I don't think those huge chunks seen now on the twice the diameter size wheels can be explained as fine dust.
You're certainly not the first person to see this clingy fine dry dust do this and be convinced it has to be damp to behave like that. You certainy wont be the last.
h ≈ 500 / (1200 × 3.71) ≈ 0.11 m (11 cm)
Quote from: Holger Isenberg on 11/29/2025 08:25 pmNever before has this effect been observed on a Mars roverVery fine grained soil does that all the time. It's been seen on Mars rover wheels for 20 years. This article has a captioned image of it on the wheels of MER-B and MSL.https://link.springer.com/article/10.1186/s40645-025-00725-3 ( specifically figure 4 - https://link.springer.com/article/10.1186/s40645-025-00725-3/figures/4 ) 'Wet' clay isn't possible on the Martian surface. It would sublimate away in the heat of day and freeze solid any other time. The 'liquid' corner of the phase diagram of water at Martian air pressure is miniscule.https://en.wikipedia.org/wiki/Phase_diagram#/media/File:Phase_diagram_of_water_simplified.svgSee...https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2023JE007880 where you'll see data showing the ambient pressure hovers right around that triple point at Jezero.The 'looks like wet soil/mud' phenomenon has plagued those observing rover ops for two decades. The behavior of VERY fine grained, VERY dry fines is quite unintuitive. I'd suggest playing around with a tray of cornflower to understand just how clingy and clumpy it can be.
Never before has this effect been observed on a Mars rover
Perseverance is currently at an altitude of -1940 m, to liquid water is possible
Especially in saline, which will shift the lower phase diagram boundary to the left.
Quote from: Dalhousie on 11/30/2025 09:32 pmPerseverance is currently at an altitude of -1940 m, to liquid water is possible Yes. I said so earlier, citing the specific measured air pressure at the Jezero site. Which is JUST high enough to get into the liquid wedge of the phase diagram.QuoteEspecially in saline, which will shift the lower phase diagram boundary to the left.Such that every time it gets warm enough for liquid water, you're pretty much guaranteed to be hot enough to boil it off due to the low atmospheric pressure. Moreover - the back of that rover is the hottest thing on the entire planet. The wheels and suspension are anodized black to heat up in the sunshine - far warmed than the air temperature in the MEDA paper I cited earlier.There is an incredibly narrow window where something might be 'damp' - so the question then becomes, where did the water come from and how did it get there given that every day the surface temperature is more than enough to boil it off.If it were really sticky damp clay - it would stick around - it would happen all over the place. It only happens when driving over incredibly fine dust, when the drive ends without leaving that dust, typically across ripple formations, and then is gone a drive later.Once drive away from that find dust.....that wheel is CLEAN. If it were damp and clingy...it would still be there.https://mars.nasa.gov/mars2020-raw-images/pub/ods/surface/sol/01690/ids/edr/browse/ncam/NLF_1690_0816971842_895ECM_N0813608NCAM02690_10_195J01.pngMartian conditions are far less Earth like, and that material is far less familiar than I think you realize.
Rather than big bolts of lightning as seen on Earth, NASA’s Perseverance rover recorded audio of small zaps similar to those from static electricity
an 30, 2026This animation shows Perseverance’s point of view during drive of 807 feet (246 meters) along the rim of Jezero Crater on Dec. 10, 2025, the 1,709th Martian day, or sol, of the mission. Captured over two hours and 35 minutes, 53 Navigation Camera (Navcam) image pairs were combined with rover data on orientation, wheel speed, and steering angle, as well as data from Perseverance's Inertial Measurement Unit, and placed into a 3D virtual environment. The result is this reconstruction with virtual frames inserted about every 4 inches (0.1 meters) of drive progress.NASA’s Jet Propulsion Laboratory, which is managed for the agency by Caltech, built and manages operations of the Perseverance rover.For more about Perseverance: science.nasa.gov/mission/mars-2020-perseverance/Credit: NASA/JPL-Caltech
NASA JPL@NASAJPLPerseverance just did something it’s never done before.On Dec. 8 and 10, 2025, the Mars rover completed drives planned by generative AI. The first-of-its-kind demonstration hints at a future of more efficient exploration and even more science. https://jpl.nasa.gov/news/nasas-perseverance-rover-completes-first-ai-planned-drive-on-mars/
A new technology developed at NASA’s Jet Propulsion Laboratory in Southern California enables Perseverance to figure out its whereabouts without calling humans for help. Dubbed Mars Global Localization, the technology features an algorithm that rapidly compares panoramic images from the rover’s navigation cameras with onboard orbital terrain maps. Running on a powerful processor that Perseverance originally used to communicate with the Ingenuity Mars Helicopter, the algorithm takes about two minutes to pinpoint the rover’s location within some 10 inches (25 centimeters). Mars Global Localization was first used successfully in regular mission operations on Feb. 2, then again Feb. 16.
The upgrade is especially valuable given how well Perseverance’s auto-navigation self-driving system has been working.
The small team began working in 2023, testing the accuracy of the algorithm they’d developed using data from 264 previous rover stops. The algorithm compared rover panoramic photos to MRO imagery and correctly pinpointed the rover’s location for every single stop.
Tapping into the HBS computer has had its challenges. To address reliability, the team developed a “sanity check”: The algorithm runs on the HBS multiple times before one of the rover’s main computers checks to ensure the results match. During testing, the team repeatedly found the rover’s position was off by 1 millimeter.