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Looking Back, Moving Forward
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By NASA
NASA/Joel Kowsky NASA launched its reimagined art program by unveiling two murals on Sept. 23, 2024. The murals, titled “To the Moon, and Back,” were created by New York-based artist team Geraluz and WERC and use geometrical patterns to invite deeper reflection on the exploration, creativity, and connection with the cosmos. The vision of this next phase is to inspire and engage the Artemis Generation with community murals and other art projects for the benefit of humanity.
NASA has long used art to tell the story of its awe-inspiring missions. Soon after its inception, the agency started a formal program commissioning artists to develop inspiring pieces like portraits and paintings that highlighted an unexpected side of the agency. In 1962, NASA’s then Administrator James Webb tasked staffer and artist James Dean with implementing the new program, and with the help of the National Gallery of Art, Dean laid the framework to artistically capture the inspiration of NASA’s Apollo program. As the NASA Art Program continues to evolve, the agency remains focused on inspiring and engaging the next generation of explorers – the Artemis Generation – in new and unexpected ways, including through art.
Image Credit: NASA/Joel Kowsky
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By NASA
4 Min Read Robotic Moving ‘Crew’ Preps for Work on Moon
The LANDO system works by using onboard sensors to scan encoded markers (similar to a QR code) on a payload, which will reveal critical information about its position and orientation relative to the LSMS. This information is used to calculate where the robotic arm exists in space and plan the motion path to pick up and move payloads. Credits: NASA/David C. Bowman As NASA moves forward with efforts to establish a long-term presence on the Moon as part of the Artemis campaign, safely moving cargo from landers to the lunar surface is a crucial capability.
Whether the cargo, also known as payloads, are small scientific experiments or large technology to build infrastructure, there won’t be a crew on the Moon to do all the work, which is where robots and new software come in.
A team at NASA’s Langley Research Center in Hampton, Virginia, spent the last couple of years infusing existing robotic hardware with a software system that makes the robot operate autonomously. Earlier this month, that team, led by researcher Dr. Julia Cline of NASA Langley’s Research Directorate, ran demonstrations of their system called LANDO (Lightweight Surface Manipulation System AutoNomy capabilities Development for surface Operations and construction).
LANDO prepares to move its payload to a safe spot on the simulated lunar surface.NASA/David C. Bowman The demos took place in an area set up to look like the Moon’s surface, complete with fake boulders and a model lunar lander. During the first demo, the team placed the payload, a small metal box, on a black pedestal. The robotic arm stretched over the scene, with its dangling hook poised to grasp the box.
As the team huddled nearby around computers, sensors on the arm scanned the surrounding area, looking for the metal box, which was outfitted with encoded markers — similar to QR codes — that revealed critical information about its position and orientation relative to the arm. Using a graphic user interface, team member Amelia Scott also chose a location for LANDO to place the payload.
During a series of slow, methodical movements, LANDO transports a payload from a pedestal to a simulated lunar surface.NASA/Angelique Herring After locating the metal box and computing a safe path to move it, the arm began a slow, deliberate movement toward its target, coming in at a precise angle that allowed the hook to select a capture point on the payload. Once engaged, the arm slowly lifted the payload from the pedestal, moved right, and gently lowered the payload to the simulated lunar surface. With the payload safely on the surface, the system carefully disengaged the hook from the capture point and returned to its home position. The entire process took a few minutes. Shortly after the first demo was complete, the team did it again, but with a small model rover.
“What we demonstrated was the repeatability of the system,moving multiple payloads to show that we’re consistently and safely able to get them from point A to point B,” said Cline. “We also demonstrated the Lightweight Surface Manipulation System hardware – the ability to control the system through space and plan a path around obstacles.”
The system’s successful performance during the September demonstration marks the end of this project, but the first step in developing a larger system to go to the Moon.
Now that the team has determined how the system should function, Cline believes the next natural step would be to develop and test an engineering design unit on one of the landers going to the Moon as part of NASA’s Commercial Lunar Payload Services (CLPS) initiative. The team is actively looking for industry partners who want to commercialize the capability.
