共查询到20条相似文献,搜索用时 31 毫秒
1.
E. Wulff-Pedersen E. -R. Neumann R. Vannucci P. Bottazzi L. Ottolini 《Contributions to Mineralogy and Petrology》1999,137(1-2):59-82
Mantle xenoliths hosted by the historic Volcan de San Antonio, La Palma, Canary Islands include veined spinel harzburgites
and spinel dunites. Glasses and associated minerals in the vein system of veined xenoliths show a gradual transition in composition
from broad veins to narrow veinlets. Broad veins contain alkali basaltic glass with semi-linear trace element patterns enriched
in strongly incompatible elements. As the veins become narrower, the SiO2-contents in glass increase (46 → 67 wt% SiO2 in harzburgite, 43 → 58 wt% in dunite) and the trace element patterns change gradually to concave patterns depleted in moderately
incompatible elements (e.g. HREE, Zr, Ti) relative to highly incompatible ones. The highest SiO2-contents (ca. 68% SiO2, low Ti-Fe-Mg-Ca-contents) and most extreme concave trace element patterns are exhibited by glass in unveined peridotite
xenoliths. Clinopyroxenes shift from LREE-enriched augites in basaltic glass, to REE-depleted Cr-diopside in highly silicic
glass. Estimates indicate that the most silicic glasses represent melts in, or near, equilibrium with their host peridotites.
The observed trace element changes are compatible with formation of the silicic melts by processes involving infiltration
of basaltic melts into mantle peridotite followed by reactions and crystallization. The Fe-Mg interdiffusion profiles in olivine
porphyroclasts adjacent to the veins indicate a minimum period of diffusion of 600 years, implying that the reaction processes
have taken place in situ in the upper mantle. The CaO-TiO2-La/Nd relationships of mantle rocks may be used to discriminate between metasomatism caused by carbonatitic and silicic melts.
Unveined mantle xenoliths from La Palma and Hierro (Canary Islands) show a wide range in La/Nd ratios with relatively constant,
low-CaO contents which is compatible with metasomatism of “normal” abyssal peridotite by silicic melts. Peridotite xenoliths
from Tenerife show somewhat higher CaO and TiO2 contents than those from the other islands and may have been affected by basaltic or carbonatitic melts. The observed trace
element signatures of ultramafic xenoliths from La Palma and other Canary Islands may be accounted for by addition of small
amounts (1–7%) of highly silicic melt to unmetasomatized peridotite. Also ultramafic xenoliths from other localities, e.g.
eastern Australia, show CaO-TiO2-La/Nd relationships compatible with metasomatism by silicic melts. These results suggest that silicic melts may represent
important metasomatic agents.
Received: 15 November 1998 / Accepted: 17 May 1999 相似文献
2.
A. D. Beard H. Downes E. Hegner S. M. Sablukov V. R. Vetrin K. Balogh 《Contributions to Mineralogy and Petrology》1998,130(3-4):288-303
Minor magmatic intrusions of kimberlite, melilitite and cpx-melilitite occur in the southern part of the Kola Peninsula,
Russia, on the Terskii Coast and near the town of Kandalaksha. They yield K-Ar ages of 382 ± 14 Ma and 365 ± 16 Ma, similar
to the magmatic rocks from the Kola Alkaline Province. The Terskii Coast kimberlites have mineralogical and geochemical affinities
with group 1 kimberlites, whereas the Kandalaksha monticellite kimberlite more closely resembles calcite kimberlites. The
lower Al2O3 content in the Kola kimberlites indicates a strongly depleted harzburgitic source, while higher Al2O3 in the melilitites suggests a lherzolitic source. The Terskii Coast kimberlites are anomalously potassic and significantly
enriched in P and Ba compared to other group 1 kimberlites. In contrast, the melilitites are sodic and are anomalously depleted
in P compared to worldwide melilitites. Trace element patterns of the Kola kimberlites and melilitites indicate the presence
of K- and P-rich phases in the mantle source. To account for the K-troughs shown by both magma types, a K-rich phase such
as phlogopite is thought to be residual in their sources; however, the anomalous K-enrichment in the Terskii Coast kimberlites
may indicate that an additional metasomatic K-rich phase (e.g. K-richterite and/or a complex K-Ba-phosphate) existed in the
kimberlite source. The P-depletion in the melilitites may suggest that a phosphate phase such as apatite remained residual
in the melilititic source. However, anomalous P-enrichment in the kimberlites cannot be explained by complete melting of the
same phase because the kimberlites are a smaller degree melt; thus, it is most likely that another metasomatic phosphate mineral
existed in the source of the kimberlites. The Kola kimberlites and melilitites are all strongly LREE-enriched but the kimberlites
have a steeper REE pattern and are significantly more depleted in HREE, indicating a higher proportion of garnet in their
source. Higher Nb/Y ratios and lower SiO2 values in the kimberlites indicate that they were a smaller degree partial melt than the melilitites. The presence of diamonds
in the Terskii Coast kimberlites indicates a relatively deep origin, while the melilitites originated from shallower depth.
The non-diamondiferous Kandalaksha monticellite kimberlite has lower abundances of all incompatible trace elements, suggesting
a higher degree of partial melting and/or a less enriched and shallower source than the Terskii Coast kimberlites. The 87Sr/86Sri, 143Nd/144Ndi and Pb isotope compositions confirm that the Terskii Coast kimberlites have close affinities with group 1 kimberlites and
were derived from an asthenospheric mantle source, while the Kandalaksha monticellite kimberlite and Terskii Coast melilitites
were derived from lithospheric mantle. Impact of a Devonian asthenospheric mantle plume on the base of the Archaean-Proterozoic
lithosphere of the Kola Peninsula caused widespread emplacement of kimberlites, melilitites, ultramafic lamprophyres and other
more fractionated alkaline magmas. The nature of the mantle affected by metasomatism associated with the plume and, in particular,
the depth of melting and the stability of the metasomatic phases, gave rise to the observed differences between kimberlites
and the related melilitites and other magmas.
