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Cloud formation in Exoplanetary Atmospheres

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arxiv 2205.00454 v1 pith:3G4O4RYN submitted 2022-05-01 astro-ph.EP astro-ph.SRphysics.comp-phphysics.space-ph

Christiane Helling This is my paper · ORCID
classification astro-ph.EPastro-ph.SRphysics.comp-phphysics.space-ph
keywords cloudformationatmospheresallowanalysisapproachbasicconcepts
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This invited review for young researchers presents key ideas on cloud formation as key part for virtual laboratories for exoplanet atmospheres. The basic concepts are presented, followed by utilising a time-scale analysis to disentangle process hierarchies. The kinetic approach to cloud formation modelling is described in some detail to allow the discussion of cloud structures as prerequisite for future extrasolar weather forecasts.

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Cited by 1 Pith paper

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  1. Overcast mornings and clear evenings in hot Jupiter exoplanet atmospheres

    astro-ph.EP 2025-07 conditional novelty 6.0 of 10

    Three hot Jupiters (WASP-39 b, WASP-94 Ab, WASP-17 b) show >5 sigma morning-evening limb differences in water absorption, with mornings muted by high-altitude aerosols.

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