Kaersutite and Kaersutite Eclogite from Kakanui, New Zealand — Water-Excess and Water-Deficient Melting to 30 Kilobars

Total Page:16

File Type:pdf, Size:1020Kb

Kaersutite and Kaersutite Eclogite from Kakanui, New Zealand — Water-Excess and Water-Deficient Melting to 30 Kilobars Kaersutite and Kaersutite Eclogite from Kakanui, New Zealand — Water-Excess and Water-Deficient Melting to 30 Kilobars P J WYLLIE j department of the Geophysical Sciences, University of Chicago, Chicago, Illinois 60637 ABSTRACT ments significantly: dehydration reactions serve to buffer supplies of volatiles, principally water, and of the other "incompatible" A natural kaersutite megacryst (compositionally equivalent to elements (for example, Ti, K) available to participate in silicate olivine nephelinite) and a kaersutite eclogite nodule (equivalent to melting reactions, thereby limiting potential degrees of melting and olivine basanite) from the Mineral Breccia, Kakanui, New Zealand, controlling both quantities and compositions of magmas gener- were reacted in sealed platinum and Pd7()Ag3o alloy capsules, both ated. It is essential to comprehension of igneous and tectonic with excess water and no additional water present, using half-inch mechanisms active at depth, therefore, that hydrous minerals capa- piston-cylinder apparatus. Near-liquidus assemblages include or- ble of participating in reactions within Earth's upper mantle be thopyroxene at pressures greater than about 15 kb in water-rich identified and characterized. portions of the olivine-basanite system but not in the olivine- The world-wide occurrence of calcic amphiboles — generally nephelinite system. Reversed high-pressure limits of the amphibole kaersutite or pargasite as primary constituents of high-pressure, stability fields (excess water) have negative values of dP/dT, which possibly mantle-derived mineral assemblages in alpine-type crosses 25 kb at 1075°C and 30 kb at 925°C in the kaersutite sys- ultramafic bodies, in ophiolite complexes, and in ultramafic tem, but which crosses 25 kb at 1025°C and 30 kb at about 775°C xenoliths in alkali basalts — suggests that these amphiboles are es- in the kaersutite eclogite system. Comparison with experimental sential hydrous phases in subcrustal environments (LaCroix, 1917; results reported elsewhere indicates that amphiboles persist to Wilshire and Binns, 1961; Oxburgh, 1964). Experimental studies highest temperatures in basaltic liquids with greatest Ti02 contents indicate that pargasite can exist at upper mantle temperatures and but with lowest Na20/(Na20 + KaO) ratios and lowest Si02 pressures in hydrous peridotite (Kushiro, 1970; Mysen and contents. Boettcher, 1972, 1973; Green, 1973a) and in hydrous basaltic Experimental results suggest that many natural nephelinite and magmas (Allen and Boettcher, 1971, 1973). Irving and Green basanite magmas evolve from hydrous picritic parent magmas (1972) reported kaersutite to be stable in hydrous nepheline through deep-seated fractionation of olivine, possibly with mugearite up to 23 kb. clinopyroxene and garnet but excluding orthopyroxene. Although This investigation was undertaken to evaluate conditions under some olivine-rich basanitic liquids may be generated by partial fu- which natural kaersutite associated with alkali basalt may form sion of hydrous mantle peridotite, it is unlikely that orthopyroxene and, further, to explore possible roles which these amphiboles may fractionation is important in their subsequent evolution. play during the evolution of magmas within the upper mantle. To Experimental observations, together with chemical and petro- these ends, natural kaersutite has been studied experimentally graphic relations, support the following model petrogenetic history under simulated upper mantle conditions in a system of its own for the Kakanui Mineral Breccia: pyrope-rich garnet and omphacit- composition, as one component of a natural kaersutite-rich garnet ic pyroxene precipitated from ascending