Vesta and extensively melted asteroids: Why HED meteorites are probably not from Vesta

· by · in ,

John T. Wasson

Earth and Planetary Science Letters
Volume 381, 1 November 2013, Pages 138–146
DOI: 10.1016/j.epsl.2013.09.002
Available online 25 September 2013

LINK

Related posts (automatically generated):

  1. Spectral characterization of V-type asteroids outside the Vesta family
  2. Vestoids, Part II: The basaltic nature and HED meteorite analogs for eight Vp-type asteroids and their associations with (4) Vesta
  3. Asteroids accretion, differentiation, and break-up in the Vesta source region: evidence from cosmochemistry of mesosiderites
  4. Asteroid (4) Vesta: I. The howardite-eucrite-diogenite (HED) clan of meteorites
  5. Differentiation and magmatic history of Vesta: Constraints from HED meteorites and dawn spacecraft data
  6. Tracking the volatile and magmatic history of Vesta from chromium stable isotope variations in eucrite and diogenite meteorites
  7. Spectral Analysis of the Quadrangles Av-13 and Av-14 on Vesta
  8. Modeling the early evolution of Vesta.
  9. Concentrations of Potassium and Thorium within Vesta’s Regolith
  10. Mineralogic Mapping of the Av-9 Numisia quadrangle of Vesta
Tags: , ,