A new microkrystite spherule-bearing diamictite is reported from below the impact spherule-bearing 3.47 Ga Antarctic Chert Member (ACM) at the base of the Apex Basalt, central Pilbara Craton, Western Australia [1,5]. The diamictite, defined as ACM-S2, consists of 0.6–0.8-m-thick spherule-bearing pebble to cobble-size chert–intraclast conglomerate separated from the main ACM-S3 by a ∼200-m-thick dolerite and ∼30-m-thick felsic hypabyssals. The microkrystite spherules are discriminated from angular to subangular detrital volcanic fragments by their high sphericities, inward-radiating fans of sericite pseudomorphs after K-feldspar, relic quench textures and Ni–Cr–Co relations. Scanning Electron Microscopy coupled with E-probe (EDS) and laser I...
Microscopic spherules (100-1000 micrometers) have been found in glacial moraine deposits in Antarcti...
Aggregates of microscopic spherules broadly similar in texture and composition to cosmic spherules o...
Asteroid impact spherule layers and tsunami deposits underlying banded iron-formations in the Fortes...
A new microkrystite spherule-bearing diamictite is reported from below the impact spherule-bearing 3...
The Archean rock record contains seventeen asteroid impact ejecta units that represent the terrestri...
The Archean rock record contains seventeen asteroid impact ejecta units that represent the terrestri...
Deciphering Earthʼs impact history before ∼2 Ga relies heavily on the lunar record and terrestrial s...
A stratigraphically consistent <20-cm-thick unit of microkrystite spherule and microtektite-bearing ...
International audienceImpactor identification is one of the challenges of large-scale impact crateri...
Introduction: Projectile identification is a critical aspect in large-scale impact cratering studies...
The only well-known terrestrial analogue of impact craters in basaltic crusts of the rocky planets i...
Impact ejecta (about 2.5 Gyr old) in the DS4 layer of the Dales Gorge BIF (Hamersley Group, Western ...
Thin layers rich in spherules formed during impacts by large extraterrestrial objects have the poten...
Thin layers rich in spherules formed during impacts by large extraterrestrial objects have the poten...
We report on the geochemical analyses of glassy spherules from sediments at three Transantarctic Mou...
Microscopic spherules (100-1000 micrometers) have been found in glacial moraine deposits in Antarcti...
Aggregates of microscopic spherules broadly similar in texture and composition to cosmic spherules o...
Asteroid impact spherule layers and tsunami deposits underlying banded iron-formations in the Fortes...
A new microkrystite spherule-bearing diamictite is reported from below the impact spherule-bearing 3...
The Archean rock record contains seventeen asteroid impact ejecta units that represent the terrestri...
The Archean rock record contains seventeen asteroid impact ejecta units that represent the terrestri...
Deciphering Earthʼs impact history before ∼2 Ga relies heavily on the lunar record and terrestrial s...
A stratigraphically consistent <20-cm-thick unit of microkrystite spherule and microtektite-bearing ...
International audienceImpactor identification is one of the challenges of large-scale impact crateri...
Introduction: Projectile identification is a critical aspect in large-scale impact cratering studies...
The only well-known terrestrial analogue of impact craters in basaltic crusts of the rocky planets i...
Impact ejecta (about 2.5 Gyr old) in the DS4 layer of the Dales Gorge BIF (Hamersley Group, Western ...
Thin layers rich in spherules formed during impacts by large extraterrestrial objects have the poten...
Thin layers rich in spherules formed during impacts by large extraterrestrial objects have the poten...
We report on the geochemical analyses of glassy spherules from sediments at three Transantarctic Mou...
Microscopic spherules (100-1000 micrometers) have been found in glacial moraine deposits in Antarcti...
Aggregates of microscopic spherules broadly similar in texture and composition to cosmic spherules o...
Asteroid impact spherule layers and tsunami deposits underlying banded iron-formations in the Fortes...