Anorthite

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Anorthite
Anorthite-rare08-38b.jpg
Anorthite crystals in a basalt vug from Vesuvius (size:6.9 × 4.1 × 3.8 cm)
General
Category Tectosilicate minerals, feldspar group, plagioclase series
Formula CaAl2Si2O8
IMA symbol An [1]
Strunz classification 9.FA.35
Crystal system Triclinic
Crystal class Pinacoidal (1)
(same H-M symbol)
Space group P1
Unit cell a = 8.1768, b = 12.8768
c = 14.169 [Å]; α = 93.17°
β = 115.85°, γ = 92.22°; Z = 8
Identification
Formula mass 278.203 g·mol−1
ColorWhite, grayish, reddish
Crystal habit Anhedral to subhedral granular
Twinning Common
Cleavage Perfect [001] good [010] poor [110]
Fracture Uneven to conchoidal
Tenacity Brittle
Mohs scale hardness6
Luster Vitreous
Streak White
Diaphaneity Transparent to translucent
Specific gravity 2.72–2.75
Optical propertiesBiaxial (−)
Refractive index nα = 1.573–1.577 nβ = 1.580–1.585 nγ = 1.585–1.590
Birefringence δ = 0.012–0.013
2V angle 78° to 83°
Melting point 1550 ± 2°C [2]
References [3] [2] [4] [5]

Anorthite (an = not, ortho = straight) is the calcium endmember of the plagioclase feldspar mineral series. The chemical formula of pure anorthite is CaAl 2 Si2O8. Anorthite is found in igneous rocks.

Contents

Mineralogy

Anorthite crystals (white) in lava from Miyake Island, Japan (size: 2.4 x 1.7 x 1.7 cm) Anorthite-221029.jpg
Anorthite crystals (white) in lava from Miyake Island, Japan (size: 2.4 × 1.7 × 1.7 cm)

Anorthite is the calcium-rich endmember of the plagioclase solid solution series, the other endmember being albite (NaAlSi3O8). Pure anorthite, containing no sodium, is rare on Earth. [6] Anorthite also refers, however, to plagioclase compositions with more than 90 molecular percent of the anorthite endmember (and up to 10 molecular percent of the albite endmember). The composition of plagioclases is often expressed as a molar percentage of An%, or (for a specific quantity) Ann, where n = Ca/(Ca + Na) × 100. [7] This equation predominantly works in a terrestrial context; exotic locales and in particular Lunar rocks may need to account for other cations, such as Fe2+, to explain differences between optically and structurally derived An% data observed in Lunar anorthites. [8]

At standard pressure, pure anorthite (An100) melts at 1550 ± 2 °C (2822 °F). [2]

Occurrence

Anorthite is a compositional variety of plagioclase. It occurs in mafic igneous rock. It also occurs in metamorphic rocks of granulite facies, in metamorphosed carbonate rocks, and corundum deposits. [3] Its type localities are Monte Somma and Valle di Fassa, Italy. It was first described in 1823. [5] It is more rare in surficial rocks than it normally would be due to its high weathering potential in the Goldich dissolution series.

It also makes up much of the lunar highlands; the Genesis Rock, collected during the 1971 Apollo 15 mission, is made of anorthosite, a rock composed largely of anorthite. Anorthite was discovered in samples from comet Wild 2, and the mineral is an important constituent of Ca-Al-rich inclusions in rare varieties of chondritic meteorites.

See also

References

  1. Warr, L.N. (2021). "IMA–CNMNC approved mineral symbols". Mineralogical Magazine. 85 (3): 291–320. Bibcode:2021MinM...85..291W. doi: 10.1180/mgm.2021.43 . S2CID   235729616.
  2. 1 2 3 Rankin, George; Wright, Fred (1915). "The ternary system CaO-Al2O3-SiO2, with optical study by F.E. Wright". American Journal of Science (229): 1–79.
  3. 1 2 Handbook of Mineralogy
  4. Mindat
  5. 1 2 Webmineral
  6. Ndimofor, A.N. (2018). The Fundamentals of Crystallography & Mineralogy. Denver: Spears Media Press. p. 68. ISBN   978-1-942876-24-3.
  7. Bennett, Emma N.; Lissenberg, C. Johan; Cashman, Katharine V. (21 May 2019). "The significance of plagioclase textures in mid-ocean ridge basalt (Gakkel Ridge, Arctic Ocean)". Contributions to Mineralogy and Petrology. 174 (6) 49. doi: 10.1007/s00410-019-1587-1 . PMC   6530810 .
  8. Wenk, H. -R.; Wilde, W. R. (1 August 1973). "Chemical anomalies of Lunar plagioclase, described by substitution vectors and their relation to optical and structural properties". Contributions to Mineralogy and Petrology. 41 (2): 89–104. doi:10.1007/BF00375035.