hydrous alkali basaltic clinopyroxenite (kaersutite eclogite), and in both of these systems magma (75 to 85 km, 1200° to 1300°C), then became trapped in with excess water present. deep-seated pockets within lherzolitic mantle, together with inter- cumulus liquid that precipitated kaersutite on cooling. Resulting EXPERIMENTAL METHODS kaersutite eclogite assemblages re-equilibrated subsolidus (75 to 85 km, 700° to 800°C) prior to being incorporated into a rapidly as- Starting Materials cending hydrous nephelinite magma, which was coprecipitating garnet, clinopyroxene, and probably kaersutite at depths >75 km The natural kaersutite megacryst (K-l) and the natural kaersutite (1100° to 1200°C). These accidental eclogitic inclusions underwent eclogite nodule (K-l4) used in this study were described by Mason partial melting during the subsequent rapid ascent, which was ter- (1966, 1968b). They were found as inclusions in the Mineral Brec- minated by an explosive eruption. Key words: experimental ig- cia Member of the Deborah Volcanic Formation at Kakanui, New neous petrology, phase equilibria, olivine nephelinite, olivine Zealand. The source locality and Mineral Breccia association have basanite, upper mantle, hydrous magma, volcanic breccia, horn- been discussed by Mason (1966, 1968a, 1968b), Dickey (1968), blende eclogite. and White and others (1972). The breccia consists of nephelinite host basalt, enclosing a suite of lherzolite, pyroxenite, dunite, kaer- INTRODUCTION sutite eclogite, and granulite nodules, as well as megacrysts of kaer- sutite, pyrope-rich garnet, aluminous clinopyroxene, anorthoclase, In theory, hydrous minerals can influence magma genesis and and ilmenite. tectonic activity within lower crustal and upper mantle environ- Mason (1966) reported a wet chemical analysis of the kaersutite1 megacryst (K-l), which he later modified (Mason, 1968a). A third * Present address: Lunar Science Institute, 3303 Nasa Road 1, Houston, Texas chemical analysis (Mason, 1969, written commun.) is compared 77058. with a microprobe analysis of the material used in these experi- Geological Society of America Bulletin, v. 86, p. 55J-J70, 7 figs., April 1975, Doc. no. 50415. 555 Downloaded from http://pubs.geoscienceworld.org/gsa/gsabulletin/article-pdf/86/4/555/3444124/i0016-7606-86-4-555.pdf by guest on 02 October 2021 556 MERRILL AND WYLLIE ments (Table 1). Trace-element contents (K, Rb, Sr, Ba, and REE) TABLE 1. ANALYSES OF EXPERIMENTAL STARTING MATERIALS of another portion of this same megacryst have been reported by Philpotts and others (1972; their specimen GSFC #21e). Weight + + + Mason (1968b) described the kaersutite eclogite nodule K-14 Per Cent 1 2 3 4 5 6 (Table 1), reporting a modal analysis (vol percent): 62 percent Si02 41.53 40.37 41.20 (41.4) (49.4) (39.4) kaersutite, 18 percent pyrope-rich garnet, 18 percent omphacitic clinopyroxene, and 2 percent ilmenite. Philpotts and others (1972) Ti02 4.46 4.38 3.20 5.1 1.5 0.5 reported trace-element contents of similar kaersutite eclogite AI203 14.35 14.90 16.35 13.7 8.4 20.2 nodules from the Mineral Breccia. Fe203 3.30 2.87 * * Apparatus and Experimental Procedures FeO 10.38* 7.95 11.40 13.9 10.8* 22.8 MnO 0.11 0.09 0.20 The megacryst and nodule samples were ground in acetone to pass a 200-mesh sieve, which discriminated against particles >74 MgO 12.84 12.80 10.93 10.2 10.5 10.3 /xm in dimension; average dimension of particles in starting mix- CaO 10.37 10.30 9.61 9.7 16.4 6.8 tures was <50 /xm. Na20 2.(8) 2.60 2.33 3.6 3.0 Resulting powders were sealed into capsules of platinum or K 2.(2) 2.05 0.86 1.4 Pd70Ag30, either dry or with measured percentages of distilled, 2° deionized water. Capsules which initially contained free water were 0.00 0.14 P2°5 tested for leaks before and after runs by application of heat; those 0.90 0.38 (1.0) which failed to expand were discarded. Capsules were run in H20+ piston-cylinder apparatus (Boyd and England, 1960) with a H2O" 0.04 0.20 Vi-in.