On 19 December 1996 as Galileo passed close to Jupiter's moon, Europa,
the magnetometer measured substantial departures from the slowly Vary
ing background field of Jupiter's magnetosphere. Currents coupling Eur
opa to Jupiter's magnetospheric plasma could produce perturbations of
the observed size. However, the trend of the field perturbations is he
re modeled as the signature of a Europa-centered dipole moment whose m
aximum surface magnitude is similar to 240 nanotesla, giving a rough u
pper limit to the internal field. The dipole orientation is oblique to
Europa's spin axis. This orientation may not be probable for a field
generated by a core dynamo, but higher order multipoles may be importa
nt as they are at Uranus and Neptune. Although the data can be modeled
as contributions of an internal field of Europa, they do not confirm
its existence. The dipole orientation is also oblique to the imposed f
ield of Jupiter and thus not directly produced as a response to that f
ield. Close to Europa, plasma currents appear to produce perturbations
with scale sizes that are smalt compared with a Europa radius.