Three-dimensional numerical simulations of the impact of Comet Shoemak
er - Levy 9 on Jupiter and the resulting vapor plume expansion were co
nducted using the Smoothed Particle Hydrodynamics (SPH) method. An icy
body with a diameter of 2 km can penetrate to an altitude of -350 km
(0 km = 1 bar) and most of the incident kinetic energy is transferred
to the atmosphere between -100 km to -250 km. This energy is converted
to potential energy of the resulting gas plume. The unconfined plume
expands vertically and has a peak radiative power approximately equal
to the total radiation from Jupiter's disc. The plume rises a few tens
of atmospheric scale heights in approximately 10(2), seconds. The ris
ing plume reaches the altitude of approximately 3000 km, but no atmosp
heric gas is accelerated to the escape velocity (approximately 60 km/s
).