ZOMG
We're actually backtracking?!?! What have they done with Ken Farley - has he been kidnapped?? He'd never stand for actually going back and deviating from the Mission Plan...
One pill makes you larger
and one pill makes you small
and the ones that Mother gives you
Don't do anything at all
When lost on another planet, our little green friend reminds us: Remember your training. Save you it can.
I'm not surprised that Mars Guy is going back to the textbook, so to speak, because we just don't have experience with a geologic setting quite like this - the moderately well-preserved rim of a ~50 km-diameter impact crater - from prior Mars exploration or Apollo (Earth, of course, has done a lousy job of preserving craters of this size). The closest example is Opportunity's exploration of Endeavour Crater, which is much smaller, with a far smoother, more degraded rim. Apollo 15 landed near the edge of the Apennine Mountains, formed by the immense Imbrium basin impact (~1100 km diameter), but the astronauts didn't have the chance to ascend the foothills to any great height during their short and very busy stay. Opportunity had access to extensive outcroppings of bedrock at Endeavour, not to mention the kind of smooth, light-toned "paver stones" that Curiosity and Perseverance have been driving over for years. The Apollo astronauts saw nothing of the kind, unsurprisingly - the Moon being completely blanketed by that powdery surface.
Those other landing sites feature nothing quite like the distinct, boulder-studded knolls and ridges that Percy is investigating, which seem related to the original crater formation process itself. These gentle hills roughly follow the regional SW to NE trend of the rim mountain Percy is climbing (zoom in just a bit on the ESA map to see the steep face of the spur north of the rover), and several feature intact, massive blocks of bedrock that I'd love to sample (see Paul Hammond's Pico Turquino post for the best example yet). Good episode by Mars Guy, and I can't disagree with him here for the most part, but believe me, he isn't laying the hardcore stuff on us yet: impact crater geology melts brains, not just rocks!
All of the above vignettes were cropped from Front Hazcam images taken on Sol 1308, at about 1 PM local time.
Given that the sun was roughly behind the camera and rover when these images were captured, the complex, light-toned surfaces of these rocks stands out, with glinting reflective patches evident, especially toward the top of the hill. I'd be intrigued to view these rocks in the late afternoon, when shadows are longer and the dusty skies of late winter aren't layering that soft sheen over everything. Given the aggressive driving schedule that the rover team has adopted for climbing the Jezero rim, though, I'm not sure that Percy will stop here for very long...
I'm afraid I can't upvote this sentiment, Paul. I feel like we need to get you to, I don't know, the Atacama? Utah, Kazakhstan, Western Australia? Nunavut, or the Dry Valleys? OK, all those places are a bit much on the oxygen and the humidity, and you wouldn't be tasting the grit and dust in your mouth, but surely they could provide some respite to weary Martians? Dear planetary science community: remember the Paul Hammonds of this world as you work! We're not mathematicians or pure theorists - planets fully engage the senses, and some people have been waiting a long time!
(TBH, I really go back and forth on the wisdom of sending astronauts ASAP, as certain incautious parties advocate. We should have done one sample return mission already - the easiest and arguably most relevant to astronaut safety was unwisely cancelled by NASA and has never been revisited, for reasons I can't understand - and I long to get those cores from the Jezero basin back. I'd really give up a lot to have them, and I often think it'd be irresponsible to send people before we've assessed the toxicity of the regolith and dust. Still, the 1960s show me how important it is to have urgency, too. I'm assuming it was incredible fun to watch the entire lunar program evolve out of nothing, and even the Voyagers launched when they did to hit a deadline. I can't imagine where this science would be without Apollo or Voyager!)
Are we really passing up all those tasty-textured boulders on the hill??
Come on, rover team! If you won't give Percy the pleasure, send me! I'll core those rocks for free. We really need astrogeologist boots on the ground...
This shot was taken by the arm-mounted WATSON camera at 10:46 PM local time, illuminated by the LED (see also shots lit from the left and right, for perspective). The boulder Percy is analyzing (see here for a daylight view) isn't as reflective as some near the rover, but then again, this part of the Jezero rim seems to have more than enough funky rock coatings for anyone!
Thanks for posting these. Do you prefer this JPL version of the overhead view to the contour-lined ESA one?
You mean "notional path to the SSW", Paul, no?
I can't find any evidence that the triangular-prismatic rock at the top centre of this image even existed before Sol 1292 (apparently visible on the left hump on the horizon in this image)... are the Martians watching us???
(To be clear, I am joking here. I just think it's really neat to see how many of these cobble and boulder-studded slopes on the Jezero rim produce these angular and seemingly resistant forms. Martian hills and mountains are pretty rounded in general - I'd hardly expect to find the Matterhorn in these ancient landscapes - but erosion has a way of surprising you in this place...
STOP STOP I'M GETTING A NOSEBLEED
(OK, I know Opportunity was a lot higher up in elevation. But that's not a fair comparison - "Oppy" was born lucky and everybody knows it. The wind was always at that rover's back and it never had to land in a 1500 km-wide hole punched out of the highlands...)
YouTube Video
Click to view this content.
