The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole
Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant...
Ausführliche Beschreibung
Autor*in: |
Giesting, Paul A [verfasserIn] |
---|
Format: |
Artikel |
---|---|
Sprache: |
Englisch |
Erschienen: |
2016 |
---|
Übergeordnetes Werk: |
Enthalten in: Meteoritics & planetary science - Lawrence, Kan. : Allen Press, 1996, 51(2016), 11, Seite 2127-2153 |
---|---|
Übergeordnetes Werk: |
volume:51 ; year:2016 ; number:11 ; pages:2127-2153 |
Links: |
---|
DOI / URN: |
10.1111/maps.12675 |
---|
Katalog-ID: |
OLC1984519018 |
---|
LEADER | 01000caa a2200265 4500 | ||
---|---|---|---|
001 | OLC1984519018 | ||
003 | DE-627 | ||
005 | 20230714224041.0 | ||
007 | tu | ||
008 | 161202s2016 xx ||||| 00| ||eng c | ||
024 | 7 | |a 10.1111/maps.12675 |2 doi | |
028 | 5 | 2 | |a PQ20161201 |
035 | |a (DE-627)OLC1984519018 | ||
035 | |a (DE-599)GBVOLC1984519018 | ||
035 | |a (PRQ)c879-cf581b9a5e0334681f84018acca8c11208669718d76c3cb88ebbab85868870df0 | ||
035 | |a (KEY)0042930920160000051001102127formationenvironmentofpotassicchlorohastingsiteint | ||
040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
041 | |a eng | ||
082 | 0 | 4 | |a 520 |a 550 |q DNB |
100 | 1 | |a Giesting, Paul A |e verfasserin |4 aut | |
245 | 1 | 4 | |a The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole |
264 | 1 | |c 2016 | |
336 | |a Text |b txt |2 rdacontent | ||
337 | |a ohne Hilfsmittel zu benutzen |b n |2 rdamedia | ||
338 | |a Band |b nc |2 rdacarrier | ||
520 | |a Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant amphibole (chloro-amphibole) forms and apply these insights to the nakhlites. Chloro-amphibole is rare, with about a dozen identified localities on Earth. It is always rich in potassium and iron and poor in titanium. In terrestrial settings, its presence has been interpreted to result from medium to high-grade alteration (>400 °C) of a protolith by an alkali and/or iron chloride-rich aqueous fluid. Ferrous chloride fluids exsolved from mafic magmas can cause such alteration, as can crustal fluids that have reacted with rock and lost H2O in preference to chloride, resulting in concentrated alkali chloride fluids. In the case of the nakhlites, an aqueous alkali-ferrous chloride fluid was exsolved from the parental melt as it crystallized. This aqueous chloride fluid itself likely unmixed into chloride-dominant and water-dominant fluids. Chloride-dominant fluid was trapped in some melt inclusions and reacted with the silicate contents of the inclusion to form potassic-chloro-hastingsite. | ||
700 | 1 | |a Filiberto, Justin |4 oth | |
773 | 0 | 8 | |i Enthalten in |t Meteoritics & planetary science |d Lawrence, Kan. : Allen Press, 1996 |g 51(2016), 11, Seite 2127-2153 |w (DE-627)193298368 |w (DE-600)1306943-3 |w (DE-576)060237333 |x 1086-9379 |7 nnns |
773 | 1 | 8 | |g volume:51 |g year:2016 |g number:11 |g pages:2127-2153 |
856 | 4 | 1 | |u http://dx.doi.org/10.1111/maps.12675 |3 Volltext |
856 | 4 | 2 | |u http://search.proquest.com/docview/1837124045 |
912 | |a GBV_USEFLAG_A | ||
912 | |a SYSFLAG_A | ||
912 | |a GBV_OLC | ||
912 | |a SSG-OLC-GEO | ||
912 | |a SSG-OLC-AST | ||
912 | |a SSG-OPC-GGO | ||
912 | |a SSG-OPC-AST | ||
912 | |a GBV_ILN_2004 | ||
951 | |a AR | ||
952 | |d 51 |j 2016 |e 11 |h 2127-2153 |
author_variant |
p a g pa pag |
---|---|
matchkey_str |
article:10869379:2016----::hfrainniomnoptsiclrhsigienhnkltsi036npisnna70nih |
hierarchy_sort_str |
2016 |
publishDate |
2016 |
allfields |
10.1111/maps.12675 doi PQ20161201 (DE-627)OLC1984519018 (DE-599)GBVOLC1984519018 (PRQ)c879-cf581b9a5e0334681f84018acca8c11208669718d76c3cb88ebbab85868870df0 (KEY)0042930920160000051001102127formationenvironmentofpotassicchlorohastingsiteint DE-627 ger DE-627 rakwb eng 520 550 DNB Giesting, Paul A verfasserin aut The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant amphibole (chloro-amphibole) forms and apply these insights to the nakhlites. Chloro-amphibole is rare, with about a dozen identified localities on Earth. It is always rich in potassium and iron and poor in titanium. In terrestrial settings, its presence has been interpreted to result from medium to high-grade alteration (>400 °C) of a protolith by an alkali and/or iron chloride-rich aqueous fluid. Ferrous chloride fluids exsolved from mafic magmas can cause such alteration, as can crustal fluids that have reacted