, compared to the wider scattering of yellow and red colors. The effect is most pronounced near sunset, when light from the sun passes through a longer path in the atmosphere than it does at mid-day.

Malin Space Science Systems, San Diego, built and operates the rover's Mastcam. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology, Pasadena, manages the Mars Science Laboratory Project for NASA's Science Mission Directorate, Washington. JPL designed and built the project's Curiosity rover. For more information about Curiosity, visit http://www.nasa.gov/msl and http://mars.nasa.gov/msl.

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By Lauren Edgar

On Sol 992 Curiosity took a short drive into Marias Pass to get a better look at the terrain ahead.  The 6 m drive on Sol 992 brought our total odometry to 10,562 m.  It also put Curiosity in a great position for targeted science over the long holiday weekend.

The 4 sol plan includes some large Mastcam mosaics to characterize the terrain and the contact between the Stimson and Pahrump units.  The plan also includes ChemCam and Mastcam observations on the targets "Hoodoo," "Pinehaven," "Red Sleep," and "Red Horn" to assess the composition of the bright outcrop and veins.  On Sol 995, Curiosity will bump closer to the outcrop, to prepare for possible contact science next week.  Curiosity will also acquire several Mastcam observations of Deimos and stars to assess the nighttime atmospheric opacity.  Sol 996 will be a "REMS-a-palooza" devoted entirely to extended environmental monitoring.

--Lauren is a Research Geologist at the USGS Astrogeology Science Center and a member of MSL science team.

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Sol 998: Contact Science at Marias Pass

Wed, 27 May 2015

By Lauren Edgar

A short bump on Sol 997 put Curiosity in a great position to investigate a few different rock units in Marias Pass, using the instruments on the rover's arm.  The 2.5 m drive brings our total odometry to 10,599 m.  With the upcoming solar conjunction (Mars will be on the opposite side of the sun from the Earth, so we can't communicate with the rover for most of the month of June), Curiosity is now parked for the next few weeks.   But we are parked in front of a beautiful outcrop that shows the contact between the underlying Pahrump unit and the overlying Stimson unit.

The goal of today's plan is to characterize the Stimson unit.  First, Curiosity will acquire ChemCam and Mastcam on part of the Stimson unit called "Ronan" (the large block in the top part of this Mastcam image) as well as a coarse-grained block named "Big_Arm."  Then we'll acquire several MAHLI images on "Ronan."  Next, Curiosity will brush "Ronan" to remove the dust, and will then take MAHLI images of the brushed area to get a better look at the grain size and textures.  And finally, we'll place APXS on the target to investigate the bulk chemistry of "Ronan."  Tomorrow's plan will likely include similar observations on the Pahrump unit.

--Lauren is a Research Geologist at the USGS Astrogeology Science Center and a member of MSL science team.

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Mars has passed behind the sun and will not emerge until the end of June.  The rovers Curiosity and Opportunity will have very minimal activity and communications will be sparse...

Sols 1003-1004: Last tactical planning before solar conjunction

Mon, 01 Jun 2015



Today is the last day of MSL tactical operations until after solar conjunction, so this will probably be the last MSL update for a few weeks.  Ryan Anderson and I are both on shift as payload uplink lead today, but because the instruments we're representing (ChemCam and MAHLI/MARDI, respectively) are already standing down in preparation for conjunction, our efforts have been focused on planning for the resumption of activities after conjunction.  We don't know precisely when tactical planning will resume, as the ability to communicate with spacecraft as Mars passes behind the Sun depends on variable solar activity.  The expectation is that the next tactical planning day will be June 25th (Sol 1026), but the schedule probably won't firm up until that week. 

The Sol 1003 plan starts with Mastcam images of the Sun to measure the amount of dust in the atmosphere, followed by another set of Mastcam/Navcam photometry images to extend the experiment started on Sol 1000.  Then Mastcam will take images of various targets near the rover, to be compared with images of the same targets taken after conjunction to look for changes caused by winds.  Later in the afternoon, the photometry and change-detection imaging will be repeated, and Mastcam will acquire a stereo mosaic of "Apikuni Mountain."   Then the focus motors of both Mastcams will be moved to their "home" positions for conjunction and Navcam will search for clouds above MSL.  The Sol 1004 plan includes only the usual RAD and REMS observations, a preview of the plan for the next few weeks.  During the break from tactical operations, the science team will have more time to analyze the wealth of data the rover has returned over the past 1000 sols.

by Ken Herkenhoff

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I have been a proponent of a laser based comm grid that rotates above and below the ecliptic that works similar to a internet router.

This way, no matter what spatial body goes into solar occlusion we will still be able to communicate.

There was a project to build something similar for the Constellation Project but it was only for Terran/Martian links.

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Mars has passed through solar conjunction, and reliable communication with the spacecraft at Mars is possible again.  As planning started this morning, we were still waiting for more data to be relayed by the orbiters to confirm that MSL is ready to resume science planning, but proceeded with tactical planning so that we would be ready when the data arrived.  The Sol 1027 plan starts with Mastcam observations of several targets that were imaged just before solar conjunction, to look for changes caused by winds or maybe Marsquakes.  Mastcam will then look at the sun to measure the amount of dust in the atmosphere, Navcam will search for dust devils, and ChemCam/Mastcam will observe nearby targets "Piegan" and "Wallace."  On Sol 1028, the arm will be used to take MAHLI images of the rocks and soil in front of the rover from various vantage points, to measure changes in their reflectance with observation geometry ("photometry").  After dusk, APXS and MAHLI will measure 3 spots on a rock called "Big Arm" that was imaged by MAHLI during the day before solar conjunction.  The nighttime images, using MAHLI's LEDs for illumination, should nicely complement the daytime images of the rock.  Finishing off the weekend plan, on Sol 1029 ChemCam will acquire some calibration data and Mastcam will take a stereo mosaic of the outcrops to the east of the rover. 

As SOWG Chair today, I was a bit worried about planning so many activities on the first day of tactical planning in a few weeks, but the team hit the ground running and did a great job.  Early this afternoon, we got word from the downlink team that the data acquired during conjunction show that the rover is in good health, and that we were therefore "go" for planning.  MSL is back in action!

by Ken Herkenhoff