Formation of Kinneyia via shear-induced instabilities in microbial mats
Katherine Thomas, Stephan Herminghaus, Hubertus Porada, Lucas, Goehring

TL;DR
This study proposes that Kinneyia fossils form through shear-induced Kelvin-Helmholtz instabilities in microbial mats, supported by theoretical predictions and laboratory experiments that replicate natural ripple patterns.
Contribution
It introduces a novel mechanism explaining Kinneyia formation as a shear-induced instability in viscoelastic microbial mats, validated by experiments matching natural patterns.
Findings
Ripple wavelength proportional to film thickness
Patterns form independently of viscosity and flow conditions
Laboratory patterns resemble natural Kinneyia in morphology and scale
Abstract
Kinneyia are a class of microbially mediated sedimentary fossils. Characterised by clearly defined ripple structures, Kinneyia are generally found in areas that were formally littoral habitats and covered by microbial mats. To date there has been no conclusive explanation of the processes involved in the formation of these fossils. Microbial mats behave like viscoelastic fluids. We propose that the key mechanism involved in the formation of Kinneyia is a Kelvin-Helmholtz type instability induced in a viscoelastic film under flowing water. A ripple corrugation is spontaneously induced in the film and grows in amplitude over time. Theoretical predictions show that the ripple instability has a wavelength proportional to the thickness of the film. Experiments carried out using viscoelastic films confirm this prediction. The ripple pattern that forms has a wavelength roughly three times the…
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Taxonomy
TopicsGeological formations and processes · Geology and Paleoclimatology Research · Paleontology and Stratigraphy of Fossils
