Results 111 to 120 of about 1,937 (173)
The group A3 chondrules of Krymka: Further evidence for major evaporative loss during the formation of chondrules [PDF]
Like Semarkona (type 3.0), Krymka (type 3.1) contains two distinct types of chondrule (namely groups A and B) which differ in their bulk compositions, phase compositions, and CL properties.
Huang, S. +2 more
core +1 more source
Shape, size, and distribution of magnetic particles in Bjurbole chondrules [PDF]
Chondrules from the Bjurbole chondritic meteorite (L4) exhibit saturation remanence magnetization (SIRM) values which vary over three orders of magnitude.
Nava, David F.
core +1 more source
En este trabajo se analiza la distribución espacial y los contenidos relativos de hierro (Fe), níquel (Ni) y azufre (S) en condros individuales separados de un fragmento del meteorito Allende, por medio de observaciones y análisis con microscopía ...
Daniel Flores-Gutiérrez +4 more
doaj
Adhesive growth and abrasion of chondrules during the accretion process [PDF]
P(論文)Droplet chondrules are classified into three groups based on the surface features. The group A chondrules, common in the equilibrated chondrites, do not have a clear boundary with the matrix. The ambiguity of the surfaces of group A can be explained
Watanabe, Seiko, Kitamura, Masao
core +1 more source
Two spinel-bearing compound chondrules from the Baszkówka meteorite [PDF]
The present paper describes two compound chondrules labelled panda and chevron, discovered in the Baszkówka meteorite. Optical microscope, electron microscope and electron microprobe studies revealed an unusual mineral composition and fabric.
Borucki, J., Stępniewski, M.
core
Petrology of chondrules in ALH-77015 (L3) chondrite [PDF]
P(論文)Chondrules in ALH-77015 (L3) chondrite were studied petrographically. Size and bulk chemical composition of about one hundred chondrules were investigated with relation to their texture. There seems to be no relation between the size and the texture,
Nagahara, Hiroko
core +1 more source
Forming the Noncarbonaceous Chondrite Parent Bodies in the Presence of the Jupiter Barrier
Meteorites can be divided into two groups—noncarbonaceous chondrite like (NC) and carbonaceous chondrite like (CC)—with distinct stable-isotope compositions. Parent bodies of NC and CC meteorites have overlapping formation ages. This suggests they formed
John Chambers
doaj +1 more source
Fast, collimated jets are ubiquitous features of young stellar objects. They are generally thought to be powered by disk accretion, but the details are debated.
Yisheng Tu +4 more
doaj +1 more source
P(論文) Textures of chondrules in the unequilibrated ordinary chondrites have been summarized on the basis of the processes of their formation inferred from the results of previous experiments. The chondrules studied are classified by their textures into the following four groups : (1) those formed by complete melting of the precursor materials, (2 ...
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