Impact-induced changes in source depth and volume of magmatism on Mercury and their observational signatures

Mantle partial melting produced the volcanic crust of Mercury. Here, the authors numerically model the formation of post-impact melt sheets and find that mantle convection was weak at around 3.7–3.8 Ga and that the melt sheets of Caloris and Rembrandt may contain partial melting of pristine mantle m...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Sebastiano Padovan, Nicola Tosi, Ana-Catalina Plesa, Thomas Ruedas
Formato: article
Lenguaje:EN
Publicado: Nature Portfolio 2017
Materias:
Q
Acceso en línea:https://doaj.org/article/e27fd91a775f48b69b28f3fc0362253d
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
id oai:doaj.org-article:e27fd91a775f48b69b28f3fc0362253d
record_format dspace
spelling oai:doaj.org-article:e27fd91a775f48b69b28f3fc0362253d2021-12-02T13:27:30ZImpact-induced changes in source depth and volume of magmatism on Mercury and their observational signatures10.1038/s41467-017-01692-02041-1723https://doaj.org/article/e27fd91a775f48b69b28f3fc0362253d2017-12-01T00:00:00Zhttps://doi.org/10.1038/s41467-017-01692-0https://doaj.org/toc/2041-1723Mantle partial melting produced the volcanic crust of Mercury. Here, the authors numerically model the formation of post-impact melt sheets and find that mantle convection was weak at around 3.7–3.8 Ga and that the melt sheets of Caloris and Rembrandt may contain partial melting of pristine mantle material.Sebastiano PadovanNicola TosiAna-Catalina PlesaThomas RuedasNature PortfolioarticleScienceQENNature Communications, Vol 8, Iss 1, Pp 1-10 (2017)
institution DOAJ
collection DOAJ
language EN
topic Science
Q
spellingShingle Science
Q
Sebastiano Padovan
Nicola Tosi
Ana-Catalina Plesa
Thomas Ruedas
Impact-induced changes in source depth and volume of magmatism on Mercury and their observational signatures
description Mantle partial melting produced the volcanic crust of Mercury. Here, the authors numerically model the formation of post-impact melt sheets and find that mantle convection was weak at around 3.7–3.8 Ga and that the melt sheets of Caloris and Rembrandt may contain partial melting of pristine mantle material.
format article
author Sebastiano Padovan
Nicola Tosi
Ana-Catalina Plesa
Thomas Ruedas
author_facet Sebastiano Padovan
Nicola Tosi
Ana-Catalina Plesa
Thomas Ruedas
author_sort Sebastiano Padovan
title Impact-induced changes in source depth and volume of magmatism on Mercury and their observational signatures
title_short Impact-induced changes in source depth and volume of magmatism on Mercury and their observational signatures
title_full Impact-induced changes in source depth and volume of magmatism on Mercury and their observational signatures
title_fullStr Impact-induced changes in source depth and volume of magmatism on Mercury and their observational signatures
title_full_unstemmed Impact-induced changes in source depth and volume of magmatism on Mercury and their observational signatures
title_sort impact-induced changes in source depth and volume of magmatism on mercury and their observational signatures
publisher Nature Portfolio
publishDate 2017
url https://doaj.org/article/e27fd91a775f48b69b28f3fc0362253d
work_keys_str_mv AT sebastianopadovan impactinducedchangesinsourcedepthandvolumeofmagmatismonmercuryandtheirobservationalsignatures
AT nicolatosi impactinducedchangesinsourcedepthandvolumeofmagmatismonmercuryandtheirobservationalsignatures
AT anacatalinaplesa impactinducedchangesinsourcedepthandvolumeofmagmatismonmercuryandtheirobservationalsignatures
AT thomasruedas impactinducedchangesinsourcedepthandvolumeofmagmatismonmercuryandtheirobservationalsignatures
_version_ 1718393005941981184