-diameter pressure chamber. Materials used within the F 0.15 graphite furnace included talc, Pyrex glass, crushable alumina, and AlSiMg 730. Talc pieces were used alone below 850°C; at Total, less 0 for F 99.05 99.70 99.71 (100.0) (100.0) (100.0) higher temperatures, Pyrex glass was used below the capsule and 100 Mq combinations of the other materials above the capsule. 69 68 57 57 63 44 Mg + Fe The "piston-out" experimental procedures described by Boyd and others (1967) was employed. Calculation of pressures exerted on samples is complicated by several factors (Bell and Williams, * Fe reported as FeO. 1971; Johannes and others, 1971), many of which are poorly un- t Partial analysis. Parentheses designate approximate values, derstood. A. J. Irving (1972, written commun.) calibrated our ap- calculated assuming sum to be 100.0. paratus against the melting curve of NaCl, using differential ther- 1. Microprobe analysis of kaersutite megacryst K-l. Applying the 2 2 3 mal analysis techniques, and obtained brackets [1082° to 1089°C, Fe /(Fe + Fe ) ratio of column 2: Fe20, 3.13, FeO 7.55. Total 14.2 ± 0.3 kb; 1213° to 1220°C, 15.4 ± 0.2 kb], which agree with includes Cr203 0.0(1). Analyst: R. B. Berrill. results Clark (1959) obtained in hydrostatic apparatus. This 2. Kaersutite megacryst K-l. Total Fe calculated as FeO: 10.92. confirms that the nominal "piston-out" pressures reported here re- Mason, personal communication, 1969. quire little correction for friction effects. Chromel-alumel ther- 3. Kaersutite eclogite nodule K-14. Whole rock. Mason, 1968b, mocouples were used up to 850°C, and Pt-PtlORh thermocouples Table 3. were used at higher temperatures. Temperatures are precise within 4. Kaersutite in kaersutite eclogite nodule K-14. Microprobe anal- 5°C and have not been corrected for pressure effects on ther- ysis for Ti, Al, Fe, Mg, Ca, Na, and K reported by Mason, 1968b, Table 4. mocouple emf. Judging from recent studies of these effects for chromel-alumel and for Pt-PtlORh thermocouples (for example, 5. Omphacitic pyroxene in kaersutite eclogite nodule K-14. Micro- probe analysis for Ti, Al, Fe, Mg, Ca, and Na reported by Mason, Getting and Kennedy, 1970), the maximum uncertainty attributa- 1968b, Table 4. ble to pressure effects is ±13°C in experiments at 1000°C (30 kb) 6.
Recommended publications
  • Comments On'kaersutite from San Carlos, Arizona, with Comments On
    MINERALOGICAL MAGAZINE, SEPTEMBER I969, VOL. 37, NO. 287 Comments on 'Kaersutite from San Carlos, Arizona, with comments on the paragenesis of this mineral' by Brian Mason MARTIN PRINZ ~ Department of Geology, University of New Mexico, Albuquerque, New Mexico 87Io6 AND C. E. NEHRU Department of Geology, Brooklyn College, Brooklyn, New York II2~O s u MM A R Y. Electron probe analyses have been made of eight kaersutites from San Carlos, A~cizona, and one from Kakanui, New Zealand; also of olivine, clinopyroxene, ilmenite, and spinel from San Carlos. There is not as yet adequate evidence that the kaersutite is an upper mantle phase. MASON (I968a) suggests that kaersutite, as exemplified by the occurrence at San Carlos, Arizona, as well as from some other localities, may represent the amphibole phase in upper mantle rocks. The possibility of amphibole as an upper mantle phase was most clearly suggested by Oxburgh (I964) since it would help explain the alkali content of basaltic rocks, which otherwise would be derived from alkali-poor ultra- mafic mantle rocks. Since we are carrying out a detailed study of the ultramafic inclusions of the San Carlos, Arizona, locality, we would like to clarify some of the petrologic significance of the kaersutite from this area because it leads us to different conclusions from those of Mason. Hopefully, our comments will be of value to others suggesting amphibole as an upper mantle phase. San Carlos locality. The kaersutite described by Mason (I968a) in the San Carlos locality occurs as a granular aggregate of anhedral crystals, with a little inter-granular ilmenite.
