Cloud formation in giant planets

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dc.creatorHelling, Christiane
dc.date2007-11-23
dc.date.accessioned2026-07-07T08:44:41Z
dc.date.available2026-07-07T08:44:41Z
dc.descriptionWe calculate the formation of dust clouds in atmospheres of giant gas-planets. The chemical structure and the evolution of the grain size distribution in the dust cloud layer is discussed based on a consistent treatment of seed formation, growth/evaporation and gravitational settling. Future developments are shortly addressed.
dc.description4 pages, Proceeding to "Extreme solar systems", eds. Fischer, Rasio, Thorsett, Wolszczan
dc.identifierhttps://arxiv.org/abs/0711.3730
dc.identifierhttp://arxiv.org/abs/0711.3730
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/142743
dc.subjectAstrophysics
dc.titleCloud formation in giant planets
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