Results 21 to 30 of about 6,913 (220)

Accretion of dust by chondrules in a MHD-turbulent solar nebula [PDF]

open access: yes, 2010
(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

open access: yesEarth and Planetary Sciences Letters, 2015
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]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
Accepted to MNRAS.
Goldberg, Aaron Z.   +2 more
openaire   +3 more sources

Chondrules and nebular shocks [PDF]

open access: yesMeteoritics & Planetary Science, 2002
Invited editorial in Meteoritics and Planetary Science, vol.
openaire   +2 more sources

Chondrules in Enstatite Chondrites [PDF]

open access: yes, 2018
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]

open access: yesIcarus, 2015
7 pages, 3 figures, 1 table.
openaire   +2 more sources

Origin of Isotopic Diversity among Carbonaceous Chondrites

open access: yesThe Astrophysical Journal Letters, 2023
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

open access: yesThe Astrophysical Journal Letters, 2023
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]

open access: yes, 2015
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]

open access: yesThe Astrophysical Journal, 2014
18 pages, 12 figures.
Jacquet, Emmanuel, Thompson, Christopher
openaire   +2 more sources

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