    [Show full text]
  • Kaersutite-Bearing Xenoliths and Megacrysts in Volcanic Rocks from the Funk Seamount in the Southwest Indian Ocean
    Kaersutite-bearing xenoliths and megacrysts in volcanic rocks from the Funk Seamount in the southwest Indian Ocean ARCH M. REID* AND ANTON P. LE ROEX Department of Geology, University of Cape Town, Rondebosch 7700, South Africa Abstract Eight samples (seven volcanic rocks and one quartz sandstone) have been dredged from the Funk Seamount, 60 km NW of Marion Island in the southwest Indian Ocean Oat. 46 ~ 15' S, long. 37 ~ 20' E). The volcanic rocks are fine-grained vesicular basanitoids and glass-rich volcanic breccias geochemically similar to the Marion Island lavas. Lavas and breccias contain a suite of megacryst minerals and of small polymineralic xenoliths, in both of which kaersutite is a prominent constituent. The megacryst suite comprises large unzoned single grains of kaersutite, plagioclase, pyroxene, magnetite and ilmenite, all showing textural evidence of resorption/reaction with the basanitoid host. The megacrysts have a limited range of compositions except for the plagioclase which ranges from oligoclase to labradorite. The small (2 mm to ~ 3 cm) xenoliths are mostly two-pyroxene amphibole assemblages with or without olivine, magnetite, ilmenite, plagioclase and apatite. The xenoliths show some evidence of reaction with the basanitoid host and most have undergone recrystallization and/or localised decompression melting. Xenolith and megacryst assemblages are interpreted as being associated with the formation and partial crystallization of a hydrous basanitoid melt at depth. KEYWORDS: kaersutite, amphibole, xenolith, Funk Seamount, Indian Ocean. Introduction megacrysts. Brown amphibole is a prominent con- stituent of both xenolith and megacryst suites. F U N K S E A M O U N T is a prominent seamount situa- Mantle xenoliths in abyssal lavas are rare and so ted 60 km to the NW of Marion and Prince Edward these samples are of particular interest.
    [Show full text]
  • Petrology of Inclusion-Rich Lavas at Minna Bluff, Mcmurdo Sound, Antarctica: Implications for Magma Origin, Differentiation, and Eruption Dynamics
    PETROLOGY OF INCLUSION-RICH LAVAS AT MINNA BLUFF, MCMURDO SOUND, ANTARCTICA: IMPLICATIONS FOR MAGMA ORIGIN, DIFFERENTIATION, AND ERUPTION DYNAMICS Mary K. Scanlan A Thesis Submitted to the Graduate College of Bowling Green State University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE August 2008 Committee: Kurt Panter (Ph.D.), Advisor John Farver (Ph.D.) Thom Wilch (Ph.D.) © 2008 Mary Scanlan All Rights Reserved iii ABSTRACT Kurt Panter, Advisor Xeno Ridge, a newly discovered group of inclusion-rich deposits located at the top of the Minna Bluff stratigraphic section, formed as a result of magmatic mixing/mingling and provides insight into magma origins, mixing and eruption dynamics, and the evolution of Minna Bluff. Phonolite to tephriphonolite lavas are contain abundant inclusions which vary in size, shape, and mineralogy. Five inclusion types are identified at Xeno Ridge. The lavas that host the inclusions are dark-gray and porphyritic with a hypocrystalline, vesicular groundmass. Minerals within the host lavas include feldspar (plagioclase = An27–An84, alkali feldspar = Ab41Or57−Ab70Or20), amphibole (kaersutite), diopside (~Wo55En35Fs10), titanomagnetite (Ti# 55), olivine (Fo45, Fo81), and apatite. Type I inclusions are highly vesicular with sinuous forms and crenulate margins with the host indicating magmatic mixing/mingling. The mineral assemblage of Type I includes kaersutite (15-20 vol. %), feldspar (plagioclase = An33−An80, alkali feldspar = ~Ab55Or45), diopside (~Wo55En30Fs6), titanomagnetite (Ti# ~75), olivine (Fo48, Fo85) and apatite. Type II inclusions are kaersutite megacrysts and glomerocrysts dominated by kaersutite with subordinate phenocrysts, microphenocrysts and groundmass composed of plagioclase (An20 – An76), titanomagnetite (Ti# 84), diopside (~Wo50En35Fs15), and apatite. Type III is a single porphyritic inclusion with phenocrysts of anorthoclase and is similar in texture and mineralogy to lavas found within the Minna Bluff stratigraphic section.
