January 27, 2021

Sols 3015-3016: Can You Dip Your Toe in When It's Always Cold and Dry?

Written by Scott Guzewich, Atmospheric Scientist at NASA's Goddard Space Flight Center
Parts of the Curiosity rover are visible in this Mars panorama

This image was taken by Left Navigation Camera onboard NASA's Mars rover Curiosity on Sol 3013 (2021-01-27 00:07:33 UTC). Credit: NASA/JPL-Caltech. Download image ›

Today Curiosity is sitting on a geological contact within the “fractured intermediate unit” and we’re investigating the “rubbly” portion of that unit. This Navcam image clearly shows the boundary between the smooth and pebbly portion of the unit and the large blocky portion we are investigating on this brief “toe dip” into the rubbly area. We will perform contact science with APXS and MAHLI on one of these blocks, termed “Beaupouvet,” and take Mastcam multispectral and mosaic images of it and other rocks in the workspace. ChemCam is acquiring passive spectra of its calibration target while the team investigates an issue with some observations last week. After contact science, we’ll drive back into the smoother pebbly portion of the unit as we continue to head for the sulfate unit higher on Mt. Sharp. On the second sol of our plan, we’ll have a sequence of activities to search for and image dust devils. We’ll also look for evening clouds, which typically become more abundant this time of year as we approach the northern hemisphere spring equinox on Mars.

January 25, 2021

To Dip a Toe or Not To Dip a Toe…

Written by Susanne Schwenzer, Planetary Geologist at The Open University
One of Curiosity's wheels is visible on this image of Mars

This image was taken by Left Navigation Camera onboard NASA's Mars rover Curiosity on Sol 3011. Credit: NASA/JPL-Caltech. Download image ›

Today’s title image shows how diverse the area is that Curiosity is currently travelling through, with a part of a wheel for scale. A close look such as this one reveals all the different textures of rock surfaces, sets of ripples, some big rocks and small pieces of rock accumulated in patches.

Today’s discussions started with some strategizing as to if to make a short excursion, nicknamed the "toe dip," in tosols’s plan or in the weekend plan. This "toe dip" is a very short deviation from our current drive route to investigate a nearby unit, in fact the contact between the unit Curiosity is standing on top of right now and a neighboring unit. These contacts between two units are always of high interest to any geologist. At contacts, we can learn so much about the succession of processes that shaped the geologic environment at the time the sediments were laid down, and well before they became rocks. Or, in fact, well before at least the upper one of them became a rock, because at a contact, a geologist can find out, if the upper unit was deposited before or after the lower unit became a hard rock. And of course, we can see, if the laying-down of the upper unit had any influence on the lower unit, or if the upper unit includes pieces of the lower unit, or if the upper unit sealed off some water flow from below and caused mineral precipitation – just to name a few of the things geologist look out for at a contact between two units.

But back to today’s plan: Yes, we decided to drive to the area for the toe dip tosol. APXS and MAHLI are investigating a target “Champagnac,” which is a large piece of rock in the multitude of options in today’s workspace, which had made itself interesting by its darker color, which could indicate a change in chemistry from the usual-colored rocks we have been investigating lately. Mastcam and the Navcams are again getting very busy this sol, with the usual workspace survey and post drive imaging to prepare the next sol. On the science activities, Mastcam will investigate the area around a target “Marnac” by executing an investigation in multispectral mode with added stereo images, as well as perform a mosaic at the area the rover will approach for the ‘toe dip’ to the contact with the nearby unit with a set of seven images.

Of course, Curiosity is doing her regular atmospheric monitoring. For this, she will image across the floor of Gale crater to see how much dust there is in the air between the rover and the distant crater rim, and she'll image toward the sun to measure the dust load in the atmospheric column. In addition, she will do image sequences to survey for clouds, dust devils, and dust lofting over the "Sands of Forvie." Other regulars include MARDI, which takes its usual image after the drive, and DAN, which surveys for water in passive mode. Another busy sol on Mars – and off she goes to dip a toe onto the contact nearby.

