P-Rich Olivines in the Impact Melt Lithology of the Chelyabinsk Meteorite

· by · in

I. B. Baziotis, L. Ferrière, P. D. Asimow, D. Topa, F. Brandstätter

47th Lunar and Planetary Science Conference (2016), Abstract #1437

LINK

Related posts (automatically generated):

  1. Comparative Study of two Chelyabinsk LL5 Ordinary Chondrite Fragments with Light Lithology and the Fusion Crust Using Mössbauer Spectroscopy
  2. Chelyabinsk meteorite: Shock metamorphism, black veins and impact melt dikes, and the Hugoniot
  3. The Gao-Guenie impact melt breccia—Sampling a rapidly cooled impact melt dike on an H chondrite asteroid?.
  4. Post-impact metamorphism of the chelyabinsk meteorite in shock experiment
  5. Nanoindenting the Chelyabinsk meteorite to learn about impact deflection effects in asteroidsOPEN ACCESS 
  6. Impact history of the Chelyabinsk meteorite: Electron microprobe and LA-ICP-MS study of sulfides and metals
  7. Comparison of two different infrared spectral analysis based evaluation of impact induced shock events of the Chelyabinsk meteorite
  8. Ar-Ar and U-Pb ages of Chelyabinsk and a re-evaluation of its impact chronology
  9. Microtextures in the Chelyabinsk impact breccia reveal the history of Phosphorus-Olivine-Assemblages in chondritesOPEN ACCESS 
  10. Search for a meteoritic component within the impact melt rocks of the Chicxulub impact structure peak ring, MexicoOPEN ACCESS 
Tags: , ,