Through CLPS, NASA is working with commercial companies to deliver science and technology demonstrations to the Moon.
The work behind LANDO could be directly infused into much larger versions of a lightweight surface manipulation system.
The LANDO team, back row, left to right: Dominic Bisio, Joshua Moser, Walter Waltz, Jacob Martin, Ryan Bowers, Brace White and Iok Wong. And kneeling, left to right: Amelia Scott, Matthew Vaughan, Julia Cline, Jessica Friz and Javier Puig-Navarro.NASA/Ryan Hill “The overall control system we’ve developed would apply to larger versions of the technology,” said Cline. “When you think about the payloads we’ll have to offload for on the Moon, like habitats and surface power systems, this is the kind of general-purpose tool that could be used for those tasks.”
The LANDO system was funded through the Early Career Initiative in NASA’s Space Technology Mission Directorate (STMD). Through STMD, NASA supports and develops transformative space technologies to enable future missions. As NASA embarks on its next era of exploration with the Artemis campaign, STMD is helping advance technologies, developing new systems, and testing capabilities at the Moon that will be critical for crewed missions to Mars.
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Last Updated Sep 25, 2024 EditorJoe AtkinsonLocationNASA Langley Research Center Related Terms
Langley Research Center Space Technology Mission Directorate View the full article
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By NASA
Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions The Solar System The Sun Mercury Venus Earth The Moon Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets Asteroids, Comets & Meteors The Kuiper Belt The Oort Cloud 3 min read
Sols 4314-4315: Wait, What Was That Back There?
A view of the right-middle wheel of NASA’s Mars rover Curiosity, one of the rover’s six well-traveled wheels. Curiosity acquired this image using its Mars Hand Lens Imager (MAHLI), located on the turret at the end of the rover’s robotic arm, on Sept. 22, 2024, sol 4312 (Martian day 4,312) of the Mars Science Laboratory Mission, at 18:37:41 UTC. NASA/JPL-Caltech/MSSS Earth planning date: Monday, Sept. 23, 2024
After a busy weekend of activities, Curiosity is ready for another week of planning. One of the activities over the weekend was our periodic check-in on our wheels to see how they are holding up on the rough terrain. The image shows the MAHLI view of the right-middle (RM) wheel, which is still holding up well despite taking some of the worst abuse from Mars.
We are planning contact science with APXS and MAHLI on “Burst Rock,” which is a target that has an interesting texture and has bright-toned clasts and a gray coating. It is part of the Gediz Vallis Ridge channel deposits and will help out understanding of the channel. Unfortunately, it was too rough to brush, but it is clean enough that we can still get good science data.
We are doing a lot of imaging and remote science today. We are taking Mastcam mosaics of multiple targets. “Log Meadow” is a target designed to get a look at the distribution of the white stones in the channel. “Grand Sentinel” is a target on the opposite side of our previous workspace, allowing us to document it from a different angle. “Tunnel Rock” and “Tombstone Ridge” are sedimentary rocks that may have ripple-like layers; examining the layer contours helps inform how rocks were formed. Lastly, “Gravel Ridge” is a target in “Arc Pass” where we are continuing to examine clasts and sedimentary layers. We also take a ChemCam LIBS observation of Log Meadow and a long-distance RMI image of “Chanbank,” another area of white stones. We round it off with a Navcam mosaic of the rover to monitor dust on the deck.
After wrapping up the targeted and contact science, we’re ready to drive. As the science team had time to look a bit more at the data collected in that region, they discovered this target that was worth going back for. We are driving back to the area of the white stones to do more contact science on rocks that look similar to the elemental sulfur we saw earlier this year. Planning ahead, I got to scout this drive on Friday, laying out the safest path and looking for parking spots that were both good for communications as well as for doing contact science. The target “Sheep Creek” is about 50 meters (about 164 feet) to the northeast, which makes the drive a challenge — the resolution of our imagery at that range makes it harder to pinpoint these small rocks. We do have really good imaging in that direction, and the terrain isn’t super scary, so the Rover Planners are going to try to make it in one drive. During the drive, we will be taking a MARDI “sidewalk” movie (a series of images looking below the rover for the entire length of the drive), which will help document the channel. On the second sol of the plan, we do some additional atmospheric and untargeted science. We have a Navcam suprahorizon movie (looking at the crater rim to evaluate dust in the atmosphere) and a dust devil movie. We also have a ChemCam AEGIS observation, where the rover will autonomously select a target to image. Overnight, CheMin does an “empty cell” analysis to confirm that the system is cleaned out and ready for the next sampling campaign.
