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Article
Water Partitioning in Planetary Embryos and Protoplanets with Magma Oceans
The water content of magma oceans is widely accepted as a key factor that determines whether a terrestrial planet is habitable. Water ocean mass is determined as a result not only of water delivery and loss, b...
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Article
Formation and Evolution of Protoatmospheres
The origin and evolution of planetary protoatmospheres in relation to the protoplanetary disk is discussed. The initial atmospheres of planets can mainly be related via two formation scenarios. If a protoplane...