HED Meteorites and Their Relationship to the Geology of Vesta and the Dawn Mission
By H. McSween, David W. Mittlefehldt, A. Beck, R. Mayne, T. Mccoy. 2011
230 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Geophysics
View Paper: https://www.semanticscholar.org/paper/7e4ecf0b3f1a182f352423d19db326f0457ee6cd
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In Astronomy and Astrophysics
In Geophysics
Citations in the corpus
- Asteroid (4) Vesta: I. The howardite-eucrite-diogenite (HED) clan of meteorites (2015, methodology): “There is crystal fractionation sequence between main-group and Nuevoaredo-group eucrites (cf. Stolper, 1977), but there might be two or ore fractionation sequences represented by main-group eucrites McSween et al., 2011).”
- Melting and differentiation of early-formed asteroids: The perspective from high precision oxygen isotope studies (2017, methodology): “…or intrusions, diogenites are orthopyroxene-rich, coarser-grained igneous cumulates, and howardites are complex impact breccias containing both diogenitic and eucritic fragments (Mittlefehldt et al., 1998; Mittlefehldt, 2015; Barrat et al., 2008, 2010; Yamaguchi et al., 2009; McSween et al., 2011).”