Add to ORKGThe Kaguya mission detected small but widespread outcrops of nearly pure ferroan anorthosite in and around large impact basins on the Moon. Along with certain lunar rocks, highly feldspathic lunar meteorites such as MIL 090034 (M34), 090036 (M36), and 090070 (M70) may provide samples of this material. We have measured the Ar-40/Ar-39 release patterns and cosmogenic Ar-38 concentrations of several small (<200 microg) samples separated from M34,36, and 70. From petrographic observations concluded that "some of the clasts and grains experienced generations of modifications," a conclusion that we examine in light of our data
Sayh al Uhaymir (SaU) 300 comprises a microcrystalline igneous matrix (grain size 10 m), dominated b...
In a histogram of lunar impact ages from the Apollo 16 site, there is a spike circa 3.9 Ga that has ...
The South Pole-Aitken (SPA) basin is the stratigraphically oldest identifiable lunar basin and is th...
Our studies of the Miller Range lunar meteorites MIL 090034, 090036, and 090070 show them to be a di...
Meteorites are ejected from random areas of the lunar surface and therefore provide geological infor...
Meteorites ejected from the surface of the Moon as a result of impact events are an important source...
Lunar meteorite, Y-86032 is a fragmental or regolith breccia enriched in Al2O3 (28-31 wt%) and havin...
The number of named stones found on Earth that have proven to be meteorites from the Moon is approx....
Certain anorthositic rocks that are rare in the returned lunar samples have been identified among lu...
The anorthositic crust of the Moon is often used as the archtypical example of a primary planetary c...
Two small samples of the new lunar meteorite Yamato-793274 have been studied for mineralogical, petr...
Miller Range (MIL) 13317 is a 32-g lunar meteorite collected during the 2013-2014 ANSMET (Antarctic ...
We report new data for the bulk compositions of two meteorites derived from the mare lava plains of ...
The data collection and the interpretation with respect to the mineralogy of meteoritic and terrestr...
The Dhofar 961 lunar meteorite was found in 2003 in Oman. It is texturally paired with Dhofar 925 an...
Sayh al Uhaymir (SaU) 300 comprises a microcrystalline igneous matrix (grain size 10 m), dominated b...
In a histogram of lunar impact ages from the Apollo 16 site, there is a spike circa 3.9 Ga that has ...
The South Pole-Aitken (SPA) basin is the stratigraphically oldest identifiable lunar basin and is th...
Our studies of the Miller Range lunar meteorites MIL 090034, 090036, and 090070 show them to be a di...
Meteorites are ejected from random areas of the lunar surface and therefore provide geological infor...
Meteorites ejected from the surface of the Moon as a result of impact events are an important source...
Lunar meteorite, Y-86032 is a fragmental or regolith breccia enriched in Al2O3 (28-31 wt%) and havin...
The number of named stones found on Earth that have proven to be meteorites from the Moon is approx....
Certain anorthositic rocks that are rare in the returned lunar samples have been identified among lu...
The anorthositic crust of the Moon is often used as the archtypical example of a primary planetary c...
Two small samples of the new lunar meteorite Yamato-793274 have been studied for mineralogical, petr...
Miller Range (MIL) 13317 is a 32-g lunar meteorite collected during the 2013-2014 ANSMET (Antarctic ...
We report new data for the bulk compositions of two meteorites derived from the mare lava plains of ...
The data collection and the interpretation with respect to the mineralogy of meteoritic and terrestr...
The Dhofar 961 lunar meteorite was found in 2003 in Oman. It is texturally paired with Dhofar 925 an...
Sayh al Uhaymir (SaU) 300 comprises a microcrystalline igneous matrix (grain size 10 m), dominated b...
In a histogram of lunar impact ages from the Apollo 16 site, there is a spike circa 3.9 Ga that has ...
The South Pole-Aitken (SPA) basin is the stratigraphically oldest identifiable lunar basin and is th...