Results 21 to 30 of about 6,913 (220)
Accretion of dust by chondrules in a MHD-turbulent solar nebula [PDF]
(Abridged) Numerical magnetohydrodynamic (MHD) simulations of a turbulent solar nebula are used to study the growth of dust mantles swept up by chondrules. A small neighborhood of the solar nebula is represented by an orbiting patch of gas at a radius of
Armitage +33 more
core +1 more source
The Origin of Chondrules: Constraints from Matrix-Chondrule Complementarity
One of the major unresolved problems in cosmochemistry is the origin of chondrules, once molten, spherical silicate droplets with diameters of 0.2 to 2 mm. Chondrules are an essential component of primitive meteorites and perhaps of all early solar system materials including the terrestrial planets.
Palme, H, Hezel, D.C, Ebel, D.S.
openaire +2 more sources
Chondrule transport in protoplanetary discs [PDF]
Accepted to MNRAS.
Goldberg, Aaron Z. +2 more
openaire +3 more sources
Chondrules and nebular shocks [PDF]
Invited editorial in Meteoritics and Planetary Science, vol.
openaire +2 more sources
Chondrules in Enstatite Chondrites [PDF]
23 pages, 4 figures. Submitted manuscript for a chapter in the book "Chondrules and the protoplanetary disc" (editors : S. Russell, H. C. Connolly Jr, A. N. Krot) to be published by Cambridge University Press in 2018. This version is free to view and download for personal use only.
Jacquet, Emmanuel +2 more
openaire +3 more sources
Compound chondrules fused cold [PDF]
7 pages, 3 figures, 1 table.
openaire +2 more sources
Origin of Isotopic Diversity among Carbonaceous Chondrites
Carbonaceous chondrites are some of the most primitive meteorites and derive from planetesimals that formed a few million years after the beginning of the solar system.
Jan L. Hellmann +7 more
doaj +1 more source
Iron Isotope Constraints on the Structure of the Early Solar System
The recent advent of nontraditional isotopic systems has revealed that meteorites display a fundamental isotopic dichotomy between noncarbonaceous (NC) and carbonaceous (C) groups, which represent material from the inner and outer solar system ...
Yves Marrocchi +2 more
doaj +1 more source
Multiple carriers of Q noble gases in primitive meteorites [PDF]
The main carrier of primordial heavy noble gases in chondrites is thought to be an organic phase, known as phase Q, whose precise characterization has resisted decades of investigation.
Amari +40 more
core +2 more sources
CHONDRULE DESTRUCTION IN NEBULAR SHOCKS [PDF]
18 pages, 12 figures.
Jacquet, Emmanuel, Thompson, Christopher
openaire +2 more sources

