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chopinite

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Journal Article
Published: 01 February 2010
American Mineralogist (2010) 95 (2-3): 260–272.
... backscatter diffraction patterns and maps, together with chemical analyses and Fe-Mg-Mn distribution among phosphates, confirm identification of the orthophosphate as sarcopside, chopinite, and farringtonite; no graftonite was found. Phosphates are found as (1) narrow rims between metal and forsterite...
FIGURES | View All (13)
Journal Article
Published: 01 March 2007
European Journal of Mineralogy (2007) 19 (2): 229–245.
...Edward S. Grew; Thomas Armbruster; Olaf Medenbach; Martin G. Yates; Christopher J. Carson Abstract Chopinite, the Mg-dominant analogue of sarcopside, is a new mineral corresponding to synthetic Mg 3 (PO 4 ) 2 -II, a high-pressure polymorph of the meteoritic mineral farringtonite. A representative...
FIGURES | View All (11)
Image
Plots of Cl/(Cl+F) vs. Mg/(Mg+Fe) for primary fluorapatite and biotite in sample 121401E, including data from Grew et al.(2006). (a) Fluorapatite. Numbers in legend refer to section; C indicates spots near chopinite, W indicates spots near wagnerite. (b) Numbers in legend refer to three sections of sample 121401E (sections 4 – 2 and 4 – 3 are from the same slice as the chopinite-bearing section, but do not contain chopinite).
Published: 01 March 2007
Fig. 6. Plots of Cl/(Cl+F) vs. Mg/(Mg+Fe) for primary fluorapatite and biotite in sample 121401E, including data from Grew et al. (2006) . (a) Fluorapatite. Numbers in legend refer to section; C indicates spots near chopinite, W indicates spots near wagnerite. (b) Numbers in legend refer
Image
Photomicrograph of fluorapatite segregation (Ap) containing four grains of chopinite (numbered, Fig. 4) in section 121401E4. Matrix is quartz (Qz); Bt 1 and 2 – biotite grains closest to chopinite (Table 9); only a tip of the second grain is visible in this photograph. Plane polarized light.
Published: 01 March 2007
Fig. 3. Photomicrograph of fluorapatite segregation (Ap) containing four grains of chopinite (numbered, Fig. 4 ) in section 121401E4. Matrix is quartz (Qz); Bt 1 and 2 – biotite grains closest to chopinite (Table 9 ); only a tip of the second grain is visible in this photograph. Plane polarized
Journal Article
Published: 01 December 2012
The Canadian Mineralogist (2012) 50 (6): 1445–1452.
...Frédéric Hatert; Encarnación Roda-Robles; Philippe de Parseval; Johan Wouters Abstract Zavalíaite, (Mn 2+ ,Fe 2+ ,Mg) 3 (PO 4 ) 2 , belongs to the sarcopside group of minerals and corresponds to the Mn 2+ equivalent of sarcopside and chopinite. It occurs at the La Empleada pegmatite, San Luis...
FIGURES
Image
Mg/Fe ratios of coexisting chladniite and sarcopside-chopinite in GRA95209 (GRA) and terrestrial (Terra) occurrences (a) and between chladniite and farringtonite in GRA95209 (b). (a) KD = (Mg/Fe)Src/(Mg/Fe)Cld; R2 = 0.936 for least-squares fit to sarcopside-chopinite (GRA95209 data only) and KD = (Mg/Fe)Grf/(Mg/Fe)Cld; R2 = 0.858 for least-squares fit to terrestrial graftonite. (b) The two points give KD (Far-Chp) = (Mg/Fe)Far/(Mg/Fe)Chp from analytical data on grains analyzed in PTS, 39 area 2-1 (Fig. 5e) and the line gives a least-squares fit for all the farringtonite data: KD = (Mg/Fe)Far/(Mg/Fe)Cld; R2 = 0.411. Chopinite in the second 3-phase assemblage did not give a satisfactory analysis, and so is not plotted. Sources for terrestrial pairs: Corbella i Cordomí and Malgarejo i Draper (1990), Černý et al. (1998), Livingstone (1980), Roda et al. (2004), F. Hatert (personal communication 2007); for GRA95209 (this study).