    [Show full text]
  • List of Abbreviations
    List of Abbreviations Ab albite Cbz chabazite Fa fayalite Acm acmite Cc chalcocite Fac ferroactinolite Act actinolite Ccl chrysocolla Fcp ferrocarpholite Adr andradite Ccn cancrinite Fed ferroedenite Agt aegirine-augite Ccp chalcopyrite Flt fluorite Ak akermanite Cel celadonite Fo forsterite Alm almandine Cen clinoenstatite Fpa ferropargasite Aln allanite Cfs clinoferrosilite Fs ferrosilite ( ortho) Als aluminosilicate Chl chlorite Fst fassite Am amphibole Chn chondrodite Fts ferrotscher- An anorthite Chr chromite makite And andalusite Chu clinohumite Gbs gibbsite Anh anhydrite Cld chloritoid Ged gedrite Ank ankerite Cls celestite Gh gehlenite Anl analcite Cp carpholite Gln glaucophane Ann annite Cpx Ca clinopyroxene Glt glauconite Ant anatase Crd cordierite Gn galena Ap apatite ern carnegieite Gp gypsum Apo apophyllite Crn corundum Gr graphite Apy arsenopyrite Crs cristroballite Grs grossular Arf arfvedsonite Cs coesite Grt garnet Arg aragonite Cst cassiterite Gru grunerite Atg antigorite Ctl chrysotile Gt goethite Ath anthophyllite Cum cummingtonite Hbl hornblende Aug augite Cv covellite He hercynite Ax axinite Czo clinozoisite Hd hedenbergite Bhm boehmite Dg diginite Hem hematite Bn bornite Di diopside Hl halite Brc brucite Dia diamond Hs hastingsite Brk brookite Dol dolomite Hu humite Brl beryl Drv dravite Hul heulandite Brt barite Dsp diaspore Hyn haiiyne Bst bustamite Eck eckermannite Ill illite Bt biotite Ed edenite Ilm ilmenite Cal calcite Elb elbaite Jd jadeite Cam Ca clinoamphi- En enstatite ( ortho) Jh johannsenite bole Ep epidote
    [Show full text]
  • Upper Mantle and Crustal Origin of Olivine-Pyroxene-Kaersutite
    VllA-12 0830h POSTER Upper Mantle and Crustal Origin of Olivine-Pyroxene- Kaersutite Megacryats, and Peridotite Curnulates and Xenoliths Rom the Bandama Volcanic Complex (Gran Ca- naria, Spain) Jose Mangas1 (36928451296; joae.mangasQhsica.ulpgc.es) Robert Clac&iatti2 (33-1-69084815; cloc&iatti@drecam cedr) Ftancisco Jase Perez-Torrado' (34-928451298; francisco.perezt3 fisi~a.ulpgces) Dominique Massare2 (33-1-69084815) (Sponsor: Emilio Herrer+A~rvpr~! 'Departamento de Fisica, Campup de Tafira, ULPGC, Las Palmas 35.017. Spain 2Laboratorie Pierre Sue, CEA, Gif sur lvette 91191, hance The Quatcrnary volcamc complex of Bandama is formed by a strornbo- lian cone and a caldera of phreatomagmatic-collapse origin It shows two lava flows of basanite cornposition and fall and base surge pyro- clastic deposits The lava Rows have alivine and augstediapside phe- riocrysts and as subordinate minerals spinel and magnetite. The pyro- ilastic deposits shvw olivine. clinopyroxene and kaersutite phenocrysts and megacrysts, pendotite cumulates (dimite, wehrlite, clinopyroxen- ite wtth olivinp, rhnopirmenite) and xenoliths (dunite 2nd Iherzolite) containing olivinc, augite-diopstde, enslatite, spmel, magnetite, phlo- gopite, apatite and pyrrhotitepentlandite Taking into aceount the val- canologd study and the microscopic, electron microprobe, microther- mometric (fluid and melt inclusions) and bulk-rock analysis of the 26 samples. we concliide that the mincrals which make up the megacrysts, curnulates and xenoliths dsplay dlfTerent characteristm between them and from the ratio to minerals oí the lava flow We interprete that thme samples were original4 under difieren1 LhermobarogeochemiraI conditions and that the basanitic magma which gave rise to the Ban- dama complex ascended fram upper mantle to the surface (-33 km ta O 5 km), trapping pendotile ciirnulates and xenoliths, and megacrysts of diKerents depths and genesis Irom the spinel stability field in the uppcr mantle lo the owanir crust (-27 km to -4.5 km) .