Warning: the video features an undignified view of the rover from about 2:10-2:30. Don't say we didn't warn you.
Don't be all proud of yourself. The rover drivers will be given control of the death ray (sorry, the "breakdown laser spectrometer") when they summit the rim as a reward for their hard work. They'll be carving out the words, "We Persevered, ******s" into the finest basement rock any rover has ever tasted.
Beat that.
Oy. Less than 5 vertical m cleared after a whole week of short slippy drives. I'm not sure what I was expecting to find on this rim, but this terrain wasn't it.
EDITED TO ADD: I meant - only 5 m on this drive, after a whole week of slippy drives, with less than 10 vertical m cleared on any one drive. And this is hardly the softest-looking crater rim we've seen on Mars...
While I'm being chatty, I'd like to ask you if you have any suggestions re: contributions to this community or instance or whatever we call it. I often see things in the raw images that I feel like pointing out here. In reading social media since this mission started, though, I see vast knowledge gaps in people's understanding of basic geology (or "earth sciences", if we can use that term for Mars - maybe "environmental sciences" is a better term), and I sometimes feel I should try to shine a light in those gaps. I've thought about breaking down some of the big science papers/results from this mission here, but I wanted to ask you about this first, as I think you have a better feel than I for what people might be interested in actually reading.
You're talking sense, Paul. As you say, opinions certainly differ, especially among people of different scientific disciplines (e.g. meterology vs. geology), and that even extends to the mission PIs. Steve Squyres was certainly driven and focused in achieving his science goals, which meant that the MER missions drove hard as well. John Grotzinger was criticized for not connecting the dots and "lacking focus" on a big flagship rover. From everything I've seen and heard, Ken Farley is being more careful in balancing priorities (and I'd say his job is a lot harder here, considering the needs of sample return!) All that being said, even pure geologists will certainly disagree amongst themselves, though we don't see that here as interested members of the public.
I'm not privy to the inner workings on this project by any means - certainly not directly. Having observed prior missions from a somewhat closer perspective, however, I see Mars 2020 as very, very driven by the work of other missions and a surprisingly broad community. Orbital spectroscopy and geologic mapping has guided this rover in detail from the very start, to a degree greater than I remember even for MSL, and I'm not aware of much debate about the rover's planned route at any point since before landing. I was personally quite surprised by the short amount of time that Percy spent in Neretva Vallis (amazing place!), to say nothing of acquiring only one sample. Yes, there aren't many spots as interesting as Bright Angel along the traverse path, but I still don't agree that one sample was enough, and I somehow doubt that I'm alone in that opinion.
I've seen dust storms before - the largest ones, the global ones, even through backyard telescopes. If you're working right on the surface, they're not fun.
I'm not often surprised anymore by whitish or light-toned materials near a rover since Spirit uncovered all that whitish silica with its dragging dead front wheel, all those years ago. It seems we often find that Mars is red only until you literally scratch the surface.
I have to say that Percy often drives right past plenty of rocks I'd like to investigate more. I know that Ken Farley et al. are doing just that with remote sensing (the results of which we aren't privy to for quite a while), so they have some idea of what they're looking at, but I'm often tantalized by a lot of this stuff.
For God's sake, stop it with the conspiracy theories. Trace Gas Orbiter would absolutely not miss the, well, methane emission, from a single baby cow, let alone an adult specimen worthy of being prepared as wagyu. Everyone knows that a Japanese master chef would quit (or worse...) before disgracing himself thus. He would never abandon a thickly-marbled specimen on a great big windy crater rim like this.
This is Mars. If you want your vulgar gyudon, there's plenty of that on the mad blue planet next door. Martian wagyu should be part of the finest sukiyaki, to be eaten in formal dress, in deeply contemplative silence.
... I should add - if you can get a sample of this rock for us, we'll even let you eat part of it. It might be a bit salty, but you can be pretty sure Martian beef is nitrate-free...
The idea that this "zebra" or "bad camo" rock could be metamorphic is really something, an interpretation I didn't even seriously consider. If this is metamorphic, one would think at first glance that it isn't more of the same material we've sorta-detected on Mars already, which is probably the hydrothermal or shock metamorphic kind. Mars Guy considered metamorphic rock in his last video only to discard it...
Then again, the Nili plateau region just beyond the crater rim is supposed to be so damned old, even for Mars, that it could preserve evidence for all kinds of craziness, and I'm not sure we can rule out that this rock isn't impact ejecta from the plateau. Maybe this thing doesn't preserve evidence for something as Earth-like as plate tectonics, but that banding pattern needs a deeper look. It may not be a match for the neatly-striped metamorphic rock of Earth, but Martian metamorphism that may have occurred deep within the crust is something we shouldn't ignore. At the very least, I'd like Mars Guy's comparison of this rock to freaking dolomite to be put to the test. There's more evidence for plate tectonics on Mars than there is for that stuff!😅
Last week, team scientists and the internet alike were amazed when Perseverance spotted a black-and-white striped rock unlike any seen on Mars before. Is this a sign of exciting discoveries to come?
