We report trace element concentrations of silicate phases in chondrules from LL3 ordinary chondrites Bishunpur and Semarkona. Results are similar to previously reported data for …
Ten whole chondrules separated from the Dhajala (H3, 4), Hallingeberg (L3), and Semarkona (LL3) chondrites were individually analyzed for bulk element composition by …
Among primitive meteorites, CR chondrites have peculiar isotopic compositions, the origin of which is uncertain and may have involved contributions from primordial molecular cloud …
We report in situ ion microprobe analyses of oxygen isotopic compositions of olivine, low-Ca pyroxene, high-Ca pyroxene, anorthitic plagioclase, glassy mesostasis, and spinel in five …
FeO-poor (type I) porphyritic chondrules formed by incomplete melting of solid dust precursors via a yet-elusive mechanism. Two settings are generally considered for their …
B Zanda - Earth and Planetary Science Letters, 2004 - Elsevier
Chondrules are submillimeter spheres that constitute up to 80% of the volume of the most primitive meteorites. That they result from the solidification of a melt in low-gravity in the early …
T Akaki, T Nakamura - Geochimica et Cosmochimica Acta, 2005 - Elsevier
We found thirty compound chondrules in two CV3 carbonaceous chondrites. The abundance in each meteorite relative to single chondrules is 29/1846 (1.6%) in Allende and …
S Maruyama, H Yurimoto, S Sueno - Earth and Planetary Science Letters, 1999 - Elsevier
Oxygen isotope compositions of individual mineral grains in two spinel-bearing chondrules have been determined by secondary ion mass spectrometry. O isotope ratios of spinel …
Chondrules in E3 chondrites differ from those in other chondrite groups. Many contain near- pure endmember enstatite (Fs< 1). Some contain Si-bearing FeNi metal, Cr-bearing troilite …