paulhammond5155

joined 2 years ago
 

Left MastCam GIF of three frames shows the closed cover of SAM. The animation shows the cover before the drop, and then two portions of powdered rock are dropped onto the cover. This is performed to measure ensure they can deliver the correct amount of sample to SAM when the cover is opened.

Sample Analysis at Mars (SAM) Instrument Suite

Gas Chromatograph: Separates gases to aid in identifying them

Mass Spectrometer: Detecting key elements necessary for life (nitrogen, phosphorous, sulfur, oxygen and carbon)

Tunable Laser Spectrometer: Detecting water vapor and understanding the history of Mars atmosphere or determining whether methane, if found, is produced by life or geologic processes

Sample Manipulation System: Wheel of 74 small cups for samples (9 cups contain calibration samples; 9 filled with chemical solvents for lower-temperature wet chemistry experiments, and 59 quartz cups that are small ovens for heating the powdered samples to extract gases)

Sensitivity: Detects less than one part-per-billion of an organic compound

Ovens: Heat most rock samples to about 1,000 degrees Celsius (about 1,800 degrees Fahrenheit) to extract gases for analysis

 

Meanwhile on the planet Mars:

Curiosity Rover drills its 43rd sample hole during June 8, 2025 (mission sol 4564)

Attached is an animated GIF of 20 HazCam subframe images captured during the drilling process.

I've added the timestamps (local mars solar time) on each frame.

Watch the shadow of the robotic arm move and the drill bit sink into the rock. Look closely and you can even see the rover tilt as the load on the drill changes.

Credits: NASA/JPL-Caltech

Edit - HazCam

 

This week it's Curiosity's turn

 

A fantastic view from the Mars Curiosity Rover using its ChemCam remote micro imager (RMI), looking towards the distant Yardang Unit. Taken this week on Sol 4562 (June 6, 2025).

The mosaic was assembled from of 7 overlapping RMI images by Kevin Gill. Credits: NASA/JPL-Caltech/LANL/Kevin M. Gill

A yardang is an elongated ridge created by wind erosion. The Yardang Unit is a layer found at the uppermost reaches of the foothills at the base of Mount Sharp, a 3-mile-tall (5-kilometer-tall) mountain that Curiosity has been ascending since 2014. The colour, texture, and tilt of the layers in the Yardang Unit make it distinct from lower layers on the mountain. Mount Sharp is an exciting place for scientists to study because it's made up of a number of layers, each representing a distinct era in the climate of ancient Mars.

Curiosity Mars rover captured a colour view of the Yardang Unit using its Mast Camera back on November 2, 2024, (Sol 4352). The mosaic is made up of 18 images that were stitched together after being sent back to Earth. The colour of that mosaic has been adjusted to match lighting conditions as the human eye would see them on Earth. LINK

 

Mission update - Published June 6, 2025

 

NASA’s Mars rover Curiosity acquired this image of a recent DRT (Dust Removal Tool) site, showing off the marks created in the rocks by DRT — a motorized, wire-bristle brush on the turret at the end of the rover's robotic arm — as well as a whitish vein that was revealed after the dust covering it was removed. Curiosity acquired this image using its Mars Hand Lens Imager (MAHLI), a camera mounted on the turret at the end of the robotic arm, which provides close-up views of the minerals, textures, and structures in Martian rocks and the surface layer of rocky debris and dust. Using an onboard process, MAHLI merges two to eight images to make a composite image of the same target acquired at different focus positions, to bring many features into focus in a single image. Curiosity merged this composite on June 4, 2025 — Sol 4560. Or Martian day 4,560 of the Mars Science Laboratory Mission — at 12:33:42 UTC. NASA/JPL-Caltech/MSSS

Written by Conor Hayes, Graduate Student at York University

Earth planning date: Wednesday, June 4, 2025

We are continuing to look for a suitable location to collect a drilled sample in this area. As you may recall from Monday's plan, we performed a short “bump” of just under 4 meters (about 13 feet) hoping to find a drill target today after Monday's analysis determined that there were no good targets in our previous workspace. Happily, today's workspace was much more cooperative, and we were able to select the target “Altadena” as our next potential drill location. Altadena is a name that we've been saving for a special target, as its namesake here on Earth is a neighborhood next to JPL that was devastated by the Eaton Fire earlier this year. We’re about to enter our next mapping quadrangle, which will come with a new set of target names, so the team decided that using Altadena as the name for this drill site was an obvious choice.

