Ontology type: schema:ScholarlyArticle
2013-02-13
AUTHORSM. Jutzi, E. Asphaug, P. Gillet, J.-A. Barrat, W. Benz
ABSTRACTThree-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... »
PAGES207-210
http://scigraph.springernature.com/pub.10.1038/nature11892
DOIhttp://dx.doi.org/10.1038/nature11892
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PUBMEDhttps://www.ncbi.nlm.nih.gov/pubmed/23407535
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