2021
DOI: 10.1029/2020je006663
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History and Future of the Martian Dynamo and Implications of a Hypothetical Solid Inner Core

Abstract: Planetary magnetism is a fundamental but imperfectly understood phenomenon that has the power to inform our understanding of the deep interiors and thermal histories of planetary bodies of all kinds (e.g., Connerney, 2015;Stevenson, 2003;Stevenson et al., 1983). For terrestrial planets, convective motions in the electrically conductive liquid metallic core can drive a global scale self-sustaining magnetic field, in a process known as a magnetohydrodynamic dynamo. This field shields the planet's atmosphere and … Show more

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Cited by 25 publications
(30 citation statements)
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References 95 publications
(223 reference statements)
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“…In all of our models the core is far hotter than the liquidus temperature observed by Gilfoy and Li (2020), with the successful models giving 𝐴𝐴 𝐴𝐴c > 1940 K at the present-day. Our successful models are also above the liquidus curve given by Stewart et al (2007) and those used by Rivoldini et al (2011) and Hemingway and Driscoll (2021) for sulfur concentrations >10 wt% S. Note that we assumed an isothermal mantle except in thermal boundary layers, and so, accounting for the roughly 100 K adiabatic increase in temperature across the convecting mantle would yield CMB temperatures roughly 100 K higher than we obtain.…”
Section: 1029/2021gl095198supporting
confidence: 53%
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“…In all of our models the core is far hotter than the liquidus temperature observed by Gilfoy and Li (2020), with the successful models giving 𝐴𝐴 𝐴𝐴c > 1940 K at the present-day. Our successful models are also above the liquidus curve given by Stewart et al (2007) and those used by Rivoldini et al (2011) and Hemingway and Driscoll (2021) for sulfur concentrations >10 wt% S. Note that we assumed an isothermal mantle except in thermal boundary layers, and so, accounting for the roughly 100 K adiabatic increase in temperature across the convecting mantle would yield CMB temperatures roughly 100 K higher than we obtain.…”
Section: 1029/2021gl095198supporting
confidence: 53%
“…(2007) and those used by Rivoldini et al. (2011) and Hemingway and Driscoll (2021) for sulfur concentrations >10 wt% S. Note that we assumed an isothermal mantle except in thermal boundary layers, and so, accounting for the roughly 100 K adiabatic increase in temperature across the convecting mantle would yield CMB temperatures roughly 100 K higher than we obtain.…”
Section: Resultsmentioning
confidence: 56%
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“…Strong crustal remnant magnetization in the southern hemisphere of Mars (72) and observations of further magnetized units suggest a dynamo that was active between 4.5 Ga and 3.7 Ga (9). The dynamo would have been thermally-driven in the first few hundred Myr (49, 50) and possibly followed by a compositionally-driven dynamo that may resuscitate through FeO exsolution (73) or inner-core crystallization (71,74,75). This, however, depends critically on the light element content and thermal state of the core.…”
Section: Main Textmentioning
confidence: 99%