The big activity in this plan is the next step in the drilling process. This activity is the “preload test,” which determines if the forces on the drill will be good while drilling, and the drill target won’t unexpectedly move or fracture. If we pass the preload test and find that the rock has the chemistry we're looking for, we'll be able to proceed with Altadena as our next drill site. If we don't, we'll have to decide whether to bump again or resume driving deeper into this potentially boxwork-bearing region.

Of course, the preload test isn't the only thing we're doing today. Coming in, it was looking like our time for other activities would be pretty tight due to power constraints imposed by preparations for drilling and keeping the rover warm during the cold Martian winter. However, we've recently implemented some new power-optimizing capabilities, which led to us having much more power today than we expected. This meant that we were able to add a whole additional hour of science time in addition to the hour that we already had scheduled.

Unsurprisingly, Altadena gets a lot of love in this plan to characterize it before we drill. This includes a ChemCam LIBS activity and a Mastcam observation, as well as some overnight observations by APXS and some MAHLI images. In addition, Mastcam will be observing some exposed stratigraphy at “Dana Point,” a light-toned vein at “Mission Trails” that will also be a ChemCam LIBS target, a few more nearby troughs, and a couple of sandy patches at “Camp Williams” to observe wind-driven sediment transport. Along with the two LIBS, ChemCam will be using its RMI camera to add to the pile of images we have of the Mishe Mokwa butte and the yardang unit off in the distance.

As the lead for the Atmosphere and Environment (ENV) group today, it looked like I was going to have a pretty light workload due to the power constraints preventing any ENV activities other than our usual REMS, RAD, and DAN observations. With the extra hour of science time, I was able to add a handful of new activities, including three Navcam cloud movies, a Navcam line-of-sight observation of dust within Gale Crater, and a Navcam survey to look for any dust devils that may be swirling around the rover. A pretty decent ENV science haul for a plan that started with nothing!

When we come into planning on Friday, we'll hopefully have passed the preload test and will be able to turn Altadena into our 43rd drill hole in the coming sols, before we continue driving up the slopes of Mount Sharp.

 

[5466x4790px] click through to see full size

[–] paulhammond5155@lemmy.world 6 points 3 days ago

Glad to help satisfy your curiosity. Feel free to ask additional questions, as there's a great community here that will try their best to answer questions.

[–] paulhammond5155@lemmy.world 11 points 4 days ago (3 children)

https://lemmy.world/u/Dicska

Water vapour has been condensed on a Mars lander, but never at these 'warmer' latitudes. The regions where NASA's rovers are exploring are much, much drier. Curiosity and Perseverance rovers have both conducted occasional searches for surface frost in the early morning, so far without success (AFAIK). The closest they've come to observing water is the super high elevation water ice clouds that have been imaged after sunset during seasonal changes in the weather.

The rest of the rover has patches of dust / regolith gathered on flat places (where it's not cleared by the wind or gravity).

The M2020 drill is the rotary-percussive type (Hammer Drill), and when it's coring or abrading it basically vibrated like crazy. So I assume that most of the dust that has accumulated on the surface of the drill, is shaken off every time it's operated. I've attached a tiled NavCam acquired at the current location 2 sols ago.

Technical mission docs provide loads of data for the drill e.g. - The percussion mechanism has a hammer mass is 200 g, the total spring stiffness is 11 N/mm, with the single-sided amplitude of motion at the base (i.e., crank shaft throw) being 5 mm and the static gap to the anvil is approximately 9 mm. The result is a system that first impacts with base motion (and impact frequency) of approximately 25 Hz and the corer typically operates the percussion mechanism between 25 Hz and 40 Hz. Impact velocities are typically between 0.5 m/s and 3 m/s but will depend on the effective coefficient of restitution of the system and other factors.

 

Here's a MastCam-Z image, checking out the condition of its rotary percussive drill and the abrasion bit used to create the patch. Credits: NASA/JPL-Caltech/MSSS

 

Meanwhile on Mars!

Perseverance rover images its latest abrasion patch. For scale the patch has a diameter of about 5 cm (2") This image from its SHERLOC WATSON camera was acquired on June 5, 2025 (Sol 1526) at the local mean solar time of 12:26. Credits: NASA.JPL-Caltech.

