Igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes
Amphibole in chassignite melt inclusions provides valuable information about the volatile content of the original interstitial magma, but also shock and postshock processes. We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published val...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Giesting, Paul A [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015 |
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| Rechteinformationen: |
Nutzungsrecht: © The Meteoritical Society, 2015. |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Meteoritics & planetary science - Lawrence, Kan. : Allen Press, 1996, 50(2015), 3, Seite 433-460 |
|---|---|
| Übergeordnetes Werk: |
volume:50 ; year:2015 ; number:3 ; pages:433-460 |
| Links: |
|---|
| DOI / URN: |
10.1111/maps.12430 |
|---|
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OLC1965317359 |
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| 520 | |a Amphibole in chassignite melt inclusions provides valuable information about the volatile content of the original interstitial magma, but also shock and postshock processes. We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published values to constrain the crystallization Cl and H 2 O content of phases in chassignite melt inclusions and the effects of shock on these amphibole grains. Using a model for the Cl/ OH exchange between amphibole and melt, we estimate primary crystallization OH contents of chassignite amphiboles. SIMS analysis shows that amphibole from NWA 2737 currently has 0.15 wt% H 2 O. It has lost ~0.6 wt% H 2 O from an initial 0.7–0.8 wt% H 2 O due to intense shock. Chassigny amphibole had on average 0.3–0.4 wt% H 2 O and suffered little net loss of H 2 O due to shock. NWA 2737 amphibole has δD ≈ +3700‰; it absorbed Martian atmosphere‐derived heavy H in the aftermath of shock. Chassigny amphibole, with δD ≤ +1900‰, incorporated less heavy H. Low H 2 O/Cl ratios are inferred for the primitive chassignite magma, which had significant effects on melting and crystallization. Volatiles released by the degassing of Martian magma were more Cl‐rich than on Earth, resulting in the high Cl content of Martian surface materials. | ||
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10.1111/maps.12430 doi PQ20160617 (DE-627)OLC1965317359 (DE-599)GBVOLC1965317359 (PRQ)c2170-ed57f2e54cd60023e09e5a38c2d1b36a9d15e7135b13fd864773d527c553d11f0 (KEY)0042930920150000050000300433igneousandshockprocessesaffectingchassigniteamphib DE-627 ger DE-627 rakwb eng 520 550 DNB Giesting, Paul A verfasserin aut Igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Amphibole in chassignite melt inclusions provides valuable information about the volatile content of the original interstitial magma, but also shock and postshock processes. We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published values to constrain the crystallization Cl and H 2 O content of phases in chassignite melt inclusions and the effects of shock on these amphibole grains. Using a model for the Cl/ OH exchange between amphibole and melt, we estimate primary crystallization OH contents of chassignite amphiboles. SIMS analysis shows that amphibole from NWA 2737 currently has 0.15 wt% H 2 O. It has lost ~0.6 wt% H 2 O from an initial 0.7–0.8 wt% H 2 O due to intense shock. Chassigny amphibole had on average 0.3–0.4 wt% H 2 O and suffered little net loss of H 2 O due to shock. NWA 2737 amphibole has δD ≈ +3700‰; it absorbed Martian atmosphere‐derived heavy H in the aftermath of shock. Chassigny amphibole, with δD ≤ +1900‰, incorporated less heavy H. Low H 2 O/Cl ratios are inferred for the primitive chassignite magma, which had significant effects on melting and crystallization. Volatiles released by the degassing of Martian magma were more Cl‐rich than on Earth, resulting in the high Cl content of Martian surface materials. Nutzungsrecht: © The Meteoritical Society, 2015. Crystallization Magma Schwenzer, Susanne P oth Filiberto, Justin oth Starkey, Natalie A oth Franchi, Ian A oth Treiman, Allan H oth Tindle, Andy G oth Grady, Monica M oth Enthalten in Meteoritics & planetary science Lawrence, Kan. : Allen Press, 1996 50(2015), 3, Seite 433-460 (DE-627)193298368 (DE-600)1306943-3 (DE-576)060237333 1086-9379 nnns volume:50 year:2015 number:3 pages:433-460 http://dx.doi.org/10.1111/maps.12430 Volltext http://onlinelibrary.wiley.com/doi/10.1111/maps.12430/abstract http://search.proquest.com/docview/1664599589 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-AST GBV_ILN_2004 AR 50 2015 3 433-460 |
