The Primary Atmospheres of Planets: The Formation, The Impact on Planet Formation and How to Characterize Them
abstract: Planets are generally believed to form in protoplanetary disks within a few million years (Myr) to several hundred Myr. But planetary embryos or protoplanets likely exist before disk gas dissipates (in three to ten Myr), capturing H2 -rich primary atmospheres from the nebula. Exploring the...
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| Format: | Doctoral Thesis |
| Language: | English |
| Published: |
2020
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| Online Access: | http://hdl.handle.net/2286/R.I.62944 |