Received: 3 March 1997 / Accepted: 7 October 1997 相似文献
3.
The Finero phlogopite-peridotite massif: an example of subduction-related metasomatism 总被引:13,自引:0,他引:13
Alberto Zanetti Maurizio Mazzucchelli Giorgio Rivalenti Riccardo Vannucci 《Contributions to Mineralogy and Petrology》1999,134(2-3):107-122
The Finero peridotite massif is a harzburgite that suffered a dramatic metasomatic enrichment resulting in the pervasive
presence of amphibole and phlogopite and in the sporadic occurrence of apatite and carbonate (dolomite)-bearing domains. Pyroxenite
(websterite) dykes also contain phlogopite and amphibole, but are rare. Peridotite bulk-rock composition retained highly depleted
major element characteristics, but was enriched in K, Rb, Ba, Sr, LREE (light rare earth elements) (LaN/YbN = 8–17) and depleted in Nb. It has high radiogenic Sr (87Sr/86Sr(270) = 0.7055–0.7093), low radiogenic Nd (ɛNd(270) = −1 to −3) and EMII-like Pb isotopes. Two pyroxenite – peridotite sections examined in detail show the virtual absence of
major and trace element gradients in the mineral phases. In both rock types, pyroxenes and olivines have the most unfertile
major element composition observed in Ivrea peridotites, spinels are the richest in Cr, and amphibole is pargasite. Clinopyroxenes
exhibit LREE-enriched patterns (LaN/YbN ∼16), negative Ti and Zr and generally positive Sr anomaly. Amphibole has similar characteristics, except a weak negative
Sr anomaly, but incompatible element concentration ∼1.9 (Sr) to ∼7.9 (Ti) times higher than that of coexisting clinopyroxene.
Marked geochemical gradients occur toward apatite and carbonate-bearing domains which are randomly distributed in both the
sections examined. In these regions, pyroxenes and amphibole (edenite) are lower in mg## and higher in Na2O, and spinels and phlogopite are richer in Cr2O3. Both the mineral assemblage and the incompatible trace element characteristics of the mineral phases recall the typical
signatures of “carbonatite” metasomatism (HFSE depletion, Sr, LILE and LREE enrichment). Clinopyroxene has higher REE and
Sr concentrations than amphibole (amph/cpxDREE,Sr = 0.7–0.9) and lower Ti and Zr concentrations. It is proposed that the petrographic and geochemical features observed at
Finero are consistent with a subduction environment. The lack of chemical gradients between pyroxenite and peridotite is explained
by a model where melts derived from an eclogite-facies slab infiltrate the overhanging harzburgitic mantle wedge and, because
of the special thermal structure of subduction zones, become heated to the temperature of the peridotite. If the resulting
temperature is above that of the incipient melting of the hydrous peridotite system, the slab-derived melt equilibrates with
the harzburgite and a crystal mush consisting of harzburgite and a silica saturated, hydrous melt is formed. During cooling,
the crystal mush crystallizes producing the observed sequence of mineral phases and their observed chemical characteristics.
In this context pyroxenites are regions of higher concentration of the melt in equilibrium with the harzburgite and not passage-ways
through which exotic melts percolated. Only negligible chemical gradients can appear as an effect of the crystallization process,
which also accounts for the high amphibole/clinopyroxene incompatible trace element ratios. The major element refractory composition
is explained by an initially high peridotite/melt ratio. The apatite, carbonate-bearing domains are the result of the presence
of some CO2 in the slab-derived melt. The CO2/H2O ratio in the peridotite mush increased by crystallization of hydrous phases (amphibole and phlogopite) locally resulting
in the unmixing of a late carbonate fluid. The proposed scenario is consistent with subduction of probably Variscan age and
with the occurrence of modal metasomatism before peridotite incorporation in the crust.
Received: 20 July 1998 / Accepted: 28 October 1998 相似文献
4.
Carbonatite metasomatized peridotite xenoliths from southern Patagonia: implications for lithospheric processes and Neogene plateau magmatism 总被引:10,自引:0,他引:10
The mineral chemistry, major and trace element, and Sr–Nd isotopic composition of Cr-diopside, spinel peridotite xenoliths
from the Estancia Lote 17 locality in southern Patagonia document a strong carbonatitic metasomatism of the backarc continental
lithosphere. The Lote 17 peridotite xenolith suite consists of hydrous spinel lherzolite, wehrlite, and olivine websterite,
and anhydrous harzburgite and lherzolite. Two-pyroxene thermometry indicates equilibration temperatures ranging from 870 to
1015 °C and the lack of plagioclase or garnet suggests the xenoliths originated from between ˜40 and 60 km depth. All of the
xenoliths are LILE- and LREE-enriched, but have relatively low 87Sr/86Sr (0.70294 to 0.70342) and high ɛNd (+3.0 to +6.6), indicating recent trace element enrichment (∼25 Ma, based on the low 87Sr/86Sr and high Rb concentrations of phlogopite separates) in the long-term, melt-depleted Patagonian lithosphere. Lote 17 peridotite
xenoliths are divided into two basic groups. Group 1 xenoliths consist of fertile peridotites that contain hydrous phases
(amphibole ± phlogopite ± apatite). Group 1 xenoliths are further subdivided into three groups (a, b, and c) based on distinctive
textures and whole-rock chemistry. Group 1 xenolith mineralogy and chemistry are consistent with a complex metasomatic history
involving variable extents of recent carbonatite metasomatism (high Ca/Al, Nb/La, Zr/Hf, low Ti/Eu) that has overprinted earlier
metasomatic events. Group 2 xenoliths consist of infertile, anhydrous harzburgites and record cryptic metasomatism that is
attributed to CO2-rich fluids liberated from Group 1 carbonatite metasomatic reactions. Extremely variable incompatible trace element ratios
and depleted Sr–Nd isotopic compositions of Lote 17 peridotite xenoliths indicate that the continental lithosphere was neither
the primary source nor an enriched lithospheric contaminant for Neogene Patagonian plateau lavas. Neogene plateau magmatism
associated with formation of asthenospheric slab windows may have triggered this occurrence of “intraplate-type” carbonatite
metasomatism in an active continental backarc setting.
