Chondrule size and related physical properties: a compilation and evaluation of current data across all meteorite groups

· by · in ,

Jon M. Friedrich, Michael K. Weisberg, Denton S. Ebel, Alison E. Biltz, Bernadette M. Corbett, Ivan V. Iotzov, Wajiha S. Khan, Matthew D. Wolman

Earth and Planetary Astrophysics
arXiv:1408.6581
Submitted on 27 Aug 2014

PDF LINK

updated (20 September 2014):

Chemie der Erde – Geochemistry
available online 20 September 2014
DOI: 10.1016/j.chemer.2014.08.003

LINK

Related posts (automatically generated):

  1. Thermal and porosity properties of meteorites: A compilation of published data and new measurements
  2. The Chondrule–Matrix Complementarity, a Big Data Approach
  3. Data on 824 fireballs observed by the digital cameras of the European Fireball Network in 2017-2018. II. Analysis of orbital and physical properties of cm-sized meteoroidsOPEN ACCESS 
  4. Chondrule Oxygen Isotope Systematics Among Different Chondrite Groups: Variety of Isotope Reservoirs in the Protoplanetary Disk
  5. The quasi-universality of chondrule size as a constraint for chondrule formation models
  6. Physical properties of the stone meteorites: Implications for the properties of their parent bodiesOPEN ACCESS 
  7. Oxygen-isotope compositions of chondrule phenocrysts and matrix grains in Kakangari K-grouplet chondrite: Implication to a chondrule-matrix genetic relationship
  8. From 2D to 3D chondrule size data: Some empirical ground truths
  9. The Flensburg (C1-Ungrouped) 2019 Meteorite Fall: Raman Spectroscopy and Compilation of Magnetic Susceptibility Data on C — Ungrouped Falls/Finds
  10. The Properties of Planetesimal Collisions under Jupiter’s Perturbation and the Application to Chondrule Formation via Impact JettingOPEN ACCESS