    [Show full text]
  • Rock-Forming Minerals of Lamprophyres and Associated Mafic Dykes from the KrušNé Hory/Erzgebirge (Czech Republic)
    Journal of the Czech Geological Society 47/12(2002) 23 Rock-forming minerals of lamprophyres and associated mafic dykes from the Kruné hory/Erzgebirge (Czech Republic) Horninotvorné minerály lamprofyrù a pøíbuzných mafických ilných hornin z Kruných hor (Èeská republika) (4 figs, 5 tabs) EDVÍN PIVEC1 FRANTIEK V. HOLUB2 MILO LANG1 JIØÍ K. NOVÁK1 MIROSLAV TEMPROK2 1 Geological Institute, Academy of Sciences of the Czech Republic, Rozvojová 135, CZ 16502 Praha 6, Czech Republic 2 Charles University, Faculty of Science, Albertov 6, CZ 12843 Praha 2, Czech Republic; e-mail: [email protected], [email protected] Electron microprobe analyses were made on micas, amphiboles, feldspars, chlorites and accessory minerals in lamprophyric dykes (kersantites, minettes, spessartites), and in associated mafic diorite to tonalite porphyries (porphyrites) of the Kruné hory (Erzgebirge) area and Mariánské Láznì region in Western Bohemia (Czech Republic). All studied rocks are altered to various degrees during deuteric and/or postmagmatic stages of evolution. The only primary mafic mineral preserved in all rock types is Mg-biotite to phlogopite, in spessartites and some diorite porphyries also Ti-rich hornblende corresponding to titanian magnesiohastingsite to kaersutite. Magmatic biotites are relatively rich in Ti with limited variations in their Mg/Fe ratios, evidently re-equilibrated during cooling or re-heating. Olivine is totally replaced by pilitic pseudomorphs and by biotite-actinolite clots. Phenocrystic clinopyroxene is completely uralitized, often in well-preserved original shapes. The secondary amphiboles correspond to Si-rich magnesiohornblende to actinolite. Chlorite and epidote are rather scarce and their impor- tant occurrences are restricted to limited number of samples.
    [Show full text]
  • Kaersutite Naca2[(Mg; Fe )4Ti](Si6al2)O22(OH)2 C 2001 Mineral Data Publishing, Version 1.2 ° Crystal Data: Monoclinic
    2+ Kaersutite NaCa2[(Mg; Fe )4Ti](Si6Al2)O22(OH)2 c 2001 Mineral Data Publishing, version 1.2 ° Crystal Data: Monoclinic. Point Group: 2=m: Commonly as well-formed phenocrysts with rhombic basal sections; prismatic, to 10 cm; as granular aggregates. Twinning: Simple or multiple twinning 100 . k f g Physical Properties: Cleavage: Perfect on 110 , intersecting at 56± and 124±; partings on 100 , 001 . Tenacity: Brittle. Hardness = 5f{6 gD(meas.) = 3.2{3.28 D(calc.) = [3.11] f g f g Optical Properties: Semitransparent. Color: Dark brown to black, typically zoned; yellow-brown, green-brown, or red-brown in thin section. Luster: Vitreous. Optical Class: Biaxial ({). Pleochroism: Strong; X = yellow, yellow-brown; Y = red, red-brown; Z = deep brown, dark red-brown. Orientation: Y = b; Z c = 0±{19±. Dispersion: r > v: Absorption: Z Y > X. ® = 1.670{1.689 ¯ = 1^.690{1.741 ° = 1.700{1.772 ¸ 2V(meas.) = 66±{82± Cell Data: Space Group: C2=m: a = 9.8903(3) b = 18.0596(5) c = 5.3152(2) ¯ = 105:4(1)± Z = 2 X-ray Powder Pattern: Boulder Dam area, Arizona, USA. (ICDD 17-478). 2.693 (100), 3.11 (80), 8.38 (65), 3.36 (65), 2.548 (65), 2.589 (55), 1.439 (55) Chemistry: (1) (2) (1) (2) SiO2 39.50 39.88 MgO 12.90 14.10 TiO2 10.33 4.69 CaO 10.91 13.05 Al2O3 11.12 14.25 Na2O 3.82 1.86 Fe2O3 0.06 9.58 K2O 1.43 1.80 FeO 9.44 0.10 F 0.14 + MnO 0.10 0.10 H2O 0.59 0.53 Total 100.20 100.08 2+ (1) Qaersut, Greenland; corresponds to (Na1:11K0:28)§=1:39Ca1:76(Mg2:89Fe1:19Ti1:17 3+ Fe0:01Mn0:01)§=5:27(Si5:93Al1:97)§=7:90O22(OH)0:59: (2) Vl·c¶³ Hora, Czech Republic; 3+ by microanalysis, corresponds to (Na0:53K0:41)§=0:94Ca2:06(Mg3:10Fe1:06Ti0:52Al0:34 2+ Fe0:01Mn0:01)§=5:04(Si5:87Al2:13)§=8:00O22[(OH)1:94F0:06]§=2:00: Polymorphism & Series: Forms a series with ferrokaersutite.