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10.1111/maps.12430 doi PQ20160617 (DE-627)OLC1965317359 (DE-599)GBVOLC1965317359 (PRQ)c2170-ed57f2e54cd60023e09e5a38c2d1b36a9d15e7135b13fd864773d527c553d11f0 (KEY)0042930920150000050000300433igneousandshockprocessesaffectingchassigniteamphib DE-627 ger DE-627 rakwb eng 520 550 DNB Giesting, Paul A verfasserin aut Igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Amphibole in chassignite melt inclusions provides valuable information about the volatile content of the original interstitial magma, but also shock and postshock processes. We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published values to constrain the crystallization Cl and H 2 O content of phases in chassignite melt inclusions and the effects of shock on these amphibole grains. Using a model for the Cl/ OH exchange between amphibole and melt, we estimate primary crystallization OH contents of chassignite amphiboles. SIMS analysis shows that amphibole from NWA 2737 currently has 0.15 wt% H 2 O. It has lost ~0.6 wt% H 2 O from an initial 0.7–0.8 wt% H 2 O due to intense shock. Chassigny amphibole had on average 0.3–0.4 wt% H 2 O and suffered little net loss of H 2 O due to shock. NWA 2737 amphibole has δD ≈ +3700‰; it absorbed Martian atmosphere‐derived heavy H in the aftermath of shock. Chassigny amphibole, with δD ≤ +1900‰, incorporated less heavy H. Low H 2 O/Cl ratios are inferred for the primitive chassignite magma, which had significant effects on melting and crystallization. Volatiles released by the degassing of Martian magma were more Cl‐rich than on Earth, resulting in the high Cl content of Martian surface materials. Nutzungsrecht: © The Meteoritical Society, 2015. Crystallization Magma Schwenzer, Susanne P oth Filiberto, Justin oth Starkey, Natalie A oth Franchi, Ian A oth Treiman, Allan H oth Tindle, Andy G oth Grady, Monica M oth Enthalten in Meteoritics & planetary science Lawrence, Kan. : Allen Press, 1996 50(2015), 3, Seite 433-460 (DE-627)193298368 (DE-600)1306943-3 (DE-576)060237333 1086-9379 nnns volume:50 year:2015 number:3 pages:433-460 http://dx.doi.org/10.1111/maps.12430 Volltext http://onlinelibrary.wiley.com/doi/10.1111/maps.12430/abstract http://search.proquest.com/docview/1664599589 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-AST GBV_ILN_2004 AR 50 2015 3 433-460 |
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10.1111/maps.12430 doi PQ20160617 (DE-627)OLC1965317359 (DE-599)GBVOLC1965317359 (PRQ)c2170-ed57f2e54cd60023e09e5a38c2d1b36a9d15e7135b13fd864773d527c553d11f0 (KEY)0042930920150000050000300433igneousandshockprocessesaffectingchassigniteamphib DE-627 ger DE-627 rakwb eng 520 550 DNB Giesting, Paul A verfasserin aut Igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Amphibole in chassignite melt inclusions provides valuable information about the volatile content of the original interstitial magma, but also shock and postshock processes. We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published values to constrain the crystallization Cl and H 2 O content of phases in chassignite melt inclusions and the effects of shock on these amphibole grains. Using a model for the Cl/ OH exchange between amphibole and melt, we estimate primary crystallization OH contents of chassignite amphiboles. SIMS analysis shows that amphibole from NWA 2737 currently has 0.15 wt% H 2 O. It has lost ~0.6 wt% H 2 O from an initial 0.7–0.8 wt% H 2 O due to intense shock. Chassigny amphibole had on average 0.3–0.4 wt% H 2 O and suffered little net loss of H 2 O due to shock. NWA 2737 amphibole has δD ≈ +3700‰; it absorbed Martian atmosphere‐derived heavy H in the aftermath of shock. Chassigny amphibole, with δD ≤ +1900‰, incorporated less heavy H. Low H 2 O/Cl ratios are inferred for the primitive chassignite magma, which had significant effects on melting and crystallization. Volatiles released by the degassing of Martian magma were more Cl‐rich than on Earth, resulting in the high Cl content of Martian surface materials. Nutzungsrecht: © The Meteoritical Society, 2015. Crystallization Magma Schwenzer, Susanne P oth Filiberto, Justin oth Starkey, Natalie A oth Franchi, Ian A oth Treiman, Allan H oth Tindle, Andy G oth Grady, Monica M oth Enthalten in Meteoritics & planetary science Lawrence, Kan. : Allen Press, 1996 50(2015), 3, Seite 433-460 (DE-627)193298368 (DE-600)1306943-3 (DE-576)060237333 1086-9379 nnns volume:50 year:2015 number:3 pages:433-460 http://dx.doi.org/10.1111/maps.12430 Volltext http://onlinelibrary.wiley.com/doi/10.1111/maps.12430/abstract http://search.proquest.com/docview/1664599589 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-AST GBV_ILN_2004 AR 50 2015 3 433-460 |
