Phase stability and density of FeS at high pressures and temperatures: implications for the interior structure of Mars

Publication Status is "Submitted" Or "In Press: 
LDEO Publication: 
Publication Type: 
Year of Publication: 
2001
Editor: 
Journal Title: 
Earth and Planetary Science Letters
Journal Date: 
Feb 15
Place Published: 
Tertiary Title: 
Volume: 
185
Issue: 
1-2
Pages: 
25-33
Section / Start page: 
Publisher: 
ISBN Number: 
0012-821X
ISSN Number: 
Edition: 
Short Title: 
Accession Number: 
ISI:000166927400004
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Abstract: 

The phase diagram of stoichiometric iron sulfide (FeS) was investigated at high pressures and temperatures (15-35 GPa, 1400-2200 K) with a laser-heated diamond anvil cell and synchrotron X-ray diffraction. The NiAs-structured polymorph of FeS is found to be stable within the P-T range of the Martian core. The density of FeS at 1600 K is measured to be 5.96 g/cm(3) at 17 GPa and 6.65 g/cm(3) at 35 GPa. The density measurements are used to evaluate structural models of Mars containing a core within the Fe-FeS system. The models that satisfy the geophysical constraints proscribe limits on the thickness of the Martian crust, the size and composition of the core, and the thickness of a perovskite-bearing layer close to the Martian core-mantle boundary. (C) 2001 Elsevier Science B.V. All rights reserved.

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