forsterite sentence in Hindi
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- Green sand for aluminum typically uses olivine sand ( a mixture of the minerals forsterite and fayalite, which is made by crushing dunite rock ).
- For instance in mafic and ultramafic melts, the MgO and SiO 2 contents determine whether forsterite olivine is precipitated or whether enstatite pyroxene is precipitated.
- Component chemicals found at Lascar include : anorthite, augite bordering on diopside, bronzite, fassaite, forsterite, hypersthene, pigeonite, and more.
- "' Wadsleyite "'is a high-pressure phase of Mg 2 SiO 4 and is polymorphous with the olivine phase forsterite.
- It is commonly occurs in rocks that contain calcite, quartz, tremolite, witherite, phlogopite, diopside, minor amounts of forsterite and taramellite.
- Lazurite is a product of contact metamorphism of limestone and typically is associated with calcite, pyrite, diopside, humite, forsterite, hauyne and muscovite.
- In the olivine structure, the main olivine series of ( Mg, Fe ) 2 SiO 4 consist of magnesium-rich forsterite and iron-rich fayalite.
- Compositions of olivine are commonly expressed as molar percentages of forsterite ( Fo ) and fayalite ( Fa ) ( e . g ., Fo 70 Fa 30 ).
- "Spitzer " observations, announced in May 2011, indicate that tiny forsterite crystals might be falling down like rain on to the protostar HOPS-68.
- MgO and SiO 2 concentrations in melts are among the variables that determine whether forsterite olivine or enstatite pyroxene is precipitated, but the water content and pressure are also important.
- Other silicates were detected as well, such as the Magnesium-rich end-member of olivine called forsterite, pigeonite, plagioclase, augite, clinopyroxene, and orthopyroxene.
- Fayalite forms solid solution series with the magnesium olivine endmember forsterite ( Mg 2 SiO 4 ) and also with the manganese rich olivine endmember tephroite ( Mn 2 SiO 4 ).
- Other examples of series include the olivine series of magnesium-rich forsterite and iron-rich fayalite, and the wolframite series of manganese-rich h�bnerite and iron-rich ferberite.
- This led the team of astronomers to speculate that the bipolar outflow from the young star may be transporting the forsterite crystals from near the star's surface to the chilly outer cloud.
- Some chondrules contain very little iron oxide ( FeO ), resulting in olivine and pyroxene that are close to forsterite ( Mg 2 SiO 4 ) and enstatite ( MgSiO 3 ) in composition.
- One of the important factors that can increase the portion of forsterite in the olivine solid solution is the ratio of iron ( II ) ions to iron ( III ) ions in the magma.
- Minerals associated with humite include grossular, wollastonite, forsterite, monticellite, cuspidine, fluoborite, ludwigite, dolomite, calcite, talc, biotite, spinel, vesuvianite, sanidine, meionite and nepheline.
- Another line of evidence is that the MgO content of olivines formed in komatiites is toward the nearly pure MgO forsterite composition, which can only be achieved in bulk by crystallisation of olivine from a highly magnesian melt.
- It is formed by a phase transformation from forsterite ( ?-Mg 2 SiO 4 ) under increasing pressure and eventually transforms into spinel-structured ringwoodite ( ?-Mg 2 SiO 4 ) as pressure increases further.
- The discovery of the forsterite crystals in the outer collapsing cloud of the protostar is surprising, because the crystals form at lava-like high temperatures, yet they are found in the molecular cloud where the temperatures are about.
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