A slowly cooled deep crust on asteroid 4 Vesta and the recent impact history of rubble pile vestoids recorded by diogenites
Author:
Publisher
Elsevier BV
Subject
Geochemistry and Petrology
Reference72 articles.
1. Comment on “The origin of eucrites, diogenites, and olivine diogenites: Magma ocean crystallization and shallow magma processes on Vesta” by B. E. Mandler and L. T. Elkins-Tanton;Barrat;Meteorit. Planet. Sci.,2014
2. Geochemistry of diogenites: still more diversity in their parental melts;Barrat;Meteorit. Planet. Sci.,2008
3. Trace element geochemistry of K-rich impact spherules from howardites;Barrat;Geochim Cosmochim Ac,2009
4. Diogenites as polymict breccias composed of orthopyroxenite and harzburgite;Beck;Meteorit. Planet. Sci..,2010
5. Determining the noble gas cosmic ray exposure ages of 23 meteorites (8 chondrites and 15 achondrites) from modeling and empirical methods;Bekaert;Meteorit. Planet. Sci..,2022
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1. Accessory mineral microstructure and chronology reveals no evidence for late heavy bombardment on the asteroid 4-Vesta;Earth and Planetary Science Letters;2024-06
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