Analytic expressions for distance-redshift relations that have been co
rrected for the effects of some inhomogeneities in the Friedmann-Rober
tson-Walker (FRW) mass density are used to illustrate the significance
of inhomogeneities in a determination of q(0) made by using Type Ia s
upernovae. The value of q(0) inferred from a given set of observations
depends on the fractional amount of matter in inhomogeneities and is
up to 50% larger than that obtained by using the standard Mattig m-z r
esult for pure-dust FRW models.