156 D21. Martian Mash-Up
Wednesday, 28 October 2020
5:30 PM - 8:00 PM
Meeting Rooms
GEOLOGIC MAP OF TERRA CIMMERIA, MARS: POTENTIAL IMPLICATIONS FOR REGIONAL PALEOMAGNETISM, PLANETWIDE PRIMORDIAL TECTONIC GEOMORPHOLOGY, AND THE STRUCTURAL HISTORY OF THE THARSIS RISE
Paper number: 156-7
Program: Technical Sessions
Time: 6:50 PM – 7:00 PM
Authors
-
Christine M. RodrigueCalifornia State University, Long Beach, Long Beach, CA
-
James M. DohmUniversity of Tokyo, Tokyo
-
Robert C. AndersonJet Propulsion Laboratory, Pasadena, CA
Abstract
We theorize that these features comprise a global fracture network – the earliest fracture fleets appearing to have predated and survived the emplacement of the dichotomy – which is represented on the MRO110B2 anomaly dataset. We invoke planetary reorientation as a possible explanation for the emplacement of these hypothetical global basement features. Furthermore, we believe that the invocation of this fracture network enables a novel and detailed explanation for the incipience and structural history of the Tharsis Rise. We offer a preliminary form of this hypothesis in this presentation.
The initial purpose of our geologic mapping efforts in Terra Cimmeria was to clarify possible far-reaching tectonic effects of the Tharsis Rise in the eastern hemisphere of Mars. While obvious surficial evidences of these tectonic effects were not found, subsurface effects are considered. We argue that the incipience of the Tharsis Rise (at the Claritas tectonic center) induced the compression of Tharsis aquifers, triggering the filling of the Eridania paleosea and widespread subsurface metasomatism prior to the shutdown of the core dynamo. We infer that the strong magnetic lineations in terrae Cimmeria and Sirenum could be attributed to this process instead of plate tectonics.
Geological Society of America Abstracts with Programs. Vol. 52, No. 6
doi: 10.1130/abs/2020AM-355306
© Copyright 2020 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.