Published: 01 February 2010
F igure 11. Mg/Fe ratios of coexisting chladniite and sarcopside-chopinite in GRA95209 (GRA) and terrestrial (Terra) occurrences ( a ) and between chladniite and farringtonite in GRA95209 ( b ). ( a ) K D = (Mg/Fe) Src /(Mg/Fe) Cld ; R 2 = 0.936 for least-squares fit to sarcopside
Image
Schematic pressure-temperature diagram showing isopleths calculated from the reaction and volume change in the Mg3(PO4)2 system (Chp 1-Far 1, Brunet & Vielzeuf 1996; Brunet et al. 1998) for chopinite-sarcopside solid solution associated with farringtonite solid solution and assuming both solid solutions are ideal and a Kd = (Mg/Fe)Far/(Mg/Fe)Chp = 2.30 (Fig. 11a). Charalampides et al. (1988) synthesized sarcopside containing 40% chopinite at 0.8 kbar, 500 °C (arrow Chp 0.4). Numbered gray-filled boxes indicate peak (I) and post peak (II, III) metamorphic conditions for the Larsemann Hills based on P-T estimates reported for the Larsemann Hills and nearby exposures (Thost et al., 1994; Fitzsimons, 1996; Carson et al., 1997). Unnumbered gray-filled box indicates synthesis conditions for (Mg0.8Fe0.2)3(PO4)2 (average composition) by London et al.(1999). Al2SiO5 relations are from Pattison (1992). And – andalusite, Chp – chopinite, Far – farringtonite, Ky – kyanite, Sil – sillimanite.
Published: 01 March 2007
Fig. 10. Schematic pressure-temperature diagram showing isopleths calculated from the reaction and volume change in the Mg 3 (PO 4 ) 2 system (Chp 1-Far 1, Brunet & Vielzeuf 1996 ; Brunet et al. 1998 ) for chopinite-sarcopside solid solution associated with farringtonite solid solution
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Maximum binary ranges in mol% Fe3(PO4)2 and Mn3(PO4)2 for compositions of (Mg,Fe,Mn)3(PO4)2 (orthophosphate) structures obtained by synthesis. Farringtonite at 1 bar, 800°C (Annersten et al. 1980; Nord and Stefanidis 1980), Mn-Fe sarcopside at 200–800 bars, 300°C (Ericsson et al. 1986), Mg-Fe sarcopside at 500–800 bars, 300–650°C (Charalampides et al. 1988), Fe-Mg chopinite at 30 kbar, 600°C (Annersten and Nord 1980), and graftonite at 1 bar, 800°C (Nord and Ericsson 1982a, 1982b). Fields for individual minerals: Far = farringtonite, Chp = chopinite, Grf = graftonite, Src = sarcopside.
Published: 01 February 2010
( Ericsson et al. 1986 ), Mg-Fe sarcopside at 500–800 bars, 300–650°C ( Charalampides et al. 1988 ), Fe-Mg chopinite at 30 kbar, 600°C ( Annersten and Nord 1980 ), and graftonite at 1 bar, 800°C ( Nord and Ericsson 1982a , 1982b) . Fields for individual minerals: Far = farringtonite, Chp = chopinite, Grf
Image
Compositions (mole proportions) of (Mg,Fe,Mn)3(PO4)2 phases analyzed in the three sections of GRA95209 (Floss 1999; McCoy personal communication 2005; McCoy et al. 2006; this study). Identity of the phases is based on electron backscattered diffraction or on being close in composition to grains so characterized. However, the identity of one composition (queried farringtonite) is richer in Fe than other farringtonite. Data for type chopinite and terrestrial compositions are from Grew et al. (2007) supplemented by analyses of sarcopside and graftonite in a sample from the Bull Moose Mine, South Dakota (this study), Loch Quoich, Scotland (F. Hatert personal communication 2007), and Cyrilov, Czech Republic (Škoda et al. 2007). Fields for individual minerals: Far = farringtonite, Chp = chopinite, Grf = graftonite, Src = sarcopside.
Published: 01 February 2010
in composition to grains so characterized. However, the identity of one composition (queried farringtonite) is richer in Fe than other farringtonite. Data for type chopinite and terrestrial compositions are from Grew et al. (2007) supplemented by analyses of sarcopside and graftonite in a sample from the Bull
Image
(a) Kikuchi pattern for chopinite section PTS, 40, area 1-2b. The numbers on the image are Miller indices for the poles at the intersection of the bands, which are produced by specific sets of crystallographic planes. The mean angular deviations for the match (b) are 0.536. The + in both images is an artifact of the calibration (basically pattern centering).
Published: 01 February 2010
F igure 2. ( a ) Kikuchi pattern for chopinite section PTS, 40, area 1-2b. The numbers on the image are Miller indices for the poles at the intersection of the bands, which are produced by specific sets of crystallographic planes. The mean angular deviations for the match ( b ) are 0.536
Image
Projection of the chopinite structure along b. M2 octahedra (Mg enriched) form unbroken edge-sharing chains parallel to a, whereas M1 octahedra (Fe enriched) alternate with vacant polyhedra (dark with line and cross pattern). PO4 tetrahedra are marked with crosses.
