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Sols 4498-4499: Flexing Our Arm Once Again
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Sols 4505-4506: Up, up and onto the Devil’s Gate
This image was taken by Left Navigation Camera onboard NASA’s Mars rover Curiosity on Sol 4503 (2025-04-07 00:33:50 UTC). NASA/JPL-Caltech Written by Catherine O’Connell-Cooper, Planetary Geologist at University of New Brunswick
Earth planning date: Monday, April 7, 2025
Over the weekend, we completed our drive up the steep side of a canyon, up onto “Devil’s Gate,” a small butte which forms part of the ridge along the top of the canyon and now we can see down into the next canyon. It is always true that we are going somewhere no one has been before – that’s the idea of an exploratory mission after all, and everyone kind of gets used to it, we don’t stop to think about it. But today, coming over the top of a hill like this and fully looking for the first time into an area that we have only had glimpses of before, it really brings it home that the mission is doing something extraordinary, something out of this world …. and brings that feeling of awe back into focus.
We did not pass SRAP (Slip Risk Assessment Process) a couple of times as we climbed up the side of this canyon, meaning that the contact science instruments (APXS and MAHLI) had to stand down for that day’s planning. However, this morning, in addition to a brand new vista, we saw that all six wheels are firmly on the ground and we passed SRAP quickly this morning, which must have been a relief to the rover planner in charge of assessing it today! (no one wants to be the bearer of bad news, day after day!)
Bedrock here has both flat bedrock and amazing large nodular features, which appear to have “wind tails” caused by winds consistently blowing in the same direction. This is a Touch and Go plan, so APXS and MAHLI are focusing on a single target, the brushed “Coronado” target on the flat bedrock in front of us. ChemCam will use LIBS to investigate the nodular features at “La Cumbre Peak.”
Near the rover, Mastcam will image some small diagenetic features at “Boulder Oaks” and the LIBS target. The 3×2 (2 rows of 3 images) “La Jolla Valley” mosaic focuses on a very nodular patch, just outside of the workspace reachable by the arm. Further from the rover, the 6×2 mosaic (2 rows of 6 images) “Los Penasquitos” looks at an amazing almost vertical vein. This discontinuous vein stretches for about 6 meters (about 18 feet), with vein fins sticking above the surface at various points, like a series of shark fins breaking the bedrock surface. Much further afield, ChemCam will acquire a long distance image on “Condor Peak,” which appears to have large scale vein networks, known as “boxwork structures” and may be an early example of the boxworks we are hoping to reach in Fall 2025.
The ENV (Environmental and Atmospheric group) planned a Mastcam “tau” measurement, to look at dust in the atmosphere. There is a paired Navcam activity, looking at dust devils towards the north of the crater on the first sol and towards the south on the second sol. A suprahorizon movie and our usual DAN and REMS measurements round out this plan.
Let’s see what the next drive will reveal to us!
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Sols 4502-4504: Sneaking Past Devil’s Gate
NASA’s Mars rover Curiosity acquired this image of the terrain around it on April 3, 2025, showing a small ridgeline on the right side, “Devil’s Gate,” and the base of Texoli butte, visible on the left side of the image. Curiosity acquired the image using its Left Navigation Camera on Sol 4500, or Martian day 4,500 of the Mars Science Laboratory mission, at 23:08:35 UTC. NASA/JPL-Caltech Written by Michelle Minitti, Planetary Geologist at Framework
Earth planning date: Friday, April 4, 2025
We continue to make progress driving up Mount Sharp, each day gaining new perspectives on the spectacular, towering buttes surrounding our path. To get to the next canyon we can ascend, we have to swing around the north end of a small ridgeline, “Devil’s Gate,” which is on the right side of the image above.
