Sols 4246-4247: Next Stop: Fairview Dome

Sols 4246-4247: Next Stop: Fairview Dome

2 min read

Sols 4246-4247: Next Stop: Fairview Dome

A grayscale photograph of the Martian surface from the Curiosity rover captures parts of the rover in the bottom half of the frame, including a crosspiece imprinted with its name and a line drawing of Curiosity. Ahead of the rover, rough, pebbly terrain in various shades of medium gray fills the rest of the frame, with scattered light gray rocks poking out of the soil. A medium-sized rock at upper left, the focus of the rover's attention, resembles a medium gray pita sandwich sitting upright on the ground.
This image was taken by Left Navigation Camera onboard NASA’s Mars rover Curiosity on sol 4244 – Martian day 4,244 of the Mars Science Laboratory mission – July 14, 2024, at 21:12:47 UTC. The grooved rock at upper left in the image, in line between the rover and the lighter-colored, rectangular rock, has been nicknamed “Jack Main Canyon” and deemed a compelling science target for Curiosity to study.

Earth planning date: Monday, July 15, 2024

Summer is in full swing in the northern hemisphere here on Earth. Warmer temperatures and fair weather make for prime opportunities for road trips and enjoying the best of the outdoors. Summer is in full swing too for the southern hemisphere of Mars and Gale crater, where Curiosity is continuing its mini (make-your-own) road trip to “Fairview Dome.”

Recent exciting stops saw Curiosity enjoy “ice cream” and take a moment to “vug out” (imagination required as to what vuggin’ out could mean in the sense of a road trip!). The workspace Curiosity presented to the science team today did not leave many options for APXS and MAHLI. The team did ultimately decide on a suitable and compelling target to deploy Curiosity’s arm in the form of “Jack Main Canyon,” located just below and left of the apparently brighter and angular rock in the upper-left of the image.

Today’s plan kicked off with a lengthy DAN passive activity and imaging of the REMS UV sensor with MAHLI. APXS followed with a short measurement on Jack Main Canyon alongside usual imaging support from MAHLI. Morning measurements with APXS, referred to as touch-and-gos (or a hover-and-go in this case, since we did not actually touch Jack Main Canyon with APXS) have become less frequent recently as the summer season’s relatively warmer temperatures hinder APXS’s data quality. Also in the first sol of the plan, ChemCam’s laser analyzed a rock named “Budd Lake,” which was also captured by Mastcam. Mastcam additionally imaged “McGee Creek,” “Granite Park,” “Lamrack Col,” and conducted a sizable 49-image mosaic on “Red Devil Lake” to round out the bulk of the science planned today. Curiosity then completed a drive of about 24 meters (about 79 feet), which is expected to mark its arrival to Fairview Dome.

Written by Scott VanBommel, Planetary Scientist at Washington University

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Jul 16, 2024

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Robotic Assembly and Outfitting for NASA Space Missions

Robotic Assembly and Outfitting for NASA Space Missions

NASA is turning to the 3D modeling experts in the community for ideas and designs to use or enhance the current state of modular robotic construction techniques. Robotic building of structures in space is an active area of research for NASA and might prove to be a path towards sustainable and scalable space exploration. This technology is essential for establishing critical long-term orbital and Lunar surface infrastructure including power/communication towers, research stations, radiation shielding for habitats, and more.

Award: $2,000 in total prizes

Open Date: July 15, 2024

Close Date: September 9, 2024

For more information, visit: https://grabcad.com/challenges/robotic-assembly-and-outfitting-for-nasa-space-missions

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Sarah Douglas

Sols 4243-4245: Exploring Stubblefield Canyon

Sols 4243-4245: Exploring Stubblefield Canyon

3 min read

Sols 4243-4245: Exploring Stubblefield Canyon

This image was taken by Left Navigation Camera onboard NASA’s Mars rover Curiosity on Sol 4241 (2024-07-11 20:34:05 UTC).