Received: 26 January 2000 / Accepted: 1 March 2000 相似文献
5.
Ultramafic lamprophyres (UML) are rare but widespread, hypabyssalrocks, rich in K, Mg, Cr, Ni, Sr, Ba, REE, and volatiles, containingless Si and more Ca than other silicate igneous rocks, and gradinginto carbonatites. They carry phenocryst combinations of olivine(Fo9272), phlogopite (rich in Ti, Fe3+ , Ba or F), Al-Ti-(Fe3+and richteritic to eckermannitic amphiboles. Groundmasses includeCa-Fe-Mg-carbonates (?partly primary), feldspathoids, Ca-Fe-Ti-Zr-garnets,soda-melilite, monti cellite, Mg-Mn-ilmenite, perovskite, serpentine,Fe- Mg-Ti-Mn-Cr-Al-spinels ? glass. Megacrysts include (?cognate)salitic pyroxenes, phiogopites or Ti-hastingsites, and morerarely, xenocrystic Cr-Ti-pyrope, orthopyroxenes and diopsides.Xenoliths include spinel and/or garnet-lherzolites, dunites,and phlogopite?amphibole-bearing pendotites. UML are readilydistinguished from kimberlites by petrological association (e.g.with ijolites), geochemistry (e.g. lower Mg, higher Ca, P),texture (e.g. lack of two olivine generations) and mineralogy(e.g. presence of groundmass feldspathoids ? melilite). UMLare distinguished also from melilitites by lower Si, Al, Na,higher Ca, K, P; more abundant primary carbonate, phiogopiteand amphibole; and by lack of groundmass olivine and phenocrystmelilite. Closer extrusive equivalents of UML may however occuramong ankaratrites. The most common UML types are aln?ite (melilite-rich)and aillikite (melilite-free, carbonate-rich). Aillikites arecompositionally closer to carbonatites than alnOites. Rarertypes include poizenite (melilite + feldspathoids), ouachitite(feldspathoids + carbonates) and damkjernite (feldspathoids+ carbonates+ < 10 per cent alkali feldspars). UML form localizeddyke-swarms or diatreme-clusters, mainly related to continentalrifting, and may represent parent magmas for coeval carbonatitecomplexes. Their additional occurrence in an oceanic setting,their mantle xenolith content, and their high mg, Cr and Ni,together suggest that many of them are primary, mantle-derivedmagmas, generated at depths between those of melilitites andkimberlites (c. 100150 km), but at higher CO2 pressuresthan melilitites. Other UML, however, have been extensivelymodified from primary compositions by fractionation, accumulation,or interaction with alkali+volatile-rich fluids. 相似文献
6.
The Lherz orogenic lherzolite massif (Eastern French Pyrenees) displays one of the best exposures of subcontinental lithospheric
mantle containing veins of amphibole pyroxenites and hornblendites. A reappraisal of the petrogenesis of these rocks has been
attempted from a comprehensive study of their mutual structural relationships, their petrography and their mineral compositions.
Amphibole pyroxenites comprise clinopyroxene, orthopyroxene and spinel as early cumulus phases, with garnet and late-magmatic
K2O-poor pargasite replacing clinopyroxene, and subsolidus exsolution products (olivine, spinel II, garnet II, plagioclase).
The original magmatic mineralogy and rock compositions were partly obscured by late-intrusive hornblendites and over a few
centimetres by vein–wallrock exchange reactions which continued down to subsolidus temperatures for Mg–Fe. Thermobarometric
data and liquidus parageneses indicate that amphibole pyroxenites started to crystallize at P ≥ 13 kbar and recrystallized at P < 12 kbar. The high AlVI/AlIV ratio (>1) of clinopyroxenes, the early precipitation of orthopyroxene and the late-magmatic amphibole are arguments for
parental melts richer in silica but poorer in water than alkali basalts. Their modelled major element compositions are similar
to transitional alkali basalt with about 1–3 wt% H2O. In contrast to amphibole pyroxenites, hornblendites only show kaersutite as liquidus phase, and phlogopite as intercumulus
phase. They are interpreted as crystalline segregates from primary basanitic magmas (mg=0.6; 4–6 wt% H2O). These latter cannot be related to the parental liquids of amphibole pyroxenites by a fractional crystallization process.
Rather, basanitic liquids mostly reused pre-existing pyroxenite vein conduits at a higher structural level (P ≤ 10 kbar). A continuous process of redox melting and/or alkali melt/peridotite interaction in a veined lithospheric mantle
is proposed to account for the origin of the Lherz hydrous veins. The transitional basalt composition is interpreted in terms
of extensive dissolution of olivine and orthopyroxene from wallrock peridotite by alkaline melts produced at the mechanical
boundary layer/thermal boundary layer transition (about 45–50 km deep). Continuous fluid ingress allowed remelting of the
deeper veined mantle to produce the basanitic, strongly volatiles enriched, melts that precipitated hornblendites. A similar
model could be valid for the few orthopyroxene-rich hydrous pyroxenites described in basalt-hosted mantle xenoliths.
Received: 15 September 1999 / Accepted: 31 January 2000 相似文献
7.
