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.
Gespeichert in:
| Autor*in: |
Toner, Jonathan D [verfasserIn] |
|---|
| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015 |
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| Rechteinformationen: |
Nutzungsrecht: © COPYRIGHT 2015 Elsevier B.V. |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Icarus - Amsterdam [u.a.] : Elsevier, 1962, 250(2015), Seite 451-461 |
|---|---|
| Übergeordnetes Werk: |
volume:250 ; year:2015 ; pages:451-461 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.icarus.2014.12.013 |
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| 520 | |a 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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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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freezing origin for soil salts</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2015</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">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.</subfield></datafield><datafield 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