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Ganymede and Callisto:Accumulation Heat Content

Conference paper
Part of the NATO Advanced Study Institutes Series book series (ASIC, volume 85)

Abstract

Using the accumulation theory for the formation o the two outermost regular satellites of Jupiter, the accumulation heat content has been obtained. The early thermal profiles show the onset of convection just at the end of the formation process, having taken into account the energy irreversibly trapped and the projectile penetration depth in the impacts. The fraction of the gravitational energy converted into thermal energy results to be larger for Callisto than for Ganymede.

Keywords

Nusselt Number Rayleigh Number Impact Velocity Thermal Profile Adiabatic Compression 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company 1982

Authors and Affiliations

  1. 1.I.A.S.Reparto di PlanetologiaRomaItaly
  2. 2.Istituto di Geologia dell’Università degli Studi di PerugiaItaly

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