High-resolution seismic reflection data are used to identify structura
l features in Naples Bay near Vesuvius Volcano. Several buried seismic
units with reflection-free interiors are probably volcanic deposits e
rupted during and since the formation of the breached crater of Monte
Somma Volcano, which preceded the growth of Vesuvius, The presumed und
ersea volcanic deposits are limited in extent; thus, stratigraphic rel
ationships cannot be established among them. Other features revealed b
y our data include (a) the warping of lowstand marine deposits by unde
rsea cryptodomes located approximately 10 km from the summit of Vesuvi
us, (b) a succession of normal step faults that record seaward collaps
e of the volcano, and (c) a small undersea slump in the uppermost mari
ne deposits of Naples Bay, which may be the result of nuee ardentes th
at entered the sea during a major eruption of Vesuvius in 1631. Detect
ion of these undersea features illustrates some capabilities of making
detailed seismic reflection profiles across undersea volcanoes.