QUESTION:
Where is the spacecraft's camera located?

ANSWER from FAQ:
Most people think that the Solid-State Imaging instrument (SSI),
which takes photos in visible light, is Galileo's only camera, but
there are actually three other cameras on board. A
photopolarimeter-radiometer will measure the polarization of light
scattered from Jupiter's clouds and the satellites' surfaces, by a
process like using polarized sunglasses to cut down on glare. In
addition, its infrared channels will sound the atmosphere and
measure satellite temperatures. The near-infrared mapping
spectrometer will map the satellites, looking for different minerals
across their surfaces. It will also study cloud structure and gas
composition in the jovian atmosphere. An ultraviolet spectrometer
and extreme ultraviolet spectrometer will investigate volatile excape
and surface composition of the Galilean satellites, the Io plasma
torus, small and large scale properties of the Jupiter clouds, and the
composition, structure, and evolution of Jupiter's upper
atmosphere. 

All four cameras are mounted on a scan platform, located near the
bottom of the orbiter. This section of the spacecraft can be
"despun," or kept from spinning with the rest of the
orbiter--otherwise, all the images would be blurry.