The geochemistry of mineral inclusions in diamond is an important sour
ce of information about the composition of the continental lithospheri
c mantle at depths exceeding 120-150 km. At these depths, two main typ
es of geochemical environment support diamond formation; they are ultr
amafic (or peridotitic) (U-type) and eclogitic (E-type) environments a
s shown by minerals that occur as inclusions in diamonds. In primary d
iamond-bearing kimberlite or lamproite rock the ratio of diamonds from
these two geochemical environments varies widely between localities.
The U-type environment dominates for the majority of diamond occurrenc
es worldwide, whereas the E-type environment dominates for a very limi
ted number of localities in South Africa, North America, and Australia
. The present study shows that an uncommonly high percentage (99.4%) o
f E-type diamonds with extremely variable inclusion assemblages is fou
nd in kimberlites in the northwestern part of the Guyana shield at Gua
niamo, Venezuela. These variations range from previously unknown silic
a-undersaturated corundum eclogite to abundant silica-rich coesite ecl
ogite assemblages representing 22% of all E-type diamonds, some of whi
ch contain syngenetic ihmenite and magnetite, The compositional variat
ions of garnet and omphacite inclusions are extremely broad. The wide
variability of the eclogitic source in which diamonds formed beneath t
he Guyana shield indicates a broadly basaltic chemistry in this enviro
nment, which may represent ancient subducted oceanic crust. Such speci
fic features have not been reported for any other diamond occurrence a
nd reflect an unusual composition of the deep lithospheric mantle in t
his area.