The results of intensive studies indicate that shock-metamorphic effects, characteristic of meteorite impact and virtually identical to those observed in Apollo samples, are common in fragments of the Luna-16 soil sample from Mare Fecunditatis. Two types of shock effects are present: (1) deformation and partial melting features in rock and mineral fragments (1-2 percent of fragments); and (2) heterogeneous glasses and glassy breccias produced by shock melting (70-80 percent of fragments). Shock effects were observed in pyroxene (deformation twin lamellae, multiple planar shock lamellae, extreme mosaicism, partial isotropization); in plagioclase (planar shock lamellae, complete isotropization to form maskelynite); and in basalt fragments (pl...
The study of shock-metamorphic features of the Zagami meteorite revealed pseudotachylite-like melt v...
The mineralogy and petrology of the Apollo 11 rocks are consistent with impact melting of ilmenite ...
The partitioning of energy and the distribution of the resultant ejecta on the moon is numerically m...
Shock metamorphism, caused by hypervelocity impact, is a poorly understood process in feldspar. This...
Our studies are highly interdisciplinary, but are focused on the processes and products of early pla...
Lunar meteorites are an important source of information about the Earth’s moon. In this study, the m...
Sayh al Uhaymir (SaU) 300 comprises a microcrystalline igneous matrix (grain size 10 m), dominated b...
Studies of lunar meteorite Dhofar 026, and comparison to Apollo sample 15418, indicate that Dhofar 0...
Lunar rocks may be classified into three major groups: (1) coarse-grained igneous rocks, (2) fine-gr...
The Apollo 15 mission returned various samples of regolith breccias, typical lunar rocks lithified b...
Studies of the chemistry and morphology of the lunar samples are reported. The presence of fragments...
Lunar rocks may be classified into three major groups: (1) coarse-grained igneous rocks, (2) fine-gr...
The first step in a petrologic study must be a classification based on observed textures and mineral...
Antarctic lunar meteorites Meteorite Hills 01210 and Pecora Escarpment 02007 are breccias that come ...
The Moon is the only planetary body, besides Earth, from which there are samples from known location...
The study of shock-metamorphic features of the Zagami meteorite revealed pseudotachylite-like melt v...
The mineralogy and petrology of the Apollo 11 rocks are consistent with impact melting of ilmenite ...
The partitioning of energy and the distribution of the resultant ejecta on the moon is numerically m...
Shock metamorphism, caused by hypervelocity impact, is a poorly understood process in feldspar. This...
Our studies are highly interdisciplinary, but are focused on the processes and products of early pla...
Lunar meteorites are an important source of information about the Earth’s moon. In this study, the m...
Sayh al Uhaymir (SaU) 300 comprises a microcrystalline igneous matrix (grain size 10 m), dominated b...
Studies of lunar meteorite Dhofar 026, and comparison to Apollo sample 15418, indicate that Dhofar 0...
Lunar rocks may be classified into three major groups: (1) coarse-grained igneous rocks, (2) fine-gr...
The Apollo 15 mission returned various samples of regolith breccias, typical lunar rocks lithified b...
Studies of the chemistry and morphology of the lunar samples are reported. The presence of fragments...
Lunar rocks may be classified into three major groups: (1) coarse-grained igneous rocks, (2) fine-gr...
The first step in a petrologic study must be a classification based on observed textures and mineral...
Antarctic lunar meteorites Meteorite Hills 01210 and Pecora Escarpment 02007 are breccias that come ...
The Moon is the only planetary body, besides Earth, from which there are samples from known location...
The study of shock-metamorphic features of the Zagami meteorite revealed pseudotachylite-like melt v...
The mineralogy and petrology of the Apollo 11 rocks are consistent with impact melting of ilmenite ...
The partitioning of energy and the distribution of the resultant ejecta on the moon is numerically m...