Knowledge of the 
 form factors
at the zero-recoil point
is crucial to extract the element 
of the Cabbibo-Kobayashi-Maskawa matrix
that parameterizes the amount of mixing between the b and c quarks,
, from experiment.
In the limit that the heavy quarks are infinitely heavy,
heavy quark effective theory (HQET)
predicts that the form factors 
, 
, and 
 are equal.
The formally dominant 
correction due to breaking of heavy quark symmetry
comes from the inclusion of a 
 dimension-three
operator in the Lagrangian that leads 
to
hyperfine-splitting between the heavy pseudoscalar and vector mesons. 
These leading order corrections are 
as required by Luke's theorem.
Recent lattice simulations using the quenched approximation of
QCD have made a big step forward in determining these zero-recoil
form factors.  Presently, however, the simulations use
light quark masses that are much heavier than the physical ones
and therefore rely on a chiral extrapolation down
to the physical quark masses. 
In this work we calculate the dominant corrections
to the form factors 
, 
, and 
in quenched chiral perturbation theory (Q
PT) 
and determine the non-analytic dependence 
on the light quark masses. 
Using these results 
to extrapolate the
quenched QCD lattice measurements of these form factors
down to the physical pion mass should give a more reliable
estimate of the errors associated with the chiral extrapolation.