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Internal constitution of Mars

Anderson, Don L. (1972) Internal constitution of Mars. Journal of Geophysical Research, 77 (5). pp. 789-795. ISSN 0148-0227. http://resolver.caltech.edu/CaltechAUTHORS:20181128-140624649

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Abstract

Models for the internal structure of Mars that are consistent with its mass, radius, and moment of inertia have been constructed. Mars cannot be homogeneous but must have a core, the size of which depends on its density and, therefore, on its composition. A meteorite model for Mars implies an Fe‐S‐Ni core (12% by mass of the planet) and an Fe‐ or FeO‐rich mantle with a zero‐pressure density of approximately 3.54 g/cm^3. Mars has an iron content of 25 wt %, which is significantly less than the iron content of the earth, Mercury, or Venus but is close to the total iron content of ordinary and carbonaceous chondrites. A satisfactory model for Mars can be obtained by exposing ordinary chondrites to relatively modest temperatures. Core formation will start when temperatures exceed the eutectic temperature in the system Fe‐FeS (∼990°C) but will not go to completion unless temperatures exceed the liquidus throughout most of the planet. No high‐temperature reduction stage is required. The size and density of the core and the density of the mantle indicate that approximately 63% of the potential core‐forming material (Fe‐S‐Ni) has entered the core. Therefore, Mars, in contrast to the earth, is an incompletely differentiated planet, and its core is substantially richer in sulfur than the earth's core. The thermal energy associated with core formation in Mars is negligible. The absence of a magnetic field can be explained by lack of lunar precessional torques and by the small size and high resistivity of the Martian core.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1029/jb077i005p00789DOIArticle
Additional Information:© 1972 American Geophysical Union. (Received June 9, 1971; revised October 27, 1971.) This research was supported by National Aeronautics and Space Administration grant NGL 05-002-069.
Group:Seismological Laboratory
Funders:
Funding AgencyGrant Number
NASANGL 05-002-069
Subject Keywords:Mars
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences2034
Record Number:CaltechAUTHORS:20181128-140624649
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20181128-140624649
Official Citation:Anderson, D. L. (1972), Internal constitution of Mars, J. Geophys. Res., 77(5), 789–795, doi: 10.1029/JB077i005p00789.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:91298
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:29 Nov 2018 21:39
Last Modified:29 Nov 2018 21:39

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