Sayh al Uhaymir (SaU) 300 comprises a microcrystalline igneous matrix (grain size 10 m), dominated by plagioclase, pyroxene, and olivine. Pyroxene geothermometry indicates that the matrix crystallized at ~1100 degrees C. The matrix encloses mineral and lithic clasts that record the effects of variable levels of shock. Mineral clasts include plagioclase, low- and high-Ca pyroxene, pigeonite, and olivine. Minor amounts of ilmenite, FeNi metal, chromite, and a silica phase are also present. A variety of lithic clast types are observed, including glassy impact melts, impact-melt breccias, and metamorphosed impact melts. One clast of granulitic breccia was also noted. A lunar origin for SaU 300 is supported by the composition of the plagioclase ...
Lunar rocks may be classified into three major groups: (1) coarse-grained igneous rocks, (2) fine-gr...
Dhofar (Dho) 925, 961 and Sayh al Uhaymir (SaU) 449 are brecciated lunar meteorites consisting of mi...
Antarctic meteorite Yamato-791197 (Y-791197) is a polymict regolith breccia from the lunar highlands...
Lunar meteorites are an important source of information about the Earth’s moon. In this study, the m...
Studies of lunar meteorite Dhofar 026, and comparison to Apollo sample 15418, indicate that Dhofar 0...
Our studies are highly interdisciplinary, but are focused on the processes and products of early pla...
Two general classes of lunar impact breccias have been recognised: fragmental breccias and melt brec...
Meteorites ejected from the surface of the Moon as a result of impact events are an important source...
Yamato (Y)-793169 and Asuka (A)-881757 are unbrecciated lunar mare meteorites that contain shocked p...
Our understanding of the formation and evolution of the primary lunar crust is based on geochemical ...
We studied 42 impact-melt clasts from lunar feldspathic regolith breccias MacAlpine Hills (MAC) 8810...
Shock metamorphism, caused by hypervelocity impact, is a poorly understood process in feldspar. This...
Northwest Africa (NWA) 032 is the youngest radio metrically dated mare basalt, with concordant Rb-Sr...
Two small samples of the new lunar meteorite Yamato-793274 have been studied for mineralogical, petr...
Lunar rocks may be classified into three major groups: (1) coarse-grained igneous rocks, (2) fine-gr...
Lunar rocks may be classified into three major groups: (1) coarse-grained igneous rocks, (2) fine-gr...
Dhofar (Dho) 925, 961 and Sayh al Uhaymir (SaU) 449 are brecciated lunar meteorites consisting of mi...
Antarctic meteorite Yamato-791197 (Y-791197) is a polymict regolith breccia from the lunar highlands...
Lunar meteorites are an important source of information about the Earth’s moon. In this study, the m...
Studies of lunar meteorite Dhofar 026, and comparison to Apollo sample 15418, indicate that Dhofar 0...
Our studies are highly interdisciplinary, but are focused on the processes and products of early pla...
Two general classes of lunar impact breccias have been recognised: fragmental breccias and melt brec...
Meteorites ejected from the surface of the Moon as a result of impact events are an important source...
Yamato (Y)-793169 and Asuka (A)-881757 are unbrecciated lunar mare meteorites that contain shocked p...
Our understanding of the formation and evolution of the primary lunar crust is based on geochemical ...
We studied 42 impact-melt clasts from lunar feldspathic regolith breccias MacAlpine Hills (MAC) 8810...
Shock metamorphism, caused by hypervelocity impact, is a poorly understood process in feldspar. This...
Northwest Africa (NWA) 032 is the youngest radio metrically dated mare basalt, with concordant Rb-Sr...
Two small samples of the new lunar meteorite Yamato-793274 have been studied for mineralogical, petr...
Lunar rocks may be classified into three major groups: (1) coarse-grained igneous rocks, (2) fine-gr...
Lunar rocks may be classified into three major groups: (1) coarse-grained igneous rocks, (2) fine-gr...
Dhofar (Dho) 925, 961 and Sayh al Uhaymir (SaU) 449 are brecciated lunar meteorites consisting of mi...
Antarctic meteorite Yamato-791197 (Y-791197) is a polymict regolith breccia from the lunar highlands...