The blocks scattered around the base of Devil’s Gate are ripe with interesting structures, which motivated the acquisition of an RMI mosaic across the ridge. Those blocks are also inconvenient for driving and parking the rover with all six wheels firmly on the ground, the latter of which is needed to be able to unstow the arm for APXS and MAHLI observations. Our last drive ended with our front wheels not quite on solid ground, so we had to forego arm work this weekend. But as you can imagine with the view around us, Devil’s Gate was not the only feature that the team was excited to image. ChemCam added a second RMI mosaic along the base of “Texoli” butte, which you can see the flank of on the left side of the image above. Mastcam planned a mosaic across an expanse of bedrock that looks like rolling waves frozen in place at “Maidenhair Falls.”
The rocks right in front of the rover were also wonderfully complex in their textures and structures. ChemCam targeted two different textures expressed in the workspace — one across fine layers at “Arroyo Burro” and one across rough, platy, and gray material at “Arroyo Conejo.” Mastcam documented the block containing both these targets with a stereo mosaic that will give us a three-dimensional view of its structures.
We planned a drive to get us further around the base of Devil’s Gate, after which we will acquire an autonomously-targeted ChemCam LIBS raster and early morning Navcam and Mastcam mosaics looking back on the path we have recently traveled. DAN is scheduled for about seven hours of data collecting across the plan, both during science blocks and our drive. The sky gets a lot of attention in this plan with suites of observations taken at two different times — near midday and early morning — to assess variability across the day. Each window of time had Navcam dust-devil and cloud movies, and measurements of the amount of dust in the atmosphere. The early morning block of observations also had multiple cloud movies cover the full sky. REMS and RAD have regular measurements across the sols.
See you Monday, when we are a bit farther past Devil’s Gate!
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Last Updated Apr 07, 2025 Related Terms
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Sols 4500-4501: Bedrock With a Side of Sand
NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera on March 28, 2025 — Sol 4494, or Martian day 4,494 of the Mars Science Laboratory mission — at 17:06:34 UTC. NASA/JPL-Caltech Written by Sharon Wilson Purdy, Planetary Geologist at Smithsonian National Air and Space Museum
Earth planning date: Wednesday, April 2, 2025
Wow, sol 4500. What an impressive number of sols (Martian days) exploring the Red Planet! This delightfully even sol number made me wonder where the Mars Exploration Rover (MER) Opportunity was at this point in her mission (Opportunity’s twin rover, Spirit, explored Gusev crater on Mars for roughly 2210 sols). As it turns out, Opportunity was driving over fairly smooth terrain on sol 4500 and was approaching a light-toned rounded hill named “Spirit Mound” on the western rim of Endeavour crater in Meridiani Planum.
I am always so impressed and proud when I stop to think about the incredible fleet of rovers we have safely landed and operated on Mars, and the amazing scientific discoveries that have resulted from these missions!
Today I served on science operations as the “keeper of the plan” for the geology and mineralogy theme group. In this role, I assembled the activities in our team planning software for this two-sol plan. Our small plan becomes part of a much larger set of instructions that will be relayed up to the rover later today. Currently, the Curiosity rover is driving up Mount Sharp over broken-up blocks of bedrock and sand through a small canyon en route to the boxwork structures ahead. This bumpy terrain can sometimes make it hard to pass the “Slip Risk Assessment Process” (SRAP) where all six wheels are required to be stable on the ground before we can unstow our robotic arm to use the contact science instruments. After our successful 8-meter drive (about 26 feet) from yestersol we passed SRAP and got to work selecting targets for contact and remote observations.
The team chose to characterize a bedrock target in front of us called “Chuckwalla” using the dust removal tool (DRT), APXS, and MAHLI. ChemCam used its LIBS instrument to analyze the chemistry of a nearby bedrock target with a knobby texture, “Pechacho,” and took a long distance RMI image to study the interesting layering in the “Devil’s Gate” butte. Mastcam assembled an impressive portfolio of observations in this two-sol plan. The team imaged variations in bedrock textures at “Jalama” and “Julian” and documented the nature of the “Mishe Mokwa” ridgeline. In addition, Mastcam imaged darker rocks within a previously acquired mosaic of Devil’s Gate and investigated narrow troughs (small depressions) within the sand in the workspace.
The environmental theme group, with their eye on the sky, included activities to measure the optical depth of the atmosphere, constrain aerosol scattering properties, and observe clouds. A very busy day of planning for sols 4500-4501, with many more to come!
