41 Astrobiology: What’s the Latest on the Search for Life, Past or Present, Outside of Earth?

Friday, 8 April 2022
1:30 PM - 5:30 PM
North Meeting Room 206


ASTROBIOLOGICAL CONSIDERATIONS IN CONCRETION FORMATION

Paper number: 41-4
Program: Theme Sessions
Time: 2:15 PM – 2:30 PM


Authors


Abstract

Diagenetic concretions are cemented mineral masses found in both clastic and chemical sedimentary rocks and can form in a range of morphologies including spheroidal. Both the MER and MSL rovers have also observed diagenetic spherules in the sedimentary rocks on Mars. Diagenetic concretions form via two end-member models: radial or pervasive growth, though concretions can grow via a combination of both mechanisms. Spheroidal concretions form via diffusion of reactants in a homogenous medium that controls the diffusion rate so that it is equal from all directions. Elongate forms form via advecting fluid. Diagenetic concretions, particularly iron (oxyhydr)oxide mineralogies are thought to form via a two-fluid mixing model where one fluid has the reactants in solution, then another fluid meets and mixes with the reactant-bearing fluid, and the concretions precipitate. Of course, in the subsurface, reservoir fluids can change from oxidizing to reducing by simply lowering and raising the water table. Because of the complexities of formation mechanisms, interactions with subsurface biota and preserved biological material, and interactions of evolving subsurface fluids over geologic time, diagenetic concretion formation mechanisms are difficult to understand, yet they preserve a record of interactions that can be deduced via petrographic and other laboratory methods utilized to interpret the mineralogy and chemistry of these forms. Life is almost certainly involved in some capacity during precipitation of these spherules as subsurface life is concentrated around redox reaction fronts; however, to what degree these forms preserve biological molecules is not known and has not been systematically studied to date. This research presents relations of different morphologies, mineralogies, and stratigraphic locations to infer formation mechanisms and link formation mechanisms to clues about biological involvement during precipitation.

Geological Society of America Abstracts with Programs. Vol. 54, No. 4

doi: 10.1130/abs/2022NC-375498

© Copyright 2022 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.