January 25, 2021

Sols 3010-3012: Bonjour, Nontron (Mars)

Written by Ashley Stroupe, Mission Operations Engineer at NASA's Jet Propulsion Laboratory
A view of Mars

This image was taken by Right Navigation Camera onboard NASA's Mars rover Curiosity on Sol 3008. Credit: NASA/JPL-Caltech. Download image ›

Curiosity is continuing to make her way through the fractured intermediate unit toward the sulfate unit. After an 80-meter drive in our last plan, Curiosity has officially crossed into the new quadrant “Nontron” and parked with this amazing view (see image). And after more than 1000 sols visiting Scotland, Curiosity is now learning French! There are more details about this new Nontron quadrant in the Sol 3007 blog.

Curiosity will be starting off the weekend taking a 360-degree, 120-frame Mastcam panorama of this spectacular location, along with some more close-up images of rocks in the rover’s vicinity. These other observations include a bright-red rock in the workspace called “La Rogue Gageac” and some pebbles (to look at movement and stratigraphy). Later on the afternoon first sol, Curiosity will be doing contact science on two targets, La Rogue Gageac and one a normal-colored rock named “Gageac et Rouillac.” We’ll brush La Rogue Gageac in order to make sure we are examining a clean surface. Then, both targets will be examined with MAHLI and APXS. This will help us to understand the local variability, as well as fit in to our regular cadence of observations to track changes in the geology and mineralogy along our route.

On the second sol of the plan, Mastcam will do an additional multispectral image of La Rogue Gageac. Then, MAHLI will take a close-up look at the middle wheel in order to examine recent changes in wear seen in recent imaging. The wear doesn’t present a risk or concern, but these additional images from another angle will provide more data and insight to the engineering team. Once the arm is stowed, Curiosity will resume the trek toward the sulfate unit. Today’s drive is about 50 meters along our strategic route. The terrain is challenging, being ridged and rocky, giving the rover drivers a fun challenge. The drive is skirting around a ridge that we can’t see behind, in order to remain mostly on the terrain that we can see and characterize. The rover will be driving through a patch that is occluded from our current location, so the rover planners are using guarded driving, which allows Curiosity to evaluate the path ahead for hazards.

The third sol will include a lot of untargeted observations, mostly geared toward environmental science. Observations include early morning line-of-sight, zenith, superhorizon, and dust devil images with Navcam, a solar Tau and crater rim extinction by Mastcam, and a lot of DAN, RAD, and REMS as always.

January 20, 2021

Sols 3007-3010: Rocketing East

Written by Michelle Minitti, Planetary Geologist at Framework
Part of Curiosity rover is visible in this image of Mars

This image was taken by Left Navigation Camera onboard NASA's Mars rover Curiosity on Sol 3005. Credit: NASA/JPL-Caltech. Download image ›

Long before Curiosity landed on Mars, the science team mapped the landing ellipse covering the area within Gale crater that the combined efforts of Jet Propulsion Laboratory engineers, orbital mechanics, and atmospheric dynamics would lead us to touch down within. To divide the work of mapping among the team, the landing ellipse was divided into quadrants, squares 1.5 km on a side. Each quadrant was named after a significant geologic terrain on Earth, where geologists also divide the terrain they explore into quadrants. The practice of dividing the terrain Curiosity explores into quadrants continued after Curiosity departed the landing ellipse, to not only help focus mapping and path planning efforts, but to serve as a source of the names we assign to targets imaged, shot, drilled, or scooped.

We entered the "Torridon” (Scotland) quadrant on Sol 1896, and save a northward jaunt back into the “Biwabik” (Minnesota, USA) quadrant for 70 or so sols, we have remained in the Torridon quadrant. Over this time, all the targets we have named have required pages and pages of place names from Scotland (and Scotland adjacent) provided mostly by our team member Dr. John Bridges (University of Leicester). Those lists have produced great target names like “Muckle Flugga,” “Oban,” and “Bogmill Pow.” But in the drive in today’s three sol plan, we are due to exit the Torridon quadrant and enter the “Nontron” (France) quadrant where our French ChemCam teammates will help us with our target pronunciations. The Nontron quadrant name is particularly appropriate for the clay-bearing terrain we find ourselves in, as Nontron is the type locality for a clay mineral called nontronite. Nontronite is part of the smectite group of clays, which are the most common types of clays on Mars. The science team decided to send the Torridon quadrant out with a bang - literally - using the name “Saxa Vord Spaceport” for a ChemCam target. Using the name of an in-the-works satellite launch site in northern Scotland also represents the speed at which we are rocketing toward the sulfate unit, having completed a nearly 100 meters drive in the last plan, and looking forward to a ~75 meters drive in this plan.