    [Show full text]
  • Petrogenesis of Fe-Ti Oxides in Amphibole-Rich Veins From
    Petrogenesis of Fe-Ti oxides in amphibole-rich veins from the Lherz orogenic peridotite (Northeastern Pyrénées, France) Jean-Pierre LORAND and Michel GREGOIRE 1 Laboratoire de Minéralogie et Cosmochimie, Muséum National d‟Histoire Naturelle et CNRS UMR 7202, CP 52, 61 Rue Buffon, 75005 Paris, France ([email protected]) 2 CNRS UMR 5562-OMP, Toulouse University, 14 Av. Edouard Belin, F-31400 Toulouse, France Abstract : Accessory, homogeneous ilmenite and rutile are important oxide phases in amphibole- rich high-pressure cumulate veins which crosscut the Lherz orogenic lherzolite massif. Those veins crystallized from alkaline melts at P = 1.2-1.5 GPa within the uppermost lithospheric mantle. Transitional basalts contaminated by peridotitic wall-rocks and then uncontaminated alkali basalts (basanites) reused the same vein conduits. Petrographic observations give evidence that Fe-Ti oxide saturation depends on the silica contents of each parental melt. The water-poor silica-rich transitional melts that generated websterites and plagioclase-rich clinopyroxenites reached early Ti- oxide saturation (1200°C; 1.5 Gpa). Rutile is as abundant as ilmenite. It is enriched in Nb-Zr-Hf by a factor of 10 to 100 relative to either amphibole or ilmenite. The amphibole pyroxenites and hornblendites crystallized from basanites reached late Fe-Ti oxide saturation after precipitation of amphibole, with ilmenite crystallizing along with phlogopite in the latter. The Lherz ilmenites are devoid of exsolution and contain very little trivalent iron. This compositional feature indicates more reducing crystallization conditions than usually inferred for alkali lavas and their megacrysts (FMQ±1). The veins incompletely equilibrated for redox conditions with their wall-rock peridotites which record more oxidizing conditions (FMQ±1).
    [Show full text]
  • A Comparative Study of Kaersutite in the Egersund Dikes and Snc Meteorites
    A COMPARATIVE STUDY OF KAERSUTITE IN THE EGERSUND DIKES AND SNC METEORITES Senior Thesis Submitted in partial fulfillment of the requirements for the Bachelor of Science Degree At The Ohio State University By Ellie Hagen The Ohio State University 2017 Approved by Dr. Michael Barton, Advisor School of Earth Sciences ii T ABLE OF C ONTENTS Abstract……………………………………………………………..………….…..ii Acknowledgements……………………………………………….……..………iii List of Figures……………………………………………………….…………….iv List of Tables………………………………………………………..……………..v Introduction…………………………….………………………………………….1 Background…………………………….…..………………………………………2 Kaersutite…………………………….…….……………..……………....2 Egersund Ol-tholeiite Geology……………...……..…………………3 Martian Geology…………..………….……………………………..……4 SNC Meteorites…………………………………………………………….4 Methods Sampling Collection…………………………….…..………….………..6 Geochemistry……………………………………..……………...………..6 Petrology……..…………..……………..………………………………….7 Data interpretation……..……………………...………..……….……...7 Results Chassigny Petrology ………………………………..…….……..………8 Shergottite Petrology……………………………………….……….…..11 Egersund Ol-tholeiite Petrology………………………….……..……14 Bulk Rock Major Element Chemistry…………………….……..…...16 Rare Earth Element (REE) Comparison……….……...….………..…19 Kaersutite Chemistry………………………………………….………...20 Discussion Petrology……………….…..…………………….………...………………24 Presence of Shock……………………………………………….............25 Geochemistry……………………………………………………………....26 Recommendations for Future Works………..………………………………..28 References Cited….……….…………………………...……………………….....29 Appendix A (Kaersutite Chemistry)………………….……………………......31
    [Show full text]
  • Abbreviations for Names of Rock-Forming Minerals
    American Mineralogist, Volume 95, pages 185–187, 2010 Abbreviations for names of rock-forming minerals DONNA L. WHITNEY 1,* AN D BERNAR D W. EVANS 2 1Department of Geology and Geophysics, University of Minnesota, Minneapolis, Minnesota 55455, U.S.A. 2Department of Earth and Space Sciences, Box 351310, University of Washington, Seattle, Washington 98185, U.S.A. Nearly 30 years have elapsed since Kretz (1983) provided riebeckite (Rbk); and albite (Ab) and anorthite (An) as well as the mineralogical community with a systematized list of abbre- plagioclase (Pl), recognizing that some petrologists have uses for viations for rock-forming minerals and mineral components. Its these mineral names. In addition, although our focus is on rock- logic and simplicity have led to broad acceptance among authors forming minerals, some hypothetical and/or synthetic phases are and editors who were eager to adopt a widely recognized set of included in our list, as well as an abbreviation for “liquid” (Liq). mineral symbols to save space in text, tables, and figures. We have also included some abbreviations for mineral groups, Few of the nearly 5000 known mineral species occur in e.g., aluminosilicates (Als, the Al2SiO5 polymorphs), and other nature with a frequency sufficient to earn repeated mention in descriptive terms (e.g., opaque minerals). The choice of abbre- the geoscience literature and thus qualify for the designation viations attempts as much as possible to make the identity of the “rock-forming mineral,” but a reasonable selection of the most mineral instantly obvious and unambiguous. common and useful rock-forming minerals likely numbers in the several hundreds.
