  The UVS instrument on the Juno mission recorded transient bright emission
from a point source in Jupiter's atmosphere. The spectrum shows that the
emission is consistent with a 9600-K blackbody located 225 km above the 1-bar
level and the duration of the emission was between 17 ms and 150 s. These
characteristics are consistent with a bolide in Jupiter's atmosphere. Based on
the energy emitted, we estimate that the impactor had a mass of 250-5000 kg,
which corresponds to a diameter of 1-4 m. By considering all observations made
with Juno UVS over the first 27 perijoves of the mission, we estimate an impact
flux rate of 24,000 per year for impactors with masses greater than 250-5000
kg.