with rock and lost H2O in preference to chloride, resulting in concentrated alkali chloride fluids. In the case of the nakhlites, an aqueous alkali-ferrous chloride fluid was exsolved from the parental melt as it crystallized. This aqueous chloride fluid itself likely unmixed into chloride-dominant and water-dominant fluids. Chloride-dominant fluid was trapped in some melt inclusions and reacted with the silicate contents of the inclusion to form potassic-chloro-hastingsite. Filiberto, Justin oth Enthalten in Meteoritics & planetary science Lawrence, Kan. : Allen Press, 1996 51(2016), 11, Seite 2127-2153 (DE-627)193298368 (DE-600)1306943-3 (DE-576)060237333 1086-9379 nnns volume:51 year:2016 number:11 pages:2127-2153 http://dx.doi.org/10.1111/maps.12675 Volltext http://search.proquest.com/docview/1837124045 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-AST GBV_ILN_2004 AR 51 2016 11 2127-2153 |
spelling |
10.1111/maps.12675 doi PQ20161201 (DE-627)OLC1984519018 (DE-599)GBVOLC1984519018 (PRQ)c879-cf581b9a5e0334681f84018acca8c11208669718d76c3cb88ebbab85868870df0 (KEY)0042930920160000051001102127formationenvironmentofpotassicchlorohastingsiteint DE-627 ger DE-627 rakwb eng 520 550 DNB Giesting, Paul A verfasserin aut The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant amphibole (chloro-amphibole) forms and apply these insights to the nakhlites. Chloro-amphibole is rare, with about a dozen identified localities on Earth. It is always rich in potassium and iron and poor in titanium. In terrestrial settings, its presence has been interpreted to result from medium to high-grade alteration (>400 °C) of a protolith by an alkali and/or iron chloride-rich aqueous fluid. Ferrous chloride fluids exsolved from mafic magmas can cause such alteration, as can crustal fluids that have reacted with rock and lost H2O in preference to chloride, resulting in concentrated alkali chloride fluids. In the case of the nakhlites, an aqueous alkali-ferrous chloride fluid was exsolved from the parental melt as it crystallized. This aqueous chloride fluid itself likely unmixed into chloride-dominant and water-dominant fluids. Chloride-dominant fluid was trapped in some melt inclusions and reacted with the silicate contents of the inclusion to form potassic-chloro-hastingsite. Filiberto, Justin oth Enthalten in Meteoritics & planetary science Lawrence, Kan. : Allen Press, 1996 51(2016), 11, Seite 2127-2153 (DE-627)193298368 (DE-600)1306943-3 (DE-576)060237333 1086-9379 nnns volume:51 year:2016 number:11 pages:2127-2153 http://dx.doi.org/10.1111/maps.12675 Volltext http://search.proquest.com/docview/1837124045 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-AST GBV_ILN_2004 AR 51 2016 11 2127-2153 |
allfields_unstemmed |
10.1111/maps.12675 doi PQ20161201 (DE-627)OLC1984519018 (DE-599)GBVOLC1984519018 (PRQ)c879-cf581b9a5e0334681f84018acca8c11208669718d76c3cb88ebbab85868870df0 (KEY)0042930920160000051001102127formationenvironmentofpotassicchlorohastingsiteint DE-627 ger DE-627 rakwb eng 520 550 DNB Giesting, Paul A verfasserin aut The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant amphibole (chloro-amphibole) forms and apply these insights to the nakhlites. Chloro-amphibole is rare, with about a dozen identified localities on Earth. It is always rich in potassium and iron and poor in titanium. In terrestrial settings, its presence has been interpreted to result from medium to high-grade alteration (>400 °C) of a protolith by an alkali and/or iron chloride-rich aqueous fluid. Ferrous chloride fluids exsolved from mafic magmas can cause such alteration, as can crustal fluids that have reacted with rock and lost H2O in preference to chloride, resulting in concentrated alkali chloride fluids. In the case of the nakhlites, an aqueous alkali-ferrous chloride fluid was exsolved from the parental melt as it crystallized. This aqueous chloride fluid itself likely unmixed into chloride-dominant and water-dominant fluids. Chloride-dominant fluid was trapped in some melt inclusions and reacted with the silicate contents of the inclusion to form potassic-chloro-hastingsite. Filiberto, Justin oth Enthalten in Meteoritics & planetary science Lawrence, Kan. : Allen Press, 1996 51(2016), 11, Seite 2127-2153 (DE-627)193298368 (DE-600)1306943-3 (DE-576)060237333 1086-9379 nnns volume:51 year:2016 number:11 pages:2127-2153 http://dx.doi.org/10.1111/maps.12675 Volltext http://search.proquest.com/docview/1837124045 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-AST GBV_ILN_2004 AR 51 2016 11 2127-2153 |
