The collision of Jupiter and Comet Shoemaker-Levy 9

Details The collision of Jupiter and Comet Shoemaker-Levy 9 The collision of Jupiter and Comet Shoemaker-Levy 9

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994icar..108....1z&link_type=abstract

Icarus, vol. 108, no. 1, p. 1-17

Other

88

Aerothermodynamics, Atmospheric Entry, Atmospheric Models, Cometary Collisions, Computerized Simulation, Hydrodynamics, Jupiter Atmosphere, Shoemaker-Levy 9 Comet, Aerodynamic Forces, Atmospheric Chemistry, Atmospheric Temperature, Bolides, Energy Dissipation, Light Curve

Scientific paper

A simple description of the disruption and deceleration of 100-m- to 5-km-diameter comets striking Jupiter is combined with numerical simulations of the subsequent explosions to predict the fate of Comet Shoemaker-Levy 9. Detailed numerical simulations of the first 3 min of the explosion were performed. Our numerical simulations begin either with hot cylinders with dimensions suggested by the disruption and deceleration model or with an initial wake constructed from a moving line charge. In all cases, extensive plumes of hot gas are expelled from the atmosphere. The models with wakes evolve about twice as fast as the initially confined models. Models of both types generate similar pressure waves into the planet. Temperatures and negative hydrogen ion opacities were computed. For atmospheric entry, light curves were computed. On entry the largest bolides could be very bright, possibly as bright as Jupiter for observers placed to see them, although for kilometer-size impactors the luminosity peak is obscured by clouds. For the fireball, light curves were computed from the numerical simulations. Metals from the vaporized comet provide electrons that dramatically increase the opacity of Jovian air at low temperature. The fireball rises through and above the atmosphere, brightening at first as its surface area increases, but later fading to invisibility as its temperature drops and its opacity plummets.

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