Cloud Formation in Giant Planets

Christiane Helling*

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

We 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.

Original languageEnglish
Title of host publicationEXTREME SOLAR SYSTEMS
EditorsD Fischer, FA Rasio, SE Thorsett, A Wolszczan
PublisherAstronomical Society of the Pacific
Pages443-446
Number of pages4
ISBN (Print)978-1-58381-666-0
Publication statusPublished - 2008
EventConference on Extreme Solar Systems - Santorini, Greece
Duration: 25 Jun 200729 Jun 2007

Publication series

NameASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES
PublisherASTRONOMICAL SOC PACIFIC
Volume398

Conference

ConferenceConference on Extreme Solar Systems
Country/TerritoryGreece
CitySantorini
Period25/06/0729/06/07

Keywords

  • DUST FORMATION
  • STELLAR WINDS
  • BROWN DWARFS
  • ATMOSPHERES
  • GROWTH
  • GRAINS

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