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...
Main Authors: | , , , , , |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2014-04-01
|
Series: | Life |
Subjects: | |
Online Access: | http://www.mdpi.com/2075-1729/4/2/142 |