Written by Ashley Stroupe, Mission Operations Engineer at NASA’s Jet Propulsion Laboratory
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Last Updated Sep 24, 2024 Related Terms
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By European Space Agency
The Sentinel-1B satellite, the second satellite of the Copernicus Sentinel-1 mission, completed its disposal process – which included lowering its orbit and passivating its systems to ensure re-entry into Earth’s atmosphere within 25 years.
This careful operation highlights the European Union’s and ESA’s commitment to space safety and sustainability and provides valuable experience for the disposal of current and future spacecraft.
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By NASA
Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions The Solar System The Sun Mercury Venus Earth The Moon Mars Jupiter Saturn Uranus Neptune Pluto & Dwarf Planets Asteroids, Comets & Meteors The Kuiper Belt The Oort Cloud 3 min read
Sols 4309–4310: Leaning Back, Driving Back
NASA’s Mars rover Curiosity captured this image of a large fractured slab of bedrock, taken by Right Navigation Camera onboard NASA’s Mars rover Curiosity on Sol 4307 — Martian day 4,307 of the Mars Science Laboratory Mission — on Sept. 17, 2024 at 15:50:36 UTC. Earth planning date: Wednesday, Sept. 18, 2024
The lengthy drive planned on Monday executed as expected, and we came in today to find our rover parked at a jaunty angle on a sloped ridge. There were some worries that the slope might limit our ability to use the arm for contact science in this plan (we don’t want to do anything that might cause the rover to slide down the slope!), but after some careful consideration, we received the good news that all six of our wheels are holding on firmly to the ground, so there was no risk of slipping.
On Monday, two different options for today’s plan were laid out. The first option, a “full contact science” plan where we don’t drive, was to be executed if Monday’s drive put us exactly where we hoped. The second, a “touch-and-go” plan where we do some light contact science before driving away, was to be executed if the drive didn’t put us where we wanted to be. As it happened, the rover was a little too enthusiastic about driving, and actually put our desired workspace under its body rather than in front where the arm could reach it. There’s always a little uncertainty in the final position after such a long drive! So, we decided to stick with a touch-and-go plan that includes a tiny backwards drive of less than a metre to reposition our desired target in front of the rover.
Although we need to re-position, we aren’t slowing down on science for even a second. We are parked in front of a large fractured slab of bedrock, which can be seen in the above image. This slab became the contact science target for this plan with DRT and APXS activities on “The Minster.” Mastcam is getting a workout today as well, with large mosaics of “North Channel,” “Buckeye Ridge,” “Quinn,” and “Island Pass.” These mosaics are all documenting various aspects of the ridge we’re sat on and the edge of the Gediz Vallis Channel, including sedimentary rocks, white sulphate materials, and gravels and fine-grained materials. ChemCam is also taking a turn on the bedrock slab with a LIBS activity on “Grand Sentinel” and a mosaic of some exposed white stones off in the distance.
The second sol of the plan, after our short drive, is largely taken over by environmental science activities, though there is our usual post-drive ChemCam AEGIS. These activities include a Mastcam tau and Navcam line-of-sight to measure the amount of dust in the atmosphere around and above us, as well as a dust devil movie, suprahorizon cloud movie, and some Navcam deck monitoring to see if our driving or the wind is moving around any of the sand and dust on the rover deck. The team is also taking the usual set of REMS, RAD, and DAN observations.
Written by Conor Hayes, Graduate Student at York University
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