The upper mantle under La Palma,Canary Islands: formation of Si−K−Na-rich melt and its importance as a metasomatic agent 总被引:3,自引:1,他引:3
E. Wulff-Pedersen Else-Ragnhild Neumann B. B. Jensen 《Contributions to Mineralogy and Petrology》1996,125(2-3):113-139
Mantle xenoliths hosted by the Historic Volcan de San Antonio, La Palma, Canary Islands, fall into two main group. Group I consists of spinel harzburgites, rare spinel lherzolites and spinel dunites, whereas group II comprises spinel wehrlites, amphibole wehrlites, and amphibole clinopyroxenites. We here present data on group I xenoliths,
including veined harzburgites and dunites which provide an excellent basis for detailed studies of metasomatic processes.
The spinel harzburgite and lherzolite xenoliths have modal ol−opx−cpx ratios and mineral and whole rock major element chemistry
similar to those found in Lanzarote and Hierro, and are interpreted as highly refractory, old oceanic lithospheric mantle.
Spinel dunites are interpreted as old oceanic peridotite which has been relatively enriched in olivine and clinopyroxene (and
highly incompatible elements) through reactions with basaltic Canarian magmas, with relatively high melt/peridotite ratio.
Group I xenoliths from La Palma differ from the Hierro and Lanzarote ones by a frequent presence of minor amounts of phlogopite (and
amphibole). Metasomatic processes are also reflected in a marked enrichment of strongly incompatible relative to moderately
incompatible trace elements, and in a tendency for Fe−Ti enrichment along grain boundaries in some samples. The veins in the
veined xenoliths show a gradual change in phase assemblage and composition of each phase, from Fe−Ti-rich amphibole+augite+Fe−Ti-oxides+apatite+basaltic
glass, to Ti-poor phlogopite+Cr-diopside±chromite+ Si−Na−K-rich glass+fluid. Complex reaction zones between veins and peridotite
include formation of clinopyroxene±olivine+glass at the expense of orthopyroxene in harzburgite, and clinopyroxene+spinel±amphibole±glass
at the expense of olivine in dunite. The dramatic change in glass composition from the broadest to the narrowest veins includes
increasing SiO2 from 44 to 67 wt%, decreasing TiO2/Al2O3 ratio from >0.24 to about 0.02, and increasing K2O and Na2O from 1.8 to >7.0 wt% and 3.8 to 6.7 wt%, respectively. The petrographic observations supported by petrographic mixing calculations
indicate that the most silicic melts in the veined xenoliths formed as the result of reaction between infiltrating basaltic
melt and peridotite wall-rock. The highly silicic, alkaline melt may represent an important metasomatic agent. Pervasive metasomatism
by highly silicic melts (and possibly fluids unmixed from these) may account for the enriched trace element patterns and frequent
presence of phlogopite in the upper mantle under La Palma.
Received: 15 January 1996 / Accepted 30 May 1996 相似文献
8.
The Urach volcanic field is unique within the Tertiary–Quaternary European volcanic province (EVP) due to more than 350 tuffaceous
diatremes and only sixteen localities with extremely undersaturated olivine melilitite. We report representative Pb-Sr-Nd
isotopic compositions and incompatible trace element data for twenty-two pristine augite, Cr-diopside, hornblende, and phlogopite
megacryst samples from the diatremes, and seven melilitite whole rocks. The Pb isotopic compositions for melilitites and comagmatic
megacrysts have very radiogenic 206Pb/204Pb ratios of 19.4 to 19.9 and plot on the northern hemisphere mantle reference line (NHRL). The data indicate absence of an
old crustal component as reflected in the high 207Pb/204Pb ratios of many basalts from the EVP. This inference is supported by 206Pb/204Pb ratios of ∼17.6 to 18.3 and ɛNd of ∼−7.8 to +1.6 for five phlogopite xenocryst samples reflecting a distinct and variably rejuvenated lower Hercynian basement.
The 87Sr/86Sr ratios of 0.7033 to 0.7035 in the comagmatic megacrysts are low relative to their moderately radiogenic Nd isotopic compositions
(ɛNd +2.2 to +5.1) and consistent with a long-term source evolution with a low Rb/Sr ratio and depletion in light rare-earth elements
(LREE). The melilitite whole-rock data show a similar range in Nd isotopic ratios as determined for the megacrysts but their
Sr isotopic compositions are often much more radiogenic due to surface alteration. The REE patterns and incompatible trace
element ratios of the melilitites (e.g. Nb/Th, Nb/U, Sr/Nd, P/Nd, Ba/Th, Zr/Hf) are similar to those in ocean island basalts
(OIB); negative anomalies for normalized K and Rb concentrations support a concept of melt evolution in the lithospheric mantle.
Highly variable Ce/Pb ratios of 29 to 66 are positively correlated with La/Lu, La/K2O, and Ba/Nd and interpreted to reflect melting in the presence of residual amphibole and phlogopite. The data suggest an
origin of the melilitites from a chemical boundary layer very recently enriched by melts from old OIB sources. We suggest
that the OIB-like mantle domains represent low-temperature melting heterogeneities in an upwelling asthenosphere under western
Europe.
Received: 9 March 1995/Accepted: 24 July 1995 相似文献
9.
N. W. A. Odling D. H. Green B. Harte 《Contributions to Mineralogy and Petrology》1997,129(2-3):209-221
An experimental method of melt inclusion synthesis within olivine crystals has been developed to determine the composition
of the melt present in a partially molten peridotite assemblage. Trace element doped peridotite was equilibrated with 5 wt%
of a C-O-H volatile source at 20 kbar/1175 °C in a piston-cylinder apparatus under buffered oxygen and sulphur fugacity conditions
[log(f
O2) ∼ IW +1 log unit, log (f
S2) ∼ Fe/FeS > +1 log unit]. A single crystal of olivine, which had been cut to a disc shape, was included in the sample capsule.
