45 Surface Processes Across the Solar System (Posters)

This session welcomes abstracts on any aspect of planetary geomorphology, including but not restricted to: Earth analogues, laboratory experiments, numerical models, planetary comparison, mapping, in situ data, or remote sensing studies.

Tuesday, 24 March 2026
8:00 AM - 12:00 PM
CCC, Ballroom C


Comparative Analysis of Stromatolite-Like Structures in Gale Crater, Mars

Paper number: 45-2
Program: Technical Sessions
Time: 8:00 AM – 8:00 AM


Authors

  • Mossbah Kolkas Presenting Author
    College of Staten Island, Staten Island, New York

Abstract

Layered rock formations imaged by NASA’s Curiosity rover in Gale Crater, Mars, display sedimentary structures that resemble terrestrial stromatolites, characterized by laminated accretionary features commonly produced by microbial mat communities. On Earth, stromatolites represent some of the oldest preserved biosignatures, recording interactions among microorganisms, sediments, and mineral precipitation in shallow aqueous environments. This study examines rover-based imaging and mineralogical data from wavy-laminated structures observed within the “Garden City” vein complex on the lower slopes of Mount Sharp and compares them with well-characterized Archean stromatolites from the Pilbara Craton, Western Australia, as well as Early Paleozoic stromatolites from the Petrified Sea Gardens of Saratoga County, New York. The association of these Martian structures with fluorite, sulfates, iron-bearing minerals, carbonates, and clay-rich sediments indicates sustained aqueous alteration under geochemical conditions that may have been conducive to microbial ecosystems. While abiotic processes remain viable explanations for the observed textures, the combined morphological and mineralogical similarities support the hypothesis that early Martian environments may have been capable of sustaining microbial life.


Geological Society of America Abstracts with Programs. Vol. 58, No. 2

doi: 10.1130/abs/2026NE-411134

© Copyright 2026 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.