“Honeycomb terrain” on Mars
Cool image time! The picture to the right, cropped, reduced, and sharpened to post here, was taken on June 30, 2026 by the high resolution camera on Mars Reconnaissance Orbiter (MRO). It shows what the scientists label as “honeycomb terrain,” though to think that explains what we are looking at is to live in a fantasy world.
I could easily place this image in my category of Martian “What the heck?!” images, pictures of geological features that defy any clear explanation at all. Near surface ice and glacial activity certainly played a part in forming this geology, as this location is at 39 degrees south latitude, well within the mid-latitudes of Mars where both are found routinely.
Crater impacts also played some part, or at least, some of the round depressions might have been formed by a bolide striking this ice-impregnated ground, causing it to quickly melt, flow, and then refreeze.
But why the swirls? That is a question I have no theory to explain. Nor does a wider look help much.
The white dot on the overview map to the right marks the location, about seven miles north of the downstream end of the glacial-filled canyon dubbed Dao Vallis, as it begins to drain into Hellas Basin, the death valley of Mars.
My first guess was that the swirls are the eddies of a glacier flowing inside a canyon, but these swirls are located on the plateau above the canyons to the south and to the east. Thus, if they indicate any flow patterns those patterns are not determined by any obvious downgrade.
MRO altimeter data suggests the flat mesa on the picture’s right is the high point — sitting about 100 feet above the surrounding swirls, with those swirls flowing around it. Yet that same data does not show any obvious downgrade in that surrounding flow.
MRO images of the western floor of Hellas basin, at its deepest point, show many features similar to these swirls that scientists have labeled “taffy terrain.” That taffy remains unexplained as well, though the present theory ascribes their formation to the flow of some “viscous fluid”, as yet unidentified.
The geology of Mars continues to baffle. It is strange and alien, though given time and some hands-on exploration, I am fully confident that future generations will untangle its mysteries.
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The best information I could find was that MRO has a vertical resolution of ~1m at the surface. The terrain looks to me like a slow flow of viscous fluid. It doesn’t take much elevation change at all to induce a liquid flow.
If this were Earth no one would look at it for more than a few seconds and decide that these are beachmarks caused by wind/water erosion, with the water level dropping down successively over time.
Since it’s Mars that not really a possible explanation.
Is it possible that successive layers of dry ice (CO2) were evaporated at different times, with the sand-blown grit eroding the edges?
It would be nice to get some geologists (Areologists?) down there to actually take samples, do some core drilling, and figure out what’s going on. Or maybe, what went on.