Dawn; the Vesta–HED connection; and the geologic context for eucrites, diogenites, and howardites
By H. McSween, R. Binzel, M. D. De Sanctis, E. Ammannito, T. Prettyman, A. Beck, Vishnu Reddy, L. Corre, M. Gaffey, T. McCord and 2 more. 2013
202 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Ecology
View Paper: https://www.semanticscholar.org/paper/ad9e6755d741569ab4433350fe3f562ee26773b9
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Citations in the corpus
- The pH of Enceladus’ ocean (2015, background): “McSween H. Y., et al. (2013) Dawn; the Vesta-HED connection; and the geologic context for eucrites, diogenites, and howardites.”
- Melting and differentiation of early-formed asteroids: The perspective from high precision oxygen isotope studies (2017, methodology): “As discussed in Section 3.3.3, the fact that the vast majority of diogenite, eucrite and cumulate eucrite samples have virtually identical 17O values lends support to the view that all of the major HED lithologies are derived from a single parent asteroid (McSween et al., 2013).”
- Asteroid (4) Vesta: I. The howardite-eucrite-diogenite (HED) clan of meteorites (2015, background): “The evidence outlined by McSween et al. (2013) in favor of Vesta as the HED parent asteroid is more compelling in my opinion, but again, does not require that this be true.”