Published: 01 March 2007
Fig. 1. Projection of the chopinite structure along b . M2 octahedra (Mg enriched) form unbroken edge-sharing chains parallel to a , whereas M1 octahedra (Fe enriched) alternate with vacant polyhedra (dark with line and cross pattern). PO 4 tetrahedra are marked with crosses.
Image
Plot of natural farringtonite, graftonite, sarcopside, and chopinite compositions in terms of the divalent cations excluding Ca. The fields for terrestrial graftonite (dashed line) and sarcopside (solid line) are largely from intergrowths (Černý et al., 1998; Corbella i Cordomí & Melgarejo i Draper, 1990; Fontan & Fransolet, 1986; Fransolet, 1977; Fransolet et al., 1986; Hurlbut, 1965; Huvelin et al. (1971); Lindberg (1950); Livingstone, 1980; Malló et al., 1995; Palache et al. (1951); Povondra et al., 1987; Roda et al., 2004; Smeds et al.,1998; Stalder & Rozendaal, 2002; Zhang, 1995). Sources of other data: chopinite (this paper); farringtonite (Fuchs et al., 1973; Bild, 1974; Buseck & Holdsworth, 1977); phosphates in meteorite GRA 95209 (Floss, 1999; McCoy et al., 2006); graftonite and sarcopside in IVA and IIIAB iron meteorites (Bild, 1974; Olsen et al., 1999); phosphate (sarcopside?) in the Brahin pallasite (Buseck & Holdsworth, 1977).
Published: 01 March 2007
Fig. 2. Plot of natural farringtonite, graftonite, sarcopside, and chopinite compositions in terms of the divalent cations excluding Ca. The fields for terrestrial graftonite (dashed line) and sarcopside (solid line) are largely from intergrowths ( Černý et al. , 1998 ; Corbella i Cordomí
Image
Chopinite (Cpn) enclosed in fluorapatite (Ap) in section 121401E4. (a) Photomicrograph of grain 1. Plane polarized light. (b) Back scattered electron image of this grain. (c) Photomicrograph of grain 3. Plane polarized light. (d) Back scattered electron image of this grain. (e) Back scattered electron image of grain 2. (f) Back scattered electron image of grain 4. Qz – quartz, Xnt – xenotime-(Y). Darker areas in the photomicrographs are secondary minerals.
Published: 01 March 2007
Fig. 4. Chopinite (Cpn) enclosed in fluorapatite (Ap) in section 121401E4. (a) Photomicrograph of grain 1. Plane polarized light. (b) Back scattered electron image of this grain. (c) Photomicrograph of grain 3. Plane polarized light. (d) Back scattered electron image of this grain. (e) Back
Image
Back-scattered electron images of phosphates in GRA95209. (a) Chladniite rim between metal and plagioclase plus enstatite, PTS, 39, area 1–8. (b) Chladniite and farringtonite in rim near forsterite, PTS, 39, area 5 (c) Forsterite with fayalite rim against chladniite and sarcopside, PTS, 39, area 1–3 (cf. rectangle in Fig. 4b). (d) Sarcopside with pitted surface surrounded by rim of chladniite, containing plates of graphite, PTS, 39, area 1–4. (e) Three-phase phosphate assemblage, PTS, 39, area 2-1. (f) Chopinite (confirmed with EBSD, Table 1, analysis Table 6) and chladniite; unmarked area is a mixture, PTS, 40, area 1. Note patch of fayalite between enstatite and forsterite. Chp = chopinite, Cld = chladniite, En = enstatite, Fa = fayalite, Far = farringtonite, Fo = forsterite, Gr = graphite, Src = sarcopside.
Published: 01 February 2010
and sarcopside, PTS, 39, area 1–3 (cf. rectangle in Fig. 4b ). ( d ) Sarcopside with pitted surface surrounded by rim of chladniite, containing plates of graphite, PTS, 39, area 1–4. ( e ) Three-phase phosphate assemblage, PTS, 39, area 2-1. ( f ) Chopinite (confirmed with EBSD, Table 1 , analysis Table 6
Image
Mn/Fe ratios of coexisting chladniite-johnsomervilleite (Jhn), sarcopside (Src)-chopinite, graftonite (Grf) and farringtonite in GRA95209 (this study), terrestrial occurrences (Terra; sources are given in caption for Fig. 11) and IIIAB iron meteorites (Olsen et al. 1999). Lines are least-squares fit to terrestrial graftonite-johnsomervilleite pairs (R2 = 0.969) and terrestrial sarcopside-johnsomervilleite pairs (R2 = 0.986).
