40Ar-39Ar analyses of a total of 26 samples from eight shock-darkened impact melt breccias of H-chondrite affinity (Gao-Guenie, LAP 02240, LAP 03922, LAP 031125, LAP 031173, LAP 031308, NWA 2058, and Ourique) are reported. These appear to record impacts ranging in time from 303 +/- 56 Ma (Gao-Guenie) to 4360 +/- 120 Ma (Ourique) ago. Three record impacts 300-400 Ma ago, while two others record impacts 3900-4000 Ma ago. Combining these with other impact ages from H chondrites in the literature, it appears that H chondrites record impacts in the first 100 Ma of solar system history, during the era of the lunar cataclysm and shortly thereafter (3500-4000 Ma ago), one or more impacts ~300 Ma ago, and perhaps an impact ~500 Ma ago (near the time...
Radiometric dating and compositional clustering of lunar impact-melt rocks form the backbone of the ...
Rb-Sr systematics, REE, Ba, Sr, Rb, K, Ca and Mg abundances were analyzed in 1) whole-rock samples f...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...
We determined Ar-39-Ar-40 ages of eight LL chondrites, and one igneous inclusion from an LL chondrit...
Studies of meteorites are based mostly on samples that fell to Earth in the recent past (i.e., a few...
Studies of meteorites are based mostly on samples that fell to Earth in the recent past (i.e., a few...
The age of the impact event is recorded in Yamato(Y)-791088,a high-iron type chondrite and has been ...
We studied 42 impact-melt clasts from lunar feldspathic regolith breccias MacAlpine Hills (MAC) 8810...
Lunar impact melt breccias provide a unique record of the timing and frequency of collisional events...
DaG 896 is an olivine-rich microporphyritic rock of komatiitic composition. Both the olivine composi...
DaG 896 is an olivine-rich microporphyritic rock of komatiitic composition. Both the olivine composi...
We investigate the thermal/impact histories of four HED meteorites: one cumulate eucrite (Lake Carne...
The L chondrite Patuxent Range (PAT) 91501 is an 8.5-kg unshocked, homogeneous, igneous-textured imp...
Lunar meteorites represent a more random sampling of lunar material than the Apollo or Luna collecti...
Boltysh was of particular interest due to its chronological proximity to the Cretaceous- Palaeogene ...
Radiometric dating and compositional clustering of lunar impact-melt rocks form the backbone of the ...
Rb-Sr systematics, REE, Ba, Sr, Rb, K, Ca and Mg abundances were analyzed in 1) whole-rock samples f...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...
We determined Ar-39-Ar-40 ages of eight LL chondrites, and one igneous inclusion from an LL chondrit...
Studies of meteorites are based mostly on samples that fell to Earth in the recent past (i.e., a few...
Studies of meteorites are based mostly on samples that fell to Earth in the recent past (i.e., a few...
The age of the impact event is recorded in Yamato(Y)-791088,a high-iron type chondrite and has been ...
We studied 42 impact-melt clasts from lunar feldspathic regolith breccias MacAlpine Hills (MAC) 8810...
Lunar impact melt breccias provide a unique record of the timing and frequency of collisional events...
DaG 896 is an olivine-rich microporphyritic rock of komatiitic composition. Both the olivine composi...
DaG 896 is an olivine-rich microporphyritic rock of komatiitic composition. Both the olivine composi...
We investigate the thermal/impact histories of four HED meteorites: one cumulate eucrite (Lake Carne...
The L chondrite Patuxent Range (PAT) 91501 is an 8.5-kg unshocked, homogeneous, igneous-textured imp...
Lunar meteorites represent a more random sampling of lunar material than the Apollo or Luna collecti...
Boltysh was of particular interest due to its chronological proximity to the Cretaceous- Palaeogene ...
Radiometric dating and compositional clustering of lunar impact-melt rocks form the backbone of the ...
Rb-Sr systematics, REE, Ba, Sr, Rb, K, Ca and Mg abundances were analyzed in 1) whole-rock samples f...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...