At run conditions the peridotite charge formed olivine, orthopyroxene, clinopyroxene, Fe-Ni sulphide and a volatile-bearing
melt. The melt phase is preserved as homogeneous glass inclusions up to 50 μm in size, trapped in situ in the olivine disc.
The major element composition of the glass inclusions showed them to be of broadly basaltic character, but with a low Mg/(Mg + ΣFe),
which is associated with precipitation of olivine from the melt inclusion onto the walls of the olivine disc during quenching.
Thus the equilibrium melt composition has been calculated from the glass inclusion composition by addition of olivine component
using the Fe/Mg exchange coefficient of Roeder and Emslie (1970); the desired Mg/(Mg + ΣFe) being determined from the composition
of olivine formed at run conditions in the peridotite section of the charge. The melt composition obtained is close to the
trend for dry melting established by Falloon and Green (1988), and it is evident that although the reduced volatiles in this
case have induced a liquidus depression of some 250 °C, there has been only a small shift in melt composition. Trace element,
carbon and hydrogen contents of thirteen melt inclusions have been determined by secondary ion mass spectrometry (SIMS). The
trace element signature is consistent with ∼29% melting in equilibrium with a lherzolitic assemblage. The equilibrium melt
has a C/H of 0.48 by weight. Carbon solubility in partial melts is thus significant under reducing conditions in the presence
of dissolved “water components” and establishes a major melt fluxing role for carbon in the upper mantle. The ubiquitous presence
of carbon and hydrogen in basaltic magmas underscores the importance of determining both the position of vapour-present solidi
and the composition of melts generated, when developing petrogenetic models.
Received: 1 July 1996 / Accepted: 25 June 1997 相似文献
10.
Summary An experimental study on the phase relationships of three potassium-rich ultramafic rocks from the Damodar Valley, Gondawana
basins, has been performed under upper mantle P–T conditions (1.0–2.5 GPa, 700–1200 °C). The Mohanpur lamproite and Satyanarayanpur
minette, both from the Raniganj basins, have been investigated with the addition of 15 wt% H2O. No water was added in the experiments done on an olivine minette from the Jarangdih coal mine, Bokaro Basin, which originally
contains 15 wt% CO2 and 2.86 wt% H2O.
In all cases, olivine is the liquidus phase followed by phlogopite. The subsolidus assemblage for the three rocks is a phlogopite-bearing
harzburgite, associated with apatite, Mg-ilmenite and carbonates for the Jarangdih rock; apatite, chromian spinel and carbonates
and priderite (only between 1.0 and 1.2 GPa) in the case of the Mohanpur lamproite, and finally apatite, chromian spinel,
rutile, and carbonate in the Satyanarayanpur sample.
Although orthopyroxene is absent in the natural potassium-rich ultramafic rocks, its presence in the run products of the Jarangdih
rock is possibly related to a reaction between olivine and a CO2-bearing fluid phase. The presence of orthopyroxene in the run products of Mohanpur and Satyanarayanpur rocks may be due to
a reaction between K-feldspar, olivine and a vapour phase to produce phlogopite and orthopyroxene.
On the basis of present experimental investigation and isotopic studies made by previous investigators, it has been suggested
that these K-rich rocks have crystallized from melts derived by vein-plus-wall-rock melting of a phlogopite-bearing harzburgite
source rock.
Received December 15, 1999; revised version accepted June 17, 2001 相似文献
11.
Olivine in spinel peridotite xenoliths from the Bismarck Archipelago northeast of Papua New Guinea, which were transported
to the surface by Quaternary basalts, shows spinel inclusions up to 25 μm long and 200 nm wide. These inclusions mainly occur
as inhomogeneously distributed needles and subordinately as octahedral grains in olivine of veined metasomatic peridotites
as well as peridotites without obvious metasomatism. The needles very often occur in swarms with irregular spacing in between
them. Similar spinel inclusions in olivine have only previously been reported from ultramafites of meteoritic origin. Composition
and orientation of the spinel inclusions were determined by transmission electron microscopy (TEM) and analytical electron
microscopy (AEM). Both the needles and the grains display a uniform crystallographic orientation in the host olivine with
[001]O1//[1ˉ10]Spl and (100)Ol// (111)Spl. The needles eare elongated parallel [010] in olivine, which is the same in all olivine grains. As these needles have no
relation to the metasomatic sections in the peridotite, it is concluded that they are primary features of the rock. Although
the composition of the spinel needles is often very similar to the large chromian spinel octahedra in the matrix, the small
octahedral spinel inclusions in olivine are in part Mg-rich aluminous spinel and sometimes almost pure magnetite. The spinel
needles are suggested to have formed by exsolution processes during cooling of Al- and Cr-rich, high-temperature olivine during
the initial formation of the lithospheric mantle at the mid-ocean ridge. The Al-rich spinel octahedra probably formed by the
breakdown of an Al-rich phase such as phlogopite or by metasomatism, whereas the magnetite was generated by oxidizing fluids.
These oxidizing fluids may either have been set free by dehydration of the underlying, subducted plate or by the Quaternary
magmatism responsible for the transport of the xenoliths to the seafloor.
Received: 25 May 2000 / Accepted: 12 July 2000 相似文献
12.
S. Maaløe 《Mineralogy and Petrology》2005,85(3-4):163-204
Summary The investigated mantle section of the Leka ophiolite complex extends 1.4 km from and 1.1 km along the exposed Moho. The foliated
peridotite contains numerous tabular and elongated dunite bodies, orthopyroxenite dikes, websterite veins, and dikes. The
foliation of the peridotite is inclined by about 45° to the Moho. The dunite bodies and the dikes cut the foliation at low
angles. The dunite bodies vary in width from 0.1 to 50 m and in length from 10 m to more than 1 km. Wider dunite bodies are
commonly surrounded by 0 to 1.0 m wide margins of dunitized peridotite. Websterite veins may be present outside these margins.