While undoubtedly the coolest name in the plan, Saxa Vord Spaceport was far from the only target name used in our busy plan. ChemCam will also shoot bedrock targets “Easthouses” and “Jarishof,” and one of the fields of pebbles (“Whaligoe”) that we commonly see distributed in discreet patches (like in the image above). APXS, MAHLI and Mastcam will get a closer look at Easthouses after ChemCam shoots it. Mastcam also planned images of the terrain around us near and far. Mosaics of “Sandsayre” and “Rackwick” to rover left and right will record bedrock textures and structures, a mosaic of the more distant “Cromalt Hills” will capture their vertical structure, and yet another mosaic will image the contact between the fractured intermediate unit we are currently driving through and the rubbly version of this unit that we recently explored.

On each sol of the plan, DAN will seek the signal of hydrogen in the ground below us using both their active and passive modes, REMS will record the weather conditions, and RAD will monitor the radiation environment. These systematic measurements are complemented by images from Navcam and Mastcam that will hopefully capture clouds and dust devils and will measure the amount of dust in the skies above all the quadrants in Gale.

January 19, 2021

Sols 3003-3006: On the Road Again

Written by Vivian Sun, Planetary Geologist at NASA's Jet Propulsion Laboratory
This image was taken by Chemistry & Camera (ChemCam) onboard NASA's Mars rover Curiosity on Sol 3001.

This image was taken by Chemistry & Camera (ChemCam) onboard NASA's Mars rover Curiosity on Sol 3001. Credits: NASA/JPL-Caltech/LANL. Download image ›

We began planning today with the good news that we received some of the previously expected data and could plan “targeted” observations on specific targets identified in the new images. One catch was that higher-resolution workspace images, a pre-requisite to using the rover arm’s Dust Removal Tool (DRT), were not received in time for today’s planning, but we were still able to plan a plan chock full of remote sensing and contact science without the DRT. Today’s plan covered four sols, one sol longer than our usual 3-sol weekend plans due to the US holiday on Monday.

The APXS and MAHLI target of choice this weekend is a target called “Tomb of the Eagles,” which will give us high-resolution composition and image data over the typical bedrock at this location. ChemCam will also acquire measurements on Tomb of the Eagles, which is useful for comparing observations from different instruments on the same target. Other planned ChemCam observations of “Geocrab,” “Parallel Roads,” and “Watch Stone” also aim to characterize the compositional variability of the local bedrock, including nodular and veiny textures that have been previously observed in this area (see image above). The latter two targets were selected for especially long rasters (20 points instead of the usual 5-10) in order to better characterize chemical variability in these rocks. Mastcam will also be busy this weekend, taking documentation images of automated ChemCam AEGIS observations from the previous plan as well as of a possible meteorite, “Obar Dheathain.” We will also take two larger mosaics of the local landscape in stereo coverage, which is useful for assessing the 3-dimensional properties of these rocks. One mosaic is on the exposed outcrop right next to our workspace; these outcrops appear as ridges in orbital images and on-the-ground images will help us determine how these ridges formed. The second mosaic looks farther away at the contact between the fractured intermediate unit and the rubbly unit on top of it. Other activities in this weekend plan include a routine APXS calibration activity, and many atmospheric observations monitoring the environment, including Navcam movies, dust devil surveys, and Mastcam taus. On Sol 3005, we will drive and continue our path to the sulfate-bearing unit. On Sol 3006, we will let Curiosity take a breather, with just REMS atmospheric measurements and basic engineering activities in the plan. After this long weekend, Curiosity and her planning team will return refreshed for more planning next week!

January 13, 2021

Sols 3001-3002: Hold Up!

