Modeling salt precipitation from brines on Mars: Evaporation versus freezing origin for soil salts
• We develop a Pitzer model for perchlorate salt mixtures on Mars. • We model salt precipitation from a WCL solution during evaporation. • Our model is a significant improvement over FREZCHEM. • We conclude that salts at the Phoenix site formed by freezing, not evaporation.
Autor*in: |
Toner, Jonathan D. [verfasserIn] |
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Format: |
E-Artikel |
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Sprache: |
Englisch |
Erschienen: |
2015 |
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Schlagwörter: |
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Umfang: |
11 |
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Übergeordnetes Werk: |
Enthalten in: Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users - Mathew, Rajeev ELSEVIER, 2018, international journal of solar system studies, Orlando, Fla |
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Übergeordnetes Werk: |
volume:250 ; year:2015 ; pages:451-461 ; extent:11 |
Links: |
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DOI / URN: |
10.1016/j.icarus.2014.12.013 |
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Modeling salt precipitation from brines on Mars: Evaporation versus freezing origin for soil salts |
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• We develop a Pitzer model for perchlorate salt mixtures on Mars. • We model salt precipitation from a WCL solution during evaporation. • Our model is a significant improvement over FREZCHEM. • We conclude that salts at the Phoenix site formed by freezing, not evaporation. |
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• We develop a Pitzer model for perchlorate salt mixtures on Mars. • We model salt precipitation from a WCL solution during evaporation. • Our model is a significant improvement over FREZCHEM. • We conclude that salts at the Phoenix site formed by freezing, not evaporation. |
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• We develop a Pitzer model for perchlorate salt mixtures on Mars. • We model salt precipitation from a WCL solution during evaporation. • Our model is a significant improvement over FREZCHEM. • We conclude that salts at the Phoenix site formed by freezing, not evaporation. |
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Modeling salt precipitation from brines on Mars: Evaporation versus freezing origin for soil salts |
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