Apart from sporadic chromite layers the dunite is very homogenous. The dunite bodies are considered to have formed by deposition
of olivine along the walls of dikes originally containing tholeiitic melt. The tholeiitic melt at first heated the peridotitic
sidewalls so that they became partially molten and dunitized. The ascending magma then eroded the sidewalls and removed olivine
as xenocrysts. When the ascent rate decreased, the temperature of the sidewalls decreased, so that olivine (Fo89–92) began to crystallize along the dike walls. There is also evidence for percolative melt migration along foliation planes,
however, the largest proportion of the melts intruded along dikes.
The websterite dikes are mostly 1 to 4 cm wide and 3 to 20 m long and dispersed with mutual distances of 20–50 m. The websterite
veins and dikes probably originated from melts that were generated along the heated sidewalls of the dunite bodies. The 0.02
to 10 m wide orthopyroxenite dikes have exceptionally high MgO contents for their SiO2 contents; about 36 wt.% MgO and 50 wt.% SiO2. They may have formed as segregates from a SiO2-rich magma, although the parent magma does not appear to have been boninitic. The parent magma may instead have formed by
second stage partial melting of depleted lherzolite. 相似文献
13.
L. Melluso S. F. Sethna M. D’Antonio P. Javeri L. Bennio 《Mineralogy and Petrology》2002,74(2-4):323-342
Summary Major element, trace element, Sr- and Nd-isotopes and mineral chemical data are reported for alkaline rocks (lamprophyres,
tephrites, melanephelinites, nephelinites and nepheline syenites) cross-cutting the Deccan Trap lava flows south (Murud-Janjira
area) and north of Mumbai (Bassein). These rocks range from sodic to potassic and have a large span in MgO (12–2 wt%). The
lamprophyres have high content of incompatible elements (e.g., TiO2 > 3.8 wt%, Nb > 130 ppm, Zr > 380 ppm, Ba > 1200 ppm), and relatively high initial (at 65 Ma) 143Nd/144Nd (0.5128) and low 87Sr/86Sr (0.7038–0.7042). They are likely to be small-degree melts (2–3%) of volatile- and incompatible element-enriched mantle
sources, similar to other alkaline rocks in the northern Deccan, though slightly more potassium-rich. The nepheline-rich rocks
have highly porphyritic textures (up to 57% phenocrysts of diopside ± olivine), and anomalously low contents of incompatible
elements (e.g., TiO2 < 1.3 wt%, Nb < 24 ppm, Zr < 100 ppm) indicating that they could not represent liquid compositions. Moreover, their very
low initial 143Nd/144Nd ratios (0.5116–0.5120), at 87Sr/86Sr = 0.7045–0.7049, are unusual in the rocks related to the Deccan Traps and identify a new end-member in this province, that
could be identified as “Lewisian-type” lower crust and/or enriched mantle. The melting episode that generated these alkaline
rocks likely occurred close to the base of the ca. 100 km-thick Indian lithosphere, very shortly after the main eruption of
the Deccan tholeiites.
Received January 14, 2000; revised version accepted September 28, 2001 相似文献
14.
Petrologic and geochemical investigation of carbonates in peridotite xenoliths from northeastern Tanzania 总被引:5,自引:1,他引:4
Cin-Ty Lee Roberta L. Rudnick William F. McDonough Ingo Horn 《Contributions to Mineralogy and Petrology》2000,139(4):470-484
Primary carbonates in peridotite xenoliths from the East African Rift in northeastern Tanzania occur as intergranular patches
with accessory minerals (olivine and spinel), as patches with accessory magmatic minerals (nepheline), and as round monomineralic
inclusions in primary olivine grains. All are characterized by calcitic compositions (Ca/Ca + Mg + Fe from 0.83 to 0.99),
extremely low SiO2 + Al2O3 + Na2O + K2O, low trace element abundance [total rare-earth element (REE) abundance <25 ppm], uniform extinction, and lack of reaction
textures with the host xenolith. Calculated Fe–Mg exchange coefficients between carbonate and primary olivine indicate disequilibrium
in most samples. Combined with the lack of significant reaction textures, this suggests that the carbonates were introduced
shortly before or during eruption of the host magma. A global compilation of electron microprobe analyses of mantle-derived
carbonates (in xenoliths, xenocrysts, and megacrysts) reveals compositional clusters near end member calcite, end member magnesite,
and stoichiometric dolomite. Eutectic liquid compositions are less common, suggesting that many carbonate inclusions reported
worldwide may be crystalline precipitates. Likewise, the calcites in this study are not interpreted to represent quenched
carbonatitic melts, but are interpreted instead to be crystalline cumulates from such melts. These inferences are consistent
with recent experiments, which show that carbonatitic melts cannot become more calcitic than CaCO3∼80 wt%. Low trace element abundance may be a diagnostic feature of cumulate carbonate, and in combination with petrography
and major element composition, serve to distinguish it from quenched carbonated liquid.
Received: 30 July 1999 / Accepted: 5 February 2000 相似文献
15.
大山头南铜镍矿化基性-超基性杂岩体位于北山褶皱带东段,侵位于长城系古硐井群变质岩中。岩相分带明显,主要包括花岗闪长岩-闪长岩相、辉长岩-橄榄苏长辉长岩相和橄榄二辉岩-纯橄岩相。铜镍矿化主要赋存于橄榄二辉岩-纯橄岩相中。岩石化学特征显示K2O、Na2O、TiO2含量较低,Mg#值介于0.74~0.85之间,MgO/FeOT的值介于1.6~3.1之间,属于铁质镁铁-超镁铁岩;AFM图解显示该岩体具拉斑玄武岩的演化趋势;稀土元素总量较低,介于6.37×10-6~37.51×10-6之间;稀土元素标准化配分曲线表现为轻稀土元素稍富集的右倾型,LREE/HREE比值介于3.03~4.11之间,轻重稀土发生了明显的分馏;采用SHRIMP锆石U-Pb方法,获得杂岩体辉长岩中锆石U-Pb年龄为374.3±3 Ma(MSWD=0.92),表明该岩体侵位于中晚泥盆世,与形成大型镍矿床的黑山岩体年龄一致,形成于洋壳俯冲阶段。该年龄的获得不仅对北山乃至中亚造山带地质构造演化具有重要意义,而且也为北山褶皱带东段铜镍找矿提供了新的方向。 相似文献
16.
