Setting the Stage: Planet formation and Volatile Delivery. (arXiv:2006.07127v1 [astro-ph.EP])
<a href="http://arxiv.org/find/astro-ph/1/au:+Venturini_J/0/1/0/all/0/1">Julia Venturini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ronco_M/0/1/0/all/0/1">M. Paula Ronco</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Guilera_O/0/1/0/all/0/1">Octavio M. Guilera</a>
The diversity in mass and composition of planetary atmospheres stems from the
different building blocks present in protoplanetary discs and from the
different physical and chemical processes that these experience during the
planetary assembly and evolution. This review aims to summarise, in a nutshell,
the key concepts and processes operating during planet formation, with a focus
on the delivery of volatiles to the inner regions of the planetary system.
The diversity in mass and composition of planetary atmospheres stems from the
different building blocks present in protoplanetary discs and from the
different physical and chemical processes that these experience during the
planetary assembly and evolution. This review aims to summarise, in a nutshell,
the key concepts and processes operating during planet formation, with a focus
on the delivery of volatiles to the inner regions of the planetary system.
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