Disk Evolution, Element Abundances and Cloud Properties of Young Gas Giant Planets

We discuss the chemical pre-conditions for planet formation, in terms of gas and ice abundances in a protoplanetary disk, as function of time and position, and the resulting chemical composition and cloud properties in the atmosphere when young gas giant planets form, in particular discussing the ef...

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Bibliographic Details
Main Authors: Christiane Helling, Peter Woitke, Paul B. Rimmer, Inga Kamp, Wing-Fai Thi, Rowin Meijerink
Format: Article
Language:English
Published: MDPI AG 2014-04-01
Series:Life
Subjects:
Online Access:http://www.mdpi.com/2075-1729/4/2/142