T. F. D. Nielsen I. P. Solovova I. V. Veksler 《Contributions to Mineralogy and Petrology》1997,126(4):331-344
Perovskite and melilite crystals from melilitolites of the ultramafic alkaline Gardiner complex (East Greenland) contain
crystallised melt inclusions derived from: (1) melilitite; (2) low-alkali carbonatite; (3) natrocarbonatite. The melilitite
inclusion (1) homogenisation temperature of 1060 °C is similar to liquidus temperatures of experimentally investigated natural
melilitites. The compositions are peralkaline, low in MgO (ca.␣5 wt%), Ni and Cr, and they are low-pressure fractionates of
more magnesian larnite-normative ultramafic lamprophyre-type melts of primary mantle origin. Low-alkali carbonatite compositions
(2) homogenise at 1060–1030 °C and are compositionally similar to immiscible calcite carbonatite dykes derived from the melilitolite
magma. Natrocarbonatite inclusions (3) homogenise between 1030 and 900 °C and are compositionally similar to natrocarbonatite
lava from Oldoinyo Lengai. Nephelinitic to phonolitic dykes which are related to the calcite carbonatite dykes, are very Zr-rich
and agpaitic (molecular Na2O + K2O/Al2O3 > 1.2) and resemble nephelinites of Oldoinyo Lengai. The petrographic, geochemical and temporal relationships indicate unmixing
of carbonatite compositions (ca. 10% alkalies) from evolving melilitite melt and continued fractionation of melilitite to
nephelinite. It is suggested that the natrocarbonatite compositions represent degassed supercritical high temperature fluid
formed in a cooling body of strongly larnite-normative nephelinite or evolved melilitite. The Gardiner complex and similar
melilitolite and carbonatite-bearing ultramafic alkaline complexes are believed to represent subvolcanic complexes formed
beneath volcanoes comparable to Oldoinyo Lengai and that the suggested origin of natrocarbonatite may be applied to natrocarbonatites
of Oldoinyo Lengai.
Received: 18 January 1996 / Accepted: 2 September 1996 相似文献
17.
Petrogenetic processes in the ultramafic, alkaline and carbonatitic magmatism in the Kola Alkaline Province: A review 总被引:1,自引:0,他引:1
Hilary Downes Elena Balaganskaya Andrew Beard Ruslan Liferovich Daniel Demaiffe 《Lithos》2005,85(1-4):48-75
Igneous rocks of the Devonian Kola Alkaline Carbonatite Province (KACP) in NW Russia and eastern Finland can be classified into four groups: (a) primitive mantle-derived silica-undersaturated silicate magmas; (b) evolved alkaline and nepheline syenites; (c) cumulate rocks; (d) carbonatites and phoscorites, some of which may also be cumulates. There is no obvious age difference between these various groups, so all of the magma-types were formed at the same time in a relatively restricted area and must therefore be petrogenetically related. Both sodic and potassic varieties of primitive silicate magmas are present. On major element variation diagrams, the cumulate rocks plot as simple mixtures of their constituent minerals (olivine, clinopyroxene, calcite, etc). There are complete compositional trends between carbonatites, phoscorites and silicate cumulates, which suggests that many carbonatites and phoscorites are also cumulates. CaO / Al2O3 ratios for ultramafic and mafic silicate rocks in dykes and pipes range up to 5, indicating a very small degree of melting of a carbonated mantle at depth. Damkjernites appear to be transitional to carbonatites. Trace element modelling indicates that all the mafic silicate magmas are related to small degrees of melting of a metasomatised garnet peridotite source. Similarities of the REE patterns and initial Sr and Nd isotope compositions for ultramafic alkaline silicate rocks and carbonatites indicate that there is a strong relationship between the two magma-types. There is also a strong petrogenetic link between carbonatites, kimberlites and alkaline ultramafic lamprophyres. Fractional crystallisation of olivine, diopside, melilite and nepheline gave rise to the evolved nepheline syenites, and formed the ultramafic cumulates. All magmas in the KACP appear to have originated in a single event, possibly triggered by the arrival of hot material (mantle plume?) beneath the Archaean/Proterozoic lithosphere of the northern Baltic Shield that had been recently metasomatised. Melting of the carbonated garnet peridotite mantle formed a spectrum of magmas including carbonatite, damkjernite, melilitite, melanephelinite and ultramafic lamprophyre. Pockets of phlogopite metasomatised lithospheric mantle also melted to form potassic magmas including kimberlite. Depth of melting, degree of melting and presence of metasomatic phases are probably the major factors controlling the precise composition of the primary melts formed. 相似文献
18.
