Shallow-crustal to mid-crustal magma-emplacement models commonly rely
on local or regional extension to solve the ''room'' problem. We argue
that existing extensional models explain the emplacement of sheeted-d
ike complexes or internally layered plutons but are not as easily reco
nciled with the emplacement of elliptically shaped plutons or batholit
hs for the following reasons: (1) rock strengths and crustal stresses
prevent large voids from existing at depth and therefore require wall-
rock extension to be balanced by magma influx; (2) rates of extension
are controlled by fault slip rates of millimetres to centimetres per y
ear and thus require numerous small injections of magma; and (3) becau
se of their sheetlike shapes and small thicknesses, these small magma
injections will cool rapidly and form sheeted plutons or dike swarms.
Extension may, however, facilitate emplacement of elliptically shaped
plutons in concert with other mechanisms if certain kinematic constrai
nts are satisfied.