Detailed petrological work was carried, out on serpentinized peridotit
e dredged and sampled by submersible fi om the southern part of the Ma
riana Trench to reveal the nature of the mantle wedge in the southern
Mariana forearc. The southern part of the Mariana Trench is important
in that we should expect to find a transect of a typical island are st
ructure; that is, from east to west, the Mariana forearc, the Mariana
are proper, the Mariana Trough (active back-are spreading center), and
the West Mariana Ridge (remnant arc). The most striking feature of pe
ridotites from the southern part of the trench is that primary hornble
nde is a major constituent mineral in many specimens. Thus, the perido
tite samples are divided into anhydrous (A-type), hydrous (H-type) and
intermediate (I-type) groups. Petrological data suggest that each typ
e of peridotite is a residue of extensive partial melting in the upper
mantle. It is argued here that the I- and H-type peridotites were mod
ified from 'proto-A-type peridotite' by fluid infiltration. The fluid
was enriched in Al, Ti, Fe, and alkalis, and may have caused changes i
n mineral and bulk chemical compositions of the peridotites. A-type pe
ridotite derives from the 'proto-A-type peridotite' directly, without
any fluid contamination. After the formation of the 'proto-A-, I-, and
I-I-type peridotites', lower-temperature fluids, probably of seawater
origin, produced retrograde metamorphism and alteration including ser
pentinization. The mantle wedge in the southern Mariana forearc was he
terogeneous in fluid supply.