Granites in both crystalline terranes and continental magmatic arcs te
nd to be circular to elliptical in map view and vary in width from abo
ut 3 to 100 km. Available gravity and structural data suggests that ma
ny of these plutons are tabular in shape with an average thickness of
about 3 km. Ductile structures observed around mesozonal granites indi
cate that space is created by a combination of lateral and vertical di
splacements of wall rocks, whereas contact relationships of epizonal p
lutons imply that only vertical displacements are involved during empl
acement. In both settings magma arrives at the emplacement site via on
e or more vertical feeder zones and flows laterally. With the exceptio
n of very high-level epizonal plutons, structural studies suggest that
space for many tabular intrusions must be provided mainly by floor-de
pression (lopolith emplacement) rather than roof-lifting (laccolith em
placement). An emplacement model for this type of tabular granite is p
roposed which involves progressive depression of the floor of an initi
ally horizontal chamber as it is filled by one or more vertical condui
ts. A crustal-scale balance in the rates of melt extraction, magma asc
ent and pluton-filling is required by the model, and transfer of mater
ial from the source to the pluton is accommodated by broadly distribut
ed deformation of low strain magnitude. The process is evaluated with
end-member cantilever and piston sinking mechanisms. The models predic
t that large (10-100 km wide), tabular plutons (less than or similar t
o 3 km thick) can be emplaced quickly (100 a to 1 Ma) with floor-depre
ssion and related wall-rock strain rates similar those expected during
tectonic deformation (10(-10) to 10(-15) s(-1)). Bulk strains in the
intervening crustal column rarely exceed a strain ratio of 1.5, which
is likely to remain undetected in the geological record unless the req
uired deformation is accommodated on discrete structures such as norma
l faults or shear zones at the base of the pluton.