About a hundred dust impacts per day were detected during the first we
ek in December 1995 by Galileo during its approach to Jupiter, These i
mpacts were caused by submicrometer-sized particles that were just abo
ve the detection limit. After the closest approach to Io on 7 December
, impacts of these small particles ceased, This effect is expected for
dust grains emitted from Io that exit the field of view of the instru
ment after the flyby. The impact rate of bigger micrometer-sized dust
grains continued to increase toward Jupiter. These dust particles are
in orbit about Jupiter or are interplanetary grains that are gravitati
onally concentrated near Jupiter.