Results 101 to 110 of about 1,937 (173)
"Dehydrated" chondrules from the Murchison (CM) chondrite [PDF]
P(論文)Two "dehydrated" chondrules (MC-5 and MC-27) were obtained from close to the fusion crust of the Murchison (CM) meteorite. They have a porphyritic texture with angular or rounded (relict) olivines containing abundant voids, recrystallized olivines ...
Inoue,Mutsuo, Nakamura,Noboru
core +2 more sources
Chondrule Dust Rim Growth: Influence of Restructuring Using Molecular Dynamics Simulations
We investigate the influence of disruptive collisions on chondrule rim growth, emphasizing the role of kinetic energy in determining the outcomes of these interactions.
Chuchu Xiang +4 more
doaj +1 more source
Experimental Reproduction of Olivine rich Type-I Chondrules [PDF]
Ordinary chondritic meteorites are an abundant type of stony meteorite characterized by the presence of chondrules. Chondrules are small spheres consisting of silicate, metal, and sulfide minerals that experienced melting in the nebula before ...
Smith, Robert K.
core +1 more source
Petrography and mineral chemistry of Escalón meteorite, an H4 chondrite, México
The Escalón meteorite, a crusted mass weighing 54.3 g, was recovered near Zona del Silencio in Escalón, state of Chihuahua, México. The stone is an ordinary chondrite belonging to the high iron group H, type 4.
Adela M. Reyes-Salas +7 more
doaj
Tungsten Isotopes and the Origin of Chondrules and Chondrites [PDF]
Chondrules and matrix from carbonaceous chondrites exhibit complementary nucleosynthetic W isotope anomalies that result from the depletion of a metallic s-process carrier in the chondrules, and the enrichment of this carrier in the matrix.
Hellmann, J., Budde, G., Kleine, T.
core +1 more source
Trace element composition of silicate minerals from Kunashak Meteorite (L6)
Major (EPMA) and trace (SIMS) element geochemistry in the silicate minerals (olivine, pyroxene and plagioclase) of Kunashak equilibrated ordinary chondrite (L6) is described. No variations in the major element concentrations of the silicate minerals have
Kristina G. Sukhanova, Olga L. Galankina
doaj
We investigated the relationship between microporosity, impact deformation, and aqueous alteration in the CM chondrite Murchison using high-resolution (1.86 μ m/voxel) X-ray computed tomography (XCT) combined with a pressurized xenon gas infiltration ...
Romy D. Hanna +5 more
doaj +1 more source
Synthesis of Si-Fe Chondrule-like Dust Analogues in RF Discharge Plasmas
Chondrules are tiny particles that occur in stony meteorites and are considered as the building blocks of early asteroids and planets. It is believed that they were formed by the fast heating of the dust in the solar nebula.
Akdaulet Baikaliyev +10 more
doaj +1 more source
Comet 81P/Wild 2 is a ∼4.5 km-sized primordial object that almost has not been modified by internal heating by ^26 Al decay. Its nucleus could have been formed by hierarchical agglomeration or gravitational collapse of pebble swarms concentrated by ...
Mingming Zhang +5 more
doaj +1 more source
The Buritizal meteorite: classification of a new Brazilian chondrite
On August 14, 1967, the reporter Saulo Gomes, working at TV Tupi, went to a small city in the State of São Paulo called Buritizal to investigate reports of a meteorite fall and write a newspaper report.
Rogerio Nogueira Salaverry +5 more
doaj +1 more source