Written by Mark Salvatore, Planetary Geologist at University of Michigan
Black and white image of Mars

This image was taken by Front Hazard Avoidance Camera (Front Hazcam) onboard NASA's Mars rover Curiosity on Sol 2999. Credit: NASA/JPL-Caltech. Download image ›

After each time Curiosity finishes a drive, the science team eagerly awaits the downlink of what is termed “post-drive imaging,” or PDI, to visualize our surroundings and to target areas of the surface for investigation. Sometimes, the expected PDI downlink is delayed, which can happen for a variety of fairly benign reasons related to hiccups in the communication pipeline (speaking with Mars can be challenging!). Today, unfortunately, was one of those days. The team didn’t get all the data down that they wanted, including imaging data that we need to plan our next drive. This means that the science team was tasked with planning several “untargeted” scientific investigations that do not rely on detailed positioning information and targeting data. Our next drive will wait until the next planning cycle.

Despite this “hiccup,” the science plan is full of some important activities. For example, we will be acquiring four sets of ChemCam LIBS chemistry observations of the surface using the Autonomous Exploration for Gathering Increased Science, or AEGIS, targeting system. This is a remarkable piece of software that allows for ChemCam to automatically identify targets of interest and acquire data without the need for human involvement. We will also be acquiring two sets of calibration observations for the ChemCam instrument - one “passive” set that only uses the instrument’s point spectrometer, and one “active” set, which uses the laser induced breakdown spectroscopy (LIBS) system to generate detailed chemical information. In addition to these calibration sequences, the environmental team will also be conducting a suite of atmospheric observations including the collection of a dust devil survey using Curiosity’s navigation cameras and observations to characterize the atmospheric dust content. Leave it to a bunch of really smart scientists to plan a packed two days of science observations without having imaging data to tell us exactly where the rover is located!

January 12, 2021

Sols 2999-3000: 3000 Sols of Exploration!

Written by Lauren Edgar, Planetary Geologist at USGS Astrogeology Science Center
A view of Mt. Sharp on Mars

This image was taken by Right Navigation Camera onboard NASA's Mars rover Curiosity on Sol 2997. Credit: NASA/JPL-Caltech. Download image ›

Three thousand sols and never a dull moment! Today we planned Sols 2999-3000 and it was a real reminder of how complex and rewarding this mission can be. Curiosity has recently completed an investigation of the “Sands of Forvie” ripple field and we are working our way back to the path that we plan to take to ascend Mt. Sharp, transitioning back into terrain with fewer broken blocks of bedrock. In the previous plan, Curiosity shifted slightly when we first unstowed the arm for the contact science activities. When the flight software detected this small but unexpected movement, the rover stopped moving the arm to await further instruction from Earth. This is exactly what we designed the software to do to make sure everything stays safe, and it means we didn’t carry out subsequent contact science or the drive over the weekend. This is a good safety check, and a reminder of how we’ve made it to Sol 3,000 with a healthy rover by making good decisions and making sure we’re on stable ground! All is well and it just means that today we have a familiar workspace and a chance to regain some of these observations before getting back on the road.

Today’s two-sol plan starts with ChemCam observation of the targets “Queyon” and “Longa Skerry” to characterize the various textures and diagenetic features present in the bedrock. Then Mastcam will acquire a multispectral observation of “St. Andrew Square” to assess some interesting color variations, and later in the afternoon MAHLI will take a closer look at targets named “Nugarth” and “Kleber.” The second sol includes a ChemCam observation of “Backagord” and a number of environmental monitoring observations to search for dust devils and monitor the dust content of the atmosphere. Then Curiosity will drive to the north to get back into smoother terrain, followed by imaging to prepare for targeting in the next plan. The next morning Curiosity will acquire a ChemCam passive sky survey to assess water vapor and dust in the atmosphere.

It’s been an exciting 3,000 sols so far, and I look forward to seeing what else we’ll discover as Curiosity continues to climb Mt. Sharp. Tonight I’ll be raising a glass to Curiosity and the science and engineering teams that have gotten us this far!

January 8, 2021

Sols 2996-2998: Retracing Our Steps

Written by Abigail Fraeman, Planetary Geologist at NASA's Jet Propulsion Laboratory
Mars terrain as seen by the Front Hazard Avoidance Camera

"Hazcam the scuff on top of a scuff," is an image taken by Front Hazard Avoidance Camera onboard NASA's Mars rover Curiosity on Sol 2995. Credit: NASA/JPL-Caltech. Download image ›

As we were finishing up our measurements at the “Sands of Forvie,” we decided to give the sand one last good kick – er, scuff – on our way out. We received images of the new scuff this morning, and it gives us an even closer look into the ripple’s interior, which will help us understand its structure. After the scuff, we planned to retrace our steps and get in position to study some rocks we’d seen from our previous sol 2977 parking location. This morning, we were happy to see the small rocks we had been targeting were indeed in our workspace. I think it’s really amazing that the rover drivers were able to place Curiosity in front of these centimeter sized objects completely autonomously AFTER scuffing the sand and then driving more than 20 m over Martian sand and rocks.