> The science team thinks that this rock has a texture unlike any seen in Jezero Crater before, and perhaps all of Mars. Our knowledge of its chemical composition is limited, but early interpretations are that igneous and/or metamorphic processes could have created its stripes. Since Freya Castle is a loose stone that is clearly different from the underlying bedrock, it has likely arrived here from someplace else, perhaps having rolled downhill from a source higher up. This possibility has us excited, and we hope that as we continue to drive uphill, Perseverance will encounter an outcrop of this new rock type so that more detailed measurements can be acquired.
I'm assuming this is one of the larger climbs/vertical displacements that Percy has managed in a single sol. This old crater rim is definitely the steepest terrain the rover has tackled, which might limit the rover's progress on driving days, but I wonder if the all bedrock we've encountered along the way is enticing the scientists enough to take it slower.
How like you people to constantly reference your tired, dirty terrestrial examples, your lousy "Earth analogues". Anyone that's been paying attention knows that Martians craft things like the ultimate artisans they are, applying the most gentle and skillful touch, tentacles perfectly co-ordinated. Humans go on and on about the "Inca City" and the "Face on Mars", but Martians work every crevice of every worthy rock.
If Earth had a real space program, or just real science, you'd see them dancing on every dust mote, and you might even catch them making lewd gestures when Perseverance fries yet another rock to "analyze" it, but you're too intent on your carbonates and silicates and phosphates...
Nuclear-powered. Ridiculous.
No, I'm not calling this a "potential biosignature" 😆
Mars Guy has documented some of the rover team's prior work on coated rocks, although I don't remember seeing any examples this visually striking.
The coated rocks which have been documented prior to this one - none of which were nearly so patchy as this one, if I recall correctly - have been interpreted as a relatively thick dust coating formed by the action of water vapor, i.e. humidity. Mars should have had some fairly recent episodes of higher atmospheric moisture caused by the tilting of Mars' axis, which would expose the polar caps to more sunlight and temporarily humidify the atmosphere while the ice is being redistributed to the new polar latitudes.
We've never had any mission climb the rim of a crater as large as Jezero before... not on Mars, or even on Luna... I'd say it's been pretty fun so far!
And all the low-lying terrain in this image was under water...
I am fascinated by Mars as it is. Even so, this amazing image really forces me to stop, and stare, and imagine this scene, imagine Mars, as it was. It's artfully framed, yes, but I'm still stunned to visualize how those old, low, rounded-down ridges in the background would look entirely different if they were encompassing open water. Every time you think you're starting to understand Mars...
I have seen thousands upon thousands of still frames from the MER, MSL and Mars 2020 missions, but very few that take the perspective seen above. I find it practical and useful for the following reasons:
- Seeing exactly which clasts and sand ripples have been in contact with the rover (notice the pebbles and cobbles that have been pushed into sand, exposing darker material). The rover's tracks aren't always evident, and this helps.
- We can easily see the state of the wheels
- We get instant perspective on the size of surface features
- We can observe sedimentation on the rover (how much sand/dust is coating it) through time
However...
Shots like this are just really cool. People already anthropomorphize rovers (and Ingenuity), because we like seeing ourselves on other worlds by proxy. People also like monster trucks, mudbogging, ATVs, and just plain getting dirty. Mars is known for being cold and arid, but the truth is, barring any possible toxins in the soil or dust, it's really a place for big kids! Geologists aren't the only ones who like to play in the rocks. There's a whole culture out there that likes to put metal to dirt or hard stone, and I don't feel like we reach them enough. More of these, please!
After reporting a while back that the SHERLOC instrument was inoperable due to a stuck, half-open dust cover, it seems that we're back in business, based on the latest images from Sol 1076 (29 Feb 2024).
I'm not sure if the engineering team will decide to leave the dust cover open, but I do know that the science team could really, really use SHERLOC, which can (and has) identified organic molecules in the rocks, including the samples we've collected. With Ingenuity losing its "wings", we can all use good news from Jezero!
Comparing recently downlinked images from Sol 1069 (22 Feb 2024), the partially closed (and apparently stuck) dust cover for SHERLOC seems to have opened by a few more degrees.
SHERLOC is one of the mission's primary instruments, used to detect organic molecules and identify minerals. Losing the full use of this instrument would be a problem.
The following sequence of images, taken several minutes apart, will show the dust cover's motion:
https://mars.nasa.gov/mars2020-raw-images/pub/ods/surface/sol/01069/ids/edr/browse/zcam/ZL0_1069_0761842926_818ECM_N0501618ZCAM05177_110085J01.png
https://mars.nasa.gov/mars2020-raw-images/pub/ods/surface/sol/01069/ids/edr/browse/zcam/ZL0_1069_0761844394_678ECM_N0501618ZCAM05177_110085J01.png
https://mars.nasa.gov/mars2020-raw-images/pub/ods/surface/sol/01069/ids/edr/browse/zcam/ZL0_1069_0761845258_706ECM_N0501618ZCAM05177_110085J01.png
Perseverance is deep within the ongoing Margin Unit campaign, where orbital signatures of carbonate minerals appear strongest.