allfieldsGer |
10.1111/maps.12675 doi PQ20161201 (DE-627)OLC1984519018 (DE-599)GBVOLC1984519018 (PRQ)c879-cf581b9a5e0334681f84018acca8c11208669718d76c3cb88ebbab85868870df0 (KEY)0042930920160000051001102127formationenvironmentofpotassicchlorohastingsiteint DE-627 ger DE-627 rakwb eng 520 550 DNB Giesting, Paul A verfasserin aut The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant amphibole (chloro-amphibole) forms and apply these insights to the nakhlites. Chloro-amphibole is rare, with about a dozen identified localities on Earth. It is always rich in potassium and iron and poor in titanium. In terrestrial settings, its presence has been interpreted to result from medium to high-grade alteration (>400 °C) of a protolith by an alkali and/or iron chloride-rich aqueous fluid. Ferrous chloride fluids exsolved from mafic magmas can cause such alteration, as can crustal fluids that have reacted with rock and lost H2O in preference to chloride, resulting in concentrated alkali chloride fluids. In the case of the nakhlites, an aqueous alkali-ferrous chloride fluid was exsolved from the parental melt as it crystallized. This aqueous chloride fluid itself likely unmixed into chloride-dominant and water-dominant fluids. Chloride-dominant fluid was trapped in some melt inclusions and reacted with the silicate contents of the inclusion to form potassic-chloro-hastingsite. Filiberto, Justin oth Enthalten in Meteoritics & planetary science Lawrence, Kan. : Allen Press, 1996 51(2016), 11, Seite 2127-2153 (DE-627)193298368 (DE-600)1306943-3 (DE-576)060237333 1086-9379 nnns volume:51 year:2016 number:11 pages:2127-2153 http://dx.doi.org/10.1111/maps.12675 Volltext http://search.proquest.com/docview/1837124045 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-AST GBV_ILN_2004 AR 51 2016 11 2127-2153 |
allfieldsSound |
10.1111/maps.12675 doi PQ20161201 (DE-627)OLC1984519018 (DE-599)GBVOLC1984519018 (PRQ)c879-cf581b9a5e0334681f84018acca8c11208669718d76c3cb88ebbab85868870df0 (KEY)0042930920160000051001102127formationenvironmentofpotassicchlorohastingsiteint DE-627 ger DE-627 rakwb eng 520 550 DNB Giesting, Paul A verfasserin aut The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant amphibole (chloro-amphibole) forms and apply these insights to the nakhlites. Chloro-amphibole is rare, with about a dozen identified localities on Earth. It is always rich in potassium and iron and poor in titanium. In terrestrial settings, its presence has been interpreted to result from medium to high-grade alteration (>400 °C) of a protolith by an alkali and/or iron chloride-rich aqueous fluid. Ferrous chloride fluids exsolved from mafic magmas can cause such alteration, as can crustal fluids that have reacted with rock and lost H2O in preference to chloride, resulting in concentrated alkali chloride fluids. In the case of the nakhlites, an aqueous alkali-ferrous chloride fluid was exsolved from the parental melt as it crystallized. This aqueous chloride fluid itself likely unmixed into chloride-dominant and water-dominant fluids. Chloride-dominant fluid was trapped in some melt inclusions and reacted with the silicate contents of the inclusion to form potassic-chloro-hastingsite. Filiberto, Justin oth Enthalten in Meteoritics & planetary science Lawrence, Kan. : Allen Press, 1996 51(2016), 11, Seite 2127-2153 (DE-627)193298368 (DE-600)1306943-3 (DE-576)060237333 1086-9379 nnns volume:51 year:2016 number:11 pages:2127-2153 http://dx.doi.org/10.1111/maps.12675 Volltext http://search.proquest.com/docview/1837124045 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-AST GBV_ILN_2004 AR 51 2016 11 2127-2153 |
language |
English |
source |
Enthalten in Meteoritics & planetary science 51(2016), 11, Seite 2127-2153 volume:51 year:2016 number:11 pages:2127-2153 |
sourceStr |
Enthalten in Meteoritics & planetary science 51(2016), 11, Seite 2127-2153 volume:51 year:2016 number:11 pages:2127-2153 |
format_phy_str_mv |
Article |
institution |
findex.gbv.de |
dewey-raw |
520 |
isfreeaccess_bool |
false |
container_title |
Meteoritics & planetary science |
authorswithroles_txt_mv |
Giesting, Paul A @@aut@@ Filiberto, Justin @@oth@@ |
publishDateDaySort_date |
2016-01-01T00:00:00Z |
