Curiosity Blog, Sols 4695-4701: Searching for Answers at Monte Grande

Curiosity Blog, Sols 4695-4701: Searching for Answers at Monte Grande

3 min read

Curiosity Blog, Sols 4695-4701: Searching for Answers at Monte Grande

A color close-up photo of the Martian surface shows dry, flaky, tan-orange ground. At the image center is a hole cored into the ground, surrounded by material dug out from the hole, which looks like a mixture of soil and sharp flakes or shards of rock, and is slightly lighter-toned than the surrounding ground.
NASA’s Mars rover Curiosity acquired this image of the “Valle de la Luna” drill hole using its Mast Camera (Mastcam) on Oct. 19, 2025 — Sol 4693, or Martian day 4,693 of the Mars Science Laboratory mission — at 02:04:29 UTC.
NASA/JPL-Caltech/MSSS

Written by William Farrand, Senior Research Scientist, Space Science Institute

Earth planning date: Friday, Oct. 24, 2025

Curiosity has successfully drilled its 44th hole on Mars, which is a major milestone in our investigation of the enigmatic “boxwork unit,” a region of resistant ridges surrounding pits or “hollows” of less-resistant rock. The drilling took place over the past weekend within the “Monte Grande” hollow at the “Valle de la Luna” target. 

Rover planning this week consisted of ensuring that the granular drill tailings from Valle de la Luna were transferred to the SAM (Sample Analysis at Mars) and CheMin (X-ray diffraction) instruments, and analyzing the results. Results from these instruments, which will provide mineralogical and other compositional information, will be especially critical for determining how the boxwork features formed, since chemistry from the APXS and ChemCam instruments and reflectance spectra from ChemCam have revealed subtle, but not striking, differences between the rocks making up the ridges and those making up the hollows. Thus, a compositional explanation for the differences between the two terrain types has yet to be determined.

While these internal studies of the Valle de la Luna samples were going on, remote sensing data were collected by Mastcam of a series of targets, as well as atmospheric remote sensing. Among the Mastcam studies being conducted is a photometry study, a kind of study usually only carried out during an extended stationary period, such as the current drill campaign. Photometry is the study of changes in the apparent reflected brightness of rocks and soils based on the illumination geometry (for example, whether the Sun is low on the horizon or high in the sky). During this photometry campaign, multiple images are collected of the same target regions at different times of day.

In the final plan of the week, as part of the ongoing assessment of the Valle de la Luna sample, material will undergo an evolved gas analysis (EGA) in which the drilled sample is baked in an oven in SAM and volatile molecules including H2O, CO2, and SO2 are released and used to further aid in the characterization of the target materials. Mastcam observations will include further images collected as part of the photometry campaign. Also mosaics of the west wall of the Monte Grande hollow will be collected as well as several atmospheric measurements.

Next week the rover will continue analyzing the drilled sample with more SAM experiments, and also analyze the tailings. The team is also starting to search for a suitable drilling location on a ridge as the next drilling site, in order to compare with the results from the Monte Grande hollow.

A rover sits on the hilly, orange Martian surface beneath a flat grey sky, surrounded by chunks of rock.
NASA’s Mars rover Curiosity at the base of Mount Sharp
NASA/JPL-Caltech/MSSS

Share

Details

Last Updated
Nov 13, 2025

Related Terms

Powered by WPeMatico

Get The Details…

Curiosity Blog, Sols 4689-4694: Drill in the Boxwork Unit is GO!

Curiosity Blog, Sols 4689-4694: Drill in the Boxwork Unit is GO!

3 min read

Curiosity Blog, Sols 4689-4694: Drill in the Boxwork Unit is GO!

A wide-angle, grayscale photo from the Mars surface shows mostly flat, medium gray, slightly rough terrain ahead of the rover, with a lighter-toned indentation in the round directly in front of it. In the distance at the upper right of the image, the ground becomes much more uneven and rocky, with a mesa rising from the ground on the horizon beyond that. Parts of the rover are visible, but dark and shadowed, around the sides and bottom of the image, including two of its wheels at the bottom of the frame.
NASA’s Mars rover Curiosity acquired this image showing the “Valle de la Luna” block in the “Monte Grande” hollow, a location it targeted for drilling the weekend of Oct. 18-19, 2025. Curiosity captured the image with its Front Hazard Avoidance Camera (Front Hazcam) on Oct. 12, 2025 — Sol 4687, or Martian day 4,687 of the Mars Science Laboratory mission — at 23:11:12 UTC.
NASA/JPL-Caltech

Written by Catherine O’Connell-Cooper, APXS Payload Uplink/Downlink Lead, University of New Brunswick

Earth planning date: Friday, Oct. 17, 2025

Curiosity has been investigating the “boxwork unit” for several months now. Readers might remember we drilled at the edge of the boxwork at “Altadena,” back in June. Since then, we have driven just under a kilometer across the boxwork unit (about 0.6 miles) and now we are ready to acquire the next drill target, in an area where the structure is really well preserved.

