A pebble accretion model for the formation of the terrestrial planets in the Solar System

Pebbles of millimeter sizes are abundant in protoplanetary discs around young stars. Chondrules inside primitive meteorites—formed by melting of dust aggregate pebbles or in impacts between planetesimals—have similar sizes. The role of pebble accretion for terrestrial planet formation is nevertheles...

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Detalles Bibliográficos
Autores principales: Johansen, Anders, Ronnet, Thomas, Bizzarro, Martin, Schiller, Martin, Lambrechts, Michiel, Nordlund, Åke, Lammer, Helmut
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2021
Materias:
Research Articles
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7888959/
https://www.ncbi.nlm.nih.gov/pubmed/33597233
http://dx.doi.org/10.1126/sciadv.abc0444

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7888959/
https://www.ncbi.nlm.nih.gov/pubmed/33597233
http://dx.doi.org/10.1126/sciadv.abc0444

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