  A survey of currently known extrasolar planets indicates that close to 20% of
their hosting stars are members of binary systems. While the majority of these
binaries are wide (i.e., with separations between 250 and 6500 AU), the
detection of Jovian-type planets in the three binaries of Gamma Cephei
(separation of 18.5 AU), GL 86 (separation of 21 AU), and HD 41004 (separation
of 23 AU) have brought to the forefront questions on the formation of giant
planets and the possibility of the existence of smaller bodies in moderately
close binary star systems. This paper discusses the late stage of the formation
of habitable planets in binary systems that host Jovian-type bodies, and
reviews the effects of the binary companion on the formation of Earth-like
planets in the system's habitable zone. The results of a large survey of the
parameter-space of binary-planetary systems in search of regions where
habitable planets can form and have long-term stable orbits are also presented.
