Add to ORKGFe-Ni-Si grains trapped in vacant regions formed by impact events on granitic rock are found in spherules included in glassy blocks on the surface of the buried Takamatsu crater, Japan
Studies of the geochemical effects of impact cratering at the Vernadsky Institute in collaboration w...
A large extraterrestrial object striking Earth at cosmic velocity melts and vaporizes silicate mater...
Abstract–Previous workers have shown that an impact ejecta layer at Massignano, Italy contains a pos...
New types of impact-related grains of Fe-Ni-Si or Fe-Si in composition found in spherules are collec...
A new microkrystite spherule-bearing diamictite is reported from below the impact spherule-bearing 3...
Il cratere di Kamil è un piccolo (45 metri in diametro) cratere da impatto situato nell’Egitto sud-o...
The only well-known terrestrial analogue of impact craters in basaltic crusts of the rocky planets i...
Tiny grains of Fe-Ni system originated from planetesimals or meteoroids can remain under solid (or m...
Previous workers have shown that an impact ejecta layer at Massignano, Italy contains a positive Ir ...
Shock effects in small terrestrial impact craters (diameter < 300 m) have been poorly studied becaus...
I-type cosmic spherules are micrometeorites that formed by melting during atmospheric entry and cons...
The study of shock-metamorphic features of the Zagami meteorite revealed pseudotachylite-like melt v...
The encounter between the Stardust spacecraft and particles from comet 81P/Wild 2 gave impacts at a ...
I-type cosmic spherules are micrometeorites that formed by melting during atmospheric entry and cons...
Meteor Crater, Arizona provides an opportunity to study, in detail, elemental fractionation processe...
Studies of the geochemical effects of impact cratering at the Vernadsky Institute in collaboration w...
A large extraterrestrial object striking Earth at cosmic velocity melts and vaporizes silicate mater...
Abstract–Previous workers have shown that an impact ejecta layer at Massignano, Italy contains a pos...
New types of impact-related grains of Fe-Ni-Si or Fe-Si in composition found in spherules are collec...
A new microkrystite spherule-bearing diamictite is reported from below the impact spherule-bearing 3...
Il cratere di Kamil è un piccolo (45 metri in diametro) cratere da impatto situato nell’Egitto sud-o...
The only well-known terrestrial analogue of impact craters in basaltic crusts of the rocky planets i...
Tiny grains of Fe-Ni system originated from planetesimals or meteoroids can remain under solid (or m...
Previous workers have shown that an impact ejecta layer at Massignano, Italy contains a positive Ir ...
Shock effects in small terrestrial impact craters (diameter < 300 m) have been poorly studied becaus...
I-type cosmic spherules are micrometeorites that formed by melting during atmospheric entry and cons...
The study of shock-metamorphic features of the Zagami meteorite revealed pseudotachylite-like melt v...
The encounter between the Stardust spacecraft and particles from comet 81P/Wild 2 gave impacts at a ...
I-type cosmic spherules are micrometeorites that formed by melting during atmospheric entry and cons...
Meteor Crater, Arizona provides an opportunity to study, in detail, elemental fractionation processe...
Studies of the geochemical effects of impact cratering at the Vernadsky Institute in collaboration w...
A large extraterrestrial object striking Earth at cosmic velocity melts and vaporizes silicate mater...
Abstract–Previous workers have shown that an impact ejecta layer at Massignano, Italy contains a pos...