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Geochemical differences between the Cadomian granites of Mancellia and the St. Malo migmatites, Armorican Massif, France

G. M. Power
Geochemical differences between the Cadomian granites of Mancellia and the St. Malo migmatites, Armorican Massif, France
Journal of the Geological Society of London (May 1993) 150, Part 3: 465-468

Abstract

Data sets used to suggest geochemical similarity between the St Malo migmatites and Mancellian granites are reinterpreted. The samples have complex distributions with outliers. Three non-parametric tests show significant statistical differences between the samples in Al (sub 2) O (sub 3) , CaO, K (sub 2) O, Cr, Ni, Sr, Y and Zr. If outliers are culled from the samples the differences become more extreme; the differences are also apparent on both principal component and multidimensional scaling plots. Geotectonic models based on a similar petrogenesis for the two rock units must be able to account for these differences.


ISSN: 0016-7649
EISSN: 2041-479X
Coden: JGSLAS
Serial Title: Journal of the Geological Society of London
Serial Volume: 150, Part 3
Title: Geochemical differences between the Cadomian granites of Mancellia and the St. Malo migmatites, Armorican Massif, France
Author(s): Power, G. M.
Affiliation: University of Portsmouth, Portsmouth, United Kingdom
Pages: 465-468
Published: 199305
Text Language: English
Publisher: Geological Society of London, London, United Kingdom
References: 6
Accession Number: 1993-016955
Categories: Igneous and metamorphic petrologyGeochemistry of rocks, soils, and sediments
Document Type: Serial
Bibliographic Level: Analytic
Illustration Description: illus. incl. 2 tables
N46°30'00" - N49°45'00", W04°49'60" - E00°00'00"
Country of Publication: United Kingdom
Secondary Affiliation: GeoRef, Copyright 2018, American Geosciences Institute. Reference includes data from Mineralogical Abstracts, United Kingdom, Twickenham, United Kingdom
Update Code: 1993

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