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Rheological decoupling at the Moho and implication to Venusian tectonics

Plate tectonics is largely responsible for material and heat circulation in Earth, but for unknown reasons it does not exist on Venus. The strength of planetary materials is a key control on plate tectonics because physical properties, such as temperature, pressure, stress, and chemical composition,...

Deskribapen osoa

Gorde:
Xehetasun bibliografikoak
Egile Nagusiak: Azuma, Shintaro, Katayama, Ikuo, Nakakuki, Tomoeki
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: Nature Publishing Group 2014
Gaiak:
Sarrera elektronikoa:https://ncbi.nlm.nih.gov/pmc/articles/PMC3957145/
https://ncbi.nlm.nih.gov/pubmed/24638113
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/srep04403
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