1966
DOI: 10.1007/bf02029646
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Some critical differences between orogenic-plutonic and gravity-stratified anorthosites

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1967
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Cited by 17 publications
(4 citation statements)
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“…Anorthosites are widely distributed in terranes of Grenville age throughout the world, but there is still no general agreement on their genesis or even their classification. (See, for example, Middlemost, 1970;Berrange, 1965. ) Since the Roseland type is so restricted in occurrence, it has not been discussed in recent review articles on anorthosite, with only one exception (Isachsen, 1969).…”
Section: Roseland Anorthositementioning
confidence: 99%
“…Anorthosites are widely distributed in terranes of Grenville age throughout the world, but there is still no general agreement on their genesis or even their classification. (See, for example, Middlemost, 1970;Berrange, 1965. ) Since the Roseland type is so restricted in occurrence, it has not been discussed in recent review articles on anorthosite, with only one exception (Isachsen, 1969).…”
Section: Roseland Anorthositementioning
confidence: 99%
“…An attempt to classify known anorthosites was proposed by Ashwal (1993) and modified by Ashwal and Bybee (2017) and Ashwal (2020). This classification includes the works of Buddington (1939Buddington ( , 1975; Berrange (1966); Romey (1968); Middlemost (1970); Moshkin and Dagelaiskaja (1972); Scoates (2000); and Namur et al (2011). Ashwal (2020) subdivided anorthosites into six basic types: (a) Primordial Anorthosites of the Moon, which are monomineralic coarse-grained rocks forming the lunar highlands, with very calcic plagioclase (An 93-98 ) that crystallized not later than 4.3 Ga;…”
Section: Introductionmentioning
confidence: 99%
“…An attempt to classify known anorthosites was proposed by Ashwal (1993) and modified by Ashwal and Bybee (2017) and Ashwal (2020). This classification includes the works of Buddington (1939, 1975); Berrange (1966); Romey (1968); Middlemost (1970); Moshkin and Dagelaiskaja (1972); Scoates (2000); and Namur et al (2011). Ashwal (2020) subdivided anorthosites into six basic types: (a) Primordial Anorthosites of the Moon , which are monomineralic coarse‐grained rocks forming the lunar highlands, with very calcic plagioclase (An 93–98 ) that crystallized not later than 4.3 Ga; (b) Archean Megacrystic Anorthosites which enclose calcic plagioclase (An61‐94, Ashwal & Bybee, 2017); (c) Proterozoic Anorthosites (massif‐type) formed between ~0.5 and ~2.6 Ga as small plutons (1–10 km 2 ) to large composite batholiths (up to 18,000 km 2 ) with their plagioclases crystals intermediate in composition (An30‐70, Ashwal & Bybee, 2017); (d) Anorthosites in layered mafic complexes in which variably thick anorthosites layers overlay mafic layers; (e) Anorthosites of oceanic settings , which by extension include those associated with ophiolites, likely resulting as cumulates from basaltic magmas (Samail‐Oman, Late Cretaceous, Pallister & Hopson, 1981; Marum‐Papua New Guinea, late Eocene, Jacques, Chappell, & Taylor, 1983); and (f) Anorthosites inclusions in other igneous rocks , originating as cognate plagioclase cumulates from the same magma as their host (cognate inclusions), as gradational differentiation products in the suite of their cognate igneous rocks, as an independent magma batch intruding the igneous host or as fragments of older anorthosites (xenolithic inclusions).…”
Section: Introductionmentioning
confidence: 99%
“…Massif-type anorthosites have certain characteristics (1): 1) They form plutons of batholithic proportions that are largely unlayered but appear to be concordant to country rock in Precambrian terranes.…”
mentioning
confidence: 99%