NASA/JPL-Caltech/MSSS/fredk

  • SpecialSetOfSieves@lemmy.world
    link
    fedilink
    English
    arrow-up
    1
    ·
    8 days ago

    I’m not sure what you mean by “erosion patterns”. Are you referring to the layers (parallel and mostly curving lines) in some of the boulders?

      • SpecialSetOfSieves@lemmy.world
        link
        fedilink
        English
        arrow-up
        2
        ·
        edit-2
        8 days ago

        Right, the layering/bedding. I see why you’d define those as grooves. Generally speaking, for sedimentary rocks (which these are), some layers “stand out” because they’re more resistant, and some get eroded more easily, making little ridges, which creates the contrast you’re seeing.

        I’ve never thought of them as soothing before - but yes, the more rounded ones remind me of underwater sand ripples you’d see in a river or large body of water, which is pretty calming, isn’t it? And since there was so much water in Gale Crater, once upon a time…

        EDITED TO ADD: On Earth the “stair-step” pattern that comes to mind for that is shale, but there are plenty of examples!

        • hsdkfr734r@feddit.nl
          link
          fedilink
          English
          arrow-up
          2
          ·
          7 days ago

          some layers “stand out” because they’re more resistant, and some get eroded more easily, making little ridges, which creates the contrast you’re seeing.

          I once saw a granite rock face with lots of sharp pointy spikes. The limestone was already eroded away. It was very exciting to step on it. :)

          yes, the more rounded ones remind me of underwater sand ripples

          Yes, the combination of texture, form and color does it for me.

          about erosion: can cosmic radiation, infrared light, and heat fluctuations cause erosion, too?

          • SpecialSetOfSieves@lemmy.world
            link
            fedilink
            English
            arrow-up
            2
            ·
            edit-2
            6 days ago

            Hmm. Well, infrared (from the Sun) and other sources of heat definitely eat away at ice, but that’s more of a thing near the south pole, where the CO2 ice goes away every spring. Rocks have been known to crack due to repeated heating and cooling, yes, so you’ve got the first part of erosion, the breaking part. Moving/transporting broken fragments is another matter, though.

            Cosmic rays do cause damage to rocks, but on a much finer scale than the cracking referred to above - you’re not going to get big chunks of the rock to break off as a result. Meteorites and Lunar samples definitely show tiny streaks (“cosmic ray tracks”) when viewed under the microscope, and I’m sure fresh Mars samples will show them as well, but it’s not the kind of thing a rover (or human) would see in the field.