Diagenetic concretion Archives

(Left) Predicted concretion diameter for different nucleation density scaling exponents α. For α ≤ 1, diffusion controls at the Mars dust grain size and predictions match observations (green band). For α ≥ 1.5, nucleation dominates even at 3 µm, predicting concretions well below the observed range, ruled out by the data. (Right) Crossover grain size as a function of α (log scale). Green region: diffusion-limited zone (crossover above Mars dust at 3 µm). Pink region: nucleation-limited zone. The graincontact derivation (dotted line, α = 1) sits within the diffusion-limited zone, consistent with observations. -- astro-ph.EP

Astrogeology, Atmospheres, Climate, Weather, Biogeochemical Cycles & Geobiology, Mars, Status Report

Martian Concretion Sizes Predicted From Two Independently Constrained Inputs: Atmospheric Dust Grain Size And Obliquity-forced Wetting Duration

by Keith CowingMarch 13, 2026March 13, 2026

Diagenetic concretions have been identified at multiple widely separated sites on Mars, including Meridiani Planum (Opportunity), Gale crater (Curiosity), and Jezero crater (Perseverance).

Diagenetic concretion

Martian Concretion Sizes Predicted From Two Independently Constrained Inputs: Atmospheric Dust Grain Size And Obliquity-forced Wetting Duration

Curiosity Mars Rover Discovers A Field Of Honeycomb Textures

Viking Science

Constraining The Lives And Times Of Exoplanets Through Evolutionary Bayesian Retrievals

Project Hephaistos — III. Characterizing Anomalous Infrared Sources Identified As Dyson-sphere Candidates

SCoRE: The Surface Composition Of Rocky Exoplanets