Published: 01 February 2010
F igure 12. Mn/Fe ratios of coexisting chladniite-johnsomervilleite (Jhn), sarcopside (Src)-chopinite, graftonite (Grf) and farringtonite in GRA95209 (this study), terrestrial occurrences (Terra; sources are given in caption for Fig. 11 ) and IIIAB iron meteorites ( Olsen et al. 1999 ). Lines
Journal Article
Published: 01 January 2008
American Mineralogist (2008) 93 (1): 252–256.
...Kim Tait; Glenn Poirier; Ralph Rowe; Paula C. Piilonen † E-mail: [email protected] © 2008 American Mineralogist 2008 E.S. Grew, T. Armbruster, O. Medenbach, M.G. Yates, C.J. Carson (2007) Chopinite, [(Mg,Fe) 3 ](PO 4 ) 2 , a new mineral isostructural with sarcopside, from...
Journal Article
Published: 01 July 2019
European Journal of Mineralogy (2019) 31 (4): 661–663.
...-pressure form of Mg 3 (PO 4 ) 2 , was named “Chopinite” in his honour ( Grew et al., 2007 ). In 2005 Christian Chopin was inducted into the prestigious Leopoldina , the German National Academy of Science founded in 1652, and in 2012 he became a member of the similarly esteemed Accademia...
FIGURES
Image
Isopleths calculated from the experimentally determined reaction and volume change in the Mg3(PO4)2 system (solid line) for end-member chopinite and farringtonite (Brunet and Vielzeuf 1996; Brunet et al. 1998) assuming ideal solid solution for both minerals (Grew et al. 2006, 2007). The KD values are taken from the analytical data on PTS, 39 area 2-1 and the least-squares fits in Figure 11 (dashed and dotted lines, respectively). Chp 65 and Far 80 are measured composition [in terms of 100 Mg/(Mg+Fe) atomic]; the other values are calculated. Charalampides et al. (1988) synthesized sarcopside with 40% Mg3(PO4)2 at 0.8 kbar, 500°C (arrow).
Published: 01 February 2010
F igure 13. Isopleths calculated from the experimentally determined reaction and volume change in the Mg 3 (PO 4 ) 2 system (solid line) for end-member chopinite and farringtonite ( Brunet and Vielzeuf 1996 ; Brunet et al. 1998 ) assuming ideal solid solution for both minerals ( Grew et al
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(a) Back scattered electron image in section 121401E19 of orthopyroxene (Opx) partially altered to phyllosilicates, including biotite, and separated from fluorapatite (Ap) and wagnerite (W) by a corona consisting of K-feldspar (lighter), quartz and oligoclase (both darker). (b) Photomicrograph of sapphirine in direct contact with quartz in section 121401E8. Hercynite (Hc) in grain next to sapphirine is largely altered to a transparent material (diaspore?). Plane light. (c) Photomicrograph of corundum in quartz in section 121401E4 – 2 (2nd cut of slice yielding chopinite). Plane light (d) Back scattered electron image of (c) showing corundum (Crn) mantled by sillimanite (S) in quartz (Qtz). Analyses are given in Table 11. Sillimanite is partially altered to phyllosilicate, resulting in speckled material.
Published: 01 March 2007
) Photomicrograph of sapphirine in direct contact with quartz in section 121401E8. Hercynite (Hc) in grain next to sapphirine is largely altered to a transparent material (diaspore?). Plane light. (c) Photomicrograph of corundum in quartz in section 121401E4 – 2 (2 nd cut of slice yielding chopinite). Plane light
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Distribution of Fe and Mg between (Mg, Fe)3(PO4)2 phases, fillowite group minerals and biotite. (a) KD = (Mg/Fe)Far /(Mg/Fe)Scp. Sources of data: Livingstone (1980), Černý et al.(1998), and Corbella i Cordomí-and-Melgarejo-i Draper (1990) for sarcopside and johnsomervilleite; Floss (1999) and McCoy et al.(2006) for farringtonite, “Mg-graftonite”, graftonite/sarcopside and chladniite in lodranite GRA 95209. (b) KD = (Mg/Fe)P /(Mg/Fe)Chp, where P is the (Mg, Fe)3(PO4)2 phosphate reported by London et al.(1999) as sarcopside. Sources of data: Camparis analyses of chopinite (average from Table 6), Camparis analyses of biotite in grains 1 and 2 (Table 9), and analyses of synthetic (Mg, Fe)3(PO4)2 and biotite from London et al.(1999).
Published: 01 March 2007
: Camparis analyses of chopinite (average from Table 6 ), Camparis analyses of biotite in grains 1 and 2 (Table 9 ), and analyses of synthetic (Mg, Fe) 3 (PO 4 ) 2 and biotite from London et al. (1999) .