Earth planning date: Friday, July 12, 2024

Curiosity, now heading uphill from the Mammoth Lakes drill site, has focused on a very interesting exposure of conglomerate rocks, consisting of pebbles cemented together by a fine-grained matrix material. On Earth, conglomerate rock is associated with downhill flows of rock and soil mixtures, often in a water-rich environment, so our science team is excited to find similar rocks on Mars. 

The local exposure of this unusual Martian deposit has been named “Stubblefield Canyon,” honoring the headwaters of the stream forming Rancheria Falls, which tumbles into Yosemite National Park’s Hetch Hetchy reservoir. All targets in this area of Mount Sharp are named after geological features near the town of Bishop, California, which sits at the foot of the Sierra Nevada mountains in the Owens Valley of California. Curiosity’s last drive ended at a detached, rubbly conglomerate slab, dubbed “Wishbone Lake” after a Y-shaped lake in upper Lamarck Lake Canyon near Mono Lake. The image above shows the Wishbone Lake slab of conglomerate rock in the rover workspace. Over the weekend, the team will investigate this target and image the surrounding terrain, collecting evidence about the formation of conglomerate rocks on Mars.

On Wednesday, Curiosity successfully completed its MAHLI imaging of “Donohue Pass” and ChemCam laser spectroscopy of “Negit Island,” followed by a 3-meter drive (about 10 feet) to Wishbone Lake. During the current plan, APXS will analyze two pebbles within the Wishbone Lake slab, “Arrowhead Spire” and “Cattle Creek.” Arrowhead Spire honors a 100-foot vertical spike of granite near Yosemite Point, above Yosemite Valley. Cattle Creek is named for a stream that flows from a hanging valley into the Twin Lakes canyon near Bridgeport, California. MAHLI will image Cattle Creek, then do a 4×1 mosaic from a distance of 25 centimeters (about 10 inches) along the edges of Wishbone Lake, centered on the Arrowhead Spire pebble. ChemCam will take laser spectra of Arrowhead Spire, as well as the “Eocene Peak” matrix material target, named for an 11,500-foot peak in the Sawtooth Ridge along the northeastern boundary of Yosemite National Park.

Using its telescopic RMI camera, ChemCam will image upper Gediz Vallis Ridge and a distant ridgeline along our future drive path. Mastcam will photograph the ChemCam laser targets, as well as interesting portions of the Stubblefield Canyon conglomerate exposure, the Mammoth Lakes drill site as seen from our new location, and an interesting linear ridge. On sol 4244, Curiosity will drive 20 meters (about 66 feet) along our path toward “Fairview Dome,” followed by post-drive imaging and AEGIS observations. Atmospheric studies during the current plan include a Navcam dust devil movie and large dust devil survey, early morning Navcam zenith and suprahorizon cloud movies, Navcam deck imaging, Navcam and Mastcam dust opacity measurements, and a late afternoon Mastcam sky survey. Next week, we expect to explore Fairview Dome, then resume our climb up Mount Sharp.

Written by Deborah Padgett, Curiosity Operations Product Generation Subsystem Task Lead at NASA’s Jet Propulsion Laboratory

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Jul 16, 2024

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Here’s How AI Is Changing NASA’s Mars Rover Science

Here’s How AI Is Changing NASA’s Mars Rover Science

6 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

In this time-lapse video of a test conducted at JPL in June 2023, an engineering model of the Planetary Instrument for X-ray Lithochemistry (PIXL) instrument aboard NASA’s Perseverance Mars rover places itself against a rock to collect data.
NASA/JPL-Caltech

Artificial intelligence is helping scientists to identify minerals within rocks studied by the Perseverance rover.

Some scientists dream of exploring planets with “smart” spacecraft that know exactly what data to look for, where to find it, and how to analyze it. Although making that dream a reality will take time, advances made with NASA’s Perseverance Mars rover offer promising steps in that direction.

For almost three years, the rover mission has been testing a form of artificial intelligence that seeks out minerals in the Red Planet’s rocks. This marks the first time AI has been used on Mars to make autonomous decisions based on real-time analysis of rock composition.