hierarchy_top_id |
193298368 |
dewey-sort |
3520 |
id |
OLC1984519018 |
language_de |
englisch |
fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">OLC1984519018</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230714224041.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">161202s2016 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1111/maps.12675</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">PQ20161201</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC1984519018</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVOLC1984519018</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(PRQ)c879-cf581b9a5e0334681f84018acca8c11208669718d76c3cb88ebbab85868870df0</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(KEY)0042930920160000051001102127formationenvironmentofpotassicchlorohastingsiteint</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">550</subfield><subfield code="q">DNB</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Giesting, Paul A</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="4"><subfield code="a">The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2016</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">Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant amphibole (chloro-amphibole) forms and apply these insights to the nakhlites. Chloro-amphibole is rare, with about a dozen identified localities on Earth. It is always rich in potassium and iron and poor in titanium. In terrestrial settings, its presence has been interpreted to result from medium to high-grade alteration (>400 °C) of a protolith by an alkali and/or iron chloride-rich aqueous fluid. Ferrous chloride fluids exsolved from mafic magmas can cause such alteration, as can crustal fluids that have reacted with rock and lost H2O in preference to chloride, resulting in concentrated alkali chloride fluids. In the case of the nakhlites, an aqueous alkali-ferrous chloride fluid was exsolved from the parental melt as it crystallized. This aqueous chloride fluid itself likely unmixed into chloride-dominant and water-dominant fluids. Chloride-dominant fluid was trapped in some melt inclusions and reacted with the silicate contents of the inclusion to form potassic-chloro-hastingsite.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Filiberto, Justin</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Meteoritics & planetary science</subfield><subfield code="d">Lawrence, Kan. : Allen Press, 1996</subfield><subfield code="g">51(2016), 11, Seite 2127-2153</subfield><subfield code="w">(DE-627)193298368</subfield><subfield code="w">(DE-600)1306943-3</subfield><subfield code="w">(DE-576)060237333</subfield><subfield code="x">1086-9379</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:51</subfield><subfield code="g">year:2016</subfield><subfield code="g">number:11</subfield><subfield code="g">pages:2127-2153</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">http://dx.doi.org/10.1111/maps.12675</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">http://search.proquest.com/docview/1837124045</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-GEO</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-GGO</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2004</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">51</subfield><subfield code="j">2016</subfield><subfield code="e">11</subfield><subfield code="h">2127-2153</subfield></datafield></record></collection>
|
author |
Giesting, Paul A |
spellingShingle |
Giesting, Paul A ddc 520 The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole |
authorStr |
Giesting, Paul A |
ppnlink_with_tag_str_mv |
@@773@@(DE-627)193298368 |
format |
Article |
dewey-ones |
520 - Astronomy & allied sciences 550 - Earth sciences |
delete_txt_mv |
keep |
author_role |
aut |
collection |
OLC |
remote_str |
false |
illustrated |
Not Illustrated |
issn |
1086-9379 |
topic_title |
520 550 DNB The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole |
topic |
ddc 520 |
topic_unstemmed |
ddc 520 |
topic_browse |
ddc 520 |
format_facet |
Aufsätze Gedruckte Aufsätze |
format_main_str_mv |
Text Zeitschrift/Artikel |
carriertype_str_mv |
nc |
author2_variant |
j f jf |
hierarchy_parent_title |
Meteoritics & planetary science |
hierarchy_parent_id |
193298368 |
dewey-tens |
520 - Astronomy 550 - Earth sciences & geology |
hierarchy_top_title |
