Compositions of carbonaceous-type asteroidal cores in the early solar system

The parent cores of iron meteorites belong to the earliest accreted bodies in the solar system. These cores formed in two isotopically distinct reservoirs: noncarbonaceous (NC) type and carbonaceous (CC) type in the inner and outer solar system, respectively. We measured elemental compositions of CC...

Descripción completa

Detalles Bibliográficos
Autores principales: Zhang, Bidong, Chabot, Nancy L., Rubin, Alan E.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2022
Materias:
Earth, Environmental, Ecological, and Space Sciences
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9481128/
https://www.ncbi.nlm.nih.gov/pubmed/36112692
http://dx.doi.org/10.1126/sciadv.abo5781

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9481128/
https://www.ncbi.nlm.nih.gov/pubmed/36112692
http://dx.doi.org/10.1126/sciadv.abo5781

Ejemplares similares