We examine the possibility that gamma-rav bursts arise from sources in
the Oort comet cloud, basing most of our arguments on accepted models
for the formation and spatial distribution of the cloud. We identify
three severe problems with such models: (1) There is no known mechanis
m for producing bursts that can explain the observed burst rate and en
ergetics without violating other observational constraints. (2) The br
ight source counts cannot be reconciled with standard models for the p
hase-space distribution of objects in the Oort cloud. (3) The observed
isotropy of the available burst data is inconsistent with the expecte
d angular distribution of sources in the Oort cloud. We therefore asse
rt that Oort cloud models of gamma-ray bursts are extremely implausibl
e.