A total dissolution technique has been developed and used to identify
and quantify the incompatible element contents of fluids trapped in in
clusions in minerals from peridotite xenoliths using ''fluids'' in the
generic sense (i.e., C-O-H fluids and melts). Fluids from lherzolites
, a wehrlite, and a harzburgite host important quantities of alkalis,
Ba, U, Th, Pb, and contain Sr and Nd as well. Quantitative application
of the technique shows that the CO2-rich fluid in a Iherzolite from N
univak Island, AK, USA and the CO2-poor melt in a lherzolite from San
Carlos, Arizona, USA, have incompatible element compositions similar t
o each other differing only in their K and Ba contents. With the excep
tion of their K contents, the trace element compositions of these flui
ds resemble those of carbonatites and kimberlites. Major and radiogeni
c isotope data from the lherzolite and a phlogopite harzburgite from N
univak suggest that the fluid trapped in the lherzolite is associated
with a carbonatite melt, linked to hydrous metasomatism in the region.
A more dilute CO2-bearing melt was identified in a wehrlite from Salt
Lake Crater, HI, USA resembling Hawaiian alkali basalt in its incompa
tible element composition. The strontium, neodymium, and lead isotope
composition of the fluids resemble those of the surrounding mantle and
do not reflect their parent/daughter ratios. Lead isotope data for fl
uid-bearing clinopyroxene in the wehrlite suggest fluid influx was rec
ent. Conventional and laser oxygen isotope analyses show that most flu
id inclusion-bearing xenoliths examined are out of oxygen isotope equi
librium. Diffusion-based arguments suggest that fluid infiltration in
these xenoliths occurred over the last 1-10 My. The fluids identified
in this study will dominate the incompatible element budget of typical
mantle peridotite if present in greater than sub-weight percent quant
ities.