「OLIVINE」の共起表現(1語右で並び替え) - Weblio英語共起表現検索


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「OLIVINE」の共起表現一覧(1語右で並び替え)

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rite sulfide assemblages within serpentinized olivine adcumulate dunite, formed from the metamorphi
Calcium-rich pyroxenes and olivine, along with nickel-iron metal, have been dete
ille is a Q-type asteroid, composed mostly of olivine and pyroxene.
mineral, surrounded by a continuous shell of olivine and containing feldspathic glass between the
this magma ocean proceeded, minerals such as olivine and pyroxene would have precipitated and sunk
ore zones containing retrogressed metamorphic olivine and distinctive bladed anthophyllite.
vers the values for silicate minerals such as olivine and pyroxene, which make up many of the rocky
are common in the minerals quartz, feldspar, olivine and pyroxene.
e composed primarily of the silicate minerals olivine and pyroxene, surrounded by feldspathic mater
um-rich pyroxene), forsterite (magnesium-rich olivine) and feldspar.
to the presence of strong absorption lines in olivine and pyroxene with little or no metals.
se transitions in the common mantle minerals, olivine and pyroxene, would occur within the pressure
t asteroids with a strong, broad 1 micrometre olivine and pyroxene feature, and a spectral slope th
cite), plagioclase, and augite, together with olivine and lesser iron-titanium oxides such as ilmen
isting mostly of the mineral augite with some olivine, anorthite and troilite.
Quartz and olivine are absent.
Small crystals of feldspar or olivine are sometimes visible in them with the unaide
Clinopyroxene (augite) and olivine are common as phenocrysts and in the matrix.
ic iron, mostly present as FeO in the mineral olivine as well as FeS (troilite).
Experiments have documented that olivine at high pressures (e.g., 12 GPa, the pressure
Minerals in basaltic andesite include olivine, augite and plagioclase.
The commonest crystals are olivine, augite and feldspar, with swarms of minute d
operly a potassic trachyandesite, composed of olivine, augite and plagioclase phenocrysts in a grou
The hill is composed of aphanitic alkaline olivine basalt, with phenocrysts of olivine.
Victorian bluestone is a basalt or olivine basalt, and is quarried by a number of compan
hed by the waves, and identified as vesicular olivine basalt.
Olivine can be present along with apatite, and locall
main mass contains several regions of massive olivine clusters up to 11 cm in diameter with thin me
tic structures are symplectites formed around olivine containing pyroxenes, amphiboles, spinel or g
Multiple melt inclusions in an olivine crystal.
1: olivine crystallizes; 2: olivine and pyroxene crystal
a type of stony-iron meteorite with beautiful olivine crystals.
el, corundum, stishovite, augite, forsteritic olivine, diopsidic clinopyroxene and several Al-Cu-Fe
In contrast, Mg-rich olivine does not occur stably with silica minerals, a
ic nodules in kimberlites in association with olivine, enstatite, chrome diopside, chromian pyrope,
A feeder dike of olivine gabbro is exposed "below" the now tilted sequ
Magmatic olivine generally has up to ~4000ppm Ni and up to 250
rapid cooling are dendritic and hopper-shaped olivine grains, and chondrules that are composed enti
intimate mixture of water ice, methanol ice, olivine grains, and complex organic compounds (tholin
Olivine has also been found in the SNC (shergottite,
mantle at shallower depths, the properties of olivine have a dominant influence upon the rheology o
ls typical of lamproites include: forsteritic olivine; high iron leucite; titanium-rich aluminium-p
sociation includes titanian augite, rhoenite, olivine, ilmenite, spinel, plagioclase and titanian p
arises from pyroxene or hornblende enveloping olivine in the same manner.
Magnesite is formed via carbonation of olivine in the presence of water and carbon dioxide,
1959 demonstrated that the iron end-member of olivine indeed transformed to the denser spinel struc
Fe-rich olivine is relatively much less common, but it occurs
Mg-rich olivine is stable to pressures equivalent to a depth
absent in a feldspathoid-bearing latite, and olivine is absent in a quartz-bearing latite.
t in the presence of water at high pressures, olivine is favored.
When metamorphic olivine is produced, the propensity for this mineral
Olivine lamproite pyroclastic rocks and dikes are som
ng metamorphism, sulfur and nickel within the olivine lattice are reconstituted into metamorphic su
The RCHAMS 'Canmore' site lists this unhewn olivine monolith as a 'possible' standing stone.
semblage and coarse jackstraw textured bladed olivine, now retrogressed to black serpentinite.
ssociated with richterite and serpentinitized olivine of mafic xenoliths in the lamproite host rock
Fukang pallasite contains large, gem quality olivine, or peridot, in a nickel-iron matrix.
Biotite, hornblende, pyroxene and scarce olivine or quartz are common accessory minerals.
e variables that determine whether forsterite olivine or enstatite pyroxene is precipitated, but th
kaersutite, magnetite, muscovite, nepheline, olivine, perthite, pyrite, pyroxene and pyrrhotite.
itic basanite which has abundant pyroxene and olivine phenocrysts.
ge pale green pyroxene and minor yellow-brown olivine phenocrysts.".
3. Common rock-forming mafic minerals include olivine, pyroxene, amphibole, and biotite.
variations in the abundance of crystallizing olivine, pyroxene, plagioclase and magnetite.
in many minerals, including; quartz, calcite, olivine, pyroxenes, micas, feldspars, halite and garn
olivine) rather than as free metal, as it is found in
pressures found at depth within the Earth the olivine structure is no longer stable.
ith pilite, a rarely used name for an altered olivine that has partially pseudomorphically replaced
volcanic rock characterized by phenocrysts of olivine, titanium-rich augite, plagioclase feldspar a
pressure increases, the O2− ions compress so olivine transforms to the spinel structure, which at
Below depths of about 410 km (250 mi) olivine undergoes a phase transition to the sorosilic
Olivine was found in the Nili Fossae formation.
Olivine was also discovered in many other small outcr
Olivine weathering to iddingsite within a mantle xeno
Olivine weathering to iddingsite within a mantle xeno
ng compositions: A larger region dominated by olivine, which is pyroxene-poor and metal-rich, and a
                                                                                                   


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