 

HazCam GIF using a few raw tiles shows the abrasion tool in action during sol 1525 (June 4, 2025) - NASA/JPL-Caltech

 

 

12 tile post-drive HazCam . Credits: NASA/JPL-Caltech

[–] paulhammond5155@lemmy.world 3 points 6 days ago

multiple columns are showing the same thing in a mix of units, hurts my head.

https://lemmy.world/u/Shadow

This should be easier to digest

[–] paulhammond5155@lemmy.world 2 points 6 days ago

At least it's recently stopped NSFW drawings :)

[–] paulhammond5155@lemmy.world 3 points 6 days ago

I've needed the excuse to simplify some of the data. Working on it :)

[–] paulhammond5155@lemmy.world 3 points 1 week ago

As you say if that was water / mud there would be a huge amount of excitement. They set up rules before landing in the event of discovering water or seeps etc that would require the rover to back away from the such area to prevent any bacteria etc that may have survived on the rover contaminating Mars. They could study such areas from a distance, but not perform contact science. However, the rover landed in 2012, and it would seem highly unlikely that anything from Earth could have survived that length of time in the temperature swings and radiation levels experienced by the rover, so those rules may have changed.

We'll get colour images in another day or so, but I think you'll see it's just rock with patches of sandy regolith. The large shallow depressions in the ground are thought to be formed by erosion resistant minerals that have been deposited by groundwater in the fractures in the bedrock surrounding the depressions. The science team are making measurements at each stop across these boxwork-like structures to confirm that theory. You'll get more detail in the mission updates posted in this community about the teams investigations and progress :)

[–] paulhammond5155@lemmy.world 3 points 2 weeks ago

It’s so shiny!!

It used to be a little less dusty. This was taken 9 days after landing

[–] paulhammond5155@lemmy.world 3 points 2 weeks ago

Fingers crossed 🤞

[–] paulhammond5155@lemmy.world 1 points 3 weeks ago

Tried to post this when it came out. Kept getting invalid URL.... Glad you managed it :)

Lemmy can be a pain sometimes...

Any idea how to post YT content so that it shows the video thumbnail ?

[–] paulhammond5155@lemmy.world 2 points 3 weeks ago

I’ll let you know as soon as I’m ready.

No problem! A very smart and kind user on Mastodon has just provided me with a link to the M20 traverse JSON. So I can now do away with several steps to get the start / stop times for each drive without having to extract the drive start / end times from the geojson from the map. Importing the start / end time is still manual, but it only takes a short time. From that data I can calculate drive time, speed (it's not quick a speedster :) ) but it may be of interest to some, I can also calculate the longest /shortest drive times, average drive times etc etc. Not sure yet what to use.

I'm hoping the 'Calc' team eventually creates an IMPORT JSON function, like the one that EXCEL has had for many years, once they do that, I can create a spreadsheet that automatically imports the data from several different JSONs after each drive and automatically populates the tables I share when the spreadsheet is opened. Until then, there will be some manual copy, convert and paste to do, but it literally takes an extra minute or two after the JSONs are published, and you're used to operating it.

Importing data manually is actually good practice, as you can see where the data comes from, and it's easier to fix in the event that JPL ever change the format of the JSONs. They did change the M20 JSON a couple of times (they added extra data fields) but the last time it was changed was a couple of years ago, the JSONs have been stable for quite some time. I didn't even notice they had changed it last time, as with the IMPORT JSON function I was using in my spreadsheet, I had specified which header fields I wanted to import, that option basically ignored the rest of the fields, only importing the fields that I needed at that time. So I did not notice the addition of the new fields, nor did their addition break my spreadsheet (a nice bonus being able to specify which fields you need, rather than importing all of them).

When you're ready for the spreadsheet, can let me know the browser you are using, and the spreadsheet package you intend to use, so I can tailor a set of instructions you can use to gather the data (JSON URLs etc) then copy, convert and drop it into the spreadsheet etc. When you open / load a JSON URL in different browsers, they can display the data with subtle variations, the LibreWolf Browser I'm using now is a little easier to use with JSONs :)

[–] paulhammond5155@lemmy.world 11 points 3 weeks ago* (last edited 3 weeks ago)

Local Mean Solar Time (LMST)

Read all about Mars time here...

https://www.giss.nasa.gov/tools/mars24/help/notes.html

"Mars 2020 (M20) - Perseverance: NASA's Mars 2020 Perseverance project specified Sol 0 as the solar day on which the rover would touch down, which occurred Feb. 18, 2021. During planning, mission controllers specified a mission clock commencing at midnight LMST for a landing site at 77.43°E. Landing occurred at 77.45°E, resulting in a difference of about 5 seconds between the mission clocks and the landing site LMST."

One of the images in this set was taken at 2025-03-01 18:37:44.42 UTC (copied from the image meta data)

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