The boxwork structures are a series of ridges and hollows, so our plan is to drill within one of the hollows and then on one of the adjacent ridges. On Monday, we did our drill triage on “Valle de la Luna” within the hollow “Monte Grande” – a multi-instrument endeavor. We assessed the chemistry using APXS and ChemCam, to make sure it is within the expected range and not something completely different from the bedrock compositions we have been tracking. The rover planners (RPs) use a “pre-load” test, putting pressure on the bedrock surface to characterize how the rover arm and rock might behave during drilling. We take multiple images (including images before and after the pre-load test), using MAHLI and Mastcam to help the RPs assess the surface of the potential drill area.

Finding a suitable place to drill in the hollows was a challenge, as the low point of each hollow (what we are most interested in) is often covered in sand or small pebbles, with just sparse bedrock peeking through, as you can see in the accompanying image. However, we got lucky here in Monte Grande. The chemistry shows that this rock is within our expected compositional range. The MAHLI images show a smoother surface in the center of the brushed area (where the drill will focus), and the before-and-after images indicated that the rock reacted well to the pre-load test. On Friday, the RPs and mission scientists pored over the data in a very intensive meeting called the “Target Acquisition Assessment Meeting,” or TAAM. We have drilled 43 holes on Mars now and it’s always nerve-wracking, waiting to see if the information we gathered during our initial contact science and preload give us a go-ahead. About midway through the planning day, we got the news that TAAM said yes to drilling here, so we will drill on the first sol of this weekend plan.

If the drill is successful, we will have no contact science for at least a week, as the arm cannot be deployed during a drill campaign. Normally, as I’m APXS PUDL (responsible for uplinking new APXS targets and assessing downlink of previous targets), the idea of a week with no contact science would be disappointing to me — but not during a drill campaign! CheMin (Chemistry Mineralogy) and SAM (Sample Analysis at Mars) will use the drilled sample to give us extra depth of information, looking at mineralogy and composition in a way that is not possible for APXS and ChemCam.

We can then use that drill data to help us interpret the APXS and ChemCam data and better understand the formation of these boxworks, especially if we can pair it with a suitable target on the ridges.

In the meantime of course, we continue to monitor the atmosphere and environment around us. The Mastcam team are planning some amazing images from this site and ChemCam will continue to characterize the nearby bedrock and image the far-off hills. 

A rover sits on the hilly, orange Martian surface beneath a flat grey sky, surrounded by chunks of rock.
NASA’s Mars rover Curiosity at the base of Mount Sharp
NASA/JPL-Caltech/MSSS

Share

Details

Last Updated
Nov 13, 2025

Related Terms

Powered by WPeMatico

Get The Details…

Curiosity Blog, Sols 4682-4688: Seven Mars Years

Curiosity Blog, Sols 4682-4688: Seven Mars Years

4 min read

Curiosity Blog, Sols 4682-4688: Seven Mars Years

A wide-angle grayscale photo from the Martian surface shows very uneven, rocky terrain covering the left side of the image from the foreground to the horizon, which falls off to smoother ground descending toward the right side of the frame, down into a crater. On the left and ridge edges of the frame, near the top, large rocky outcrops arise from the horizon, while more peaks are visible but hazy in the far distance. Portions of the rover’s shadow darken the lower left and right corners of the image.
NASA’s Mars rover Curiosity acquired this image that looks down toward both the floor of Gale Crater, where we started our journey up Mount Sharp more than a decade ago, and toward the “Monte Grande” hollow that we hope will contain our next drill target. Curiosity captured the image using its Front Hazard Avoidance Camera (Front Hazcam) on Oct. 9, 2025 — Sol 4684, or Martian day 4,684 of the Mars Science Laboratory mission — at 21:28:14 UTC.
NASA/JPL-Caltech

Written by Diana Hayes, Graduate Student at York University, Toronto

Earth planning date: Friday, Oct. 10, 2025

This week was one of seasonal changes and milestones for the mission. As was mentioned several weeks ago, Mars has now moved out of its “cloudy season” and is transitioning into the “dusty season” as the planet moves closer to the Sun. This means that we should expect to see an increase in dust lifting and dust-devil activity over the next several months. With more dust in the atmosphere, we expect to lose the beautifully clear skies that have allowed us to take pictures of features at tremendous distances from the rover, like a mountain 57 miles (91 kilometers) away, outside of Gale Crater. We’ll also be keeping an eye out for the possible development of a global dust storm this season, as one has not occurred since 2018

