Apatite chemical composition, determined by electron microprobe and laser-ablation inductively coupled plasma mass spectrometry, as a probe into granite petrogenesis
Lk. Sha et Bw. Chappell, Apatite chemical composition, determined by electron microprobe and laser-ablation inductively coupled plasma mass spectrometry, as a probe into granite petrogenesis, GEOCH COS A, 63(22), 1999, pp. 3861-3881
Major, minor, and trace element abundances in apatites from various I- and
S-type (igneous and sedimentary) granites of the Lachlan Fold Belt have bee
n determined using electron microprobe and laser ablation inductively coupl
ed plasma mass spectrometer. The results show that apatite can accommodate
many minor and trace elements, whose concentrations and ratios are relative
ly sensitive to factors controlling many of the fundamental differences bet
ween I- and S-type granites. Apatites from S-type granites generally have h
igher F but lower Cl contents than those from I-type granites, which is asc
ribed mainly to the loss of Cl during the weathering processes forming the
source rocks of S-type granites, although fractional crystallisation can ca
use significant enrichment in F as well. High Mn and Fe contents in apatite
s from S-type granites, and high S and As abundances in apatites from mafic
I-type granites, result from different oxygen fugacities and degrees of Al
saturation (or aluminosity) between metaluminous mafic I-type magmas and p
eraluminous S-type and felsic I-type magmas. There are systematic and disti
nctive differences in absolute rare-earth element (REE) abundances, REE dis
tribution patterns, and element ratios (e.g., La/Y, Sm/Nd, etc.) between ap
atites from different types of granite. The strong Eu depletion that charac
terises apatites from S- and felsic I-type granites is interpreted here to
be a result of the uniqueness of crystal chemistry of apatite and high EU2/EU3+ ratios in S-type and felsic I-type magmas, which are more reduced and
peraluminous than mafic I-type magmas. Strong REE (La to Eu) and Tn enrich
ment in apatites from mafic I-type granites and marked Nd depletion in apat
ites from most S-type and felsic I-type granites are caused by the precipit
ation and fractionation of monazite in the parental magmas of the latter ro
cks. Substitution mechanisms are responsible for high Na in apatites from S
-type and felsic I-type granites, and for high Si in apatites from mafic I-
type granites, and may also have important effects on REE partitioning betw
een apatite and melt. Thus, apatite chemistry can be used as an excellent i
ndicator of granite petrogenesis. The results have important implications f
or identifying different types of granite and are potentially significant f
or determining the provenance of sedimentary rocks. Copyright (C) 1999 Else
vier Science Ltd.