50Ti Evidence for Different Refractory Precursors in Chondrules

· by · in , , ,

Ebert S. Render J. Brennecka G. A. Burkhardt C. Bischoff A. Kleine T.

80th Annual Meeting of the Meteoritical Society 2017 [#6255]

abstract

“Different refractory precursors in chondrules are necessary to explain the different 50Ti isotope data for Na-rich chondrules in ordinary and CO3 chondrites. ”

Related posts (automatically generated):

  1. Genetic relationship between Na-rich chondrules and Ca,Al-rich inclusions? – Formation of Na-rich chondrules by melting of refractory and volatile precursors in the Solar Nebula
  2. Refractory inclusions as Type IA chondrule precursors: Constraints from melting experiments
  3. Chromium Isotopic Evidence for an Early Formation of Chondrules from the Ornans CO Chondrite
  4. Mixing and transport of dust in the early solar nebula as inferred from titanium isotope variations among chondrulesOPEN ACCESS 
  5. Oxygen isotopic diversity of chondrule precursors and the nebular origin of chondrules
  6. Multiple CV Chondrule Precursors Originating from the Inner and Outer Solar System: Evidence from Cr-Ti-O Isotope Systematics of Allende Chondrules
  7. Chromium Isotopic Evidence for an Early Formation of Chondrules from the Ornans CO Chondrite
  8. Mineralogically zoned chondrules in ordinary chondrites as evidence for open system chondrule behaviour
  9. Barred olivine chondrules in ordinary chondrites: Constraints on chondrule formationOPEN ACCESS 
  10. Trace Element Composition of Silicate Minerals in the Chondrules and Matrix of the Buschhof Meteorite
Tags: , , , , , , ,