Back in August, we celebrated 13 Earth years since Curiosity landed in Gale back in 2012. This Monday, Oct. 6, a bit after 1 a.m. UTC (8 p.m. EDT Oct. 5), our intrepid rover marked its seventh full Mars year on the surface. (Because Mars is farther from the Sun than Earth is, a year on Mars — or one full trip around the Sun — lasts 687 Earth days.) Curiosity is only the second vehicle on Mars to reach that milestone, behind only Opportunity. Although Curiosity has not yet matched Opportunity’s longevity or distance driven, over the last seven Mars years we have put together the longest and most comprehensive record of the modern Martian climate. REMS has been recording weather conditions at least once an hour almost every hour since 2012, and RAD has now measured surface radiation conditions for more than a full solar cycle, data that will be critical to future human exploration of Mars. We’ve taken more than 3,000 cloud movies and countless more observations of atmospheric opacity, dust lifting, and dust-devil activity. I’ve been a member of our environmental science team for just over five (Earth) years now (or about 2 ½ Mars years), and I can still hardly believe that I’ve been able to help contribute to this incredible legacy. Although our well-traveled rover is now in its fifth Extended Mission, as a team we have no intention of slowing down any time soon.

Other than celebrating these milestones, this week was focused on setting up for the first of our two planned drills in the boxwork region. This first drill will be in one of the boxwork “hollows.” We’re currently targeting a hollow we’ve nicknamed “Monte Grande,” with the goal that we’ll be set up to drill there next week. Once we’re done at Monte Grande, we plan to drive up to one of the raised ridges that give the boxwork region its spiderweb-like appearance. By comparing the results of these two drill campaigns, our hope is that we’ll be able to gain a better understanding of the processes in Mars’ past that led to the formation of these fascinating features. 

As we prepare to drill, both science theme groups continued their usual cadence of contact science and remote sensing to characterize the local geology and environment. This weekend will be particularly busy on the environmental science side of the mission, with coordinated observations with APXS and ChemCam to track seasonal changes in the composition of the atmosphere. We’ll also be using SAM’s Tunable Laser Spectrometer instrument to measure the amount of atmospheric methane at Gale. This is an activity that we’ve performed periodically over the mission, and has inspired much spirited debate over the sources and destruction mechanisms of Martian methane

Here’s to many more years of roving and scientific discovery!

A rover sits on the hilly, orange Martian surface beneath a flat grey sky, surrounded by chunks of rock.
NASA’s Mars rover Curiosity at the base of Mount Sharp
NASA/JPL-Caltech/MSSS

Share

Details

Last Updated
Nov 13, 2025

Related Terms

Powered by WPeMatico

Get The Details…

Curiosity Blog, Sols 4675-4681: Deciding Where to Dig Into the Boxworks

Curiosity Blog, Sols 4675-4681: Deciding Where to Dig Into the Boxworks

3 min read

Curiosity Blog, Sols 4675-4681: Deciding Where to Dig Into the Boxworks

A grayscale photo from the Martian surface shows a landscape with an elevated ridge running from the foreground, at the bottom left  of the image, toward the middle right side of the frame, with two branches extending toward the left side of the frame, creating a U-shaped depression between them. The top of the ridge is much lighter colored than the medium gray surrounding terrain, which extends off to the horizon at the top of the frame, and is interspersed with areas of scattered small, jagged rocks and wavy sand deposits.
NASA’s Mars rover Curiosity acquired this image using its Right Navigation Camera, showing the three types of geologic features that have held the mission team’s attention for months — a bright, arcuate boxwork ridge, a darker, sand-filled hollow, and, in the distance, the “Mishe Mokwa” butte. Curiosity captured the image on Oct. 2, 2025 — Sol 4677, or Martian day 4,677 of the Mars Science Laboratory mission — at 15:49:32 UTC.
NASA/JPL-Caltech

Written by Michelle Minitti, MAHLI Deputy Principal Investigator at Framework

Earth planning date: Friday, Oct. 3, 2025

Before Curiosity landed 13 years ago, the science team eyed all the geologic wonders scattered across the flanks of Mount Sharp and looked forward to the day when we could put the rover to work on them. We have visited so many of these wonders — valleys, river channels, lakebeds — and found a few that we were not expecting. 

Since Sol 4600, we have been exploring the heart of one of these long-awaited wonders — the boxwork structures — to uncover what created this expansive network of ridges and hollows. Each stop along the traverse since then has been an exercise in systematic detective work. 

