The age of the impact event is recorded in Yamato(Y)-791088,a high-iron type chondrite and has been dated using the Rb-Sr chronometer. A brief mineralogical characterization was made of the chondrite as well. The obtained impact age is 1024±47Ma. When Y-791088 recorded the impact event, it might not have been on the surface of the parent body, but rather deep. Therefore, some sulfide was not vaporized and Rb was not lost during the impact. Metal phases were once homogenized and plessite, consisting of two phases, is really scarce. After the impact, the parental body could not have lasted long before separating into pieces
The 11th Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites, Poster presentatio...
Impact cratering is one of the dominant geologic processes affecting asteroids. It results in shock-...
The 13th Symposium on Polar Science/Ordinary sessions [OA] Antarctic meteorites, Thu. 17 Nov
The Yamato-794046 H chondrite and its inclusion were dated by the Rb-Sr method as part of a consorti...
40Ar-39Ar analyses of a total of 26 samples from eight shock-darkened impact melt breccias of H-chon...
Rb-Sr systematics, REE, Ba, Sr, Rb, K, Ca and Mg abundances were analyzed in 1) whole-rock samples f...
We have studied Yamato (Y)-790964 and-790143,which are unusual paired impact-melted LL chondrites. S...
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...
The L chondrite Patuxent Range (PAT) 91501 is an 8.5-kg unshocked, homogeneous, igneous-textured imp...
We determined Ar-39-Ar-40 ages of eight LL chondrites, and one igneous inclusion from an LL chondrit...
Rb-Sr isotopic study as well as petrologic investigations have been done on sixteen individul chondr...
A comprehensive geochemical study of the Chelyabinsk meteorite reveals further details regarding its...
The Sr isotopic compositions and Rb and Sr abundances, as well as major element abundances in olivin...
^Ar-^Ar analyses were performed on the host phase of an H-clast bearing chondrite Yamato-75097 (L6)....
The 11th Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites, Poster presentatio...
Impact cratering is one of the dominant geologic processes affecting asteroids. It results in shock-...
The 13th Symposium on Polar Science/Ordinary sessions [OA] Antarctic meteorites, Thu. 17 Nov
The Yamato-794046 H chondrite and its inclusion were dated by the Rb-Sr method as part of a consorti...
40Ar-39Ar analyses of a total of 26 samples from eight shock-darkened impact melt breccias of H-chon...
Rb-Sr systematics, REE, Ba, Sr, Rb, K, Ca and Mg abundances were analyzed in 1) whole-rock samples f...
We have studied Yamato (Y)-790964 and-790143,which are unusual paired impact-melted LL chondrites. S...
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...
The L chondrite Patuxent Range (PAT) 91501 is an 8.5-kg unshocked, homogeneous, igneous-textured imp...
We determined Ar-39-Ar-40 ages of eight LL chondrites, and one igneous inclusion from an LL chondrit...
Rb-Sr isotopic study as well as petrologic investigations have been done on sixteen individul chondr...
A comprehensive geochemical study of the Chelyabinsk meteorite reveals further details regarding its...
The Sr isotopic compositions and Rb and Sr abundances, as well as major element abundances in olivin...
^Ar-^Ar analyses were performed on the host phase of an H-clast bearing chondrite Yamato-75097 (L6)....
The 11th Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites, Poster presentatio...
Impact cratering is one of the dominant geologic processes affecting asteroids. It results in shock-...
The 13th Symposium on Polar Science/Ordinary sessions [OA] Antarctic meteorites, Thu. 17 Nov