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We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published values to constrain the crystallization Cl and H 2 O content of phases in chassignite melt inclusions and the effects of shock on these amphibole grains. Using a model for the Cl/ OH exchange between amphibole and melt, we estimate primary crystallization OH contents of chassignite amphiboles. SIMS analysis shows that amphibole from NWA 2737 currently has 0.15 wt% H 2 O. It has lost ~0.6 wt% H 2 O from an initial 0.7–0.8 wt% H 2 O due to intense shock. Chassigny amphibole had on average 0.3–0.4 wt% H 2 O and suffered little net loss of H 2 O due to shock. NWA 2737 amphibole has δD ≈ +3700‰; it absorbed Martian atmosphere‐derived heavy H in the aftermath of shock. Chassigny amphibole, with δD ≤ +1900‰, incorporated less heavy H. Low H 2 O/Cl ratios are inferred for the primitive chassignite magma, which had significant effects on melting and crystallization. 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Igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes |
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igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes |
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Igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes |
| abstract |
Amphibole in chassignite melt inclusions provides valuable information about the volatile content of the original interstitial magma, but also shock and postshock processes. We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published values to constrain the crystallization Cl and H 2 O content of phases in chassignite melt inclusions and the effects of shock on these amphibole grains. Using a model for the Cl/ OH exchange between amphibole and melt, we estimate primary crystallization OH contents of chassignite amphiboles. SIMS analysis shows that amphibole from NWA 2737 currently has 0.15 wt% H 2 O. It has lost ~0.6 wt% H 2 O from an initial 0.7–0.8 wt% H 2 O due to intense shock. Chassigny amphibole had on average 0.3–0.4 wt% H 2 O and suffered little net loss of H 2 O due to shock. NWA 2737 amphibole has δD ≈ +3700‰; it absorbed Martian atmosphere‐derived heavy H in the aftermath of shock. Chassigny amphibole, with δD ≤ +1900‰, incorporated less heavy H. Low H 2 O/Cl ratios are inferred for the primitive chassignite magma, which had significant effects on melting and crystallization. Volatiles released by the degassing of Martian magma were more Cl‐rich than on Earth, resulting in the high Cl content of Martian surface materials. |
| abstractGer |
Amphibole in chassignite melt inclusions provides valuable information about the volatile content of the original interstitial magma, but also shock and postshock processes. We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published values to constrain the crystallization Cl and H 2 O content of phases in chassignite melt inclusions and the effects of shock on these amphibole grains. Using a model for the Cl/ OH exchange between amphibole and melt, we estimate primary crystallization OH contents of chassignite amphiboles. SIMS analysis shows that amphibole from NWA 2737 currently has 0.15 wt% H 2 O. It has lost ~0.6 wt% H 2 O from an initial 0.7–0.8 wt% H 2 O due to intense shock. Chassigny amphibole had on average 0.3–0.4 wt% H 2 O and suffered little net loss of H 2 O due to shock. NWA 2737 amphibole has δD ≈ +3700‰; it absorbed Martian atmosphere‐derived heavy H in the aftermath of shock. Chassigny amphibole, with δD ≤ +1900‰, incorporated less heavy H. Low H 2 O/Cl ratios are inferred for the primitive chassignite magma, which had significant effects on melting and crystallization. Volatiles released by the degassing of Martian magma were more Cl‐rich than on Earth, resulting in the high Cl content of Martian surface materials. |
| abstract_unstemmed |
Amphibole in chassignite melt inclusions provides valuable information about the volatile content of the original interstitial magma, but also shock and postshock processes. We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published values to constrain the crystallization Cl and H 2 O content of phases in chassignite melt inclusions and the effects of shock on these amphibole grains. Using a model for the Cl/ OH exchange between amphibole and melt, we estimate primary crystallization OH contents of chassignite amphiboles. SIMS analysis shows that amphibole from NWA 2737 currently has 0.15 wt% H 2 O. It has lost ~0.6 wt% H 2 O from an initial 0.7–0.8 wt% H 2 O due to intense shock. Chassigny amphibole had on average 0.3–0.4 wt% H 2 O and suffered little net loss of H 2 O due to shock. NWA 2737 amphibole has δD ≈ +3700‰; it absorbed Martian atmosphere‐derived heavy H in the aftermath of shock. Chassigny amphibole, with δD ≤ +1900‰, incorporated less heavy H. Low H 2 O/Cl ratios are inferred for the primitive chassignite magma, which had significant effects on melting and crystallization. Volatiles released by the degassing of Martian magma were more Cl‐rich than on Earth, resulting in the high Cl content of Martian surface materials. |
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Igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes |
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Schwenzer, Susanne P Filiberto, Justin Starkey, Natalie A Franchi, Ian A Treiman, Allan H Tindle, Andy G Grady, Monica M |
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