Emergence of two types of terrestrial planet on solidification of magma ocean View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2013-05-29

AUTHORS

Keiko Hamano, Yutaka Abe, Hidenori Genda

ABSTRACT

Terrestrial planets can be divided into two distinct types on the basis of their evolutionary history during solidification from their initial molten state: type I planets (such as Earth) solidify within several million years and retain most of their water, and type II planets (possibly such as Venus), formed inside a critical distance, are desiccated by hydrodynamic escape. More... »

PAGES

607-610

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/nature12163

DOI

http://dx.doi.org/10.1038/nature12163

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1002044847

PUBMED

https://www.ncbi.nlm.nih.gov/pubmed/23719462


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