T59 Unconventional Ideas and Outrageous Hypotheses II: In Honor of Warren B. Hamilton
Sunday, 22 September 2019
1:30 PM - 5:30 PM
Room 127ABC, North Building
EVOLUTION AND TECTONICS OF THE ROCKY PLANETS ARE DRIVEN BY THEIR MASS, MOONS AND ORBITAL RADII
Paper number: T59-10
Program: Technical Sessions
Time: 4:15 PM – 4:30 PM
Authors
-
Anne HofmeisterWashington University, St. Louis, MO
Abstract
Earth ~ Venus >> Moon > Mars > Mercury > Vesta
Small objects generate little heat by spin loss, and lose their internal heat rapidly. Thus, this order is nearly congruent with object mass, as well as with the gamma ray intensities of these bodies, and their relative magmatic and tectonic activities. Power produced by radionuclides and spin loss both decline exponentially on Ga timescales and is preferentially delivered to upper zones where rocks are weakest. Specific energy of the Moon is inordinately large and perhaps overestimated, due to its surficial Th anomaly.
Activity is affected by distance (r) from the Sun. (1) Proximity rapidly despun Venus and Mercury, so their tectonic activity ceased long ago, in contrast to the Earth and even Mars. (2) Post-accretion impacts of km-sized bodies promoted early surface process, especially on the innermost bodies since impactor flux varies as ~1/r2, and the energy of each goes as ~1/r. (3) Blackbody temperatures go as 1/√r and determine the physical state of H2O and other volatiles, which affect planetary magmatism and differentiation. This temperature and object mass explain atmosphere retention and constitution across the Solar System, with volatile loss limiting igneous differentiation. (4) Earth is far enough from the Sun to have retained its water, spin, and Moon, whose presence drives surficial plate tectonics. All other rocky objects are long-since dead, except for Io which is also gravitationally pumped.
Geological Society of America Abstracts with Programs. Vol. 51, No. 5
doi: 10.1130/abs/2019AM-335315
© Copyright 2019 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.