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Sols 4495-4497: Yawn, Perched, and Rollin’
NASA’s Mars rover Curiosity acquired this image of the upcoming “boxwork” structures to its west, using its Chemistry & Camera (ChemCam) Remote Micro-Imager (RMI). The ChemCam instrument studies the chemical composition of rocks and soil, using a laser to vaporize materials, then analyze their elemental composition using an on-board spectrograph. The ChemCam RMI is a high-resolution camera atop the rover’s mast. Curiosity captured this image on March 27, 2025 — Sol 4493, or Martian day 4,493 of the Mars Science Laboratory mission — at 15:35:21 UTC. NASA/JPL-Caltech/LANL Written by Natalie Moore, Mission Operations Specialist at Malin Space Science Systems
Earth planning date: Friday, March 28, 2025
Womp, womp. Another SRAP (Slip Risk Assessment Process) issue due to wheels being perched on these massive layered sulfate rocks. With our winter power constraints as tight as they are, though, keeping the arm stowed freed up more time to check some lines off our rover’s weekend list. To do: SAM activity to exercise Oven 2 (check!), Navcam 360-degree “phase function” sky movie to monitor scattering of Martian clouds (check!), APXS atmospheric measurements of argon (check!), ChemCam passive sky measurements of oxygen (check!), and a drive of about 50 meters (about 164 feet) to the southwest (check!). Curiosity gets busy on the weekends so us PULs can do some lounging.
On the Mastcam team, we’ve been pretty busy in the layered sulfate unit. The rocks are rippled, layered, fractured, and surrounded by sandy troughs. Where did it all come from? What current and past processes are at play in this area? This weekend we’re collecting 70 images to help figure that out. ChemCam is helping by collecting chemistry measurements of the lowest block in this Navcam image, with two targets close by aptly named “Solana Beach” and “Del Mar.” To help conserve power, we’ve been trying to parallelize our activities as much as possible. Recently this means Mastcam has been taking images while ChemCam undergoes “TEC Cooling” to get as cold as possible before using their laser.
We’re all hoping the arm can come back from vacation next week.
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Sols 4493-4494: Just Looking Around
NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera on March 25, 2025 — sol 4491, or Martian day 4,491 of the Mars Science Laboratory mission — at 17:16:50 UTC. NASA/JPL-Caltech Written by Alex Innanen, atmospheric scientist at York University
Earth planning date: Wednesday, March 26, 2025
It’s my second shift of the week as the Environmental theme lead and keeper of the plan (a bit of a mouthful we shorten to ESTLK) and today started out feeling eerily similar to Monday. Once again, Curiosity is posing like a geologist, which means that once again we can’t unstow the arm and will be skipping contact science. The silver lining is that this means we have extra time to have a good look around.
The plan also looks similar to Monday’s — targeted remote sensing on the first sol before driving away, and then untargeted remote sensing on the next. On sol 4493 we start our remote sensing, almost as remote as we can get, with a suprahorizon movie looking for clouds in the south. A dust-devil survey rounds out the sol’s environmental observations, and then the geology theme group can get down to the serious business of looking at rocks. For Mastcam this means observing a group of bedrock targets all called “Observatory Trail” (one of which you can see in the middle of the image above), pointing out some interesting veins in “Point Loma,” and casting their gaze out toward “Black Butte” (which I could not think of a fun pun for…). ChemCam has a LIBS observation of “Cholla,” as well as two long-distance observations of the Texoli Butte and the boxwork structures. Our second sol is a little more restrained, as untargeted sols tend to be. But Curiosity will still have plenty of energy after a good rest. We’re taking advantage of that with an extra-long dust-devil movie. Even though we’re in our cloudy season, we still sometimes see dust lifting, and having that extra time to look out for it increases our chances of catching a wind gust or a dust devil in action. Alongside that we also have a Mastcam tau observation to keep an eye on the amount of dust in the atmosphere, and wrap up with a ChemCam AEGIS activity to autonomously choose a LIBS target.
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