Gy. Peng et al., INCLUSIONS OF PHLOGOPITE AND PHLOGOPITE HYDRATES IN CHROMITE FROM THEHONGGULELENG OPHIOLITE IN XINJIANG, NORTHWEST CHINA, The American mineralogist, 80(11-12), 1995, pp. 1307-1316
Two types of chromite deposits occur in the Hongguleleng ophiolite in
Xinjiang, northwest China. One is located in the mantle sequence, the
other occurs in the transition zone between the mantle sequence and la
yered cumulates. Abundant primary silicate inclusions such as phlogopi
te, pargasite, clinopyroxene, orthopyroxene, and olivine are found in
the segregated chromite, but silicate inclusions occur only rarely in
accessory chromite of the ultramafic rocks from the transition zone an
d cumulates. These silicate phases are considered to have been entrapp
ed as discrete and rare composite inclusions during magmatic precipita
tion of chromite rather than formed by postmagmatic entrapment. Phlogo
pite is the most abundant mineral found as inclusions in chromite in t
he Hongguleleng ophiolite. There are two types of substitutions for K
in the phlogopite inclusions: (1) Na substitutes for K, and phlogopite
shows a continuous range from almost pure sodium phlogopite to phlogo
pite; (2) Ca partially substitutes for K, resulting in the formation o
f Ca-bearing phlogopite. It is proposed that the alkalic aqueous liqui
d (melt) responsible for the formation of the phlogopite inclusions wa
s derived from the mixture of the K-rich aqueous liquid related to the
subduction of the oceanic slab and the Na-rich aqueous liquid from th
e primary magma of the ophiolite. Two types of phlogopite hydrates, hy
drate I and possibly a new hydrate (hydrate H), occur as inclusions in
the chromite and result from later hydrothermal processes. The fractu
res from brittle deformation provided passage for meteoric water to en
ter and react with the phlogopite inclusions. Compared with those in t
he transition zone, the inclusions of phlogopite and phlogopite hydrat
es in the mantle sequence are characterized by (1) smaller grain size
and greater abundance, (2) undulatory extinction, (3) higher Si, Cr, N
i, and Ca, and (4) lower Ti and Al. These differences are possibly due
to (I) P, T, and composition of chromite-precipitating magma, (2) sub
solidus reequilibration with the host chromite, and (3) postmagmatic d
eformation and hydrothermal processes.