Add to ORKGformation is still not known- common scenarios are formation in a protoplanetary nebular environment: e.g. X-wind model [1] or nebular shock fronts, where pre-cursor grains are heated by collisions with gas [2]
Chondrules are a major component of primitive meteorites and are thought to be among the first solid...
The primordial asteroid belt contained at least several hundred and possibly as many as 10,000 bodie...
Beneath the fusion-encrusted surfaces of the most primitive stony meteorites lies not homogeneous ro...
The exact process of chondrule formation is still not known - common scenarios are formation in a pr...
The exact process of chondrule formation is still not known. The most common scenarios are formation...
We are investigating chondrule formation by nebular shock waves, using hot plasma as an analog of th...
Introduction: Chondrules are the dominant com-ponent in primitive meteorites. Their modal abundance...
To investigate the formation of chondrules in gas-grain collisions, we conducted experiments where m...
Gas dynamic shock waves in a low temperature nebula have been considered to be a leading candidate m...
In recent years many models of chondrule formation have been proposed. One of those models is the pr...
Context. The formation of chondrules in the protoplanetary nebulae causes many questions concerning ...
Chondrules are millimeter-sized rounded igneous rocks within chondritic meteorites. Their textures a...
We propose that the nebular shocks currently favored as a model to form chondrules and other anneale...
Abstract-We investigate the possible formation of chondrules by planetesimal bow shocks. The formati...
Chondrules are crystallized droplets of silicate melt formed by rapid heating to high temperatures (...
Chondrules are a major component of primitive meteorites and are thought to be among the first solid...
The primordial asteroid belt contained at least several hundred and possibly as many as 10,000 bodie...
Beneath the fusion-encrusted surfaces of the most primitive stony meteorites lies not homogeneous ro...
The exact process of chondrule formation is still not known - common scenarios are formation in a pr...
The exact process of chondrule formation is still not known. The most common scenarios are formation...
We are investigating chondrule formation by nebular shock waves, using hot plasma as an analog of th...
Introduction: Chondrules are the dominant com-ponent in primitive meteorites. Their modal abundance...
To investigate the formation of chondrules in gas-grain collisions, we conducted experiments where m...
Gas dynamic shock waves in a low temperature nebula have been considered to be a leading candidate m...
In recent years many models of chondrule formation have been proposed. One of those models is the pr...
Context. The formation of chondrules in the protoplanetary nebulae causes many questions concerning ...
Chondrules are millimeter-sized rounded igneous rocks within chondritic meteorites. Their textures a...
We propose that the nebular shocks currently favored as a model to form chondrules and other anneale...
Abstract-We investigate the possible formation of chondrules by planetesimal bow shocks. The formati...
Chondrules are crystallized droplets of silicate melt formed by rapid heating to high temperatures (...
Chondrules are a major component of primitive meteorites and are thought to be among the first solid...
The primordial asteroid belt contained at least several hundred and possibly as many as 10,000 bodie...
Beneath the fusion-encrusted surfaces of the most primitive stony meteorites lies not homogeneous ro...