High PT experiments were performed in the range 2.5–19 GPa and 800–1,500°C using a synthetic peridotite doped with trace elements
and OH-apatite or with Cl-apatite + phlogopite. The aim of the study was (1) to investigate the stability and phase relations
of apatite and its high PT breakdown products, (2) to study the compositional evolution with P and T of phosphate and coexisting
silicate phases and (3) to measure the Cl-OH partitioning between apatite and coexisting calcic amphibole, phlogopite and
K-richterite. Apatite is stable in a garnet-lherzolite assemblage in the range 2.5–8.7 GPa and 800–1,100°C. The high-P breakdown
product of apatite is tuite γ-Ca3 (PO4)2, which is stable in the range 8–15 GPa and 1,100–1,300°C. Coexisting apatite and tuite were observed at 8 GPa/1,050°C and
8.7 GPa/1,000°C. MgO in apatite increases with P from 0.8 wt% at 2.5 GPa to 3.2 wt% at 8.7 GPa. Both apatite and tuite may
contain significant Na, Sr and REE with a correlation indicating 2 Ca2+=Na+ + REE3+. Tuite has always higher Sr and REE and lower Fe and Mg than apatite. Phosphorus in the peridotite phases decreases in the
order Pmelt ≫ Pgrt ≫ PMg2SiO4 > Pcpx > Popx. The phosphate-saturated P2O5 content of garnet increases from 0.07 wt% at 2.5 GPa to 1.5 wt% at 12.8 GPa. Due to the low bulk Na content of the peridotite,
[8]Na[4]P[8]M2+
−1
[4]Si−1 only plays a minor role in controlling the phosphorus content of garnet. Instead, element correlations indicate a major contribution
of [6]M2+[4]P[6]M3+
−1
[4]Si−1. Pyroxenes contain ~200–500 ppm P and olivine has 0.14–0.23 wt% P2O5 in the P range 4–8.7 GPa without correlation with P, T or XMg. At ≥12.7 GPa, all Mg2SiO4 polymorphs have <200 ppm P. Coexisting olivine and wadsleyite show an equal preference for phosphorus. In case of coexisting
wadsleyite and ringwoodite, the latter fractionates phosphorus. Although garnet shows by far the highest phosphorus concentrations
of any peridotite silicate phase, olivine is no less important as phosphorus carrier and could store the entire bulk phosphorus
budget of primitive mantle. In the Cl-apatite + phlogopite-doped peridotite, apatite contains 0.65–1.35 wt% Cl in the PT range
2.5–8.7 GPa/800–1,000°C. Apatite coexists with calcic amphibole at 2.5 GPa, phlogopite at 2.5–5 GPa and K-richterite at 7 GPa,
and all silicates contain between 0.2 and 0.6 wt% Cl. No solid potassic phase is stable between 5 and 8.7 GPa. Cl strongly
increases the solubility of K in hydrous fluids. This may lead to the breakdown of phlogopite and give rise to the local presence
in the mantle of fluids strongly enriched in K, Cl, P and incompatible trace elements. Such fluids may get trapped as micro-inclusions
in diamonds and provide bulk compositions suitable for the formation of unusual phases such as KCl or hypersilicic Cl-rich
mica. 相似文献
19.
Cenozoic lamprophyre dykes occur widely along the Ailao-Shan-Red-River (ASRR) shear zone related to the Indian–Eurasian collision. Two generations of lamprophyres have been found at the Daping gold deposit in the southern part of the ASRR shear zone and have been investigated by using phlogopite 40Ar/39Ar dating and whole-rock major and trace element as well as Sr and Nd isotope geochemical analyses. The 40Ar/39Ar plateau ages of phlogopite from the two generations of lamprophyres bracket the emplacement of auriferous quartz veins in the Daping deposit between 36.8 ± 0.2 Ma and 29.6 ± 0.2 Ma, consistent with the timing of gold mineralization in other parts of the ASRR shear zone. Geochemical data suggest that these lamprophyres most likely originated from a subduction-modified mantle source consisting of phlogopite-bearing spinel lherzolite, which underwent partial melting with contributions from crust materials. In particular, the second generation lamprophyres are characterized by more primitive geochemical features than the first, suggesting that secular source evolution probably resulted from post-collisional slab break-off mantle convection and remelting from ascending asthenosphere after subducted lithosphere break-off. Widespread and episodic occurrences of lamprophyres and other potassic volcanism in the eastern Tibetan Plateau were probably related to the onset of transtensional tectonics along the ASRR shear zone during Oligocene. A genetic model involving transtensional tectonics has been proposed for lamprophyres and gold mineralization in the ASRR shear zone. 相似文献
20.
Summary Ti-bearing phlogopite-biotite is dominant in Ugandan kamafugite-carbonatite effusives and their entrained alkali clinopyroxenite
xenoliths. It occurs as xeno/phenocrysts, microphenocrysts and groundmass minerals and also as a major xenolith mineral. Xenocrystic
micas in kamafugites and carbonatites are aluminous (> 12 wt% Al2O3), typically contain significant levels of Cr (up to 1.1 wt% Cr2O3), and are Ba-poor. Microphenocryst and groundmass micas in feldspathoidal rocks extend to Al-poor compositions, are depleted
in Cr, and are generally enriched in Ba. In general, xenocrystic micas occupy the Al2O3 and TiO2 compositional field of the xenolith mica, and on the basis of Mg#, and high P, T experimental evidence they probably crystallised
at mantle pressures. Mica xenocryst Cr contents range from those in Cr-poor megacryst and MARID phlogopite to higher values
found in primary and metasomatic phlogopites in kimberlite-hosted peridotite xenoliths. Such Cr contents in Ugandan mica xenocrysts
are considered consistent with derivation from carbonate-bearing phlogopite wehrlite and phlogopite-clinopyroxenite mantle.
Olivine melilitite xenocryst micas are distinguished by higher Mg# and Cr content than mica in clinopyroxenite xenoliths and
mica in Katwe-Kikorongo mixed melilitite-carbonatite tephra. Higher Al2O3 distinguishes Fort Portal carbonatite xenocrysts and some contain high Cr. It is suggested that the genesis of Katwe-Kikorongo
olivine melilitite and Fort Portal carbonatite involves a carbonate-bearing phlogopite wehrlite source while the source of
the mixed carbonatite-melilitite rocks may be carbonate-bearing phlogopite clinopyroxenite.
Received January 24, 2000; revised version accepted September 27, 2001 相似文献