Meteoritics & planetary science |
isfreeaccess_txt |
false |
familylinks_str_mv |
(DE-627)193298368 (DE-600)1306943-3 (DE-576)060237333 |
title |
The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole |
ctrlnum |
(DE-627)OLC1984519018 (DE-599)GBVOLC1984519018 (PRQ)c879-cf581b9a5e0334681f84018acca8c11208669718d76c3cb88ebbab85868870df0 (KEY)0042930920160000051001102127formationenvironmentofpotassicchlorohastingsiteint |
title_full |
The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole |
author_sort |
Giesting, Paul A |
journal |
Meteoritics & planetary science |
journalStr |
Meteoritics & planetary science |
lang_code |
eng |
isOA_bool |
false |
dewey-hundreds |
500 - Science |
recordtype |
marc |
publishDateSort |
2016 |
contenttype_str_mv |
txt |
container_start_page |
2127 |
author_browse |
Giesting, Paul A |
container_volume |
51 |
class |
520 550 DNB |
format_se |
Aufsätze |
author-letter |
Giesting, Paul A |
doi_str_mv |
10.1111/maps.12675 |
dewey-full |
520 550 |
title_sort |
formation environment of potassic-chloro-hastingsite in the nakhlites mil 03346 and pairs and nwa 5790: insights from terrestrial chloro-amphibole |
title_auth |
The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole |
abstract |
Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant amphibole (chloro-amphibole) forms and apply these insights to the nakhlites. Chloro-amphibole is rare, with about a dozen identified localities on Earth. It is always rich in potassium and iron and poor in titanium. In terrestrial settings, its presence has been interpreted to result from medium to high-grade alteration (>400 °C) of a protolith by an alkali and/or iron chloride-rich aqueous fluid. Ferrous chloride fluids exsolved from mafic magmas can cause such alteration, as can crustal fluids that have reacted with rock and lost H2O in preference to chloride, resulting in concentrated alkali chloride fluids. In the case of the nakhlites, an aqueous alkali-ferrous chloride fluid was exsolved from the parental melt as it crystallized. This aqueous chloride fluid itself likely unmixed into chloride-dominant and water-dominant fluids. Chloride-dominant fluid was trapped in some melt inclusions and reacted with the silicate contents of the inclusion to form potassic-chloro-hastingsite. |
abstractGer |
Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant amphibole (chloro-amphibole) forms and apply these insights to the nakhlites. Chloro-amphibole is rare, with about a dozen identified localities on Earth. It is always rich in potassium and iron and poor in titanium. In terrestrial settings, its presence has been interpreted to result from medium to high-grade alteration (>400 °C) of a protolith by an alkali and/or iron chloride-rich aqueous fluid. Ferrous chloride fluids exsolved from mafic magmas can cause such alteration, as can crustal fluids that have reacted with rock and lost H2O in preference to chloride, resulting in concentrated alkali chloride fluids. In the case of the nakhlites, an aqueous alkali-ferrous chloride fluid was exsolved from the parental melt as it crystallized. This aqueous chloride fluid itself likely unmixed into chloride-dominant and water-dominant fluids. Chloride-dominant fluid was trapped in some melt inclusions and reacted with the silicate contents of the inclusion to form potassic-chloro-hastingsite. |
abstract_unstemmed |
Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant amphibole (chloro-amphibole) forms and apply these insights to the nakhlites. Chloro-amphibole is rare, with about a dozen identified localities on Earth. It is always rich in potassium and iron and poor in titanium. In terrestrial settings, its presence has been interpreted to result from medium to high-grade alteration (>400 °C) of a protolith by an alkali and/or iron chloride-rich aqueous fluid. Ferrous chloride fluids exsolved from mafic magmas can cause such alteration, as can crustal fluids that have reacted with rock and lost H2O in preference to chloride, resulting in concentrated alkali chloride fluids. In the case of the nakhlites, an aqueous alkali-ferrous chloride fluid was exsolved from the parental melt as it crystallized. This aqueous chloride fluid itself likely unmixed into chloride-dominant and water-dominant fluids. Chloride-dominant fluid was trapped in some melt inclusions and reacted with the silicate contents of the inclusion to form potassic-chloro-hastingsite. |
collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-AST GBV_ILN_2004 |
container_issue |
11 |
title_short |
The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole |
url |
http://dx.doi.org/10.1111/maps.12675 http://search.proquest.com/docview/1837124045 |
remote_bool |
false |
author2 |
Filiberto, Justin |
author2Str |
Filiberto, Justin |
ppnlink |
193298368 |
mediatype_str_mv |
n |
isOA_txt |
false |
hochschulschrift_bool |
false |
author2_role |
oth |
doi_str |
10.1111/maps.12675 |
up_date |
2024-07-04T00:42:46.474Z |
_version_ |
1803607098237386752 |
fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">OLC1984519018</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230714224041.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">161202s2016 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1111/maps.12675</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">PQ20161201</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC1984519018</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVOLC1984519018</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(PRQ)c879-cf581b9a5e0334681f84018acca8c11208669718d76c3cb88ebbab85868870df0</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(KEY)0042930920160000051001102127formationenvironmentofpotassicchlorohastingsiteint</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">550</subfield><subfield code="q">DNB</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Giesting, Paul A</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="4"><subfield code="a">The formation environment of potassic-chloro-hastingsite in the nakhlites MIL 03346 and pairs and NWA 5790: Insights from terrestrial chloro-amphibole</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2016</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">Potassic-chloro-hastingsite has been found in melt inclusions in MIL 03346, its paired stones, and NWA 5790. It is some of the most chlorine-rich amphibole ever analyzed. In this article, we evaluate what crystal chemistry, terrestrial analogs, and experiments have shown about how chlorine-dominant amphibole (chloro-amphibole) forms and apply these insights to the nakhlites. Chloro-amphibole is rare, with about a dozen identified localities on Earth. It is always rich in potassium and iron and poor in titanium. In terrestrial settings, its presence has been interpreted to result from medium to high-grade alteration (>400 °C) of a protolith by an alkali and/or iron chloride-rich aqueous fluid. Ferrous chloride fluids exsolved from mafic magmas can cause such alteration, as can crustal fluids that have reacted with rock and lost H2O in preference to chloride, resulting in concentrated alkali chloride fluids. In the case of the nakhlites, an aqueous alkali-ferrous chloride fluid was exsolved from the parental melt as it crystallized. This aqueous chloride fluid itself likely unmixed into chloride-dominant and water-dominant fluids. Chloride-dominant fluid was trapped in some melt inclusions and reacted with the silicate contents of the inclusion to form potassic-chloro-hastingsite.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Filiberto, Justin</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Meteoritics & planetary science</subfield><subfield code="d">Lawrence, Kan. : Allen Press, 1996</subfield><subfield code="g">51(2016), 11, Seite 2127-2153</subfield><subfield code="w">(DE-627)193298368</subfield><subfield code="w">(DE-600)1306943-3</subfield><subfield code="w">(DE-576)060237333</subfield><subfield code="x">1086-9379</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:51</subfield><subfield code="g">year:2016</subfield><subfield code="g">number:11</subfield><subfield code="g">pages:2127-2153</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">http://dx.doi.org/10.1111/maps.12675</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">http://search.proquest.com/docview/1837124045</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-GEO</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-GGO</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2004</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">51</subfield><subfield code="j">2016</subfield><subfield code="e">11</subfield><subfield code="h">2127-2153</subfield></datafield></record></collection>
|
score |
7.4007235 |