Evolutionary dichotomy for rocky planets
Linda T. Elkins-Tanton ()
Additional contact information
Linda T. Elkins-Tanton: Carnegie Institution for Science, Washington DC 20015, USA.
Nature, 2013, vol. 497, issue 7451, 570-572
Abstract:
A simple model shows that a rocky planet close to its star may solidify so slowly that its water is lost to space and the planet becomes desiccated, whereas a planet farther out may solidify quickly and retain its water. See Letter p.607
Date: 2013
References: Add references at CitEc
Citations:
Downloads: (external link)
https://www.nature.com/articles/497570a Abstract (text/html)
Access to the full text of the articles in this series is restricted.
Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.
Export reference: BibTeX
RIS (EndNote, ProCite, RefMan)
HTML/Text
Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:497:y:2013:i:7451:d:10.1038_497570a
Ordering information: This journal article can be ordered from
https://www.nature.com/
DOI: 10.1038/497570a
Access Statistics for this article
Nature is currently edited by Magdalena Skipper
More articles in Nature from Nature
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().