PIXL Viewed on Mars
PIXL, the white instrument at top left, is one of several science tools located on the end of the robotic arm aboard NASA’s Perseverance rover. The Mars rover’s left navcam took the images that make up this composite on March 2, 2021
NASA/JPL-Caltech

The software supports PIXL (Planetary Instrument for X-ray Lithochemistry), a spectrometer developed by NASA’s Jet Propulsion Laboratory in Southern California. By mapping the chemical composition of minerals across a rock’s surface, PIXL allows scientists to determine whether the rock formed in conditions that could have been supportive of microbial life in Mars’ ancient past.

Called “adaptive sampling,” the software autonomously positions the instrument close to a rock target, then looks at PIXL’s scans of the target to find minerals worth examining more deeply. It’s all done in real time, without the rover talking to mission controllers back on Earth.

“We use PIXL’s AI to home in on key science,” said the instrument’s principal investigator, Abigail Allwood of JPL. “Without it, you’d see a hint of something interesting in the data and then need to rescan the rock to study it more. This lets PIXL reach a conclusion without humans examining the data.”

rock target nicknamed “Thunderbolt Peak”
This image of a rock target nicknamed “Thunderbolt Peak” was created by NASA’s Perseverance Mars rover using PIXL, which determines the mineral composition of rocks by zapping them with X-rays. Each blue dot in the image represents a spot where an X-ray hit.
NASA/JPL-Caltech/DTU/QUT

Data from Perseverance’s instruments, including PIXL, helps scientists determine when to drill a core of rock and seal it in a titanium metal tube so that it, along with other high-priority samples, could be brought to Earth for further study as part of NASA’s Mars Sample Return campaign.

Adaptive sampling is not the only application of AI on Mars. About 2,300 miles (3,700 kilometers) from Perseverance is NASA’s Curiosity, which pioneered a form of AI that allows the rover to autonomously zap rocks with a laser based on their shape and color. Studying the gas that burns off after each laser zap reveals a rock’s chemical composition. Perseverance features this same ability, as well as a more advanced form of AI that enables it to navigate without specific direction from Earth. Both rovers still rely on dozens of engineers and scientists to plan each day’s set of hundreds of individual commands, but these digital smarts help both missions get more done in less time.

“The idea behind PIXL’s adaptive sampling is to help scientists find the needle within a haystack of data, freeing up time and energy for them to focus on other things,” said Peter Lawson, who led the implementation of adaptive sampling before retiring from JPL. “Ultimately, it helps us gather the best science more quickly.”

Using AI to Position PIXL

AI assists PIXL in two ways. First, it positions the instrument just right once the instrument is in the vicinity of a rock target. Located at the end of Perseverance’s robotic arm, the spectrometer sits on six tiny robotic legs, called a hexapod. PIXL’s camera repeatedly checks the distance between the instrument and a rock target to aid with positioning.

Temperature swings on Mars are large enough that Perseverance’s arm will expand or contract a microscopic amount, which can throw off PIXL’s aim. The hexapod automatically adjusts the instrument to get it exceptionally close without coming into contact with the rock.

“We have to make adjustments on the scale of micrometers to get the accuracy we need,” Allwood said. “It gets close enough to the rock to raise the hairs on the back of an engineer’s neck.”

Making a Mineral Map

Once PIXL is in position, another AI system gets the chance to shine. PIXL scans a postage-stamp-size area of a rock, firing an X-ray beam thousands of times to create a grid of microscopic dots. Each dot reveals information about the chemical composition of the minerals present.

Minerals are crucial to answering key questions about Mars. Depending on the rock, scientists might be on the hunt for carbonates, which hide clues to how water may have formed the rock, or they may be looking for phosphates, which could have provided nutrients for microbes, if any were present in the Martian past.

There’s no way for scientists to know ahead of time which of the hundreds of X-ray zaps will turn up a particular mineral, but when the instrument finds certain minerals, it can automatically stop to gather more data — an action called a “long dwell.” As the system improves through machine learning, the list of minerals on which PIXL can focus with a long dwell is growing.

