Miller Range (MIL) 13317 is a 32-g lunar meteorite collected during the 2013-2014 ANSMET (Antarctic Search for Meteorites) field season. It was initially described as having 25% black fusion crust covering a light- to dark-grey matrix, with numerous clasts ranging in size up to 1 cm; it was tenta-tively classified as a lunar anorthositic breccia. Here we present the petrography and geochemistry of MIL 13317, and examine possible pairing relationships with previously described lunar meteorites
Miller Range (MIL) 05035 is a lunar gabbroic meteorite. The mineralogy, Fe/Mn ratios in olivine and ...
Yamato-86032 is a shock-lithified anorthositic fragmental breccia. It consists mainly of highly feld...
The anorthositic crust of the Moon is often used as the archtypical example of a primary planetary c...
Lunar meteorite MET 01210 (hereafter referred to as MET) is a 22.8 g breccia collected during the 20...
Miller Range (MIL) 05035 is a crystalline lunar mare gabbroic meteorite collected in Antarctica in 2...
Lunar meteorite NWA 11421 is provisionally placed with the "NWA 8046 clan" of similar stones (the "A...
Meteorites are ejected from random areas of the lunar surface and therefore provide geological infor...
Antarctic Meteorite ALHA 81005. This small, special meteorite has been the focus of much attention. ...
Meteorites ejected from the surface of the Moon as a result of impact events are an important source...
Abstract Miller Range (MIL) 13317 is a heterogeneous basalt-bearing lunar regolith breccia that prov...
Two small samples of the new lunar meteorite Yamato-793274 have been studied for mineralogical, petr...
Our studies of the Miller Range lunar meteorites MIL 090034, 090036, and 090070 show them to be a di...
Miller Range (MIL) 05035 is a lunar gabbroic meteorite. The mineralogy, Fe/Mn ratios in olivine and ...
By the 1988-1989 field season, more than 10 specimens of lunar meteorites have been recovered in Ant...
The geology of the Moon represents nearly a continuous geological record from its formation during t...
Miller Range (MIL) 05035 is a lunar gabbroic meteorite. The mineralogy, Fe/Mn ratios in olivine and ...
Yamato-86032 is a shock-lithified anorthositic fragmental breccia. It consists mainly of highly feld...
The anorthositic crust of the Moon is often used as the archtypical example of a primary planetary c...
Lunar meteorite MET 01210 (hereafter referred to as MET) is a 22.8 g breccia collected during the 20...
Miller Range (MIL) 05035 is a crystalline lunar mare gabbroic meteorite collected in Antarctica in 2...
Lunar meteorite NWA 11421 is provisionally placed with the "NWA 8046 clan" of similar stones (the "A...
Meteorites are ejected from random areas of the lunar surface and therefore provide geological infor...
Antarctic Meteorite ALHA 81005. This small, special meteorite has been the focus of much attention. ...
Meteorites ejected from the surface of the Moon as a result of impact events are an important source...
Abstract Miller Range (MIL) 13317 is a heterogeneous basalt-bearing lunar regolith breccia that prov...
Two small samples of the new lunar meteorite Yamato-793274 have been studied for mineralogical, petr...
Our studies of the Miller Range lunar meteorites MIL 090034, 090036, and 090070 show them to be a di...
Miller Range (MIL) 05035 is a lunar gabbroic meteorite. The mineralogy, Fe/Mn ratios in olivine and ...
By the 1988-1989 field season, more than 10 specimens of lunar meteorites have been recovered in Ant...
The geology of the Moon represents nearly a continuous geological record from its formation during t...
Miller Range (MIL) 05035 is a lunar gabbroic meteorite. The mineralogy, Fe/Mn ratios in olivine and ...
Yamato-86032 is a shock-lithified anorthositic fragmental breccia. It consists mainly of highly feld...
The anorthositic crust of the Moon is often used as the archtypical example of a primary planetary c...