Today we planned MAHLI and APXS observations on two rocks in our workspace, and we named the spots we observed “Nugarth” and “Kleber.” We’re also going to study the rock with the Kleber target in two additional places using ChemCam, and we named these new spots “St. Andrew’s Square,” and “St. Vigeans.” We’ll finish up our characterization with some multispectral observations that will tell us about the color properties of the rocks, and in addition to more targeted Mastcam mosaics to observe other features in the area in color at high resolution. Finally, we’ll take some long distance RMI mosaics looking higher up Mt. Sharp and perform a variety of environmental science observations, including studying the composition of the atmosphere using SAM. After completing our observation, we’ll pack up and hit the road once more, driving more than 60 meters back to our strategic route and onwards to the sulfate unit!

January 6, 2021

Sols 2994-2995: Scuff the Scuff

Written by Fred Calef, Planetary Geologist at NASA's Jet Propulsion Laboratory
Close-up view of a ripple crest

A close-up MAHLI view of a ripple crest at the edge of the "Sands of Forvie." Credit: NASA/JPL-Caltech/MSSS. Full image and caption ›

The "Sands of Forvie" campaign continues on with further exploration of the ripples and sand disturbed by a previous wheel scuff. On sol 2994, ChemCam targets include "Tiroran" and "Trearne Quarry" looking at sand grain chemistry with respective Mastcam color documentation. A new MAHLI image of "Traquair" will provide another close-in view of sand grain color and morphology. Interestingly, on sol 2995, we'll turn the rover in place to re-scuff a ripple to provide a three dimensional view into how the sand grains built up over time. During the turn, we'll take a mid-drive Mastcam mosaic of the new scuff area. Afterwards, the rover will take Mastcam images for ripple change detection, a clast survey, a MARDI image, and a Navcam dust devil survey.

January 5, 2021

Sol 2993: Taken With a Grain of 'Sand'

Written by Lucy Thompson, Planetary Geologist at University of New Brunswick
surface of Mars

Front Hazcam image of the APXS on the “Ratharsair,” trough target after overnight analysis in the previous plan. The ripple crest, along which the “Airor” crest target is situated, to the left of the arm. The disturbed scuff can also be seen between the two front wheels. Credit: NASA/JPL-Caltech. Download image ›

We are in the midst of a mini-campaign to further examine eolian (wind erosion, transport and depositional) processes on Mars. Curiosity is parked on a dark sand sheet investigating the composition and texture of the sand grains from different regions of the sand sheet, as well as any current motion of sand grains. Yesterday, Curiosity imaged a coarser grained, darker ripple crest (“Airor”) and a finer grained, redder trough area (“Ratharsair”) with MAHLI, and investigated the composition of the trough target with APXS. In the plan today, those images will be utilized to take even closer-up, higher resolution images of the crest and trough targets with MAHLI. These will facilitate detailed analysis of grain size, shape and colour. The APXS will analyze the composition of the trough target in this plan, and differences in the chemistry between the trough and crest can then hopefully be linked to grain texture and eolian processes. We also planned ChemCam LIBS measurements and accompanying Mastcam documentation imaging of the “Kames Bay” sand target. In order to look for motion of sand grains, Mastcam and MARDI change detection images will be taken at approximately the same time of day as they have been in the previous few plans.

As the APXS strategic planner, not only was I involved in helping to oversee today’s APXS activities, but also in the pre-planning of upcoming APXS observations for the next plan. We will try to get APXS compositional data on an area disturbed and scuffed with the rover wheels before driving away. This should allow us to compare the composition of the surface of the sand sheet with the subsurface, perhaps providing further insights into eolian processes.

The environmental group planned standard observations to monitor the atmosphere including Navcam suprahorizon and dust devil movies. Standard REMS, RAD, DAN passive and active measurements will also be acquired.