“PIXL is kind of a Swiss army knife in that it can be configured depending on what the scientists are looking for at a given time,” said JPL’s David Thompson, who helped develop the software. “Mars is a great place to test out AI since we have regular communications each day, giving us a chance to make tweaks along the way.”

When future missions travel deeper into the solar system, they’ll be out of contact longer than missions currently are on Mars. That’s why there is strong interest in developing more autonomy for missions as they rove and conduct science for the benefit of humanity.

More About the Mission

A key objective for Perseverance’s mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet’s geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust).

Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis.

The Mars 2020 Perseverance mission is part of NASA’s Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.

JPL, which is managed for NASA by Caltech in Pasadena, California, built and manages operations of the Perseverance rover.

For more about Perseverance:

mars.nasa.gov/mars2020/

News Media Contacts

Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-2433
andrew.c.good@jpl.nasa.gov

Karen Fox / Alana Johnson
NASA Headquarters, Washington
202-358-1600 / 202-358-1501
karen.c.fox@nasa.gov / alana.r.johnson@nasa.gov

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Anthony Greicius

NASA Announces Leadership Changes

NASA Announces Leadership Changes

Two portrait images side by side. On the left is Clayton P. Turner, director of NASA Langley Research Center. On the right is Dawn Schaible, deputy director of NASA Glenn Research Center .
Clayton Turner, director of NASA’s Langley Research Center in Hampton, Virginia (left), and Dawn Schaible, deputy director of NASA’s Glenn Research Center in Cleveland (right).
Credit: NASA

NASA Administrator Bill Nelson announced Tuesday Dr. Kurt Vogel, associate administrator for the Space Technology Mission Directorate (STMD), is retiring from the agency. NASA Langley Research Center Director Clayton Turner will become the acting associate administrator for STMD, and NASA Glenn Research Center Deputy Director Dawn Schaible will become acting Langley center director. The changes are effective immediately, and for Turner and Schaible, these will be temporary assignments.  

“I’d like to thank Dr. Vogel for his service at NASA and wish him well in the future,” said Nelson. “Our Space Technology Mission Directorate and Langley Research Center are in good hands with Clayton and Dawn, and I look forward to continuing to work with them as we lead NASA into the future.”

Dr. Vogel has served as the head of STMD since January. Before leading STMD, Vogel served as director of space architectures and was chair of NASA’s Agency Cross-Directorate Federated Board. Vogel has more than 30 years of U.S. government service, primarily in the Defense Department, as a technical leader, senior program manager, and chief technologist.

Turner has been Langley’s center director since September 2019 and has served the agency for more than 30 years. He has held several roles at NASA Langley, including engineering director, associate center director, and deputy center director. Throughout his NASA career, he has worked on many projects for the agency, including: the Earth Science Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation Project; the materials technology development Gas Permeable Polymer Materials Project; the Space Shuttle Program’s Return to Flight work; the flight test of the Ares 1-X rocket; the flight test of the Orion Launch Abort System; and the entry, descent, and landing segment of the Mars Science Laboratory.

At NASA Langley, Schaible will lead a diverse group of more than 3,000 civil servant and contractor scientists, researchers, engineers, and support staff, who work to advance aviation, expand understanding of Earth’s atmosphere, and develop technology for space exploration. At NASA Glenn, Schaible has shared with the center director responsibility for planning, organizing, and managing the agency level programs and projects assigned to the center. Before becoming Glenn’s deputy director in February 2023, Schaible was the director of engineering for Langley. Prior to that, Schaible was appointed the NASA deputy chief engineer after serving as the manager of the Systems Engineering Office for the NASA Engineering and Safety Center. She began her career with NASA at the Kennedy Space Center in 1987, where she held a number of lead engineering and management positions for the Space Shuttle and International Space Station Programs.

To learn more about NASA’s Space Technology Mission Directorate, NASA’s Langley Research Center, and NASA’s Glenn Research Center, visit:

https://www.nasa.gov

-end-

Meira Bernstein / Allard Beutel
Headquarters, Washington
202-358-1600
meira.b.bernstein@nasa.gov / allard.beutel@nasa.gov

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Tiernan P. Doyle