APXS and ChemCam analyses from the center of a ridge, to its edges, and into its neighboring hollow looked for chemical variations that indicate what is holding the ridges together, making them higher than the hollows. Mastcam and ChemCam RMI imaging mapped the architecture of the ridges and hollows looking for structures that provide clues to their formation. Their imaging of more distant features such as the buttes that rise hundreds of meters on either side of the valley hosting the boxworks helped define the geologic context of the area. MAHLI imaging of ridge and hollow targets sought variations in grain size that might indicate how the boxwork bedrock was deposited. DAN surveyed the ground under the rover at every stop, measuring hydrogen (and thus assumed, water) content to see how it varies between ridges and hollows. 

This week, the team ingested all the results from this thorough exploration to make a decision about our next drill site, where SAM and CheMin will have their chance to interrogate the boxworks. The rover will head north to the “Monte Grande” hollow in which we identified promising bedrock for sampling. Eventually, we will drill a ridge but that is for a future blog. Comparing the mineralogy, volatile content, and organic chemistry of the ridges and hollows will give us our most detailed insight into how the boxworks formed.

REMS and RAD do not particularly care if they are parked over a ridge or hollow, as the sky above is their domain. Both instruments kept their steady watch on the weather — Martian and space, respectively. Navcam and Mastcam helped with the environmental watch by measuring dust in the atmosphere, looking for dust devils, and capturing the last of the cloudy season. 

A rover sits on the hilly, orange Martian surface beneath a flat grey sky, surrounded by chunks of rock.
NASA’s Mars rover Curiosity at the base of Mount Sharp
NASA/JPL-Caltech/MSSS

Share

Details

Last Updated
Nov 13, 2025

Related Terms

Powered by WPeMatico

Get The Details…

Expedition 73 Crew Works Cardiovascular Research and Spacesuits on Thursday

Expedition 73 Crew Works Cardiovascular Research and Spacesuits on Thursday

The new HTV-X1 cargo spacecraft from JAXA (Japan Aerospace Exploration Agency) is pictured in the grips of the Canadarm2 robotic arm after completing its arrival at the International Space Station on Oct. 29, 2025.
The new HTV-X1 cargo spacecraft from JAXA (Japan Aerospace Exploration Agency) is pictured in the grips of the Canadarm2 robotic arm after completing its arrival at the International Space Station on Oct. 29, 2025.
NASA

Cardiovascular research and spacesuit maintenance topped the schedule for the Expedition 73 crew aboard the International Space Station on Thursday. The orbital residents studied how living in space affects blood circulation, swapped advanced gear on a spacesuit, and installed a new life support experiment.

NASA Flight Engineer Jonny Kim spent the first half of his shift in the Columbus laboratory module wearing electrodes scanning his chest with an ultrasound device to help doctors understand how his heart function and structure is adapting to weightlessness. After lunchtime, Kim jogged on the COLBERT treadmill then worked out on the advanced resistive exercise device while wearing a heart rate monitor that recorded his cardiac activity. The data collected throughout the day may inform researchers of the cardiovascular risk astronauts face as NASA and its international partners plan missions to the Moon, Mars, and beyond.

Roscosmos cosmonauts Sergey Ryzhikov and Alexey Zubritsky, station commander and flight engineer respectively, partnered together exploring how blood circulates to and from the smallest vessels in the human body in microgravity. The duo took turns wearing sensors on their forehead, fingers, and toes to monitor blood flowing to the microcirculatory and tissue systems. Results may help researchers develop techniques to protect long-duration space crews and prepare them for the return to Earth.

Flight Engineers Zena Cardman and Mike Fincke of NASA worked together throughout Thursday servicing a spacesuit inside the Quest airlock. Cardman and Fincke first swapped a life support device inside the suit that provides ventilation and cooling during a spacewalk. Afterward, the pair installed a radio inside the suit that enables communications between spacewalkers, crew members inside the station, and mission controllers on the ground.

JAXA (Japan Aerospace Exploration Agency) Flight Engineer Kimiya Yui spent his day inside the Kibo laboratory module installing a new carbon dioxide removal system delivered aboard the HTV-X1 cargo spacecraft on Oct. 29. The advanced life support technology seeks to demonstrate the efficient removal of carbon dioxide from a spacecraft to promote future Artemis missions to the Moon.

Roscosmos Flight Engineer Oleg Platonov started his day wearing sensors and a blood pressure cuff observing how his blood vessel health is affected by weightlessness and radiation. Afterward, he and Ryzhikov took turns pedaling for an hour on the station’s exercise cycle while wearing chest electrodes and a blood pressure cuff for a fitness evaluation.

Daily health monitoring and exercise are essential for astronauts living in microgravity for months or years at a time. The health and research data collected informs strategies to protect future crews on deep space missions.

Powered by WPeMatico

Get The Details…

Mark A. Garcia