    [Show full text]
  • Kaersutite-Bearing Gabbroic Inclusions and the Late Dike Swarm of Kangerdlugssuaq, East Greenland
    MINERALOGICAL MAGAZINE, SEPTEMBER 1975, VOL. 40, VP. 259-83 Kaersutite-bearing gabbroic inclusions and the late dike swarm of Kangerdlugssuaq, East Greenland C. KENT BROOKS Institute of Petrology, University of Copenhagen R. G. PLATT Grant Institute of Geology, University of Edinburgh~ SUMMARY. The Kangerdlugssuaq late dike swarm, which strikes at a high angle to the well-known East Greenland coastal swarm, is described and chemical analyses presented. The basic members are characterized by a high potassium content. A variety of kaersutite-bearing gabbroic inclusions in one member of this swarm is described in detail and microprobe analyses of clinopyroxenes, amphi- boles, plagioclases, sheet silicates, and spinel minerals are presented. On the basis of this evidence it is deduced that these inclusions derive from a cumulate sequence formed at depths of between 5 and to km beneath the Lower Tertiary land surface. It is likely that fractionation of such assemblages causes a transition, at relatively low pressure, from undersaturated to oversaturated compositions, but the products appear to be quantitatively minor. IN contrast to the well-known, coast-parallel dike swarm of East Greenland (Wager and Deer, I938), there exists almost no information on the later, fjord-paralM swarm in Kangerdlugssuaq. In this paper we present petrological and chemical data on these rocks together with a detailed study of the minerals from an interesting suite of kaer- sutite-bearing plutonic inclusions in a member of the swarm. Within the lower Tertiary igneous province of East Greenland (Brooks, 1973a and b), kaersutite-bearing dike rocks have earlier been described by Vincent (I953), while a dike containing kaersutite megacrysts, associated with sahlite and diopside megacrysts and ultramafic inclusions, all of high-pressure origin, has recently been described from Wiedemanns Fjord, I5O km to the east, by Brooks and Rucklidge (1973).
    [Show full text]
  • Compositional Controls on the Formation of Kaersutite Amphibole in Shergottite Meteorites
    Lunar and Planetary Science XXXV (2004) 1177.pdf COMPOSITIONAL CONTROLS ON THE FORMATION OF KAERSUTITE AMPHIBOLE IN SHERGOTTITE METEORITES. K.M. Pitman 1,2 and A.H. Treiman 3. 1Dept. of Physics & Astronomy, Louisi- ana State University, Baton Rouge, LA 70803, USA <[email protected]>. 2Space Science Institute, Boul- der, CO 80303, USA. 3Lunar and Planetary Institute, Houston, TX 77058, USA <[email protected]>. Introduction: The shergottite basalts, meteorites of Johnson Space Center), we mapped both sections, con- Martian origin, contain rare small grains (~10-100 µm firmed optical identifications of kaersutite, and qualita- diam.) of kaersutite, a Ca-amphibole rich in Al and Ti tively identified the kaersutites’ host pyroxene and [1-3]. Kaersutites have been used to estimate the water nearby phases (Fig. 1a). Quantitative chemical analyses content of shergottites and the Martian mantle [4]; were obtained by EMP/WDS (Cameca SX100 at JSC), however, questions remain about the original water content of the amphiboles [5] and if they formed from using natural and synthetic standards. Chemical compo- magma [6]. We investigated the petrographic settings of sitions of the kaersutite, other inclusion phases, and amphiboles in two shergottites and confirm that these host pyroxenes are consistent with earlier results on amphiboles occur only in multiphase inclusions in py- these shergottites (Table 1, [1-3,7-9]). roxene. In fact, kaersutite is found only in pigeonite. Petrography and Mineral Chemistry: Kaersutite This suggests that the occurrence of amphibole is con- has been reported only in multi-mineral inclusions in trolled in part by the composition of its host phase.
    [Show full text]