The younger (<2000 a) nephelinites at Oldoinyo Lengai are peralkaline, with
alkalinity indices ([Na + K]/Al) ranging from 1.43 in wollastonite nepheli
nite to 2.15 in combeite nephelinite. They have a common set of phenocrysts
(nepheline, clinopyroxene, Ti-andradite, combeite and apatite) but some ph
enocrysts and groundmass phases are different (e.g. wollastonite phenocryst
s and groundmass melilite in wollastonite nephelinite, and phenocrystal sod
alite and groundmass lamprophyllite, 'delhayelite' and aegirine-rich pyroxe
ne in combeite nephelinite). Examination of silicate-carbonate spherules fr
om the 1993 eruption showed that natrocarbonatite unmixed from (formerly) c
arbonate-saturated wollastonite nephelinite, with strong partitioning of al
kalis, Ba, Sr and halogens into the carbonate melt. Compared with wollaston
ite nephelinite, combeite nephelinite is enriched in these elements, and th
e model proposed here is that their enhancement in combeite nephelinite is
due to CO2 loss from the parental melt, precluding the exsolution of natroc
arbonatite; the alkalis, Ba, Sr and halogens perforce remain in the silicat
e melt, enhancing its peralkalinity and leading to precipitation of alkali-
, Ba-, Sr- and halogen-rich phases.