The volcanic rocks erupted in the Rabaul area mostly belong to a calc-
alkaline association here designated the ''main series'' They range fr
om high-alumina basalt (minimum SiO2=48.4%) through medium-K basaltic
andesite, to high-K andesite, dacite and rhyodacite (maximum SiO2=69.3
%). Rare sodic rhyolites (SiO2 approximate to 73-75%) are mineralogica
lly and geochemically distinct from the main-series volcanics. The rhy
olites contain quartz and hornblende, whereas the main-series volcanic
s have a quartz-free, anhydrous mineralogy, even in the most siliceous
rhyodacites. Amphibole and biotite which occur rarely in dacite are d
euteric. Major and trace elements in the main-series rocks show cohere
nt, continuous variation trends against SiO2. Rhyolite analyses consis
tently depart from these trends, particularly for the incompatible ele
ments K, Rb, Ba, Zr, Y and REE. Least-squares mass-balance calculation
s for major elements and Rayleigh fractionation computations for trace
elements show that the main-series magma compositions can be modelled
stepwise as products of a pure crystal fractionation process. Rhyolit
e cannot be derived from main-series magma by crystal fractionation. G
eochemical scatter in the main series may be caused by co-genetic magm
a mixing, as seen in the Malaguna Pyroclastics and Latlat Pyroclastics
units. Hybrid mixing between main-series magma and rhyolite is rare,
but may account for some anomalous medium-K dacites such as the Kulau
Ignimbrite. Derivation of parental high-alumina basalt by partial melt
ing in the mantle wedge is assumed, while rhyolite, which has an inapp
ropriate geochemistry for a partial melt from subducted lithosphere is
thought to be a product of partial melting of high-alumina basalt und
erplating the crust. Volcanic hazard is related to magma composition,
with dacite (SiO2>65%) and rhyolite capable of producing ignimbrite be
ing the most dangerous. Changes in the style of Rabaul volcanicity thr
oughout the life of the caldera are not well documented, but progressi
ve weakening of the faulted substructure may now be allowing more prim
itive basalts and less-fractionated intermediate magmas to reach the s
urface more freely.