The structure of the asteroid 4 Vesta as revealed by models of planet-scale collisions View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2013-02-13

AUTHORS

M. Jutzi, E. Asphaug, P. Gillet, J.-A. Barrat, W. Benz

ABSTRACT

Three-dimensional simulations of the global evolution of asteroid 4 Vesta under two overlapping planet-scale collisions closely reproduce its observed shape; but expected large areas of olivine-rich rocks and pure diogenites are not observed on the surface, possibly implying that the outer ∼100 km is composed mainly of a basaltic crust (eucrites) with ultramafic intrusions (diogenites). More... »

PAGES

207-210

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/nature11892

DOI

http://dx.doi.org/10.1038/nature11892

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1045262195

PUBMED

https://www.ncbi.nlm.nih.gov/pubmed/23407535


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