Early oxidation of the martian crust triggered by impacts

Despite the abundant geomorphological evidence for surface liquid water on Mars during the Noachian epoch (>3.7 billion years ago), attaining a warm climate to sustain liquid water on Mars at the period of the faint young Sun is a long-standing question. Here, we show that melts of ancient mafic...

Descripción completa

Detalles Bibliográficos
Autores principales: Deng, Zhengbin, Moynier, Frédéric, Villeneuve, Johan, Jensen, Ninna K., Liu, Deze, Cartigny, Pierre, Mikouchi, Takashi, Siebert, Julien, Agranier, Arnaud, Chaussidon, Marc, Bizzarro, Martin
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2020
Materias:
Research Articles
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7608801/
https://www.ncbi.nlm.nih.gov/pubmed/33127679
http://dx.doi.org/10.1126/sciadv.abc4941

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7608801/
https://www.ncbi.nlm.nih.gov/pubmed/33127679
http://dx.doi.org/10.1126/sciadv.abc4941

Ejemplares similares