Plagioclase





















































































Plagioclase

Plagioklas1.jpg
A photomicrograph of a plagioclase crystal under cross polarized light. The plagioclase crystal shows a distinct banding effect called polysynthetic twinning.

General
Category
Feldspar mineral group, tectosilicate

Formula
.mw-parser-output .nobold{font-weight:normal}
(repeating unit)
NaAlSi3O8 – CaAl2Si2O8
Crystal system Triclinic
Crystal class Pinacoidal (1)
(same H-M symbol)
Space group
C1
Identification
Color White, gray, bluish white, reddish white, greenish white
Crystal habit Massive to granular
Twinning Common, albite law striations on {001}[1]
Cleavage Good on {001} and {010}
Tenacity Brittle

Mohs scale
hardness
6 - 6.5
Luster Vitreous
Streak White
Diaphaneity Transparent to translucent
Specific gravity 2.62 (albite) to 2.76 (anorthite)[1]
Optical properties Biaxial (+) albite, biaxial (-) anorthite[1]
Refractive index Albite: nα 1.527, nβ 1.532 nγ 1.538
Anorthite: nα 1.577 nβ 1.585 nγ 1.590[1]
Solubility Albite insoluble in HCl, anorthite decomposed by HCl [1]
References [2]



Plagioclase displaying cleavage. (unknown scale)




In volcanic rocks, fine-grained plagioclase can display a 'microlitic' texture of many small crystals.


Plagioclase is a series of tectosilicate (framework silicate) minerals within the feldspar group. Rather than referring to a particular mineral with a specific chemical composition, plagioclase is a continuous solid solution series, more properly known as the plagioclase feldspar series (from the Ancient Greek for "oblique fracture", in reference to its two cleavage angles). This was first shown by the German mineralogist Johann Friedrich Christian Hessel (1796–1872) in 1826. The series ranges from albite to anorthite endmembers (with respective compositions NaAlSi3O8 to CaAl2Si2O8), where sodium and calcium atoms can substitute for each other in the mineral's crystal lattice structure. Plagioclase in hand samples is often identified by its polysynthetic crystal twinning or 'record-groove' effect.


Plagioclase is a major constituent mineral in the Earth's crust, and is consequently an important diagnostic tool in petrology for identifying the composition, origin and evolution of igneous rocks. Plagioclase is also a major constituent of rock in the highlands of the Earth's moon. Analysis of thermal emission spectra from the surface of Mars suggests that plagioclase is the most abundant mineral in the crust of Mars.[3]




Contents






  • 1 Plagioclase series members


    • 1.1 Endmembers


    • 1.2 Intermediate members




  • 2 See also


  • 3 References


  • 4 External links





Plagioclase series members


The composition of a plagioclase feldspar is typically denoted by its overall fraction of anorthite (%An) or albite (%Ab), and readily determined by measuring the plagioclase crystal's refractive index in crushed grain mounts, or its extinction angle in thin section under a polarizing microscope. The extinction angle is an optical characteristic and varies with the albite fraction (%Ab). There are several named plagioclase feldspars that fall between albite and anorthite in the series. The following table shows their compositions in terms of constituent anorthite and albite percentages.
















































Plagioclase minerals and their compositions
Name % CaAl2Si2O8

% NaAlSi3O8
Image
Anorthite 90–100 10–0
Anorthit Miyake,Japan.JPG
Bytownite 70–90 30–10
Feldspar - Bytownite Sodium calcium aluminum silicate Crystal Bay Minnesota 2689.jpg
Labradorite 50–70 50–30
Labradorite.jpg
Andesine 30–50 70–50
01722 Andesine.jpg
Oligoclase 10–30 90–70
Oligoclase-Sunstone from India2.jpg
Albite 0–10 100–90
Albite2.jpg


Endmembers




  • Anorthite was named by Gustav Rose in 1823 from the Ancient Greek meaning oblique, referring to its triclinic crystallization. Anorthite is a comparatively rare mineral but occurs in the basic plutonic rocks of some orogenic calc-alkaline suites.


  • Albite is named from the Latin albus, in reference to its unusually pure white color. It is a relatively common and important rock-making mineral associated with the more acid rock types and in pegmatite dikes, often with rarer minerals like tourmaline and beryl.



Intermediate members


The intermediate members of the plagioclase group are very similar to each other and normally cannot be distinguished except by their optical properties. The specific gravity in each member (albite 2.62) increases 0.02 per 10% increase in anorthite (2.75).



  • Bytownite, named after the former name for Ottawa, Ontario, Canada (Bytown), is a rare mineral occasionally found in more basic rocks.



Labradorite displaying typical iridescent effect termed labradorescence. (unknown scale)




  • Labradorite is the characteristic feldspar of the more basic rock types such as diorite, gabbro, andesite, or basalt and is usually associated with one of the pyroxenes or amphiboles. Labradorite frequently shows an iridescent display of colors due to light refracting within the lamellae of the crystal. It is named after Labrador, where it is a constituent of the intrusive igneous rock anorthosite which is composed almost entirely of plagioclase. A variety of labradorite known as spectrolite is found in Finland.


  • Andesine is a characteristic mineral of rocks such as diorite which contain a moderate amount of silica and related volcanics such as andesite.


  • Oligoclase is common in granite, syenite, diorite, and gneiss. It is a frequent associate of orthoclase. The name oligoclase is derived from the Greek for little and fracture, in reference to the fact that its cleavage angle differs significantly from 90°. Sunstone is mainly oligoclase (sometimes albite) with flakes of hematite.



See also




  • Hypersolvus

  • List of minerals

  • Subsolvus



References





  1. ^ abcde Klein, Cornelis and Cornelius S. Hurbut, Jr.; Manual of Mineralogy, Wiley, 20th ed., 1980, pp.454-456 .mw-parser-output cite.citation{font-style:inherit}.mw-parser-output q{quotes:"""""""'""'"}.mw-parser-output code.cs1-code{color:inherit;background:inherit;border:inherit;padding:inherit}.mw-parser-output .cs1-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-limited a,.mw-parser-output .cs1-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/Lock-gray-alt-2.svg/9px-Lock-gray-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/a/aa/Lock-red-alt-2.svg/9px-Lock-red-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration{color:#555}.mw-parser-output .cs1-subscription span,.mw-parser-output .cs1-registration span{border-bottom:1px dotted;cursor:help}.mw-parser-output .cs1-hidden-error{display:none;font-size:100%}.mw-parser-output .cs1-visible-error{font-size:100%}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration,.mw-parser-output .cs1-format{font-size:95%}.mw-parser-output .cs1-kern-left,.mw-parser-output .cs1-kern-wl-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right,.mw-parser-output .cs1-kern-wl-right{padding-right:0.2em}
    ISBN 0-471-80580-7



  2. ^ Webmineral data


  3. ^ Milam, K. A.; et al. (2010). "Distribution and variation of plagioclase compositions on Mars". Journal of Geophysical Research: Planets. 115 (E9). doi:10.1029/2009JE003495.




External links


















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